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English Pages 735 Year 2002
Engineering Thermodynamics Work and Heat Transfer
GORDON ROGERS YON MAYHEW
PEARSON
Education
Copyrig ht© 1967 by G.F.C. Rogers & Y.R. Mayhew. Copyrig ht© 1992 by Pearson Education Limited. This edition is published by arrangement with Pearson Education, Ltd. This book is sold subject to the condition that it shall not, by way of trade or otherwise, be lent, resold, hired out, or otherwise circulated without the publisher's prior written consent in any form of binding or cover other than that in which it is published and without a similar condition including this condition being imposed on the subsequent purchaser and without limiting the rights under copyright reserved above, no part of this publication may be reproduced, stored in or introduced into a retrieval system, or transmitted in any form or by any means (electronic, mechanical, photocopying, recording or otherwise), without the prior written permission of both the copyright owner and the abovementioned publisher of this book. ISBN 8131702065 First Impression, 2006 Second Impression, 2007 This edition is manufactured in India and is authorized for sale only in India, Bangladesh, Bhutan, Pakistan, Nepal, Sri Lanka and the Maldives. Circulation of this edition outside of tliese territories is UNAUTHORIZED. Published by Dor ling Kindersley (India) Pvt. Ltd., licensees of Pearson Education in South Asia. Head Office: 482, F.I.E., Pataparganj, Delhi 110 092, India. Registered Office: 14 Local Shopping Centre, Panchsheel Park, New Delhi 110 017, India. Printed in India by Pushp Print Services.
Contents
Preface to the Fourth Edition Preface to the Third Edition Preface to the Second Edition Preface to the First Edition Prologue Why study thermodynamics? How to use this book Part I
Principles of Thermodynamics
Introduction
xiii xv XVI
xvii XIX
xix xx
1
3
1
Fundamental Concepts 1.1 Thermodynamic properties 1.2 Temperature 1.3 Wor k and heat
7 7 10 11
2
The First Law of Thermodynamics 2.1 The cycle 2.2 The First Law of Thermodynamics 2.3 Mechanical equivalent of heat 2.4 Corollaries of the First Law
15 16 18 19
NonFlow Processes 3.1 The energy equation and reversibility 3.1. l Wor k and reversibility 3.1.2 Heat and reversibility 3.2 Co�stant volume process 3.3 Constant pressure process 3.4 Polytropic process Adiabatic process 3.5 3.6 Isothermal process
24 25 27 29 29 31 33 34
3
15
24
V
4
Flow Processes 4.1 The steadyflow energy equation Open systems with steady flow 4.2 4.2.1 Boiler and condenser 4.2.2 N ozzle and diffuser 4.2.3 Turbine and compressor 4.2.4 Throttling 4.2.5 Reciprocating compressor 4.3 Nonsteadyflow processes 4.4 Cycles consisting of steadyflow processes
36 36 41 41 42 43 44 44 45 47
5
The Second Law of Thermodynamics and Reversibility Cycle efficiency 5.1 The Second Law of Thermodynamics 5.2 The Clausius statement of the Second Law 5.3 Reversibility and irreversibility 5.4 5.4.1 Friction 5.4.2 Transfer of heat across a finite temperature difference 5.5 Reversible and irreversible _cycles
50 50 51 53 54 55
Corollaries of the Second Law 6.1 Reversible engines operating between only two reservoirs 6.2 Thermodynamic temperature scale 6.3 Engines operating between more than two reservoirs 6.4 Consequences of the Second Law for nonflow processes 6.5 Characteristics of entropy 6.5.1 Determination of values of entropy 6.5.2 Entropy as a criterion of reversibility 6.6 Consequences of the Second Law for steadyflow processes 6.7 Validity and limitations of the laws of thermodynamics 6.8 Summary of Chapters 1 to 6
62 62 63 66 71 73 73 75
General Thermodynamic Relations 7.1 Properties to be related Exact differentials 7.2 Some general thermodynamic relations 7.3 Measurable quantities 7.4 7.4.1 Equation of state 7.4.2 Coefficient of expansion and compressibility 7.4.3 Specific heat capacities 7.4.4 JouleThomson coefficient Graphical determination of entropy and enthalpy 7.5 7.6 Analytical determination of entropy and enthalpy 7.6.1 Perfect gas 7.6.2 The van der Waals gas Change of phase 7.7
86 87 87 90 93 93 94 96 98 100 103 106 110 112
6
7
vi
59 60
77 80 82
7.8
7.9
Part II
Processes undergone by solids and liquids 7.8.1 Constant volume process 7.8.2 Isothermal process 7.8.3 Isentropic process Exergy and the Gibbs function 7.9.1 Exergy in closed systems 7.9.2 Exergy and steadyflow open systems 7.9.3 The Gibbs function and the steadyflow system
Applications to Particular Fluids
Introduction
8
9
10
115 115 115 116 117 118 120 122 127 129 130
Properties of Fluids The unit of temperature and the International 8.1 Temperature Scale Properties of liquids and vapours 8.2 8.2.1 pvT data 8.2.2 uhs data and specific heat capacities 8.3 Tables of properties 8.3.1 Saturation table 8.3.2 Superheat table 8.3.3 Compressed liquid table 8.4 Diagrams of properties 8.4.1 Temperatureentropy diagram 8.4.2 Enthalpyentropy diagram 8.4.3 Pressureenthalpy diagram 8.5 Properties of a perfect gas 8.5.1 Equation of state of a perfect gas 8.5.2 Amountofsubstance and the molar gas constant 8.5.3 Other property relations for a perfect gas 8.5.4 Temperatureentropy diagram for a perfect gas 8.6 Kinetic theory and the properties of real gases 8.6.1 Kinetic theory of gases 8.6.2 Properties of real gases
130 136 136 141 145 145 148 149 150 150 153 155 156 156 158 159 164 166 166. 169
NonFlow Processes Constant volume process 9.1 Constant pressure process 9 .2 9 .3 · Polytropic process 9.4 Adiabatic process 9.5 Isothermal process 9.6 Irreversibility and the free expansion
173 173 175 177 180 184 187
Flow Processes 10.1 Boiler and condenser Adiabatic 10.2 steadyflow processes 10.3 Throttling process 10.4 Reversible steadyflow process
189 189 190 195 197 vii
10.5 10.6 10.7
11
12
13
14
viii
Isothermal steadyflow process Multistream steadyflow processes Nonsteadyflow processes 10.7.1 Filling a reservoir from an infinite source of fluid 10.7.2 Maximum work attainable by allowing a reservoir of fluid to discharge via a turbine
Vapour Power Cycles
11.1 11.2 11.3 11.4 11.5 11.6 11.7 11.8 11.9 11.10 11.11
Criteria for the comparison of cycles Carnot cycle Rankine cycle Reheat cycle Regenerative cycle Economiser and air preheater Steam cycles for nuclear power plant Backpressure and extraction turbines, and cogeneration Lowtemperature power cycles The ideal working fluid and binary cycles Economic assessment
198 200 201 201 204 206
207 209 214 219 222 229 231 234 239 243 246
Gas Power Cycles
248
12.4 12.5 12.6 12.7 12.8 12.9
254 254 256 259 259 262 263 266 270
12.1 12.2 12.3
Internalcombustion engines and airstandard cycles Simple gas turbine cycle Gas turbine cycles with heat exchange, intercooling and reheating 12.3. l Simple cycle with heat exchangeJ.'. 12.3.2 Intercooling and reheating Closedcycle gas turbine Combined gas and steam cycles Reciprocating engine cycles Otto, Diesel and mixed cycles Mean effective pressure as a criterion of performance Cycles having the Carnot efficiency
Heat Pump and Refrigeration Cycles
13.1 13. 2 13. 3 13. 4 13. 5
Reversed Carnot cycle and performance criteria Practical refrigeration cycles Water refrigerator Absorption refrigerators Gas cycles
Properties of Mixtures
14.1 14.2 14.3 14.4 14.5
An empirical law for mixtures of gases Mixtures of perfect gases The mixing process Gas and saturated vapour mixtures Hygrometry (or psychrometry) 14.5.1 Airconditioning plant
248 251
273
273 275 280 281 285 289
289 291 297 301 308 312
14.6 15
14.5.2 Cooling towers Hygrometric chart
Combustion Processes 15.l Fuels Chemical equations and conservation of mass 15.2 15.3 Experimental products analysis First Law applied to combustion processes 15.4 15.4. I Internal energy of combustion t1ui 15.4.2 Enthalpy of combustion and its relation to �ai 15.4.3 U−T and H−T diagrams 15.5 Experimental determination of i'lii0 and L1h0 and calorific values Efficiency of power plant and of combustion processes 15.6 Dissociation 15.7 15.7.1 The van't Hoff equilibrium box 15.7.2 Maximum work of a chemical reaction and equilibrium constants Tabulation of thermodynamic reaction data 15.8 Limitations of the thermodynamic analysis 15.9
Part lll Work Transfer Introduction
315 318
321 321 323 328 333 334 336 340 343 346 349 350 351 359 365
367
369
16
Reciprocatin g Expanders and Compressors Work transfer in reversible reciprocating machines 16.1 16.1.1 Machine cycle analysis 16.1.2 Steadyflow analysis I 6.2 The indicator diagram 16.3 Reciprocating air compressors 16.4 The steam engine Rotary positive displacement compressors I 6.5
371 371 373 374 375 379 385 392
17
Reciprocating InternalCombustion Engines The working of IC engines 17.1 Criteria of performance for IC engines 17.2 Factors limiting the performance of I C engines 17.3 17.3.1 The SI engine 17.3.2 The CI engine 17.4 Comparison of real IC engine processes with airstandard cycles 17.5 Maximum work of a chemical reaction
395 395 400 402 402 407
OneDimensional Steady Flow and Jet Propulsion 18.1 Isentropic flow in a duct of varying area 18.1.1 Derivation of the basic equations 18.1.2 Phenomena in nozzles operating off the design pressure ratio
418 419 420
18
411
415
427 ix
Metastable flow of vapours The momentum equation 18.3.1 Isentropic flow in a duct of varying area 18.3.2 Heat addition to frictionless flow in a duct of constant area 18.3.3 Irreversible adiabatic flow in a duct of varying area Jet propulsion engines 18.4.1 Propulsion engines using atmospheric air 18.4.2 Rocket motors
430 433 436
Rotary Expanders and Compressors 19.1 Momentum principles applied to flow through a rotor 19.1.1 Axial thrust on the rotor 19:1.2 Torque exerted by or on the rotor 19.2 Axialflow turbines 19.2.1 Impulse stage 19.2.2 Velocitycompounded impulse stage 19.2.3 Reaction stage 19.2.4 Multistage turbines and internal losses 19.2.5 · Stage efficiency, overall efficiency, reheat factor and polytropic efficiency 19.3 Axialflow compressors 19.4 Radialflow turbines 19.4.1 Outwardflow turbines 19.4.2 Inwardflow turbines 19.5 Radialflow compressors
450 450 451 452 453 458 461 463 466
Direct 20.1 20.2 20.3 20.4 20.5
486 487 48.9 491 492 494
18.2 18.3
18.4
19
20
Part IV
Conversion
Thermionic converters Thermoelectric converters Photovoltaic generators Magnetohydrodynamic generators Fuel cells
436 437 441 441 444
471 475 480 480 481 483
Heat Transfer
497 499
21
501 501
Introduction
X
Conduction Fourier's law of heat conduction 21.1 21.2 Onedimensional steady conduction through a composite wall 21.3 Radial steady conduction through the wall of a tube The differential equation of threedimensional 21.4 conduction 21.5 Numerical solution of twodimensional steady conduction
504 507 509 516
21.6
22
Unsteady conduction 21.6.1 The quenching of a billet 21.6.2 Numerical solution of unsteady onedimensional conduction
Convection 22.1 Some results of simple boundary layer theory 22.1.1 Flow of fluid over a flat plate 22.1.2 Flow of fluid through a cylindricar tube 22.1.3 Shear stress due to eddy motion 22.2 Forced convection in laminar flow over a flat plate 22.2.1 Derivation of the heat flow equation of the boundary layer 22.2.2 Solution of the heat flow equation 22.2.3 Solution applicable to liquid metals 22.3 Forced convection in fullydeveloped laminar flow through a tube 22.4 Forced convection in turbulent flow and the Reynolds analogy 22.4.1 The simple Reynolds analogy 22.4.2 The PrandtlTaylor modification of the Reynolds analogy 22.5 The principles of dynamic similarity and dimens:onal analysis applied to forced convection 22.6 Heat transfer from a vertical ":'all by free convection 22.7 The principles of dynamic similarity and dimensional analysis applied to free convection 22.8 Convection with change of phase 22.8.1 Condensation of a vapour on a vertical surface 22.8.2 B oiling of liquids Heat transfer enhancement 22.9 22.9.1 Fluidised beds 22.9.2 Specialgeometry condenser surfaces 22.9.3 Heat pipes
523 523 525
533 534 534 538 541 545 547 548 553
555 558 562 566 571 580 583 585 586 591 597 597 598 599
23
Radiation 23.1 The laws of blackbody radiation 23.2 Kirchhoff's law and greybody radiation Radiation exchange between two black surfaces 23.3 Radiation.exchange between two grey surfaces 23.4 Radiation from gases and flames 23.5
601 601 605 610 615 618
24
Combined Modes of Heat Transfer The heat exchanger 24.1 Heat flow through a wall 24.2 Heat flow through a fin 24.3 24.3.1 The solution of the differential equation for a prismatic fin
620 620 628 630 631 xi
24.4
24.3.2 Some questions pertinent to fin design Thermocouple in a gas stream
Appendices Appendix A Dimensions and Units A. I Introduction A.2 SI and coherence A.3 The unit symbol for temperature: K or °C? A.4 Amountofsubstance and molar quantities A.5 Further reading Appendix B Problems Appendix C References Appendix D Nomenclature
Index
xii
634 636
638 638 640 643 644 644 646 692 697 703
Preface to the Fourth Edition
Over the years the publisher has kindly allowed the authors to make improvements at many of the reprintings but, as this was always subject to no change in pagination, the revised material was not always in the best location or expressed as clearly as it could have been. The authors were pleased that Longman offered to reset completely this new edition, enabling them to make a thorough revision and to enjoy seeing their work in a more aesthetically pleasing form. Presented with this opportunity, the authors asked themselves whether their methodology, based on Keenan's Thermodynamics published in 1941, was still appropriate for the 1990s. Having looked again at the chief contenders, namely the BornCaratheodory and KeenanHatsopolous approaches, the authors remain convinced that the wellestablished route still provides the best way of introducing thermodynamics to engineering students. One fundamental change was required, however: it seemed wise to adopt the sign convention for work transfer which is now widely used by physicists and chemists and by an increasing number of engineers abroad. Although the change may appear to be trivial it has repercussions throughout much of the book. So too do some of the minor changes of notation and methods of handling units necessitated by international agreements. Some important topics were in need of a revised presentation, and others, having grown in importance, required a more extensive coverage. The way in which the perfect gas was introduced was less than perfect; it has been given a more rigorous treatment. Most books including our own had worked with an unsound definition of the equilibrium constant; this has been rectified as part of a general updating of the presentation of thermochemical concepts. We have revised the treatment of axialflow turbines, adopting the modern convention of measuring blade angles from the axial instead of the tangential direction. This change arose from experimental work on flow through cascades of blades, stimulated by the advent of the gas turbine and its axialflow compre�sor. Growing concern with energy conservation and the environment has led us to make more space available for discussion of combined cycle plant, cogeneration schemes, lowtemperature power cycles, and pollution problems. Numerous books devoted solely to heat transfer have appeared since this book was first published in 1957. We still feel, however, that the coverage provided in Part IV is worth retaining: for many students it is all they arc likely to need on the subject, while for others it is a succinct introduction. We have been able to deal with some new topics, if only briefly, and improve the treatmcnt xiii
of others. We made some changes in the previous edition in recognition of the growth in computational techniques; we have not carried this further because we believe that what is important at undergraduate level is a firm grasp of physical principles. The worked examples and problems have been revised and increased in number. At the suggestion of teachers we have added a section in the Prologue with what we hope are helpful hints on how the book might be used in conjunction with a course of lectures. In conclusion, we particularly wish to thank Carrie Pharaoh for retracing the figures so good humouredly, and Jennifer Scherr of Queen's Building Library for checking references. Our · wives deserve special thanks for putting up with less attention than they had a right to expect from two semiretired academics. Bristol 1992
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G.F.C.R. Y.R.M.
Preface to the Third Edition
Although minor additions and improvements have been made to the text and references to take account of recent work and current applications of thermo dynamics, no substantial changes have been made in this third edition. Its prime purpose is to convey to students the outcome of much international effort to standardise nomenclature, units and methods of presenting technical data. The importance of this should not be underestimated. If the everincreasing output of technical literature is to be assimilated, unremitting attention must be paid to ways of making it easily digestible. Readers can no longer afford the time to battle with ambiguities and idiosyncrasies. It is vital that students  the authors of tomorrow  should acquire good habits during their undergraduate studies. When preparing the second edition in 1966 it was necessary to anticipate certain decisions relating to the introduction of SI ( Systeme International d'Unites). The authors failed to anticipate the choice of Kinstead of °Kas a symbol for the kelvin unit of temperature, and failed to foresee the new definition of the mole. (The formal decisions were taken in 1968 and 1971 respectively.) This third edition has afforded the authors the opportunity to bring the book up to date in these respects, and in others associated with a more rigorous attitude to the concept of a physical quantity and its units which has repercussions in the way equations should be written and_ data presented in graphs and tables. The reader is referred particularly to the rewritten Appendix A on dimensions and units. Bristol 1980
G.F.C.R. Y.R.M.
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Preface to the Second Edition
This edition of the book in SI units has been produced in the hope that it will play its part in furthering the change from British to metric units which is to take place during the next few years. Examples and problems have been worked out using data contained in the second edition of Thermodynamic and Transport Properties of Fluids (SJ Units) (Basil Blackwell, 1967). The first edition of the book, and the tables in British units, will continue to be available as long as required. While preparing this edition, the opportunity has been taken to bring the material up to date in some major and many minor respects. A large part of Chapter 8 has been rewritten to accommodate changes in the approach to the definition of temperature units and the adoption of the triple point as the datum state for steam tables. The treatment of regenerative cycles has been revised. Material has been added to Chapters 7 and 15 to include an introduction to the concept of availability and the closely associated use of the Gibbs function and other chemical thermodynamic data; the section on calorific values has been brought into line with the new British Standard. A chapter has been added on direct conversion; although inevitably little more than descriptive, it is hoped that it will encourage some students to pursue the subject further as a postgraduate study. Owing to the widespread use of computers, numerical methods of dealing with nonsteady heat flow problems have been substituted for the less flexible graphical methods described in the previous edition. Additional material is included on liquid metals as heat transfer media, and on boiling. Various other topics which have assumed importance since the book was first written, such as cycles for nuclear power plant and the Wankel engine, ·have also been included, and the references have been revised to bring greater benefit from further reading. The general plan of the book is unchanged. The authors still believe that classical macroscopic thermodynamics provides the best introduction to the subject for mechanical engineers, and that any real attempt to deal with statistical thermodynamics and irreversible thermodynamics is best left to postgraduate courses. We wish to acknowledge the invaluable help given by Dr M. Hollingsworth, who reworked the problems of Appendix B in SI units to provide the reader with answers. And once again we thank Mr C. J. Spittal, our librarian, for his work in checking the references. Bristol 1967 xvi
G.F.C.R. Y.R.M.
Pref ace to the First Ed it ion
This book is intended for engineering students and covers the fundamentals of applied thermodynamics courses up to honours degree standard. The following presentation has been adopted. An exposition of the principles of thermodynamics is given in Part I without reference to the behaviour of any particular substance. Part II opens with a discussion of the properties of fluids, and the principles of Part I are then applied to closed and open systems assuming that the properties are best related (a) in tables and (b) by simple equations. This is followed by an analysis of power and refrigeration cycles. Part II ends with a study of gas and vapour mixtures and combustion processes. Parts I and II are chiefly concerned with relations between fluid properties and the quantities of work and heat which accompany changes of state. The way in which the work and heat transfers are effected in practice is described in Parts III and IV respectively. Part III is divided broadly into work transfers associated with (a) positivedisplacement machines and (b) nonpositive displacement machines. For the latter, a more detailed analysis of flow processes is required than is given in Parts I and II, and therefore a chapter on onedimensional flow is included. This chapter is designed as a bridge between the sciences of thermodynamics and fluid dynamics and, to avoid obscuring the fundamental links, concepts such as total temperature and Mach number have not been used. The usual classification of modes of heat transfer is adopted in Part IV, with the emphasis placed on methods of approach rather than on the presentation of established empirical data. We do not suggest that our order of presentation is suitable as a direct introduction to the subject, and the book is not designed as a substitute for a course of lectures. Most students are best introduced to a subject by a careful juxtaposition of principle and application, and the book leaves it open to the lecturer to choose any preferred order of presentation. But, although a mixture of principle and application is necessary in a lecture course, it can leave the student with serious misconceptions, and it by no means follows that he will gain a sufficient grasp of the principles to be able to tackle unfamiliar problems. Our object has been to produce a book which will enable the student to distinguish principle from application; a reading of the first six chapters, as revision late in his first year, should enable him to make this distinction. It should also help him lo appreciate the elegance and power, as well as the limitations, of the science he is using. Our second concern has been to provide a book of reference lo which the xvii
student can turn for the elucidation of difficult points. A rigorous approach cannot often be _used in a lecture· course, partly for lack of time and partly because it would be inappropriate when introducing the student to a new idea. In this book, however, a rigorous proof or explanation is given wherever practicable for the benefit of the better student who is not satisfied with simplifications. A few words are necessary about two of the appendixes. Many of the problems provided in Appendix B are intended to amplify points onlytouched on in the text. To this extent they should be regarded as an integral part of the book. The answers to the problems, and to the worked examples in the text, have been obtained using the abridged tables of properties arranged by us and published separately as Thermodynamic Properties of Fluids and Other Data (Basil Blackwell, 1957). Most of the references, given in Appendix C, are to be regarded as suggestions for further reading and also as acknowledgement of sources. A few classical papers of academic interest are also included. Finally we wish to acknowledge our particular indebtedness to two books which we have found a source of inspiration: J. H. Keenan's Thermodynamics (Wiley, 1941), and E. R. G. Eckert's Introduction to the Transfer of Heat and Mass (McGrawHill, 1950). We also wish to thank our colleagues at Bristol Dr B. Crossland, Mr T. V. Lawson and Dr P. Woodward  for their useful suggestions after reading parts of the manuscript. Mr C. J. Spittal, of the University Library, has been most helpful in obtaining papers and checking the references. Bristol 1957
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G.F.C.R. Y.R.M.
Prologue
Why study thermodynamics?
Since the Industrial Revolution there has been an exponential growth of population and of material wealth. This growth has been associated with the everincreasing use of energy in machines. The revolution began with coal, and has progressed through the use of petroleum, natural gas and uranium. Hydroelectric and geothermal power have made, and can make, only a small contribution on a world scale, although they are highly significant to certain countries with no indigenous resources of fossil fuel. Easily exploited reserves of both fossil fuel and uranium are limited, and many will approach exhaustion in the lifetime of present students. There are two obvious consequences: first, ways have to be found of using our energy resources more efficiently; and secondly, in the long term, other sources of power must be developed. It is the science of thermodynamics which enables us to deal quantitatively with the analysis of machines which are used to convert chemical or nuclear energy into useful work. It is therefore an essential study for those hoping to improve the effectiveness with which we use our existing energy resources. The optimisation of total energy schemes involving combined electricity production and process or district heating, or the assessment of combined gas and steam turbine plant (Cogas plant), to Lake but two examples, inevitably involve thermodynamic analysis. One of the important consequences of the Second Law of Thermodynamics is that unnecessarily large temperature differences used for the transfer of heat incur a \vasle of energy. A knowledge of the associated subject of heat transfer, dealt with in Part IV of this book, is also essential in an energyconscious world. Thermodynamics is likely to play a vital role in the solution of the longterm problem also. IL may not help in itself lo throw up suggestions for new sources of power, but it is an essential tool for evaluating correctly the potential of new ideas. For example, it will be used to assess proposals for more effective ways of using solar energy, whether in devices which convert it into electricity, or less directly by photosynthesis in plant life from which alcohol or methane fuels can be obtained. It will also be used if ways can be found of harnessing the fusion process. Like fission, fusion will provide heat which can be converted to electricity in more or less conventional power plant. Such solutions would provide mankind with safe and nonpolluting sources of power for an indefinitely long period. xix
Are these massive sources of power really needed? Certainly it is possible for a few small groups to live in selfsupporting communes. However, if we care for the bulk of mankind (approximately 5.3 x 10 9 and probably doubling in under 40 years), continued expansion of power production is essential if only to produce the energy required for modern methods of food production. But it is needed not merely for this: experience in the developed nations suggests that the world population will be stabilised only when the standard of living has been raised substantially in the developing countries. Failure to stabilise it will lead inevitably to famine and conflict over living space. Finally, some of the other reasons why more energy is likely to be needed in the.future are: (a) (b) (c)
To enable lowergrade metallic ores to be used, and to operate waste reclamation plant to recover scarce materials To produce secondary fuels for land, sea and air transport, and the necessary hydrocarbon feedstock for the chemical industry, when natural oil and gas become scarce To reduce environmental pollution from power plant and industrial processes, which will become increasingly important as the population increases.
The increase in demand will be offset to some extent by energy conservation measures, and by new inventions which will enable society's needs to be met with a smaller expenditure of scarce resources. The development of micro electronics, and of optical fibres as a substitute for copper wire, are two recent examples of such inventiveness. There is little doubt, however, that there will be a large net increase in demand from the world as a whole because, at present, twothirds of the world uses energy at about onetenth of the rate used in the developed countries. In studying engineering in general,' and thermodynamics in particular, the student is laying a foundation which will enable him to make a substantial contribution to the welfare of mankind. To whet the appetite, the accompanying diagram shows the range of energy resources at man's disposal and the ways in which they might be used. Not all of the devices mentioned have been developed to date, and some may never be economic, but most of them receive some attention in this book. Other devices dealt with, which do not appear in this schematic diagram because they do not involve the production of power, are refrigerators, heat pumps, airconditioning plant and heat exchangers. How to use this book
Some suggestions as to how the book might be used were given in the Preface to the First Edition, but few, new readers feel inclined to read an old preface. In response to requests for guidance, we will repeat here some of what was said there and enlarge upon it. The first point we made was as follows: 'We do not suggest that our order of presentation is suitable as a direct introduction to the subject, and the book is not designed as a substitute for a course of lectures. Mosl students are best introduced to a subject by a careful juxtaposition of principle and application, and the book· leaves it open to the· Ice! urer to choose any preferred order of xx
SI
Battery
Cl
1 Chemical direct conversion
1
I
Gas
1‘
IC engines
01
_ Rejected heat
Steam turbine (or engine)
V
I Hydraulic turbine
I Stirling engine
Process industries district heating
Gas turbine (closed cycle)
I Direct solar radiation
MHD (topper)
I
1 Windmill generator
Thermionic generator (topper)
I
Vegetation
! Wave generator
I Thermoelectric generator (bottomer)
Photoelectric generator
Direct conversion
I Rankine cycle plant
1 I 1 I Tides Water Wind Photosynthesis Oceanic temperature reservoir difference I I
After conversion to heat
I I Fusion Geothermal
I
I
I
Production of hydrogen or hydrocarbon
I Fission
I Indirect solar radiation
I Earth's energy
1 Atomic energy
I
I
Cogas plant
Gas turbine (open cycle)
Fuel cell
C( al
I Fossil fuel
I Income
I Capital
Energy sources
presentation.' Thus a firstyear course can be built from an interweaving of material from the first six chapters of Part I with that from the first six of Part II. Some lecturers prefer to use steam, and others air, as a first example of a working fluid. Using the authors' superheat tables, which include internal energy data, the former can give the student an early feel frn: systems whose internal energy is a function of two independent properties. Principles are not obscured by the algebraic manipulation of equations which normally accompany the introduction of the concept of a perfect gas. Those who choose to start with air probably do so because they believe that the student is already familiar with the concept of a perfect gas, and that early manipulation of thermodynamic equations is beneficial. With this approach, care has to be taken to see that the student realises .that a system whose internal energy and enthalpy depend only on temperature is a very special case. There are several decisions 'of this kind that the lecturer has to make; another is whether the Second Law should be dealt with before or after the open system is introduced. We went on to say, in the original Preface, that although a mixture of principle and application is necessary in a ·lecture course, it can leave the student with serious misconceptions. It certainly does not always lead to the firm grasp of principle which enables unfamiliar problems to be tackled. Our object has been to produce a book which distinguishes clearly principle from application. To make full use of this feature, the student should be encouraged to read the first six chapters as revision late in the first year. Experience has shown that the greatest benefit is obtained from such a reading if the student produces two logical trees. These will start from the First and Second Laws respectively, proceeding from the general to the more specific as one moves down the tree. Thus some statements· and equations apply to closed systems and others to open systems; some to any fluid, others only to a perfect gas; some to particular processes and others only when those processes are reversible. Setting out the corollaries of the Second Law as part of this logical sequence is a particularly valuable part. of the exercise. We suggest that although the lecturer might indicate what is required, there should be no handouts of complete trees. The whole exercise loses much of its value in fixing the logical structure of the subject in the mind if the student does not do the work. Effort of this nature should enable the student to appreciate the elegance and power, as well as the limitations, of thermodynamics. Another point we made in the original Preface was that our aim was 'to provide a book of reference to which the student can turn for the elucidation of difficult points. A rigorous approach cannot often be used in a lecture course, partly for lack of time and partly because it would be inappropriate when introducing the student to a new idea. In this book, however, a rigorous proof or explanation is given wherever practicable for the benefit of the better student who is not satisfied with simplifications.' It is worth emphasising here, as stated in a footnote on the first page of the chapter, that Chapter 7 should be omitted at a first reading. Although it appears in Part I, because it is concerned with general thermodynamic principles, it deals with advanced matters which are normally introduced at the end of an undergraduate course or at postgraduate level. It is only fair to say, however, that some of the rigour just referred to cannot be achieved without the knowledge conveyed in that chapter.
xxii
The widespread adoption of SI has made life for students both easier and more difficult. When using properly constructed physical equations in conjunction with coherent SI units, everything drops out easily and correctly but without requiring much thought. As a consequence, students can lose an awareness of the pitfalls which may be encountered when using nonSI units or even legitimate SI multiples; the latter, though legitimate, are not part of the coherent set of units. The student is well advised to digest Appendix A, on dimensions and units, early in the first year. One final word of warning. A manual of solutions to the problems in Appendix B has been produced for the benefit of teachers and students who do not have easy access to helpful discussions with others. Students who look at any solutions manual before attempting the problems are wasting their time; not only will they learn little, but worse still they will be deceiving themselves into thinking they know something when they do not.
xxiii
Part I Principles of Thermodynamics
Introduction
In this book the student will be introduced to a wide range of engineering plant: steam turbines, reciprocating engines, turbojets and rockets, combustion systems, refrigerators and heat pumps, direct conversion devices such as fuel cells, compressors, boilers, condensers, cooling towers and heat exchangers. What determines their place in the book is that they are concerned with the transfer of heat and work, in many cases with the ultimate object of converting one form of energy into another. In every case they make use of the way a fluid behaves as it is compressed or expanded, heated or cooled. These features imply that the design of the equipment must involve the science of thermodynamics, because this is the science dealing with the relations between the properties of a substance and the quantities of 'work' and `heat' which cause a change of state. Before a satisfactory analysis of such changes can be made, it is necessary to introduce some carefully defined concepts. The idea of a system plays an important part in thermodynamics; it may be defined as a region in space containing a quantity of matter whose behaviour is being investigated. This quantity of matter is separated from its surroundings by a boundary, which may be a physical boundary, such as the walls of a vessel, or some imaginary surface enveloping the region. Before any thermodynamic analysis is attempted it is essential to define the boundary of the system, because it is across the boundary that work and heat are said to be transferred. The term surroundings is restricted to those portions of matter external to the system which are affected by changes occurring within the system. When the same matter remains within the region throughout the process under investigation it is called a closed system, and only work and heat cross the boundary. An open system, on the other hand, is a region in space defined by a boundary across which matter may flow in addition to work and heat. Part I is primarily concerned with the behaviour of a particular form of :!,;tfor — a simple fluid. A simple fluid may be a gas (e.g. oxygen), a vapour (e.g. steam), a liquid, or a mixture of such substances provided they do not react chemically with one another (e.g. dry or humid air). Closed and open systems containing such fluids are the main concern of engineering thermodynamics. Chemical and physical thermodynamics deal with a wider variety of systems
3
Principles of Thermodynamics
and phenomena, .e.g. solids, surface films, electric cells, mixtures undergoing chemical reactions, thermoelectric effects, and magnetic substances (see Refs 5 and 8). These are not the main concern of this book, although some consideration is given in Part II to the chemical reactions involved in the combustion of fuel, and in Part III there is a brief introduction to thermoelectric and other phenomena which make possible the direct conversion of an energy source into electricity. It follows that in Part I, and indeed for most of the book, a system may be defined less generally as a region in space containing a quantity of fluid. If the fluid is flowing into, out of, or through the region, it is an open system. Some examples are (a) a gas expanding from a container through a nozzle, (b) steam flowing through a turbine, and (c) water entering a boiler and leaving as steam. Examples of a closed system are (a) a mixture of water and steam in a closed vessel, and (b) a gas expanding in a cylinder by displacing a piston. From the last example it will be seen that the boundary separating a closed system from its surroundings need not be fixed; it may expand or contract to accommodate any change of volume undergone by the fixed quantity of fluid. The processes undergone by the fluid in a closed system are described as nonflow processes, whereas those undergone by the fluid in an open system are referred to as flow processes.
When chemical, surface tension, electrical and magnetic effects are absent, any closed system can only change its condition or state for one or both of the following reasons: (a) there will be a change of state if a part of the boundary is displaced by a force so that some mechanical work is done, e.g. when a force is applied to a piston to compress a gas; (b) there will be a change of state if the system is brought into contact with a portion of the surroundings which is at a different temperature, i.e. if heat is allowed to flow across the boundary. Thus the engineer is concerned to know the way in which the state of a system changes when work and heat cross the boundary. The state* of a system at any given instant is determined by the values of its properties at that instant. The sort of characteristic which can be used to describe the condition of any object under investigation must always be found by experience, and will depend upon the nature of the investigation. From the standpoint of thermodynamics, many observable characteristics will be irrelevant; for example, shape and colour are irrelevant characteristics of the systems considered in this book. On the other hand, shape would be an important characteristic of any thermodynamic system involving surface tension effects. Those characteristics of a system which can be used to describe its condition or state, and which are relevant to the investigation, are termed the properties of the system. These properties are not all independent of one another; for example, for a perfect gas it is known that the temperature must have a definite value if the pressure and volume are fixed, in accordance with the wellknown equation of state pv = RT. Classical thermodynamics has been built up from a * The term 'state' is sometimes used in textbooks on heat to refer to the solid, liquid or vapour form of a substance, but these forms are referred to as 'phases' in thermodynamics.
4
Introduction
study of closed systems, and it has been found by experiment* that only two properties are necessary and sufficient to determine the state of a closed system containing a simple fluid. This state may be termed the thermodynamic state of the fluid, and the properties of the fluid from which these two may be chosen are called the thermodynamic properties. When the thermodynamic state has been determined by a knoMedge of two thermodynamic properties, any third thermodynamic property can be found from a relation expressing it as a function of the two known properties. It will be assumed in Part I that these relations have been determined by experiment for all the fluids likely to be used in engineering systems; the equation of state of a perfect gas is merely one such relation. The study of open systems is complicated by the fact that the fluid is in motion. If attention is concentrated on a portion of the fluid entering the system, it will be realised that it posseses a relevant mechanical state in addition to a thermodynamic state. The mechanical properties necessary to determine its mechanical state are (a) velocity relative to the fixed boundary of the system and (b) position in the gravitational field, i.e. height above some datum level. Both these characteristics may change during the passage of the fluid through the system, and they may affect events which occur within the system and the work and heat which cross the boundary; they cannot therefore be omitted from an analysis of open systems. The two mechanical properties are independent of one another and, moreover, are independent of the thermodynamic properties. For example, the fact that a perfect gas is flowing through a pipe with a certain velocity in no way changes the fact that at any point the pressure, volume and temperature of an element of the gas are related by pv = RT. All the relations between the thermodynamic properties which will be developed in the following pages are similarly independent of whether the fluid is in motion or changing its position in the gravitational field. Thus the mechanical state is something which can be superimposed upon the thermodynamic state without disturbing the relations between the thermodynamic properties. It will appear later that this makes it possible for the body of knowledge built up from a study of closed systems to be applied to the analysis of open systems. We are now in a position to summarise the contents of Part I, which present the fundamentals of thermodynamics without reference to any particular fluid. First, we note that experiment has shown that the state of a closed system is determined when two thermodynamic properties are known, and that all the other thermodynamic properties are then determined. We shall assume that sufficient experimental information is available to enable any third thermodynamic property to be found if two are known. Secondly, the state of a system changes when work or heat cross the boundary. Thermodynamics provides a means of relating the quantities of heat and work with the change of state, i.e. with the variation of the properties of the fluid. The structure of thermodynamics * Advanced students will find an interesting logical analysis of this procedure in Ref. 2, Chapter 1.
5
Principles of Thermodynamics
rests upon two important principles called the First and Second Laws of Thermodynamics. These cannot be proved and are treated as axioms; their validity rests upon the fact that neither they, nor any deductions made from them, have ever been disproved by experience. The First Law is initially stated with reference to closed systems, and it is applied to various processes which such systems may undergo. It is then applied to open systems. The First Law is an expression of the principle of the conservation of energy. With the aid of this law it is possible to calculate the quantities of heat and work which cross the boundary of a system when given changes in properties occur, e.g. the work done by steam expanding through a given range of pressure in a turbine, the work required to produce a given pressure rise in an air compressor, or the heat required to generate steam at a given pressure in a boiler. A second class of problems is concerned with how much of the heat, normally supplied by burning fuel, can be converted into work by a heat engine; or, again, how much work is required to extract a given amount of heat from a body in a refrigerator. These are problems concerning the efficiency of power plant, and they can be solved with the aid of the Second Law of Thermodynamics. The Second Law is an expression of the fact that it is impossible to convert all the heat supplied to an engine into work; some heat must always be rejected, representing a waste of energy. As with the First Law, the second is enunciated with reference to closed systems, and then its consequences for open systems are deduced. In the final chapter, which may be omitted on a first reading, some important general relations between the thermodynamic properties are deduced from the First and Second Laws. This introduction opened with a list of engineering plant, in the design of which thermodynamics plays a vital role. It may not be out of place to end it with a reminder that the complete design of any of the plant mentioned must involve other engineering sciences, such as mechanics of machines and properties of materials. The engineer will be concerned not only with the behaviour of the working fluid, but also with the stresses and strains and vibrtion problems that are inevitable consequences of trying to meet the thermodynamic requirements as economically as possible. No student of engineering — however science based his courses may be — should forget that his ultimate aim is the design of new equipment which is both more efficient in operation, and cheaper to produce and maintain, than its predecessor. The natural resources of our planet are not unlimited.
6
1 Fundamental Concepts
Before the basic structure of thermodynamics can be outlined, it is necessary to define some of the concepts more thoroughly than has been attempted in the Introduction to Part I, paying particular attention to temperature, work and heat. Accordingly, this chapter is devoted to a discussion of such fundamental concepts. We shall have in mind here only closed systems, consisting of a simple fluid in the absence of chemical, surface tension, electrical and magnetic effects.
1.1 Thermodynamic properties
The idea of a system has been presented in the Introduction to Part I. A closed system is fully defined when the following details are known:
(a) The fluid, e.g. air, hydrogen or water (b) The boundary between the fluid under consideration and its surroundings (c) The mass of fluid with the boundary.
The state of the system has yet to be determined; for this a knowledge of its properties is required. To define the state of a closed system, only the thermodynamic properties of the fluid are relevant. Any such property must be some characteristic that can be measured, and it must have a unique numerical value when the fluid is in any particular state. Pressure, volume and temperature are obvious examples. The value of a property must be independent of the process through which the fluid has passed in reaching that state. It follows that a change in the value of a property depends only on the initial and final states of the systems, and is independent of the process undergone by the system during the change of state. Using pressure as an example, a gas at state 1 may have a pressure of 5 atm, and after a compression process to state 2 a pressure of 8 atm. The change in pressure is an increase of 3 atm however the compression is carried out. If dP is any infinitesimal change in a property during a process, the total change between 7
Principles of Thermodynamics
[1.1]
states 1 and 2 can be written as 1'2
dP = P2  P1 1
Mathematically speaking, dP is an exact differential.* Consider the following mechanical analogy. A cyclist travels from point 1 at a height z1 above sea level, to point 2 on a hill z2 above sea level. Treating the cyclist as the system, his height above sea level can be regarded as a property of the system because the change in height (z2 — z1) is independent of the path, i.e. the process, by which the cyclist travels from 1 to 2. The work done by the cyclist, however, is not independent of the process; it clearly depends upon whether he has chosen a short or long route between 1 and 2 and whether he has a following or head wind. Consequently the work done, although a measurable quantity, is not a property. If, during any infinitesimal part of a process, a measurable quantity which depends upon the process is denoted by dX, dX is not an exact differential and f 2
dX
X2 
X1
When the quantity is not a property, the integration between state 1 and state 2 must be written as 2
dX = X12 (or simply as X) Further discussion of quantities which are not properties will be deferred to section 1.3, which deals with the concepts of work and heat. We have already noted the experimental fact that when the values of two properties are known, the state of a closed system is completely determined. An important assumption is implicit in this statement, i.e. that the system is in thermodynamic equilibrium. A system is said to be in thermodynamic equilibrium if no further changes occur within it when it is isolated from the surroundings in such a way that no heat and work can cross the boundary. The properties, such as pressure and temperature, must be uniform throughout the system when it is in equilibrium. If the pressure is not uniform, owing to turbulence for example, spontaneous internal changes occur in the isolated system until the turbulence has died down and the pressure has become uniform. Similarly, if there are temperature gradients in the isolated system, a spontaneous redistribution of temperature occurs until all parts of the system are at the same temperature. Only under conditions of equilibrium can single values of pressure and temperature be ascribed to the system, and thus be used to determine its state. It will always be assumed in this book that the system is in equilibrium at the beginning and end of any process, and therefore that the end states are determined when the values of two properties are fixed.
It follows that the initial and final states of any closed system can be located * The concept of an exact differential is defined in Chapter 7.
8
[1.1]
Fundamental Concepts
as points on a diagram using two properties as coordinates. If the system is imagined to pass through a continuous series of equilibrium states during the process, the intermediate states could also be located on the diagram, and a line representing the path of the process could be drawn through all the points. Such a process is called a reversible process; it will be found to be an ideal process analogous to the frictionless process so often referred to in mechanics. In all real processes, however, the system is not in equilibrium in any of the intermediate states. These states cannot be located on the coordinate diagram because the properties do not have single unique values throughout the system. Such processes are called irreversible processes. They are best represented on a diagram by a dotted line joining the initial and final state points, to indicate that the intermediate points are indeterminate. Such a line indicates mean values of the properties during the process. The full significance of the ideas of reversibility and irreversibility will appear later. Pressure, specific volume and temperature are three properties observable by the senses. Pressure p is defined as the force exerted by the fluid on unit area of the boundary, and the unit* we normally employ is the bar (1 bar = 105 N/m2 = 1 /1.013 25 atm). The specific volume v is the volume of unit mass of fluid, usually quoted in m3/kg. It is the reciprocal of the density p, defined as mass per unit volume, but it is conventional to use specific volume rather than density as one of the properties in thermodynamics. Temperature is a property deserving special attention and it will be introduced in section 1.2. Three more thermodynamic properties — internal energy, enthalpy and entropy — will emerge as consequences of the First and Second Laws of Thermodynamics. Although they are not directly observable by the senses, they are essential to the structure of thermodynamics. From these six properties, two may be selected to determine the state of a closed system in thermodynamic equilibrium, and the values of the remaining four are then fixed. Care must be taken to see that the two chosen properties are independent of one another, i.e. it must be possible to vary one of these properties without changing the other. Obviously p and v are not independent properties because one is simply the reciprocal of the other; this fact is recognized in that density is not included in the six properties to which refererice was made. But, less obviously, pressure and temperature are not always independent properties: when a liquid is in contact with its vapour in a closed vessel, it is found that the temperature at which the liquid and vapour are in equilibrium is always associated with a particular pressure and one cannot be changed without the other. Pressure and temperature cannot be used to determine the state of such systems, although other pairs, such as pressure and specific volume, may be so used. As stated in the Introduction, it will be assumed throughout Part I that if any two independent properties are known, the others can be found from experimental data relating to the particular fluid under consideration. If, for example, p and v are known, any third property x must be a function of these * The INI;m 2 is called the pascal (Pa), so I bar = 105 Pa. Dimensions and units are discussed in Appendix A.
9
[1.2]
Principles of Thermodynamics Fig. 1.1 I),
Vz
•
•
•
•
•
•
Va
VI,
Pa
•
Pb
•
Table of properties
_
Values of temperature (or internal energy or enthalpy or entropy)
i I I Py
•
•
•
•
Pr
•
•
•
a
two, i.e. x = (13.(p, v). For some fluids the functions are simple, and algebraic equations are used to relate the properties; for others the function is complicated and the experimental data are most conveniently presented in tabular form. Fig. 1.1 shows such a table, the dots denoting values of temperature corresponding to the various combinations of p and v. Similar tables can be prepared with internal energy, enthalpy or entropy as the third property. It is assumed in Part I that either a set of equations or a set of tables is available for each fluid likely to be encountered in engineering systems. 1.2 Temperature
Two systems are said to have equal temperatures if there is no change in any of their observable characteristics when they are brought into contact with one another. Consider a system A consisting of a gas enclosed in a vessel of fixed volume fitted with a pressure gauge. If there is no change of pressure when this system is brought into contact with a second system B, say a block of metal, then the two systems are said to have the same temperature. Experiment shows that if the system A is brought into contact with a third system C, again with no change of pressure, then B and C when brought into contact will also show no change in their characteristics. That is, if two bodies are each equal in temperature to a third body they are equal in temperature to each other. This principle of thermal equilibrium is often called the zeroth law of thermodynamics; the possibility of devising a means of measuring temperature rests upon this principle. The temperatures of any group of systems may be compared by bringing a particular system, known as the thermometer, into contact with each in turn. System A performs this function in the foregoing example. Such a system must possess an easily observable characteristic termed a thermometric property, e.g. the pressure of a gas in a closed vessel, the length of a column of mercury in a capillary tube, or the resistance of a platinum wire. A scale of temperature could be defined by assigning numbers to divisions on the pressure gauge, to points spaced at intervals on the capillary tube, or to divisions on the meter registering the resistance of the wire; units so formed are called degrees of 10
[1.3]
Fundamental Concepts
temperature. These temperatures scales would be quite arbitrary, and each instrument would have its own scale. The necessary conditions for a temperature scale to be reproducible when any given thermometric property is used will be discussed in Chapter 8, as well as the means adopted for comparing scales resulting from the use of different thermometric properties. The reason for postponing the definition of temperature scales is that the practical procedure of constructing an empirical scale of temperature is irrelevant to the structure of thermodynamics. It will be shown that a temperature scale can be defined as a consequence of the Second Law of Thermodynamics without reference to any particular thermometric property, and consequently this has been adopted as the ultimate standard. In Part I, where the analysis is carried out only in symbolic form, no numerical scale need be assigned to the property temperature. The qualitative terms 'high' and low' will be used, however, thereby adopting the conventional terminology which originates from our sense of hotness and coldness. 1.3 Work and heat
The limitations placed upon the closed systems considered here* imply that only the application of work or heat can cause a change of state, or conversely that a change of state must be accompanied by the appearance of work or heat at the boundary. As in mechanics, work is said to be done when a force moves through a distance. If part of the boundary of a system undergoes a displacement under the action of a pressure, the work done W is the product of the force (pressure x area) and the distance it moves in the direction of the force. Fig. 1.2a illustrates this with the conventional piston and cylinder arrangement, the heavy line defining the boundary of the system. The base unit of work in the SI system is the newton metre (N m), also called the joule (J); we shall use the more convenient kilojoule (kJ) which is 10' N m. Fig. 1.2b illustrates another way in which work might be applied to a system. Here the boundary really consists of the inner surface of the vessel and the surfaces of the paddle. A force is exerted by the paddle as it changes the momentum of the fluid, and since this force moves during the rotation of the paddle some work is done. To calculate the paddle work it would be necessary to know all the forces acting on the paddle Fig. 1.2 Moving part of boundary
Work due to movement of part of a boundary
Moving part of boundary
Fixed boundary
I W(+)
W (+)
Rotor shaft
(a)
(b)
(c)
* See Chapter 20 for a brief discussion of a broader concept of work.
11
[1.3]
Principles of Thermodynamics
or rotor surfaces and their displacements; this information would be difficult to obtain in practice. For this reason, when work is transmitted via a shaft it is more convenient to include within the system boundary the paddle (or rotor) and the shaft up to the section at the boundary, as shown in Fig. 1.2c. The work transmitted across the boundary so defined is then calculated from the product of the torque and the angular displacement of the shaft. The analogy of the cyclist was used in section 1.1 to indicate that work is a quantity which is not a property of a system. Work is a transient quantity which only appears at the boundary while a change of state is taking place within a system. Work is' something' which appears at the boundary when a system changes its state due to the movement of la part of the boundary under the action of a force. Although there cannot be said to be any work in a system either before or after the change has taken place, work may be said to 'flow' or 'be transferred' across the boundary. This is a somewhat loose way of speaking; it will be shown in the next phapter that it is 'energy' which is transferred, and that work is the particular form of energy transfer associated with the movement of a force at the boundary. Heat, denoted by the symbol Q, may be defined in an analogous way to work as follows. Heat is `something' which appears .at the boundary when a system changes its state due to a difference in temperature between the system and its surroundings. Again anticipating the next chapter, the 'something' is a form of energy transfer, this time the form associated with a temperature difference. Heat, like work, is a transient quantity which only appears at the boundary while a change is taking place within the system. It is apparent that neither d W nor dQ is an exact differential (section 1.1), and therefore any integration of the elemental quantities of work or heat which appear during a change from state 1 to state 2 must be written as 2 J
dW =
2 W12
(or W) and
dQ =
Q12
(or Q)
Although in thermodynamics there cannot be said to be any heat in a system either before or after a change of state, loosely speaking heat may be said to 'flow' or 'be transferred' across the boundary. Strictly speaking it is energy which is transferred, but to say 'the heat transferred' is a shorthand way of saying 'the energy transferred by virtue of a temperature difference'.* It is necessary to adopt a sign convention to indicate the direction in which the work and heat flow. The traditional sign convention in engineering has been to take the work done by the system on the surroundings as positive, and heat flow from the surroundings into the system as positive. It arose from the fact that the science of thermodynamics grew out of the need to explain the behaviour of heat engines, which are essentially devices where there is a net flow of heat into the system and a net flow of work out of it. It seemed natural
* Strictly speaking, the word 'heat' alone means this just as the word 'pedestrian' means 'a man transporting himself on foot'. However, our language requires an explicit verb in a sentence; so we say 'heat is transferred from A to B' and 'there is a pedestrian walking in the road'.
12
Fundamental Concepts
[1.3]
to choose these as the positive quantities. Thermodynamics now has much wider application, and physicists, chemical engineers and most European engineers have found it more logical to take all flows into a system as positive — whether of heat, work, or fluid mass and momentum which play a prominent part in open systems. We propose to adopt the newer convention for this and subsequent editions of the book. Thus: Work done by the surroundings on the system and heat flowing from the surroundings into the system are taken as positive. Conversely: Work done by the system on the surroundings and heat flowing from the system into the surroundings are taken as negative. The exact definition of the unit of heat must be deferred until the concept of energy has been introduced formally. The old calorimetric definition may be mentioned, however; it is so called because it originates from the early experiments on heat carried out with calorimeters. The unit of heat was defined as that quantity which would raise the temperature of unit mass of water, at standard atmospheric pressure, through one degree on some temperature scale. Not only does the unit depend upon the temperature scale used, but careful experiments showed that a slightly different quantity of heat was necessary at different points on the chosen temperature scale, i.e. the unit depended on the temperature of the water at the beginning of the onedegree rise. Thus a unit called the kilocalorie (kcal) was defined originally as the heat required to raise one kilogram of water one degree on the Celsius scale of temperature. (Similarly, the British thermal unit (Btu) and Celsius heat unit (Chu) were defined as the quantities of heat required to raise one pound of water one degree Fahrenheit and one degree Celsius respectively.) Later, more carefully defined units were used, such as the 15 °C kcal for which the temperature rise must be from 14.5 to 15.5 °C. Socalled calorimetric heat units are still in use; for most practical purposes these are identical with calorimetric units defined in terms of the properties of water, but these calorimetric units are now defined in terms of work units. This is discussed further in section 2.3. Summarising: neither heat nor work is a property of a system, but both are transient quantities, only appearing at the boundary while a change of state occurs within the system. Although they cannot, therefore, be used to describe the state of a system, heat and work can be used to describe the process undergone by the system during a change of state. For example, using the cyclist analogy, the work done by the cyclist might indicate whether he had chosen a short or long route. Or again, consider a vessel of constant volume containing a gas. Let the gas undergo a change of state in such a way that the pressure and temperature are increased. This change could be obtained by placing the vessel in contact with a body at a higher temperature, or as in Fig. 1.2b by churning the gas with a rotating paddle. Thus the same final state could be 13
Principles of Thermodynamics
[1.3]
reached by the provision of either heat or work. Moreover, both heat and work could be added simultaneously in an infinite number of different proportions to produce the same final state. From this example it is clear that quantities of heat and work are functions not only of the initial and final states of the system, but also of the process undergone by the system.
14
2 The First Law of Thermodynamics
The structure of thermodynamics rests upon two fundamental laws. The First Law, introduced in this chapter, is concerned with the principle of conservation of energy as applied to closed systems which undergo changes of state due to transfers of work and heat across the boundary. The First Law cannot be proved; its validity rests upon the fact that neither it, nor any of its consequences, have ever been contradicted by experience.
2.1 The cycle
A closed system is said to undergo a cyclic process, or cycle, when it passes through a series of states in such a way that its final state is equal in all respects to its initial state. This implies that all its properties have regained their initial values. The system is then in a position to be put through the same cycle of events again, and the procedure may be repeated indefinitely. Work can be transferred continuously by devising machines which undergo cyclic processes. Consider the simple, idealised, mechanical system consisting of a frictionless pulley and a weightless rope shown in Fig. 2.1a. Let a force be applied to raise the weight through a certain distance, a force only infinitesimally greater than the weight. Work is done on the system, and hence the quantity is positive. Now let the weight descend slowly to its original position by reducing the force until it is infinitesimally smaller than the weight (Fig. 2.1b). Since the pulley is frictionless, an infinitesimal difference between the weight and the applied force is sufficient to set the system in motion. The system does work on the surroundings in overcoming the applied force (it could, in fact, be used to raise another weight), so that this time the quantity is negative. The system has now returned to its original state and, in the limit, both quantities of work are equal in magnitude. For the whole cyclic process, therefore, EW=0 A circle on the summation sign is used to signify that the algebraic summation of all the increments of work SW is carried out over a complete cycle. Now consider what happens if, for the second part of the cycle, the force is removed from the rope and a brake shoe is applied to the pulley to restrain the downward acceleration of the weight (Fig. 2.1c). When the weight has been 15
[2.2]
Principles of Thermodynamics Fig. 2.1 A cyclic process
Boundary
OW
(a)
oW
(b)
(c)
restored to its original position, it will be noticed that the system has not reached its initial state in all respects, for the temperature of the pulley and brake shoe is higher than it was originally. To restore the system to its original state and so complete the cycle, heat may be permitted to flow across the boundary of the system. If desired, the quantity of heat may be measured by allowing it to raise the temperature of water in a calorimeter. This process is illustrated diagrammatically in Fig. 2.1c. As no force moves in the surroundings of the system during the last part of the cycle, no work is done, and E SW 0 0 The net work done during this cycle is a positive quantity equal to the work required to raise the weight initially. On the other hand, a quantity of heat has crossed the boundary into the surroundings (i.e. the calorimeter). Since. no heat crosses the boundary in the first part of the cycle and a negative quantity appears in the second, E 812 0 0 and is negative. From this experiment it appears that when a system is taken through a complete cycle, the algebraic summation of the quantities of either work or heat which cross the boundary may have some value other than zero. Since the change in the value of any property over a complete cycle must be zero, because the initial and final states are identical, this is a further illustration of the fact that work and heat are not properties of a system. 2.2 The First Law of Thermodynamics
Experiments similar to those described in section 2.1 were first carried out. by Joule (1843). He found that the net quantity of heat delivered by the system was directly proportional to the net quantity of work done on the system during the cycle. The First Law of Thermodynamics may be expressed as a generalisation 16
[2.2]
The First Law of Thermodynamics
of this result covering all cyclic processes, irrespective of whether net amounts of heat and work are supplied to the system or to the surroundings; the only constraint is that if one is net into the system, the other must be net out of the system. Because of the historical association of the first law with heat engine cycles, namely cycles producing a net amount of work on the surroundings, the law is usually stated in the following form: When any closed system is taken through a cycle, the net work delivered to the surroundings is proportional to the net heat taken from the surroundings. However, the converse is also true, namely: When a closed system is taken through a cycle, the net work done on the system is proportional to the net heat delivered to the surroundings. In this latter form, the statement relates to heat pump and refrigerator cycles. These statements may be expressed in mathematical form by E SQ oc E SW and E SQ cc. E,SW net in
net out
net out
(2.1)
net in
In section 2.3 we shall reconcile these mathematical statements with our sign convention, thereby merging the two statements into one. A simple type of cyclic process is indicated in Fig. 2.2. The system is a gas enclosed by a cylinder and piston. If a source of heat is applied to the system the gas expands, pushing the piston before it and doing work on the surroundings; the gas may then be returned to its original st. e by applying a sink of heat, i.e. a body at a lower temperature than the gas. In the second part of the cycle, the gas contracts and some work is done by the surrounding as the piston moves inwards. This is a straightforward closed system undergoing a series of nonflow processes during which the fluid does not move bodily but merely expands and contracts. The First Law is adopted as an axiom and provides one of the two foundation stones upon which the structure of classical thermodynamics rests. Joule's experiments, and others of the same nature, are not proofs of the First Law; they merely lend support for its adoption as an axiom by providing instances which do not contradict the law. A proof could only be formulated if the First Law could be shown to be a consequence of some even broader and more general
Fig. 2.2 A simple cycle undergone by a gas ?
OW 8Q (
ow
17
[2.3]
Principles of Thermodynamics
proposition about nature.* Certain propositions about the behaviour of thermodynamic systems can be deduced from the laws of thermodynamics; they may be termed corollaries. These corollaries are often most conveniently proved by reductio ad absurdum, i.e. the contrary of a proposition is assumed to be true, and the consequences are then shown to lead to a contradiction of The fundamental axiom. Before deducing the corollaries of the First Law, which help to bring out all its implications, the constant of proportionality implicit in the expression (2.1) will be discussed.
2.3 Mechanical equivalent of heat
If the constant of proportionality is denoted by /, and taking due account of the sign convention, expression (2.1) can be rewritten as f ESQ + EN/ = 0
(2.2)
/ is called the mechanical equivalent of heat or Joule's equivalent; it expresses the number of work units which are equivalent to one heat unit. Once a work unit and a heat unit have been adopted, experiments such as those carried out by Joule can be used to find the value of /. For such experiments it has been customary to use a calorimetric definition of the unit of heat. If the kJ and the kcal are chosen as the units of work and heat respectively, the value of is found to be approximately 4.19 kJ/kcal. Similarly in the older, but now obsolete, systems of units, / ,;.1427
kgf m N kcal
778
ft lbf N Btu
1400
ft lbf Chu
These values are sufficiently accurate for most engineering calculations when both calorimetric and mechanical units are employed. Strictly speaking, once the First Law has been established and heat and work are interpreted as forms of energy transfer, the need for separate units vanishes. Certainly there is no justification for two sets of absolute standards, e.g. the primary standards of mass, length and time to which the unit of work may be referred, and a standard thermometer and mass of water of a certain purity to which the unit of heat may be referred. This was recognised in 1929 when the First International Steam Table Conference decided to define a heat unit in terms of a work unit. The definition accepted today was laid down at the Fifth International Conference on the Properties of Steam (1956) in terms of the joule (J) as the standard unit of work (see Appendix A). A heat unit defined in terms of the joule depends only on the primary standards of mass, length and time. This International Table kilocalorie, unit symbol kcal, although * Indeed this has been done by Keenan and Hatsopoulos, who showed that both the First and Second Laws are consequences of a more basic generalisation about the existence of stable states (i.e. about the fact that there are states which cannot undergo a finite change without a permanent finite change in the environment). This work is best described in Ref. I I.
18
The First Law of Thermodynamics
[2.4]
often written without the subscripts, is defined as 1 kcal, = 4.1868 kJ The number was chosen so that calorimetric methods of measuring quantities of heat can still be used for ordinary purposes.* Another kilocalorie defined in terms of the joule, and still used in physical chemistry, is the thermochemical kilocalorie defined as 1 kcal", = 4.184 kJ Since no fundamental distinction can now be made between the unit of heat and the unit of work, and the 'mechanical equivalent of heat' / is recognised merely to be a conversion factor between different units, / can be dropped from equation (2.2), which can now be written as E SQ + E SW = 0
(2.3)
It is understood that the same unit, for us the kJ, is used consistently for both heat and work. Equation ( 2.3), in conjunction with our sign convention, can now be taken to express the First Law. Some of the corollaries of the First Law may now be considered. 2.4 Corollaries of the First Law
Corollary 1 There exists a proper change in its value is equal to th transfers during any change of st Proof Assume that the converse of the , .e. that E(SQ + SW) depends upon the process, as well as upon the end states 1 and 2, and so cannot be equal to the change in a property. The procedure is to show that this contradicts the First Law. Consider any two processes A and B by which a system can change from state 1 to state 2 (Fig. 2.3). The assumption is that in general (2.4)
(502 + 814 )A E (8Q + 614/)8
The subscripts A and B are used to indicate the process for which the summation is carried out. In each case let the system return to its original state by a third * Bearing in mind that I kgf = 9.80665 N, the kcal is related to the metric technical unit of work by 1 kcal =
4.1868 x 10' kgf m = 426.935 kgf m 9.806 65
The old British units are related to the kJ by the definitions 1.8
Btu lb
=1
Chu lb
= 4.1868
kJ which lead to 1 ft lbf — kg
1 778.169
Btu =
I
Chu
1400.70
These definitions ensure that specific heat capacities in calorimetric units are numerically identical in all systems of units — see section 8.2.2.
19
[2.4]
Principles of Thermodynamics Fig. 2.3 Proof of existence of a property 'internal energy'
O
0.
Property Y
process C. For each of the complete cycles AC and BC so formed, we have
E (8Q +
SW) Ac = (8i2 + 8 W)A + (sQ 1 2
+ svi)c
2
E ( 612 + W)Bc = E ( 812 + 1
+ (802 + W)c 2
If the assumption described by the inequality (2.4) is true, it follows that
E( 812 + W)Ac
E 8Q + 8 Mac
But this contradicts the First Law expressed by equation (2.3), which implies that these quantities must be equal since they are both zero. Therefore the original proposition, that Ef(SQ + dW) is independent of the process, must be true. If the property so discovered is denoted by U, the corollary can be expressed mathematically as 2
(812 + SW) = U2 —
U1
1 Or, writing Q12 and W12 for the net quantities of heat and work crossing the boundary during the change of state, Q12 + W12 = (U2
U1)
(2.5)
Q and W carry the subscript 12 to indicate that the process follows some path between states 1 and 2 at which the internal energies are U 1 and U2. Normally we shall omit the subscript on Q and W when the end states are selfevident. When considering a succession of processes, however, it will often be helpful to indicate the steps by retaining the subscripts and writing (Q, 2 + W12), (Q2 3 + W23 ) and so on. The property U is called the internal energy of the system, and equation (2.5) is called the nonflow energy equation. Expressed verbally: the increase in internal energy of a closed system is equal to the heat supplied to the system plus the work done on the system. The adjective 'internal' has been adopted to distinguish this form of energy from mechanical forms which might be superimposed on the system. Thus if the system is moving as a whole and changing its position 20
The First Law of Thermodynamics
[2.4] Boundary
Fig. 2.4 The importance of defining the boundary of a system Redistribution of internal energy
Flow of heat
(a)
(b)
in the gravitational field, we know from mechaniCs that the system will possess kinetic and potential energy in addition to internal energy. It should be noted that the First Law is more than a mere definition of the internal energy by a statement to the effect that SU = 8$2 + SW It states that the internal energy is a quantity different in kind from the quantities of work and heat. Internal energy, being a property, can be said to reside in the system and it can be increased or decreased by a change of state. It is only energy which can truly be said to flow across the boundary, and the terms 'work' and `heat' simply refer to two different causes of the flow of energy. As already stated, if the flow occurs as the result of the movement of a force at the boundary it is termed work, and if it occurs because of a temperature difference between the system and surroundings it is called heat. Suppose a system consists of two bodies at different temperatures, the boundary being imagined to be an insulating wall isolating the two bodies from their surroundings (Fig. 2.4a). This would represent a system in a nonequilibrium state, since at least one property, temperature, is not uniform throughout the system. Energy will flow from one body to another until the temperatures are identical, when the system will be in equilibrium and any property will have the same value in all parts of the system. The term 'heat' has no meaning in this situation as no energy crosses the boundary. On the other hand, if one body is considered to be the system and the other to be part of its surroundings as in Fig. 2.4b, and energy flows from one to the other owing to the temperature difference, then heat is said to cross the boundary. It follows that the first step in the enunciation of any thermodynamic problem must be to define the system. The terms in any physical equation must have the same dimensions and be expressed in the same units. Since Q and W are to be expressed in kJ, U must be in kJ; but if Q and W were in kcal then U would also be in kcal. It is important to notice that the energy equation is concerned with changes in internal energy. The First Law suggests no means for assigning an absolute value to the internal energy of a system at any given state. For practical purposes, however, it is possible to adopt some state, say state 0, at which the energy is arbitrarily taken to be zero, and then find the changes of energy when the system proceeds from this reference state to a series of states 1, 2, 3 etc. In this way values of U 1 , U2 , U3 etc. can be found and tabulated as in Fig. 1.1, although they are strictly values of (U1 — U0), ( U2 — U0), ( U3 — U0) etc. In all engineering applications of thermodynamics only changes in energy are of 21
Principles of Thermodynamics
[2.4]
interest, and consequently what state is chosen as the reference state is unimportant. For example, between states 2 and 3, defined say by the values (p2, v2) and (p3, v3), the change of internal energy can be found from the table of properties as ( U3 — U2). The quantity ( U3 — U2 ) is strictly ( U3 — U0) — ( U2 — U0) but, since U0 cancels, the reference state is irrelevant. Although latent forms of energy due to chemical and nuclear bonds are present in the fluid, these forms remain constant in any change of state during which chemical and nuclear reactions do not take place. The only forms of energy which can change are those associated, on the kinetic theory of fluids, with the kinetic energy of the molecules and the potential energy due to intermolecular forces; 'random molecular energy' might be used as a collective term when thinking of the mechanical model. It is this random molecular energy which is envisaged when the term 'internal energy' is applied to a closed system in equilibrium. When the system is not in equilibrium, the internal energy can include macroscopic mechanical forms, both kinetic and potential, associated with the movement of relatively largescale elements of fluid; under these circumstances the symbol E will be used in place of U. The internal energy quoted in tables of properties always refers to the fluid when in a state of equilibrium. The internal energy of a closed system remains unchanged if the system is isolated from its surroundings.
Corollary 2
No formal proof of this proposition is required once the first corollary has been established; it follows directly from equation (2.5). If the system is isolated from its surroundings, Q and W are both zero and hence AU must be zero. The system represented by Fig. 2.4a is an example of an isolated system. All that happens in this case is a spontaneous redistribution of energy between parts of the system which continues until a state of equilibrium is reached; there is no change in the total quantity of energy within the system during the process. Corollary 2 is often called the Law of Conservation of Energy. It is sometimes loosely applied to the whole universe to suggest that the energy of the universe is constant. Such an extrapolation may be admissible only if the universe can be regarded as finite, because the proposition has been inferred from our experience of finite systems. 3 A perpetual motion machine of the first kind is impossible.
Corollary
The perpetual motion machine was originally conceived as a purely mechanical contrivance which, when once set in motion, would continue to run for ever. Such a machine would be merely a curiosity of no practical value, and we know that the presence of friction makes it impossible. What would be of immense value is a machine producing a continuous supply of work without absorbing 22
[2.4]
The First Law of Thermodynamics
energy from the surroundings; such a machine is called a perpetual motion machine of the first kind. It is always possible to devise a machine to deliver a limited quantity of work without requiring a source of energy in the surroundings. For example, a gas compressed behind a piston will expand and do work at the expense of the internal energy of the gas. Such a device cannot produce work continuously, however; for this to be achieved the machine must be capable of undergoing a succession of cyclic processes. But equation (2.3) states that if a net amount of heat is not supplied by the surroundings during a cycle, no net amount of work can be delivered by the system. Thus the First Law implies that a perpetual motion machine of the first kind is impossible.
23
3 NonFlow Processes
In this chapter the nonflow energy equation expressing the First Law will be given particular forms relating to various special processes which occur in closed systems. It will be shown that these processes may be classified further into reversible and irreversible processes. For the former class the energy equation may be expressed in a particularly useful form because the quantities of heat and work can each be stated in terms of changes in the properties of the system. The equations so derived are quite general in that they apply to any fluid.
3.1 The energy equation and reversibility
In section 2.4 the nonflow energy equation was presented in the form Q + W = (U 2
 U1 )
It has already been stated that we shall only consider systems which are in equilibrium in their initial and final states. When the system is in equilibrium, all the properties are uniform throughout the system and, in particular, each unit mass of the system will have the same internal energy.* Thus, if u represents the internal energy of unit mass, and in is the mass of the system, it is possible to write U = mu. In the same circumstances the volume V is equal to mu. u is termed the specific internal energy just as u is the specific volume, although the adjective 'specific' is often omitted when referring to internal energy. It is often convenient to work with specific quantities throughout an analysis and then multiply the final result by the mass of the system. Thus the nonflow energy equation is usually written as Q+ W = (u 2 — u1)
(3.1)
implying that Q and W are the quantities of heat and work per unit mass of fluid. For the particular class of processes known as reversible processes, the system is imagined to pass through a continuous series of equilibrium states. In such cases the equation may be applied to any infinitesimal part of the process between the end states, and the energy equation may be written in the differential * This statement only applies to systems consisting of a fluid in a single phase or, when more than one phase is present, if the phases are homogeneously mixed. 24
[3.1]
NonFlow Processes
form dQ + dW = du
(3.2)
The analysis of a reversible process may therefore be carried out by considering an infinitesimal part of the process undergone by unit mass, and overall changes which occur between the end states can be found by an integration performed at the conclusion of the analysis followed by multiplication by the mass of the system. During irreversible processes, on the other hand, the system does not pass through a series of equilibrium states. It is not possible to write mu for the internal energy of the system in any intermediate state because (a) a single value of u cannot be used to define the random molecular energy of the fluid, and (b) this energy is not the only relevant form if the fluid is turbulent. Each elemental mass Sm may have a different specific internal energy e which must include the kinetic and potential energy of the mass Sm. It is possible to consider an infinitesimal part of an irreversible process, but only by writing dQ + dW = dE where E = E (e Sm). Consequently, to evaluate dE it would be necessary to find the change in the specific internal energy of each of the elemental masses of which the system is composed — an impossible task. When considering irreversible processes, therefore, the energy equation can be used only in the integrated form of equation (3.1), and it is then sufficient to be able to assign values of u to the end states. This can be done because these are always assumed to be states of equilibrium. For the system to pass through a series of equilibrium states, and therefore to undergo a reversible process, it may be shown that the work and heat must cross the boundary under certain particular conditions. These conditions will be discussed for work and heat in turn.
3.1.1 Work and reversibility
Let us consider a closed system where a part of the boundary is allowed to move under such conditions that the external restraining force is only infinitesimally smaller than that produced by the pressure of the system. Fig. 3.1 illustrates such a system. The area of the piston is A, the pressure of the fluid at any instant is p, and the restraining force exerted by the surroundings is infinitesimally smaller than pA. If p is assumed constant during an infinitesimal movement of the piston over a distance dl, the work done in moving the external force pA through this distance must be pA dl. But A dl = d V, the infinitesimal change of volume, and therefore dW = —p d V The negative sign is required because in an expansion d V is positive, whereas d W is negative because work is being done on the surroundings. If the expansion occurs from a pressure p, to a pressure p2, in such a way that the restraining
25
[3.1]
Principles of Thermodynamics
Fig. 3.1 A reversible process
v, d/
V2
Specific volume
force is changed continuously so that it is never materially different from pA, the total work done can be found by summing all the increments of work: 2 W = 
p dV
(3.3)
The conditions under which this expansion has been imagined to proceed are just those necessary for the expansion to be reversible. No pressure gradients or eddies are set up in the fluid, and the properties are uniform throughout the system at all times. The system passes through a series of equilibrium states, and the process may be represented by a full line on the p—v diagram (Fig. 3.1). The area under this curve is given by IT p dv. Comparison with equation (3.3) shows that the area represents the magnitude of the work done per unit mass of fluid. The reason for the use of the term 'reversible' is now apparent; the expansion may be stopped at any point and reversed by only an infinitesimal change in the external force. The system will then return through the same series of states, and exactly the same quantity of work will be done by the surroundings on the system as has been done by the system on the surroundings in the original process. d V would be negative for the compression, and hence — p d V would appear as a positive quantity in agreement with the sign convention adopted for work. It is easy to show that — fp dv is not always equal to the work done per unit mass, and that the equality only holds when the system passes through a series of equilibrium states. Fig. 3.2a shows a container divided into two compartments by a sliding partition. One part contains a mass of gas at a pressure pi and specific volume v1, and the other is evacuated. When the partition is withdrawn, the gas undergoes an expansion which is not restrained in any way by an opposing force at the moving boundary; the process is called a free expansion. When the system has settled dqwn to a new state of equilibrium it may have a pressure p, and specific volume v2 . The end states could be located on the p—v diagram, but the fact that a process had occurred could only be indicated by a dashed line. Each intermediate state is indeterminate because no single values of p and v can be ascribed to the system as a whole. Some intermediate points could be found, however, if the process were carried out in a number of steps as in Fig. 3.2b. After each partition is withdrawn, and the gas has settled down to an equilibrium state, the pressure and volume could be measured and 26
NonFlow Processes
[3.1] Fig. 3.2 The free expansion and irreversibility
Pt
(a)
P2 u v2 Specific volume (c)
(b)
the corresponding state point plotted on the p—v diagram. If a dashed curve is drawn through all such points, as in Fig. 3.2c, the area under the curve could be found and this would be equal to I i p dv. Yet no work has been done by the system on the surroundings at all, because no external force has been moved through a distance. This is an extreme case; in general there is some restraining force at a moving boundary, and some work will be done by the fluid during the expansion. But, unless the process is reversible, the magnitude of the work done per unit mass will always be less than I p dv. This point will be elaborated in section 5.4, where it is also noted that for a compression the magnitude of the work done on the system is always greater than I p dv unless the process is reversible. When it is helpful to emphasise that equation (3.3) is valid only for reversible processes, the equation may be written as 2 2 Wr e v = — (p dv) or W = — f (p dv)'rev 1
1
The condition for reversibility, that the external force in the surroundings should differ only infinitesimally from the internal force due to the pressure of the fluid, means that there is no excess force available for accelerating the fluid or boundary. Thus it implies that the reversible expansion or compression is an infinitely slow process. Since any real process must occur within a finite time, it is clear that the reversible process is an ideal process, i.e. one which may be approached but is never actually achieved in practice. 3.1.2 Heat and reversibility
The part of the surroundings which exchanges energy with a system by virtlue of the fact that it is at a different temperature is called a heat reservoir; it may be a source or sink of heat. Usually the term 'reservoir' is restricted to mean a source or sink of such capacity that any quantity of heat which crosses the boundary during a process is insufficient to change its temperature. A practical source of large capacity might be the gases produced by the continuous
27
Principles of Thermodynamics
[3.1]
combustion of a fuel, or a mass of condensing vapour; a practical sink might be a river, the earth's atmosphere, or a mass of melting solid. Consider two methods of raising the temperature of a fluid contained in a closed vessel from 100 to 200 degrees of temperature. An infinite heat source of, say, 300 degrees might be used for the purpose. Under these circumstances heat will flow at a finite rate across the boundary. There will be a temperature gradient set up in the fluid because the fluid nearest to the source will always be hotter than the fluid at the opposite end of the vessel. The system cannot, therefore, be in a state of equilibrium during the transfer of energy. On the other hand, if this source is replaced by a series of heat sources ranging in temperature from (100 + dB) to (200 + do), so that the active source is never more than infinitesimally different in temperature from the system, temperature gradients will not be produced in the fluid and the system may be presumed to pass through a series of equilibrium states. Moreover, at any point in the process only an infinitesimal change in the temperature of the source is necessary for it to become a sink and for the direction of the process to be reversed. Thus a transfer of energy by virtue of a temperature difference can be carried out reversibly only if the temperature difference is infinitesimally small. This implies that the rate at which the transfer can proceed is infinitely slow, and once again it appears that the reversible process cannot be completely achieved in practice. Practical methods by which a reversible heat transfer process can be approached are available, and one is described in section 12.9. A number of particular nonflow processes may now be considered, each of which may or may not be performed reversibly. When they are performed irreversibly, the nonflow energy equation may be applied in the integrated form Q + W = (u2 — u1) because the end states are always assumed to be states of equilibrium. When they are performed reversibly, the energy equation may also be applied in the differential form dQ + dW = du And, in addition, the work transfer can be expressed in terms of the properties of the system, i.e. dW = —p dv, so that dQ — p dv = du It might be supposed, by analogy, that when heat is transferred during a reversible process it too can be expressed in terms of properties. As temperature is clearly associated with heat, it might be one of the properties. For example, we might be able to write dQ = B dx, where 0 is the temperature and x some other property. This is in fact the case. As a consequence of the Second Law of Thermodynamics it will be shown that two suitable properties can be defined, and that dQ = Tds, where T is the absolute thermodynamic temperature and s is the property entropy. We shall not, at this stage, presuppose the relation dQ = Tds, but will point out the type of problem in which it might prove useful.
28
NonFlow Processes
[3.3]
3.2 Constant volume process
The discussion in section 1.3 has already shown that there are an infinite number of processes which can produce a given change of state and during which the volume remains constant. Any combination of quantities of heat and work can be used which will satisfy the equation
Q + W = (u2 — ui ) remembering that u, and u2 are fixed when the initial and final states are given. The only restriction is that W must be zero or positive, because during a constant volume process work can only be done in practice by some method of churning the fluid. The process of increasing the internal energy of a system by using the viscous or frictional effects inherent in any movement of a fluid is one to be avoided. Such a process involves a degradation of energy because, as will be shown later, no practical method exists of making all the internal energy available again as work. Consequently, whenever reference is made to a constant volume process, it will always be to one in which the work is zero unless otherwise stated. Thus the energy equation for a constant volume process is usually written as
Q = (u, — u1 )
(3.4)
That is, the quantity of heat is equal to the change of internal energy. If, in addition to the work being zero, it is stipulated that the heat is transferred by virtue of an infinitesimally small temperature difference, then the process is reversible and the energy equation can be written in differential form as dQ = du
(3.5)
There is one, and only one, constant volume process which can join two given end states when the process is reversible. It is worth noting that the integrated form of equation (3.5) is (3.4), so that the overall quantity of heat transferred during a constant volume process from state 1 to state 2 does not depend upon the provision of a reversible method of transferring the heat, but merely on the assumption that the work is zero.
3.3 Constant pressure process
A closed system undergoing a process at constant pressure is illustrated in Fig. 3.3. The fluid is enclosed in a cylinder by a piston on which rests a constant weight. If heat is supplied, the fluid expands and work is done by the system in overcoming the constant force; if heat is extracted, the fluid contracts and work is done on the system by the constant force. In the general case,
Q+ W = (u2 — u1 ) Work might also be done on the system simultaneously by churning the fluid with a paddle, and this positive quantity of work must then be included in the 29
Principles of Thermodynamics
Fig. 3.3
[3.3]
14'
A process at constant pressure
term W If no paddle work is done on the system, and the process is reversible, dQ — p dv = du
(3.6)
Since p is constant, this can be integrated to give Q — p(v2 — v1 ) = (u2 — u 1 )
(3.7)
If the initial and final states are known, e.g. if p, v, and v2 are given, a definite quantity of heat Q is transferred during the process which can be calculated from (3.7). There is therefore only one reversible constant pressure process which can join the two given states. A further simplification of the energy equation is possible if a new property is introduced. Since p is constant, p dv is identical with d(pv). Thus the energy equation can be written as dQ — d(pv) = du or dQ = d(u + pv) The quantity (u + pv) occurs so frequently in thermodynamics, particularly in equations relating to open systems, that it has been given a special name and symbol, the specific enthalpy h. Because enthalpy is defined merely as a combination of the properties u, p and v, it is itself a property. That is, a change in enthalpy between two states depends only upon the end states, and is independent of the process. Values of the enthalpy are included in tables of properties of fluids and, as with internal energy, the values given are always differences between the enthalpy at various states and the enthalpy at some reference state where it is arbitrarily assumed to be zero. Since only changes of enthalpy are of interest, this information is adequate. In terms of specific quantities, h=
+ pv
(3.8)
and for any mass of fluid m, in a state of equilibrium, H = U + pV
(3.9)
where H = mh, U = mu and V = ►nv. The units of enthalpy must be those of 30
[3.4]
NonFlow Processes
energy; therefore we shall express enthalpy in kJ and the specific enthalpy in kJ/kg. Using this derived property, the energy equation corresponding to (3.6) becomes dQ = dh
(3.10)
or, in the integrated form, Q = (h 2 — h1)
(3.11)
Thus the heat added in a reversible constant pressure process is equal to the increase of enthalpy,* whereas it was equal to the increase of internal energy in the reversible constant volume process. Equation (3.11) does not apply if the process is irreversible; it is an integrated form of the special equation (3.6), and has not been deduced directly from the general equation.
3.4 Polytropic process
The constant volume and constant pressure processes can be regarded as limiting cases of a more general type of process in which both the volume and the pressure change, but in a certain specified manner. In many real processes it is found that the states during an expansion or compression can be described approximately by a relation of the form pv" = constant, where n is a constant called the index of expansion or compression, and p and v are average values of pressure and specific volume for the system. Compressions and expansions of the form pv" = constant are called polytropic processes. When n = 0 the relation reduces to p = constant, and when n = co it can be seen to reduce to v = constant by writing it in the form env = constant. For the reversible polytropic process, single values of p and v can truly define the state of a system, and d W = — p dv. The work done per unit mass during a change from state 1 to state 2 may then be found by integration as follows. For the initial, final and any intermediate state, P1vi =
P2 V"2 =
PV"
Therefore 2
W=—
j..
p dv = —pl y n'
I n
2 dv _ p1 v,(v1"— vl H)
—
n—1
1 v" 1—n
= P2V2V2
—
n 1—n P1V1V1
n—1
— P2 V 2 —
P1 V 1
n—1
(3.12)
The integrated form of the energy equation for a reversible polytropic process * It is this particular relation which led to the adoption of the term 'total heat' as an alternative to enthalpy. Such a name is misleading because the enthalpy is related to the heat supplied only in the special case of a reversible constant pressure process, whereas the property is used in the analysis of many other processes where it bears no direct relation to a quantity of heat.
31
[3.4]
Principles of Thermodynamics Fig. 3.4 Polytropic processes
+ve n
n=
b c/ / / +ve
= n
n
co
may therefore be written as (P2v2  Pi vi)
(3.13) = (u2 — u 1 ) nFor any given reversible polytropic process, i.e. one joining two given end states, definite quantities of heat and work cross the boundary. For example, if the end states are defined by (pi , v1 ) and (p2, v2 ), the index n can be found, and W and Q calculated from (3.12) and (3.13). Some reversible polytropic processes are represented in Fig. 3.4 on the p—v diagram. The lower righthand quadrant contains expansion processes starting from an initial state represented by point 1, and the upper lefthand quadrant contains compression processes starting from the same initial state. The area under the curve or line represents the magnitude of the work done in each case, i.e. under a it is zero, under bit is p(v2 — v1), and under c it is (p2 v2 — pi v1 )/(1 — n). The larger the value of n, the more nearly does the polytropic curve approach the vertical line representing the constant volume process. This fact could also be found by differentiating pv" = constant to give vs' dp + pnv" dv = 0 Q+
Or
dp = np (3.14) dv Thus the slope of the curve increases in the negative direction with increase of n. Although it is physically possible for processes to fall into the other two quadrants, they do not often arise in practical systems. These would be processes during which the pressure and volume increase or decrease simultaneously, and would imply a negative value of n if they were polytropic processes. An example of a system in which p and v increase simultaneously is illustrated in Fig. 3.5, wherein a piston is controlled by a spring. When heat is supplied to the fluid the restraining force increases as the expansion of fluid compresses the spring. The pressure of the fluid is always equal to the spring force divided by the piston area, and consequently the pressure must increase linearly with volume as shown on the p—v diagram. The process would be represented by a straight line in the upper righthand quadrant of Fig. 3.4; it would of course only be a 32
NonFlow Processes
[3.5]
Fig. 3.5
p
Simultaneous increase of pressure and volume
polytropic process if the projected line passed through the origin (i.e. when = —1). 3.5 Adiabatic process
The term adiabatic is used to describe any process during which heat is prevented from crossing the boundary of the system. That is, an adiabatic process is one undergone by a system which is thermally insulated from its surroundings. For adiabatic nonflow processes, therefore, the energy equation reduces to W = (u2 — u 1 )
(3.15)
In an adiabatic expansion, work is done by the system at the expense of its internal energy; in an adiabatic compression, the internal energy is increased by an amount equal to the work done on the system. If the initial and final states are known, the values u 1 and u2 are determined and the work done can be calculated. We shall proceed to show that in the case of a reversible adiabatic process there is only one process which can join the end states, i.e. that there is a definite relation between p and v. In this case, therefore, the work done can be predicted when the initial state and only one property of the system in its final state are known. We shall suppose that Pi and v1 are known, and that it is required to find the work done by the system during a reversible adiabatic expansion to p2 . For this process the energy equation may be written in differential form as p dv = —du If a known algebraic equation u = rewritten as
(3.16) v) relates p, v and u, (3.16) may be
p dv = — d0p, v) and integrated. The result will be a definite relation between p and v, e.g. v = f(p). v2 can be found by putting p = p2 in f(p). Consequently u 2 and u, can be found from 4(p, v), and the work can be calculated using equation (3.15). If no simple algebraic equation relates p, v and u, the following graphical method could, in principle, be used: (a) First, a series of constant pressure lines are drawn on a diagram using u and v as coordinates, from the information contained in the table of properties (Fig. 1.1). For each pressure in the table a series of values of u and v are given, and these pairs of values can be represented by points on the diagram. All points relating to one pressure, pa, say, are joined up 33
Principles of Thermodynamics
[3.6]
Fig. 3.6 The reversible adiabatic process
by interpolation between pm and pn curves
p2
to form a constant pressure line. This is repeated for a series of pressures A, covering the range pi to p2 as shown in Fig. 3.6. Pb, • • • (b) Secondly, the path of the reversible process is traced out on the diagram starting from the initial state 1. Recasting equation (3.16) in the form du/dv = —p, it is seen that at any point in the process the slope of the curve is negative and equal in magnitude to the pressure at that point. Through each constant pressure line a series of short parallel lines can be drawn with a slope equal to —p. The path of the process will be represented by a curve drawn from point 1 so that its slope is always the same as that of the short parallel line where it intersects each constant pressure line. (c) Lastly, since the final pressure p2 is known, the final state can be located on the curve, and the value of u2 can be read off the diagram. The work done can then be calculated from (3.15). The foregoing graphical procedure is very lengthy. Looking ahead, it is easy to show that the calculation can be considerably simplified if we can write dQ = T ds for a reversible process, where T is the absolute thermodynamic temperature (section 6.2) and s is the property entropy (section 6.4). Then, since dQ = 0 for an adiabatic process, ds = 0 when it is reversible and the entropy must remain constant. The foregoing problem may be solved by finding s corresponding to pi and vi from the tables of properties, and then, since s2 = si , finding v2 corresponding to p2 and s2. Corresponding values of u1 and u2 can also be found from the tables, and the problem is solved. This illustrates one possible use of the property entropy. 3.6 Isothermal process
When the quantities of heat and work are so proportioned during an expansion or compression that the temperature of the fluid remains constant, the process is said to be isothermal. Since temperature gradients are excluded by the 34
NonFlow Processes
[3.6]
definition, the reversibility of an isothermal process is implied. If it were not reversible a single value of the temperature could not be allotted to the system as a whole in all the intermediate states. It should be noted, however, that the term 'isothermal' is often ascribed to processes which are not reversible but during which the average temperature of the bulk of the fluid remains constant. It is possible to show that for a reversible isothermal process a certain definite relation must exist between p and v, and consequently the work done has a definite value which can be predicted. For any reversible process the energy equation is dQ — pdv = du or 2
Q
p dv = (u2 — u1 ) f
A relation between p, v and temperature B must exist, either as some equation of state 0 = 4(p, v), or in the form of a table of properties. Consequently, if the temperature remains constant, a definite relation exists between p and v which may be determined analytically or graphically. If p„ v 1 and p2 are given, v2 can be found from this particular p—v relation. The work done may be found either by integrating p dv between these limits, or by finding the area under the curve on a p—v diagram. Since the end states are known, u 1 and u2 can be found, and consequently Q can be calculated from the energy equation if it is required. There is no need to outline the graphical procedure required if no simple function relates p, v and the temperature 0, because once again, looking ahead, the problem is much more easily solved by the use of the entropy s and the absolute thermodynamic temperature T For a reversible process dQ = Tds, and since T is constant in the case of an isothermal process it is possible to integrate this expression directly. Thus for a reversible isothermal process, Q = T(s2 — s1 ), where T = T, = T2 . If p, and v1 are known, s1 , T1 and u1 can be found from tables of properties. Since p2 and T2 ( = T1 ) are known, s2 and u2 can also be found from the tables. Thus Q can be calculated from T(s2 — s1 ), and the work transfer can then be found from W=(u2 — u1) — Q
35
4 Flow Processes
This chapter is devoted to a discussion of various flow processes which occur in open systems. Since the energy equation expressing the First Law has been deduced with reference to closed systems, the first step is to deduce an equivalent equation for open systems. Flow processes may be classified into steadyflow and nonsteadyflow processes, and since the former are of greater interest they are considered first. Finally, the idea of a cycle consisting of steadyflow processes is presented. The application of the concept of reversibility to flow processes will be deferred until Chapters 5 and 6,
4.1 The steadyflow energy equation
A diagrammatic sketch of a typical open system is shown in Fig. 4.1. Fluid flows through the system at a uniform rate, while heat and work are transferred between the fluid and surroundings also at a uniform rate. The work is done in this instance by allowing the fluid to impinge on a row of turbine blades. Useful work done by the turbine is transferred to the surroundings via a shaft and is called shaft work. Note that the boundary has been drawn outside the container for clarity, although it should be imagined to encompass only the fluid.* If the rotor is included also, /with the boundary cutting the shaft, then the work done can be deduced from the torque in the shaft and the angular displacement; detailed knowledge of the forces exerted by the fluid on the turbine blading is then unnecessary. The idea behind this procedure was introduced in section 1.3 when dealing with paddle work in closed systems. With any open system, the boundary is assumed to cut the entrance and exit ducts where the properties of the fluid are known, i.e. at crosssections 1 and 2 in Fig. 4.1. At any given point in the flow, an element of the fluid has a relevant mechanical state in addition to a thermodynamic state. Any of the mechanical and thermodynamic properties may change as the element passes through the system, so that both types of property are relevant to the analysis. For the flow to be regarded as steady, the rate of mass flow (kg/s say) must be constant and the * In fluid mechanics the boundary is often referred to as a control surface and the system as control volume.
36
a
[4.1 ]
Flow Processes
Fig. 4.1 Open system with heating chamber and turbine
W
same at inlet and outlet, and the properties of the fluid at any point in the open system must not vary with time. The latter condition means that all elements of fluid flowing past a given point will always have the same mechanical and thermodynamic states. The properties will, in general, be different at different points in the system, and therefore any given element of fluid passes through a series of states on its way through the system. It is possible to regard the continuousflow process as a series of nonflow processes undergone by an imaginary closed system, and Fig. 4.2 illustrates this.* The boundary of the closed system includes the fluid contained in the open system at any instant, plus a portion of the fluid about to enter the system. The imaginary closed system must then be supposed to undergo a deformation as indicated by the succession of Figs 4.2a, b and c. Continuous flow may be regarded as a succession of these nonflow processes, carried out for every element of fluid entering the open system. It now becomes possible to apply the energy equation which has been developed from a study of closed systems. First consider the state of the imaginary closed system in the configuration shown in Fig. 4.2a. Fig. 4.3 shows an enlarged view of the part of the system containing the element of fluid which is about to enter the open system. The thermodynamic and mechanical states of the element of mass Sm may be assumed to be known. The random molecular energy of the element is U1 say, and if the element is moving with a velocity C1 at a height z1 above some reference level, it also possesses kinetic energy 18m Ci and potential energy Sm gzi. The total energy of the mass Sm is therefore U i + 18m C? + am gzi If we assume that the element is small enough for the thermodynamic properties to be uniform throughout its extent, this becomes 8m(u, + IC? + gzi ) At the instant when mass Sm reaches the boundary of the open system, let the fluid within the open system possess a total quantity of internal energy E'. E' includes the kinetic and potential energies of the fluid elements within the boundary of the open system; the possibility of using the term 'internal energy' •
* This approach was suggested in a paper by Gillespie and Coe (Ref. 9), and used by Keenan in his Thermodynamics (Ref. 6).
37
[4.1]
Principles of Thermodynamics Fig. 4.2 Imaginary nonflow process
It
(a)
(b)
1
(c)
in this way has already been noted in section 2.4. For reasons which will appear later, however, there is no need to specify the different forms of energy of which E' consists; nor does it matter that this quantity of fluid is not in a state of equilibrium and that the mass of fluid is unknown. The total internal energy of the imaginary closed system in its initial state (Fig. 4.2a) is E' + 8m(u, + iC1+ gzi ) Now consider the state of the closed system in the configuration shown in Fig. 4.2c. Since, for steady flow, the properties of the fluid at any point in the open system do not change with time, the quantity of energy contained within the original boundary must still be E'. Therefore, if a mass Sm leaves the open system at some part of the boundary where the properties are denoted by subscript 2, the final internal energy of the imaginary closed system (Fig. 4.2c) will be E' +6m(u2 +4C+ gz2 ) Lastly, we must consider how the imaginary closed system changes its state from that in Fig. 4.2a to that in Fig. 4.2c. In this period of time we may assume that SQ units of energy are transferred to the system as heat, and that SW units of energy are transferred to the system as work via a shaft. The shaft work SW is not the only work transferred as far as the imaginary closed system is concerned
Fig. 4.3 Elemental mass crossing inlet plane 1
Internal energy Kinetic energy Potential energy
Sin u Elm gz
/ Internal energy E' Area A Pr
1,
38
Reference level
Flow Processes
[4.1]
because parts of its boundary move at sections 1 and 2. For the element Om to enter the open system, the imaginary closed system must be compressed, its volume decreasing by 8m v1 . This is accompanied by a force p,A moving a distance I = 8m vi /A, where A is the crosssectional area of the element, as illustrated in Fig. 4.3. The work done by the surroundings on the system is therefore 8m p1 v 1 . Similarly, it can be shown that the work done by the closed system on the surroundings, as 8m is expelled from the open system, is 8m p2 v2 .* The net work done on the system during the change represented in Fig. 4.2 is therefore 8W — ort4P 2 v2 — POO We may now apply the energy equation to the imaginary closed system and write 8Q + {OW — Onl(P2v2 — Pi vi)}
= {E' + 8m(u2 + 1C1 + gz2 )} — { E' + 8m(u, + IC? + gz 1 )}
(4.1)
The quantity E' cancels, and by writing the enthalpy h for (u + pv), the equation reduces to
8Q + 8W = 8m(h2 +
+ gz2) — 8m(h, +
+ gz 1 )
The continuous steadyflow process consists of the sum total of all the elemental mass transfers across sections 1 and 2; it may therefore be represented by the equation E8Q + 8W = E8m(h2 +
1C1 + gz 2) — am(h,
+ gz,)
+
This equation can be simplified considerably if the properties are uniform over the crosssection of flow at inlet and outlet. Thus if every 8m enters the system with the properties h 1 , C1 , z1 and leaves with the properties h2 , C2 , z2 , the equation can be written as ESQ + aW = (h2 + 1C + gz2 )am — (h1 +
+ gz,)aom
We may now write m, Q and W for am, ESQ and ES W,, where these quantities are associated with any arbitrary time interval. The equation then becomes
Q+
= ml(h2 — hi ) +
— C1)+ g(z 2 — z1 )}
If we divide throughout by m, we can write the equation as
Q+ W= {(h2 — h 1 )+ f(C3 —
+ g(z2 — z1 )}
where Q and W are the heat and work transfers per unit mass flowing through the system. Here care must be taken in checking units: if Q and W are expressed * The product pu has been called flow work, flow energy and pressure energy by various authors. Such names may be misleading, and there is no need to give this quantity any special name at all. The term arises out of the need to view the flow process as a series of nonflow processes, and so far as the open system is concerned it is merely the product of two properties, pressure and specific volume; it is not a part of the energy of the system, nor does it represent any work done on or by the open system.
39
[4.1]
Principles of Thermodynamics
in terms of energy, then there is implied a factor of unit mass before the brace; while if Q and W are expressed in terms of energy per unit mass, no dimensional factor is implied before the brace. The most useful form of these equations is obtained when we consider unit time interval during which the mass flowing through the system is the mass flow rate di, and Q and W become the rates Q and W. The equation then assumes the form +
= th{(h2 —
+ f(Ci —
+ g(z2 — z1)}
(4.2)
Equation (4.2) expresses the relation between rates of heat and work transfer and the properties of the fluid at, inlet and outlet of an open system. It is called the steadyflow energy equation, and provides the basic means for studying most open systems of importance in engineering. The assumptions upon which equation (4.2) is based may be summarised as follows: (a) The mass flow at inlet is constant with respect to time, and equal to the mass flow at outlet. (b) The properties at any point within the open system do not vary with time. (c) The properties are constant over the crosssection of the flow at inlet and outlet. (d) Any heat or work crossing the boundary does so at a uniform rate. Note that no assumption has been made about the nature or configuration of the steady flow within the open system, and the steadyflow energy equation applies whether there is viscous friction or not. It corresponds to the general nonflow energy equation (3.1). It is not possible for all these conditions to be satisfied in any practical process. For example, when a fluid flows through a pipe, it is known that viscous friction causes the velocity to fall rapidly to zero in the layer adjacent to the wall. Friction between the layers of fluid will also slightly affect the distribtition of the thermodynamic properties across the pipe. Thus assumption (c) is not completely justified. Nevertheless, experiments have shown that equation (4.2) can be applied in these circumstances with sufficient accuracy for practical purposes if mean values of the properties are used. To take another example, it is not necessary for assumption (b) to be satisfied rigorously. The properties at any point within the open system may be allowed to fluctuate. Provided that they return to the same values periodically, the equation can still be applied. Under these circumstances, the quantities Q and W represent the average heat transferred and work done per unit mass, over a period of time appreciably longer than that required for tine cyclic variation of the internal energy E'. Finally we must note an important equation which follows directly from assumptions (a) and (c). It is known as the continuity equation, and expresses the principle of conservation of mass in steady flow. If rh is the rate of mass flow, we have A1 C1 A2C2 (4.3) m= V1
40
V2
Flow Processes
[4.2]
The steadyflow energy equation will now be applied to various open systems of particular importance. In all these examples the potential energy term g(z 2 — z1 ) is either zero or negligible compared with the other terms. It has been included in equation (4.2) for the sake of completeness, but will henceforth be omitted. It may appear, for example, in the analysis of hydraulic machinery where the fluid is a liquid and the enthalpy and heat terms are negligible; but such systems are not considered in this book. 4.2 Open systems with steady flow 4.2.1 Boiler and condenser
Fig. 4.4 illustrates a boiler, the fluid entering as a liquid and leaving as a vapour at a constant rate. In this case no work is done on or by the fluid as it passes through the system, and hence Hi = 0. The velocities of flow are usually quite low, so that the difference between the kinetic energies at inlet and outlet is negligible compared with the other terms of the equation. This is verified by a numerical example in section 10.1. The steadyflow energy equation for this open system reduces to Q = rh(h2 — h1 )
(4.4)
where Q is the rate of heat transferred to the boiler. All that is necessary to calculate Q is a knowledge of the thermodynamic state of the fluid as it enters and leaves the boiler, and the mass flow. Fig. 4.5 illustrates a simple surface condenser. The vapour passes over a bank of tubes, and is condensed as it comes into contact with the surface of the tubes. The tubes are maintained at a lower temperature than the vapour by a flow of cooling water. The cooling water is not part of the fluid of this opensystem, but acts as a sink of heat in the surroundings. Equation (4.4) also applies to this system, although in this case h1 is greater than h2 and Q is negative. Fig. 4.4
Vapour
Simple watertube boiler
2
Liquid —a. Gases to flue
I WI. When the pressure is constant, a decrease of internal energy of a fluid is normally accompanied by a decrease of volume (water between 0°C and 4°C being an exception). Thus v'2 is less than v2 , and the perfectly restrained process might be shown by the full line 12'. The magnitude of the work done during the actual process, in moving the constant force pa A a distance (v2 — v,)/ A, is equal to pa(v, — v1 ). This is * A column of air in the surroundings will also have been accelerated and viscous forces in the surroundings will contribute to the damping; for simplicity we may neglect this effect, e.g. by assuming the surroundings to have negligible viscosity.
56
[5.4]
Second Law of Thermodynamics
represented by the area of the shaded rectangle. It is clearly less than the area under the dotted curve, which is given by .Qp dv, where p is interpreted as the average pressure at any point in the expansion. By a similar argument it can be shown that a compression, carried out under sitnilar conditions, would require an amount of work equal to p2 (v1 — v2 ) to be done on the system by a constant force p2 A in the surroundings. This work is equal to the area of the shaded rectangle in Fig. 5.3c. In this case the work done is greater than the magnitude of f i p dv. The magnitude of the work of expansion can be increased, and that of compression reduced, by applying the external force in a series of steps decreasing successively from pi A to pa A in the former case, and increasing 'successively from p„A to p2 A in the latter. The difference between the magnitudes is then reduced. In the limit, when the external force never departs by more than an infinitesimal amount from that due to the pressure of the fluid, the work done will be numerically equal to ff p dv in each case and the processes become reversible. In an actual reciprocating engine the mass of the piston and other moving parts is considerable, but most of the kinetic energy acquired by these is stored in the flywheel and recovered. The piston is prevented from undergoing the oscillation which would occur if the piston were free, and the kinetic energy acquired by the fluid exists in the form of eddies which are damped out by viscous friction. The creation and dissipation of kinetic energy is therefore a continuous process throughout the expansion or compression. With normal piston speeds the quantity of energy dissipated in this way is very small, and the effect of fluid friction can usually be ignored. Thus, when a calculation of the work done during a practical nonflow expansion or compression is made on the assumption that it is a reversible process, it provides not only a criterion of perfection but also a close approximation to the actual value.* It will not be such a good approximation when special devices are used to introduce turbulence, as in some compressionignition engines. Friction in steadyflow processes When considering the effect of friction during flow processes, it is usually found to be by no means negligible. In nozzles, turbines and rotary compressors, the speed of flow is high and fluid friction is considerable. Consider first the effect of friction in a nozzle. Let the thermodynamic state of the fluid at the inlet be defined by (p1, h1 ), and let the inlet velocity be C1. Assume that the outlet pressure is fixed at some value p2 , this being chosen as the independent property of the final state. The appropriate steadyflow energy equation (4.5) states that j(Ci —
= (h1 — 112 )
* We are here referring to the work done on or by the fluid. Some of this work will be dissipated externally by piston friction, but this is expressed separately by the mechanical efficiency of the machine — see section 16.2.
57
[5.4]
Principles of Thermodynamics Fig. 5.4 Irreversibility due to friction in flow processes
2' P
P2
p/ or
Ii 2
h
(a)
/
/
I
I
II I
I
I I I I I I I
Pi
P2
,
h
h? ' h , (b)
(c)
Friction always produces a force opposing the motion, and after the expansion to pressure p2 the stream of fluid moves more slowly than it would have done had there been no friction. If the values which the dependent properties would have after frictionless flow are denoted by primes, this means that C2 < Consequently it follows that h2 > h'2, since the First Law must be satisfied, i.e. I( C'22 —
= (h, — h'2 )
During the process with friction, some of the directional kinetic energy (1C2 ) is being continually transformed into random molecular energy (u). But at any given pressure an increase of u must involve an increase in the specific volume v, and consequently an increase in enthalpy (u + pv). In effect, some of the initial enthalpy which could have produced an increase in kinetic energy has been prevented from doing so by friction. It is often helpful to represent a steadyflow process on a coordinate diagram, although it cannot be completely defined in this way. Thethermodynamic state of the fluid at the inlet and outlet may be represented by points on a diagram using two thermodynamic properties as coordinates, and a line joining the points can be used to represent the process.* A full line will always be used to denote a frictionless process, and a dashed line to denote a process where friction is present. Such diagrams only partially represent the process because the changes in mechanical properties are not shown. Fig. 5.4a shows the expansion process in a nozzle on a ph diagram. Fig. 5.4a can equally well represent the expansion in a turbine between pressures pi and p2. With the usual assumptions, i.e. adiabatic flow and equal inlet and outlet velocities, the energy equation is = — h2 ) If the flow is frictionless it may be written = th(h, — h2) where I I471 I > I 14/ I and h'2 < h2 . Similarly, Fig. 5.4b can represent the processes * Strictly speaking, the intermediate points only have meaning if every element of fluid flowing through the system passes through the same series of thermodynamic states. This implies that the properties are uniform at right angles to the flow throughout the system — not merely at the inlet and outlet, which was all we had to assume when deriving the steadyflow energy equation. When this additional assumption can be made, the flow is called 'onedimensional' (see Chapter 18).
58
[5.4]
Second Law of Thermodynamics
in either a diffuser or a rotary compressor. As always, friction results in the final enthalpy being greater than it would have been after a frictionless process to the same final pressure. Considering the case of a rotary compressor, this means that the actual work of compression th(h2 — h1 ) is greater than the frictionless work rii(W2 — h1 ). As an example, we may show that friction makes an expansion in a turbine irreversible. The dashed curve 12 in Fig. 5.4c illustrates this process. As before, we shall find processes by which the fluid can be returned to its initial state, and then show that the surroundings cannot be returned to their initial state without contradicting the Second Law. Let the fluid flow through a rotary compressor on leaving the turbine, so that it is compressed without friction to the original pressure (curve 23). The enthalpy drop in the turbine must have been less than the enthalpy rise in the compressor, because friction was present in the expansion. Therefore some net work, given by rh{(h3 — h2 ) — (h1 — h2 )} = ►h(h3 — h1 ) must be supplied by the surroundings. The fluid can be returned to its final state by cooling it at constant pressure without change of velocity, the quantity of heat entering the surroundings being equal to rh(h3 — h1 ) from equation (4.4). To return the surroundings to their initial state, a heat engine would be required to convert rh(h3 — h1) units of heat into rh(h3 — h1 ) units of work. This is impossible according to the Second Law, and therefore the process in the turbine cannot have been reversible.
5.4.2 Transfer of heat across a finite temperature difference
Consider the process of allowing heat to flow from a source to a fluid at a lower temperature, when the difference between the temperature of the source and the fluid is finite. If the fluid is a closed system having fixed boundaries, the quantity of heat supplied is equal to the increase of internal energy. Alternatively, if the heat is supplied to a fluid flowing in a duct under conditions such that the velocity remains unchanged, the quantity of heat is equal to the increase of enthalpy, equation (4.4). In either case the fluid may be restored to its initial state by allowing the same quantity of heat to flow across the boundary into a sink. Even if this second process is carried out so that the temperature of the sink is never more than infinitesimally lower than that of the fluid, the difference in temperature between the source and the sink will be finite. If the original process is to be reversible, it must be possible to transfer the quantity of heat from the sink to the source without incurring any further changes in the surroundings. This is impossible because, according to corollary 1 of the Second Law (section 5.3), some work would have to be supplied by the surroundings. Thus the process of heat transfer across a finite temperature difference is irreversible. We have already noted that a temperature difference is essential if any heat transfer is to take place in a finite time, so that all real transfers of heat must be irreversible. 59
Principles of Thermodynamics
[5.5]
5.5 Reversible and irreversible cycles
A cycle is reversible if it consists only of reversible processes. When such a cycle is reversed, all the quantities of work and heat crossing the boundary are reversed in direction without their magnitude being affected. The cycle may consist of reversible nonflow processes, or it may be an open or closed cycle consisting of reversible steadyflow processes. The original conception of a reversible cycle was due to Sadi Carnot (Ref. 4). He conceived of a particular cycle, called the Carnot cycle, which will be examined in detail in Part II. It is sufficient to note here that it is one of a special class of reversible cycles during which all the heat enters the system from a source at constant temperature, and all the heat leaving it is rejected to a sink at constant temperature. It follows that the processes during which heat is exchanged with the surroundings must be isothermal, the temperature of the fluid never differing by more than an infinitesimal amount from the fixed temperature of the source or sink. A cycle may be thought of as reversible without this limitation. If the temperature of the fluid changes during any heat transfer process, all that is necessary is that the source or sink be a series of reservoirs covering the required range of temperature. At any instant during the process, heat must be exchanged between the system and the particular source or sink which differs only infinitesimally in temperature from the fluid in the system. This idea has already been introduced in section 3.1.2. Engines operating on this type of reversible cycle will be shown symbolically by Fig. 5.5. The quantity Q1, for example, can be regarded as the sum of the infinitesimal quantities of heat received from the hot reservoirs. It is the limited class of reversible cycles, of which the Carnot cycle is a member, that plays an important part in the deduction of the corollaries of the Second Law. If the term 'reservoir' is restricted, in the manner suggested in section 3.1.2, to a source or sink of invariable temperature, then this class of reversible cycles will comprise those of engines or heat pumps operating between only two reservoirs. If any of the processes in a cycle are irreversible, the whole cycle is irreversible. The efficiency of an engine in which irreversible processes occur must always be less than that of the hypothetical reversible engine. For example, if friction Fig. 5.5
Series of hot reservoirs
Representation of reversible engine operating between more than two reservoirs
Series of cold reservoirs
60
[5.5]
Second Law of Thermodynamics
occurs during the expansion in the turbine of the steam power plant shown in Fig. 4.11, the work output of the turbine is reduced. The enthalpy at exit • from the turbine is thereby increased, and more heat must be rejected in the condenser to bring the fluid back to the same state before it passes through the feed pump. The First Law is still satisfied, i.e. IQ I = I WI + I Q2 I ) but the cycle efficiency I w1/1Q, I is reduced. If the efficiency of a cycle is calculated on the assumption that all the processes are reversible, this provides a figure for the maximum possible efficiency of power plant operating on that cycle.
61
Corollaries of the Second Law
The Clausius statement of the Second Law has been presented in section 5.3 as the first corollary. Other corollaries are concerned with: (a) the characteristics of reversible engines operating between only two reservoirs, (b) the thermdynamic scale of temperature, (c) the characteristics of engines operating between a series of reservoirs, and (d) the property entropy. The way in which entropy can be used to simplify calculations concerning nonflow processes has already been indicated in Chapter 3. This chapter ends with a description of the way entropy may be used in the analysis of steadyflow processes, followed by a few remarks on the limitations of the laws of thermodynamics and a summary of Chapters 1 to 6. The reader is reminded that for much of this chapter the symbols 01 and Q2 refer to the magnitudes of the heat transfers.
6.1 Reversible engines operating between only two reservoirs
Corollary 2 It is impossible to construct an engine operating between only two heat reservoirs which will have a higher efficiency than a reversible engine operating between the same two reservoirs.
Proof Assume the converse of this proposition to be true; let X be such an engine, having an efficiency IN. Let it receive heat Q, from the source, do work K, and reject heat (Q, — Wx ) to the sink. Then it is assumed that tlx > ri ft, where rlR is the efficiency of a reversible engine R operating between the same two reservoirs (Fig. 6.1a). If the reversible engine also receives heat Q, from the source, it will do work WR such that 14/„ < gix , and the heat rejected will be (Q, — WR ) which is greater than (Q, — Wx ). Let the reversible engine be reversed and act as a heat pump (Fig. 6.1b). It now receives heat (Q, — WR ) from the lowtemperature reservoir, receives work WR from the surroundings, and rejects heat Q, to the hightemperature reservoir. If the engine X is coupled to the heat pump, and the latter feeds heat Q, directly 62
[6.2]
Corollaries of the Second Law
Fig. 6.1 Can an engine have a higher efficiency than its reversible equivalent?
_.\
(a)
(b)
into the former, the combined plant represents a heat engine receiving heat — (Q, — Wx ) = (Wx — WO from the surroundings, and delivering an equivalent amount of work. According to the Second Law this is impossible, and the assumption that !i x > cannot be true. Consequently the original proposition must be true.
(Q1 —
All reversible engines operating between the same two reservoirs have the same efficiency.
Corollary 3
Once the second corollary has been proved, no special proof is required for the third. If two reversible engines differ in efficiency when operating between the same two reservoirs, then one must have a higher efficiency than the other. This is impossible if corollary 2 is true. Since all reversible engines operating between the same two reservoirs have the same efficiency, this efficiency must depend upon the only feature which is common to them all, namely the temperatures of the reservoirs: it is called the Carnot efficiency. 6.2 Thermodynamic temperature scale
4 A scale of temperature can be defined which is independent of any particular thermometric substance, and which provides an absolute zero of temperature.
Corollary
Proof Let us consider the reversible engine operating between only two reservoirs represented symbolically in Fig. 6.2a. Corollary 3 implies that its efficiency depends only on the temperature of the reservoirs, and therefore that it is independent of the particular properties of the working fluid and of the quantity of heat Q0 supplied to the engine. But
 Qo — Q = 1 QQ0
and hence it follows that reservoirs.
Q0
Q/Q0
is a function only of the temperatures of the
63
[6.2]
Principles of Thermodynamics Fig. 6.2 Hot reservoir
Use of a hypothetical reversible engine to construct a temperature scale
Q
Cold reservoir T
(a)
(b)
Let us now allot a positive number To to some reservoir in a convenient reference state which is easily reproducible (e.g. a pure substance melting at a definite pressure); further, let us define the temperature T of any other reservoir by the equation Q T = To —
(6.1)
Qo
The value T is then fully and uniquely determined by (a) the arbitrary choice of To and (b) the ratio Q/Qo which, as a consequence of the Second Law, is a fixed and definite quantity for the two given reservoirs. If Q is measured for several sinks at different temperatures and plotted against T obtained from (6.1), we obtain by definition a scale of temperature which is linear in Q. The slope of the line in Fig. 6.2b is Qo / To. The unit of temperature now follows as the fraction 1 / To of the interval from T = 0 to To. The temperature scale defined in. this way is called the, thermodynamic scale, because it is dependent solely on the laws of thermodynamics and not upon the properties of any particular substance. It is an absolute scale because it presents us with the idea of an absolute zero, i.e. T = 0 when Q = 0. The Second Law implies that Q can in fact never be zero, and we may therefore deduce that absolute zero is a conceptual limit and not a temperature which can ever be reached in practice.* It may be helpful if we visualise the scale as being constructed by a series of reversible engines (Fig. 6.3a), each operating between only two reservoirs and each producing the same quantity of work. Each sink is a source for the following engine, the heat entering a reservoir being equal to the heat leaving it. If the temperatures of the reservoirs are defined in the way suggested by equation (6.1), then Q 0 — Qt
Qi
TO
Q2
T2 T3
Q2
=
T1
12 ',
Q3
(6.2)
And the efficiencies of the engines therefore become TO 110
T1 —
T1
To
/1=
T2
T2 — T3 I
n.2 —
(6.3)
* Strictly speaking, it is necessary to invoke the Third Law (see end of section 7.9.1) to deduce the unattainability of absolute zero: this is discussed in Ref. 8.
64
Corollaries of the Second Law
[6.2] Fig. 6.3 An absolute thermodynamic temperature scale
T0
•
To
0
Q2
T2 =
Q2 Q3 Q3 Q4 Q4
Q2
Qi
95
10
Q1 ,,, 12 1 =— To 11 — Q1 Q0
=
T= Q2 = TO
Qo
100
5
95
To
5 90
85
10
Q3 ,r 13 — — io QO
80
Q4 T4 = To Qo
(a)
90
95 To 100
20
80 T = — To 100
100
5
20
20 T — T0 100 5
=
10 10
10
15
To
100
5
T = — To 100 5 — To T= =5 100
5 77717/777/777
To
T=0
(b)
'77/7771777/777 (c )
But since w= tioQ0 =
=n2Q2 = •••
it follows that Qo
To
(To — To =
Q Q2 (T, — T2 ) = (T2 T, T2
— T3) =
Using equations (6.2), this reduces to (T0 —
= ( T, — T2 ) = (T2 — T3 ) = . . .
(6.4)
Thus the differences between the temperatures of successive reservoirs are the same and can provide intervals or units of temperature. To may be as high as we wish to make it, and the intervals may be made as small as desired by increasing the number of engines in the series. The series of reservoirs could , theoretically be used as a standard set of temperatures with which to calibrate any practical thermometer. Figs 6.3b and c illustrate the effect of increasing the number of engines. The last possible engine in the series is one which rejects an amount of heat equal to the work W; according to the Second Law the next engine in the series is an impossibility. It is evident that the temperature of the sink of the last possible engine is reduced as the number of engines is increased, but as long as W is finite the scale must stop short of absolute zero. Note that the choice of 100 units for Q, in the scales of Figs 6.3b and c is quite arbitrary; a discussion of the accepted way in which numbers are assigned to the thermodynamic scale is left to section 8.1. Although it has been internationally agreed to define the thermodynamic 65
Principles of Thermodynamics
[6.3]
temperature by writing T = To(Q/Q0), it could have been defined in an infinite variety of ways without losing its character of being independent of the properties of any particular substance. For example we could define a scale, on which the temperature is denoted by say, by writing = o ln(Q/Q0); on this scale the temperature would range from — co to + co. This was in fact the first scale proposed by Kelvin. The simplest expression has been adopted, however, not because the scale is linear in Q when formed by reversible engines producing equal work, but because it simplifies the relations between temperature and the other thermodynamic properties. (This point will be appreciated after a study of Chapter 8.) It is the existence of these relations which makes the measurement of thermodynamic temperature a practical possibility, since they enable the temperature to be deduced from measurements of other properties. The practical details of measurement need not concern us here; they are referred to in section 8.1. It will be assumed for the remainder of Part I that all temperatures are measured on the thermodynamic scale, and they will be denoted by T As a result of Corollaries 2 and 3, the most important characteristics of engines operating between only two reservoirs may now be stated as follows: (a) All reversible engines, operating between a source at temperature T, and a sink at temperature T2, have an efficiency equal to (T, — T2)/ T,; see equation (6.3). (b) For a given value of T2, the efficiency increases with increase of T1 . Since the lowest possible temperature of a practical infinite sink is fixed within close limits, i.e. the temperature of the atmosphere or ocean, it may be said that a given quantity of heat is more useful for producing work the higher the temperature of the source from which it is received. (c) For all reversible engines operating between only two reservoirs, Q1 /Ti = Q 2 / T2 . If an engine is irreversible, its efficiency is less than (T1 — T2 )/ T,. For the same heat received Q 1 , the heat rejected Q2 must be greater than that rejected by a reversible engine operating between the same two reservoirs. Therefore, for irreversible engines operating between only two reservoirs, Q1 / T, < Q2 / T2 . It is important to note that when applying statements (a), (b) and (c) to reversible engines, the temperature T refers both to the temperature of the reservoir and to the temperature of the fluid exchanging heat with it. On the other hand, when considering irreversible engines, T refers to the temperature of the reservoir only; the temperature of the fluid may then not be the same as that of the reservoir and different parts of the fluid may have different temperatures. The three results (a), (b) and (c) will now be used in the deduction of the characteristics of reversible engines operating between more than two reservoirs. 6.3 Engines operating between more than two reservoirs
In many practical cycles the heat is received and rejected during processes which involve a continuous change in the temperature of the fluid. It has been explained that these cycles can still be considered reversible if the source and sink are each assumed to consist of an infinite number of reservoirs differing infinitesimally 66
Corollaries of the Second Law
[6.3]
from one another in temperature. At any instant during a heating and cooling process, heat must be exchanged between the system and a source or sink which differs only infinitesimally in temperature from the fluid in the system. We have seen that the efficiency with which a given quantity of heat can be converted into work by a reversible engine operating between reservoirs at T, and T2 is given by (T1 — T2 )/ Ti or (1 = T2 / T,). Now let T1 and T2 be the maximum and minimum temperatures of the working fluid in a reversible engine operating between more than two reservoirs. Only a fraction of the heat supplied can be received at T'„ and only a fraction of the heat rejected can be rejected at T2. The remaining part of the heat supplied must be converted into work with an efficiency less than (1 — T2 / T',), because the temperatures of the remaining sources are less than T1 and the temperatures of the remaining sinks are greater than T. Thus the efficiency with which the total heat received is converted into work must be less than (T', — T'2)/ T',. This result may be summarised as the following corollary. Corollary 5 The efficiency of any reversible engine operating between more than two reservoirs must be less than that of a reversible engine operating between two reservoirs which have temperatures equal to the highest and lowest temperatures of the fluid in the original engine. The most important characteristic of engines operating between more than two reservoirs is presented as the sixth corollary of the Second Law; it is known as the Clausius Inequality. Corollary 6 Whenever a system undergoes a cycle, (dQ/T) is zero if the cycle is reversible and negative if irreversible, i.e. in general f(dQ/ T) 5 0. Proof First consider an engine operating between a finite number of reservoirs. The engine is represented in Fig. 6.4a; it may be reversible or irreversible. Let quantities of heat Q1a, 0 ,...,165• • • Q1,, be supplied from sources at temperatures Tia, T1„,..., T1„, and quantities of heat Q2p, Q2q, , Q2z be rejected to sinks at T2 p, , T2z . Now let the sources be supplied with their quantities of heat by a series of reversible heat pumps receiving quantities of heat Qoa, 0 ....0135• • • 5 Q0n from a single reservoir at To. Similarly, let the sinks reject their quantities of heat to a series of reversible heat engines which in turn reject quantities of heat Qop, Q0q,..., Qoz to the single reservoir at To . T, may be any temperature, providing it is less than the temperature of any of the reservoirs of the original engine. The whole plant is represented in Fig. 6.4b. The work delivered by the original engine is given by n
z
EQ1 EQ2 a P
67
[6.3]
Principles of Thermodynamics Fig. 6.4 Proof of the Clausius inequality
(a)
The work delivered by the auxiliary engines is E(Q2 Q0) and the work supplied to the heat pumps must be i(121 —
Q0)
The series of sources and sinks plays no effective part in the transformations of energy, and the complete plant is a system undergoing a cyclic process while exchanging heat with a single reservoir (of temperature T0 ). It follows from the Second Law that the net work overall cannot be into the surroundings, but must be either zero or into the plant. Thus we can write, for the composite,cyclic system, (net workfrom main engine) + (net work front set of reversible engines) — (net work to set of reversible heat pumps) 5 0 This statement can be rewritten, from the First Law, as
E Q1  E Q2 + E (Q2  Q0)  E (Q 1 — 120) o a
p
p
a
which reduces to
E Q0  E Q0 0 a
But for each of the reversible heat engines and heat pumps which operate between only two reservoirs, we can write equations of the form Q1 T1
68
Q = —° TO
between a and ri
Corollaries of the Second Law
[6.3]
Q Q2 = —° T2 To
between p and z
Therefore, substituting for the Q0 terms in the previous inequality, we have Qi
To
_
a Ti
p
Q 2 s S1
Before proceeding to deduce the consequences of the Second Law for 72
[6.5]
Corollaries of the Second Law
steadyflow processes, we shall discuss some of the more important characteristics of the property entropy.
6.5 Characteristics of entropy 6.5.1 Determination of values of entropy
The property entropy arises as a consequence of the Second Law, in much the same way as the property internal energy arises from the First Law. There is, however, an important difference. The change in internal energy can be found directly from a knowledge of the heat and work crossing the boundary during any nonflow process undergone by a closed system. The change in entropy, on the other hand, can be found from a knowledge of the quantity of heat transferred only during a reversible nonflow process. Since equations (6.8) and (6.9) apply to reversible processes, during which the system passes through a series of equilibrium states, they may be applied to any unit mass of the system. The entropy per unit mass, or specific entropy, will be denoted by s, and S = ms when the system is in equilibrium. It is possible, therefore to write the equations as 2 ( dQ =S2 — S1 (6.10) 1 T)rev ds =
(6.11) )rev
implying that dQ is the increment of heat transferred per unit mass of fluid in the system. As with internal energy, only changes of entropy are normally of interest. The entropy at any arbitrary reference state can be made zero, and the entropy at any other state can then be found by evaluating (dQ/ T) for any reversible process by which the system can change from the reference state to this other state. Since no real process is reversible, values of entropy cannot be found from measurements of Q and T in a direct experiment. The entropy is a thermodynamic property, however, and it can be expressed as a function of other thermodynamic properties which can be measured in experiments involving real processes. Two important relations of this kind can be obtained by combining the equations expressing the First and Second Laws. Thus the First Law yields the equation (dQ)rev = du + p dv and combining this with equation (6.11) we have T ds = do + p dv
(6.12)
Alternatively, substituting du = dh — d(pv), we get T ds =
— v dp
(6.13) 73
[6.5]
Principles of Thermodynamics p
Fig. 6.7 Graphical determination of
p
T
entropy
(6)
(a)
(c)
Equations (6.12) and (6.13) are general relations between properties which apply to any fluid. Moreover, when integrated they give the difference in entropy between any two equilibrium states, regardless of whether any particular process joining them is carried out reversibly or not.* We may show how equation (6.12) can be used for compiling tables of values of entropy as follows. The entropy at state 1, defined by (pt , v1 ) say, relative to the entropy at some reference state 0, defined by (po, v0 ), is given by 1
s t — so =
P —du + f —uv 0T o T
(6.14)
The integrals can be evaluated graphically by the following procedure. The end states can be plotted on a p—v diagram and joined by any arbitrary curve as in Fig. 6.7a. (The curve can be chosen arbitrarily because the change of entropy depends only on the end states.) For several pairs of values of p and v along the curve, equilibrium values of u and T can be found from tables of properties. Finally, curves of 1/ T versus u, and p/T versus v, can be plotted as in Figs 6.7b and c. The shaded areas under these curves will be equal to the integrals on the righthand side of equation (6.14), and hence s1 can be found assuming s, is arbitrarily chosen to be zero. Values of s for any other state, defined by different values of p and v, may be obtained in a similar way, and the results can be presented in a table of the form shown in Fig. 1.1. When the properties of a fluid can be related by simple algebraic equations, the integrals of equation (6.14) can be evaluated analytically, and a simple equation for s in terms of p and v, or any other two independent properties, can be determined. Once the functions relating the entropy and other properties have been established, whether expressed algebraically or in the form of a table, there is no need to find the change of entropy by evaluating j(dQ/T),rev• It can be found directly from a knowledge of other properties in the initial and final states.
* The only proviso is that the states must be capable of being joined in principle by a reversible process, because this is assumed in deriving (6.12) and (6.13). Normally this is so. An example to the contrary is when a vapour in a metastable state (supersaturated) changes to a wet vapour in a stable state (see sections 8.2.1 and 18.2). Tables of entropy do not refer to metastable states and this special case can be ignored here.
74
Corollaries of the Second Law
[6.5]
6.5.2 Entropy as a criterion of reversibility
One use of the property entropy has already been indicated in sections 3.5 and 3.6, where it was shown to simplify calculations concerned with reversible adiabatic and isothermal nonflow processes. Another use is suggested by Corollary 8, namely that the change of entropy can be used as a criterion of reversibility. If a nonflow process is adiabatic, this corollary can be applied directly; it states that the entropy will remain unchanged if the process is reversible. When the process is not adiabatic the criterion may be applied in the following way. Any system together with its surroundings can be regarded as one single system. If the term 'surroundings' is used in a special sense to mean only that portion of matter outside a system which is affected by the changes under consideration, the system plus surroundings may be called the `universe'. The quotation marks will be retained as a reminder that the word is used in this restricted sense. The 'universe' is an isolated system, and its entropy must either increase or remain constant in accordance with Corollary 8. If its entropy is determined before and after a change, an increase indicates that the process must have been irreversible. The way in which the entropy changes can therefore still be used as a criterion of reversibility, although when the process is not adiabatic it is necessary to refer to the entropy of the 'universe' and not merely to that of the system. Before presenting an example of this use of the property entropy, we must see how the change in the entropy of a reservoir may be evaluated. It will be remembered that a reservoir is assumed to be a source or sink of such capacity that the quantity of heat leaving or entering it does not cause its temperature to change by more than an infinitesimal amount. Any change in the specific entropy (or any other specific property) is similarly infinitesimal, but since the mass of the reservoir is large, the total entropy change is finite. Because the elements of the reservoir undergo only infinitesimal changes, the process undergone by the reservoir as a whole when the quantity of heat Q enters or leaves it must be considered reversible. If the constant temperature of the reservoir is T, it follows that the entropy change of a reservoir is simply WT. Let us now consider the process of transferring a quantity of heat Q from a reservoir at Ti to a system at a constant lower temperature T2, via an intervening medium which is a poor conductor (Fig. 6.8a). The source and conductor are the surroundings of the system. There is a temperature gradient along the conductor during the passage of energy through it. The heat Q enters the system Fig. 6.8
Fluid boundary layers
External irreversibilities
QI
T,
T,
Poor conductor
System (a)
"1"1 >
1w1=1,2,11$221
T2
T2
Dividing wall
(b)
< T2
(c) 75
Principles of Thermodynamics
[6.5]
by virtue of an infinitesimal temperature difference at the boundary. The system therefore passes through a series of equilibrium states and, as far as the system is concerned, it undergoes a reversible change. Since its temperature remains constant at T2 , there is an increase in the entropy of the system equal to Q/ T2 . The entropy change in the surroundings must now be considered. The change in the entropy of the reservoir is a decrease of Q/T„. No change of entropy occurs in the conductor because it is in exactly the same state after the quantity of energy has passed through it as it was initially. Thus the entropy of the `universe' has increased because Q/ T2 > Q/T,. The complete process must therefore be irreversible. The form of irreversibility just discussed is usually described as external because no dissipation of energy takes place within the system; the irreversibility occurs in the surroundings. Energy can be said to be 'wasted' or 'degraded' because the quantity Q has been transferred to a lower temperature level without producing any of the work of which it is capable. If To is the lowest temperature of any natural infinite sink, such as the atmosphere or ocean, the maximum efficiency with which a quantity of heat at temperature T can be transformed into work is (T — To )/T. Therefore the maximum quantity of work which Q at Ti could theoretically have produced is Q(T, — To )/ T1 , while after its conduction to T2 it is capable of producing only Q( T2 — To)/ T2 units of work. No means exist for returning this quantity of heat to the original temperature level without some expenditure of work (Corollary 1), and so some energy has been irretrievably degraded in the sense that its capacity for producing work has been permanently decreased. An external irreversibility is inevitably present when heat is conducted from one fluid to another through a dividing wall.* For example, when heat is transferred from the furnace gases to the water in a boiler, there is always a considerable temperature difference between the main body of hot gas and the main body of water. Briefly, this is because there are relatively stationary boundary layers of fluid on both sides of the boiler tube which are poor conductors of heat (Fig. 6.8b). The temperature drop across them is therefore considerable. The quantity of heat transferred to the working fluid in an engine can be calculated from the change in the average values of the properties of the fluid during the heat transfer process, and this quantity is the same whether the source is at a much higher, or only an infinitesimally higher, temperature. Thus although an external irreversibility results in the loss of some capacity for producing work, this loss is not expressed directly in the cycle efficiency of a heat engine. The cycle efficiency of the engine illustrated in Fig. 6.8c is still given by I WI/1 0211 = (1421I 1Q21)/1Q11, and the values of 1Q11 and IQ21 are independent of the temperature differences (Ti— Ti ) and (T, — T2 ). The temperature differences adopted in practice are governed by the area of heat transfer surface that is regarded as economic. If the cycle were modified to operate over nearly the full range of temperature available, T', to T2, a higher cycle efficiency would be achieved but a very large heat exchange surface would * A detailed analysis of this process is given in Part IV,
76
Corollaries of the Second Law
[6.6]
be required, so putting up the capital cost. The importance of balancing capital and running costs when designing power plant is discussed in section 11.11. The other source of irreversibility, fluid friction, does cause a dissipation of energy within the system, and it is said to produce an internal irreversibility. The changes in the fluid properties are affected by friction, as explained in section 5.4.1, and the cycle efficieticy is always reduced by this form of irreversibility. 6.6
Consequences of the Second Law for steadyflow processes It must be emphasised that entropy is a thermodynamic property. The entropy
of any element of fluid is a function only of the thermodynamic state and, as already pointed out, such functions are independent of whether the fluid is flowing or not. Each element of fluid of mass 8m in an open system may have a different value of the specific entropy s'. The total entropy S' of the fluid in the system at any given moment is given by S' = E(Sm s'). During any steadyflow process, S' remains constant because the properties at all points within the system do not change with time. We may imagine the steadyflow process to consist of a succession of elementary nonflow Processes as in section 4.1. First, let us consider a steadyflow process during which no heat is allowed to cross the boundary, although work may do so. The entropy of the imaginary closed system in its initial configuration (Fig. 4.2a) is given by Sm s, + S' where s, denotes the specific entropy of the element of fluid which is about to enter the open system. Similarly, the entropy of the closed system in its final configuration is 8m s2 + S' Since the imaginary nonflow process is adiabatic, the final entropy of the closed system must be either greater than or equal to the initial entropy (Corollary 8). Therefore Stn s2 +
S'
8m s, + S'
or 8m s2 > Sin s,
For the steadyflow process we therefore have E(8m s2 ) E(Sm s, ) Since each element of fluid enters the open system with the same properties, denoted by subscript 1, and leaves with the same properties, denoted by subscript 2, this expression reduces to s2
s,
(6.15)
Thus for an adiabatic steadyflow process, the specific entropy of the fluid leaving the system must be greater than or equal to the specific entropy at entry. If the process is reversible, i.e. frictionless, s2 = s,; otherwise s2 > s, . The 77
Principles of Thermodynamics
[6.6]
reversible adiabatic steadyflow process may therefore be called an isentropic steadyflow process. Since a large number of practical steadyflow processes may be assumed adiabatic, relation (6.15) is most useful. First, the principle of increasing entropy informs us of the direction of any real adiabatic flow process; it must occur so that the fluid changes from a state of lower entropy to a state of higher entropy. Sometimes this principle can be used effectively to show that certain flow processes are impossible. For example, in the study of gas dynamics it is used to show that a flow of gas through a shock wave can only be accompanied by a rise in pressure because a fall in pressure implies a decrease of entropy of the gas. Secondly, the equality of entropy at the inlet and outlet of an open system, when the adiabatic process is reversible, can simplify the analysis of many steadyflow processes. Consider for example an adiabatic expansion in a turbine, where the fluid enters with an initial thermodynamic state defined by (p1, vi ), and leaves with a pressure p2 . The values of h1 and si can be found from tables of properties. If the expansion is assumed to be reversible, s2 will be known because it is equal to s1. The final state is now completely determined by the properties p2 and s2, and the value of h2 can also be found from the appropriate tables. The work done can then be found from the steadyflow energy equation W = th(h 2 — h i ) If the adiabatic process is irreversible, the final state cannot be predicted; all that is known is that s2 > si . For the same value of p2 this can be found from the tables of properties to imply that h2 is greater than it would have been after a reversible expansion. This result is in agreement with the earlier discussion of the effect of irreversibility on the expansion in a turbine (section 5.4). But, as already pointed out, the effect of friction cannot be neglected in most steadyflow processes. In practice it is usual to calculate the required quantity on the assumption that the process is reversible, and then multiply the result by a process efficiency to give a more realistic estimate. The process efficiency .in the case of a turbine is defined by turbine efficiency —
work done during the real expansion work done during an isentropic expansion
Process efficiencies must be found empirically, i.e. by carrying out tests on actual components. Their definition is somewhat arbitrary, and no fixed form can be adopted which will apply to all processes. So far we have only considered adiabatic steadyflow processes. The analysis leading up to relation (6.15) must now be repeated for the case of an open system which is exchanging heat with the surroundings. Consider the case of the reversible steadyflow process. When it is reversible, the individual nonflow processes of which it is assumed to consist must also be reversible. In general the heat crosses the boundary along a finite length of the system as the temperature of the fluid changes in the direction of flow. Let increments of heat 8120, 8Q6, , SQ„ cross the boundary at points where the fluid temperature is 78
Corollaries of the Second Law
16.6]
T„, To,..., T,„ during the change of configuration of the imaginary closed system (Fig. 4.2). Then equation (6.8) applied to this process becomes n 8Q (Sms2 +S')—(Sm st +S')= E — a
and hence Sm Sy — Sm s1 =
E
8Q T
Similar equations can be written for every elemental mass passing through the open system. Adding these equations we have, for the whole steadyflow process,
E(Sm s2) — Eom = z To simplify this equation we must assume not only that each elemental mass Sm enters with the specific entropy s1 and leaves, with s2 , but also that each element exchanges 8,1, SQb,... with the surroundings when the temperature is Ta, Tb, . If we make this additional assumption the equation reduces to n 8Q S2— S1 =
where SQ is the quantity of heat per unit mass transferred across the boundary at the point where the fluid temperature is T Also, if the temperature increases continuously from T, to T2 during the process, the equation may be written in the form 12 dQ
s2 — s1 =
—
(6.16)
.
In the special case where T is constant during the process, e.g. when the fluid is a liquid which is being vaporised at constant pressure, equation (6.16) becomes f2
s, —
s2
= — dQ T
and therefore Q = T(s2 — s 1 ) where Q is the heat transfer per unit mass between inlet and outlet. Or, if th is the rate of mass flow and Q the rate of heat transfer per unit time, Q = MT(s, — s1 )
(6.17)
It must be emphasised that equations (6.16) and (6.17) apply only to an internally reversible process, i.e. a frictionless process,* because they are derived * Since friction results in an increase of entropy, it is possible to imagine an irreversible steadyflow process in which the amount of heat rejected results in a decrease of entropy which is just equal to the increase caused by friction. In such circumstances s, will equal s, . Although strictly speaking this would be an isentropic process, it is an unimportant kind. Less ambiguity arises if the term 'isentropic' is restricted to mean a reversible adiabatic process, as will be done throughout this book.
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[6.7]
from equation (6.8). Nevertheless, in many practical cases where heat is received or rejected during a steadyflow process these equations can be applied with sufficient accuracy. For example, the velocity of flow in a boiler or condenser is low, and the effect of friction is negligible. 6.7 Validity and limitations of the laws of thermodynamics
With its emphasis on logical structure, and its reference to axioms and corollaries, this account of thermodynamics may have obscured the important fact that thermodynamics is essentially an experimental science. It is not a branch of mathematics, like Euclidean geometry, although it makes use of mathematical tools as do all the physical sciences. The two 'axioms' of thermodynamics are hypotheses put forward to explain a wide variety of phenomena and a vast range of experimental data. Every experiment which confirms a deduction from a hypothesis confirms and strengthens the validity of the hypothesis itself. The mathematical tools are merely used to draw every possible observable and verifiable consequence from the hypothesis. When a hypothesis is sufficiently well established, it achieves the status of a law. The First and Second Laws of thermodynamics are so well established that we may confidently assume they will remain unchanged in the face of new developments. They may, of course, be shown to be of more limited application than was first supposed, and to be special cases of a more general hypothesis — in much the same way that Newtonian mechanics has been subsumed in the theory of relativity. Indeed this has already happened to some extent with the discovery that mass can be transformed into energy. Mit this has in no way invalidated the application of classical thermodynamic theory to systems in which mass is effectively conserved. It is worth noting some possible restrictions upon the generality of the laws of thermodynamics.* We have already observed that it may not be permissible to apply the First Law to the whole universe to suggest that its total energy is constant. A similar extrapolation of the Second Law is sometimes made which is equally questionable. Since all real processes are irreversible, the entropy of all 'universes' must increase whenever a change occurs within them. This has led to the broad generalisation that the entropy of the universe as a whole is increasing. But the Second Law, like the first, is an expression of the observed behaviour of finite systems and it is not certain that the universe can be regarded as finite. Moreover, the significance of the Second Law for systems consisting of living organisms is not yet clear. There is a definite limit to' the applicability of the laws of thermodynamics at the other end of the scale of magnitude; the laws cannot be applied to microscopic systems which contain only a small number of molecules. The reasons for making this statement are as follows. The thermodynamic state of any system can be completely described by `macroscopic' properties, i.e. properties which are directly observable by the * Advanced students will find a stimulating discussion of this in Ref. 2.
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senses, such as pressure, volume and temperature. Other properties defined in terms of these or deduced as consequences of the laws of thermodynamics are also used but, though more abstract, they are none the less macroscopic in the sense that they are quite independent of any theory as to the molecular or atomic structure of matter. By constructing hypotheses about the 'microscopic' nature of matter, it is possible to regard these macroscopic properties as averages of microscopic quantities. Thus pressure can be regarded, on the kinetic theory of fluids, as the average value of all the rates of change of momentum due to molecular impacts on a unit area of the boundary. These hypotheses must yield results in agreement with the observed macroscopic behaviour of matter, and changes in such hypotheses do not require any modification to be made to the structure of classical thermodynamics. An assumption as to the nature of matter can, however, place a r9striction on the field of application of thermodynamics. The kinetic theory indicates that a thermodynamic system must be large enough to contain a great number of molecules. If a system consists of only a few molecules the concept of pressure, for example, is meaningless. The force exerted by the system on its boundaries would be finite at the points of impact of the molecules and zero at all other points: thus the 'pressure' would not be uniform over the surface nor constant with respect to time, and it would be useless as a characteristic for describing the state of the system. Since, for example, one cubic centimetre of air at atmospheric pressure and temperature contains about 25 x 1018 molecules, this restriction is of little practical importance to engineers. The way in which the laws of thermodynamics lose their meaning when applied to microscopic systems is illustrated by the following discussion of a microscopic engine which appears to contradict the Second Law. On the kinetic theory, the molecules of a gas are rushing about at random with various velocities. If a plate is suspended in the gas it will be bombarded on both faces by the molecules and, on the average, the number and force of the impacts on each face will be equal. If the plate is made so small that only a few molecules are bombarding each face at any given instant, then sometimes the force exerted on one side will be larger than that on the other. The plate could be made to operate a ratchet mechanism, the ratchet wheel only moving when the force on one particular side of the plate predominates. The wheel might turn a winch and raise a weight, so doing work on the surroundings. This microscopic engine does work continuously by merely extracting energy from the gas, e.g. the atmosphere, and no second reservoir is necessary. Such an engine contradicts the Second Law of Thermodynamics. This argument is open to refutation, on the grounds that the microscopic engine is impossible in principle because it would itself be subject to the random motion of the molecules. We have shown how the Second Law loses its meaning when applied to microscopic systems or to an infinite universe. When applied to macroscopic finite systems it has been found to be valid, but it is worth emphasising that its usefulness is limited. The limitation can be seen more clearly from some of the corollaries, such as the Clausius Inequality, rather than from the statement of the law itself. The limitation results from the fact that the corollaries of the Second Law only provide definite quantitative statements about reversible 81
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[6.8]
processes. Only for such processes is it possible to predict the work and heat transfers crossing the boundary of a system. For irreversible processes the law merely provides statements of trend, e.g. that the entropy of an isolated system must increase, and quantitive predictions of energy transfers cannot be made. In engineering calculations empirical 'correction factors' (e.g. process efficiencies) are often used to supplement the Second Law. In effect they express the degree of reversibility of real processes, and they will be introduced formally in Part II. Sometimes a process efficiency is insufficiently illuminating and recourse is made to additional empirical relations which are found to be applicable to a limited range of phenomena. Relations of this kind are used in Part IV, i.e. Fourier's law of heat conduction and Newton's law of viscosity. They all take the form of proportionalities between a quantity transferred in an irreversible process and a property gradient. The constants of proportionality in the examples mentioned are the 'thermal conductivity' and 'viscosity' respectively. These 'laws.' are approximate empirical relations, whose accuracy can be determined by direct experiment; their inaccuracy is manifested by the fact that the 'constants of proportionality' are not in fact constant but vary with the conditions of the experiment (temperature, pressure, or their gradients etc.). The laws of thermodynamics, like Newton's laws of motion, are quite different in kind, being fundamental hypotheses upon which the respective sciences as a whole are based, and which can only be true, false, or shown to be part of an even broader generalisation about nature. We began this section by trying to dispel a misconception that might have resulted from the systematic presentation of the theory, and we may end on the same note. It should not be supposed from this exposition that the science of thermodynamics developed historically in neat logical steps. In common with every science, the concepts which led to a systematic ordering and satisfactory understanding of experience, and which now seem so obvious, required for their birth centuries of experiment and the flashes of insight of some remarkable men. Although a definitive history of thermodynamics has yet to be written, some brief but stimulating accounts can be found. The student will be well advised to supplement his systematic study with a reading of the short historical survey given in Ref. 10. 6.8 Summary of Chapters 1 to 6
With the thoughts of section 6.7 in mind, we may now return to our logical account, and survey briefly the ground we have covered. We opened by defining terms such as 'system', 'property', `temperature', 'work' and 'heat', although they did not all permit of simple definition with equal rigour. For example, we were able to note a few of the characteristics of the concepts of work and heat, such as the fact that they are not properties, but we were unable to define them completely until the First Law was enunciated. This is always the case with any really fruitful concept in an experimental science. Such concepts cannot be described completely in everyday language, and are only definable in terms of the way in which they play their part in the logical framework of the theory. 82
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Corollaries of the Second Law
The more fruitful they are in enabling observable consequences to be deduced from the general law, the more they must rely on the logical structure for their definition;* energy and entropy are excellent examples of such concepts. The notion of energy arose when we applied the First Law to a noncyclic process. We saw that when heat and work cross the boundary of a closed system, there is a property of the system which increases by an amount equal to the net quantity of heat and work entering the system. We called this property the 'internal energy', and we explained the phenomenon by suggesting that heat and work are merely different ways in which 'energy' can be transferred between a system and its surroundings. Energy is the first outstandingly fruitful concept in thermodynamics, and it should be noted that it cannot be defined in terms we have already used without circularity. For example, it is pointless to say that energy is the capacity for doing work, and then define work as a form of transfer of energy. It is nearer the truth to say that energy is a concept which is necessary for the deduction of a variety of observable consequences from the First Law. The First Law refers to any cycle, whether that of a heat engine or a heat pump — and there is nothing in it to say that heat and work are not equivalent in all respects. We might have a cycle (a) in which all the heat supplied is converted into work, or (b) in which all the work supplied is converted into heat. The necessity for the Second Law arises from the fact that heat and work are not equivalent in all respects. The Second Law is not reciprocal like the first, in the sense that it states (a) to be impossible without denying the possibility of (b). It is this lack of reciprocity in the behaviour of cycles which is the fundamental reason why the concept of reversibility has to be introduced. When the consequences of the Second Law for a noncyclic process were deduced, we found that only in the absence of friction and heat transfer across a temperature difference can a change take place without a degradation of energy. When either of these causes of irreversibility is present during a process, some inherent capacity for producing work, in the system or its surroundings, is permanently lost. When the process is reversible, on the other hand, any changes brought about in the system and its surroundings can be undone; nothing irretrievable has occurred. The implications of the Second Law can only be properly expressed in terms of measurable consequences, by using our mathematical tools to deduce a new property of a system — namely entropy. This property could not be deduced in quite such a direct way as internal energy. We had first to show that all reversible engines operating between, the same two reservoirs must have the same efficiency. This, in turn, led us to infer that the efficiency must be a function only of the temperature of the reservoirs — since, in every other respect the engines may differ from one another. When the temperatures of the two reservoirs are defined in such a way that their ratio is equal to the ratio of the quantities of heat leaving and entering the reservoirs, we found that we could devise a * For the advanced student who is philosophically inclined, an interesting discussion of why this , is so can be found in Ref. 1.
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[ 6.81
temperature scale which was independent of the behaviour of any particular substance and which was an absolute scale in the sense that a meaning could be given to the idea of zero temperature. Once we had decided to use temperatures measured on this thermodynamic scale, we were able to widen the scope of our enquiry and investigate the behaviour of engines operating between more than two reservoirs. We found that when the cycle is reversible, the integration of all such quantities as (dQ/T) round the complete cycle must be equal to zero. If the cycle is reversible, there can be no more than an infinitesimal difference in temperature between the reservoirs and the system undergoing the cycle at the points where each quantity of heat dQ is transferred across the boundary. Therefore T can refer to the system as well as the reservoir. It becomes probable that (dQ/T) represents a change in a property of the system, since the total change for the complete reversible cycle is zero. We proved that this is in fact the case, by showing that the integral of (dQ/T) between the end states of any reversible process is independent of the process. The property whose change is given by j(dQIT)re,, is called the entropy of the system. It differs from the internal energy, whose change is given by f(dQ + d W), because the change in entropy can be evaluated from 1(dQ1T) only when the process is reversible. This is no great drawback since we can usually find a reversible process which can be imagined to connect any two given end states and for which we can evaluate 1( dQ/ T) in terms of other properties. The lack of reciprocity in the Second Law can now be expressed in terms of the property entropy. We showed that for any isolated system the entropy must either remain constant or increase; it increases if any process occurring in the isolated system is irreversible. The degradation of energy consequent upon an irreversibility is thereby manifested as an increase in the entropy of the system plus surroundings, or 'universe'. All real processes must occur in such a direction that the state of the 'universe' changes from one of lower to one of higher entropy. Although the reasoning required to deduce the existence of entropy from the Second Law is more complex than that required to deduce the internal energy from the First, the two concepts are of the same type. They are both consequences of empirical laws and are to this extent grounded in experience. If entropy appears the more mysterious, it is only because it is less familiar; the student meets the concept of energy in his early study of mechanics. It is because each is the consequence of an empirical law of great generality that these properties have such significance — much greater significance, for example, than the property enthalpy which was arbitrarily defined as a combination of other properties purely for convenience. The utility of the concepts of internal energy and entropy only becomes apparent when the principles of thermodynamics are applied to particular systems. For the closed systems we are considering, it is an experimental fact that any property can be expressed as a function of two other independent properties when the system is in equilibrium. This fact, together with the laws of thermodynamics, enables a great many useful relations between the properties to be deduced which are universally valid for all such systems. These general 84
[6.8]
Corollaries of the Second Law
relations are deduced in the next chapter, although they need concern only the advanced student. They are necessary because values of the internal energy and entropy are most conveniently obtained indirectly from measurements of other properties; indeed the latter can be obtained in no other way since no system can be put through a reversible process in practice. The next chapter indicates how these general relations may be used when tables of properties are to be compiled. So far we have assumed, and we shall do so again in Part II, that tables of properties are available for any substance we need consider, e.g. that given the values of p and v at any state we shall know the corresponding values of the other properties. We have already shown that this information enables the behaviour of both closed and open systems to be analysed and predicted when the processes are reversible, and also that some of the calculations would be extremely tedious, or even impossible, without the use of the concept of entropy. All this part of the exposition in these first six chapters will be further illustrated in Part II by numerical calculations relating to systems consisting of particular fluids.
85
7 General Thermodynamic Relations*
With the aid of the two laws of thermodynamics and the differential calculus, it is possible to deduce general relations between the thermodynamic properties which hold for any of the limited class of systems considered in this book. Since relations between thermodynamic properties are independent of whether the substance is in motion or not, we need refer only to closed systems. The distinguishing characteristics of the systems considered here are that, when in equilibrium, ( a ) they only change their state when heat and mechanical work cross the boundary, and (b) only two independent properties are necessary to determine their thermodynamic state. These conditions are satisfied, in the absence of surface, gravitational, electric End magnetic effects, by any system consisting of a single substance, even if more than one phase is present. They are also satisfied by systems consisting of a mixture of substances, provided that no chemical reaction is taking place; for example, air is normally treated as a single substance. When mixtures which react chemically are considered, it must be emphasised that only for stable states of chemical equilibrium are two properties sufficient to define the system completely. A mixture of H 2 and 02 at atmospheric temperature is in an apparently stable state only because the reaction H 2 +102 —> H 2 O leading to the most stable state is very slow at that temperature. When such quasistable states of chemically reacting systems are to be considered, more than two properties are required to define the state: in our foregoing example, the proportions of H 2 , 02 and H 2 O in the mixture must be specified as a third property. For a treatment of systems whose composition is variable, the reader is referred to texts on chemical thermodynamics. Some of the more important thermodynamic relations are deduced in this chapter— principally those which are useful when tables of properties are to be compiled from limited experimental data, and those which may be used when calculating the work and heat transfers associated with processes undergone by a liquid or solid. It should be noted that the relations only apply to a substance in the solid phase when the stress, i.e. the pressure, is uniform
* This chapter should be omitted on the first reading.
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[7.2]
General Thermodynamic Relations in all directions; if it is not, a single value for the pressure cannot be allotted to the system as a whole. The chapter ends with an introduction to the concept of exergy and its relation to the Gibbs function.
7.1
Properties to be related We are already acquainted with six properties which may be used to describe the thermodynamic state of a system: pressure, volume, temperature, internal energy, enthalpy and entropy. The first three are directly measurable characteristics. The absolute measurement of pressure and volume presents no difficulty, and we have seen that the introduction of the thermodynamic scale as a consequence of the Second Law makes an absolute measurement of temperature possible. The internal energy u was shown to be a property as a consequence of the First Law and, since the enthalpy h is defined as a function of u, p and v, h is itself a property. Lastly, the entropy s was shown to be a property as a consequence of the Second Law. Two other properties will be added to the list, although they are of less significance to engineers. These are the Helmholtz function f and the Gibbs function g, arbitrarily defined in a similar way to enthalpy by the expressions: f = u — Ts g = h — Ts h, f and g are sometimes referred to as thermodynamic potentials, and g is often referred as the free energy for reasons which will be apparent after a reading of section 7.9. Both f and g are useful when considering chemical reactions,
and the former is of fundamental importance in statistical thermodynamics. The Gibbs function is also useful when considering processes involving a change of phase. Of the eight properties p, v, T, u, h, s, f and g, only the first three are directly measurable. We shall find it convenient to introduce other combinations of properties which are relatively easy to measure and which, together with measurements of p, v and T, enable the values of the remaining properties to be determined. These combinations of properties might be called 'thermodynamic gradients'; they are all defined as the rate of change of one property with another while a third is kept constant. Before proceeding to define them, and to deduce general relations between the properties, it is necessary to review certain theorems concerning the mathematical properties of differentials
7.2 Exact differentials
When the state of a system can be defined by two independent properties, it follows that any third property must be a function of these two. In general terms, any property z can be expressed as z = z(x, y), where x and y are two independent properties. This implies that if x and y change to new values x' 87
[7.2]
Principles of Thermodynamics Fig. 7.1 Geometric interpretation of partial differentials
Constant x Constant y
i
1
dz" —(_ 'z , ay
dy
(x,y,z)
r
az dz' = () dx ax
r)
—
x' (a)
(b)
and y', z will have a new definite value z' irrespective of the process. The function can therefore be represented by a threedimensional surface, as in Fig. 7.1a. Now consider an infinitesimal change from a state defined by the point x, y to that defined by (x + dx), (y + dy). It should be clear from Fig. 7.1b that the change in z is given by dz = I a z I dx + az ) dy x
(7.1)
In mathematics it is common to omit the subscripts on the partial differential coefficients because it is obvious which variable is being maintained constant. However, in thermodynamics it is often necessary to refer to these coefficients out of context of such equations as (7.1). Since any one of the many thermodynamic properties might be kept constant during the change, it is essential to retain the subscript so that we know which third property is being considered. Equation (7.1) is quite general and applies to any infinitesimal change of state. Suppose an infinitesimal change occurs in such a way that z is a constant. Then dz is zero, and (az ) dx — — (az) dy ax FY x But since z is constant, dx = ((34) dy , 2 and substituting for dx in the previous equation we have oz x(— ay ( z) () ax )z
(7.2)
aX y
This is a relation between the three gradients at any point on the threedimensional surface of Fig. 7.1a, he. it is a general relation between the three properties x, y and z at any state and does not refer to a process. 88
[7.2]
General Thermodynamic Relations
Equations frequently arise in thermodynamics in the form (7.3)
dz = M dx + N dy
where, although x and y are known to be properties, z is not necessarily a property. The coefficients M and N may be constants or functions of x and y. An example is provided by the energy equation for a reversible nonflow process: dQ = du + p dv. If an equation such as (7.3) can be expressed in the form of (7.1), it may be inferred that z is a property and that z = z(x, y). If this cannot be done, the equation cannot be directly integrated to give z = z(x, y); z is not a property, and the change in z depends upon the path of the process as well as on the values of x and y at the end states. A simple test by which equations (7.1) and (7.3) can be compared for identity may be devised as follows. Equations (7.1) and (7.3) are identical if M=
az ) ax
and
N = az) OY )x
Differentiating these equations, we have
(am _ a (az)1 a2z ay )x ) 5tayax),J x axay 1 = 02 z (aN) ( ayax
ax
But if z = z(x, y), the magnitude of the second derivative of z with respect to x and y is independent of the order of differentiation, and hence
(am = (aN) ax ay )x )
(7.4)
4
It follows that if (7.4) is satisfied, equations (7.1) and (7.3) are identical, and the quantity z in (7.3) must be capable of being expressed as a function of x and y. dz is then referred to as an exact or perfect differential. Conversely, if the quantity z in (7.3) is known to be a property, (7.4) must be satisfied. Reverting to the example provided by the energy equation for a closed system, M = 1 and N = p in this case. Therefore (aM )
\ay i x \Dv j„
=0 and
( ax ) 4) Iv \du
Reflection on the process of heating a gas at constant volume indicates that in general the rate of change of pressure with internal energy at constant volume cannot be zero. Thus the two partial differential coefficients are not equal, so that dQ cannot be an exact differential and Q is not a property. In order to integrate such an equation the path of the process must be specified in addition to the end states. In this case the path is fixed when the variation of p with v is known.
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[7.3]
When (M dx + N dy) is not an exact differential, it can always be made exact by multiplying throughout by an integrating factor. For our example the integrating factor is 1 / T, because the expression then becomes equal to (dQ/ T), the differential of the property entropy. ds can be substituted for (dQ/ T) in this case because the equation dQ = du + p dv applies to a reversible process. It is important to realise that we have not introduced entropy in the same way as h, f or g — as an arbitrary combination of other properties. The fact that (du + p dv)/ T is an exact differential is a consequence of the Second Law; it is neither selfevident nor a purely mathematical deduction.* This accounts for the considerable significance which attaches to entropy. As the following sections will show, it is possible to deduce a large number of useful relations between the properties of a substance which do not contain entropy at all, but which could not have been deduced without its help.
7.3 Some general thermodynamic relations
The First Law applied to a closed system undergoing a reversible process states that dQ = du + p dv From the Second Law, ds = ( d—Q— T
rev
Combining these equations we have T ds = du + p dv or du = T ds — p dv
(7.5)
The properties h, f and g may also be put in terms of T, s, p and v as follows: dh = du + p dv + v dp = T ds + v dp
(7.6)
df = du — Tds — s dT = —pdv — sdT
(7.7)
dg = dh — T ds — s dT = v dp — s dT
(7.8)
Each of these equations is a result of the two laws of thermodynamics. * In this book we are dealing mainly with systems whose state is determined by two independent properties. The Second Law is not required to show that an integrating factor exists for a total differential which is a function of two variables; this is an established fact in the theory of functions. But the same does not necessarily apply to functions of more than two variables, and the Second Law tells us that even for such cases (ezg. systems involving electric, magnetic or surface tension effects) there always exists an integrating factor for dQ, and that this factor is 1 / T.
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General Thermodynamic Relations
Since du, dh, df and dg are exact differentials, we can express them as du = (au ) ds + au dv as u ay s ah dh = (— )
as P
011) ds + (aP s dp
(If = (af ) dv + ( af ) dT al) T oT v
ag
dg = (
.)
UP
ag
dp + ( ,..._,) dT C1
T
P
Comparing these equations with (7.5) to (7.8), we may equate the corresponding coefficients. For example, from the two equations for du we have
(au ( ) _p = T and as),, av s The complete group of such relations may be summarised as follows:*
(au ) 7, (ah as ), as ), (au ) (af av) , P av )T ah) _( ag ) apI T
(7.10)
a )
(7.12)
af
aT j„
= —s =
( DT p
(7.9)
(7.11)
Finally, making use of the fact that equation (7.4) must hold for equations (7.5) to (7.8), we have
(oat)n _ (a as ) v (as )r ( OT) ap
(71") u = (;v)
(7.13) (7.14) (7.15)
* These relations may be obtained by an alternative argument. Consider equation (7.5), for example; it is quite general and applies to any infinitesimal process. Applying it first to an infinitesimal process at constant volume, we have (du), = T(ds),, or (au/ as), = T Applying it to an infinitesimal process at constant entropy, we have (du), = — p(dv), or (au/Ov), = —p.
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Principles of Thermodynamics
( av) = _( as) aT )1,
[7.3]
(7.16)
op)T
These last four equations are known as the Maxwell relations. It must be emphasised that equations (7.9) to (7.16) do not refer to a process, but simply express relations between properties which must be satisfied when any system is in a state of equilibrium. Each partial differential coefficient can itself be regarded as a property of state. The state may be defined by a point on a threedimensional surface, the surface representing all possible states of stable equilibrium. Suppose, for example, that the coordinates of Fig. 7.1a are u, v and s. If u and v are specified, s is determined, and any gradient of the surface at the point (u, v, s) is also determined. The gradient of a curve formed by the intersection of a horizontal plane with the surface is (au/av)s, and equation (7.10) informs us that the gradient at any point on this curve is always negative and numerically equal to the pressure at that point. All the relations (7.9) to (7.16) can be interpreted graphically in this way. To deduce equations (7.9) to (7.12) we took four forms of the equation expressing the laws of thermodynan1ics, and compared each with an equation expressing one property in terms of two others. The two independent properties were so chosen that a direct comparison could be made of the differential coefficients, e.g. we took u = u(s, v) for comparison with equation (7.5). However, we need not limit the analysis in this way. For example, writing u = u(T,v) we have du = l au dT + (7.: au) dv aT t , tiv r Equating this to (7.5) we get
() dT + (au du = T ds — p du aT av)T or
Tds = (— au ) dT + 1p + (Pt—i ) dv al) T OT „ In this case we may take s = s(T,v) to provide an equation for direct comparison of coefficients, i.e. ds =
aT „
dT + (7. 3.5 ) dv cv T
Then
( as) _ ( au aTi „ 7AaT)„ (as) 1 { T 92
(au
(7.17) (7.18)
General Thermodynamic Relations
[7.4]
Since there are eight properties, and in general each can be written as a function of any other two, it is clear that a very large number of relations can be derived. No attempt will be made here to expand the number of relations systematically,* although a few others will be deduced in the course of illustrating the use of these general relations. It must be remembered that relations obtained by using expressions of the form z = z(x, y) are only valid if x and y are independent. Thus relations based on the assumption that p and T are independent cannot be applied to a mixture of phases. For example, the righthand equations of (7.11) and (7.12) were obtained by writing g = g(p, T). It is shown in section 7.7 that when the temperature or pressure of a mixture of phases is maintained constant, g is constant also. If equations (7.11) and (7.12) were valid they would imply that v and s are zero under these conditions, which is obviously untrue. 7.4 Measurable quantities
Of the eight thermodynamic properties listed in section 7.1, only p, v and T are directly measurable. We must now examine the information that can be obtained from measurements of these primary properties, and then see what other easily measurable quantities can be introduced. 7.4.1 Equation of state
Imagine a series of experiments in which the volume of a substance is measured over a range of temperature while the pressure is maintained constant, this being repeated for various pressures. The results might be represented graphically by a threedimensional surface, or by a family of constant pressure lines on a v—T diagram. It is useful if an equation can be found to express the relation between p, v and T, and this can always be done over a limited range of states. No single equation will hold for all phases of a substance, and usually more than one equation is required even in one phase if the accuracy. of the equation is to match that of the experimental results. Equations relating p, v and T are called equations of state or characteristic equations. Accurate equations of state are usually complicated, a typical form being B C pv = A + — + — + v2
where A, B,C,... are functions of temperature which differ for different substances. An equation of state of a particular substance is an empirical result, and it cannot be deduced from the laws of thermodynamics. Nevertheless the general form of the equation may be predicted from hypotheses about the microscopic structure of matter. This type of prediction has been developed to a high degree of precision for gases, and to a lesser extent for liquids and solids. The simplest postulates about the molecular structure of gases lead to the concept of the * A comprehensive collection can be found in Ref. 3.
93
[7.4]
Principles of Thermodynamics
perfect gas, which has the equation of state pv = RT. Experiments have shown that the behaviour of real gases at low pressure and high temperature agrees well with this equation. Additional refinements to the assumptions lead to the more complicated equations of state. A brief statement of the main assumptions is given in Chapter 8, but for a description of the theory itself the reader is referred to books on the kinetic theory of gases and statistical mechanics.
7.4.2 Coefficient of expansion and compressibility
An equation of state is not the only useful information that can be obtained from p—v—T measurements.: When the experimental results are plotted as a series of constant pressure lines on a v—T diagram, as in Fig. 7.2a, the slope of a constant pressure line at any given state is (aulaT)p. If the gradient is divided by the volume at that state, we have the value of a property of the substance called its coefficient of cubical expansion /3. That is,
=
1( av v aT)p
(7.19)
Values of /3 can be tabulated for a range of pressures and temperatures, or plotted graphically as in Fig. 7.2b. For solids and liquids over the normal working range of pressure and temperature, the variation of /3 is small and can often be neglected. In tables of physical properties /3 is usually quoted as an average value over a small range of temperature, the pressure being atmospheric. This average coefficient may be symbolised by /3, and it is defined by V2  V1
— 1),(71— To Fig. 7.2a can be replotted to show the variation of volume with pressure for various constant values of temperature, as in Fig. 7.3a. In this case the gradient of a curve at any state is (av/ap)T . When this gradient is divided by the volume at that state, we have a property known as the compressibility K of the substance. Since this gradient is always negative, i.e. the volume of a substance always decreases with increase of pressure when the temperature is constant, the
Constant lines
Fig. 7.2 Determination of coefficient of expansion from pvT data
p Constant
Slope =
(a)
94
p lines
v
1.7) p
(b)
[7.4]
Fig. 7.3
General Thermodynamic Relations
V
Constant
Determination of
K=
lines
T
1 ( aV)
compressibility from pvT
Constant p lines
V\,apl T
data
av
Slope =
T
(b)
(a)
compressibility is usually made a positive quantity by defining it as
1 ( av)
(7.20)
vap ) T
Again, for solids and liquids K can be regarded as a constant for many pUrposes. In tables of properties it is often quoted as an average value over a small range of pressure at atmospheric temperature, i.e. V2 — V1
K
vi(P2 — Pi) When f3 and K are known, equation (7.2) may be used to find the third partial differential coefficient involving p, v and T Thus (7.2) becomes
(Op) (aT) (ov) aT v av p
Since
( ay)
and
aT) p
T
1
—
ay
= —KV
( ap T
we have
aP =
\aT
(7.21) K
When the equation of state is known, the coefficients of cubical expansion and compressibility can be found by differentiation. For a perfect gas, for example, we have ( Dv
R
T)p — p
and
( Dv ) ap
RT T
P
2
Hence
1 ( ay) R 1 vaT ) p pu T 1 ( av) _ RT vaph, p2v
_
1 P 95
Principles of Thermodynamics
[7.4]
It will be found in section 7.5 that information about the relation between p, v and T is not sufficient to enable the other properties to be determined, and other measurable quantities must be introduced. These will be discussed in the remainder of this section.
7.4.3 Specific heat capacities There are three more partial differential coefficients which are relatively easily determined experimentally. Consider first the quantity (aulaTL. During a process at constant volume, the First Law informs us that an increase of internal energy is equal to the heat supplied. If a calorimetric experiment is conducted with a known mass of substance at constant volume, the quantity of heat Q required to raise the temperature of unit mass by AT may be measured. We can then write ( Au
(Q )v — AT)„
The quantity obtained in this way is known as the mean specific heat capacity at constant volume over the temperature range AT It is found to vary with the conditions of the experiment, i.e. with the temperature range and the specific volume of the substance. As the temperature range is reduced the value approaches that of (au/aT)„, and the true specific heat capacity at constant volume is defined by
au c, = (— a T) This is a property of the substance, and in general its value varies with the state of the substance, e.g. with temperature and pressure. The First Law also implies that the heat supplied is equal to the increase of enthalpy during a reversible constant pressure process. Therefore a calorimetric experiment carried out with a substance at constant pressure gives us
COT),
=( Q ) AT
which is the mean specific heat capacity at constant pressure. As the range of temperature is made infinitesimally small, this becomes the rate of change of enthalpy with temperature at a particular state defined by T and p, and the true specific heat capacity at constant pressure is defined by ah Cp=() OT p also varies with the state, e.g. with pressure and temperature. Descriptions of experimental methods of determining c,, and cv can be found in texts on physics. When solids and liquids are considered, it is not easy to measure cu owing to the stresses set up when such a substance is prevented
Cp
96
[7.4]
General Thermodynamic Relations
from expanding. Fortunately a relation between c p, c,,, /3 and ic can be found as follows, from which c,, may be obtained if the remaining three properties have been measured. From equations (7.5) and (7.6) we can write
T ds = du + p dv = dh — v dp Putting u = u( T, v) and h = h(T, p), we can also write respectively / du = ( au dT + au dv = c dT + au dv all T v Dv T \ aT/„ / ) \ d7, + ah) (_ dp = cp dT + (— dh = ah ) dp aT ap T ap IT p
Substituting for du and dh in the above equation for T ds, we arrive at
cv dT + { p + (
T
Oh } dv = cp dT — Iv — (— ) 1 dp {u( ap T
As this equation is true for any process, it will also be true for the case when dp = 0, and hence
(cp — cu)(dT)p = {p + ( u ) } (dv)p or
CP
— Cv = IP
ou
ay DvT
4a;()T
aT) p
Now from equations (7.15) and (7.18) we have
(op) (as)
f + p T ov T } () 1
and therefore CP —
OT a =T CT)( av )
p
Finally, from equations (7.19) and (7.21), cp—•C„=
/32 Tv
(7.22)
K
Thus at any state defined by T and v, cv can be found if c p, /3 and K are known for the substance at that state. The values of T, v and K are always positive and, although /3 may sometimes be negative (e.g. between 0 and 4 °C water contracts on heating at constant pressure), #2 is always positive. It follows that cp is always greater than cv. By making use of equation *(7.9), other expressions for c p and ci, can be
97
[7.4]
Principles of Thermodynamics
obtained. Thus since
au) (,„)
.) Cy_
(,,
(.T
we have cv = Ti
as FT
)
(7.23)
,,
Similarly,
as as),(aT),
Oh
P
aT)„
and consequently as
CP
=
(7.24)
T( — aT ),
These two relations will be found useful when expressing entropy in terms of measurable quantities (section 7.5). 7.4.4 JouleThomson coefficient
Consider the partial differential coefficient (DT/ap)h. We have already noted in section 4.2 that if a fluid is flowing through a pipe, and the pressure is reduced by a throttling process, the enthalpies on either side of the restriction may be equal. Fig. 7.4a illustrates the process: the velocity increases at the restriction, with a consequent decrease of enthalpy, but this increase of kinetic energy is dissipated by friction as the eddies die down after the restriction. The steadyflow energy equation implies that the enthalpy of the fluid is restored to its initial value if the flow is adiabatic and if the velocity before the restriction is equal to that downstream of it. These conditions are very nearly satisfied in the following experiment; it was first carried out by Joule and Thomson (Lord Kelvin), and is usually referred to as the JouleThomson experiment. Fig. 7.4
T
Determination of
Constant h lines
Joule—Thomson coefficient P2, T,
p1, Ti
P2, T2
//4'/////////< 1,/// pi, Ti Slope = 1.1
0////7)7/////7/
I
I (a)
98
(b)
[7.4]
General Thermodynamic Relations
A fluid is allowed to flow steadily from a high pressure to a low pressure through a porous plug inserted in a pipe. The pipe is well lagged so that any heat flow to or from the fluid is negligible when steady conditions have been reached. Furthermore, the velocity of flow is kept low, and any difference between the kinetic energy upstream and downstream of the plug is negligible. A porous plug is used because the local increase of directional kinetic energy, caused by the restriction, is rapidly reconverted to random molecular energy by viscous friction in the fine passages of the plug. Irregularities in the flow die out a very short distance downstream of the plug, and temperature and pressure measurements taken there will be values for the fluid in a state of thermodynamic equilibrium. With the upstream pressure and temperature maintained constant at pi and T1, the downstream pressure p2 is reduced in steps and the corresponding temperature T2 is measured. The fluid in the successive states defined by the values of p2 and T2 must always have the same value of the enthalpy, namely the value of the enthalpy corresponding to the state defined by pi and Ti . From these results, points representing equilibrium states of the same enthalpy can be plotted on a T—p diagram, and joined up to form a curve of constant enthalpy. The curve does not represent the throttling process itself, which is irreversible. During the actual process the fluid undergoes first a decrease and then an increase of enthalpy, and no single value of the specific enthalpy can be ascribed to all elements of the fluid. If the experiment is repeated with different values of pi and T1, a family of curves may be obtained covering a range of values of enthalpy (Fig. 7.4b). The slope of a curve at any point in the field is a function only of the state of the fluid; it is the JouleThomson coefficient µ, defined by =(
aT ap)h
The change of temperature due to a throttling process is small and, if the fluid is a gas, it may be an increase or a decrease. At any particular pressure there is a temperature, the temperature of inversion, above which a gas can never be cooled by a throttling process. If a gas is to be liquefied by the Linde process, it must first be cooled below the temperature of inversion. It may be seen that both c p and µ are defined in terms of p, T and h. The third partial differential coefficient based on these three properties can therefore be found from equation (7.2), i.e.
(ah) \apir\avh\ah Hence
ah) _ 491:)) T =
(7.25) P
Summarising: experimental methods are available for determining the p—v—T relation (and hence /3 and K), and also values of ci,, c„ and µ at any state. We
99
Principles of Thermodynamics
[7.5]
must now see how the values of the remaining properties (s, h, u, f and g) can be determined from these experimental data.
7.5 Graphical determination of entropy and enthalpy
Let us assume that v is expressed as a function of p and T in the form of a family of curves (Fig. 7.5). For practical purposes, and in particular for compiling tables of properties, it is sufficient if we can determine the change in entropy and enthalpy between any state (p, T) and an arbitrary reference state (po, To ). The values of these properties at the reference state may be denoted by so and /10; they are usually put equal to zero. Since the change in a property is independent of the process, any convenient path may be considered. We shall proceed from the reference state to any other state by means of a reversible constant pressure process at Po followed by a reversible isothermal process at T (Fig. 7.5). The change in entropy along any constant pressure line can be found by integrating (as/OT)p with respect to T It is notpossible to derive an expression for (as/aT)p in terms of p, v and T, but we may make use of equation (7.24) in the form ( as
c,
aT ) p T The change of entropy between state (Po, To ) and state (po, T) is then given by SOT
dT
SO = To
T
Po
where so,. is used to denote the entropy at a state defined by po and any temperature T Experimental data for c,, at pressure po may be expressed by a single curve of c p versus T, from which Fig. 7.6a can easily be constructed. The integral is then given by the area under the curve between To and any required temperature T The change of entropy along any isothermal can be found by integrating (as/ap)T with respect to p. This coefficient can be expressed in terms of primary Po, T
Fig. 7.5 A possible path between the
Constant p lines
reference state and any other state
Po , To
ov
Slope = (H )p
General Thermodynamic Relations
[7.5] Fig. 7.6 Graphical determination of entropy
cp
av Constant pc, line
T
Constant T lines
aT
Po
(a)
(b)
properties, since the Maxwell relation (7.16) states that av)
a.$) (aP )T
)p
Hence, on integration between the state (po, T) and the state (p, T), we have P V S — SOT = — If a
aT
Po
dp p
The integration may be performed graphically if values of (av/aT)p are plotted against pressure as in Fig. 7.6b. This can be done by measuring the slopes of the constant pressure lines in Fig. 7.5 at the required temperature T The integral is then given by the area under the curve between Po and p. The complete expression for the entropy at any state defined by (p, T), in terms of the entropy at the reference state and the measurable properties p, v, T and c,,, becomes Tr
s = so +
aV
dT}— To
T
Po
Po
aT
i dp p
(7.26)
T
An expression for the enthalpy of a substance can be found in a similar way. The change in enthalpy along a constant pressure line can be found by integrating (ah/aT)p. Since this partial differential coefficient is equal to c,,, the change of enthalpy between the reference state (Po, To), and any other state where the pressure is also po, is given by T p
h oT — ho ={ I To C
dT Po
In this case the integral can be evaluated directly from the curve of c p versus T Again, only values of c p at the pressure Po need be known. To find the change of enthalpy along the isothermal path, we must integrate the partial differential coefficient (Oh/ Dp)r. This quantity may be expressed in terms of p, v and T, although the expression is not given directly by a Maxwell relation as in the case of (as/ap)T . The required expression can be obtained, by repeating the analysis used to determine equation (7.18), but in this case starting with the equations expressing h as a function of p and T Alternatively, the argument contained in the footnote indicated just before equation (7.9) may 101
Principles of Thermodynamics
[7.5]
be used as follows. Applying (7.6) to an infinitesimal isothermal process, we have (dh)T = (Tds)T + (v dp)T Dividing throughout by the change of pressure, this becomes
(— ah ) = T ( as) + v ap T r The Maxwell relation (7.16) may be used to eliminate the entropy term to give
ah) ar) r
ay aT
(7.27) p
Equation (7.27) could now be integrated as it stands, although it would involve the evaluation of two integrals. By substituting T for 1/ T, one of the integrals is eliminated. Thus (7.27) can be written as
(av)
(av) (at (ah p alit)p a7))7, = v T
5t
v
p
and hence
ah) .)1))t.
art)
(7.28)
1p
Integrating between state (po , T) and state (p, T), we have
a rt
h — hoT = fI, .
41 at p T
The integration can be performed graphically if Figs 7.7a and b are constructed. Fig. 7.7a can be deduced directly from the p—v—T data in Fig. 7.5. Then, by measuring the slopes of the constant pressure lines at the required temperature T (and therefore a particular value of t), the appropriate curve of Fig. 7.7b is obtained. The integral is equal to the area under this curve between the limits Po and p. The complete expression for the enthalpy may be written as h = ho + j f c p dT} + To
Fig. 7.7 Graphical determination of enthalpy
VT
Constant p lines
Po
P Po
(
a vt
at
) dp
(avt at
(7.29) }T
p
Constant
T lines
)p
Po
(b)
102
[7.6]
General Thermodynamic Relations
As already stated, so and ho are usually assigned the arbitrary value of zero. It is worth emphasising that the p—v—T data alone are insufficient for the determination of the entropy and enthalpy. Some additional information about the substance along a line of reference states is evidently necessary. It is not essential for the additional data to consist of experimental values of c p; values of the JouleThomson coefficient can be used instead. Thus from equation (7.25) we have c =
(ah) T
and hence from (7.28), Cp =
1 (act)
at
p
The partial differential coefficient (avriat)p is already used in equation (7.29), and values of this quantity at the reference pressure Po and any temperature T can be read from Fig. 7.7b. The required values of c p can then be determined if µ is known for various temperatures at pressure Po. Once the entropy and enthalpy have been obtained, the remaining properties u, f and g are easily found. For example, u = (h — pv) and both h and v are known for any pair of values of p and T Similarly, f is found from (u — Ts) and g from (h — Ts). Note that the value of u at the reference state cannot be zero if ho is put equal to zero. At the reference state (po, To ), the internal energy is uo = ho — Povo = — Po vo It should also be noted that it has been assumed that no discontinuity occurs in the experimental curves during the change from the reference state to the state (p, T). This assumption is invalid if a change of phase occurs, and in such cases it is necessary to determine the changes of entropy and enthalpy in more than two steps. This matter will be referred to again in section 7.7. The following section shows how expressions for the entropy and enthalpy may be deduced when the p—v—T data are given in the form of an equation of state. After a general example, we shall consider two important hypothetical substances which are characterised by two particular equations of state. When the equation of state is known, it is usually easier to work from first principles rather than use equations (7.26) and (7.29).
7.6 Analytical determination of entropy and enthalpy
A typical equation of state giving u as an explicit function of p and T is provided by v=
RT +A— p T2
where R, A and B are constants. We have seen that in addition to this information 103
Principles of Thermodynamics
[7.6]
we require a knowledge of c p or it along a line of reference states. Let us assume that, over the required range of temperature, experiment shows c p to vary linearly with T at zero pressure. That is, when p = 0,
c = C + DT where C and D are constants. The problem is to find expressions for s and h at any state defined by pressure p and temperature T, and we may assume that the values of s and h are put equal to zero at an arbitrary reference state (po,T0 ). We shall work from first principles, and check the result by applying (7.26) and (7.29). Considering s as a function of p and T,
as DT
ds = (—
dT + ( p
as ) dp, Dp T
Using equation (7.24) and the Maxwell relation (7.16), this becomes
ay dp DT p
ds = c—PdT — (—
T
(7.30)
The next step is to find an expression for c p in terms of p and T This can be done because the variation of c p along a line of reference states is given. Using (7.24) again and differentiating,
c = T(L s aT
p
and — ac° = T a2S ap T aT ap
On substitution of the Maxwell relation (7.16), this becomes
(acp)
ap T —
7,( a2 aT.2
Differentiating the characteristic equation, treating p as constant,
( Dv) R 2B and + T )p — p T 3
o2 v
——
6B
Hence
(Dcp = 6B ap IT T 3 Integrating, and remembering that when p = 0, cp = C + DT, we have cp
6B dp) = C + DT + 6Bp T3 T3 = ( f
Substituting for (av/aT)p and c p in equation (7.30), ds = (C + DT +
104
6Bp)dT (R B + L )dp T3 p T3
[7.6]
General Thermodynamic Relations
R p dp) = (— + D)dT — — dp + 2B(L dT — T4 T3 = (— + D)dT — pdp 2Bd (
T3
(7.31)
)
By integration between the reference state (po , To) and any other state (p, T), we obtain s = C ln( T + D(T — To ) — R ln P—
To
Po
— 2B I1 — p0 T3 V,
The enthalpy can be obtained from equation (7.6), dh = Tds + vdp Substituting for Tds from (7.31), and for v from the equation of state, we have dh = (C + DT +
=
(C
+
RT 2B RT )dT — ( + )dp + ( +A T3 p T2 P
B )
6Bp
T2
dp
2p ) DT)dT + A dp + 3B( dT — idp T' T2
= (C + DT)dT + A dp
3B d( ±) I TZ
Therefore h = C(T — To ) +
2
(T 2 — V) ) + A(P — Po ) — 3B( P
P° )
T2 T1
As a check, we may deduce these expressions for s and h from equations (7.26) and (7.29). We have already obtained expressions for c p and (a, v/aT) p, so equation (7.26) becomes s = so
T C + f ro
(— T
D +
6B p P R 2B 4 ) dT} — ti ( + T , , 3 )dp} T T p. po p
I T = so + C ln — + D(T — To ) — 2Bp0 13 — To T Tg
— R In
p
2B
— — (P — Po) T3 Po
= so + Cln— + D( T — To) — R In — 2B( P P° ) To T 3 V, Po
Since s = 0 when p = Po and T = To , so = 0, and this becomes identical with the previous result. In order to use (7.29) we must first find (Ovi/at)p. From the equation of state, VT =
+ AT
BT 3 and
aVT
OT
= A — 3BT 2 )p
105
[7.6]
Principles of Thermodynamics
Hence (7.29) becomes h = hp +
(C +
6Bp DT + — )dT} + T
To
Po
(A — 3htt 2)dp} T
Po
= h0 + C(T — To) + —(T 2 — TO) — 3BPo(1—)
2
2
o.
3B
+ A(p   T  Po) D 2
P
= 120 + C(T — To) + — (T 2 — T4) + A(p — Po) — 3B(, 2
) —To
This again equals the former result when ho is put equal to zero. We may now consider two simple characteristic equations which are of particular significance. All gases at low pressures and high temperatures have an equation of state approximating to the perfect gas equation pv = RT
A better approximation is provided by the van der Waals equation p+ ;)(v — b) = RT R, a and b are constants for any particular gas. The significance of these equations is discussed more fully in Chapter 8, but a few of their consequences will appear here in the course of deducing the relevant expressions for entropy and enthalpy.
7.6.1 Perfect gas Certain information about the internal energy, enthalpy and specific heat capacities of a perfect gas is implicit in the equation of state. Transforming equation (7.18), we have (au \ _ 7,t as V T U7)) 7.
p
which, on substituting the Maxwell relation (7.15), can be written (aav)T T (aaPT)v P But from the equation of state pv = RT,
( op) = R = p aT)„ v T Therefore av ) (au
106
=
0
(7.32)
[7.6]
General Thermodynamic Relations
This means that when T is constant, u does not vary with v. But the existence of an equation of state of any kind implies that when T is constant, p and v are not independent properties. Consequently it also follows that u does not vary with p when T is constant. The final conclusion must be that for a perfect gas u is a function only of T Since the enthalpy is defined as (u + pv), and pv = RT, it follows immediately that h also is a function only of T It is of interest to note that this implies that the temperatures before and after a throttling process must be equal, and therefore that the JouleThomson coefficient it of a perfect gas is zero. The specific heat capacities are defined by
au c„ = (OT )
and
Oh c =( P DT) p
But for a perfect gas u and h are not functions of v and p, and the partial notation may be dropped. Thus du
c, = —
dT
and
dh
c= P dT
and c, and c p are either constants or functions of temperatures only. A relation between c p, c„ and R follows immediately. Since dh = du + d(pv), we have in this case dh = du + RdT and hence
c p — c, = R
(7.33)
Thus, although c p and c, may vary with temperature, their difference is constant. This important result can also be obtained in another way. Froth (7.22) we have the general relation [12 Tv C p — Cv = IC
When pv = RT it has already been shown in section 7.4.2 that /3 and lc are equal to 1/ T and 1/p respectively. Therefore
pv c p — cv = — = R T
Expressions for enthalpy and internal energy can now be written as T
h = h, + i c p dT and To
CT
u = u, + J
c,,.dT To
In this case h and u may be put equal to zero along a line of reference states at To, since they are independent of pressure. We have seen that the perfect gas equation implies that c p and c, are independent of p and v; they must therefore be either constant or some function 107
[7.6]
Principles of Thermodynamics
of temperature. A perfect gas is sometimes defined as one which both satisfies the equation pv = RT, and has constant specific heat capacities. The enthalpy and internal energy of a perfect gas defined in this way are therefore given by the expressions h = c p(T — To ) and
u = c„(T — To)
when u0 and /10 are put equal to zero. And the changes in these properties between any two states at T, and T2 are h2 — h, = cp(T2 —
(7.34)
u2 — u, = cu (T2 —
(7.35)
It now remains to find an expression for the entropy. The simplicity of the equation of state enables equation (7.6) to be used. Writing cp dT for dh, and R/p for vIT, (7.6) becomes ds =
T
dT — — dp p
Therefore, when s is put equal to zero at the reference state (Po, To), T
s=
c
2dT— Rln — To T
Po
If c„ is constant, this reduces to T , P s = cp in — — R in — To Po And the change of entropy between states defined by (pi , TO and (p2, T2 ) is T2 P2 S 2 — Si = C p In— — R In
T,
(7.36)
Pi
In this section, and in Chapter 8, we have introduced the perfect gas by defining it as a substance which has the equation of state pv = RT. It then follows that u and h are functions only of T When approaching the subject in this way, we are assuming that the absolute thermodynamic temperature T can be measured independently of the concept of a perfect gas. Now it is true that this can be done in principle by using a Carnot engine, and even in practice by making use of the ClausiusClapeyron equation (see section 7.7). Or we can adopt the argument that all this is a matter of history and that the International Temperature Scale (ITS90, see section 8.1) on which our instruments are calibrated is essentially equivalent to the thermodynamic scale. But it is a fact that, over a wide range of temperature, thermodynamic temperatures used for fixed points on the International Temperature Scale have been measured by gas thermometry. It is therefore instructive to see how the procedure can be justified without involving a circular argument. What we have to do is to define a perfect gas independently of the concept of thermodynamic temperature, and to
108
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[7.6]
show that an empirical temperature measured by a thermometer using such a gas is identical with the thermodynamic temperature. This we can do as follows. Real gases are known to approximate asymptotically to two laws as their pressures are lowered. First, they obey Boyle's law (7.37)
pv = constant)" constant Secondly, they follow the JouleThomson law h = h(8)
(7.38)
which can be established from the JouleThomson porous plug experiment described in section 7.4.4. Here B denotes empirical temperature measured on any arbitrary scale, and the function h(0) depends on the scale used as well as on the particular gas considered. Boyle's law enables us to define a gas temperature 0, which is a linear function of pv, i.e. pi) = AO,
(7.39)
where A is an arbitrary constant. Extrapolating the product pv to zero provides us with an absolute zero for the perfect gas temperature scale. This, as yet, cannot imply that this zero coincides with that of the absolute thermodynamic scale. Furthermore, we have to show that 0, is identical with the absolute thermodynamic temperature T From a combination of the first and second laws we can write ds =
v dp I jam} T T
Tt
aT
dT — (1)) dp
But because s is a property and therefore ds is a perfect differential, it follows from equation (7.4) that
a s dh(o)i aptT dT j T
s a ( v )1 1.01A TLi p
(7.40)
the derivative within braces on the LHS being total in view of equation (7.38). The LHS of equation (7.40) must be zero, as the term inside braces is merely some function of temperature, and hence from the RHS it fellows that
f a ATv =0 ta7 )}p and therefore (7.41)
v = CP) From equations (7.39) and (7.41) we can write v = TCp) =
AO,
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Principles of Thermodynamics
or G PCP) = AO
(7.42)
Equation (7.42) can only be true for all values of the independent variables p and T if each side is equal to a constant, say K, and hence A
(7.43)
K
From equation (7.39) it is clear that A can be chosen arbitrarily, and thus A/ K can be made equal to unity. Thus we have established that the perfect gas temperature 0, and the absolute thermodynamic temperature T can be made identical, and that they have a common zero datum. To end the discussion on the equivalence OG a 7', we can conclude the following: (a)
From equation (7.38) it follows that h = h(T), and furthermore, because RT, it also follows that u = u( T). (b) From (a) it follows that c,, = and cv = (au/ 0T), for a perfect gas are functions of temperature only. To assume that they are constant is a convenience, approximately true over limited ranges of temperature, and is in no way relevant to the main virtue of the concept of the perfect gas, namely that °G = T (c) By following a procedure similar to the one used in proving the identity OG T, it is possible to show that for a gas which obeys the Boyle and JouleThomson laws, 1/0, is an integrating factor for the energy equation dQ = du + p dv = dh — v dp, without recourse to the Second Law. It is thus possible to arrive at the limited concept of gas entropy dsG = dQ/0, using the First Law only. In fact any differential which is a function of two independent variables must have an integrating factor, but,any differential in more variables has an integrating factor only if it possesses certain special characteristics. The Second Law's contribution, in the mathematical sense, consists in implying first that the integrating factor of dQ is the same, namely 1/ T, for all systems whose state is determined by two independent properties, and secondly that it still exists and is the same, namely 1/ T for more complex systems requiring more than two properties to fix the state. u = h — pv = h(T) —
own,
7.6.2 The van der Waa/s gas
The characteristic equation first suggested by van der Waals is one of a class of such equations in which v is not expressed as an explicit function of p and T It can be recast, however, with p expressed explicitly as a function of v and T, i.e. RT a P=
110
v6v2
[7.6]
General Thermodynamic Relations
In this case it will obviously be more suitable to consider v and T as the independent properties defining the state of the gas. An expression for entropy in terms of v and T can be found as follows: ds=1 as dT + ( as ) dv
aT „
av
T
Using (7.23) and the Maxwell relation (7.15), this becomes ds =
T
dT +
ap`\ dv a Tit,
(7.44)
This is the equivalent of equation (7.30). For the van der Waals gas,
ap ) aT
u—b
So (7.44) becomes
ds =
T
dT +
R dv
—b
and on integration, IT c V — b s = so + t dT + R Inve, — b To T
(7.45)
And if c„ can be assumed constant.,
, T , v 1 b s = so + cv i n— + R i n— — To vo I b When an equation of state has the form p = p(v, 71, it is easier to find the internal energy first and then deduice the enthalpy. Treating u as a function of v and 'T,
du = ( au ) dT + ( au ) dv aT „ au T But (au/aT)v = c„, and from (7.32',) we have
( au) T ( ap ) T
RT P= b
a P = —2
Therefore
a v2
du = cv dT + — dv Integrating, we get (' T U = 140 I
J
c„ dT+
a
(7.46)
To
111
[7.7]
Principles of Thermodynamics
For any state defined by (v, T), the value of u is given by (7.46), p is given by the equation of state, and consequently the enthalpy can be determined from (u + pv). It is apparent that the van der Waals equation, unlike the perfect gas equation, implies that the internal energy and enthalpy vary with both v and T To find whether c also varies with v, we may derive a suitable expression for (acv/av)T . Differentiating (7.23) we get
(act,
T
av
(
a2s aTav)
Using the Maxwell relation (7.15), this becomes
( ct) av T
T( a2 P)
8'1' 2 i v
From the van der Waals equation, ( ap
=
R
v— b
and
( a2P) — 0 aT2
Therefore
Cav )T and hence cv is independent of v. We may again infer that c, is also independent of p and that it can therefore be a function only of T It is evident that even this more accurate equation of state implies that cv is independent of p and v, and this is not for any real gas. 7.7 Change of I:te
While a substanc$ is undergoing a change of phase, the temperature and pressure are not independoit variables. At any given pressure the change takes place at a definite temperature — the saturation temperature Ts., . The field of equilibrium states covering alchange of phase from liquid to vapour is represented by the series of constani pressure lines on the T—v diagram of Fig. 7.8. An important Fig. 7.8 P'
Change of phase and the Clausius—Clapeyron equation
P
T
vg (a)
112
(b)
[7.7]
General Thermodynamic Relations
expression for the rate of change of p with Tsa, can be deduced with the aid of the Gibbs function. From equation (7.8) we have dg = dp — s dT Since p and T are constant during the change of phase, dg is zero, i.e. the Gibbs function is constant. Equating the values of g at the two extreme conditions we have gf
= bi g
where subscripts f and g refer to the saturated liquid and vapour states. If the pressure is changed by an infinitesimal amount from p to (p + dp), the saturation temperature will change from Tsg, to (T + dT)sg„ and the Gibbs function from g to (g + dg). At this new pressure we must also have (g + dg)f (g + dg)g
It follows that dgf = dgg vf dp — sr dTs., = ug dp — sg dTga, or (vg — vf ) dp = (sg — sr) d'Esa,
Now the change of state from f tog occurs at constant temperature and pressure, and thus — —
hg — h f Tat
The previous equation therefore becomes dp d'Tsa,
— hf
(7.47)
Tsat (t)g — v f )
This is known as the ClausiusClapeyron equation; it applies equally to changes from the solid to the liquid phase (fusion, i f) and from the solid to the vapour phase (sublimation, i g). For a small change of pressure Ap, the latent enthalpy (hg — 11,) and difference of specific volumes (ug — v1) can be considered constant, and the average rate of change of pressure with saturation temperature can be written as (Ap/A'Tsat ). In this form the ClausiusClapeyron equation permits the latent enthalpy to be estimated from measurements of vf , ug and the saturation temperatures at two nearby pressures. The ClausiusClapeyron equation also points to one possible way of measuring thermodynamic temperature. Equation (7.47) can be rewritten as d Tsai Tat
ufg dp hfg
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Principles of Thermodynamics
[7.7]
and integrated between (To, pa ), defined by some fixed point, and (T, p), at which the temperature is to be measured. (To, pa) may, for example, be the triple point of water, discussed in section 8.2. This integration yields T In (— = TO
PV
dp
po hrg
sat
Measurements of h fg and vfg over the range pa to p can be made independently of temperature, and T can thus be found. By using solid—vapour, solid—liquid and liquid—vapour changes of phase, as well as different substances, a continuous and wide range of T can be covered. This method of measuring absolute thermodynamic temperature is not used in practice because gas thermometry is more accurate. At the end of section 7.5 it was pointed out that equations (7.26) and (7.29) cannot be applied directly if a change of phase occurs between the reference state and the state at which the entropy and enthalpy are required. When a change of phase occurs, the p—v—T data in Fig. 7.5 will appear as in the v—T diagram of Fig. 7.8b. When the reference state lies within one phase region, and the second state lies within another, the changes in entropy and enthalpy may be found by adding the changes associated with each of four steps, e.g. (a) from state (po , To ) to state 1, (b) from state 1 to state 2, (c) from state 2 to state (pa, T), and (d) from state (po, T) to state (p, T). The changes of entropy and enthalpy during processes (a), (c) and (d) can be found in the way already described. During the constant pressure process (b), however, c p is infinite since the temperature remains constant. For this step the latent enthalpy at po must be known. The value of this quantity may be found by a calorimetric experiment, or by using the ClausiusClapeyron equation as already explained. The change of enthalpy between state 1 and state 2 is then known, since it is equal to hrg, and the change of entropy can be found from S2 — S1 —
h1
h2 T1
The derivation of the ClausiusClapeyron equation has been given here as an example of the use of the Gibbs function. Another example of interest to engineers is provided by the following. We have seen that the Gibbs function has a unique value at any given pressure (or temperature) providing two phases are present. This fact can be used to simplify the calculation of the change of enthalpy during an isentropic process when the final state is in the twophase region. Such calculations are frequently made when analysing the performance of steam turbine plant. By definition g = h — Ts, so that the change of enthalpy during the process can be written as h 2 — h1 = (g2 + T2s2)
(7.48)
Since the process is isentropic, s2 = s1 , and assuming the initial state of the substance is known, the values of h f and s 1 can be found from tables of properties. If the final pressure is given, both T2 and g2 can also be found from the tables, 114
[7.8]
General Thermodynamic Relations
and consequently (7.48) enables (h2 — h1 ) to be calculated. Values of h in the twophase region are not given directly in tables because they depend upon the relative amounts of liquid and vapour in the mixture. The somewhat lengthier method of calculating the enthalpy change when values of g are not available is given in section 10.2. 7.8 Processes undergone by solids and liquids
In a study of heat engines we are primarily concerned with processes undergone by a gas, or a vapour in contact with its liquid, and Part II is devoted to the consideration of such systems. Some processes undergone by solids or liquids will be considered briefly in this section, however, as they provide simple examples of the use of the general thermodynamic relations. Only reversible nonflow processes are considered, but the equations deduced apply equally to solids and liquids with the proviso mentioned in the introduction to this chapter that for solids the stress must be uniform in all directions. 7.8.1 Constant volume process
It was pointed out in section 7.4 that the specific heat at constant volume of a solid or liquid is not easy to measure because of the large pressure required to maintain the substance at constant volume. The rise of pressure consequent upon an increase of temperature at constant volume can be found as follows. Equation (7.21) states that aP
= )6' K
For solids and liquids the variations of and K with pressure and temperature are small. These properties may be assumed constant for many purposes, and mean values /3 and R can be used. With this approximation, the above relation can be integrated for a constant volume process to give p1) ,=, (T2 To
(7.49)
7.8.2 Isothermal process The change of volume accompanying a change of pressure during an isothermal process can be found from the compressibility of a substance. Thus from equation (7.20),
1 ( Di) /3 ap)T Since the volume of a solid or liquid changes only slightly with pressure, a mean value i3 may be chosen. This, together with a mean value of K, enables the 115
Principles of Thermodynamics
[7.8]
expression to be integrated. Since T is constant for an isothermal process, dv = — urc dp and
u2 — v1
—vK(p2 — Pi)
(7.50)
The work done during an isothermal process is given by W=— (
p du .:UR T
P2 Pi
p dp ,,,,,,_ —
2
— pt) lot)
(7.51)
The heat supplied during the isothermal process can be found by using equation (7.30), namely
ds = dT — 8v ( ) dp T aT p
From (7.19), (au / aT)p is equal to fly, and for an isothermal process dT is zero. Hence
ds = — fly dp or dQ = Tds = — Tick dp Again assuming constant mean values iq and 15, this can be integrated to give
Q
(7.52)
—T fiv(P 2 — 19 1)
The change in internal energy can be found from the energy equation, i.e. by substituting (7.51) and (7.52) in u2 — u1 =
Q+w
7.8.3 /sentropic process During an isentropic process, the change in pressure, temperature or volume, accompanying a given change in any one of these properties, can be found as follows. Using equation (7.30) again, and rewriting it as
Tds = c p dT — fluT dp we have, when ds is zero, cp dT = PvTdp Since the temperature rise will be small, a mean value of T can be used in the righthand side of the equation, so that PUT (T2 — Ti ) ^ _ (P2 cp
116
Pt)
(7.53)
General Thermodynamic Relations
[7.9]
Similarly, to find T in terms of v, equation (7.44) can be rewritten as Tds = c,„ dT + T( aP ) dv
aT
But from (7.21), Op / OT)„ = 16/K, and therefore when ds is zero, Tfl
cv dT = — — dv And hence on integration,
—
(T2 — T1 )
.(v2 — v1 )
(7.54)
C„K
Finally, eliminating (T2 — T1 ) between (7.53) and (7.54), l cl, — =(/)2 —
(P2 — P1)
VK Cv
v1)
(7.55)
The work done during an isentropic process is
W= —
p dv)
Using the differential form of equation (7.55), it follows that W
Ree JP' Cp
p dp
p ,
la5 cv
2 EP
2 2 (P2 — Pi)
(7.56)
From the energy equation it follows that this must be equal to the change in internal energy. 7.9 Exergy and the Gibbs function
We close this chapter with an introduction to the concept of exergy, and a further discussion of the use of the Gibbs function. Exergy (sometimes known as availability) is a measure of the maximum useful work that can be done by a system interacting with an environment which is at a constant pressure po and temperature T0. The simplest case to consider is that of a heat reservoir (i.e. a heat source of infinite capacity and therefore invariable temperature) of temperature T We have seen that the maximum efficiency with which heat withdrawn from a reservoir may be converted into work is the Carnot efficiency. Thus the exergy of a reservoir at T providing a heat, transfer Q, in surroundings at T,, is Q(T — To )/ T. The case of greatest interest in engineering is that of a system undergoing a noncyclic process while doing work. Any power plant, even if part of it involves a secondary working fluid being taken through a cycle, when considered as a 117
Principles of Thermodynamics
[7.9]
whole, is a system undergoing a noncyclic process (e.g. see Fig. 11.1). Such a system can be considered to undergo the process while interacting ultimately with a single reservoir, namely the atmosphere at po and To, and the fluid will be incapable of producing any further work when it has reached a state of equilibrium with the surroundings. A comparison of the actual work performed with the maximum possible, starting from a given initial state, is an indication of the effectiveness of the plant used. It will be convenient to consider closed systems and steadyflow open systems separately. In what follows we shall consider systems whose initial states are such that they do work on the surroundings when degenerating to state (po, To ). Similar arguments can be pursued for systems requiring work done on them in order to bring them to state (po , To ), but for simplicity only the former type of system will be considered. 7.9.1 Exergy in closed systems
Let us consider a cylinder containing a compressed fluid at (p,,T,), the cylinder being closed by a piston. We shall calculate the useful work done when the system has reached a state which is in equilibrium with the surroundings and which therefore can be denoted by subscript 0. The initial and final internal energies U 1 and U0 are fixed by the end states (P t , T1 ) and (po, To ), and the work done by the fluid during the expansion, from the First Law, is I WI = — (U, — U1 ) + Q
(7.57)
The useful work done by the fluid on the piston is less than this, because work Po( — V1 ) is done on the surrounding medium which is at a constant pressure p0 .* Thus the useful work W' is I W'l = —(U0 — U 1 ) + Q — po(Vo — V1 )
(7.58)
The principle of increasing entropy states that the sum of the changes of entropy of the surroundings ASo and of the system AS is greater than or equal to zero. Now the change of entropy of the surroundings which are at a constant temperature To, when Q units of heat are transferred from them to the system, is —Q/To . We can therefore write / AS +I —
To
0
or Q * When calculating the work done on a piston elsewhere in the book, we do not subtract the work Po( Vo — l/i) because we always consider the boundary of the system to be the face of the piston, thus ignoring the question of whether this work is entirely transferred to a shaft linked to the piston or whether some of it is transferred to the atmosphere behind the piston. When we are concerned with a sequence of processes constituting a machine cycle, the net work done on the atmosphere in this way is zero, and the total work and the useful work over the machine cycle are equal.
118
[7.9]
General Thermodynamic Relations
and hence W'i
— (U0 — U1 ) + To(So —
— po( Vo — V1)
The maximum value is obtained when the process is reversible and the equality holds, and thus the exergy of the system can be written 1W1. = ( + po — To S, ) — ( Uo + po Vo — To So ) = A 1 — Ao
(7.59)
A = (U + po V — To S) is called the nonflow exergy function. It is seen to be a composite property — composite because it is a property not only of the system but also of its surroundings. In general it will be possible to think of an infinite variety of paths linking states (pi , Ti ) and (Po, To ), both irreversible and reversible; equation (7.59) implies that of these, the reversible paths will all yield the same useful work, namely I 14/1„,ax . Because the surroundings are at the invariable temperature To, the process can be conceived reversible only if either (a) all the heat is transferred when the system is at To (e.g. during process i — 0 in Fig. (7.9a), or (b) the heat exchange with the surroundings is via appropriate reversible Carnot engines working between the system and the surroundings (e.g. during process i — 0 in Fig. 7.9b). It is interesting to note that when the system is in state 0, A is identical with the Gibbs function G defined in section 7.1. Thus G = H — TS which, when expanded and referred to state 0, becomes Go = Ho — To So = U o + PoVo — ToSo = Ao
(7.60)
Let us now consider what appears to be a trivial case, namely when the identity (Pr, T1) = (Po, To) applies. When the closed system contains a gas, this identity also implies identical states and would yield zero work if, say, we compress and expand the gas isentropically. Less obvious is the case of a fluid changing phase isothermally, say from saturated liquid f to saturated vapour g. This still is in accord with the identity, although the states initially and finally are not the same. It would be meaningful to ask what useful work could be produced.
Fig. 7.9 Achieving maximum work from a closed system in surroundings at constant Po and To
T 1
Pi Po
7 To
0
(a)
(b)
119
[7.9]
Principles of Thermodynamics
Applying equation (7.59), I WI. = (U10 + Po KO — ToSfo) — (U go
Po Vgo — Tosco) (7.61)
= — (Hfgo — ToSfgo) or, using equation (7.60), I Wi. = G10 — G80
Since H18 = TSfg, it must be concluded that no useful work can be derived from this process, and all the work done resulting from the absorption of latent heat from the surroundings is expended in doing useless work Po ( Vgo — V10 ) against the pressure po . It follows that G, = Gg, a result already derived in section 7.7. Another case where the initial and final values of p and T are the same, but where the states are different, is when a chemical reaction occurs and reactants R at (po , To ) change to products P at (po, To ). Then we have for the maximum useful work I
Wimax = ( URo + Po VRO ToSRo) = (HR0 — Hp()) To(Spo
UPO + Po //PO TOSPO)
S ) = —4H o + To(Spo — SRO)
(7.62)
Or IWlmax = (GR0 — GK.) = — AG0
(7.63)
AH0 is the enthalpy of reaction discussed in section 15.8 (and in sections 15.4 to 15.6 under the less general title of enthalpy of combustion). It is thus seen that the maximum magnitude of the useful work that can be derived from a closed system containing reactants at (po , To ) in surroundings at (Po , TO is not in general equal to —41/0, because To(Spo — SRO ) usually differs from zero. In calculating the entropy difference (40 — SRO ), the entropies of the reactants and products must be known relative to a common datum. Such information is available as a result of the Third Law of Thermodynamics,* which defines the absolute entropy of substances at absolute zero and thus provides the required common datum. 'Products' in this context must be further qualified as constituents which are in chemical equilibrium taking account of dissociation, and this is discussed more fully in section 7.9.3. 7.9.2 Exergy and steadyflow open systems
Let us imagine that we have an infinite reservoir feeding fluid at (pr , TO with velocity C, at height z, to an open system at a steady rate. In order to derive the maximum amount of work from the system when discharging the fluid into * The Third Law of Thermodynamics postulates that for any pure substance in thermodynamic equilibrium the entropy approaches zero as the absolute thermodynamic temperature approaches zero. Nernst first stated the law in 1907 in a different form, and it is often referred to as the Nernst Theorem. A discussion of the law is outside the scope of this book; the law's main sphere of application is in chemical thermodynamics and lowtemperature physics.
120
[7.9]
General Thermodynamic Relations
surroundings at (po, To ), the fluid must leave at (po, To ) with zero velocity and at the lowest possible datum level zo . Then from the steadyflow energy equation we get IWI = — (thho + thgzo — thh —
— thgzi) +
+ thaCi + gz1)} — {Ho + thgzo} +
=
(7.64)
In practice, particularly when doing an overall analysis of plant such as boilers, turbines or condensers, the kinetic and potential energy terms can be omitted because they are insignificant. When analysing say a turbine, stage by stage in detail, the kinetic energy terms are significant and have to be carried throughout the analysis. For simplicity we shall omit the kinetic and potential energy terms in what follows. With open systems the whole of I gi I is useful work, the work done by and on the surroundings as the fluid enters and leaves the system being included in the enthalpy terms. We can use the same argument as before to establish Q in terms of entropy, and we therefore have I WI
+ T40 — g1)
— ( 14 —
(7.65)
Again the maximum work will be done when the process is reversible and the equality holds. Thus the exergy of the fluid in state 1 is IW
=(II1 — T0,1)  (Clo — WO) = El —Bo
(7.66)
where the quantity B = (H — To S) = (U + pV — To S) is called the steadyflow exergy function. B differs from the nonflow exergy function A = (U + po V — To S) in the pressure term. At state 0, A B G. When a system works between states 1 and 2, where 2 is intermediate between 1 and 0, the maximum useful work quantities associated with the end states are (I gi lmax)1 = B 1 — E0
and (I W Imax)2 = B2 E0
and thus the maximum work available between states 1 and 2 is (7.67)
Wimax)12 = B1 — B2
As an illustration of the use of B, let us consider a gas expanding in a turbine from state (p 1 , T1 ) to a pressure po. Since state 1 is an arbitrary state, the temperature reached after isentropic expansion will not necessarily be To; let us say it will be as in Fig. 7.10a. The rate of work attainable during the isentropic expansion, per unit mass flow, is
I W lisen =
h1) =
p( 7" — T1)
(7.68)
whereas during an actual adiabatic expansion the work will be I WI = — cp(Ti — T1)
(7.69)
The isentropic efficiency of the turbine is then conventionally expressed as I/1/ /linen —
. " isen TAy
(7.70) 121
[7.9]
Principles of Thermodynamics
T
Fig. 7.10
Achieving maximum work from a steadyflow open system in surroundings at constant Po and To
(b)
(a)
Now the maximum useful work per unit mass flow, as derived from the specific exergy function b = B I m, is Lax = 1)1 — 1)0 = (h 1 —110 )— To(s, — so) T,
Pi
,= co(Ti — To ) — c p To in — + RTo ln To Po = c,„(T, — 'I'D+ c p(r— To ) — c To ln = cp(T,— T;) + c pTo t()— 1 — ln
To
(T l' Pi — + RT0 ln—  Po T; To To
(7.71)
We may call the ratio I WI/I WI. the effectiveness E of the process. It is clear that rh„„ s except when cp To [( TW To) — 1 — ln( 7V To)] = 0, and this is = To. Thus the isentropic efficiency possible only in the special case when is a measure not of the fraction of the maximum useful work actually utilised, but merely of the fraction of work available from a particular type of process, i.e. from an adiabatic expansion. Fig. 7.10b illustrates how, in principle, the exhaust gas at T; from an isentropic turbine could supply heat to a series of Carnot engines in order to obtain I W I max as calculated from the exergy function. 7.9.3 The Gibbs function and the steadyflow system
A steadyflow system of particular importance is one in which the fluid enters and leaves at (po, To ). In this case B = G at both entry and exit. When the fluid is . also identical in state at entry and exit, this leads to the trivial case W Imax = G o — Go = 0. Even when the state is not the same, e.g. when the fluid changes phase from saturated liquid f to saturated vapour g, we again have zero work, I W I. = Gfo — Ggo = 0, because the Gibbs function is constant during a change of phase at constant temperature. A case of practical importance, where (p, T) but not the state is identical at entry and exit, arises when considering systems in which chemical reactions occur as in external combustion power plant (see Figs 11.1 and 12.3). For such plant the maximum amount of work would appear as W 'max = °R0 °PO — 122
616 0
(7.72)
[7.9]
General Thermodynamic Relations
or, in terms of the enthalpies and entropies, (7.73) = (liao — TAto) (flpo — TAO = — + To(gpo — That the above expressions are similar to the equivalent equations (7.62) and (7.63) applying to a closed system is not surprising; here we are neglecting the kinetic and potential energy terms, and for the closed system we subtracted the po A V work from I WI. It is of course only under the special conditions of (Pi, T1 ) = (Po, To ) that the two expressions for I WImax and I 14/ Imax are similar. Equations (7.72) and (7.73) have to be qualified in two respects. First, if the products leaving at (Po, To) can still react with the atmosphere, further work could still be done. In combustion, excess air is normally one of the reactants and such further reaction is then negligible, but with other reactions this point may be of importance. Secondly, strictly speaking additional work could still be derived from the products by letting each expand isothermally and reversibly to the partial pressure at which the particular constituent in the products exists in the atmosphere, perhaps by using devices with semipermeable membranes (see sections 14.3 and 15.7). For example, the partial pressure of CO2 in the atmosphere is quite low, while its partial pressure in common products is quite high. Because such processes are impracticable at present, they will be ignored in evaluating I W Imax • If we define the effectiveness of a combustion power plant as I WI/I Wimax, where I W IATM is given by equation (7.73), it is a matter of indifference whether Alio is the value with water in the products as a liquid of a vapour, because the difference between using the one or the other is automatically compensated by the change in the value of the entropy term. That this must be so can be deduced from a comparison of equations (7.72) and (7.73) and the fact that the Gibbs function does not vary during an isothermal change of phase. The need to specify the phase of the water in the products when using conventional definitions of power plant efficiency was * emphasised in sections 15.6 and 17.5. When discussing in section 17.5 the possibility of using I W I/I 14/ Imax in preference to conventional thermal efficiencies for assessing the performance of combustion power plant, we made use of the result of section 15.7.2 for the purpose of evaluating I W In that section we derived Pit I Imax by considering a van' t Hoff equilibrium box operating in surroundings at pa = pe (where pe is the standard state pressure, 1 bar) and at some arbitrary temperature To. We took the simple reaction CO + 102 + CO2 as a specific example, and showed that the maximum work attainable from this reaction in surroundings at (p9, To ) is I WImax=ri To ln Kt
(7.74)
where ii is the molar rate of flow of CO. K 9 is the equilibrium constant given by K° —
(Pco / Pe) (Pco/ Pe)(Po2/ P6)"2
* As stated at the beginning of this chapter, the authors' intention is that it should be left until a preliminary study of the book has been completed, and we underline this here by using the past tense.
123
[7.9]
Principles of Thermodynamics
In principle, KG could be a function of two independent properties, say p and T, determining the state in the equilibrium box. It was proved in section 15.7.2 that KG' was independent of that pressure. However, KG could be a function of the temperature T which is kept equal to the temperature To of the surroundings. It is in fact found by experiment that KG varies markedly with T (= T0). The subscript on KG refers to the temperature of the reaction, i.e. Kt is Ke at To. The form of the relation (7.74) for I 14/ Lax is quite general for all chemical reactions between perfect gases. The remainder of this section is devoted to a discussion of the implications of equating the two. expressions for I 14/ ..Imaxo namely (7.72) and (7.74). It follows immediately that In Kt = —
Agt
(7.75a)
To
and, as we can select To arbitrarily, in general Rio K e = —
(7.75b)
T
Age is the change of molar Gibbs function at (pe, T), namely co — 01). It should be remembered that Ke could, for example, refer to the equation CO + 102 —) CO2 or to the equation 2C0 + 02 2CO2, giving numerically different equilibrium constants
(Pco2/Pe)
(Pco2/Pe)2
and
(Pco/Pe)(Po2 /Pe)"2
(Pco/Pe)2 (Po2 /11°)
It is important to evaluate KG and Age in equations (7.75) for the same form of chemical equation. As stated above, KG is a function of T, and equations (7.75) imply that this must be true of Age. The relation between K° and Age implies that a relation between KG and Age can also be derived, and such a relation can prove particularly useful. Let us proceed by finding (a In K G / OT) p, first at To, and then by varying the reference temperature To. The partial notation can be omitted because K G has been found to be independent of the total pressure p of the mixture. From equation (7.12), then, we can write &no SPo = — dno and gr,c, = — dT dT and substituting in equation (7.73) we obtain
4§t
AR ( dao
d(An) d no ) To To dT dT To dT
or 1 d(Ago) Aat d (An) TI dT To ) To dT
124
Ant
[7.9]
General Thermodynamic Relations
Since, from equation (7.75a), d (t eg) = — R —(ln d Kt) dT To dT it follows that d A (ln Ks ) = dT RT1
(7.76)
Or
d(1/T)
(ln K) = A
R
(7.77)
Equation (7.76), or its equivalent form (7.77), is known as the van' t Hoff isobar. It provides a relation between Ke, temperature T and the enthalpy of reaction AI, which is itself a function of temperature. The relation between 10 and T is difficult to obtain experimentally. However, relations between AP and Age on the one hand, and T on the other, can be obtained more easily, and values of IC' can then be derived from (7.75) or (7.77) over a range of temperature. Furthermore, just as AP at any temperature T can be calculated from a single known value of AR at To together with specific heat capacity data over the range To to T (see section 15.4), equation (7.77) makes it possible for the value of Ke to be calculated at any temperature T from that single value of AR; together with the same specific heat capacity data. This is explained in greater detail in section 15.8. Equations (7.75) and (7.77) can serve a further purpose. Values of 10, Ake and V' are often obtained from different sources using different experimental sources or methods. Such data can be checked for thermodynamic selfconsistency using these equations. To sum up: in this section we have introduced the concept of exergy; related two exergy functions to other thermodynamic functions; and indicated how the concept can provide the basis for less arbitrary definitions of the effectiveness of processes than those in common use. The reader can find a detailed discussion of the rational definition of efficiency of internalcombustion plant in Ref. 12, together with derivations of overall optimum working conditions for several types of externalcombustion power plant. Furthermore, it is claimed that an `exergy balance' is one of the best methods for pinpointing the processes which contribute most to the overall loss due to irreversibilities in complex plant (e.g. in regenerative steam power plant). Certainly it can contrast the relative effects of internal and external irreversibilities, which a mere consideration of cycle efficiency cannot do. To distinguish it from the simple energy balance, such an analysis is often called a Second Law analysis: for further details the reader may consult Ref. 13. Finally, we have employed the concept of maximum work to derive useful relations between the equilibrium constant K e, the enthalpy of reaction Aht and the corresponding change of Gibbs function A.
125
Part II Applications to Particular Fluids
Introduction
The principles of thermodynamics have been explained in Part I without reference to any particular fluid. In Part II we shall apply these principles to closed and open systems consisting of either (a) liquids and vapours whose properties are most conveniently related in tabular form, or (b) gases whose thermodynamic properties can be related by simple algebraic equations. We shall still be concerned only to relate the heat and work crossing the boundary with the changes in the properties of fluid; the detailed analyses of the ways in which the work and heat transfers are effected are dealt with in Parts III and IV respectively. For example, we shall calculate the theoretical work done when a fluid enters a turbine with a certain state and is expanded to a lower pressure, but we shall not stop to consider how the turbine blading should be designed so that the actual work is as near the theoretical value as possible. Part II opens with a description of the characteristics of typical working fluids used in power plant. This is followed by examples of nonflow, steadyflow and nonsteadyflow processes undergone by water and steam, considered as an example of a liquid and vapour, and air, considered as an example of a gas. The performance of the more important thermodynamic cycles is then analysed; for example, it is shown how the cycle efficiency and work ratio can be calculated when the working fluid is taken through a given cycle of states. When engines of the same sort are being compared, the work ratio provides an indication of the size of plant required for a given total output and also an indication of how far the actual efficiency will fall short of the theoretical value. Finally, there is a chapter showing how the behaviour of systems consisting of a chemically inert mixture of fluids can be deduced from a knowledge of the properties of the constituents, and a chapter which is devoted to the thermodynamic aspects of combustion.
129
8 Properties of Fluids
Before describing the way in which the properties of a real fluid are related, with the aid of numerical examples, some system of units must be adopted. Of the three primary properties— pressure, specific volume and temperature — the adoption of units for the first two presents little difficulty. Pressure will always be expressed in bars, and specific volume in cubic metres per kilogram (see Appendix A). A pressure gauge or manometer usually measures the pressure relative to atmospheric pressure. The absolute value, which we shall always imply by the symbol p, can easily be obtained by adding the barometric pressure to the gauge pressure. The unit of temperature needs more careful attention, and the first section is devoted to this topic. This is followed by a description of the characteristics of a liquid and a vapour. The most convenient method of tabulating values of the thermodynamic properties is discussed, and the more important graphical representations are described. Finally, the special case of a gas is dealt with, and it is shown how the assumption of a simple equation of state can lead to an easy analytical treatment of the relations between the properties.
8.1 The unit of temperature and the International Temperature Scale
Temperature measurement is now a field of study by itself, and only the briefest outline can be given here.* Let us first consider the procedure for setting up any empirical state of temperature. As explained in section 1.2, temperature may be defined in terms of the variation of some thermometric property such as the length of a column of liquid in a tube, the pressure of a gas maintained at constant volume, the resistance of a wire, or the EMF produced by a thermocouple. Three items of information must be specified if a scale of temperature is to be reproducible: (a) The particular thermometric substance and property used (b) The numbers to be attached to two standard fixed points (c) The relation between the temperature and the thermometric property * A comprehensive survey of the whole field can be found in Ref. 22, and short summaries in Refs 23 and 32.
130
Properties of Fluids
[8.1]
which is to be used for interpolating between the fixed points and extrapolating beyond them. We shall discuss items (b) and (c) first. Two reference points, called the upper and lower fixed points, may be located on the scale of the thermometer by bringing it into contact with two systems in turn, each at a definite and reproducible temperature. For example, the lower fixed point may be provided by a mixture of ice and water in equilibrium at standard atmospheric pressure, and the upper fixed point by a mixture of water and steam in equilibrium at standard atmospheric pressure. When in a state of equilibrium both these mixtures provide definite and reproducible temperatures. On the Celsius scale the ice and steam points are assigned the numbers 0 and 100 respectively, while on the Fahrenheit scale the corresponding numbers are 32 and 212. There are therefore 100 units or degrees of temperature between the fixed points on the Celsius scale, and 180 on the Fahrenheit scale. We have now to decide how to interpolate between the fixed points and extrapolate beyond them. In the early days of thermometry the simplest procedure was adopted, i.e. the scale was divided into a number of equal parts. This implies that the temperature is defined as a linear function of the thermometric property. Thus, if 0 and X are the numerical values of the temperature and thermometric property, 0= aX + b
The constants a and b are determined by the numbers allotted to the fixed points. On the Celsius scale, a and b can be found by solving the simultaneous equations 0 = aX, + b,
100 = aXs + b
where Xi and Xs are the numerical values of the thermometric property at the ice and steam points. The solution is a=
100 XS
—
b—
Xi'
100X1 X,— Xi
Substituting these values in the original equation for the temperature, we get Oc — 100
X — X, X, — X;
If this procedure is repeated for the Fahrenheit scale we have
0, = 32 + 180
X — Xi XS —Xi
It follows that the relation between the numerical values of temperature on the two scales is 0, = 32 + 1.80c Provided the same thermometric substance and property are used, there is no 131
Applications to Particular Fluids
[8.1]
fundamental difference between the two scales we have been considering. A temperature measured on one scale can always be converted into a temperature measured on the other with mathematical precision. For the moment then, let us assume we are using the Celsius system of numbering, and consider what happens when the substance or property is changed. For example, we might construct the following two scales. For a liquidinglass thermometer we could write Oc = 100 1 Is — I, where 1 is the length of the column of liquid. And for a constantvolume gas thermometer, where p is the pressure, we would have 100 P
Pi
PS —
Pi
If linear interpolation is used : in this way, we find that when any two thermometers using either different thermometric properties or substances are brought into contact with the same heat reservoir, the readings will not be identical except at the fixed points. For example, if the temperature measured by a constantvolume hydrogen thermometer is 40 °C, the temperature recorded by a typical mercuryinglass thermometer will be 40.11 °C and by a platinum resistance thermometer 40.36 °C. If one thermometric property does not vary linearly with the other, the two temperature scales, defined linearly in terms of these properties, cannot be identical except at the fixed points. Unfortunately there is nothing in the foregoing method of setting up a temperature scale to suggest why we should adopt one type of thermometer rather than another as a standard instrument. Moreover the scales are not absolute, because the zero is assigned to some arbitrary point fixed only by convention. Now we have seen (section 6.2) that an absolute scale of temperature arises as a consequence of the Second Law, and that this thermodynamic scale is independent of any particular thermometric substance or property. Also, the temperature defined in this way enables us to introduce the useful concept of entropy. This theoretical scale is clearly a good candidate for adoption as the ultimate standard. It will be recalled that the thermodynamic temperature T must satisfy the relation T = T0 — Qo
(8.1)
where Q and Q, are the quantities of heat absorbed and rejected by a reversible engine operating between reservoirs at T and To. But this relation does not completely determine the scale; we have still to fix the size of the interval or unit of temperature. It was pointed out in section 6.2 that this could be varied by altering the number of engines in the series shown in Fig. 6.3, and there are two ways of approaching the problem. First, we may choose two fixed points, such as the ice point 1; and the steam 132
Properties of Fluids
[8.1]
point Ts, and define the number of degrees between them. For example, we can write Ts — = 100 units. This is equivalent to placing 100 reversible engines in the series between the fixed points. When used in conjunction With the equation Ts/ = Qs/ Q;, this arbitrary choice fully defines a linear thermodynamic scale. Qs/Q; has a unique value because the efficiencies ( = 1 — la/Qs ) of all reversible engines operating between Ts and T, are the same, and thus the two simultaneous equations yield unique values of Ts and T. The main advantage of this approach to the definition of the thermodynamic scale is that it provides a scale which coincides exactly at the fixed points with all empirical scales based on the same fixed points. The second approach, adopted internationally in 1954, is the more obvious one of assigning an arbitrary number to To at one easily reproducible fixed point. Then any other temperature is uniquely defined by T = To(Q/Qo) for the reason just discussed. This approach is equivalent to fixing the number of engines in Fig. 6.3 hf:tween the fixed point and absolute zero. The fixed point chosen for the definition of the thermodynamic scale is the triple point of pure water. A detailed discussion of this state is given in the next section; here it
suffices to say that it is the state at which the solid, liquid and vapour phases can coexist in equilibrium and it is easily reproducible. The pressure of the triple point is very low, i.e. 0.006 112 bar, but the temperature is only slightly above that of the ice point at atmospheric pressure. The internationally agreed number for the triple point To is 273.16, and thus: The unit of thermodynamic temperature is the fraction 1/273.16 of the thermodynamic temperature of the triple point of water.
The unit is called the kelvin, denoted by the unit symbol K. It is pertinent to ask why such an odd number has been chosen. The reason lies in the fact that with this method of definition no exact value can now be attached to Ts — T and it becomes a matter of experiment. The choice of 273.16 K for To, however, makes Ts — T, 100 K within 0.005 K, and thus the new unit is still for many practical purposes the same size as on all previous empirical Celsius scales. The kelvin is not the only thermodynamic unit in use. The other thermodynamic unit, rapidly falling into disuse, is the rankine, which is the fraction 1/(1.8 x 273.16) = 1/491.688 of the thermodynamic temperature of the triple point of water. Thus the kelvin is 1.8 times as large as the rankine (unit symbol R). Nonabsolute versions of the thermodynamic scales are obtained by shifting the zero datum of the scales. For example, the Celsius thermodynamic scale employs the same size of unit or interval as the Kelvin scale, but has its datum at 273.15 K, i.e. at a temperature 0.01 K below the triple point. It should be noted that, although the temperature unit on the thermodynamic Celsius scale is identical with the kelvin, it is customary to denote temperatures measured relative to the 273.15 K datum by the symbol °C. Thus we can write 0 °C = 273.15 K exactly 133
[8.1]
Applications to Particular Fluids
Fig. 8.1
Tc
TK
Relations between thermodynamic scales of temperature
71; =
TR
Tc + 273.15 K
T,
TR
1.8
1 — ( TF + 459.67 R) 1.8
I
TR
T',=
TK — 273.15K
T.
1 —(TR — 491.67R) 1.8
I — (T, — 32 R) 1.8
TR =
1.8 TR
1 .8 Tc + 491. 67 R
TR
TF + 459.67 R
TF =
1.8 TR — 459.67 R
1.8 T, + 32 R
TR — 459.67 R
TF
By choosing this datum we find that 0 °C x ice point, 100 °C ,cr., steam point (both at 1 atm) and therefore have a scale directly comparable with empirical Celsius scales described at the beginning of this section. Similarly, the Fahrenheit thermodynamic scale has the zero datum moved to 459.67 R, i.e. 32.018 R below the triple point, thereby yielding ice and steam points of approximately 32 °F and 212 °F. By shifting the zero we do not alter the fact that the scales are based on the laws of thermodynamics and not on the characteristics of a particular substance, but it does mean that the temperatures are no longer absolute. The relations between the temperatures on the four scales are summarised in Fig. 8.1. In this book, Fahrenheit and Rankine scales will never be used, and it will be clear from the context (or unit notation K and °C) whether an absolute or Celsius temperature is being referred to. Temperature will therefore always be denoted simply by T It should be realised that the unit Celsius (°C) is anomalous in that it fulfils two functions: it tells us that (a') the unit used is the kelvin (K), and (b) the datum is at the absolute temperature of 273.15 K. No other unit symbol serves a dual function like this. And no other quantity is given two symbols for the same unit, namely °C and K. Difficulties arise when subtracting Celsius temperatures, and when multiplying or dividing physical quantities whose units involve a mixture of °C and K. The problem is discussed in Appendix A.3, but the procedures to be adopted can be summarised as follows: (a) The symbol °C should be used only for temperature scale values, for which the datum is the absolute temperature 273.15 K. (b) When subtracting two Celsius temperatures, the unit for the difference is always K, e.g. T2 — Tt = 50 °C — 34 °C = 22 K. (c) When multiplying and dividing quantities whose units involve a mixture of °C and K, the °C and K can be cancelled because they are the same unit. The foregoing is a logical account of the definition of a thermodynamic unit of temperature; the determination of a temperature by using a reversible engine and measuring Q/Qo is of course a practical impossibility. Various indirect methods have been devised of which some details can be found in Ref. 20. These methods usually involve the use of an elaborate type of gas thermometer and are the province of the physicist father than the engineer. The measurement of 134
[8.1]
Properties of Fluids
a single temperature requires months of careful scientific work and the procedures are too intricate for the direct calibration of even precision instruments. For this reason a procedure for establishing a practical scale was adopted, originally at the Seventh General Conference of Weights and Measures in 1927; it was then called the International Practical Temperature Scale 1927 or IPTS27 for short. The latest revision was agreed under the name of International Temperature Scale 1990 or ITS90. Apart from the greater practicality of the instruments used for establishing the ITS90 — namely platinum resistance thermometers over most of the range — there is a further reason for its adoption: the accuracy with which thermodynamic temperatures can be measured by gas thermometry is relatively modest, whereas the reproducibility of measurements on the ITS90 is very great. (No figures for accuracy and reproducibility are given here because they vary over the temperature scale.) Thus two experimenters can agree very closely indeed when measuring a temperature on the ITS90, but they would both be uncertain to a greater degree how far they are from the equivalent thermodynamic temperature. When a distinction needs to be drawn between thermodynamic and ITS90 temperatures, the latter are marked by a subscript 90, i.e. T90. The procedure for constructing the ITS90 is, very briefly, as follows. The thermodynamic temperatures of various easily reproducible states — the triple, melting, freezing and boiling points of very pure substances — have been measured to the best accuracy available by gas thermometry. These temperatures range from the triple point of hydrogen (13.8033 K) to the freezing point of copper (1357.77 K), and they provide a skeleton of fixed points treated as exact values for the purpose of the ITS90. The complete scale is defined by five overlapping ranges, with closely specified instruments (e.g. purity of platinum), and elaborate nonlinear interpolating equations whose constants are calculated from measurements at an appropriate number of intermediate fixed points. The ranges and instruments are as follows: (a) For 0.65 K to 5 K: vapour pressure of 3He and 4He (b) For 3 K to 24.5561 K: constantvolume gas thermometer (c) For 13.8033 K to 273.16 K: platinum resistance thermometer of specified purity (d) For 273.15 K to 1234.93 K; platinum resistance thermometer of specified purity, but using different fixed points and interpolating equations from those used in (c) (e) For 1234.93 K and above: instrument using a blackbody cavity in conjunction with the Planck law of radiation (see equation (23.11)). Further details can be found in Refs 25 and 32. The ITS90 is used by standards laboratories for calibrating scientific instruments. Direct reference to the thermodynamic scale is unnecessary, because the fixed points and interpolation formulae are chosen in such a way that the temperature measured on ITS90 closely approximates the thermodynamic temperature; the difference is within the limits of the present accuracy of measurement. It will be assumed in the following chapters that all temperatures 135
Applications to Particular Fluids
[8.2]
are measured by instruments calibrated to read the ITS90; they are thereby virtually thermodynamic temperatures and the symbol T not T90, will be used. 8.2 Properties of liquids and vapours
We noted in section 1.1 that a knowledge of two independent properties suffices to determine the thermodynamic state of a fluid when it is in equilibrium, and therefore that any other thermodynamic property is a function of the chosen pair of independent properties. We shall consider first the relation between the primary properties p, v and T; the equation expressing this relation for any particular fluid is called the equation of state* or characteristic equation of the fluid. Except for socalled perfect gases, considered in sections 8.5 and 8.6, no simple algebraic equation can be found which will cover all possible states, and the relation is best expressed in either graphical or tabular form. It must be emphasised that the equation of state is essentially an empirical relation; it cannot be deduced by thermodynamic reasoning. Assumptions as to the microscopic structure of a liquid or vapour can lead to a prediction of the form of the equation, but there still remain constants which must be determined by experiment for each substance. We shall refer to this type of prediction again when we consider the behaviour of real gases; for the moment we will consider only the graphical expression of p—v— T relations obtained by direct measurement. Although we are concerned mainly with liquids and vapours it will be necessary to refer briefly to the solid phase also, because of the adoption of the triplepoint of water as a standard fixed point. 8.2.1 p—v—T data
Since we have three variables to consider, the obvious procedure is to measure the variation of one with another while the third is kept constant, and to repeat this for a range of values of the third variable. Imagine unit mass of ice below freezing point, enclosed in a cylinder by a piston under a constant load such that the pressure is one atmosphere (1 atm = 1.013 25 bar). Let us follow the events which occur as heat is transferred to the cylinder while the pressure is kept constant. The temperature rises and the ice expands until a temperature of 273.15 K (0 °C) is reached, as indicated by the full line AB in Fig. 8.2. Further heating does not continue to raise the temperature of the ice, but causes a change to the liquid phase (BC). The change of phase occurs at constant temperature and is accompanied by a reduction in specific volume. The heat required for this process is called the latent heat of fusion; because the pressure is constant, the heat transfer is equal to the change of enthalpy (a property change), which is consequently called the latent enthalpy of fusion. With the system of units used in this book, this enthalpy will be measured in kJ/kg. In contrast to latent enthalpy, the enthalpy change of a substance while its * The relation between p, v and T is sometimes called the 'thermal' or 'temperature' equation of state to distinguish it from 'caloric' equations of state such as u = u(v, T) or It = h(p, T). When using the term 'equation of state' on its own, we shall imply the relation between p, v and T
136
Properties of Fluids
[8.2] Fig. 8.2
G l p= 1 atm G
Isobars on T — v diagram
Vaporisation
373.15 K (100°C)
—F
Er — — —
H2 O 277 K —D Fusion 273.15 K  C B (0 °C)
I Normal substance B
C A
temperature changes is sometimes referred to as sensible enthalpy. Further heating, of what is now a liquid, results in a rise of temperature, a contraction in volume until the temperature is about 4 °C (point D), and subsequent expansion until a temperature of 373.15 K (100 °C) is reached (E). At this point a second phase change occurs at constant temperature with a large increase in volurhe until the liquid has been vaporised (F). The heat required in this case is called the latent heat of vaporisation and the associated enthalpy change is called the latent enthalpy of vaporisation. When vaporisation is complete, the temperature rises once more (FG). Water behaves in an anomalous way compared with other substances, in that it contracts on melting and also contracts before it expands when its temperature is raised above the melting point. The dashed curve in Fig. 8.2 shows the behaviour of normal pure substances. Constant pressure lines such as those in Fig. 8.2 are sometimes called isobars. It must be emphasised that in this and subsequent property diagrams the change in volume of the solid and liquid has been greatly exaggerated in comparison with the volume changes due to the liquid—vapour phase change or the heating of the vapour; the diagrams are not to scale. Let us now consider what happens to water when the same sequence of events is followed through at a lower pressure (Fig. 8.3a). First, there is a slight rise in the melting point (as predicted by the ClausiusClapeyron equation (7.47)). Secondly, there is a marked drop in the boiling point and a marked increase in the change of volume which accompanies evaporation. When the pressure is reduced to 0.006 112 bar, the melting and boiling temperatures become equal and the change of phase, ice—water—steam, is represented by a single horizontal line (bcf). As explained in the previous section, the temperature at which this occurs has been accepted internationally as a fixed point for the absolute temperature scale and is by definition 273.16 K. Only at this temperature, and the pressure of 0.006 112 bar, can ice, water and steam coexist in thermodynamic equilibrium in a closed vessel, and bcf is called the triple point line. If the pressure is reduced still further the ice, instead of melting, sublimates directly into steam.
137
[8.2]
Applications to Particular Fluids
Fig. 8.3 Families of isobars on T—v
P> PC = 221.2 bar
T
T
diagram: (a) water; (b) normal substance
T, = 647.3 K
Critical point p > 1 atrrt G
= 1 atm = 1.01325 bar
c,e b Triple point line 273.16 K
B
2
Sublimation (a) Water
(b)
Normal substance
Consider now the behaviour at pressures above atmospheric. The shape of the curves is similar to that of the atmospheric isobar, but there is a marked reduction in the change of volume accompanying evaporation. At a sufficiently high pressure this change of volume falls to zero, and the horizontal portion of the curve reduces to a point of inflexion. This is referred to as the critical point, and the properties at this state are known as the critical pressure pc, critical temperature Tc. and critical volume DC, The values for water are pc, = 221.2 bar, T. = 647.3 K, v. = 0.003 17 m3/kg At pressures above critical, there is no definite transition from liquid to vapour and the two phases cannot be distinguished visually. The latent enthalpy of vaporisation falls to zero at the critical pressure, and at higher pressures the term has no meaning. Fig. 8.3b shows the corresponding behaviour of normal substances. As the only difference is in the behaviour near the triple point line, only the lefthand portion of the diagram has been shown. It is apparent that normally both the melting and boiling points rise with increase in pressure and that liquids expand on heating at all pressures and temperatures. It is instructive to show graphically how the sublimation, melting and boiling temperatures vary with pressure as in Fig. 8.4, because the origin of the term `triple point' lies in this method of presenting the information. The boiling point curve is obtained by following arrow 1 in Fig. 8.3 from the triple point line to the critical point, and the sublimation point curve by following arrow 2 as the pressure is reduced below the triple point value. Two melting point curves are shown, the full line being for water and the dashed line for normal substances. These are obtained by following arrow 3 in Figs 8.3a and b respectively. The numerical values in Fig. 8.4 refer only to water. In the foregoing we have considered how T varies with v at constant p, and 138
[8.2] Fig. 8.4
Properties of Fluids 71[K]
Triple point of water 647.3
Critical point
373.15 Fusion normal substance 273.16 273.15
Triple point
MM. maa.
Fusion
SP" 0.006 112
1.013 25
221.2
p1 [bar]
for the purpose of introducing the pattern of behaviour of the three phases this is very convenient. We have seen, however, that a p—v diagram is more useful for depicting practical processes. By following a succession of constant temperature (i.e. horizontal) lines in Fig. 8.3, it may be seen that the corresponding p—v diagram of Fig. 8.5 is obtained (the points E, F, G and c, f, g correspond to those in Fig. 83a). Alternatively, each of the isothermals can be imagined to be obtained by allowing a liquid to expand isothermally behind a piston. Since we shall have no need in practice to refer to behaviour in the solid phase, only the portion referring to a liquid and vapour is shown and itis unnecessary to distinguish between water and other substances in what follows. Various terms have been introduced to characterise the different states through which the substance passes during the expansion 1234. From 1 to 2 the substance is an unsaturated liquid, while at 2 it is a saturated liquid. Between 2 and 3 it is a twophase mixture of liquid and vapour or wet vapour. At 3 it is a saturated vapour, and from 3 to 4 an unsaturated vapour. If all the points representing saturated liquid and vapour states are joined to form a curve, i.e. cNf in Fig. 8.5 p—v diagram for water
p/[bar] Critical point 221.2
1.013 25 647
4 0.006 112
c
Triple point line
' 3k
g
373. 1 k 273 IS k V
139
Applications to Particular Fluids
[8.2]
Fig. 8.5, the line separating the liquid and twophase regions is called the saturated liquid line, and the line separating the vapour and twophase regions is called the saturated vapour line. The two lines meet at the critical point N. It is evident that when a substance exists in a saturated state, or as a wet vapour, the pressure and temperature are not independent properties. For example, if p and T are given, the state is not determined because it might lie, anywhere on the line 23. If the substance is known to be a saturated li or a saturated vapour, then the value of either p or T is sufficient to determine its state; and if the substance is a wet vapour, a knowledge of either p and v, or T and v, may be used to determine its state. The pressure at which a liquid vaporises, or a vapour condenses, is called the saturation pressure corresponding to the given temperature; alternatively, the temperature at which these phenomena occur is called the saturation temperature corresponding to the given pressure. The choice of phrasing depends on whether the temperature or pressure is being used as one of the independent variables. Substances referred to as gases are those which lie in the region above the critical isothermal T, at ordinary pressures and temperatures, i.e. they are substances which have a very low critical temperature. This should not be regarded as a rigid definition, however, and the terms 'gas' and 'vapour' are often used synonymously. A substance in a state lying above T cannot be liquefied by isothermal compression; it must first be cooled below the critical temperature. This explains why some substances, e.g. oxygen and hydrogen, were originally called 'permanent gases'. The critical temperatures of these substances are far below the temperature of any freezing mixture that was available in the early days of the science, and more sophisticated methods of liquefaction had not then been devised. A vapour in a state lying along the saturated vapour line fN on Fig. 8.5 is sometimes called a dry saturated vapour, although the additional adjective 'dry' is superfluous in this instance. The term dry vapour may refer to a saturated or an unsaturated vapour. When the vapour is unsaturated, i.e. in a state lying to the right of fN, it is more usual to speak of it as a superheated vapour. The reason for this last term becomes clear when it is realised that the temperature of an unsaturated vapour is always greater than the saturation temperature corresponding to the pressure of the vapour. For example, an unsaturated vapour in state G on curve 34 has the temperature TG, which is higher than the saturation temperature corresponding to the pressure pG. This saturation temperature is the temperature of an isothermal passing through point F. The difference between the actual temperature, and the saturation temperature corresponding to the actual pressure, is called the degrees of superheat. Similarly, an alternative term is also used for an unsaturated liquid, namely compressed liquid. This is because liquid in a state lying to the left of cNM always has a pressure which is greater than the saturation pressure corresponding to the actual temperature of the liquid. Figs 8.3 and 8.5 are twodimensional representations of the relation between three variables. They illustrate effectively the practical method of obtaining such a relation, i.e. by observing the way one property varies with another while the 140
[8.2]
Properties of Fluids
Fig. 8.6
pvT surface for water
third is kept constant. A threedimensional model, however, gives a clearer picture of the fact that only two properties need to be fixed to determine the state of the substance. If p, v and T are plotted along three mutually perpendicular axes as in Fig. 8.6, all possible equilibrium states lie on a surface called the pvT surface. Any reversible process, i.e. succession of equilibrium states, can be represented by a line on the surface. A minor qualification is necessary: under certain conditions it is possible for a substance to be in a state .of equilibrium represented by a point not on the surface. But such a state is not one of stable equilibrium; it must be either an unstable or a metastable state. If it is unstable, any infinitesimal disturbance causes the substance to undergo a spontaneous irreversible process which returns it to a state of stable equilibrium lying on the pv T surface. If the state is metastable, a finite disturbance is necessary; an example of this kind of phenomenon is discussed in greater detail in section 18.2. Having found the empirical relation between the properties p, v and T, the problem that remains is the determination of the internal energy, enthalpy and entropy in terms of the two primary properties chosen to describe the state of the substance. The procedure is somewhat complicated because u, h and s are not directly measurable properties. A proper analysis of the procedure is given in Chapter 7 for advanced students; all that is attempted in the next section is an indication of one possible method in simple terms.
8.2.2 uhs data and specific heat capacities
A method of computing the value of the entropy s at any state defined by (p, v), relative to the value at some reference state (po, v0 ) has been described in section 6.5.1. The equations expressing the First and Second Laws were combined 141
Applications to Particular Fluids
[8.2]
to yield the equation 1 1
SI
p
du + — dv
=
T
(8.2)
0T
and it was shown how the integrals could be evaluated graphically. Now we assumed for this process of integration that, in addition to the p—v—T data, we had a table of properties giving u for various pairs of values of p and v. This latter information is just as empirical as the p—v—T data. Moreover, the p—v—u relation cannot be deduced from the p—v—T relation; some additional experimental information is necessary. Since h = u + pv, values of enthalpy can be obtained directly from the p—v—u relation for ranges of values of p and v, and no additional experiments are required to determine this property. We have thus arrived at the position that both s and h can be expressed in terms of p and v when the p—v—T and p—v—u relations have been determined experimentally. We have already described how the p—v—T data can be obtained; it is the determination of p—v—u data that we have now to discuss. A method of measuring changes of internal energy is suggested by the application of the nonflow energy equation to a constantvolume process, i.e. Q = (u2 — u1 ). We can imagine unit mass of the liquid being heated in a closed container of volume vo. The heat required to raise the pressure from po to pi , p2, p3 etc. can be measured, and these quantities of heat will be equal to the changes of internal energy between state (vo, po ) and the various states (vo, p1), (vo, p2) etc. This procedure can be repeated for other values of v and, if the value of u at state (Po, vo) is put equal to zero, we shall have a series of values of u for a range of states defined by values of p and v. We can then proceed to calculate values of h and s in the manner suggested. It is not essential that the empirical information required to supplement the p—v—T data be in the form of p—v—u data. In Chapter 7 we show how data on specific heat capacity can be used for the purpose. Chapter 7 also describes a method of calculating values of s which only requires sufficient supplementary information to cover a single line of reference states, e.g. a ieries of states at constant pressure, instead of the whole field of possible states. This method obviously requires much less experimental work to be performed. We shall not pursue this matter here, but since we shall find the idea of specific heat capacity particularly useful when dealing with the properties of gases, we will end this section with a discussion of this concept. Originally the specific heat capacity was defined as the heat required to raise the temperature of unit mass of substance one degree. Since the quantity of heat depends upon the process employed to raise the temperature, and an infinite number of processes are possible, there is an infinite number of specific heat capacities. However, only two came to be used in practice: that at constant volume (c,,) was defined as the heat required to raise the temperature of unit mass one degree during a reversible constant volume process, and that at constant pressure (cp) as the heat required to raise unit mass one degree during 142
Properties of Fluids
[8.2]
Fig. 8.7 v2
Determination of c from v u—T data
ut
cv
=
au
aT
v,
Vo
Slope = (au
T (a)
(b)
a reversible constant pressure process.* Now the quantities of heat added during these two processes are equal to the changes in internal energy and enthalpy respectively. The foregoing definitions can therefore be written as c
_ Q,,_Au AT AT'
Ah c = —=— AT AT
(8.3)
The values of cv and c,,, defined in this way, are found to vary with the value of AT i.e. with the range of temperature used in the experiment, and also with the state of the substance at the beginning of the heating process. To ,make the definitions yet more precise, it is the practice in thermodynamics to use the following definitions: Cu=
C
( au\ aT)„
(8.4a)
P11)
(8.4b)
= ( aTI „
These definitions are the limit of the original definitions (8.3) as AT approaches zero. cv and c, can each be seen to be the rate of change of one property with another while a third is kept constant. This is why in general the partial notation is necessary. Being defined solely in terms of properties, c,, and c,, must themselves be properties; they are therefore a function of any two independent properties that can be used to define the state of the substance. This will be made clear if we outline a method for their measurement. cv can easily be found by carrying out the experiment already described for the purpose of obtaining the p—v—u data. If the temperature is measured instead of the pressure, the results can be expressed on a u— T diagram, as in Fig. 8.7a. The slopes of the constant volume lines can be measured at various temperatures to give values of cv corresponding to various values of v and T These may be plotted as in Fig. 8.7b. Note that the arbitrary choice of a reference state, at which u is put equal to zero, does not affect the values of c5. The choice of * It is only necessary that the constant volume process be internally reversible, i.e. that there should be no paddle work, because then the quantity of heat is quite definite and depends only on the equilibrium end states (see section 3.2). However, the constant pressure process must be carried out slowly to make the effect of friction negligible during the expansion, and this implies la,slow rate of heat addition.
143
Applications to Particular Fluids Fig. 8.8 Specific heat capacity at constant pressure
4.8
5.0
4.6
I AC.s. ) ' l''' c
4.0
?,..
.P
. 4.4 .ak
150 bar
o
4.2
ik
3.0 10 0
2.0
300 bar
4.0
[8.2]
50 100 150 200 250
1.0
400 450
Temperature/MI
Temperature/1°C]
(a) Water
(h) Steam
reference state merely fixes the origin of the coordinates in relation to the family of curves in Fig. 8.7a, and does not affect the slope of the curves at any given state defined by values of T and v. A similar plot of cp versus T, this time for various constant values of the pressure, can be obtained by heating the substance at constant pressure, plotting h versus T for various values of p, and measuring the slopes of these curves. The actual variation of c,, with T and p, for water and steam, is depicted in Figs 8.8a and b. It will be noticed that the curves only cover a range of states up to the line of saturation states. This is because the concept of specific heat capacity is meaningful only when the substance exists in a single phase. When more than one phase is present, as in the case of a wet vapour, a substance undergoes a change in enthalpy without any change of temperature during a constant pressure process. c,, would therefore be infinite. The difference between c,, and cv for liquids is very small. Liquids have a low coefficient of expansion, i.e. the change of volume with temperature during a constant pressure process is negligible. Such a process is therefore effectively also a constant volume process, and we can write ( eh) Also, when p is constant the increase of enthalpy is effectively equal to the increase of internal energy because dh = du + d(pv) = du + pdv
du
Therefore for liquids,
ah) a7) p
( au) a7)„
or cp c,,
It is also worth noting that over normal ranges of temperature and pressure the variation of cp and c, is small: this applies to both liquids and vapours. In general, temperature has a greater effect than pressure, but even the variation with temperature can often be neglected for approximate calculations. Thus when the range of temperature and pressure is not too large in any process considered, mean values of c,, and can be chosen and assumed constant for 144
[8.3]
Properties of Fluids
that particular process. As we shall show later, this procedure considerably simplifies many calculations. Finally, a word about units. In the SI the coherent unit of c, and c„ is the J/kg K, and the multiple we shall normally use is the kJ/kg K. When calorimetric heat units are used, it is evident from their definition (see footnote in section 2.3) that the value of the specific heat capacity will be the same in any system, e.g. 1 kcal/kg K= 1 Chu/lb K= 1 Btu/lb R and that all such units of specific heat capacity are 4.1868 times greater than the kJ/kg K.
8.3 Tables of properties
We are now in a position to describe the most convenient way of setting out the relations between p, v, T, u, h and s in a tabular form. The simple type of table illustrated in Fig. 1.1 is not used in practice because, by adopting the following method, the necessary information can be presented in a much more condensed form. All the properties for the whole fluid of Fig. 8.5 can be given in three tables, and for many purposes sufficiently accurately in only two. 8.3.1 Saturation table
We have noted that when a substance is known or specified to be either a. saturated liquid or a saturated vapour, its state is completely determined when the value of one property is given. If pressure is chosen to be the independent variable, the corresponding saturation values of all other properties of the liquid and vapour can be set out as in Fig. 8.9. The subscripts f and g refer to saturated liquid and saturated vapour respectively. The subscript s is added to temperature because this is the same for both phases in the saturated state; when temperature is chosen to be the argument of the table, p carries the subscript s and these two columns are interchanged. Sometimes, for brevity, the internal energy is not listed because it can easily
Fig. 8.9 Table for saturated water and steam
P
7
[bar]
PC]
of
r
vg
1
L kg i 0.006 112 0.010 1 1.013 25 1 220 221.2
0.01 7.0
0.001 000 2 0.001 000 1
m 1 kg ] 206.1 129.2
100.0
0.001 044
1.673
373.7 374.15
0.002 69 0.00317
0.003 68 0.00317
si.
h,
s9
of
lig
/If
[L kg]
kJ
F kJ 1
rkJ1
r kJ
F kJ 1
kg
g
[kg ]
[kg
L kg K
L kg K i
0 29
2375 2385
2501 2514
0 0.106
9.155 8.974
419
2507
419
2676
1.307
7.355
1949 2014
2097 2014
2008 N84
2178 2084
4.289 4.430
4.552 4.430
0.0006 29
]
145
Applications to Particular Fluids
[8.3]
be obtained from the values of p, v and h, i.e. of = hf — pv f and ug = hg — pvg The values of of may also be omitted, or given in a separate shorter table, because the specific volume of a liquid varies so little with pressure. Thus, for water, of varies only from 0.001 00 m3/kg at the triple point to 0.001 29 m3/kg at a pressure of 50 bar, whereas when the liquid is transformed into saturated vapour the respective specific volumes become 206.1 m3/kg and 0.0394 m3/kg. Indeed it is often sufficiently accurate to assume a constant value for vf, and for water at moderate pressures' the value of 0.001 m 3/kg is frequently used. On the other hand, where brevity is not important, the differences (h, — h f) and (sg — s f) are allotted columns in the table because they are so frequently required. For convenience they are denoted by the symbols hfg and sig. Since the heat added in a reversible constant pressure process is equal to the increase of enthalpy, the latent heat of vaporisation must be equal to hfg. It will be appreciated that the tables only give the difference between the internal energy, enthalpy or entropy at any state and the value of the respective property at a reference state. The internal energy and enthalpy cannot be zero at the same reference state, however, because they are related by h = u + pv. Thus if u is put equal to zero at a state defined by (po, vo), the value of h at this state is po vo. For steam tables, based on the International Skeleton Tables 1963, the liquid at the triple point is chosen as the datum state and both uf and sf are put equal to zero at this state.* The value of the enthalpy at this state is therefore h f = + pv f = 0 + 0.006 112[bar] x 1051"21 x 0.001 000 2 [ 31 kg L bar x 10 3 [
kN m kJ or J Nm
= 0 +0.006112 x 0.001 000 2 x 102 kJ/kg = 0.000 611 2 kJ/kg
(8.5)
The saturation table for steam extends from the triple point pressure of 0.006 112 bar to the critical pressure of 221.2 bar. At the critical pressure the properties with subscript f become equal to the corresponding properties with subscript g, i.e. ufg, kg and sfg are all zero. A knowledge of the properties along the saturation line enables the properties at any state in the wet region to be easily computed, and no separate table is required. The reason is that a wet vapour is a mixture of saturated liquid and saturated vapour. When two masses of the same substance, at the same pressure * In earlier steam stables the datum state used was saturated liquid at 0 °C, whereas the lowest temperature at which saturated liquid can exist is 0.01 °C (see the boiling curve in Fig. 8.4). Thus the datum state was an unstable state arrived at by extrapolation. Furthermore, it was hr and not ur which was put equal to zero at the datum state. The shift to the new datum has little effect on numerical values, amounting only to —0.0416 kJ/kg for enthalpy and —0.000 15 kJ/kg K for entropy.
146
[8.3]
Properties of Fluids
and temperature, are brought together, they will be in equilibrium with oneanother and there will be no change in pressure or temperature. The same argument can be applied to any intensive property, i.e. to any property whose value is independent of the mass of the system. It cannot be applied to extensive properties, such as V, U, H and S, whose values depend upon the amount of substance under consideration. An extensive property of a combination of the two masses is equal to the sum of the corresponding extensive properties of the individual masses. For example, if two masses m1 and m2 at the same pressure and temperature have specific volumes v1 and v2, the total volume on combination is given by V, = V, + V2 = Mi
M2 V2
will be meaningful to speak of the specific volume of the combination if the two masses are homogeneously mixed. Then we have
It
V3 
V3
M I lli
m3
M2V2
M1 + M2
All the specific properties, which are derived from extensive properties, can be treated in this way. The foregoing provides the clue to the treatment of a wet vapour. Unit mass of wet vapour can be regarded as a mixture of x kg of saturated vapour and (1 — x) kg of saturated liquid, each having different specific properties denoted by subscripts g and f respectively but the same pressure and temperature. These specific properties can be read from the saturation table when the pressure or temperature of the wet vapour is known. Any specific property of the wet vapour can then be found by adding the corresponding extensive properties of the two constituents which together make up unit mass of wet vapour. Thus u = (1 —x)uf +xug h = (1 — x)h f + xhg s = (1 — x)s, + xsg When the difference columns are given in the tables, i.e. properties denoted by the subscript fg, less arithmetic is required if the equations are expressed in the form (8.6) U = Uf
XUf g
h = h f + xh fg
(8.7)
s = s f + xsig
(8.8)
The physical interpretation of (8.7), say, is that the enthalpy of unit mass of wet vapour is equal to the enthalpy of unit mass of saturated liquid plus the increase of enthalpy entailed by the evaporation of a proportion x at constant pressure. The specific volume of the wet vapour is similarly given by v = (1 — x)vr +
g
(8.9) 147
Applications to Particular Fluids
p/[bar]
T [°C]
( 7;/[°C]) 15 (198.3)
20 (212.4)
30 (233.8)
40 (250.3)
vs ug he sg vg Li, hs ss vs us he sg v8 ug
ha ss
0.1317 2595 2792 6.445 0.0996 2600 2799 6.340 0.0666 2603 2803 6.186 0.0498 2602 2801 6.070
v u h s
[8.3]
200
250
300
350
400
450
0.1324 2597 2796 6.452
0.1520 2697 2925 6.711 0.1115 2681 2904 6.547 0.0706 2646 2858 6.289
0.1697 2784 3039 6.919 0.1255 2774 3025 6.768 0.0812 2751 2995 6.541 0.0588 2728 2963 6.364
0.1865 2868 3148 7.102 0.1386 2861 3138
0.2029
0.2191 3035 . 3364 7.423 0.1634 3030 3357 7.283 0.1078 3020 3343 7.082 0.0800 3010 3330 6.935
v
u h s v u h
s v/[m3/kg] u/[kJ/kg] h/[kJ/kg] s/[kJ/kgK]
6.957
0.0905 2845 3117 6.744 0.0664 2828 3094 6.584
2952 3256 7.268 0.1511 2946
3248 7.126 0.0993 2933 3231 6.921 0.0733 2921 3214 6.769
NB: The entries throughout are regarded as pure numbers, and therefore the symbols for the physical quantities should be divided by the appropriate units as shown at p/[bar] = 40 and explained in Appendix A, section A.1. Because of lack of space,
this has not been done for the other pressures in Fig. 8.10 or for any of the pressures in Fig. 8.11. Fig. 8.10 Table for superheated steam
but this time the expression is modified in a different way. The term containing vf can often be neglected, and in this case v = xv
(8.10)
This simplification cannot be employed when the fiaction x is small or the pressure high, but equation (8.10) will always be used unless otherwise stated. The quantity of saturated vapour in unit mass of wet vapour, denoted by x, is referred to as the dryness fraction, or quality, of the vapour. The dryness fraction increases from 0 to 1 as the state of the substance changes from E to F in Fig. 8.5. It is a quantity which depends only on the state of the wet vapour, and it is therefore a property. In effect we have chosen to define the state of a wet vapour by (p, x).* If p and v are known, however, it is a simple matter to find x from (8.9) or (8.10) and then use (8.6), (8.7) and (8.8) to calculate the remaining properties. 8.3.2 Superheat table
When the vapour is superheated, the two properties usually chosen as the independent variables for the table are pressure and temperature. At any given pressure a superheated vapour may have any temperature greater than the saturation value. Fig. 8.10 illustrates one method of tabulation which enables the values of v, u, h and s to be found at any state defined by a pair of values * One practical reason for doing this is that in many circumstances the dryness fraction is more easily measured than the specific volume. A method of measuring the dryness fraction is described in section 10.3.
148
Properties of Fluids
[8.3]
p/[bar] (7;/[°C]) 100 (311.0) 221.2 (374.15)
500
1000
T/[°C]
0.01
100
200
300
350
374.15
P. v 1/10 2 hr sr
0.006112 0.1000 0 0
1.01325 0.1044 419 1.307
15.55 0.1157 852 2.331
85.92 0.1404 1345 3.255
165.4 0.1741 1671 3.779
221.2 0.317 2084 4.430
(v  v1)/102 (h  hr ) (s  se ) 2 (u  v f )/10 (h  hi) (s  sr)
0.0005 +10 0.000
0.0006 +7 0.008
0.0009 +4 0.013
0.0007 2 0.007
0.0011 +22 +0.001
0.0012 +17 0.017
0.0020 +9 0.031
0.0051 12 0.053
0.0107 34 0.071
(v  v r )/10 2 (h  h f ) (s  sr) (v  v r )/10 (h  hr ) (s  sr)
0.0023 +49 0.000
0.0024 +38 0.037
0.0042 +23 0.068
0.0117 21 0.134
0.0298 94 0.235
0.161 269 0.670
0.0044 +96 0.007
0.0044 +76 0.070
0.0075 +51 0.124
0.0191 17 0.235
0.0427 119 0.385
0.180 415 0.853
0 0 0
NB: See note to Fig. 8.10. Fig. 8.11
Table for compressed water
The properties of superheated steam have been obtained for pressures up to 1000 bar and temperatures up to 800 °C. It will be noticed that the numbers in any vertical column cease when the saturation temperature corresponding to the pressure becomes greater than the value of the temperature at the head of the column. In abridged tables, where space saving is important, these columns are sometimes headed with 'degrees of superheat' rather than with the actual temperature of the vapour. There will then be no vacant spaces in the table. Owing to the need for two independent variables, the superheat table is inevitably much more lengthy than the saturation table. For this reason the internal energy is often not included and must be found from (h  pv).
(p, T).
8.3.3 Compressed liquid table
When the pressure of a liquid is higher than the saturation pressure corresponding to the temperature of the liquid, the state lies in the region to the left of MNc in Fig. 8.5. The pressure and temperature can be varied independently, and can therefore be considered to be the independent variables as in the case of a superheated vapour. Consequently the properties may be tabulated in the same way, i.e. as in Fig. 8.10. In fact it is possible to combine the compressed liquid and superheat tables by entering the compressed liquid data in the vacant spaces of Fig. 8.10. It is found, however, that the properties of a liquid change very little with pressure and it is often more convenient to list the compressed liquid values as deviations from the corresponding saturation values taken at the same temperature. Such a table is shown in Fig. 8.11. At ordinary pressures, say below 50 bar, deviations are very small and the properties v, u, h and s can ibe assumed to equal the saturation values vf, u f, h1 and sr at the temperature of 149
Applications to Particular Fluids
[8.4]
the compressed liquid. This is equivalent to assuming that curves such as 12 in Fig. 8.5 are vertical straight lines (i.e. that the liquid is incompressible), and that the internal energy of a compressed liquid is a function only of temperature. We shall usually make this assumption in subsequent chapters. • The properties of water in its liquid and vapour phases have been investigated more thoroughly than those of any other substance. They are of particular interest to engineers owing to the extensive use of steam as a working fluid in heat engines. Several international conferences have been held to correlate the results obtained in various countries and by various experimental techniques.* At the Sixth International Conference on the Properties of Steam (1963), agreement was reached on a set of values to each of which was attached a tolerance indicating the agreed margin of experimental error. These values comprise, the International Skeleton Tables 1963. (There have been only relatively minor revisions to these tables since.) The tolerances are well within the degree of accuracy required for any engineering calculations. The National Engineering Laboratory, Scotland, has used these values in computing the full set of NEL Steam Tables 1964 (Ref. 1), which employ sufficiently small intervals to make accurate interpolation a simple matter. For student use, an abridged set of steam tables is included in Thermodynamic and Transport Properties of Fluids (Ref. 17). The numbers appearing in subsequent examples are taken from these abridged tables and, where interpolation is necessary, linear interpolation is always used. It should be noted that several sources provide computer programs of properties for various fluids from which data can be extracted. These programs can be particularly useful in repetitive calculations such as Occur when optimising the design of process and power plant, or when evaluating experimental results. From a didactic point of view, it is important that a student familiarises himself with the handling of properties via tables and charts before plunging into the blackbox treatment provided by computers. 8.4 Diagrams of properties
The characteristics of a liquid and a vapour have already been described by referring to diagrams using p and v, or T and v, as coordinates. Diagrams with other pairs of properties as coordinates will be shown to be useful for various purposes in later chapters, and three such diagrams are described in this section, namely the T—s, h—s and p—h diagrams. Property charts do not entirely take the place of tables because values of the properties cannot be read from them with as great an accuracy as they are given in tables. 8.4.1 Temperature—entropy diagram
When analysing the characteristics of heat engine cycles it is often helpful to plot the cycle on a diagram having temperature and entropy as the coordinates. * An interesting account of this work may be found in Ref. 21.
150
[8.4]
Properties of Fluids Constant p lines
Fig. 8.12
T
Temperature—entropy diagrams
(a)
(b)
Fig. 8.12a illustrates this. If the processes in the cycle are reversible, the heat supplied during the cycle is given by 2 Q12 =
Tds
J
and the heat rejected by Q21
— f
Tds
2
These quantities are represented by the areas under the curves 12 and 21. It follows that the area enclosed by a reversible cycle represents the net heat supplied and hence, from the First Law, the net work done by the system on the surroundings. In its simplest form the T—s diagram consists of a series of constant pressure lines and the saturation curve. The general shape of the curves can be deduced from the general property relation (6.13): T ds = dh — v dp Noting that the v dp term is zero when p is constant, the equation reduces to dh
ds = —
T
From equation (8.4b) dh can be expressed in terms of c p as cp dT, and it follows that dT
ds = c P
T
We have been able to drop the partial notation of equation (8.4b), because we have no longer a second independent variable along the chosen path, namely a path at constant p. The value of c p can still be a function of T, but if we can assume it to be constant, or take a mean value over the temperature range TA to TB at the particular pressure p, we can find the approximate shape of the curve. Integrating the expression for ds between an arbitrary value TA and the saturation value TB ( TA < TB ) we obtain, for the shape of the constant pressure 151
Applications to Particular Fluids
[8.4]
curve in the liquid region (AB in Fig. 8.12b), s, — sA = cp f
° dT TB — = cp In — TA A T
As the enthalpy rise continues, the temperature remains constant at TB until the saturated vapour state C is reached. The enthalpy of vaporisation is equal to hfg, and hence the change of entropy sfg is equal to hig/TB. Thereafter the entropy increases in accordance with the equation ds = c
d P TT
where c p is for the superheated vapour. The constant pressure line therefore continues from C to D with much the same shape as in the liquid region but of steeper slope. The slope of a curve on the T—s diagram is d T/ds, which for a constant pressure line equals T/c p, and (cpl'yap < 1c 1 • . p,liq Since hfg falls with increase of pressure, the length BC decreases, and the family of constant pressure lines appears as in Fig. 8.12b. With water, the line representing a constant pressure of 0.006 112 bar cuts the temperature axis at 273.16 K, because this is the reference state at which the entropy is put equal to zero. Fig. 8.12b is out of proportion, because at any given temperature the change of entropy with pressure in the liquid region is in fact negligible. On any reasonable scale the constant pressure lines are so close together in the liquid region as to be indistinguishable, and for practical purposes they may be assumed to coincide with the saturated liquid line. Fig. 8.13 shows the T—s diagram for steam drawn to scale. In view of the fact that the dryness fraction is used as one of the parameters Fig. 8.13 Temperatureentropy diagram for steam
800.0
.0
750 N 700
.0 N
650 I): 600 :151 1.; 550 [.) 500 450 400 350 300 273.16 250
152
0
I I I I 2 3 4 5 6 7 8 9 Specific entropy/[kJ/kg K]
10
[8.4]
Properties of Fluids
defining the state of a wet vapour, it is useful to have lines of constant dryness fraction superimposed on the diagram. From equation (8.8) we have x = (s — sf )/sfg. Therefore points on the constant dryness fraction line of value x can be obtained by marking off, on each horizontal constant pressure line such as BC in Fig. 8.12b, a length equal to x(BC) from the saturated liquid end. The line of constant quality x is then found by joining up the points so obtained, as in Fig. 8.13. It is also useful to have a general idea of the shape of constant volume and constant enthalpy lines in the wet and superheat regions. In the superheat region a constant volume line will be of similar shape to a constant pressure line, because, using equation (6.12) and a similar argument to that used for the constant pressure path, we have for a constant volume path dT ds cp T Because c„ is always less than c, (see section 7.4.3 for a formal demonstration), at any given state the constant volume line is always steeper than the constant pressure line. In the wet region a constant volume line, of value v say, can be plotted in the following way. At any given temperature or pressure, of and vg can be found from the saturation table. Using the chosen value v, the corresponding value of the dryness fraction x can be found from equation (8.9). With x and either p or T known, it is possible to locate the point on the diagram. If this is repeated for other temperatures, the series of points representing states having the volume v can be joined to form a constant volume line. Such lines are found to be concave downwards in the wet region. Finally, the general shape of a constant enthalpy line has been indicated in Fig. 8.13. In the wet region it may be located by the method already described for a constant volume line, except that equation (8.7) is used instead of (8.9). In the superheat region, points of constant enthalpy can be located by finding the pressure, at various temperatures, which corresponds to the chosen value of h. This may be done by interpolation from the superheat table. The fact that the resulting curve tends towards the horizontal as the amount of superheat increases can be deduced from a knowledge of the behaviour of a perfect gas. The more a vapour is superheated the more closely does it behave like a perfect gas, and we shall show in section 8.5 that the enthalpy of a perfect gas is a function only of temperature. Thus if the enthalpy remains constant so must the temperature, and hence the tendency of the curve to flatten out at high degrees of superheat. It is worth noting the fact that as the pressure falls at constant enthalpy, a wet vapour eventually becomes drier and if it is not too wet originally it becomes superheated; section 10.3 describes how this fact may be used in the measurement of the dryness fraction of a wet vapour. 8.4.2 Enthalpy—entropy diagram
The diagram in which the enthalpy and entropy are used as coordinates is known as the Mollier diagram after its proposer. It is very useful when analysing the performance of adiabatic steadyflow processes, such as occur in nozzles, 153
Applications to Particular Fluids Fig. 8.14 Enthalpyentropy diagram for steam
4000
[8.4]
E Ki
3500
3000
Co 2500 c a . .13 2000
'"• 0
Critical point
ted vapour p line
1r . 0. 1500 20 bar .b.
1000
500
0
2
4 6 8 Specific entropy/[kJ/kg K]
10
diffusers, turbines and compressors, and a glance at equations (4.5) and (4.6) will show why. For example, the work done by a fluid flowing through a turbine is equal to the drop in enthalpy between inlet and outlet (assuming no change in kinetic energy). Consequently, if the thermodynamic state of the fluid at inlet and outlet can be located as points on the h—s diagram, the vertical distance between the two points is proportional to the work done. Adiabatic processes which are also reversible, i.e. isentropic processes, are represented by vertical lines on the diagram. The Mollier diagram is shown in Fig. 8.14. It may be seen to be a distorted form of the T—s diagram—distorted in such a way that the constant enthalpy lines become straight and horizontal. The constant pressure lines in the liquid region merge into the saturated line as before, and are straight in the wet region for the following reason. The increase of enthalpy from a saturated liquid state to any state of quality x at the same pressure is xhrg. Since this is equal to the heat added in a reversible constant pressure process, the increase of entropy is xh fg/T, where T is the saturation temperature corresponding to the given pressure. Thus the increase of entropy is directly proportional to the increase of enthalpy in the wet region, the slope of the constant pressure line (dh/ds)p being equal to T The slope of successive constant pressure lines increases, 154
Properties of Fluids
[8.4]
because the saturation temperature increases with pressure. In the superheat region, the slope at any state is also equal to the temperature T at that state, because the increase of entropy is given by ds = dh/T. There is therefore no discontinuity at the saturation vapour line; the constant pressure lines start with a slope determined by the saturation temperature and curve upwards as the temperature increases. Constant dryness fraction lines can be added by dividing each straight line in the wet region in the ratio x to (1 — x) as before, and they are shown by the dashed curves in Fig. 8.14. Constant temperature lines are usually added in the superheat region; in the wet region they coincide with the constant pressure lines. As already explained in connection with the T—s diagram, the enthalpy becomes more nearly dependent on temperature alone as the amount of superheat increases. It follows, therefore, that on the h—s diagram constant temperature lines must tend towards the horizontal as shown in the figure. It should be noted that lines of constant degrees of superheat are sometitnes used instead of lines of constant temperature, and that largescale charts for practical use only show the most useful part of the diagram, enclosed by the. dashed rectangle. The fact already mentioned, that a reduction of pressure at constant enthalpy eventually results in the drying and superheating of a wet vapour, is clearly seen on the h—s diagram because the process is represented by a horizontal line. 8.4.3 Pressure—enthalpy diagram
A diagram showing the properties of a fluid on a pressure—enthalpy basis is of somewhat limited use, but as we shall refer to it later when considering refrigeration problems it deserves a brief mention here. Since pressure is one of the coordinates of this diagram, the main family of curves comprises those of constant temperature. In the liquid region they are substantially vertical (see Fig. 8.15) because the effect of pressure on the enthalpy is negligible. They then run horizontally across the saturated vapour line since they are also lines of constant pressure in the wet region. In the superheat region they fall steeply Fig. 8.15 Pressure—enthalpy diagram
Constant T lines
Constant v lines
0
Constant s lines
Enthalpy
155
Applications to Particular Fluids
[8.5]
and approach the vertical for the same reason that they approach the horizontal on the enthalpy—entropy diagram. It is usual to add lines of constant volume in the wet and superheat regions, lines of constant dryness fraction in the wet region, and lines of constant entropy in the superheat region; these have the shape shown in Fig. 8.15.
8.5 Properties of a perfect gas At pressures and temperatures usually obtaining in engineering applications, many substances are to be found in a state lying to the right of curve MNf in Fig. 8.5. In this section we shall restrict our attention to two regions in this field: (a) the region of high temperature, where the temperature is in excess of twice the absolute critical temperature; and (b) the region of low pressure, where the pressure is one atmosphere or less. The socalled 'permanent' gases, oxygen, hydrogen, nitrogen etc., all lie in the first region at ordinary working temperatures (the critical temperatures of the specified gases being 154.8 K, 33.99 K and 126.2 K respectively). The water vapour in the atmosphere lies in the second region, and is in fact superheated steam at very low pressure. The behaviour of substances in these two regions of states approximates very closely to that of a hypothetical substance known as a perfect gas. The perfect gas is a particularly useful concept because the properties are related by very simple equations. As before, we shall start by considering the relation between the primary properties p, v and T
8.5.1 Equation of state of a perfect gas The relation between p, v and temperature was first investigated by Robert Boyle in England, and somewhat later by Edme Mariotte in France, in the middle of the seventeenth century. The conclusion reached at the time, called Boyle's law or the BoyleMariotte law, can be recast into the following form: when varying the, pressure and volume of a gas while keeping the temperature constant, the product (pv) remains constant. Therefore, if we plot products of (pv) against p for a sequence of rising temperatures, we should obtain a set of horizontal lines shown dashed in Fig. 8.16a. We now know that such ideal behaviour is not obeyed by real gases exactly, but we have to enter ranges of very high pressure or regions close to the critical pressure and temperature of the gas, before significant departures from Boyle's law can be observed. The lowest curve in Fig. 8.16a is a curve close to critical conditions. If the temperature used on the family of isothermal curves is the absolute thermodynamic one, we observe another important fact. When the (pv) intercepts R1 , R2, R3,... on the p = 0 ordinate are plotted against T, the relation is exactly linear; moreover, (pv),,=.0 tends to zero at T = 0. Therefore, if we plot pv/T against p, the intercepts collapse into a single point R as shown in Fig. 8.16b. 156
Properties of Fluids
[8.5]
Fig. 8.16
p—v—T data for gases
100 R5 R4 or)
450 T K  413
0.25 Ry 0.20
350
3
R2
T/[K] = 450 350 250
„ 0.15 250
50
i—t 0.10 2.1E
R,
Tclk_x(1 '"1
0.05
Saturation line 200 p/[bar] 100 (a)
100
200 p/[bar]
Mathematically this conclusion can be stated as* pu t T
R
It is clear from Fig. 8.16 that any equation relating p, v and T which will express the relation accurately will be complicated, particularly at high pressure and near critical conditions. Fortunately, for gases over a wide range of p and T, it is sufficiently accurate for most purposes to use the simple equation of state pv = RT
( 8.11 )
If this equation were valid for all pressures and temperatures, the results depicted in Fig. 8.16b would collapse on to the single dashed line. The hypothetical substance which obeys the equation of state in this way is called a perfect gas or an ideal gas. The lower the pressure and the higher the temperature, the more nearly does a real gas approximate to a perfect gas. This can be explained on the basis of a theory as to the microscopic structure of a gas (see section 8.6). The constant R is called the specific gas constant, or often simply the gas constant. If a mass m of gas is considered, the equation of state for a perfect gas becomes pV = mRT The product pV has the dimensions of energy, and in our system of units should be expressed in kJ. It is shown in equation (8.5) that when p is measured in bars (1 bar = 10 5 N/m 2 = 10 5 Pa) and V in m 2, pV must be multiplied by * The perceptive student will note a possible logical flaw in the argument. What is this flaw? The clue lies in the fact that we have assumed that the thermodynamic temperature T can be measured independently of the notion of a perfect gas. In fact, except at extremely low and very high temperatures, the gas thermometer provides the only practical means of measuring an absolute thermodynamic temperature. The circularity in the argument can be avoided by proving that a perfect gas temperature 0,, defined by pv = RBA is identical with the absolute thermodynamic temperature T, and this is done formally at the end of section 7.6.1.
157
[8.5]
Applications to Particular Fluids
105 / 103 = 100 to obtain a result in kJ. The units of R which we shall employ are kJ/kg K.
8.5.2 Amountofsubstance and the molar gas constant
Although the gas constant differs for different gases, the equation of state can be generalised to include all perfect gases by making use of an important law of chemistry. Before doing so, however, we must introduce another measure of a quantity of matter: it is the amountofsubstance, symbolised by n, and its unit is the mole.* This was defined in 1971 as one of the base units of the SI by the following statement: The mole is the amountofsubstance of a system which contains as many elementary entities as there are atoms in 0.012 kilogram of carbon 12. (When the mole is used, the elementary entities must be specified and may be atoms, molecules, ions, electrons, other particles, or specified groups of such particles.) In this book the entities will always be groups of identical atoms or molecules, or groups of specified mixtures of atoms and/or molecules (as with 'air'), as will be clear from the context. Furthermore, it will always be convenient to work in kilomoles, the unit symbol being kmol. The number of entities in 1 kmol of carbon 12, each of mass m( I2C), or by definition in 1 kmol of any other substance X having entities of mass m(X), is 12 kg kmol m( 12 c) The mass per kmol of any substance, called the molar mass fn", is therefore given by nt = N ion(X) =
12 kg m(12c) kmol 1 } m(X) —
(X) m(
kg
C) kmol
(The tilde ( ) will be used throughout this book to denote quantities per unit amountofsubstance, namely socalled molar quantities.) Several important points can be made as follows: (a)
(b)
(c) (d)
NA is the Avogadro constant which, according to the latest measurements, is equal to 6.022 137 x 1026 kmol t..,) will be recognised as the definition of relative The ratio m(X)/ii2m(12— atomic mass A, or relative molecular mass Mr , depending upon whether X is an atomic or a molecular species. ,12 m( 12 C) is the unit of measurement on the 'atomic The denominator — weight' scale. It is called the unified atomic mass unit and is symbolised by u. u is numerically equal to 1/NA , and hence 1 u = 1.660 565 5 x 10 27 kg.
* At present the authors may be alone in hyphenating the term 'amountofsubstance', but the reasons for doing so are discussed in Appendix A. It will be interesting to see if it becomes standard practice.
158
Properties of Fluids
[8.5)
(e) (f)
fil, when measured in kg/kmol (or g/mol), is numerically equal to A, or Mr but it is not dimensionless. It follows from (e) that the mass ni of an amountofsubstance n becomes nl = nfii
(8.12)
Equation (8.11) can now be applied to a molar mass nl, the volume of which is called the niolar volume 13, to yield (8.13a)
pu = fRT
The fundamental law of chemistry required to generalise this equation of state is known as Avogadro's law. To explain the empirical fact that gases combine in simple integral ratios of volumes, Avogadro (1811) suggested that equal volumes of all gases contain the same number of molecules, when the volumes are measured under the same conditions of temperature and pressure. His argument can be found in any elementary textbook on chemistry. It is not exact in practice but, as with the equation of state, the accuracy of the law improves as the pressure of the gas is reduced. Now since a molarmass in contains the same number of molecules whatever the gas (i.e. the Avogadro constant), fi must be the same for all gases at the same p and T It follows from equation (8.13a) that the product n1R must be the same for all gases. This product is known as the molar (or universal) gas constant, and it will be symbolised by R. Equation (8.11) can therefore be written in a form which applies to all perfect gases, and approximately to all real gases, as p13 =
(8.13b)
Or, if V is the volume of an amountofsubstance n, pV = nIZT Experiment shows that an average value for the volume of 1 kmol of the `permanent' gases is 22.4141 m 3 at standard atmospheric pressure (1 atm = 1.013 25 bar) and 0 °C. The value of 11 is thus found to be R—
pi3 T
—
100 x 1.013 25 x 22.4141
kJ
273.15
kmol K
= 8.3145
kJ kmol K
The gas constant for any particular gas can be obtained from 11 R=— ,For example, for oxygen 02 , R—
8.3145 kJ/kmol K 32 kg/kmol
— 0.260 kJ/kg K
8.5.3 Other property relations for a perfect gas
We have already noted in section 8.2.2 that a knowledge of the equation of state is not, by itself, sufficient to enable the other thermodynamic properties 159
Applications to Particular Fluids
[8.5]
to be determined. Some additional experimental data are necessary before u, or s can be expressed in terms of two of the measurable properties p, v and T It is possible to show that this is so for the perfect gas without difficulty. We have seen that the combination of the First and Second Laws gives rise to equation (6.12), i.e. 1 ds = — du + — dv T T This is a general relation between thermodynamic properties which must be satisfied by any substance. If we now apply this general equation to a perfect gas, the equation of state enables p to be eliminated to give ds
I R — du + — dv T v
(8.14)
The expression for enthalpy is obtained more simply. From the definition of enthalpy we have h = u + pv which for a perfect gas becomes h = u + RT
(8.15)
It is evident from (8.14) and (8.15) that we require an expression for u in terms of v and T; when this is known, u can be eliminated from each of these equations to give expressions for s and h in terms of T and v. It so happens that there is very simple expression for the internal energy of a perfect gas. First, we may note that the internal energy is a function only of temperature, i.e. u = u(T)
(8.16)
This can be shown to be a direct consequence of the equation of state of a perfect gas, but the proof is somewhat difficult and it has been dealt with at the beginning of section 7.6.1. Strictly, in view of that proof, experimental verification of equation (8.16) is superfluous, but it is worth while to record briefly the experiments of GayLussac followed up by Joule in the first half of the nineteenth century. The principle followed is illustrated in Fig. 8.17, which shows two vessels which may be put into communication with one another by opening a valve. One vessel contains the pressurised gas under investigation, and the other is evacuated. The temperature of the gas is measured both before opening the valve, and after allowing the gas to reach equilibrium having Fig. 8.17 The Joule experiment
160
Properties of Fluids
[8.5]
expanded freely into the evacuated vessel. If the vessels are perfectly insulated on the inside surfaces, we may conclude from the nonflow energy equation that the internal energies initially and finally are the same. The internal energy u is a function of two independent properties, e.g. u = u( T,, v) or u = u(T, p). Both p and v have changed in the expansion. If the temperature is found not to change, as was indeed observed by Joule, then it may be concluded that the internal energy must be a function of temperature only, as stated in equation (8.16); this conclusion is called Joule's law. The weakness of Joule's experiments was that he surrounded his vessels by a water bath to serve as a detector of any temperature changes. Even if he had insulated the vessels themselves, their heat capacity would have masked even significant changes of gas temperature and therefore departures from Joule's law. For reasons which will be discussed in section 8.6.1, a gas in the socalled `Joule free expansion' should display a small drop in temperature. If Joule's law is taken as valid, however, it follows that, in view of the equation of state pv = RT h = u + pv = u(T) + RT = h(T)
(8.17)
That is, the enthalpy also must be a function of temperature only. Subsequently, Joule and Thomson (Lord Kelvin) carried out steadyflow throttling experiments to verify this relation directly, and these did not suffer from the masking effects of heat capacity and defective insulation. The experiments, discussed in section 7.4.4, indeed revealed departures from the JouleThomson law h = h(T), and consequently from Joule's law u = u(T). The departures, however, were significant only in those regions of state in which departures from pv = RT were significant also. An important simplification follows from Joule's law, namely that a change of specific internal energy Au can be expressed as a product of a temperature rise AT and c,„ irrespective of whether the process is one at constant volume or not. From equation (8.4a), = ( au cv aT)„ However, we can drop the partial notation and the subscript v because for the perfect gas u is a function only of T Hence we obtain the result that cv =
du = f( T) dT
(8.18a)
It follows directly that du = cv dT
(8.18b)
and that the important simplification suggested above is indeed valid. A similar simplification for enthalpy is obtained from equations (8.4b) and (8.17), from which it follows that the general expression = (T ail ) T p 161
Applications to Particular Fluids
[8.5]
becomes for a perfect gas c P
(8.19a)
f(T)
dT
It follows again directly that (8.19b)
dh = cp d T
irrespective of whether the process is one at constant pressure or not.* That c p and cv are related by a very simple expression can be deduced as follows. From the definition of enthalpy, = u + pv, we can write dh = du + d(pv) which combined with equations (8.11), (8.18b) and (8.19b) becomes cp dT = cv dT + R dT
or (8.20)
cp — c = R
Equation (8.20) yields the important result that for any gas having the equation of state pv = R'T, although cv and c p may each be functions of temperature, their difference must always be constant and equal to the specific gas constant R. Furthermore, because R is a positive quantity, cp is always greater than cv.
We may now recall that at the beginning of this subsection we stated that a knowledge of the equation of state is not, by itself, sufficient for the calculation of the properties u, h or s. It should now be clear that the experimental data required for this purpose can be values of either c,, or cp as functions of T; they are alternatives in view of the relation (8.20). Although the variations of cv and c p with T are too large to be ignored completely, for many calculations it is sufficiently accurate to use a mean value over the temperature range of interest and treat it as a constant. Then, for example, equations (8.18) and (8.19) can be easily integrated to give u2 — u i = cv(T2 — T1 ) and h2 — hi = cp(T2 T1 )
(8.21)
These equations are relations between properties and are valid for any process undergone by a perfect gas for which cp and c p can be regarded as constant. In certain nonflow processes, each side of the respective equations is equal to * For the somewhat more advanced reader having some knowledge of partial differentials, the following way of looking at Joule's law, u = u(T); and the equivalent JouleThomson law, h = h(T), may be useful. Consider an infinitesimal process undergone by a real gas having two independent properties; then u = u(7; v) and h = h(T, p). It follows that
ah aT
dT + 814 ( ) du and dh = (—
dp r Joule's law implies that (au/MT = 0, and that (du/ 8T)„ can therefore be written as (du/dT), dropping the partial notation. The coefficient (du/dT) will be recognised as the specific heat capacity at constant volume, c„, introduced in section 8.2.2, but with the Joule's law constraint that c„ is a function only of T From the JouleThomson law, by a similar argument, we have c p = (dh/dT)=. f(T). du =
162
aT „
av
dT +
p
[8.5]
Properties of Fluids
the heat transferred. More explicitly, when W is zero in a constant volume nonflow process, Q = (u2 — u1 ) and therefore Qv = c„ (T2 — T1 ); and likewise for a reversible constant pressure nonflow process, Q = (h2 — h1 ) and therefore QP = cp( T2 — T1 ). The expressions for Qv and Q, are seen to be consistent with the primitive definitions of cv and c,, given in equation (8.3). Unless otherwise stated we shall always assume that it is sufficiently accurate to use mean values of ci, and c,,, and in effect we shall be considering a perfect gas to be defined as one obeying the two equations
pv = RT and cv (or c p) = constant
(8.22)
Furthermore, when taking a mean value of cv or c,, from tables over a temperature range T1 to T2 , we will adopt a simple approximate method as follows: mean c = c at mean T, where T = 4( T2 + 11) Another approximate method would be mean c = 1(c at T, + c at T2 ) These two mean values would only be equal, and identical with the true weighted mean value given by 2 1 true mean c — c dT T2 — T, 1. if c varied linearly with T Note that this expression for the true mean value is equivalent to the equally correct equations true mean c„ —
h 2 — hi and true mean c = P T2 — Tl
— U1 T2 —
U
To complete this section on the property relations of a perfect gas, we have to deduce expressions for the entropy in terms of any two of the measurable properties p, v and T From equations (8.14) and (8.18) we have
. R dT + — dv • T ll
ds = and hence
S2 — S I =
T2 In— + R Ti
V
v,
(8.23)
—UTTlike—tr— ie internal energy and enthalpy, the entropy is a function of both temperature and volume. The relations between the entropy and the other two combinations of primary properties, p and T or p and v, can easily be obtained as follows. From the equation of state, Pi vi = P2 u2 T2 163
[8.5]
Applications to Particular Fluids
Substituting for v2 /v1 in (8.23) we have T2 p, T, s2 — s, = ci In — + R ln Ti P2 Ti T2
R) In — Rln P2 — Ti Pi and using (8.20) this reduces to T2 P2 s2 — s, = cp In — — R ln — Ti Pi Similarly, by substituting for T2 / T, in (8.23) we get finally = (C„
(8.24)
v2 (8.25) ln P2 — + In — v, Pi It may be helpful if the charaCteristics of a perfect gas are summarised as follows: (a) The equation of state is pv = RT. (b) A consequence of (a) is that u = u(T). (c) From (b) and the definition of co it follows that c„ = 4(T) or is constant, and that du = co dT for any infinitesimal process. (d) From (b) and the definition of enthalpy it follows that h = h(T). (e) From (d) and the definition of cp it follows that dh = c p dT for any infinitesimal process, and that cp — co = R. (f) If a perfect gas is defined as also having constant specific heats, the following relations are valid irrespective of the process joining the end states 1 and 2: S2 — SI =
,Cp
u2 — u, = c„(T2 — h2 — h, = cp( — T2 S2 — Si = Cu ln —
T,
+ R In
T2 = C P In— —
T1
P2 P1
vi
R In P2 Pi v2 vi
= Cu ln — + cp ln — 8.5.4 Temperature—entropy diagram for a perfect gas A T—s diagram showing the properties of a perfect gas usually consists simply of a family of constant pressure lines, as in Fig. 8.18. It may be constructed in the following manner. First a reference state is chosen for which the entropy is considered to be zero, e.g. a state defined by (po, To). The increase of entropy from this state to any other state at po, but at some other temperature T, can be found from equation (8.24). Thus in general T, — P2 R In — s2 — s, = Ti P1 Cp
164
Properties of Fluids
[8.5] p> Po
Fig. 8.18 Temperature—entropy
Po
P < Po
diagram for a perfect gas
Constant p lines To
which in our case reduces to T s = c In — To
(8.26)
The value of s can be found for several values of T, and the points so obtained can be joined up to form the constant pressure line Po on Fig. 8.18. Now consider the isothermal compression process denoted by 12 on Fig. 8.18. The pressure increases from Po to p and, since T is constant, equation (8.24) reduces to s2 — s, = — R In — Po It is evident that (s2 — s1 ) is the same at any temperature. This suggests that any constant pressure line p can be found by stepping off horizontal distances from the line p„,, each equal to R ln(p/p0 ). In this way a series of constant pressure lines can be rapidly constructed. It should be noticed that although the horizontal distance between any two constant pressure lines is the same at any temperature, the vertical distance increases with increase of temperature. This is due to the curvature of the constant pressure lines, and is clearly indicated by the dashed lines in the figure. Constant volume lines could be added to the diagram, using equation (8.23). The general shape of the curves is the same except that they have a slightly steeper slope than the constant pressure lines at any given point. The slope of a constant pressure line can be found from the differential form of (8.26), i.e. ds =
c T
dT
and hence dT
T
ds
cP
165
Applications to Particular Fluids
[8.6]
Similarly the slope of a constant volume line is dT ds
T c„
Since c, < c p, the constant volume line must have the steeper slope. 8.6 Kinetic theory and the properties of real gases
Although thermodynamics is concerned solely with the behaviour of macroscopic systems, it is sometimes helpful to have in mind a mechanical model which exhibits the microscopic structure of the system. Such a model is particularly helpful when discussing the way in which real gases differ from a perfect gas. 8.6.1 Kinetic theory of gases
On the kinetic theory of gases, a gas is conceived as a large number of minute hard particles, i.e. molecules, moving about at random with very high velocities. The pressure and temperature, which are terms used to describe the observed macroscopic phenomena, can then be explained in terms of the microscopic behaviour of the molecules. Thus pressure is regarded as the average force per unit area on the walls of the container due to bombardment by the molecules, and the absolute temperature is regarded as being proportional to the mean of the squares of the velocities of the molecules, i.e. to their average kinetic energy of translation. Any problem concerning the behaviour of gases is thereby reduced to one of mechanics. The kinetic theory has been developed to the point where most of the observed phenomena can be explained and predicted with the use of classical mechanics.* At points where the theory apparently breaks down, the difficulties can be resolved by the use of quantum mechanics. The concept of a perfect gas can be shown to be a consequence of making the simplest assumptions about the molecules, and this part of the kinetic theory can be found in any elementary textbook on physics. The main assumptions are as follows: (a) The molecules are perfectly elastic and perfectly rigid, implying that no momentum or time is lost during collisions with the wall of the containing vessel. (b) The volume occupied by the molecules is negligible compared with the total volume. (c) The attractive forces between adjacent molecules are negligible. The first assumption seems reasonable because no loss of pressure is observed when a gas is kept in a closed vessel over a long period, and one can only conclude that no loss of momentum occurs as the result of a vast number of collisions with the wall. The second assumption seems reasonable because a gas can be so easily compressed, and the last because a gas readily expands to * For a clear account of the theory, see Ref. 14.
166
Properties of Fluids
[8.6]
fill any space into which it is introduced. With these assumptions and the ordinary laws of mechanics, the characteristics of a perfect gas can be predicted quite simply; for example, we can obtain the form of the equation of state, Joule's law and Avogadro's law. — If assumptions (b) and (c) are not strictly true, it is easy to see why real gases behave more like a perfect gas as the pressure is reduced and the temperature raised. At the lower pressures the molecules are on the average further apart, so that the volume occupied by the molecules is a smaller proportion of the total volume and the attractive forces are less. At the higher temperatures the molecules are moving past one another with higher velocities; they are near one another for a shorter period, and consequently the attractive forces have less effect. By making more realistic assumptions, the behaviour of real gases can also be predicted. For example, more accurate forins of the equation of state can be deduced by allowing for the volume occupied by the molecules and the attractive forces between them. The van der Waals equation provides a simple example, i.e. (p + ±1)(1)
b) = RT
Here R, a and b are constants which differ for different gases. The a/v2 term takes account of the attractive forces, while b takes care of the volume of the molecules. The departure from Joule's law is also easily explained by modifying assumptions (b) and (c). We know that the internal energy of a real gas depends slightly on a volume as well as on temperature, and that a slight drop of temperature must accompany a free expansion under adiabatic conditions. Let us see if this is to be expected of a van der Waals gas. An expression for the internal energy of a gas obeying the van der Waals equation of state is derived in Chapter 7 (equation (7.46)); in differential form it is a du = cv dT + — dv For an adiabatic free expansion the change in internal energy is zero, so that for this process we have a cv dT = — — dv v2 The constant a, indicating the forces of attraction between the molecules, is always positive for gases. Therefore, since dv is positive in an expansion, dT must be negative. The physical explanation becomes clear when it is remembered that the internal energy includes both the kinetic energy of the molecules and the potential energy due to the attractive forces (section 2.4). If the analogy of a stretched spring is borne in mind„it is evident that the potential energy is increased by the expansion because the molecules are further apart. Since the internal energy is unchanged, the kinetic energy of the molecules must have decreased, and this is reflected in a drop of temperature. 167
Applications to Particular Fluids Fig. 8.19 Variation of c, with temperature for nitrogen at ordinary pressures
[8.6]
1.0
w 0.9 ou
0.8
0.7
0
500
1000
1500
2000
Temperature/[K]
Before leaving the kinetic theory, it is worth noting the behaviour which it predicts for the specific heat capacities of perfect gases. According to this theory, co should be constant and equal to the increase in the total kinetic energy of the molecules per degree rise of temperature. The value predicted for c,, varies with the complexity of the molecules; for example, co is 3R/2 for a monatomic gas and 5R/2 for a diatomic gas. This difference is explained by the fact that monatomic gases possess translational kinetic energy only, whereas more complex molecules possess energy of rotation also, and all forms of energy are increased as the temperature is raised. For any given type of molecule, however, there is nothing in the simple kinetic theory to suggest why the increase in total energy per degree rise should be different at different temperatures. For helium, of molar mass 4 kg/kmol, co becomes (3/2)(8.3145/4) kJ/kg K = 3.118 kJ/kg K, and this prediction is in excellent agreement with observation at all temperatures. For nitrogen, a diatomic gas of molar mass 28 kg/kmol, co should be (5/2)(8.3145/28) kJ/kg K = 0.742 kJ/kg K, which agrees with observation over a wide range of temperature up to about 400 K (Fig. 8.19). Above this temperature, however, co gradually increases owinglo the fact that the molecules acquire vibrational energy as well as translational and rotational kinetic energy. This gradual rise cannot be predicted by the theory based on classical mechanics, although quantum theory does provide a satisfactory explanation. Quantum theory also suggests that at very low temperatures co for polyatomic gases should gradually drop to the value 3R/2 valid for monatomic gases, implying thereby that rotational motion of the molecules ceases at such temperatures. This has in fact been confirmed for hydrogen at 40 K, but for heavier molecules this is expected to happen much closer to absolute zero and experimental evidence is lacking. Finally, it is worth noting the physical meaning which the concept of entropy acquires when a model based on the microscopic structure of the system is considered. We have seen that any irreversibility results in an increase in the entropy of an adiabatic system; this is the important 'principle of increasing entropy'. On the microscopic view, an irreversibility is always associated with an increase in the disorderly motion of the molecules. For example, during an adiabatic expansion of a gas, internal viscous friction will result in a reduction in work done by the gas because the internal energy, i.e. random molecular 168
Properties of Fluids
[8.6]
energy, is higher in the final state than it would otherwise have been. Similarly, in an adiabatic expansion through a nozzle, viscous effects convert directional kinetic energy of a stream, which is fully available for doing work on say a turbine blade, into such random energy. Or again, two gases when mixed represent a higher degree of disorder than when they are separated, and we shall see in section 14.3 that there is an increase in entropy involved in an irreversible mixing process. In all natural processes irreversibilities are present, and there is a tendency to proceed towards a state of greater disorder. It is possible to establish a quantitative measure of disorder—in terms of a particular definition of the concept of probability—and then to derive a relation between entropy and this concept of probability. We are then led to a statistical interpretation of the Second Law and to a branch of the subject known as statistical thermodynamics. 8.6.2 Properties of real gases
Accurate equations of state are inconvenient for everyday calculations because they lead to unwieldy expressions. They are mostly used for the preparation of tables and diagrams of properties. When tables are not available, and for conditions where the perfect gas laws are too inaccurate, correction factors may be applied to the perfect gas relations. Thus the equation of state, for example, can be written as pv = ZRT
(8.27)
where Z is the compressibility factor. The value of this factor depends upon the gas, and it is also a function of the pressure and temperature. The combination of Z = (1)(p, T) and equation (8.27) is the complete equation of state. Charts have been prepared for the more common gases, showing Z plotted against pressure for various temperatures. Fig. 8.20 shows the compressibility chart for nitrogen. The advantages of plotting Z = (1)(p, T) directly, are that (a) a much smaller range of values is required and (b) it shows at once how far the gas deviates from a perfect gas. The disadvantage is that, when v is one of the known parameters of state, a method of successive approximation is required to obtain the unknown property. For example, when v and T are given, p must be found from the perfect gas equation and a first approximation to Z obtained Fig. 8.20 Compressibility factor for nitrogen
2.2 Pc =
k 1.8
34 bar
= 126 K
'1,
3201(
0.6
200 200 400 600 800
Pressure/[bar]
169
Applications to Particular Fluids
[8.6]
from the chart. Using this value of Z, a new value of p can be calculated from (8.27), a better approximation to Z obtained from the chart, and so on. It so happens that the shape of the curves in the region to the right of the critical isothermal Te in Fig. 8.5 is much the same for all gases, although the scales are different. This suggests that the scales might be brought into line if the properties were quoted as fractions of the critical values, i.e. as PR =
P
T
VR =
vc
Pc
pR , vR and TR are referred to as the reduced properties. If the experimental pR —vR — TR data for all gases were found to lie on the same set of curves, we could conclude that any two gases at the same p, and TR have the same value of vR. This statement is known as the law of corresponding states. It can be expressed by saying that there is a functional relation vR = (I)( PR
TR)
which holds for all gases. It can be shown as follows that, if the law of corresponding states were true, it would be possible to compile a single set of curves expressing the variation of Z/ZC with pR and TR which would hold for all gases. Thus since
pv pc vc pR vR pR VR RT RTC TR T_ R then if vR = (I)(pR, TR) with 4:p the same for all gases, Z/Z, must be a unique function of PR and TR . Unfortunately such a set of curves could not yield the necessary result that Z —> 1 as PR —> 0 for all gases, because it is an experimental fact that Z,, differs .for different gases. This is simply a way of saying that the law of corresponding states is not true. Although too inaccurate to be used in this way, a modified form of the law is sometimes useful. The modified form asserts that Z = f(pR , TR ), with the function f the same for all gases. The generalised compressibility chart of Fig. 8.21 expresses the function f. Note that the chart implies that Z. = 0.22 for 1.2 compressibility 1.0 Er
0.8
1: 0.6 II
N 0.4 0.2 0
170
1
2
3
4 5 6 Reduced pressure pR
7
8
9
10
[8.6]
Properties of Fluids
all gases, which is not the case, but at least it expresses the fact that Z —> 1 when pR —> 0. Furthermore its use only involves a knowledge of pc and To and not of vc which in general is not known accurately. (Critical data can be found from any tables of physical constants; see Ref. 33, for example.) Values of Z taken from the chart may deviate by as much as 10 per cent from the experimental value for a particular gas, but the chart is useful when very little experimental data are available for a substance, and also for showing when the assumption of perfect behaviour (Z = 1) is no longer sufficiently accurate for a given purpose. Its use suffers from the disadvantage previously mentioned in relation to Fig. 8.20, that when v is one of the known parameters of state, successive approximation is necessary to determine the unknown property. We have briefly indicated the method of dealing with the properties of real gases by referring to the p—v—T relation as an example. We cannot here go into the equivalent method for determining values of the other thermodynamic properties. This whole topic is of particular concern to chemical engineers;and a much fuller treatment can be found in textbooks on chemical engineering thermodynamics.* At the beginning of section 8.5 we suggested that a gas can be treated as perfect when the temperature is more than twice the critical temperature, or the pressure is one atmosphere or less. Fig. 8.21 shows the latter criterion to be valid at all temperatures, since for most gases a pressure of one atmosphere corresponds to a reduced pressure of under 0.1. The first of these rough guides ( TR > 2) is apparently not valid for all pressures. and ceases to be true for a reduced pressure greater than about 5. For most gases, however, this corresponds to a much higher pressure than is generally encountered in engineering applications, e.g. the corresponding pressure for nitrogen is 170 bar. For our purposes we shall always be in a position to assume that a gas has the characteristic equation pv = RT. The second part of the definition of a perfect gas—that the specific heat capacities are constant—is not nearly such a good approximation. The slight variation of the specific heats with pressure can usually be neglected; indeed, in view of the decision to use the perfect gas equation of state, the specific heats must be treated as pure functions of temperature if we wish to be consistent (see section 8.5.2). Fig. 8.19 shows the variation of cc with temperature for nitrogen. The corresponding curve for c,, can easily be obtained by using the relation (8.20) between the specific heats and the gas constant. If the approximate procedure of using a mean specific heat is not sufficiently accurate, some form of equation can be. used such as c = a + bT + cT 2 where a, b and c are constants. The change of enthalpy, for example, can, then be obtained analytically as T2
h2 — h, = f (a + bT + cT 2)dT T1
* See Ref. 4, Chapter 4, and also Ref. 15.
171
[8.6]
Applications to Particular Fluids
Although air is strictly speaking a mixture of gases, its composition is sufficiently invariable for it to be treated as a single gas. Tables of properties of air which take account of the variation of cp are available (Refs 12 and 9). The tables of Keenan and Kaye cover the range for which the p—v—T data can be accurately represented by the perfect gas equation of state, so that the tables of internal energy and. enthalpy require only one independent parameter— namely temperature. The internal energy and enthalpy are arbitrarily put equal to zero for all states at absolute zero of temperature. The entropy of a perfect gas, however, has been shown to be a function of two independent properties. To avoid complicating the table by introducing a second independent parameter, the entropy is not given directly for all states, but a new variable 4 is tabulated in its place. The differential form of equation (8.24) is R ds = 1dT — — dp When the reference state is chosen at absolute zero and some pressure po, the entropy at any state defined by (p1 ,T1 ) is given by c
Si
dp —
dT — R
= I
Jo T
Po P
Ti
=
Pi .2 dT— Rln0 T Po
The change of entropy between any two states 1 and 2 is therefore given by Ti S2 — Si = f
o T
Ti c
— f o T
— R ln P2 Pi
Finally, if we write T
dT
40 =
o T the change of entropy becomes P2 S2 — Si = 40 2 — — R In —
(8.28)
Pt The variable 4 is a function of temperature only and may therefore be tabulated in the same way as the internal energy and enthalpy. Equation (8.28) is used when the change of entropy between two states is required. We shall not make use of such tables in subsequent chapters; for our purpose it will be sufficiently accurate to use a mean c p.
172
9 NonFlow Processes
Nonflow processes have been classified and analysed in general terms in Chapter 3. The processes were characterised by (a) the volume, pressure or temperature remaining constant; (b) the heat transfer being zero; or (c) the pressure and volume varying in such a way that pvn is constant. Most nonflow processes of practical interest approximate to one, or a succession, of these processes. In this chapter we shall apply the analysis to closed systems consisting of particular fluids. Each process will be dealt with assuming the fluid to be (a) a vapour and ( b) a perfect gas with constant specific heat capacities. Tables of properties must be used in the first case, but in the second the analysis can be carried out using algebraic relations. Steam is used as an example of a vapour, and we shall make use of the abridged tables of Ref. 17. Air is considered as an example of a perfect gas, and the following values will be used for cp and R: cp = 1.005 kJ /kg K,
R= 0.287 kJ /kg K
It follows from equation (8.20) that cv = 0.718 kJ/kg K For a summary of the relations between the properties of a perfect gas, which are valid for any process whether reversible or irreversible, the reader is referred to the end of section 8.5.3.
9.1 Constant volume process
If there is no paddle work, the energy equation for unit mass of any fluid undergoing a constant volume process is Q =u2  U 1 When the fluid is a perfect gas this becomes Q = cr (T2 — T1 ) For a perfect gas we also have the following relations between properties which 173
[9.1]
Applications to Particular Fluids
are valid for any two states of the same volume. From the equation of state, P P2 Ti T2 and from the definition of entropy, S
r 2 do T2 = 2 dT = c„ ln — —s1 = ( 1 T 1 T rev
The latter equation can also be obtained by putting u2 = u, in the general expression for the entropy change, equation (8.23). Example 9.1
A fluid in a closed vessel of fixed volume 0.14 m 3, exerts a pressure of 10 bar at 250 °C. If the vessel is cooled so that the pressure falls to 3.5 bar, determine the final temperature, heat transfer and change of entropy.
(a) Steam (Fig. 9.1a) The first step is to find the mass of fluid in the system. Since T1 is greater than the saturation temperature corresponding to pi , the vapour is initially superheated. Using the superheat table we find v1 = 0.2328 m 3 /kg. Since V = 0.14 m 3, nt—
V v1
=
0.14 _ 0.6014 kg 0.2328
The vapour must be wet in its final state because mug is 0.6014 x 0.5241 0.3152 m 3, which is greater than 0.14 m 3. The temperature must therefore be the saturation temperature corresponding to 192 , i.e. t2 = 138.9 °C. The dryness fraction can be found from equation (8.10), i.e. x2 =
V
0.14
niug2
0.3152
=0.444
NB: If the accurate equation (8.9) is used, x2 because 0.443. From the superheat table: u1 = 2711 kJ/kg From the saturation table: = uf2 + x2 ufg2 = 584 + 0.444(2549 — 584) = 1457 kJ/kg
10 bar
Fig. 9.1a
P
1 3.5 bar
174
NonFlow Prc
[9.2]
Fig. 9.1 b
T
3.5 bar
Heat transfer: Q = m(u2 — u 1 ) = 0.6014(1457 — 2711) = —754 kJ
From the superheat table s, = 6.926 kJ/kg K, and from the saturation to s2 = s12 + x2 sf,2 = 1.727 + (0.444 x 5.214) = 4.042 kJ/kg K Change of entropy: S2 — S1 = M(S2 — Si ) = 0.6014(4.042 — 6.926) = — 1.734 kJ/E (b) Air (Fig. 9.1b) Mass of gas: p1 V
100 x 10 x 0.14
RT,
0.287(250 + 273)
m ——
= 0.933 kg
Final temperature: T2 =
P2
T, =
Pt
.5 523 = 183 K L 10
Heat transfer: Q = mcp(T2 —
= 0.933 x 0.718(183 — 523) = —228 kJ
Change of entropy: S2 —
S1
183 = MCv In T2 = 0.933 x 0.7181n = —0.703 kJ/K T1 523
9.2 Constant pressure process
For a reversible constant pressure process undergone by unit mass of any fluid 2 W = —p f du= —p(v 2 — u 1 ) Q = (u 2 — u 1 ) — W = (u2 — u1 ) + p(v2 — v,)= h 2 — h i
When the fluid is a perfect gas, W = —R(T2 — Q=cp(T2 — T1)
1
[9.2]
Applications to Particular Fluids
For a perfect gas we also have the following relations between properties which are valid for any two states of the same pressure: V1
V2
T,
T2 12
2
d
—)
S2 — S1 =
T
T2 dT = c ln — P rev =f 1 T TI
The latter equation can also be obtained by putting p2 = expression for the entropy change, equation (8.24). Example 9.2
p, in the general
A mass of 0.2 kg of fluid, initially at a temperature of 165°C, expands reversibly at a constant pressure of 7 bar until the volume is doubled. Find the final temperature, work and heat transfers in two cases: (a) when the fluid is steam with an initial dryness fraction of 0.7, (b) when the fluid is air.
(a) Steam (Fig. 9.2a) Initial specific volume: v, = x, vg, = 0.7 x 0.2728 = 0.191 m3/kg Final specific volume: v2 = 2v1 = 0.382 m 3 /kg
Since v2 > vg2 , the vapour must be superheated in its final state. From the superheat table by interpolation, the final temperature is = 300 + T2
0.382 — 0.3714 0.4058 — 0.3714
50 = 315°C
Work transfer: W=
— mp(1)2 — v1 ) = —0.2 x 100 x 7(0.382 — 0.191) = —26.7 kJ
From the saturation table: h, = hi, + x 1 hrg l
= 697 + (0.7 x 2067) = 2144 kJ/kg
From the superheat table, by interpolation: 15
h 2 = 3060 + — (3164 — 3060) = 3091 kJ/kg
50
Fig. 9.2a
p
176
7 bar
NonFlow Processes
[9.3]
Fig. 9.2b
7 bar
T
Heat transfer:
Q = m(h2 — 110 = 0.2(3091 — 2144) = 189 kJ (b) Air (Fig. 9.2b) Initial volume: 1/ =
mRT,
0.2 x 0.287 x 438
Pi
100 x 7
— 0.035 92 m3
Final volume: V2 = 2 = 0.071 84 m' Final temperature: V2 T2 = 17 1
= 876 K
Work transfer: W = —p(V2 — V1 ) = —100 x 7 x 0.035 92 = —25.1 kJ Heat transfer:
Q = mc p(T2 —
= 0.2 x 1.005 x 438 = 88.0 kJ
9.3 Polytropic process
When a polytropic process is reversible, the work transfer is given by equation (3.12), i.e. W—
(P2v2 — Pi vi)
(9.1)
n— 1
Therefore, from the energy equation,
Q = ( u2 — u 1 )
(132v2 — Pi vi)
n— 1
When the fluid is a perfect gas, these expressions can be written as
W=
R n—1
(T2 —
T1)
Q = cv (T2 — Ti) n 1 (T2 TO = (c,
n
R 1 )(T2 —
Ti)
177
[9.3]
Applications to Particular Fluids
Since p1 v; = p2 vS and pv = RT, we also have the following relations between properties which are valid whether the process is reversible or irreversible: T2 = (P2 )(n "/" pi Ti
(9.2)
T2 ( V2 )1 " —=—
(9.3)
T1
v,
The change of entropy is best found from first principles as in the following example. Example 9.3
A mass of 0.9 kg of fluid, initially at a pressure of 15 bar and a temperature of 250°C, expands reversibly and polytropically to 1.5 bar. Find the final temperature, work and heat transfers, and change of entropy, if the index of expansion is 1.25.
(a) Steam (Fig. 9.3a) From the superheat table: v, = 0.152 m 3 /kg Final specific volume: n 1 /n '1)
= 0.1520 x 101 /1.25 = 0.959 m 3/kg
P2 Vg2 is 1.159 m 3 /kg so that the vapour is wet in the final state, and the temperature is the saturation value corresponding to 1.5 bar, i.e. T2 = 111.4 °C.
'Dryness fraction: x2 =
'
v2 V g2
=
0.959 1.159
— 0.827
Work transfer: m W = n — 1 (P2v2 — Pivi) 100 x 0.9 0.25
{(1.5 x 0.959) — (15 x 0.152)) = —303 kJ
Fig. 9.3a
T
15 bar
1.5 bar
9 4 V
178
[9.3]
NonFlow Processes
From the superheat table: u 1 = 2697 kJ/kg From the saturation table: 14 2 = u f2 + X2 Ufg2 = 467 + 0.827(2519 — 467) = 2164 kJ/kg Heat transfer: Q = m(u2 — u 1 )— W = 0.9(2164 — 2697) + 303 = —177 kJ si = 6.711 kJ/kg K s2 = s12 + x2s,g2 = 1.434 + (0.827 x 5.789) = 6.222 kJ/kg K Change of entropy: S2 — Si = M(S2 Si )= 0.9(6.222 — 6.711) = — 0.440 kJ/K (b) Air (Fig. 9.3b) Final temperature: p
0.25/1.25
)(n — 1)/n
T2 = T,
= 523 (— 10
Pi
= 330 K
Work transfer: W— mR (T2 T„) = n—I
0.9 x 0.287 (330 — 523) = — 199 kJ 0.25
Heat transfer: Q = mcv( T2 — T1 ) — W = {0.9 x 0.718(330 — 523)} +199 = 74.3 kJ Change of entropy, from first principles: 1 R dQ) P e ds = ( — = — du + — du = dT + — du (for perfect gas) T T r„ T T s2 — s, = cv in= + R In T 1
= cv In
T2 T1
v2 v,
R n—1
Fig. 9.3b
T2 In — (using (9.3))
T
T1
15 bar 1.5 bar
.25 = const. 250 °C 2
T2
179
[9.4]
Applications to Particular Fluids
R
=( cv
in
n—1
T2
T1
0.287 )
S2 — Si = 0.9(0.718
0.5 2
In
330 523
= 0.178 kJ/K
9.4 Adiabatic process
For a fluid undergoing an adiabatic process the energy equation per unit mass reduces to W= (u2 — u 1 ) When the fluid is a perfect gas, W = co( T2 — For a perfect gas undergoing a reversible adiabatic (i.e. isentropic) process, we can deduce the following relations between properties: 0 = cv dT + p du (First Law)
R dT = p du + u dp (equation of state) Eliminating dT from these two equations, we obtain cv 0 = (1 + 1)p dv + — v dp
=
dv + cu t) dp (since R = c p — c p)
Writing c p/cv = y, this reduces to du dp
y—+—=U p and on integration, y In u + In p = constant
pvY = constant
(9.4)
Since we also have pv/T = constant, we can eliminate v and p in turn to give
Tp(1')/' = constant
or
T2 = (P2
= constant or
T2
T1
(9.5)
Pi
Ti
=
( V2 )17
—
v1
(9.6)
It is evident from (9.4) that, for a perfect gas, the reversible adiabatic process is a special case of the reversible polytropic process, and (9.5) and (9.6) can be obtained by putting n = y in (9.2) and (9.3). y is called the index of isentropic expansion or compression. As in the case of the specific heat capacities, for real gases y varies with temperature and pressure (mainly with the former), but a 180
NonFlow Processes
[9.4]
mean value can be used for most purposes. If we put n = y in the expression for the work transfer in a polytropic process, we have W= R (T2 — T1 ) y — 1 This can easily be shown to be identical with the expression already derived, as follows: (T2 TO — —
c— c
cp /c,— 1
(T2 — Ti ) = cv (T2 —
In a reversible adiabatic process s2 = s1, and equation (9.4) could have been obtained by putting this result in the general expression (8.25). If this is done we have 2 cp 11111
ln
vl
P2 Pi
and hence P2
(v1 v2
)7
Pi Since the process is reversible, the foregoing relation applies to any pair of states between the end states, and consequently throughout the process pv• = constant Example 9.4
Assuming the process in Example 9.3 is isentropic (instead of polytropic with index 1.25), find the final temperature and the work done.
(a) Steam (Fig. 9.4a) To find the final state we make use of the fact that s2 = s1 , and from the superheat table, s1 = 6.711 kJ/kg K. Since s1 = s2 < sg2, the vapour must be wet in the final state, and therefore T2 = 111.4°C (i.e. Ts at p2 ). From S1 = S2 = Sf2
X2 Sfg2
we have x2 =
Fig. 9.4a
P
.92 — sf2
6.711 — 1.434
Sf g 2
5.789
T
= 0.912
15 bar 1.5 bar
2 S 181
Applications to Particular Fluids
Fig. 9.4b
[9.4]
T
15 bar 1.5 bar
From the superheat table: u, = 2697 kJ/kg From the saturation table: U2 = Uf 2 + X2 Ufg2 = 467 + (0.912 x 2052) = 2338 kJ/kg
Work transfer: W = m(u2 — u 1 ) = 0.9(2338 — 2697) = —323 kJ (b) Air (Fig. 9.4b) For air, c 1.005 = P— 1.40 c 0.718 Final temperature: T = T1 P2 )(Y1"7 = 523(1 Y /3.5 = 271 K 10 P1 Work transfer: W = mcv( T2 —
= 0.9 x 0.718(271 — 523)
—163 kJ
For a vapour, there is no simple and unique relation between p and v which applies to every isentropic expansion and compression. Nevertheless it is sometimes convenient to assume an approximate relation of the polytropic form pvn = constant; n then becomes the index of isentropic expansion or compression, although it is not necessarily equal to the ratio c p/cv. Indeed, if part of the process occurs in the wet region, where c p = co, this ratio has no meaning. The value of n can be found, as in the following example, by substituting the values of p and v at the end states in the expression pi v"i = p2 v1 There is no unique value for n; it varies with the end states. As a rough approximation, however, the following average values of n may be used for steam: n = 1.035 + 0.1x when 0.7 < x < 1.0, where x is the initial dryness fraction; this is known as the Zeuner's equation n = 1.135 when most of the process occurs in the wet region 182
NonFlow Processes
[9.4]
with the steam initially saturated or slightly superheated when the process occurs mostly in the superheat region
n = 1.30
Example 9.5
Steam, initially dry saturated, expands isentropically from a pressure of 15 bar to 0.1 5 bar. Find the index of isentropic expansion.
We have (Fig. 9.5) s, = s, = sgl
=
6.445 kJ/kg K
s2 — s12 6.445 — 0.755 = 0.784 x2 =
7.254
Sfg2
iii
v, = vg1 = 0.1317 m 3 /kg 1)2 = X2 Vg2 =
0.784 x 10.06 = 7.887 m3/kg
If we can write p i 11. = p2 vn2 , then 15 x 0.1317" = 0.15 x 7.887" from which n = 1.125. Fig. 9.5
T
15 bar
This approximate method of treating the isentropic expansion or compression of a vapour as polytropic will be found useful in Chapter 18. Although it must be remembered that the isentropic process is only strictly polytropic when the fluid is a perfect gas with constant specific heats, when the vapour is steam and superheated throughout the process the approximation is very close to actual behaviour, as is indicated by the following. It has been found that over a wide field in the superheat region the u—p—v data are related by the simple equation 1 u —B=n—
1
(9.7)
p(v — C)
where the empirical constants n, B and C are n = 1.3,
B = 1943 kJ/kg,
C = — 0.000 175 m3 /kg
This equation was originally proposed by H. L. Callendar. By inspection of the superheat table it can be seen that, at pressures below 100 bar, C is always less 183
[9.5]
Applications to Particular Fluids
than 1 per cent of v. For many engineering purposes C can be ignored, and thus
u—B—
1 n—1
pv
(9.8)
From equation (9.8) it is possible to deduce rigorously* that the following set of relations must hold for an isentropic process:
pv"
= constant,
Tv1"1) = constant,
pi
Tngn — 1) =
pv / T
constant
(9.9)
= constant
n is the constant having the value 1.3, and in this context is the index of isentropic expansion or compression. The last equation in (9.9) does not imply that the perfect gas equation is applicable, because it only applies to an isentropic process and the constant pv/ T is different for different isentropic processes (i.e. it depends on the value of s). Finally we may note that since h = u + pv, equation (9.8) can be written h—B—
n—1
(9.10)
pv
It follows that for superheated steam any change in enthalpy is given very closely by n h2
=
n
—
1 (P2v2 — P 1)
And for an isentropic process, for which we have seen that p2 v1 = p, vq, this becomes
h2 — =
n
n—1
n
(n— 1)/n
p v {( 1 )
—1
P1 n )(n — 1)/n
= (hi —
—1
B){(
(9.11)
Pi Relations (9.9) and (9.11) are particularly useful when dealing with supersaturated states, discussed in section 18.2, which are not covered by steam tables.
9.5 Isothermal process
For unit mass of any fluid undergoing a reversible isothermal process,
Q = T(s2 — s1 ) and hence from the energy equation, W = (u2 — u1 ) — Q = (u2 — 141 )— T(s 2 — s1 ) When the fluid is a perfect gas (for which u is a function only of temperature), * This is a useful exercise for students who have studied Chapter 7; the main equations required are (7.13), (7.14), (7.23) and (7.24).
184
NonFlow Processes
[9.5]
u2 = u1 and it follows from the energy equation that
Q = w Making use of the equation of state, we can find W from p dv if the process is reversible. Thus for a reversible isothermal process undergone by a perfect gas, 2 2 dv Q= —W=j p dv = RT f — = RT1n — v2 v, 1 1v
(9.12)
For a perfect gas we also have the following relations between properties which are valid for any two states of the same temperature: P1 V1
= P2 V2
1 2 f (dDrev S2 — SI = —
T ,
=
R In — v2 (from equation (9.12)) v,
The latter equation can also be obtained by putting T2 = T1 in the general expression for the entropy change. Since my, = p2v2, equation (9.12) can be written alternatively as (9.13)
Q=—W= Pi
and hence also s2 — Si = —R In
P2 Pi
It is evident that for a perfect gas the reversible isothermal process is another special case of a reversible polytropic process, i.e. one for which n = 1. Note that we cannot put n = 1 in equation (9.1) to obtain the work transfer—the reason being that the integral of dv/v" is In v when n = 1. Example 9.6
A fluid, initially at 155.5°C and 1 bar, is compressed reversibly and isothermally to a state where the specific volume is 0.28 m3 /kg. Find the change of internal energy, change of entropy, and heat and work transfers, per kg of fluid. (a) Steam (Fig. 9.6a) From the superheat table, by interpolation: 5.5 u, = 2583 + — 76 = 2591 kJ/kg 50 Since v, = 0.28 m 3 /kg is less than the specific volume of saturated vapour at 155.5°C, the vapour must be wet in its final state. Hence x, =
v2 Vg2
=
0.28 0.3427
—0.817
u2 = u12 + x2 urg2 = 655 + (0.817 x 1910) = 2215 kJ/kg 185
[9.5]
Applications to Particular Fluids Fig. 9.6a
Change of internal energy: u2 — u1 = 2215 — 2591 = —376 kJ/kg From the superheat table, by interpolation:
.5
s1 = 7.614 + L 0.220 = 7.638 kJ/kg K 50 Also: s2 = s12 + x2 s1g2 = 1.897 + (0.817 x 4.893) = 5.895 kJ/kg K Change of entropy: s2 — s1 = 5.895 — 7.638 = —1.743 kJ/kg K Heat transfer: ' Q = T(s2 — si ) = 428.5( — 1.743) = —747 kJ/kg Work transfer: W = (u2 — u1 ) — Q = —376 + 747 = 371 kJ/kg (b) Air (Fig. 9.6b) Change of internal energy is zero. Initial specific volume: vi =
RT
—
Pi
0.287 x 428.5 = 1.230 m 3 /kg 100x 1.0
Change of entropy: 0.28 V2 s2 — si = R In — = 0.2871n— = —0.425 kJ/kg K v1 1.23 Fig. 9.6b
T
p
T2 = T,
1 bar
NonFlow Processes
[9.6] •
Heat transfer: Q = T(s2 — s1 ) = 428.5( — 0.425) = —182 kJ/kg I
Work transfer: W = —Q = 182 kJ/kg
9.6 Irreversibility and the free expansion
We noted in section 5.4.1 that most practical nonflow processes can be assumed reversible. Nevertheless it is worth reviewing our position when the processes we have considered are irreversible: (a)
(b)
Constant volume, constant pressure, polytropic and isothermal processes: when these are irreversible we must know either W or Q in addition to the end states before the unknown can be determined. Adiabatic process: when this is irreversible the work transfer can be predicted if the end states are known, but when it is reversible only one property in the final state need be known. The adiabatic process differs from the others in that only one property in the final state can be varied independently; the final state then depends upon the amount of irreversibility present.
To illustrate the principle of increasing entropy, we shall consider as a final example the Joule free expansion for a perfect gas (see section 8.5.3). In this case both Q and W are zero and the entropy of the gas must increase because the process is irreversible and adiabatic. Example 9.7
Air, initially at a pressure and temperature of 3.5 bar and 15 °C, is enclosed in a vessel 0.06 m3 in volume. The air is allowed to expand into an evacuated vessel also 0.06 m3 in volume. If the process is adiabatic, find the change in entropy of the air.
The mass of air in the system (Fig. 9.7) is given by in =
NV, RT1
=
100 x 3.5 x 0.06 0.287 x 288
— 0.254 kg
From the energy equation, since W = Q = 0, u2 — u 1 = 0. If air can be treated as a perfect gas, T2  T1 = 0. also. To find the change of entropy;
T
Fig. 9.7
V
V, =0.06 m3 0.12 m3
S
187
[9.6]
Applications to Particular Fluids
either we can use the general expression (8.23), or, if we wish to work directly from the equation defining entropy, ds = (d0/ T1rev, ' we can adopt the following procedure. The irreversible process can be 'replaced' by any suitable reversible path which joins the two given states defined by ( V, = 0.06 m3, T, = 288 K) and ( V2 = 0.12 m 3, T2 = 288 K) and for which Q can be easily calculated. The obvious choice is a reversible isothermal path; then using equation (9.12) we have V2
S2  SI =  12 (daev =
T
tt;
R ln — vi
Since v2 /v, = V2 / = 2, we get finally S2  Si =
188
mR In
oz vi
= 0.254 x 0.2871n 2 = 0.0505 kJ/K
10 Flow Processes
In Chapter 4 it was shown how the heat and work crossing the boundary during a steadyflow process can be related to the properties of the fluid at the inlet and outlet of an open system. This relation, the steadyflow energy equation (4.2), was applied to some important open systems but without reference to any particular fluid. As in Chapter 9, we shall again consider the fluid to be either steam or air and illustrate the applications with numerical examples. As pointed out in section 5.4.1, the irreversibility due to viscous friction cannot be neglected unless the velocity of flow is very small. In many cases it is necessary to calculate the unknown quantity assuming the process to be reversible, and multiply the result by a process efficiency. Various process efficiencies are introduced in the following examples. A second artifice for dealing with irreversibility in adiabatic steadyflow processes is also mentioned: this involves treating the process as a polytropic process. Finally, this chapter ends with the consideration of multistreani processes and nonsteadyflow processes.
10.1 Boiler and condenser
Since the work done in a boiler or condenser is zero, the steadyflow energy equation reduces to = rh{(h 2 — h i ) + 1(C3 — CO} The velocity of flow in the inlet and outlet pipes is small, and, as the following example will show, the change in kinetic energy can be neglected. The velocity in the boiler or condenser itself is even smaller, so that the effect of friction can be neglected and the process can be regarded as internally reversible. This implies that there is no pressure drop due to friction, and the pressure can be assumed constant throughout the system. In the following example of a steam boiler plant, it is assumed that before the steam leaves the system it is passed through a separate bank of tubes, the superheater, situated in the stream of furnace gases. Fig. 4.4 shows a boiler without a superheater. 189
(10.2]
Applications to Particular Fluids
Example 10.1
1 500 kg of steam is to be produced per hour at a pressure of 30 bar with 100 K of superheat. The feed water is supplied to the boiler at a temperature of 40 °C. Find the rate at which heat must be supplied, assuming typical values for the velocity at inlet and outlet: 2 m/s in the feed pipe and 45 m/s in the steam main. In Section 8.3.3 we agreed to assume that the enthalpy of a compressed liquid is equal to the enthalpy of saturated liquid at the same temperature. Therefore, from the saturation table at 40°C, h, = 167.5 kJ/kg. The saturation temperature at 30 bar is 233.8°C, and the outlet temperature is therefore 333.8°C. From the superheat table, by interpolation,
h, = 2995 +
33.8 50
122 = 3077.5 kJ/kg
The rate of heat transfer required is Q = 1;1{(h2 — hi) +
— Ci)}
1500 [ kg] 1 (3077.5 — 167.5)[ id] 36001_ s kg + 1(452 — 22)
2
[ 1 kg rn 2 Nmi 1 r kJ 1
kg s2 or kg 103 I_Nrn
kJ = (1212.5 + 0.42)[— ] = 1213 kW It is easy to see that the change of kinetic energy of 0.42 kW can be neglected.
10.2 Adiabatic steadyflow processes
For the reasons given in sections 4.2.2 and 4.2.3, the processes in a nozzle, diffuser, turbine and rotary compressor can be assumed adiabatic. The energy equation for the nozzle or diffuser, where W = 0, becomes 4(Ci —
= (11 1 — 112 )
And for the turbine or rotary compressor, when the velocity at inlet is approximately the same as that at outlet, the energy equation reduces to 14/ = rii(h 2 — h 1 )
The state of the fluid is usually known at the inlet of these systems, but only one property, e.g. the pressure, can be arbitrarily fixed at the outlet. To fix the final thermodynamic state of the fluid, and hence determine h 2 , it is necessary to assume the process to be reversible; the flow is then isentropic and we can use the fact that s2 = s,. This has been explained in section 6.6, and the subsequent examples should make the point clear. When the fluid is a perfect gas, the foregoing special forms of the energy 190
Flow Processes
[10.2]
equation become: 1(Ci — CD= c p(T, — T2 )
Nozzle and diffuser: Turbine and rotary compressor:
14/ = riic p( T2 —
Also, from equation (8.24) we have, for a perfect gas, S2 — Si =
Cp
In T2 — R In P2 Ti Pi
This equation relates the difference in entropy between states 1 and 2 to the pressure and temperature of the gas at these states. The fact that the gas is flowing during any process has no effect on relations between its thermodynamic properties, and the equation can therefore be applied to the thermodynamic states of a perfect gas at the inlet and outlet of an open system. For any isentropic steadyflow process (s2 — s1 ) is zero, and we shall arrive at the same relation between p and T that we deduced for the isentropic nonflow process, i.e. equation (9.5): T2 Ti
(P2 )(Y 1)/Y PI/I
This, together with pi v,/T,= p2 v2/T2, yields T2
v2 1  r
T1
v,
Plvi = p2 02 and — = —
Thus the relations between the thermodynamic properties of a perfect gas in its initial and final states are the same for both isentropic steadyflow and isentropic nonflow processes. Since the velocity of flow is very high in a nozzle, diffuser, turbine or rotary compressor, the effect of friction cannot be neglected. Nevertheless the laws of thermodynamics do not enable quantitative predictions to be made for irreversible processes. One method of accounting for the effect of viscous friction is to calculate the unknown quantity assuming the process to be reversible and then to multiply the result by a process efficiency to obtain a more realistic estimate. The value of the process efficiency must be determined from tests carried out on a similar system. For nozzles it is usual to define the efficiency in terms of the outlet kinetic energy as nozzle efficiency 1N —
(C2 )2
(10.1)
C2 is the actual outlet velocity, while C'2 is the outlet velocity which would have been achieved had the final pressure been reached isentropically. A prime will always be used to denote the result obtained by assuming the process to be isentropic. Diffusers are designed to obtain the maximum possible pressure rise at the expense of a given reduction in velocity, and the process efficiency is often 191
[10.2]
Applications to Particular Fluids
defined by diffuser efficiency tip =
P2
 Pi
(10.2)
PZ — Pi
Here p2 is the actual outlet pressure, p'2 is the pressure which would result from an isentropic process leading to the same outlet velocity. Note that process efficiencies are always defined in such a way that they are positive numbers less than unity. This explains the different ways of defining process efficiencies for turbines and rotary compressors, namely (10.3)
w 141 and rIc = — = T
When the fluid can be treated as a perfect gas, and the change in kinetic energy between inlet and outlet can be ignored, these become T2 T, —
and

C
11
T2

T,
The way in which process efficiencies are used will be illustrated in the following examples. Apart from the fact that these efficiencies are always defined in such a way that they are numerically less than unity, their definitions are quite arbitrary; they should be regarded merely as empirical correction factors. Since all the foregoing process efficiencies are defined by comparing the actual process with an isentropic process, they may be called isentropic efficiencies. Example 10.2
A fluid expands from 3 bar to 1 bar in a nozzle. The initial velocity is 90 m/s, the initial temperature 150°C, and from experiments on similar nozzles it has been found that the isentropic efficiency is likely to be 0.95. Estimate the final velocity.
(a) Steam (Fig. 10.1a) From the superheat table, h, = 2762 kJ/kg,
s'2 = s, = 7.078 kJ/kg K
Since s'2 < sg2 , the vapour must be wet on leaving the nozzle after a reversible
Fig. 10.1a
192
Flow Processes
[10.2]
Fig. 10.1b
expansion. Hence x
s'2 — s f2
7.078 — 1.303
Sig2
6.056
— 0.954
h2 = hf2 + x'2 11f,2 = 417 + (0.954 x 2258) = 2571 kJ/kg From the energy equation, (c2)2 /[m 2 /s2 ] 902 — (2762 — 2571)
2 x 103
(C'2 )2 = 0.390 x 106 m 2 /s2 C2 = t1si(C2)2 = 0.95 x 0.390 x 106 m 2 /s 2 C2 = 609 m/s (b) Air (Fig. 10.1b)
After a reversible expansion the final temperature would be n T2 = T1 (5
(y 
PI Assuming Y = 1.40, we have 0.4/1.4
T2 = 423( 3
= 309 K
From the energy equation, (C2 )2 /[m 2 /s2 ] — 902 2 x 103
— 1.005(423 — 309)
(C2 )2 = 0.237 x 106 m 2 /s2 CZ = 0.95 x 0.237 x 106 m 2 /s 2 C2 = 475 m/s Example 10.3
A fluid enters a turbine at the rate of 14 kg/s with an initial pressure and temperature of 3 bar and 150 °C. If the final pressure is 1 bar and the isentropic efficiency of the turbine is 0.85, find the power developed and the change of entropy between inlet and outlet. pi , Ti and p2 are the same as in the previous example, and Figs 10.1 a and b, which show changes in the thermodynamic properties only, also apply to this case. 193
[10.2]
Applications to Particular Fluids
(a) Steam Using the results of Example 10.2, we have hi = 2762 kJ/kg,
x' = 0.954,
h'2 = 2580 kJ/kg
From the energy equation, W' = ?NW, — h,) = 14 x ( —182) = —2548 kJ/s or kW W
= 0.85 x ( —2548) = —2170 kW
To find the change of entropy we must first determine the actual final state, i.e. state 2: hi — 112 = th(h i — h'2) = 0.85 x 182 = 154.7 kJ/kg h2 = 2762 — 154.7 = 2607 kJ/kg x2
h2 — hf2 2607 — 417 — 0.970 h182 2258
s2 = sf2 + x2Sfg2 = 1.303 + (0.970 x 6.056) = 7.177 kJ/kg K Since s2 = 7.078 kJ/kg K, the change of entropy is S2 — gi
= rh(s2 — s1 ) = 14 x 0.099 = 1.39 kJ/s K
(b) Air From Example 10.2b, T2 = 309 K. The actual work transfer is given by W = nithc p( T'2 —
= 0.85 x 14 x 1.005(309 — 423) = —1363 kW
The actual final temperature can be found from T, —
T2 = T2 =
—
T2)
423 — (0.85 x 114) = 326 K
The values of pi , Ti , p2 and T2 can be substituted in the appropriate general expression (8.24) for the change of entropy. Alternatively, we can replace the irreversible path 12 in Fig. 10.1b by a reversible path consisting of the isentropic process 12' and the reversible constant pressure process 2'2. We then have S2 —
S1 = g2 — g2 — (— d° 2'
'
7
rev
thc ln T2 P T2
326 = 14 x 1.0051n 309=0.753 kW/K It is worth mentioning one other method of accounting for irreversibility in an adiabatic flow process. The actual thermodynamic path of all these adiabatic processes may be regarded as being approximately polytropic in form, i.e. we may assume that pv" = constant 194
Flow Processes
[10.3]
The polytropic expression can only have a meaning if p and v are regarded as average values at any point in the process because, although we normally assume that every elemental mass of fluid has the same properties at inlet and outlet of an open system, not all elements necessarily pass through exactly the same series of states between inlet and outlet. The value of the index of an irreversible adiabatic expansion or compression is not equal to y even when the fluid is a perfect gas; n is an empirical constant depending on the amount of friction. If n is known from previous experiments on a similar system, an unknown final state can then be predicted by making use of the equation Pivi = P2 vi Or, when the fluid is a gas, we can also use T2 Ti
(V 2 y  WI P1
Once the final state has been determined, the energy equation, which applies to both reversible and irreversible processes, can then be used in the usual way.
10.3 Throttling process
The throttling process is an adiabatic steadyflow process, but it was not included in the previous section because this was concerned with adiabatic processes which ideally should be isentropic. The throttling process is essentially irreversible: it is a means of reducing the pressure of a fluid by intentionally introducing friction into the flow. In section 4.2.4 we noted that the throttling process was such that h, = h, When the fluid is a perfect gas, it follows that Ti = T2 The fact that a slight change of temperature is observed when the fluid is a real gas has been noted in section 7.4.4, and it indicates that the enthalpy of a real gas is not a function only of temperature. When a gas or vapour is throttled, the specific volume downstream of the restriction is greater than it is upstream, i.e. v2 > v1 . If the restriction is in a pipe of uniform diameter, the continuity equation (4.3) implies that C2 > C1 . Nevertheless, the following example shows that for ordinary flow velocities the kinetic energy terms in the energy equation are negligible and for practical purposes h, = Example 10.4
Air flows at the rate of 2.3 kg/s in a 15 cm diameter pipe. It has a pressure of 7 bar and a temperature of 95°C before it is throttled by a valve to 3.5 bar. Find the velocity of the air downstream of the restriction, 195
[10.3]
Applications to Particular Fluids
Fig. 10.2
7 bar 3.5 bar
and show that the enthalpy is essentially the same before and after the throttling process. Also find the change of entropy. Fig. 10.2 illustrates the process. The temperature actually falls as the fluid velocity increases through the restriction, and then rises because most of this increase in kinetic energy is dissipated by friction. The initial specific volume is v, =
RT,
—
0.287 x 368 100 x 7
P
— 0.151 m 3 /kg
and the initial velocity, from the continuity equation, is C, =
?nu, A
=
2.3 x 0.151 x 4 n(0.15)2
— 19.65 m/s
Similarly, the final velocity is C2 =
m R T2
2.3
A p2
0.287
r m i T2
(n/4)(0.15)2 100 x 3.51_ s [K]
= 0.1067
[
T2 s [K]
Since Q and W are zero, the energy equation for a perfect gas reduces to — c p 7' + c p 72 2 + 1C2 2— 1 1C2 21 or 1.005
T2 1(0.1067)2 TZ T, 1(19.65)2 — 1.005 + + [K] 103 [K 2 ] [K] 103
and hence T, T, " + 5.66 x 10 6 — + 0.192 [K] [K 2 ] [K] Without further calculation it is evident that the kinetic energy terms can be ignored and T2 is effectively equal to T1 . Hence the final velocity is C2 = 0.1067 x 368 = 39.3 m/s Since the process is adiabatic and irreversible, the fluid must undergo an increase of entropy as it flows through the system. The initial and final thermodynamic states could be joined by a reversible nonflow isothermal process, and hence s2 — s, = — S, = 196
2
(dQ ) = T rev — Si ) =
35 R In PZ = —0.2871n . = 0.199 kJ/kg K 7 Pi x 0.199 = 0.458 kJ/s K
Flow Processes
[10.4] Fig. 10.3 Throttling calorimeter
Sampling tube
Before leaving the throttling process, we may note how use is made of it in the throttling calorimeter for the determination of the dryness fraction of a wet vapour. Normally the state of a fluid is most conveniently determined by measuring the intensive properties p and T, but for a wet vapour these are not independent properties. The throttling calorimeter, illustrated in Fig. 10.3, enables a wet state 1 to be determined by measuring p and T alone. A steady stream of wet vapour is sampled from the main flow and passed through a small orifice in a welllagged chamber. The vapour pressure, initially pl , falls to some value p2 as a result of the throttling process. Since h2 = h1, it is evident from the h—s diagram (Fig. 8.14) that if the pressure drop is sufficient and the vapour not too wet, the sampled vapour will be superheated after the expansion. The thermodynamic state can therefore be determined by measuring the independent properties p2 and T2. The enthalpy h2 can then be found from the superheat table. If the initial pressure pi is also measured, and the corresponding values of h f and /ifs are taken from the saturation table, the dryness fraction is found from xi =
h, — h fi h fgi
h2 — hf1 h fgl
The process must of course be continued long enough for the calorimeter to reach a steady temperature before readings are taken. The chief difficulty is in ensuring that the sample is representative of the main flow: unfortunately the liquid accumulates on the wall of the pipe, and the sample tends to be drier than the main stream as a whole. 10.4 Reversible steadyflow process
An expression for the work transfer in a reversible steadyflow process, whether adiabatic or not, which is equivalent to the expression d W = —p dv that applies to a nonflow process, can often be very useful. This will be particularly apparent in Chapter 16. We will develop the basic equation here, however, because we shall want to use a special version of it in Chapter 11 to 197
[10.5]
Applications to Particular Fluids
calculate the work required to compress a liquid passing through a boiler feed pump. We will assume that the change in kinetic energy is negligible, so that the steadyflow energy equation reduces to 2
W = til(hi  hi)  =
dh —
For a reversible process, 2
=
Tds
th
and from the re ation between properties, equation (6.13), 2
11
2
Tds = f (dh — vdp) i
The equation for W then becomes 2
W =rim
1 .
2
dh — rh f (dh — v dp) = iit
vdp
(10.4)
Equation (10.4) applies to adiabatic or nonadiabatic processes, provided that they are reversible and that changes in kinetic energy are negligible. To evaluate W we need to know the relation between v and p along the path 12. For example, if the reversible process is adiabatic and the fluid is a perfect gas, pvY = constant. If the fluid is a liquid which can be assumed incompressible, v = constant and (' 2
141 = rim
dp = 1111)( 02 — Pi)
(10.5)
This is the special case which we shall need to use in Chapter 11.
10.5 Isothermal steadyflow process
It was pointed out in section 4.2.5 that a reciprocating compressor (or expander) can be regarded as an open system undergoing a steadyflow process, provided that a receiver is included between the cylinder and the measuring section to damp out the pulsations. The fluid flows through a reciprocating machine at a comparatively slow rate and there is time for an appreciable amount of heat to be exchanged with the surroundings. It is possible to imagine a limiting case in which the temperature of the fluid remains constant throughout its passage through the system. This is the case considered here. Since we have postulated low velocities, the energy equation reduces to +
= th(h2 — h i )
When the fluid is a perfect gas, (h2 — h1 ) is zero because the enthalpy is a function only of temperature. For the isothermal expansion or compression of 198
Flow Processes
[10.5]
a perfect gas we therefore have =—w If the process is assumed reversible, these equations can be evaluated to find the work done when the states of the fluid are known at inlet and outlet. Thus, when the fluid is a vapour, (h2 — h1 ) and (s2 — s1) can be found from tables of properties and, since the temperature T is constant, Q can be calculated from thT(s2 — s1 ). Hence W can be found from the energy equation. When the fluid is a perfect gas, a simple expression for W can be deduced in terms of the temperature T and the inlet and outlet pressures Pi and p2. Thus putting T = constant in (8.24), s, — s 1 = — R In P2 PI and hence W = —Q = thRTin i Pi •
(10.6)
Equation (10.6) is in fact the same expression that was obtained for the work transfer when a perfect gas undergoes a reversible nonflow isothermal process (section 9.5). The same equality of work does not hold when the fluid is a vapour because in a nonflow process Q + W = th(u2 — u1 ) Only when the fluid is a perfect gas are the flow and nonflow isothermal work transfers the same, because only then does (u2 — u1 ) = (h2 — h1 ), both being zero. Owing to the comparatively low fluid velocities, the effect of fluid friction in a reciprocating machine is small. Hence the question of introducing a process efficiency to take account of irreversibility in this type of process has not arisen in practice. There remain the questions of how to predict the work transfer when the heat exchanged is not sufficient to maintain the temperature constant, and how mechanical friction is taken into account. These matters will be dealt with in Chapter 16. Example 10.5
Recalculate the work and heat transfers per unit mass for Example 9.6, assuming that the isothermal compression occurs in a steadyflow process.
The thermodynamic states before, during and after compression are identical with those of the nonflow process of Example 9.6. The processes for steam and air are therefore depicted respectively by Figs 9.6a and b, and some of the required property values can be taken from that example. (a) Steam The heat transferred is the same as for the nonflow process, i.e. Q = T(s2 — s1 ) = —747 kJ/kg. From the energy equation the work done is W = (h, — hi ) — Q 199
Applications to Particular Fluids
[10.61
From the superheat table, by interpolation, 5.5 h, = 2777 + — 99 = 2788 kJ/kg 50 x2 has been found to be 0.817, and thus h2 = hf + x2 hfa = 417 + (0.817 x 2258) = 2262 kJ/kg Hence W = (2262 — 2788) + 747 = 221 kJ/kg (b) Air The heat transferred is the same as for the nonflow process, i.e. Q = — 182 kJ/kg. Also, since (h2 — h1 ) = (u2 — u1 ), both being zero, the magnitudes of the work and heat transfers are equal as for the nonflow process. 10.6 Multistream steadyflow processes
Reference to section 4.1 will show that, provided the streams do not react chemically with one another, there is nothing inherent in the derivation of the steadyflow energy equation (4.2) to prevent its application to an open system in which more than one stream of fluid enters and leaves the system. The enthalpy, kinetic energy and potential energy terms associated with each stream can be summed at the inlet and outlet respectively, to give the following equation: + 14/ =
E th(h + iC 2 + gz) — E rit ( h + iC 2 + gz) in
out
Also, for conservation of mass we have the equation rh = out
in
One simple example of a multistream system is given here, but other more important cases can be found in Chapter 14. Example 10.6
Steam is to be condensed by direct injection of cold water. The steam enters the condenser at a rate of 450 kg / h with a dryness fraction 0.9 and a pressure 1 atm. The estimated heat loss from the condenser to the surroundings is 8500 kJ /h. If the cold water enters with a temperature of 15 °C, and the mixture of condensate and cooling water is to leave at 95 °C, determine the rate of flow of cooling water required. Fig. 10.4 illustrates the system. The energy equation, neglecting the kinetic and potential energy terms, becomes = rh3 h3 —
+ rh2 h2 )
and for conservation of mass, rh3 = 200
+ rh2
Flow Processes
[10.7]
Fig. 10.4
2
Cold water
From the saturation'table, 11, = 11„ + x, hrg, = 419.1 + (0.9 x 2256.7) = 2450 kJ/kg /12 = 62.9 kJ/kg,
11, = 398.0 kJ/kg
Therefore —8500 = (450 + M2 )398 — {(450 x 2450) + M2 62.91 = 2730 kg/h 10.7 Nonsteadyflow processes The only nonsteadyflow processes we shall consider are those undergone by the fluid in an open system as it changes from one equilibrium state to another. The appropriate energy equation has been derived in section 4.3, namely equation (4.9). If we neglect the potential energy terms, as we have done with the steadyflow processes, the equation becomes Q + 14/ = (m"u" +
+ E8m 2 (h 2 +10 — E8m i (h, +1CD
Q and W refer to the quantities of heat and work crossing the boundary of the open system during the time it takes for the system to change from one equilibrium state to another. The term (m"u" — m't4') refers to the change of internal energy of the system between these two equilibrium states, and the remaining two terms refer to the summation of the quantities of enthalpy and kinetic energy leaving and entering the system with each element of fluid. We shall now apply this equation to two particular cases. 10.7.1 Filling a reservoir from an infinite source of fluid Fig. 10.5 illustrates the system. An air bottle of volume V contains air at pressure p' and temperature T'. It is to be filled from a compressed air line maintained at a constant pressure p, and temperature T,. We require to find the mass and temperature of the air in the bottle after the valve has been opened to allow the pressure in the bottle to rise to the supply pressure p,. 201
[10.7]
Applications to Particular Fluids Fig. 10.5 Filling a compressed air bottle
We may assume that when the valve is opened the air enters the bottle so rapidly that the process is adiabatic. If we draw the boundary in such a way that the entrance to the open system is in the main supply line, the thermodynamic properties of the fluid at station 1 are constant throughout the process, and C 1 is negligible. The velocity will be high in the locality of the valve—but local transformations of energy within the open system do not concern us. Also, no fluid leaves the system, and W is zero. The energy equation therefore reduces to (m"u" — m'u') = h i E6m, Since mass is conserved, (in" — m') = E8m, and hence (m"u" — m'u') = li,(m" — in')
(10.7)
In our example the fluid is air, which can be treated as a perfect gas. Consequently (10.7) can be written as c„(m"T" — m' T') = c p Ti (m" — m') Moreover, we also have m"
p" V / RT" p"/T"
m'
p' V / RT'
p'/T'
and
p" = pi
Substituting these in the energy equation, we get c,
(p,IT" Pi /7
p,/ T" 1) T" —T ')= cpT,( p'/T' j
Since p', T', pi and T1 are given, this equation can be used to find T". Having found T" we can find m" from , pi t/ m' = RT" Note that in the foregoing treatment we have assumed the internal energy to be zero at absolute zero. The reference state chosen can be important for the following reason. By rewriting equation (10.7) explicitly in terms of an internal energy ur relative to the internal energy tic, at some arbitrary reference state 0, 202
Flow Processes
[10.7]
we have in"(u'' +u0 )—m'(u'+u0 ) = h 1 (m" — m')
and hence, since h 1 = h„ + h0 = 'Z r! + u0 + po t)°, we get (in" tic —
+ no1m" —
=
+ Po vo )(in" — in') + no1n1" — in')
Although the terms involving u0 cancel, there remains the po vo term which arises because the enthalpy and internal energy cannot normally both be zero at the same reference state. The exception is when the fluid is a perfect gas and the reference temperature is absolute zero, because then po vo = R To = 0. In the following numerical example which deals with steam, the Po vo term is not zero but can be neglected because it is equal to only 0.000 611 2 kJ/kg in the reference state used in the tables, namely saturated liquid at the triple point. Example 10.7
A vessel of volume 0.085 m3 contains steam at 1 bar and 0.8 dryness fraction. The vessel is momentarily connected to a steam main in which the steam is at 20 bar and 260 °C. If the pressure in the vessel is allowed to rise to the main pressure, estimate the final state and mass of the steam in the vessel.
Making the appropriate assumptions, the energy equation (10.7) can be used, i.e. (m"u" — mitt') = Min" — m') From the superheat table, by interpolation, 10 50
h, = 2904 + ( x 121) = 2928 kJ/kg
From the saturation table, u' = 417 + (0.8 x 2089) = 2088 kJ/kg in' —
V x'i/g
0.085 = 0.0627 kg 0.8 x 1.694
„ V 0.085[m 3] in — — v" v" Substituting these values in the energy equation we get ( 0.085 [rn3] u" v"
= 2928
— 0.0627[kg] x 2088 [
kJ y 0.085[m3] [kg v
kJ D kg
0.0627[kg] )
or 2928 620 [kJ/m 3] v"/[m3 /kg] u"/v"
1
The final pressure p" is 20 bar, but no exact algebraic relation between 203
[10.7]
Applications to Particular Fluids Fig. 10.6
103 x 24 {2928 [m3 /kg]/v" — 620} 22
20
18 250
350 400 300 Temperaturb/[° C]
450
u", v" and p" is known. A graphical method can be used to solve the equation as follows: 20 bar and °C 400 300 350 v"/[m3 /kg] 0.1255 0.1386 0.1511 u"/[kJ/kg] 2 744 2 861 2 946 (u"/v")/[kJ/m3] 19 500 21 900 20 600 {2928 [m 3 /kg]/v" — 620} 22 700 20 500 18 800 By plotting the last two lines of figures against temperature as in Fig. 10.6, it is found that the steam has a temperature of 343 °C in the final state. That the final temperature in the vessel is higher than the temperature in the steam main is due to the fact that the steam is recompressed adiabatically in the vessel after being throttled. The final mass of steam in the vessel can now be found. At 20 bar and 343 °C, by interpolation from the superheat table, 43 v" = 0.1255 + — 0.0131 = 0.1368 m 3 /kg 50 Hence „ V 0.085 — 0.621 kg m = v" 0.1368
NB: If the approximate relation between p, v and u given by equation (9.7) is used, v" = 0.135 m 3 /kg and m" = 0.63 kg. 10.7.2 Maximum work attainable by allowing a reservoir of fluid to discharge via a turbine
This example has already been introduced in general terms in section 4.3, and Fig. 4.10 illustrates the system. By making suitable assumptions, the energy equation was shown to reduce to —W = (m'u' — m"u") — Eom,h, The maximum work will be obtained when the expansion through the turbine is reversible. Since we are assuming the process to be adiabatic, the additional assumption of reversibility implies that the process is isentropic. In the following numerical example we shall consider the fluid to be air. 204
Flow Processes
[10.7]
Example 10.8
A tank of volume 0.3 m3 is filled with air at a pressure and temperature of 35 bar and 40 °C. The air is allowed to discharge through a turbine into the atmosphere, until the pressure in the tank has fallen to the atmospheric level of 1 bar. Find the maximum amount of work that could be delivered by the turbine. The air in the tank progressively decreases in pressure and temperature
from p' and T' to p" and T". But since the pressure p2 at the outlet is constant, i.e. atmospheric, and the expansion is isentropic, the temperature T2 at the outlet must also remain constant during the process. This can be made clear by the following argument. Consider the mass of air which remains in the tank at the end of the expansion and treat it as a closed system. This mass, originally occupying only a fraction of the volume of the tank, expands isentropically during the process. If at any instant the pressure and temperature is p and T, then we have T T'
)(Y  IVY P (
10'
But p and T must also represent the pressure and temperature of the air as it enters the turbine at this particular instant, and since the expansion through the turbine is also isentropic,
T2 T
( P2)(Y 1)1' p
Multiplying this pair of equations we get T2 T'
( P2 p
1
T' and p' are the given initial conditions in the tank, and p2 is constant, i.e. atmospheric pressure. Therefore T2 must be constant also. Moreover, since p" = p 2, the final temperature of the air in the tank must be equal to From the conservation of mass, and the fact that T2 is constant, the energy equation becomes —W = c,(m' T' — m" T") — c p T2(m' — m") where 2
tn' =
p' V RT' p" V RT"
=
—
0.4/1.4
(Y 1 )/Y
p
T" = T2 = T'(—
= 313 (
100 x 35 x 0.3 0.287 x 313 100 x 1 x 0.3 0.287 x 113
35
= 113K
— 11.68 kg
— 0.925 kg
Hence W = —0.7181(11.68 x 313) — (0.925 x 113)1 + 11.005 x 113(11.68 — 0.925)1 = —1330 kJ 205
11 Vapour Power Cycles
One common method of producing mechanical power employs the transfer of heat from a reservoir to a working fluid which is taken through a thermodynamic cycle. The cycles considered in this chapter have two characteristics in common: (a) the working fluid is a condensable vapour which is in the liquid phase during part of the cycle, and (b) the cycle consists of a succession of steadyflow processes, with each process carried out in a separate component specially designed for the purpose. Each component constitutes an open system, and all the components are connected in series so that, as the fluid circulates through the power plant, each fluid element passes through a cycle of mechanical and thermodynamic states (see section 4.4). To simplify the analysis, we shall assume that the change in kinetic and potential energy of the fluid between entry and exit of each component is negligible compared with the change of enthalpy. Also, when evaluating the work and heat transfers during the various processes in a cycle, it will normally be convenient to consider the steadyflow energy equation per unit mass rather than for a rate of flow th as was done in equation (4.2). The energy equation for our present purpose therefore becomes 0+W = h2 — We shall also assume, in the main, that the processes are reversible. Cycles composed of reversible processes are called ideal cycles. After a discussion of suitable criteria for comparing their effectiveness, various ideal cycles are analysed in turn. The Carnot cycle is considered first, and the Rankine cycle is then presented as a logical modification of this to meet certain practical considerations. Finally, other modifications used in modern power plant are described. Although the working fluid usually employed is steam, because it is cheap and chemically stable, the principles presented here apply equally to any condensable vapour. The characteristics of an ideal working fluid are discussed, and a possible power plant where steam would be quite unsuitable is described. The chapter ends with a section on economic assessment. This is to remind the student that, although this book is almost solely concerned with
206
Vapour Power Cycles
[11.1 ]
technical matters, one should never forget that economic factors usually determine which of alternative technical solutions are adopted in practice.
11.1 Criteria for the comparison of cycles
The choice of power plant for a given purpose is determined largely by considerations of operating cost and capital cost. The former is primarily a function of the overall efficiency of the plant, while the latter depends mainly on its size and complexity. In general the efficiency can always be improved by adding to the complexity of the plant, so that a suitable compromise between low operating and low capital costs must be reached. Consider first the efficiency of the plant. Fig. 11.1 illustrates essential features of the type of power plant considered here. Until the 1950s the hightemperature reservoir had always been a stream of hot gases produced by the continuous combustion of a hydrocarbon fuel in air. Since then a large number of nuclear power plant have been built wherein the source of heat is nuclear fission. On a more modest scale, plant using solar heat sources are being used in suitable locations (see Ref. 28). These new sources of energy do not affect the main discussion here, which is concerned with factors which govern the performance of the vapour cycles themselves. Whatever the source of energy, the overall thermal efficiency of a vapour cycle plant is suitably assessed by the proportion of latent energy in the fuel, or more generally of the energy available in the source, which is converted into useful mechanical work. This overall efficiency can be expressed as the product of two efficiencies: (a) the combustion efficiency or source efficiency, which expresses the proportion of the available energy transferred as heat to the working fluid; and (b) the cycle efficiency, which expresses the proportion of this heat which is converted into mechanical work. In this chapter we are concerned with the comparison of various cycles and with the calculation of cycle efficiency. (Calculation of combustion efficiency requires a knowledge of the thermodynamics of mixtures and chemical reactions, and must be left until Chapter 15 and in particular section 15.6.) Onc should always be aware, however, that modifications to a cycle to improve its cycle efficiency may incur a penalty in reduced combustion or source efficiency unless steps are taken to avoid it. Situations where such interaction of cycle and source efficiency is significant are considered in sections 11.6 and 11.7. Let us now recapitulate briefly the reasons why the cycle efficiency is not zero:
Fig. 11.1 The essential elements of a vapour power plant
Fuel and air
Products of combustion
Source V Qi
>w V Q2 Sink (atmosphere)
207
Applications to Particular Fluids
[11.1]
Thermodynamic The Second Law expresses the fact that even in the best power cycle some heat must be rejected. This best form of cycle was shown in section 6.1 to be one in which: (a) all the heat supplied is transferred while the working fluid is at a constant upper temperature To, and all the heat rejected leaves while the working fluid is at a constant lower temperature Tb; and (b) all the processes are reversible. The efficiency of such a cycle is (To — Tb)/ Ta, irrespective of the working fluid. If the cycle, even though reversible, is such that the temperature of the working fluid changes during a heat transfer process, the cycle efficiency will be less than ( — 'Tb)/T„, where Ta and Tb now refer to the maximum and minimum temperatures reached by the working fluid (section 6.3). Practical All real processes are irreversible, and irreversibilities reduce the cycle efficiency (section 5.5). It is a simple matter to calculate the efficiency of a cycle when all the processes are assumed to be reversible. The result is known as the ideal cycle efficiency. By introducing process efficiencies as defined in Chapter 10, it is also possible to estimate the actual cycle efficiency. The ratio 6f the actual cycle efficiency to the ideal cycle efficiency is called the efficiency ratio. Some cycles are more sensitive to irreversibilities than others. That is, two cycles may have the same ideal cycle efficiencies, but after allowing for the same process efficiencies we find that their actual cycle efficiencies are markedly different. A high ideal cycle efficiency is not therefore by itself a good indication of whether or not the cycle will provide a power plant of high overall efficiency. An additional criterion which indicates the cycle's sensitivity to irreversibilities is required. Such a criterion is furnished by the work ratio rw. Any power cycle consists of one or more processes where work is done by the working fluid and others where work is absorbed. The work ratio is defined as the ratio of the net work output to the gross work output. Irreversibilities, accounted for by process efficiencies, always have the effect of decreasing work outputs and increasing work inputs. Thus if the ideal gross output is only slightly greater than the ideal work input, i.e. if rw is only slightly greater than zero, quite a small amount of process inefficiency is sufficient to reduce the net output to zero and the actual cycle efficiency will drop to zero. On the other hand, as the work ratio approaches unity, the same amount of process inefficiency will have a much smaller effect on the net work output and hence on. the actual cycle efficiency. This point is illustrated in Fig. 11.2, by taking two ideal cycles involving work output WT from a turbine and work input We to a compressor. The cycles have the same heat input Q1 , and cycle efficiency rj, and thus the same net work W, but have radically different work ratios. It is seen that when process efficiencies th and ric for the turbines and compressors are taken into account (see equation (10.3)), the efficiency ri of the cycle having a low work ratio drops much more than that for a cycle having a high work ratio. Summarising, we may say that a high ideal cycle efficiency together with a
high work ratio provide a reliable indication that the real power plant will have a good overall efficiency. 208
Vapour Power Cycles
[11.2] Fig. 11.2 Ideal
The effect of work ratio
Q,„
With 'IT = rle = 0.9
Cycle I
Cycle 2
Cycle I
Cycle 2
120
120
120 90 67.8 22.2 0.247 0.185
120 36 1.1 34.9 0.969 0.291
WT 100 We 61 net W 39 rw 0.390 0.325 II
40 I 39 0.975 0.325
The next consideration is some criterion which will indicate the relative size of plant for a given power output; the complexity of the plant will be obvious from inspection of the ideal cycle. Here again the work ratio sometimes serves as a useful criterion. The component producing the work output has to provide the power for the component requiring the work input, and therefore a work ratio approaching unity indicates that these components will be of least possible size for a given net power output. Most practical vapour cycles, however, have work ratios very near unity; the work ratio is then not very informative and a more direct criterion for size is necessary. In general, the size of the components will depend on the amount of working fluid which has to be pathed through them. A more direct indication of relative sizes of steam plant is therefore provided by the specific steam consumption (SSC), i.e. the mass flow of steam required per unit power output.* It is usually expressed in kg/kW h. If the magnitude of the net work output per unit mass flow is I W1/[kJ/kg] = I WI/[kW s/kg], the SSC can be found from SSC =
1 _ I WI (
1 I W1/[kJ/kg]
kg kW s
x 3600
s h
3600 ) kg I Wald/kg] ) kW h
11.2 Carnot cycle One ideal cycle in which the heat is taken in at a constant upper temperature ( Ta ) and rejected at a constant lower temperature ( Tb) is that suggested by Sadi Carnot (Ref. 2). It consists of two reversible isothermal processes at Ta and Tb respectively, connected by two reversible adiabatic (isentropic) processes. When the working fluid is a condensable vapour, the two isothermal processes are easily obtained by heating and cooling at constant pressure while the fluid is a wet vapour. The cycle is represented on the T—s diagram for steam in Fig. 11.3, and a diagrammatic sketch of the plant.accompanies it. Saturated water in state 1 is evaporated in a boiler at constant pressure to * If the effect of different working fluids is being investigated, account must be taken of their different densities because it is strictly the volume flow which is relevant.
209
[11.2]
Applications to Particular Fluids Fig. 11.3 The Carnot cycle
2
W23 (  y e )
Boiler Expander 3
Q12 (+ve )
Q34 (— ye)
Condenser 4
Compressor W41 (+ve)
form saturated steam in state 2, the heat added being Q12 = h2 — The steam is expanded isentropically to state 3 while doing work in a turbine or reciprocating engine.* The work transfer is W23 — (h3 — h2 ) After expansion the steam is then partially condensed at constant pressure while heat Q34 = h4 h3 is rejected. Condensation is stopped at state 4, where s4 = s1. Finally the steam is compressed isentropically in a rotary or reciprocating compressor to state 1, the work transfer being W41 = (h1 h4) The calculation of the work and heat transfers in the separate processes can be carried out by the methods given in Chapter 10. Example 11.1
Calculate the heat and work transfers, cycle efficiency, work ratio and specific steam consumption of a Carnot cycle (Fig. 11.3), using steam between pressures of 30 and 0.04 bar.
From tables we find that at 30 bar T1 = T2 = 507.0 K and h i = hr = 1008 kJ/kg,
h2 = he = 2803 kJ/kg
Putting s4 = s1 and s3 = s2 (see section 10.2), we find that at the condenser pressure of 0.04 bar, at which T3 = T4 = 302.2 K, x3 = 0.716 and x, = 0.276 For the remainder of this chapter we shall refer to this component as a turbine. The operation of turbines and reciprocating engines is described in detail in Chapters 19 and 16, and the circumstances in which one or the other is preferable are mentioned in section 16.4.
210
Vapour Power Cycles
[11.2]
Hence from h = h f + xhfg we have h3 = 121 + x3 2433 = 1863 kJ/kg h, = 121 + x42433 = 793 kJ/kg The turbine work is W23 = (h3 — // 2 ) —940 kJ/kg and the compressor work is W41 = (h1 — IO= 215 kJ/kg The heat transfers in the boil& and condenser respectively are Q 12 = (h 2 — h 1 ) = 1795 kJ/kg Q34 = (h4 — h3 ) = —1070 kJ/kg The net work for the cycle is therefore W = W23 + W41 = 725 kJ/kg and this is equal to —(Q12 + Q34) as expected from the First Law. The cycle efficiency, as defined by equation (5.2), is =
I WI
=
Q12
725
= 0.404
1795
This must, of course, also be given by — T3 507.0 — 302.2 T,
507.0
— 0.404
The work ratio is r, =
W 725 — — 0.771 W23 940
and the specific steam consumption is SSC =
1 IWI
=
3600
= 4.97 kg/kW h
725
The wider the range of temperature, the more efficient becomes the cycle. The lowest possible temperature of the condensing steam is governed by two factors. The first is the temperature of the sink of heat—atmosphere, ocean or river—for which an average figure of 15 °C may be assumed. (Only natural sinks of heat need he considered; the additional work obtained by using a refrigerated sink could never be greater than the work required for the refrigeration, and with real irreversible processes would always be less.) The second is the temperature difference required for the heat transfer process. The rate of heat transfer is approximately proportional to the surface area across which heat flows, and the temperature difference between the condensing steam and the cooling fluid (see Part IV). In practice, the required rate of heat transfer can be obtained 211
[11.2]
Applications to Particular Fluids
Fig. 11.4
0.5
Variation of Carnot
Boiler pressure 30 bar 0.4
efficiency with condenser pressure
:(2 0.3 U 0.2
U 0.1 90 0 1.00
Condenser temperature/[°C] 60 40 80
0.75
0.50
0.25
0
Condenser pressure/[bar]
with a reasonable size of condenser only if a temperature difference of 10 K to 15 K is provided. The lowest practical condensing temperature in a cycle is therefore 25 °C to 30 °C, the corresponding pressure being 0.032 bar to 0.042 bar. The condenser pressure of 0.04 bar used in Example 11.1, for which the saturation temperature is 29.0 °C, will be used in all the other examples in this chapter. To show how important it is to keep the condenser pressure as low as possible, the variation of cycle efficiency with condenser pressure has been calculated for a constant boiler pressure of 30 bar and the results are presented in Fig. 11.4. The maximum possible temperature of the working fluid, in power plants of the kind considered in this chapter, is governed by the strength of the materials available for the highly stressed parts of the plant, e.g. boiler tubes or turbine blades. This metallurgical limit may be assumed to be 600 °C to 650 °C for steam plant at present, the exact figure depending upon the life required of the plant. For a Carnot cycle operating with steam in the wet region, the highest possible temperature is that corresponding to the critical state: T, = 374.15 °C and pc = 221.2 bar. Modern materials cannot, therefore, be used to their best advantage with this cycle when steam is the working fluid. Fig. 11.5 shows the variation of cycle efficiency and steam consumption with boiler pressure, for a constant condenser pressure of 0.04 bar. It is evident that in the higher pressure range there is only a small gain in cycle efficiency for increased boiler pressure. The cost of the boiler, pipe lines and turbine casing increases with boiler pressure. Moreover the specific steam consumption, and hence the size of plant, increases after a certain pressure is 0.6
Fig. 11.5
10 Condenser pressure 0.04 bar
Variation of Carnot
0.5
efficiency and SSC with boiler pressure
9 11
E
0.4
8
0.3
7 5 U 6 tn
0 0.1
5 200 250
1)
212
50
300
350
1(11) 150 Boiler pressure/]bar]
374.15 200
4 250
Vapour Power Cycles
[11.2]
reached. Evidently the most economic pressure must be determined by reaching a compromise between low operating cost and low capital cost. In the previous section we pointed out that the ideal cycle efficiency is not by itself a good guide to the probable overall efficiency of the actual plant. The work ratio for the cycle in Example 11.1 is, by comparison with other types of vapour cycle, quite low (0.771), and we must expect irreversibilities to have an appreciable effect on the cycle efficiency and steam consumption. The following example shows the effect of assuming values less than unity for the process efficiencies of the turbine and compressor when the boiler and condenser pressures are 30 bar and 0.04 bar as before. Example 11.2
Recalculate Example 11.1 with isentropic efficiencies of 0.80 for the compression and expansion processes ( Fig. 1 1.6 ), to estimate the actual cycle efficiency and steam consumption.
The actual turbine work is h 2 ) = 0.80(h3 — 112 ) = —752 kJ/kg W23 = and the actual compressor work is W41 = (h 1 — h4 ) =
(//', — h4) 0.80
— 269 kJ/kg
The net work is therefore W = W23 + W41 = —483 kJ/kg The enthalpy in state 1 is
1 hi = ha + Wai —062 kJ/kg and hence the heat transfer to the boiler is Q12 = (h2
h1)
1741 kJ/kg
The thermal efficiency is 17 =
RI = 0.277 Q12
and the specific steam consumption is SSC =
1 I WI
Fig. 11.6
=
3600
7.45 kg/kW h
483
T
213
[11.3]
Applications to Particular Fluids
The previous examples show that the cycle efficiency is reduced by irreversibilities from 0.404 to 0.277, and that the steam consumption is increased from 4.97 kg/kW h to 7.45 kg/kW h. We shall show that more practical forms of steam cycle have work ratios nearer unity and so are much less affected by irreversibilities.
11.3 Rankine cycle
There are two major reasons why the Carnot cycle is not used in practice: first, because it has a low work ratio; and secondly, because of practical difficulties associated with the compression. It would be difficult to control the condensation process so that it stopped at state 4, and then carry out the compression of a very wet vapour efficiently. The liquid tends to separate out from the vapour and the compressor would have to deal with a nonhomogeneous mixture. Moreover the volume of the fluid is high and the compressor would be comparable in size and cost with the turbine. It is comparatively easy, on the other hand, to condense the vapour completely, and compress the liquid to boiler pressure in a small feed pump. The resulting cycle, shown in Fig. 11.7, is known as the Rankine cycle. It is evident without calculation that the efficiency of this cycle will be less than that of the Carnot cycle operating between the same temperatures, because all the heat supplied is not transferred at the upper temperature. Some heat is added while the temperature of the liquid varies from T5 to T1 . It is also evident, from the Comparative areas of the two cycles, that the net work output per unit mass of steam is greater in the Rankine cycle (in section 8.4.1 it was shown that the area = ( T ds),.e„ = dQ = IWI). It follows that the steam consumption is less and the work ratio is greater. Thus, in spite of a lower ideal cycle efficiency, the actual cycle efficiencies may not be so different, and the size of the Rankine plant will certainly be much smaller. The following example verifies these deductions. Fig. 11.7
2
The Rankine cycle
T
214
Vapour Power Cycles
[11.3]
Example 11.3
Calculate the cycle efficiency, work ratio, and steam consumption of the Rankine cycle in Fig. 11.7, working between the same pressures as the Carnot cycle in Example 11.1. Estimate the actual cycle efficiency and specific steam consumption when the isentropic efficiencies of the expansion and compression processes are each 0.80.
(a) Ideal cycle As in Example 11.1, h2 = 2803 kJ/kg and h3 = 1863 kJ/kg And the turbine work is, as before, W23 = (h3 — h2 ) = —940 kJ/kg Using equation (10.5), the feed pump work of compression W45 is given by
= 0.001(30 — 0.04) x 100 = 3 kJ/kg
W45 = Vf (P5 —
And since the process is adiabatic, we. have directly from the steadyflow energy equation W45 = (h5 — h4)
Now h4 = he = 121 kJ/kg, and hence h5 = W45 +
= 3 + 121 = 124 kJ/kg
The heat supplied is then Q52 = (h2 — h5 ) = 2803 — 124 = 2679 kJ/kg
Therefore IWI 940 — 3 Q 52
2679
W
rw —
W23 SSC — 1
1
—
=0.350
940 — 3 940
— 0.997
3600
IWI 940 — 3
— 3.84 kg/kW h
(b) Actual cycle (Fig. 11.8) Actual expansion work is W23 = —0.80 x 940 = —752 kJ/kg and the actual compression work is 3 W45 = 0.80=4 kJ/kg
The enthalpy at state 5 now becomes h5 = h4 + W45 = 125 kJ/kg 215
Applications to Particular Fluids
[11.3]
Fig. 11.8
and the heat supplied is Q52 = (h2 h5) = 2803 — 125 = 2678 kJ/kg
Therefore =
I WI 752 — 4 =
Q 52
SSC =
2678
= 0.279
1
3600 = —4.81 kg/kW h I WI 752 — 4
The first point to note from the previous example is that the compressor work, or feed pump term, is very small compared with the other energy transfers. When the boiler pressure is comparatively low, a good approximation to the ideal cycle efficiency will be obtained if it is neglected. The approximate calculation yields the following results for the ideal cycle of the previous example: W z W23 = —940 kJ/kg, ,ct, 0.350,
Q52 (h2  h4) = 2682 kJ/kg
SSC P., 3.83 kg/kW h
This confirms the fact that the points representing states 4 and 5 almost coincide on the T—s diagram if it is drawn to any reasonable scale (see section 8.4.1). The second point worth noting is that the difference between the performance of the ideal and actual cycles is much smaller than in the case of the Carnot cycle working between the same pressures and with the same process efficiencies. This is emphasised by the following table, in which the actual cycle performances are compared with the ideal values. For the assumed operating conditions the actual cycle efficiency of the Rankine plant (0.279) is slightly greater than that of the Carnot plant (0.277). Cycle
rw
Efficiency ratio
Carnot Rankine
0.771 0.997
0.686 0.797
Actual SSC Ideal SSC 1.50 1.25
Fig. 11.9 shows the results of a series of ideal cycle calculations with various boiler pressures and a constant condenser pressure of 0.04 bar. The cycle efficiency does not increase continuously with boiler pressure up to the critical 216
Vapour Power Cycles
[11.3] Fig. 11.9 Variation of Rankine cycle efficiency and SSC with boiler pressure
5
0.5 0
11
0.4
SSC
: 61). 0.3
Condenser pressure 0.04 bar
U 0.1 0
200 250 I i 50
Boiler temperature/N1 300 350 374.15 I I I 0 100 150 200 250 Boiler pressure/[bar]
pressure, but reaches a maximum when the pressure is about 160 bar. The reason is that the latent heat, and therefore the proportion of the heat supplied which is transferred at the upper temperature, becomes smaller as the pressure increases. Sooner or later the effective average temperature at which the heat is added starts to decrease and the efficiency falls. For a high efficiency it is essential to keep the condenser pressure as low as possible. However, where space is restricted as in a steam locomotive, or where no cooling water is available, the condenser is omitted and an open cycle is used (see section 4.4). When the boiler feed water temperature is 100 °C, the ideal cycle efficiency is then identical with that of a closed cycle plant condensing at 1 atm. The condition of the fluid is the same at entry to the boiler in the two cases, and the fact that the fluid entering the boiler is not the same as that leaving the turbine makes no difference. If the boiler feed water temperature is less than 100 °C, the efficiency will be reduced because more 'sensible heat' must be added in the boiler. It has already been remarked that the metallurgical limit cannot be approached when the steam leaves the boiler in a saturated condition. But by placing in the combustion gases a separate bank of tubes (the superheater) leading saturated steam away from the boiler, it is possible to raise the steam temperature without at the same time raising the boiler pressure. The Rankine cycle then appears as in Fig. 11.10, from which it is evident that the average temperature at which heat is supplied is increased by superheating and hence the ideal cycle
Fig. 11.10 The Rankine cycle with superheat
Qas
Superheater
S
217
[11.3]
Applications to Particular Fluids Fig. 11.11 Effect of superheating on the performance of the Rankine cycle
0.5 0.4
0.3 0.2
5
Y1
4
SSC
0.5 — 11
3
Boiler pressure 30 bar 2U 0.1 —Condenser pressure 1 '63 0.04 bar 0 0 200 400 600 800 Superheat temperature/[°C] (a)
5
it
0.4
4
0.3
3 te,
0.2
SSC
2
Superheat temperature 600 °C 1`c%') 0.1 Condenser pressure 0.04 bar 0 0 0 50 100 150 200 250 Boiler pressure/[bar] (b)
efficiency is increased. There is very little change in susceptibility to irreversibilities, the work ratio being so very near unity in the unsuperheated Rankine cycle that the slight increase obtained by superheating makes very little difference. Nevertheless, the specific steam consumption is markedly reduced, the net work per unit mass of steam being much greater, so that the added complexity of a superheater is compensated by a reduction in the size of other components. Fig. 11.11a shows the variation of ideal cycle efficiency and specific steam consumption with superheat temperature up to 800 °C. There is evidently still much to be gained by improving hightemperature materials. Unlike the efficiency of the unsuperheated cycle, the efficiency of the superheated cycle increases continuously with pressure. Fig. 11.11b illustrates this for a cycle with 0.04 bar condenser pressure and superheating to 600 °C—the metallurgical limit for longlife plant. There is an additional reason why superheating is always used in practice. In the unsuperheated cycle of Example 11.3 the dryness fraction at the turbine exhaust is 0.716. Inspection of the T—s diagram shows that with higher boiler pressures the turbine exhaust would become even wetter. This is a very undesirable feature, because, droplets in the steam erode the blading and reduce the turbine isentropic efficiency; see section 19.2.4. In practice the dryness fraction at the turbine exhaust is not allowed to fall below about 0.88. Superheating increases the dryness fraction, although with the present metallurgical limit in the range of 600650 °C it is not always by itself sufficient to maintain the dryness fraction above 0.88. For example, when the steam enters the turbine at 160 bar and 600 °C, the turbine exhaust dryness fraction after isentropic expansion to 0.04 bar is 0.772; irreversibilities in the turbine tend to increase the dryness fraction but they would not bring the value up to 0.88. With supercritical cycles (i.e. when 2345 in Fig. 11.10 is a supercritical isobar) this problem is even more severe; the remedy lies in the use of reheat cycles, discussed in the next section. Fig. 11.11b shows the ri and the SSC curves extended beyond the critical pressure of 221.2 bar. It would appear'that the use of pressures beyond 160 bar, let alone supercritical pressures, is hardly justified. However, when reheating and regenerative feed heating are applied to such cycles, as described in the next two sections, it becomes worth using such extreme pressures. 218
Vapour Power Cycles
[11.4] Fig. 11.12 The reheat cycle
4
HP turbine 5
T
Supercritical pressure
11.4 Reheat cycle
With the reheat cycle the expansion takes place in two turbines. The steam expands in the highpressure turbine to some intermediate pressure, and is then passed back to yet another bank of tubes in the boiler where it is reheated at constant pressure, usually to the original superheat temperature.* It then expands in the lowpressure turbine to the condenser pressure. The cycle appears as in Fig. 11.12, and the following example shows the effect of reheating on the ideal cycle efficiency and specific consumption. A boiler pressure of 30 bar has been assumed for the sake of comparison with the other examples in this chapter, although this is well below the most economical pressure for which to design a reheat cycle plant. Example 11.4
Find the ideal cycle efficiency and specific steam consumption of a reheat cycle (Fig. 11.12) operating between pressures of 30 and 0.04 bar, with a superheat temperature of 450°C. Assume that the first expansion is carried out to the point where the steam is dry saturated and that the steam is reheated to the original superheat temperature. The feed pump term may be neglected. From tables, h2
V
hi = 121 kJ/kg,
h 5 = 3343 kJ/kg,
s5 = 7.082 kJ/kg K
" bI, To find the intermediate reheat pressure p6, we find from the saturation 11 table the pressure at which sg = s5. This gives
p6 = p7 = 2.3 bar and hence h6 = 2713 kJ/kg
* It has been suggested that as an alternative to the conventional reheat scheme, it is better to reheat the steam near the turbine via a liquid metal circulating between the boiler and reheater. The appreciable pressure drop in the lengthy conventional reheat circuit is avoided, but this gain is partially offset by the extra temperature drop required for the liquid metal circuit.
219
[11.4]
Applications to Particular Fluids Fig. 11.13 Use of the h—s diagram
h
From the superheat table, h, = 3381 kJ/kg and s, = 8.310 kJ/kg K At the turbine outlet, x8 = 0.980 and h8 = 2505 kJ/kg The total quantity of heat transferred to the steam in the boiler is Q25 + Q67 = (h5 — h2 )
(h, — h6 ) = 3222 + 668 = 3890 kJ/kg
and the total turbine work is W56 + W78 — (h6 — h5 ) (h8 h„) = —630 — 876 = —1506 kJ/kg The cycle efficiency is therefore =
I(W56 + W78)1 1506 — =0.387 Q25 + Q67 3890
and the specific steam consumption is SSC =
1 3600 = = 2.39 kg/kW h I WI 1506
This example, as well as the other examples in this chapter, can be solved more quickly by means of an h—s chart. This is illustrated in Fig. 11.13. The chart usually covers only the superheat region and the twophase region near the saturated vapour line, and it cannot therefore be used for finding h 1 , h2 and h3. It enables one, however, to find h5, h6, h, and h8 more quickly than by means of tables. Comparing the foregoing results with those of Examples 11.1 and 11.3, and the appropriate values from Fig. 11.11a (all cycles with a boiler pressure of 30 bar and a condenser pressure of 0.04 bar), we arrive at the following table for ideal 220
Vapour Power Cycles
[11.4]
cycles:
SSC/[kg/kW h]
Carnot
Rankine (no superheat)
Rankine (superheat to 450°C)
Reheat (to 450°C)
0.404 4.97
0.350 3.84
0.375 2.98
0.387 2.39
It can be seen that reheating reduces the steam consumption appreciably, as might be expected from consideration of the area of the cycle on the T—s diagram which equals the magnitude of the net work output per unit mass of steam. This reduction is a particularly important consideration in higherpressure cycles because it implies a smaller boiler—an expensive item in highpressure plant. However, this decrease in size cannot completely offset the disadvantage of the added complexity, and it must be stressed that the main reason for reheating is to avoid too wet a. condition in the turbine. It is clear that reheating makes only a little difference to the ideal cycle efficiency. Whether it increases or decreases the efficiency, in comparison with the Rankine cycle having the same conditions in the boiler and condenser, depends upon the point in the expansion at which reheating is carried out. The reheat cycle can be regarded as a combination of the Rankine cycle and the cycle abcd (or a' b'c'd) in Fig. 11.14. If the latter has a lower efficiency than the Rankine cycle, the efficiency of the combination will be lower also. The effective average temperature at which the heat is added in the cycle abcd may well be lower than that in the Rankine cycle if the intermediate pressure is too low. Cycles using supercritical pressures have been coming into operation in recent years. With such cycles the problem of moisture in the turbine is even more severe, and the use of reheating is essential. So far, it has been possible to avoid the additional complication of reheating at more than one point in the expansion, although doublereheat units are now being considered. Typical modern supercritical and subcritical ideal cycles are compared in the following table, where reheating is assumed to occur when the steam is just saturated (x. = 1
Fig. 11.14 The effect of reheat pressure on the cycle efficiency
T
221
[11.5]
Applications to Particular Fluids
in Fig. 11.14): Superheat to 600 °C
SSC/[kg/kW h] xexit
Superheat and reheat to 600 °C
160 bar
350 bar
160 bar
350 bar
0.453 2.31 0.772
0.486 2.37 0.708
0.468 1.76 0.954
0.485 1.80 0.871
Although the increase in efficiency resulting from the use of supercritical pressures seems small, it should not be discounted. A 1 per cent increase in efficiency for a cycle which has an actual efficiency of say 40 per cent is equivalent to 1/0.4 = 2.5 per cent saving in fuel—a saving well worth having. Nevertheless it is true to say that a marked improvement in efficiency of the reheat cycle cannot be obtained by using higher pressures; it can be achieved only by developing new hightemperature alloys or other materials for turbine blading and superheater tubing and thereby raising the metallurgical limit.
11.5 Regenerative cycle
The efficiency of the unsuperheated cycle (Fig. 11.7) is less than the Carnot efficiency ( l'a — Tb)/ Ta, because some of the heat supplied is transferred while the temperature of the working fluid varies from T5 to Ti . If some means could be found to transfer this heat reversibly from the working fluid in another part of the cycle, then all the heat supplied from an external source would be transferred at the upper temperature and the Carnot cycle efficiency would therefore be achieved. A cycle in which this artifice is used to raise the efficiency is called a regenerative cycle. One method which is theoretically possible is indicated in Fig. 11.15. The feed water, at T6 , is passed into passages in the turbine casing at the point where the expanding steam has a temperature only infinitesimally greater than T6. The water flows in a direction opposite to that of the expanding steam, and Fig. 11.15 A hypothetical regenerative cycle
222
Vapour Power Cycles
[11.5]
is thereby heated to a temperature only infinitesimally smaller than T2 before it passes into the boiler. At all points the heat transfer is effected by an infinitesimal temperature difference and the process is therefore reversible. Most of the expansion in the turbine is no longer an adiabatic process, but follows the path 234. Since the heat rejected in process 23 equals that supplied in process 61, the shaded areas on the T—s diagram of Fig. 11.15 must be equal. The heat supplied from the external source is equal to the area under line 12, and the heat rejected to the external sink equals the area under line 45. Inspection of the areas involved shows that not only are the efficiencies of the regenerative cycle and the Carnot cycle 1278 equal, but the steam consumptions also. On the other hand the work ratio of the regenerative cycle, requiring the negligible pump work ( h6 — h5 ), is very much higher than that of the Carnot cycle and is comparable with that of the Rankine cycle. Such a regenerative cycle is impractical for two reasons. First, it would be impossible to design a turbine which would operate efficiently as both turbine and heat exchanger. Secondly, the steam expanding through the turbine would reach an impracticably low dryness fraction. For these reasons the basic idea of regeneration is applied in a somewhat different way: instead of the feed water being taken to the turbine, some of the turbine steam is taken to the feed water. The simplest approximation to a practical regenerative cycle is shown in Fig. 11.16. Consider 1 kg of steam in state 2 passing from the boiler into the turbine. This steam is expanded to an intermediate state 3, at which point a quantity y kg is bled off and taken to a feed water heater. The remaining (1—y) kg is expanded to condenser pressure and leaves the turbine in state 4. After condensation to state 5, the (1—y) kg of water is compressed in the first feed pump to the bleeding pressure (p6 = p3). It is then mixed in the feed water heater with y kg of bled steam in state 3, and the 1 kg of mixture leaves the heater in state 7. A second feed pump compresses the water to boiler pressure, state 1. In this cycle the average temperature at which the heat is added from an external source is higher than in the Rankine cycle, and therefore the efficiency is increased. The cycle is not a true ideal cycle, because the mixing process between steam at state 3 and water at state 6 is irreversible. In the limit, as the number of bleedings and feed water heaters is increased to infinity, the mixing processes 2
Fig. 11.16 A simple regenerative cycle using one feed water heater
W2; W  34
Q45
6 1 kg
— y) kg 5 Feed pump 1 kg I < 7
W71
Feed heater
Feed pump 6
W56
223
Applications to Particular Fluids
[11.5]
become reversible, all the heat from the external source is supplied at the upper temperature, and the cycle will therefore have the Carnot efficiency. Since a regenerative cycle of this kind is really a combination of cycles undergone by different quantities of fluid, there is some difficulty in portraying it on a T—s diagram. Fig. 11.16 must be interpreted as implying that (1 — y) kg is carried through cycle 5 6 7 1 2 3 4 5, while y kg follows the path 71237. Example 11.5 Find the cycle efficiency and specific steam consumption of a regenerative 1 cycle with one feed heater, if the steam leaves the boiler dry saturated at 30 bar and is condensed at 0.04 bar (Fig. 11.16). Neglect the feed pump work. It is first necessary to select the pressure p3 at which the steam is to
be bled off. It is shown later that the cycle efficiency is a maximum when the temperature T3 is approximately halfway between T2 and T4 , i.e. T2 + T4 233.8 + 29.0 — 131.4°C 2 2
T 1
and hence p3 = 2.8 bar We can now calculate the correct mass y kg to be bled off at p7 . Consider the heater as an adiabatic open system (Fig. 11.17). No work is done and the energy equation reduces to 0 = 1h7 — yh3 — (1 — y)h6 Putting h6 = 115, we find that Y
h7
h5
h3 — h5
From tables, 11 5 = 121 kJ/kg and h7 = 551 kJ/kg Also, h2 = 2803 kJ/kg and s2 = 6.186 kJ/kg K Putting s2 = s3 = s4, we find
Fig. 11.17 The feed water heater as an adiabatic open system
x3 = 0.846,
h3 = 2388 kJ/kg
x4 = 0.716,
h4 = 1863 kJ/kg
y kg
1 kg 7
224
Vapour Power Cycles
[11.5]
Hence 551 — 121 y=
2388 — 121
— 0.1897
The heat transferred in the boiler is Q12 = (h2 — h 1 ) = 2803 — 551 = 2252 kJ/kg The turbine work is W23 + W34 = 1(h3 h2 ) + (1 y)(h4 h3) = —415 — 425 = —840 kJ/kg Therefore l(W23 + W34)I
=
Q12
840 2252
= 0.373
and the specific steam consumption is SSC =
1
00
I WI = 3640 8
= 4.29 kg/kW h
In Fig. 11.18 the cycle efficiency is plotted against bleed temperature, all the other conditions remaining constant. It can be seen that the cycle efficiency is a maximum when the bleed temperature is approximately equal to the mean of the boiler and condenser temperatures, and that a slight deviation from this value does not affect the efficiency significantly. Comparing the results of Example 11.5 with those of the ideal unsuperheated Rankine cycle in Example 11.3, the efficiency has been increased from 0.350 to 0.373 with the use of only one feed heater. On the other hand the specific consumption has been increased from 3.84 kg/kW h to 4.29 kg/kW h. In practice the best return for the additional capital cost is obtained with several feed heaters, the exact number depending on the steam conditions. The proper choice of the bleed pressures is a matter of lengthy optimisation calculations which cannot be entered into here. The open heater, in which the bled steam is freely mixed with the feed water, is not often used because of the large number Fig. 11.18 Effect of bleed temperature on the cycle efficiency
0.38
Boiler pressure 30 bar Condenser pressure 0.04 bar
0.37 :5 0.36
U 0.35 0
0.04 /
0.2 i 50
LO
Bleed pressure/[bar] 10 2 I I 100 200 150
250
Bleed temperature/[°C]
225
[11.5]
Applications to Particular Fluids Fig. 11.19 A regenerative cycle with three feed water heaters
1 kg
19 14
Heater 1
kg 15
18 (y„ + Yb + Yr) kg (y„ + yb) kg Heater 3 Heater 2
T
of feed pumps required (i.e. number of heaters + 1). Fig. 11.19 illustrates a plant using three heaters of the closed type, in which the heat is transferred through banks of tubes. For example, considering heater 1, the bled steam in state 5 drains from the feed heaterin state 14 as a separate stream; this is different from the open heater arrangement of Fig. 11.16. The drain in state 14 can be pumped back into the feed line at point 1 by means of a small drain or drip pump, but a more common arrangement is to cascade it back through throttle valves, via the lowerpressure feed heaters, to the condenser. The advantage of doing this is that only one feed pump is required; a similar train of open heaters would require four feed pumps in the feed water line. The throttling of the 226
Vapour Power Cycles
[11.5]
drains is accompanied in practice by the formation of some steam, and this can lead to rapid erosion in the cascade line. To avoid this erosion, the drains are throttled into large flash chambers (not shown) which reduce the velocity and therefore the erosion. Considering the T—s diagram in Fig. 11.19, the feed water leaving the feed pump in state 10 is successively heated to temperatures T11, T12 and T1 which, ideally, are equal to the saturation temperatures T17, T15 and T13* respectively. In practice T11 < T17 , T12 < T15 , T1 < T13 , the differences usually being referred to as the terminal temperature differences of the heaters. Similarly the condensed bled steam should drain at temperatures T14 = T12, T16 = T11 and T18 = T10. Such ideal conditions can only be achieved with closed heaters having infinitely large heat exchange areas. The following example, which is concerned with the ideal cycle, assumes such limiting conditions to exist.
Example 11.6
Calculate the ideal cycle efficiency and specific steam consumption of a regenerative cycle using three closed heaters as shown in Fig. 11.19. The steam leaves the boiler at 30 bar superheated to 450°C, and the condenser pressure is 0.04 bar. Choose the bleed pressures so that the temperature difference ( T2 — T9 ) is divided into approximately equal steps. (Such a choice of bleed pressures makes the efficiency of the ideal cycle approximately a maxiMum.) Making the temperature differences ( T2 — T13), ( T13 — T15 ), ( T15 — T17 ), (T17 — T9) approximately equal, the bleed pressures become 11, 2.8 and 0.48 bar. All the relevant enthalpies in the plant can now be found. Before. during and after expansion in the turbine these are
h4 = 3343 kJ/kg,
h5 = 3049 kJ/kg
h6 = 2749 kJ/kg,
h7 = 2458 kJ/kg,
h8 = 2133 kJ/kg
In finding the enthalpies in the feed line, the following assumptions will be made: (a) The feed pump term is negligible, i.e. h9 h10 . (b) In throttling the condensed bled steam, which is a process of equal initial and final enthalpy, the state after throttling lies approximately on the saturation line; e.g. in throttling from 14 to 15, h14 = h15 will be identical with hl corresponding to pressure p6. (c) The enthalpy of the compressed liquid in the feed line is approximately equal to that of saturated liquid at the same temperature, e.g. h12 x h15.
* It might appear feasible, where the bled steam is initially superheated and condensed in a counterflow heater, for the exit temperature of the feed water to attain the superheat temperature, e.g. Ti = T5 in heater 1. This ideal cannot be achieved, however, because the difference between the sensible enthalpy capacities of the bled superheated steam and the feed water would necessitate heat transfer from colder steam to hotter feed water over the temperature range T13 4 Ts . Although the condition T1 = T5 is impossible, the heater could be designed so that the ideal feed temperature T1 is slightly above T13, but this possibility will be neglected in what follows.
227
[11.5]
Applications to Particular Fluids
With these assumptions we can write h10 = hls = h19 = h9 = 121 kJ/kg h11 = h16 = h17 = 336 kJ/kg h12 = h14 = 12 15 = 551 kJ/kg h1 = h13 = 781 kJ/kg To determine the correct amounts of steam to be held for each heater per kg of steam leaving the boiler, an energy equation can be written down for each heater. First heater:
1h1 + )V114 — ya h, — 1h12 = 0 Y. =
h13 — h„
— 0.0921
h5 — h15
Second heater:
1 h12 + (Ya + Yb)h16 — Ybh6 — 1h 11 — ya k, = 0 h„ h 17 — 0.0809 Yb = (1 — Ya) h6 — h17
Third heater:
114 1 + (Ya + Yb Ye)1118 — Ych7
(Ya Yb)h17
— 1h1, = 0 ya = ( 1 — ya yb)
h17
h9
— 0.0761
h7 — h9
(Always start with the highestpressure heater so as to have only one unknown at each step in the calculation.) We can now calculate the heat and work transfers for the cycle. The heat added in the boiler is 12 1 , 4 = (h 4 — h 1 ) = 2562 kJ/kg and the heat rejected in the condenser is Q8,9 = 1 h9 — ( 1 —
Y. — Yb —
— (Ya + Yb + Ye)h19
= —1511 kJ/kg The work done in the turbine is W4,8 = 1(h 5 h4) ( 1
Ya)(h6
h5) + ( 1 —
Ya — Yb)(h7 — h6)
+ (1 — ya — yb — yc)(h8 — h7 ) = — 1051 kJ/kg (As a check, W4 , 8 must also be given by W4,8 The cycle efficiency is
= 1W4' 81 — 0.410 Q1,4
and the specific consumption is SSC =
228
1 I WI
=
3600 = 3.43 kg/kW h 1051
(Q1,4 + 128,9)
1051 kJ/kg.)
[11.6]
Vapour Power Cycles
The ideal efficiency and steam consumption for the Rankine cycle corresponding to the cycle 92489 in Fig. 11.19 can be found from Fig. 11.11a to be 0.375 and 2.98 kg/kW h. For the regenerative cycle these become 0.410 and 3.43 kg/kW h. Apart from the marked improvement in cycle efficiency, regeneration has the advantage of easing the difficulties in the design of the blading at the lowpressure end of the turbine. With the Rankine cycle this blading has to pass a very large volume flow and the blades must be undesirably long. By bleeding, the volume flow at the lowpressure end is considerably reduced; this is indicated by the stepped outline of the turbine in Fig. 11.19. The size of the condenser is also reduced, which partially compensates for the additional feed heating components. It is necessary to point out that if the isentropic efficiency of the turbine is not unity, points 5, 6, 7, 8 on the T—s diagram will not be vertically below point 4. To estimate the actual cycle efficiency with an irreversible expansion it is necessary to know the path of the expansion (i.e. line of condition), and this is considered in section 19.2.5. With modern steam conditions the best compromise between additional capital costs and improved efficiency is obtained when a train of about eight feed heaters is used. It is common to include one open heater at a moderate pressure which incorporates a deaerator, because dissolved air leads to corrosion in the boiler, and is detrimental to heat transfer and the maintenance of a high vacuum in the condenser. There will normally be two closed heaters at pressure below the open heater, with the condensed bleed cascading back into the condenser. At pressures above the open heater there will be about three closed heaters whose condensate cascades back into the open heater. A description of modern plant and a more detailed thermodynamic analysis of regenerative cycles can be found in Refs 18 and 34 respectively. The observant student may have noticed that to call the 'open feed heater' a heater is a misnomer. The component is an adiabatic mixing chamber, and no 'heat' in the thermodynamic sense is involved in the process.
11.6 Economiser and air preheater
So far we have been comparing the performance of the various cycles on the basis of cycle efficiency, and have assumed in effect that the combustion process can be carried out with equal efficiency in all plants. This is not, in fact, the case. Without discussing combustion efficiency in detail, it can be appreciated that if the combustion gases leave the boiler plant at a temperature higher than atmospheric, some of the latent energy in the fuel is being wasted. Useful work could still be obtained by operating a cycle between the exhaust gas temperature and atmospheric temperature. With the Carnot cycle, the lowest temperature at which the exhaust gases can leave the plant is the upper temperature of the cycle. With the Rankine cycle, on the other hand, the exhaust gases could be reduced, ideally, to the temperature of the water leaving the feed pump. A reduction in exhaust gas temperature is accomplished in practice by passing the feed water through a bank of tubes, the economiser, situated in the chimney. 229
[11.6]
Applications to Particular Fluids
Flue gases
Fig. 11.20 Diagrammatic sketch of a boiler plant with (a) an economiser and (b) an air preheater
Flue gases
Economiser
Air
Feed water from condenser
Super To turbine
4) heater Grate (a)
(b)
The flow is in the direction indicated in Fig. 11.20a, so that the hottest gases are transferring heat to the hottest water, and the temperature difference between the fluids is kept to a minimum throughout the process. One limitation is that the products of combustion should not normally be cooled below their dew point (see section 14.5), otherwise condensation containing corrosive acids may cause serious damage to the economiser tubes. The dew point of sulphuric acid vapour is at a higher temperature than that of pure water vapour, and in practice 150 °C is considered the safe lower limit. For small commercial and domestic boilers burning natural gas which is free of sulphur, it is economical to use stainless steel components and this limit is unnecessary; these are called condensing boilers. It would appear that the advantage of higher ideal efficiency possessed by the Carnot cycle is at least partly diminished by its inability to abstract all the energy available in the products of combustion—a further argument in favour of the practical superiority of the Rankine cycle. The regenerative cycle suffers from the same disadvantage as the Carnot cycle in this respect. If an economiser is added to the cycle shown in Fig. 11.19, the minimum temperature to which the combustion gases can be cooled is Ti . When a large number of feed heaters is used, the feed water entering the boiler is nearly at boiling point and an economiser becomes superfluous. An alternative method of reducing the temperature of the combustion gases, which can be used with all the cycles, is known as air preheating. The air preheater is a bank of tubes in the chimney through which the combustion air passes before reaching the grate, as in Fig. 11.20b. The combustion gases are cooled while the temperature of the air is increased prior to combustion. Since the reactants start with a higher temperature, less fuel need be burnt to arrive at the same products temperature. The net result is an increase in combustion efficiency comparable with that obtained with an economiser. Air preheating is often used in conjunction with an economiser in Rankine and reheat plants, but the degree of preheating cannot be carried as far as in the regenerative plant where no economiser is fitted. (It is worth noting that the most common type of air preheater is not a fixed bank of tubes, but a rotating matrix of the type illustrated schematically in Fig. 24.5.) One practical consequence of cooling the combustion gases is that only a 230
Vapour Power Cycles
(11.7]
small amount of natural draught can be obtained in the chimney. The heat exchanging banks of tubes, grate and chimney require a fair pressure gradient to maintain the necessary air flow for combustion. For this reason a forced draught, produced by a fan, is always used in modern boiler plant. The power expended on driving the fan is small compared with the advantage gained by improving the combustion efficiency. Enough has been said to indicate that a complete evaluation of an externalcombustion power cycle must take account of the interdependence between the combustion and cycle efficiencies. The adoption of means to improve one efficiency may easily lead to the reduction of the other. A formal analysis of the plant as a whole is possible using the concept of exergy introduced in section 7.9, and Refs 12 and 13 of Part I provide a good introduction to this approach. 11.7 Steam cycles for nuclear power plant
Nuclear power plant have been developed mainly on what can be called conventional lines, by using the nuclear reactor as a source of heat for a steam cycle. Some effort is being directed towards the direct conversion of nuclear energy into electrical energy, e.g. via the magnetohydrodynamic generator briefly described in Chapter 20, but these efforts still have to bear fruit. Here we shall discuss briefly some of the consequences arising from the application of nuclear energy sources to steam cycles. Although the principles discussed in the preceding sections apply also to nuclear plant, there exist a number of difficulties peculiar to such plant. They arise largely from present restrictions on the maximum permissible temperature which 'fuel' elements in a reactor are allowed to reach, and from the use of a secondary fluid to transfer energy from them to the steam. There is every prospect that further development of reactor materials will ease these restrictions and therefore remove at least some of these peculiar difficulties. Fig. 11.21a shows diagrammatically a simple scheme employing a secondary fluid which circulates through the reactor and transfers heat to the steam boiler. Fig. 11.21
Reactor coolant
Simple nuclear power plant
T
Heat exchanger (steam boiler) Circulator pump (a)
(b)
231
[11.7]
Applications to Particular Fluids Fig. 11.22 An application of the temperature—enthalpy diagram
T
T
L _ Boiling fluid
Tax
`las 2,5 Steam
o
Pinch point
ItQ — .H —)I Enthalpy H
Enthalpy H
(a)
(b)
In early reactors the permissible maximum temperature Trnax of the secondary fluid leaving the reactor was below the critical temperature of steam, and it might appear that the cycle shown in Fig. 11.21 b would have been the obvious choice. However, quite apart from the difficulty of excessive moisture in the turbine which such a choice would entail, it should be remembered that the secondary fluid falls in temperature as it flows through the heat exchanger, and therefore the saturation temperature of the steam must be well below Tn.. This is most easily appreciated on the T—H diagram of Fig. 11.22a, where H is the product of mass flow and specific enthalpy of the respective fluids. AH must be the same for the two curves, it being equal to the total quantity of heat transferred. The saturation temperature is chosen so that at the socalled pinch point the secondary fluid temperature is marginally higher than the saturation temperature, and it can be seen that under these conditions a certain amount of superheating is possible. The use of such T—H diagrams, and the significance of pinch points, will be illustrated in examples in sections 11.9 and 12.5. The secondary fluid temperature drop, for a specified heat transfer, can be varied by varying the mass flow as indicated in Fig. 11.22b. A higher mass flow enables a higher saturation temperature to be used for the power cycle and thus a higher steam cycle efficiency to be obtained, but it also entails a higher circulating pump power, and it is the net (turbine—pump) work which is important. It is obvious that the steam conditions cannot be optimised on the basis of steam cycle efficiency alone, but must be considered in conjunction with the pumping power of the secondary fluid circuit. An analogous interaction of cycle and combustion efficiency was discussed in section 11.6, but such interactions are not nearly as critical as those in the nuclear reactor. Until recently, all British plant of commercial size have used a gas as the secondary fluid, namely compressed CO2, and the pumping power for gas is large and increases rapidly with the mass flow. An alternative coolant, widely used around the world, is pressurised water. It has good heat transfer characteristics (i.e. much less heat transfer area is required) and needs much less pumping power, but a coolant circuit breakdown can have more serious consequences. Even better heat transfer characteristics are offered by liquid metals such as sodium, but these fluids add to safety problems and capital cost and so far have been used only in experimental 'breeding' reactors which have exceptionally small 232
Vapour Power Cycles
[11.7] Fig. 11.23
Reactor coolant
Dualpressure cycle Steam side T
— LP — HP
11, g #31r, sEl • 1.) .; 4 12181 ▪ II x !at l
Feed heaters (a)
Enthalpy H (b)
reactor cores and consequently very restricted heat transfer surface area. It should be appreciated that the number of possible secondary fluids is limited because, as with any material in the reactor core, the nuclear characteristics play an overriding role. In particular, materials must have only a very weak capacity for absorbing neutrons—unless of course they are put there specifically for that purpose in the form of control rods. A secondary fluid which changes phase (e.g. boiling water) undergoes no temperature drop as it condenses in the heat exchanger and would enable the highest possible saturation temperature to be used for the steam cycle. But it carries the risk of 'burnour of the reactor fuel elements (see section 22.8.2) and it requires from the designer a precise knowledge of boiling heat transfer which until recently has been lacking. A further difficulty which arises with a boiling fluid in a reactor derives from the fact that the nuclear reactions in the fuel elements are appreciably affected by the ratio of vapour to liquid surrounding the elements, and very close control of the boiling process is essential. One attraction of using boiling heat transfer to steam is that the secondary fluid circuit can be dispensed with by passing the steam directly into the turbine, although care has to be taken to avoid steam leakage from any part of the circuit because it may be contaminated with radioactivity. Nothing very final can be said about the best choice of cycle, because reactor materials and metallurgical limits are still changing rapidly. With gas cooling, British practice has been to use a dualpressure cycle, a simplified version of which is shown in Fig. 11.23. It is seen to incorporate regenerative feed heating to improve cycle efficiency, and other refinements (not shown) are mainly concerned with the reduction of moisture by reheating, moisture extraction or some method of steam drying. Comparing Figs 11.22a and 11.23b, it can be seen that the dualpressure cycle improves the cycle efficiency by reducing the average temperature difference between the secondary fluid and steam, or in other words by increasing the average temperature at which heat is supplied to the working fluid in the cycle. Further information on steam cycles for nuclear power plant can be found in Ref. 35. 233
[11.8]
Applications to Particular Fluids
11.8 Backpressure and extraction turbines, and cogeneration
In many industrial processes, as well as in central heating, heat has to be supplied at a moderately low temperature. A common method of supplying such heat is to evaporate water at the appropriate temperature and pressure, transfer the heat to the process fluid by condensing the steam in a heat exchanger, and then return the condensate to the boiler. This is illustrated in Fig. 11.24. In all such plant, coal, oil or gas is used as the source of energy, and the energy is made available at a temperature far in excess of that of the process steam. To adopt such a scheme is very wasteful from the thermodynamic point of view, because the large temperature difference between the products of combustion and the process steam is not used to produce work. In most industries requiring process heat, electrical or mechanical power is required at the same time. It is more economical, therefore, to utilise the temperature difference between the metallurgical limit and the process steam temperature for the production of work, and obtain the process heat from the heat rejected in the steam condenser. Such a plant is illustrated in Fig. 11.25. A turbine exhausting into a condenser at a relatively high pressure, in which the rejected heat is employed usefully, is called a backpressure turbine. It is clear that, apart from the thermodynamic economy achieved in combining the power and heating plant, the capital cost is also reduced. A single boiler serves two purposes, and the usual condenser of the power plant becomes superfluous as it is replaced by the process heat exchanger. The use of a backpressure turbine is practical if the power and heat requirements are fairly steady and well matched. When the power requirements are larger than those that can be obtained from a simple backpressure turbine,
Fig. 11.24
T
A simple heating plant
QI2
Process heat exchanger
Q21
T
Fig. 11.25 WS6
A backpressure turbine plant
Backpressure turbine
Q23 12 4 .
6 temperature
Q14
61
Q45
1— 2
234
()
Process heat exchanger
—29 °C
Vapour Power Cycles
[11.8] Fig. 11.26 A passout or extraction turbine plant
an extraction or passout turbine can be used. In this alternative scheme some of the steam is expanded to the lowest possible temperature of about 29 °C, the remainder being extracted from the turbine at the correct intermediate temperature (Fig. 11.26). The extracted steam is condensed in the process heat exchanger and finally returned to the boiler. This scheme enables variations in power and heat requirements to be at least partly accommodated by controlling the amount of extracted steam. Schemes involving the combined production of heat and power are variously known as CHP plant, cogeneration plant, or total energy plant. Some at least of the heat requirement is seasonal, e.g. the part concerned with building heating, and it is not always easy to match the heat and power demands. The economic viability of CHP plant for industry often rests upon the financial terms under which excess power can be sold to the country's electricity network, or the price at which the network is prepared to sell shortfalls to the industry. In the past, developments in this area were often inhibited by satutory regulations or legislation designed to protect existing technologies. With the new emphasis on energy conservation, both for economic reasons and because of increasing concern with environmental damage (atmospheric pollution, acid rain, greenhouse effect etc.), serious consideration is being given to the use of backpressure or passout turbines in large power stations located near cities. The rejected heat would be conveyed to buildings by hot water mains. Inevitably some electricity production capacity is lost and must be made up from other power stations in the generating network. A useful criterion of performance is provided by a ratio 0 given by 0=
heat produced for district heating extra heat used in network to replace lost electricity
The denominator could be evaluated on the basis of the average efficiency of baseload power stations in the network. The ratio 0 might be termed the thermal advantage and is a crude measure of the saving in fuel consumption. Up to now, when capital and maintenance costs are included, the economic advantage over heating appliances in individual buildings has been marginally against such schemes in the UK. The saving in fuel consumption and reduction in environmental damage, however, would be very considerable: see Ref. 38 for an example. 235
[11.8]
Applications to Particular Fluids
Example 11.7
The lowpressure turbine of a power station is to be replaced by a passout turbine so that heat can be supplied to a town. Two schemes are considered, illustrated in Fig. 11.27. In both cases the inlet conditions for the turbine are 11 bar and 560 °C, and the condenser pressure is 0.04 bar. The isentropic efficiency of the turbine expansion can be taken as 0.90, and 1 11 bar
Fig. 11.27
T
Cogeneration plant for district heating scheme
• Pressurised In hot water
m2 (h2 — h7 ) = 100 MW
(a) 100 °C
50 °C
ii12(h2 hg2) = 12.9 MW
ni2(ho — h7) = th (hfiao — him) = 87.1 MW 16.2 (til2h7)
103.3 116.2 (th2hg2) (til2h2)
H/[MW]
tit2(h2 — h7 ) = 50 MW
ma(ha — h6) = 50 MW
T
2
3
6 50 °C
62 (th3h6)
75 °C
.
7
100 °C
In7
Te (b)
g3
3
p
P
m.,
52.5 r56 2  8.1 (dr3hga) (th .h3) (th2/17) 3 H/[MW]
51.6 58.1 (rii2h,2)(412h2
Vapour Power Cycles
[11.8]
the average baseload power station efficiency is nbi = 0.36. Heat at the rate of 100 MW is to be provided to pressurised water circulating to dwellings in the town. Compare the thermal advantage 0 of the following schemes: (a) A single bleed point is used at a pressure which provides steam with a saturation temperature of 100 °C for the district heating. ( b) The districtheating hot water is to be heated in two stages, with half the heat provided by steam bled as in scheme ( a ), and half by steam bled at a pressure corresponding to a saturation temperature of 75 °C. In both schemes the bled steam is condensed without subcooling before being returned to the boiler. The effect of feed pump work can be neglected. Sketch the processes undergone by the Steam and hot water on a T—H diagram and determine the minimum rate of flow of hot water in each of the schemes, assuming that the return temperature of the water for both schemes is 50 °C and that the water enthalpy increases linearly with temperature. Finally, calculate the temperature of the pressurised water leaving the plant in each case. From the steam h—s chart, assuming a straight line of condition (see sections 11.5 and 19.2.5), h 3 = 2825 kJ/kg,
h2 = 3010 kJ/kg,
h4 = 2498 kJ/kg
and from tables, 116 = 314 kJ/kg,
11, = 419 kJ/kg
Let rh, be the passout steam at p2 = 1.013 25 bar, and rib be the passout steam at p3 = 0.3855 bar.
Thermal advantages For scheme (a), the heat transfer to pressurised hot water is
= 1112(h2  117),
th 2 —
100 000 (3010 — 419)
— 38.60 kg/s
The loss of electric power is 4W = th2 (h 2 — /14 ) Hence =
°
A W/11,,
—
(3010 — 419)
— 1.822
(3010 — 2498)/0.36
For scheme (b), for equal contributions of heat to the pressurised water, th e =
th 3 =
ZQ
50 000
(h 2 — /17 )
(3010 — 419)
/0
50 000
(113 — h6 )
(2825 — 314)
= 19.30 kg/s
= 19.91 kg/s
237
[11.8]
Applications to Particular Fluids
A147 = rh2(h2 — h4) + rh3(h3 — h4) = 19.30(3010 — 2498) + 19.91(2825 — 2498) = 9882 + 6511 = 16 393 kW —
100 000 — 2.196 16 393/0.36
Flow rates Fig. 11.27a shows the T—H diagram for scheme (a). The enthalpy values on the abscissa are the products of the specific enthalpies of the steam, and its flow rate th2 determined by the 100 MW heat specification. The minimum water flow rate ritw is prescribed by the line starting at the return temperature of 50 °C which just touches the pinch point P2: lower flows imply a water temperature which lies above P2 , and heat then cannot flow from the steam to the water. Hence (thw)min
87 100 [kW] 87 100[kW] of — hf5 ) (419 — 209)[kJ/kg] f
415 kg/s
Fig. 11.27b shows the TFI diagram for scheme (b). It is not immediately obvious whether the value (thw)min should be deduced from the water T11 line when it just touches P2 or P3 . We shall assume that the minimum flow is governed by P2. Let us check that, with this assumption, the water temperature Tp falls below P3. As the water T—H line is straight, Tp/[°C] — 50 (52.5 — 6.2)
100 — 50 (51.6 — 8.1) + (56.2 — 6.2)
and hence Tp = 74.8 °C, i.e. just below the temperature of the steam of 75 °C at P3 . The reader can easily verify that if we were to make Tp = 75 °C, the water temperature at P2 would lie slightly above 100 °C, namely at 100.6 °C. We can now calculate (rh,„,),,,in for scheme (b). With the water T—H line just touching P2 , (mw)min
{(56.2 — 6.2) + (51.6 — 8.1)) 103[kW] = 445.2 kg/s (419 — 209)[kJ/kg]
In practice, a design will specify a temperature difference of several degrees at all the pinch points, and the values of (riOrnin calculated here are limiting values only.
Exit temperatures The exit temperature Te for the pressurised water for scheme (a) will be given by Te/[°C] — 50 100 — 50 and hence Te = 107.4 °C. 238
100 103.3 — 16.2
[11.9]
Vapour Power Cycles
For scheme (b), Te will be given by Te /[°C] — 50 100 — 50
50 + 50 (56.2 — 6.2) + (51.6 — 8.1)
and hence Te = 103.5 °C. We have seen that of the two schemes in Example 11.7, scheme (b) is better from the thermodynamic point of view. This is not surprising because the average temperature difference between steam and water is less in scheme (b), and hence the effect of this cause of irreversibility is lower. The transfer of heat in the two schemes is typical of the kind of situations encountered in the process industries, where it is also important to optimise the thermodynamic performance of plant by reducing temperature differences in heat transfer. When one fluid changes phase, an attempt to reduce temperature difference may lead to the kind of pinch point problem outlined in the foregoing example, namely the danger of wasting heat exchanger area by not completing the desired heat transfer process. Once the temperature difference drops to zero in a heat exchanger, all heat transfer ceases. It is relatively easy to avoid this situation arising under design point conditions as we have seen, but in practice it is essential to see that it cannot happen under offdesign, or partload, operating conditions also. This can be done by what is called pinch point analysis, which is described in Refs 41 and 42. Such an analysis is also used to optimise the thermodynamic performance of complex multistream process plant by so arranging heat exchanges between the streams that a minimum of heat is required from an external source. In essence one is trying to minimise the effect of irreversibilities due to temperature differences. Although we have chosen to introduce the idea of cogeneration schemes in this chapter, and hence their realisation via steam turbine driven plant, it should be appreciated that the waste heat from any combustion power plant can be used for such schemes. Any smallscale CHP plant for an individual factory, hospital complex, or large leisure centre with swimming pool and ice rink, is more likely to use an electric generator driven by a reciprocating internalcombustion engine or gas turbine. In such applications the lowgrade heat and electrical power requirements are often roughly constant through the year and in a ratio suited to these power plants. A few simple case studies with economic assessment can be found in Ref. 42. 11.9 Lowtemperature power cycles
Much of this chapter has been concerned with various modifications to the simple Rankine cycle to make the best possible use of energy sources which are at a high temperature. In this section we will consider vapour power plant for electricity generation which make use of lowtemperature sources such as waste heat from a factory process, hot water from a geothermal reservoir, or solar radiation absorbed in a shallow lake or 'solar pond'. Because of the small temperature drop available, only the simple Rankine cycle can be used and the 239
[Ma)
Applications to Particular Fluids 0.701 bar (H20) 32.4 bar (R134a)
Fig. 11.28 2
Comparative performance
Condenser
of lowtemperature cycles with alternative working
T 90°C
o cooling tower
fluids
0.0234 bar (H20) 5.72 bar (R134a)
From lowtemp. source
Working
x2
n
fluid Steam R134a
0.877 0.934
0.164 0.140
in
vg,
V,
V,
V2
Boiler duty
Condenser duty
[kg/s]
[m3/kg]
[m3/s]
[m3/s]
Tii
[MW]
[MW]
2.36 36.0
2.361 0.00462
5.58 0.166
120 1.21
21.5 7.29
6.08 7.13
5.08 6.13
cycle efficiency will be low. This is not serious, however, because the 'fuel' is free. The cost of electricity generated by such plant will depend on the capital cost, the effective life of the plant (i.e. the period over which the capital cost must be written off), and the maintenance cost. A low efficiency does imply large components for a given power output, and hence inevitably a high capital cost. As might be expected, the type of working fluid used in refrigerators and heat pumps (see section 13.2) is much more suitable than steam for lowtemperature power plant. The main reason, as we will see, is that the specific volume of such vapours at low temperature is much less than that of steam, with the consequence that the turbine can be much smaller and less expensive. Turbogenerator units, sealed to avoid loss of working fluid, and suitable for use with a variety of lowtemperature sources, are available in modules of up to 1 MW of electrical output. To illustrate the significance of the specific volume of the vapour, the cycle in Fig. 11.28 has been evaluated for two working fluids—steam and Refrigerant 134a (or R134a). The turbine output is 1 MW in each case. A turbine isentropic efficiency of 90 per cent was assumed, the feed pump term was neglected, and the fluid properties were taken from Ref. 17. The salient results are given in the table incorporated in Fig. 11.28. The main points to be noted, where the R134a has the advantage over steam, are as follows: (a) The dryness fraction at outlet from the turbine is appreciably higher (0.934 versus 0.877), so that there should be no serious problems arising from droplets impinging on the turbine blades (discussed at the end of section 19.2.4). (b) Although a much higher mass flow is required for the given power output (36.0 kg/s versus 2.36 kg/s), this is not significant. The specific volume of R134a vapour is so much less than that of steam that the volume flow rates % and V2, upon which the size of the turbine depends, are some 30 and 100
240
Vapour Power Cycles
[11.9]
times smaller. Moreover, the ratio of the outlet to inlet volume flows is also very much less (7.29 versus 21.5). This means that all the design problems arising from the need to accomodate the vast volume flow at the lowpressure end of steam turbines are avoided (see section 19.2). (c) From the pressures shown on the T—s diagram, it is clear that the pressure in the R134a plant is nowhere less than atmospheric. There are no problems associated with the vacuum that is required in steam condensers, as discussed in sections 14.4 and 22.8.1. The only points at which steam seems to have the advantage over R134a are as follows: (a) The efficiency of the R134a cycle is lower — but we have already pointed out that this is not directly of importance when the 'fuel' is free. (b) An indirect effect of the lower efficiency is a larger boiler duty (I 14/ 1 /q) and condenser duty (114/1/r/ + I W I). Whether the boiler and condenser would actually be larger for the R134a plant depends on the relative heat transfer characteristics of the vaporising liquids and condensing vapours (see section 22.8). Before leaving the subject of lowtemperature vapour cycles, it is worth mentioning one particular scheme which makes use of a source which is virtually at atmospheric temperature—namely the ocean. We refer to what is called an ocean thermal energy conversion (OTEC) plant, which makes use of the temperature difference existing between the surface of the ocean and its deeper levels. In certain tropical locations, a temperature difference of about 20 K is available without having to use water from a depth much over 300 m. Fig. 11.29 includes a diagrammatic representation of such a plant, showing typical values of inlet and outlet temperatures of the sea water: 28 °C and 26 °C for the boiler, and 7 °C and 10 °C for the condenser. Assuming minimum temperature differences of 2 K between sea water and working fluid, the maximum and minimum temperatures of the Rankine cycle will be 24 °C and 12 °C, as indicated on the T—H diagram. This time taking the working fluid to be ammonia, again using the properties given in Ref. 17, and assuming turbine and feed pump isentropic efficiencies of 90 per cent, the cycle efficiency is readily found to be 0.0354. With such a very low efficiency it is not surprising that the plant turns out to be extremely large. Thus for a plant of 100 MW turbine output, the boiler and condenser heat capacities would be 01 =
114/1
=
100 = 2825 MW and 1021 = (01 + W) = 2725 MW 0.0354
The capacities of the corresponding components of a fossilfuel steam power plant of 0.40 cycle efficiency would be 250 MW and 150 MW. Thus for the same work output, the OTEC boiler and condenser would be about 11 times and 18 times larger than thecorresponding components in conventional plant. It is not surprising that OTEC plant turn out to have a high capital cost. As discussed in section 11.8 and illustrated in Example 11.7, we have plotted the ammonia cycle, and the processes undergone by the warm and cold sea 241
Applications to Particular Fluids
[11.9]
Fig. 11.29 An ocean thermal energy
T
Floating platform Turbine
conversion (OTEC) plant
Warm water 4
3
%Mr Warm water pump
10°C
5
28 °C Condenser Boiler 111/1
300 m 26°C
Feed pump
Cold water
T
24°C
26 °C
2K 2'
Cold water pump
til A
5'
28°C 4
51 •
— 2K 7°C' c ±L1 thc " 100 x 0.012 85 x 30 — 0.285 kg/min Its T— 0.462 x 293
Similarly, the mass of air is
(p — p.3)1.,
100(1.0 — 0.012 85)30 = 35.22 kg/min Ra T 0.287 x 293
me3
The heat transferred in the heater is therefore 023 = {35.22 x 1.005(20 — 10.7)}
+ {0.285 x 1.86(20 — 10.7)} = 329.2 + 4.9 = 334.1 kJ/min To find the heat 012 transferred in the cooler, the energy equation is applied to the open system bounded by planes 124. Thus 12 = (tha2ha2
ths2ha2
thw4hw4)
(tha 1 hal + rhs1 hsl)
This equation can be rearranged, remembering from conservation of mass that /1%3 = Ma2 = ma l = rha and di., = ths2 + mw4, to give either 012 = Thaepa(
— T1)
(rhs2hs2
thvi4hw4
thsl hal)
(a)
Or
012 = rhac,,,(T2 — T1) + ths2 c„,(T2 — T1) + rh,,4 (hw4 — hat) — 141 (b) Now ph. = 35.22 kg/min, ths2 = rho = 0.285 kg/min. rh,1 can be found from the inlet state. Thus Pal
=
41 PQ1 = 0.90 x 0.05629 = 0.05066 bar
The inlet specific humidity, from equation (14.25), is = 0.622
Pe i Pi — Pal
—
0.622 0.050 66 1.0 — 0.050 66
= 0.0332 kg steam/kg dry air 314
Properties of Mixtures
[14.5]
and hence msl = w i rris = 0.0332 x 35.22 = 1.169 kg/min mw4 = rh„ — ths2 = 1.169 — 0.285 = 0.884 kg/min is The apparent advantage of using the second expression (b) for that the enthalpy term involving »7,2 can be easily calculated from the perfect gas approximation for steam (as was indeed done when calculating Q23). But when some of the steam or water changes phase in the process, there is very little saving in labour and the use of expression (a) reduces the chance of errors from algebraic manipulation. All enthalpies must then be calculated relative to the triple point datum of the steam tables. This approach will be adopted here. The temperature of the condensed vapour will be equal to T2, and hence h,,v4 = 44.9 kJ/kg from the h f column of the saturation table. The enthalpy hs2 = (hg at 10.7 °C) = 2519.8 kJ/kg. The enthalpy h,1 can be found from hsi = (hg at Psi) + cps(71 — 7; at Psi) = 2561.3 + 1.86(35 — 33.1) = 2565 kJ/kg Alternatively, h51 can be found interpolating along any lowpressure line in the superheat table, because h is almost independent of p. Choosing the closest pressure to psi , namely 0.05 bar, h51 = 2561 +
35 — 32.9 (2594 — 2561) = 2565 kJ/kg 50 — 32.9
The energy equation for the cooler therefore becomes 0012 = 35.22 x 1.005(10.7 — 35) + {(0.285 x 2519.8) + (0.884 x 44.9) — (1.169 x 2565)) — 1.1 x 60 = — 3166 kJ/min Here again, as we noted at the end of our analysis of condensers, the thermodynamic analysis only enables the required rates of heat transfer to be found. Further information is required before the necessary size of the cooling and heating coils can be determined. To reduce the quantities of heat involved, and therefore the size of the heat transfer surfaces, and yet maintain the freshness in the room, it is usual to draw about onethird of the total air supply from the atmosphere and to recirculate the remainder from the rooms (see Fig. 14.8). 14.5.2 Cooling towers Steam power stations, refrigerating plant and many other industrial processes require large quantities of cooling water. If the plant is not situated near a natural source such as a river, it is necessary to cool the water after use and recirculate it. One of the most effective methods is to use the principle of evaporative cooling in a cooling tower. The warm water is sprayed into the tower near the top and allowed to fall through a packing of slats which break 315
Applications to Particular Fluids Fig. 14.11 Induceddraught cooling tower
[14.5]
Hot water 0090171791717
Packing
L.
_J Air
Cold wan.
up the stream and provide a large wetted surface to facilitate evaporation. A current of air passes up the tower, either naturally as in a chimney, or induced by a fan as shown in Fig. 14.11. The warm water is cooled, mainly by evaporation, while the air is raised in temperature and saturated, or nearly saturated, with water vapour. The water may be cooled to a temperature below that of the air entering the tower—ideally to the wetbulb temperature of the air. The rate of cooling falls off as this equilibrium condition is approached, and the increase in height of tower which would be required to obtain the last possible few degrees of cooling is uneconomic. Generally, the tower is designed for the outlet water temperature to be about 8 K greater than the wetbulb temperature of the atmosphere. The cooling towers described above are a form of directcontact heat exchanger. The advantages of this type over the conventional one, where the two fluids are separated by a solid wall, are twofold: first, the heat exchanger can be much smaller; and secondly, the water can be cooled to a lower temperature. (It can be cooled to within only a few degrees of the drybulb temperature in the conventional type.) The disadvantages are also twofold. First, some of the cooling water is lost by evaporation and has to be replaced continuously by expensively treated fresh water. Secondly, a group of large cooling towers can have an undesirable effect on the local environment. The vapour condenses above the towers and, if it is not cooled sufficiently rapidly, clouds can be formed some distance away which throw dense shadows over agricultural crops. These disadvantages have lgd to the development of the socalled hybrid tower in which initial cooling is performed in a conventional heat exchanger, followed by evaporative cooling towards the wetbulb temperature in a directcontact heat exchanger. For an introduction to the theory of design of cooling towers, and further references, the reader may turn to Refs 16 and 11. The design is a problem in both heat and mass transfer from droplets and liquid films, and the detailed analysis to determine the volume of packing required for a given cooling duty is outside the scope of this book. 316
Properties of Mixtures
[14.5]
Example 14.10
Air enters the base of a naturaldraught cooling tower at the rate of 1100 m3 / min with a pressure of 1 bar, a temperature of 15°C, and a relative humidity of 65 per cent. The water enters the tower at 38°C and leaves at 17 °C. If the air leaves the tower at 32°C in a saturated condition, find the mass flow of water entering the tower and the percentage loss of water by evaporation. Fig. 14.12 illustrates the system. At the air inlet section 1 we have
Psi = 49 IPg l = 0.65 x 0.017 04 = 0.01108 bar —
psi 1.1
R8 T
—
100 x 0.011 08 x 1100 0.462 x 288
— 9.16 kg/min
(p — psi )1/
100(1.0 — 0.011 08)1100
Ra T
0.287 x 288
rhai =
= 1316 kg/min
At the air outlet section 2 we have Ps2 = Pg2 = 0.047 54 bar co2 = 0.622 Since
Ps2
0.622 x 0.047 54
p — ps2 (1.0 — 0.047 54)
— 0.031 05
a2 = mal, rhs2 = W2tha 1 = 0.03105 x 1316 = 40.86 kg/min
Water is lost by evaporation at the rate of rris2 — rrisi = 40.86 — 9.16 = 31.7 kg/min Neglecting changes of kinetic energy and heat loss from the tower to atmosphere, the energy equation is (riza2 ha2 ths2hs2 thw4hw4) — (the I hal + 641 hal thw3 hw3) = Or in more convenient form, rhacpa( T2 —
His hs
+ (rhs2
(thwahwa thw3hw3) = 0
1 bar 32 °C = 100%
Fig. 14.12 Naturaldraught cooling tower
3 38 °C 1000 m3/min 1 bar 15 °C = 65% 17 °C
317
[14.5]
Applications to Particular Fluids
From conservation of mass, met
mw4 =
64;3 and hence mw4 = mw3 — 31.7 kg/min
From the saturation table, since To at po. is 8.48 °C, 141 = ho + cps(TI — T) = 2516 + 1.86(15 — 8.48) = 2528 kJ/kg and k2 = ho = 2559.3 kJ/kg,
h,„,3 = 143 = 159.1 kJ/kg
14,,4 = /114 = 71.3 kJ/kg Finally, taking cp„ = 1.005 kJ/kg K, we get 1316 x 1.005(32 — 15) + {(40.86 x 2559) — (9.16 x 2528)} + {(rk,3 — 31.7)71.3 — thw3 159.1} = 0 The water flow at inlet thw3 is consequently 1160 kg/min. The percentage loss by evaporation is 1142 62'1
100 = 2.7 per cent
thw3 14.6 Hygrometric chart Calculations involved in the type of problem considered in section 14.5 can be considerably simplified if use is made of the hygrometric chart, Fig. 14.13. This chart enables the enthalpy of humid atmospheric air, of any relative humidity, Fig. 14.13 The hygrometric chart
0
318
10
20 30 Drybulb temperature/[°C]
40
Properties of Mixtures
[14.5]
to be read off directly. The enthalpy of the mixture is expressed as kJ per kg of dry air in the mixture. If this quantity is denoted by H, then H = ha + whs Although he is fixed solely by the temperature of the air (drybulb temperature T), the value of coh, depends upon the specific humidity and both the pressure and the temperature of the air. Thus equation (14.25) indicates that when w and p are known, the partial pressure of the vapour ps is determined. If in addition the temperature T is known, then hs is fixed. The chart is drawn for a fixed barometric pressure so that w and T can be regarded as the only independent variables. These form the ordinate and abscissa scales respectively, and lines of constant enthalpy H are plotted on the diagram. Equation (14.29) shows that, for a given barometric pressure, the relative humidity 4) is a function of w, ps and p8. p, is the saturation pressure corresponding to the drybulb temperature T, and we have already seen that ps is a function of w for a fixed barometric pressure. It follows that 4) is also a function of w and T, and therefore lines of constant relative humidity can be added to the diagram. Since humidity measurements are so often made in terms of wet and drybulb temperatures, lines of constant wetbulb temperature are also included. Note that the wetbulb temperature at any state along the saturation line (49 = 100 per cent) is equal to the drybulb temperature, and also the dew point, at that state. Lines of constant dew point are horizontal because they are also lines of constant specific humidity. The constant wetbulb temperature lines slope down towards the right of the diagram and follow very closely the lines of constant enthalpy. Finally, lines of constant specific volume va of the dry air in the mixture are usually included. v„ is a function of the drybulb temperature T and the partial pressure of the air (p — ps). But we have seen that ps is a function of 0) and p, and so, for a given barometric pressure p, va is a function of T and o). The way in which the hygrometric chart can be used to simplify the solution of a problem will be indicated briefly by referring to the airconditioning plant of Fig. 14.10. The process undergone by the mixture can be represented as in Fig. 14.14, points 1 and 3 being located from the given values of T and 4) at the inlet and outlet of the system. The temperature T2 to which the air must Fig. 14.14 Use of hygrometric chart
co,
co2 = (03 V.3 20 35 Drybulb temperature/[°C]
319
[14.5]
Applications to Particular Fluids
be cooled can be read directly from the chart. Before applying the energy equation, the next step must be to find the mass flow of dry air because all the `specific' quantities on the chart refer to unit mass of dry air. Thus va3 is read from the chart, and hence rha can be found from V3/va3, where V3 is the volume flow of mixture delivered. The energy equation for the heating process, i.e. between planes 2 and 3 in Fig. 14.10, can be written in the convenient form 023 = rha(H3 — H2)
since the values of H are in kJ/kg of dry air in the mixture, and ma does not change between planes 2 and 3. Both H3 and H2 can be read from the chart, and so Q23 can be determined directly. Similarly, the energy equation for the cooling and condensing process can be written as 012 = ►ha(H2 — H 1 )
tilw4hw4 — 141
and H1 can be read from the chart, 141 is given, and hw4 can be found from the saturation table in the usual way; it remains to find mw4. For conservation of mass, H2
= ths2 rhw4
or rh" = rha(o), — w2)
Both col and w2 can be read from the chart, and therefore rh„ and thence Q12 can be rapidly calculated. Although a hygrometric chart is drawn for a particular barometric pressure, it can be used without much loss of accuracy for any reasonable variation in this pressure. For example, the chart of Ref. 6 is drawn for a pressure of 1 atm, but it can be used without sensible error between 0.9 and 1.1 bar. All the information conveyed by the chart can also be obtained in the form of tables such as those of Ref. 29.
320,
15 Combustion Processes
Previous chapters have been wholly concerned with the behaviour of fluids which remain in the same chemical state throughout the processes considered. Here we shall deal with the thermodynamic aspects of a particular type of process involving chemical reactions, namely combustion. The term 'combustion' refers to the fairly rapid reaction, usually accompanied by a flame, which occurs between a fuel and an oxygen carrier such as air. The molecules of fuel and air have a certain amount of energy stored in the bonds between their constituent atoms, a form of internal energy which we have not had to consider hitherto because it remains constant for all processes not involving chemical reactions. In the new molecules formed by a reaction this 'chemical' energy is at a lower level, and the energy thus released can be transferred to the surroundings in the form of heat. Combustion is therefore said to be an exothermic reaction. After the relevant combustion equations which relate the masses of reactants and products are discussed, methods of applying the energy equation to the combustion process are examined and the efficiency of such a process is defined. The idea of a reversible combustion process is introduced, and a method of estimating the effect of dissociation is described. Many properties required for the analysis of chemical reactions cannot be measured directly and have to be derived from others. The interrelation between the various properties, the method of their tabulation, and tests for selfconsistency are discussed. Some important aspects of combustion cannot be handled by thermodynamic reasoning alone; the rate at which a reaction proceeds and the stability of flames are two examples of great importance in the design of internal combustion engines. The chapter concludes with a brief discussion of the limitations of thermodynamic analysis.
15.1 Fuels Most common fossil fuels consist mainly of hydrogen and carbon, whether the fuel be solid (e.g. coal), liquid (e.g. petroleum) or gaseous (e.g. natural gas). We 321
[15.1 ]
Applications to Particular Fluids Fig. 15.1 Typical ultimate analyses of coals
Coal Anthracite Bituminous Lignite
C
H
0
90.27 74.00 56.52
3.00 5.98 5.72
2.32 13.01 31.89
N+ S
Ash
1.44 2.26 1.62
2.97 4.75 4.25
shall assume that the chemical analysis of the fuel is known.* For solid and liquid fuels the analysis is usually quoted as a percentage by mass of each chemical element in the fuel; it is termed an ultimate analysis. The analysis of a gaseous fuel, on the other hand, is usually given in terms of the percentage by volume of each gas or type of hydrocarbon present. In coal, the combustible elements are chiefly carbon (C) and hydrogen (H) with a minor quantity of sulphur (S); the incombustibles are nitrogen (N), moisture (H2 0) and small quantities of minerals which form the ash after combustion. Typical ultimate analyses of the three main types of coalanthracite, bituminous coal and ligniteare given in Fig. 15.1. Since there are numerous varieties of each type of coal, the figures can only serve as a rough guide. Moreover the analyses refer to dry coals; the moisture content is as low as 1 per cent in anthracite, varies from 2 to 10 per cent in the bituminous coals, and is as high as 15 per cent in lignite. Petroleum oils are complex mixtures of a large number of different hydrocarbons. These hydrocarbons have been classified into groups, the most common being paraffins (having a molecular formula of the form C„H 2„,2 ), olefins and naphthenes (C„1/2,,)t and aromatics (typically Cr,H2,, _ 6 ). Although analysis in terms of actual compounds is difficult and sometimes impossible, the ultimate analysis is a simple matter and Fig. 15.2 gives typical examples. The analyses are very similar and the choice of fuel for a particular application depends mainly on other characteristics such as viscosity, ignition temperature, knocking tendency (in petrol engines), coking tendency (in gas turbines) and so on. Most hydrocarbons in petroleum deposits occur naturally as a liquid, but a few exist in the gaseous phase at atmospheric temperature. At present, North Sea gas fields meet most of the UK's commercial and domestic needs for gaseous fuel. Methane (a paraffin, CH,), known as 'marsh gas' and 'firedamp' when occurring naturally, is produced, by the decay of organic matter. Sewage works Motor petrol
Fig. 15.2 Typical ultimate analyses of petroleum oils
C
H S
85.5 14.4 0.1
Vaporising oil Kerosene 86.8 12.9 0.3
86.3 13.6 0.1
Diesel oil (gas oil)
Light fuel oil
Heavy fuel oil
86.3 12.8 0.9
86.2 12.4 1.4
86.1 11.8 2.1
* See Ref. 19 for complete data on typical fuels. t Although olefins and naphthenes have the same C/H ratio, they are distinguished by an important difference in molecular structure.
322
Combustion Processes
[15.2] Fig. 15.3 Typical volumetric analyses of gaseous fuels
Coal gas Producer gas Blast furnace North Sea gas
H2
CO
`CH4'
49.4 12.0 2.0
18.0 29.0 27.0
20.0 2.6
C4H8 2.0 C2 H4 0.4
93.0
C2 H6 4.8
02
N2
CO2
0.4
6.2 52.0 60.0 2.0
4.0 4.0 11.0 0.2
and biodigesters on farms can supply methane for local use as a supplementary fuel. Prior to the Second World War, the most widely used gaseous fuels were formed by heating coal in various ways. Typical compositions of three forms—coal (or town) gas, producer gas, and blast furnace gas—are given in Fig. 15.3, with that of North Sea gas for comparison. Hydrogen and carbon monoxide are easily isolated, but the various hydrocarbons are usually grouped into two types representing respectively an average composition of the paraffins in the gas (assumed to have the formula CH4) and an average of the remainder (C„H,,,). In the following sections concerned with typical combustion calculations, we shall neglect the effect of minor elements, such as sulphur, in the fuel. Although for the purpose of setting out mass and energy balances this is permissible, it should not be thought that the presence of a small quantity of a substance is always unimportant. Thus sulphur in fossil fuels is the principal cause of 'acid rain'. Less well known are the effects of such impurities as sodium and vanadium. These produce corrosive compounds which attack engine components. Vanadium compounds, for example, break down the protective oxide layer on turbine blades and effectively prevent the use of the cheaper oils as fuel for gas turbines. The presence (or absence) of an impurity may well determine the choice of fuel for a particular application. 15.2 Chemical equations and conservation of mass
The first step in the description of a combustion process is the formulation of the chemical equation which shows how the atoms of the reactants are rearranged to form the products. Before the chemical equation can be written it is necessary to know the number of atoms of each element in the molecules of the reactants and products. In any purely chemical, as opposed to nuclear, reaction the process is simply one of rearrangement of the atoms to form new molecules, and the total number of atoms of each element is unchanged. A chemical equation expresses the principle of the conservation of mass in terms of the conservation of atoms. Consider the simple chemical equation expressing the complete combustion of carbon and oxygen to carbon dioxide: C+
02 4
CO2
(15.1)
This equation states that one atom of carbon will combine with one molecule of oxygen (2 atoms of 0) to produce one molecule of carbon dioxide (1 atom 323
Applications to Particular Fluids
[15.2]
of C + 2 atoms of 0). The number of atoms of each element is the same on either side of the equation, and the arrow represents the direction of the reaction. Equation (15.1) can also represent the amountofsubstance involved in the reaction and be written as 1 kmol C + 1 kmol 02 1 kmol CO2
(15.2)
Since the molar masses of the substances are numerically equal to the relative atomic or molecular masses,* equation (15.2) can be converted into a mass equation as follows: (15.3) 12 kg C + 32 kg 02 —> 44 kg CO2 Now all gases occupy equal volumes per kmol when reduced to the same pressure and temperature. Although this is strictly true only for perfect gases, it is substantially true for all gases and dry vapours at moderate pressures. If any of the reactants or products are in the solid or liquid phase, the volume occupied by them can be neglected in comparison with the volume of the gases present. It follows that equation (15.2) is also equivalent to 0 vol. C + 1 vol. 02 —> 1 vol. CO2
(15.4)
Equation (15.4) implies that the volume of the products is equal to the volume of the reactants, when measured at the same pressure and temperature. If insufficient oxygen is present for all the carbon to burn to carbon dioxide, some will burn to carbon monoxide. The reaction is then symbolised by C + 102 CO
(15.5)
Carbon monoxide can be subsequently burnt to carbon dioxide, the appropriate equation being CO + 102 —> CO2
(15.6)
It is for this reason that the combustion of carbon to carbon monoxide is said to be 'incomplete', and to carbon dioxide 'complete'. Equations similar to (15.1) to (15.4) can be written for the combustion of hydrogen, the other main constituent of a hydrocarbon fuel: H2 4 '102 4 H2 0 1 kmol H2 + 2 kmol 02 1 kmol H2 0 2 kg I12 + 16 kg 02 —* 18 kg H2 O 1 vol. H2 + 2 vol. 02 9 1 vol. H2 O (yap) 0 vol. H2 O (liq)
(15.7)
* For a discussion of the relation between amountofsubstance, molar mass and relative atomic or molecular mass, see section 8.5.2. Various 'atomic weight' scales have been used in the past. A chemical scale was fixed when the existence of three isotopes of oxygen of differing mass was not known; it was formed by allotting the number 16 to a 'mean' oxygen atom. This proved unsatisfactory because the proportions of oxygen isotopes vary in nature. When nuclear studies became important a physical scale was adopted in which the number 16 was attached to the most common isotope of oxygen (160). In 1961 a new scale was adopted by both chemists and physicists based on a particular isotope of carbon (' 2 C) which was assigned the value 12. Values on the old chemical scale and new '2 C scale differ only by about 0.004 per cent. For combustion calculations, whole number values (e.g. C 12, 0 16, H 1, N 14) are sufficiently accurate, and thus these changes in the basis of the relative atomic mass scale are insignificant.
324
Combustion Processes
[15.2]
The abbreviation (yap) or (liq) must be included when the phase of a reactant or product is in doubt. In most engineering combustion systems the necessary oxygen is obtained by mixing the fuel with air.* For our purposes it will be sufficiently accurate to use the following figures for the composition of air:
Volumetric analysis % Gravimetric analysis %
02
N2
21 23.3
79 76.7
Here the symbol N is used to denote not only the nitrogen, but all the inert gases present in air which remain unchanged throughout the reaction. The molar mass of N2 can be taken as 28 kg/kmol, and that of air as 29 kg/kmol. (A more precise composition of air is given in Ref. 17.) The following two examples, concerning a liquid and a gaseous fuel respectively, show how chemical equations may be used (a) to predict the analysis of the products of combustion when the composition of the fuel and the air/fuel ratio are known, and (b) to determine the stoichiometric (or correct) air/fuel ratio. A stoichiometric mixture is one in which there is theoretically just sufficient oxygen to burn all the combustible elements in the fuel completely. In practical combustion systems the time available for the reaction is limited and excess air must be provided to ensure complete combustion. This is not only because of imperfect mixing of the fuel and air, but also because the inert gas molecules obstruct the reaction between the active molecules of fuel and oxygen. The analysis of the products of combustion may be quoted on a volume or a mass basis. In either case, if the water vapour is assumed to be present as it is in the hot exhaust gases from an engine, the analysis is called a wet analysis. When the vapour is assumed to be condensed and removed, it is called a dry analysis. Example 15.1
Determine the stoichiometric air/fuel ratio for a petrol approximating to hexane C6 H14. Hence deduce the chemical equation if the petrol is burnt in 20 per cent excess air, and the wet volumetric analysis of the products (a) if all the water vapour is present, and (b) if the products are cooled to an atmospheric pressure and temperature of 1 bar and 15°C. Determine also the dry volumetric analysis. Finally, estimate the chemical equation if only 80 per cent of the air required for stoichiometric combustion is provided. Chemical equation Since the combustion is theoretically complete with a stoichiometric mixture, the products will consist only of CO2, H2 O and the N2 brought in with the air. The amount of oxygen required can be found by first balancing the carbon * The chief exception is the rocket motor, described in section 18.4.2. In this case the necessary oxygen is obtained from liquid oxygen, liquid ozone, or some oxygen carrier such as hydrogen peroxide or nitric acid.
325
[15.2]
Applications to Particular Fluids
and hydrogen atoms on each side of the equation and then summing the number of atoms of oxygen in the products: C61114 + 9102 6CO3 + 7H,0 86 kg C6 H 4 + 304 kg 02 + 264 kg CO2 + 126 kg H2 O Since air contains 23.3 per cent by mass of oxygen, we have stoichiometric air/fuel ratio =
304 x 100 86 x 23.3
— 15.17
If there is 20 per cent excess air, the equation, including the nitrogen, becomes C6 H14 + 1.2{9102 + ( 79 )91N2} 21 6CO2 + 7H2 0 + (0.2)9102 + 1.2I
9 21
)911\12
Wet volumetric analysis (a) The amountofsubstance of the products is 6(CO2 ) + 7(H2 0) + 1.9(0 2 ) + 42.89(N2 ) = 57.79 kmol Now the mole fraction of a constituent equals the volume fraction (equation (14.18)). The wet volumetric analysis if all the water vapour is present is therefore CO2 OZ
6x 100
57.79
= 10.38%;
1.9 x 100 57.79
= 3.29%;
H2 O 7x 10012.11% 57.79 N2
42.89 x 100 — 74.22% 57.79
(b) The partial pressure of saturated water vapour at 15°C is 0.017 04 bar. The mole fraction of the water vapour in the mixture, from equation (14.17), is x5 =
0.017 04 — 0.017 04 1.0
If y is the amountofsubstance of water vapour remaining in the products after cooling, the total amountofsubstance becomes {(57.79 — 7)[kmol] + y}, and therefore y
50.79 [ kmol] + y
— 0.017 04
from which y = 0.88 kmol. The total amountofsubstance of products under these conditions is 51.67 kmol in the vapour state, and the volumetric analysis becomes CO2 11.61%; H2 O 1.70%; 02 3.68%; N2 83.01% 326
Combustion Processes
[15.2]
Dry volumetric analysis
Merely cooling the products does not remove the water vapour entirely. If all the vapour is assumed to be removed, say by a drying agent, the total amount of substance is 50.79 kmol. The dry analysis is CO, 11.81 %; 02 3.74 %;
N2
84.45 %
Chemical equation with insufficient air
When insufficient air is supplied for complete combustion, some of the carbon will burn to carbon monoxide, and there may also be some free hydrogen. Insufficient information is given for the determination of the chemical equation. Hydrogen, however, has a greater affinity for oxygen than has carbon, and if the mixture is not too rich in fuel it is reasonable to assume that all the hydrogen will be burnt.* We can then write, for the rich mixture, 79 C611, 4 + 0.8 {9102 + (21 "2 79 aCO2 + bC0 + 7H2 0 + 0.81— ) 91N2 21 From the carbon balance, 6=a+b From the oxygen balance, 0.8 x 91 = a + b/2 + 7/2 Solving these simultaneous equations, we get a = 2.2 and b = 3.8. The chemical equation is therefore C61114 + 7.602 + 28.6N2 2.2CO2 + 3.8C0 + 7H2 0 + 28.6N2 Example 15.2
A gaseous fuel has the following percentage composition by volume: CO 12.6%;
H 2 41.6%; CH 4 26.6%; 0 2 1.9%;
CO, 2.6%; N 2 14.7% Find the wet volumetric and gravimetric analyses of the products of combustion when 10 per cent excess air is provided.
The solution can be set out in tabular form. The first table determines the oxygen required for stoichiometric combustion, and the amounts of CO2 and H2 O produced thereby, per mole of fuel burnt. Note that the amount of oxygen in the fuel is taken into account when estimating the oxygen required from the air. * An accurate prediction of the products analysis for a mixture lacking sufficient oxygen for complete combustion can only be obtained by the method outlined in section 15.7.2. This makes use of additional information in the form of equilibrium constants for the various reactions.
327
Applications to Particular Fluids
kmol Reactants CO H2 CH4 02 CO2 N2
kmol fuel
02 required
Reaction CO +102 CO2 H2 + 102 ÷ H2O CH4 + 202 > CO2 + 2H2 0
0.126 0.416 0.266 0.019 0.026 0.147
0.063 0.208 0.532 0.019
0.126 — 0.266 — 0.026 —
0.784
0.418
—
1.000
Products H2 O CO2
0.416 0.532
0.948
I
So 0.784 kmol of oxygen is required, per kmol of fuel burnt, for stoichiometric combustion. Since 10 per cent excess air is provided, 0.0784 kmol of oxygen is additionally present and remains unchanged throughout the process. The total amount of nitrogen in the products is 9 1.1 7 )0.784 + 0.147 = 3.392 kmol/kmol of fuel 21 ( The analyses of the products by volume and by mass (see equation (14.23)) are therefore as in the following table:
Products CO2 H2 O 02 N2
kmol kmol fuel (a)
% by volume
0.418 0.948 0.078 3.392
8.6 19.6 1.6 70.2
4.836
100.0
m* [kg/kmol]
kg kmol fuel m x (a)
% by mass
44 18 32 28
18.39 17.06 2.50 94.98
13.8 12.8 1.9 71.5
132.93
100.0
* Note from section 8.5.2 that when measured in kg/kmol (or g/mol), is numerically equal to A, or Mr but is not dimensionless.
15.3 Experimental products analysis
When investigating the effectiveness of combustion plant it is often necessary to analyse the products experimentally. By taking samples at different stages of a reaction the combustion process can be studied, and the analyses can be used to discover lack of uniformity in fuel—air distribution. A products analysis also enables the air/fuel ratio to be computed in cases where direct measurement of the rate of air flow is not easily accomplished. A brief description of various exhaust gas analysers can be found in Ref. 8. The most common method is by successive absorption of the CO2, 02 and CO as in the Orsat apparatus (Fig. 15.4). The sample of exhaust gas is drawn into the measuring burette by lowering the levelling bottle containing water. This known volume of sample at atmospheric temperature and pressure is forced in succession into each of the reagent bottles which contain the absorbents. The 328
Combustion Processes
[15.3] Fig. 15.4 Orsat apparatus for exhaust gas analysis
From sample bottle
—100
Tap Jl
)
Measuring burette Water jacket Levelling bottle
Reagent bottle
Tubes to increase wetted surface
volume is measured after each absorption process by returning the sample to the burette and bringing it to atmospheric pressure with the aid of the levelling bottle. The change in volume after a particular constituent has been absorbed is then the partial volume of that constituent in the original sample (see section 14.2). The gas which remains is assumed to be nitrogen. The resulting analysis is by volume and is on a dry basis. Although most of the water vapour is condensed when the sample is first cooled to atmospheric temperature, the sample is nevertheless saturated with water vapour at this temperature throughout the analysis because the sample is contained in the measuring burette over water. The reason why the Orsat apparatus yields a true dry analysis is therefore not obvious, and it is left to the following example to show that this is so. A second example shows how the analysis can be used to compute the air/fuel ratio when the percentage by mass of carbon in the fuel is known. Example 15.3
A sample of exhaust gases, when cooled to atmospheric temperature, has the following percentage composition by volume: CO2 a;
H2 0 b;
02 c;
Ne d
Show that the Orsat analysis yields the true dry analysis, which is evidently CO2
100a 100 — b'
02
100c 100 — b
112
100d 100 — b
Since the sample is in contact with water at a constant temperature throughout the analysis, the partial pressure ps of the water vapour must remain constant at the saturation value. But from equation (14.17), Ps = ns p n
and the pressure p of the mixture is atmospheric. It follows that ris/n is constant. 329
Applications to Particular Fluids
[15.3]
Since n decreases as absorption of the constituents proceeds, ns must decrease also, implying that some of the water vapour condenses. a, b, c and d can be regarded as kmol of constituent per 100 kmol of mixture, so that initially
b n 100
ns
If n„ represents the number of kmol of water vapour condensed during absorption of a kmol of CO,, the mole fraction of vapour in the remaining mixture is
b — n„ 100 — (a + ns,) Hence 100
ab b — ns, from which n51 = 100 — b 100 — (a + nsi)
The first percentage contraction of volume noted from the Orsat apparatus is therefore
a + ns, —
100a 100 — b
which is the percentage by volume of CO2 in a dry sample. Similarly, if n52 is the number of kmol of water vapour condensed on absorption of the 02 we have b 100
b — (N I + ns2) + c + n52 )
100 — (a +
After substituting for n„, this gives
be ns2 =
100 — b
The second contraction noted from the Orsat apparatus is therefore
c + ns2
100c 100 — b
which is the percentage by volume of 02 in a dry sample. The remaining volume, consisting of N2 and water vapour, is 100 — (a + ns, + c + ns2 ) After substituting for n51 and n52, this reduces to 100d 100 — b which is the percentage by volume of N2 in a dry sample.
330
Combustion Processes
[15.3]
Example 15.4
A petrol has the following ultimate analysis: C 83.7%; H 16.3% If the dry products analysis by volume is CO2 11.8%; 02 3.7%;
N2
84.5%
determine the air/fuel ratio used.
Carbon balance method Treating the volume fractions as mole fractions, 1 kmol of dry products contains 0.845 kmol of N2 . Now 0.845 kmol of N2 are brought in with 100 0.845 x 28 ( — ) = 30.85 kg of air 76.7 1 kmol of dry products contains 0.118 kmol of CO2 , which in turn contain 0.118 x 12 kg of carbon. This amount of carbon implies the combustion of 0.118 x 12 0.837
— 1.692 kg of petrol
Thus 1 kmol of dry products is produced when 30.85 kg of air are burnt with 1.692 kg of petrol, i.e. air/fuel ratio =
30.85 1.692
— 18.2
The foregoing method, using a carbon balance between reactants and products, is the most satisfactory when carbon is the predominant element in the fuel. The result may be inaccurate, however, if the exhaust gases are smoky, indicating unburnt carbon not included in the products analysis. An oxygen—hydrogen balance can be made as a check, although since the relevant quantities are relatively small the result is more open to error from inaccuracies of measurement.
Oxygen—hydrogen balance method First, 1 kmol of dry products contains 32(0.118 + 0.037) = 4.960 kg of 02 But the oxygen accompanying the nitrogen is 0.845 x 28 (
23.3 76.7
) = 7.187 kg
Hence (7.187 — 4.960) = 2.227 kg of 02 have combined with the hydrogen in the fuel to form water vapour. It follows from equation (15.7) that 2.227/8 kg of H 2 are involved, which corresponds to 2.227 8 x 0.163
— 1.708 kg of petrol 331
Applications to Particular Fluids
[15.3]
Therefore 30.85 kg of air are associated with 1.708 kg of fuel, i.e. air/fuel ratio =
30.85 — 18.1 1.708
With coalburning appliances there is an additional complication because some of the combustion products will be in solid form. The analysis of the refuse is easily accomplished by heating a sample above its ignition temperature in a stream of oxygen. The loss of weight is measured and assumed to be carbon, while the remainder is the ash. The following example shows how a complete mass balance can be compiled for a combustion process if the composition of the fuel, gaseous products and refuse are measured. In general the air will have a certain moisture content, which can be found by wet and drybulb temperature measurements (sections 14.5 and 14.6), and this is also taken into account in the example. Example 15.5
Determine the complete mass balance for a combustion process, on the basis of 1 kg of coal burnt, given the following data: Fuel consumption (fractions by mass): C 0.69; H 0.03; 0 0.04; N 0.01; H2 O 0.10; ash 0.13 Dry exhaust gas analysis (fractions by volume): CO2 0.146; CO 0.020; 02 0.055; N2 0.779 Refuse analysis (fractions by mass): C 0.40; ash 0.60 Air: drybulb temperature 22.8°C, wetbulb temperature 15.5°C.
The mass of refuse m, per kg of fuel burnt can be found from an ash balance, i.e. 0.6 in, = 0.13 kg and hence m, = 0.217 kg. (b) The mass of dry gaseous products can be found from a carbon balance. Basis: 1 kg of fuel. = 0.69 kg or 0.0575 kmol Carbon in fuel Carbon in refuse = 0.4 x 0.217 = 0.087 kg or 0.0072 kmol Carbon in gaseous products = 0.603 kg or 0.0503 kmol Basis: 1 kmol of dry gaseous products. = 0.146 kmol Carbon in CO2 = 0.020 kmol Carbon in CO Carbon in gaseous products = 0.166 kmol Ratio of dry gaseous products to fuel = 0.0503/0.166 = 0.303 kmol/kg. The dry gaseous products per kg of fuel are therefore: CO2 = 0.146 x 0.303 = 0.0442 kmol or x 44 = 1.95 kg CO = 0.020 x 0.303 = 0.0061 kmol or x 28 = 0.17 kg 02 = 0.055 x 0.303 = 0.0167 kmol or x 32 = 0.53 kg or x 28 = 6.61 kg NL = 0.779 x 0.303 = 0.236 kmol Total = 9.26 kg (a)
332
Combustion Processes
[15.4]
(c) The mass of dry air can be found from a nitrogen balance. Basis: 1 kg of fuel. Nitrogen in gaseous products = 0.236 kmol (from (b)) Nitrogen in fuel = 0.01/28 = negligible Nitrogen required from air = 0.236 kmol Dry air supplied = 0.236/0.79 = 0.299 kmol or x 29 = 8.67 kg (d) The mass of water vapour in the air, found from the hygrometric chart or tables, is specific humidity = 0.0081 kg/kg of dry air. Therefore the mass of water vapour in the air per kg of fuel = 0.0081 x 8.67 = 0.07 kg. (e) The water vapour in the gaseous products can be found from a hydrogen balance. Basis: 1 kg of fuel. H2 O entering with air = 0.07 kg = 0.10 kg H2 O in fuel H2 O from combustion of H 2 = 0.03 x 9 = 0.27 kg Total = 0.44 kg
Mass balance summary Reactants Fuel Dry air Moisture
1.00 kg 8.67 kg 0.07 kg 9.74 kg
Products Dry gases Moisture Refuse
9.26 kg 0.44 kg 0.22 kg 9.92 kg
The degree of balance obtained is an indication of the accuracy of the analyses of fuel and products of combustion.
15.4 First Law applied to combustion processes
The First Law of Thermodynamics applies to any system, and the nonflow and steadyflow energy equations deduced from this law must be applicable to systems undergoing combustion processes. Before these equations can be used, however, data must be available from which we can find the change of internal energy or enthalpy when the chemical composition of the system changes as well as the thermodynamic properties. As we shall see, we shall need to develop two new concepts for this purpose, namely internal energy of combustion and enthalpy of combustion. To develop these concepts we shall consider a hypothetical sequence of processes undergone by a stoichiometric mixture of a fuel and air which involves a chemical reaction going to completion. Although we shall have combustion in mind, the ideas apply to any chemical reaction. Let us first consider the change of internal energy. 333
[15.4]
Applications to Particular Fluids
15.4.1 Internal energy of combustion AC/6
Since the internal energy is a function of state, a change of internal energy is independent of the path of the process. Consider a nonflow combustion process, starting with a stoichiometric mixture of the fuel and air in an arbitrary state (p„ T1 ) and ending with the products in another arbitrary state (p2, T2 ). The process can conveniently be regarded as consisting of three successive processes via intermediate reference or socalled standard states, as shown in Fig. 15.5. The reactants are brought to a standard state (1)0,1'0 ) by some process a—b not involving a chemical reaction; the reaction b—c is then brought about in such a way that the products are at the standard state (po, To ); and finally the products are brought to the final state (p2 , T2 ) by some process c—d. We may write ( Up2 — URI ) = ( Up2 — Um ) + (Um — URO) + ( UR0 — URI )
(15.8)
where subscripts R and P refer to reactants and products respectively, and subscripts 1 and 2 refer to the initial and final states. The first and third terms on the righthand side represent changes of internal energy in processes not involving a chemical reaction, which can be evaluated by the methods applying to mixtures presented in Chapter 14. The middle term has to be obtained from additional experimental information because it involves a chemical reaction. However, by choosing a path which always involves the same pair of standard states at (po, To), only one piece of information is required for any given chemical reaction. The standard pressure Po agreed by international convention is pe = 1 bar, the superscript e denoting this reference pressure. The corresponding difference in internal energy, denoted by An is equal to
DUo = E40 — U,8,0 where the superscript e refers to pe and the subscript 0 to the standard temperature To . Again by international agreement, To is chosen to be 298.15 K = 25 °C. Furthermore, it is usual to associate AU,1 with the combustion of 1 kmol of fuel and to use the molar symbol Ain. This is the quantity called the internal energy of combustion. Two important points must be noted here. First, the volume Vo at state c is not necessarily equal to the volume V0 at state b. From the discussion in section 15.2 it should be clear that only when the amountofsubstance of the gaseous products in state c, ni,, is equal to that of the gaseous reactants in state b, Reactants
Fig. 15.5 Imaginary path linking the end states of a combustion process
Reactant
Products
Products
PO t TO ,i 1
ii.
pi ,T1
P21T2
U
U a
334
b
c
d
Combustion Processes
[15.4]
are the volumes equal (as they are in the reaction of equation (15.4) and are not in that of equation (15.7)). This point is of some importance because of the way in which 6,4 is determined experimentally for solid and liquid fuels, a problem discussed more fully in section 15.5. Here it suffices to say that Ain is deduced from the heat Q released in a constant volume process, and that the magnitude of Q is very nearly equal to the magnitude of Ain. The second point to be made is that to return the system to its original temperature To after an exothermic reaction, as combustion is, some heat must be transferred to the surroundings. Q is thus negative, and it must be concluded that there has been a reduction of internal energy of the system even though the temperature is the same for the reactants and the products. The explanation is that each molecule possesses potential energy stored in the bonds between the constituent atoms, and this energy—which we may term chemical energy—is smaller for the molecules of the products than it is for the molecules of the reactants. In the process b—c this energy is normally released to the surroundings as heat (although a small quantity could be transferred as work if Yob 0 Yoe). It follows that for an exothermic reaction Aiit must be a negative quantity. Let us now rewrite equation (15.8) for the molar quantity of the fuel involved, namely v„ —
UR1)
= (up2 —
LI") +
+ (URO — UR1)
(15.9)
where the first and third terms on the righthand side relate to quantities associated with 1 kmol of fuel reacting. In combustion processes the mixtures of reactants and products normally consist of gases and vapours at low pressure which can be assumed to behave as perfect gases, and possibly some liquid and solid substances. In all such cases the internal energy can be taken as a function only of temperature, so that subscripts 0, 1 and 2 in equation (15.9) can be taken to refer to To, T1 and T2. It has also been found that at normal pressures 64, though it depends on the choice of To, depends only insignificantly on pe. Therefore we can often dispense in practice with the superscript e, and frequently there is no need to refer to pressure at all when applying equation (15.9). (Important exceptions are dealt with in sections 15.7 and 15.8.) Using known u or c,, data, and assuming that no changes of phase occur during the processes a— b and c—d, the first and third terms on the righthand side of equation (15.9) can therefore be found from an appropriate choice of the following equations: Up2 — Upo =
E ni(fiu — ai0) = E thevi( T2 — To) P
or
= > mi(ui2 — P
URI =
URO
E ni(a R
or
P
=E R
ui.) = E mic„,( T2 —
TO)
P
(15.9a)
= E nieui( To — T1) R
— ui1 ) = E mi cui( To —
T1)
R
335
[15.4]
Applications to Particular Fluids
Here ni and mi are the amountofsubstance and the mass of constituent i (per kmol of fuel reacting), and 5,4 and cvi are its molar and specific heat capacities. If any constituent undergoes a change of phase in the temperature range T1 To data must also be known and included in the summation. or To —> T2 , the Ufg
15.4.2 Enthalpy of combustion and its relation to Ain
Considerations similar to those raised in relation to internal energy in the previous subsection also apply when establishing the change of enthalpy between reactants in state 1 and products in state 2. Thus the change of enthalpy can be broken down into three steps: (Hp2 — HR1) = (142 — Hp0) + Agt + (Hp, — HR1)
(15.10)
This equation is equivalent to (15.9), i.e. it applies to 1 kmol of fuel. The enthalpy of combustion AR is explicitly given by AR; = (Hp at p°, To ) — (Hp at I,' , To )
As with Ai4, Agt is only very slightly dependent on the choice of the standard pressure, and in practice the superscript e can often be omitted: this we will do until the end of section 15.6. The standard temperature To is, as before, 298.15 K = 25 °C. The first and third terms in equation (15.10) can be calculated from one pair of equations below, the choice depending upon what data are available: Hp2 — Hp() = En,(E,2 g,o )
or
= E mph, —
= E ntepi( T2 — To) Emi cp,(T2 — To) (15.10a)
HRO
HR1 =
or
E ni(gio — E„) R
E ni,pi( To — T1 ) R
= E mow — h11) = E mi cp,(To — T1) R
R
The set of equations (15.10a) is equivalent to that of (15.9a). Direct experimental determination of Ago is carried out in a steadyflow gas calorimeter, which is described briefly in section 15.5. When quoting values of Alio or Ago, it is necessary to specify the phase of any individual reactant or product which may be in doubt. The magnitude of Ago for a liquid hydrocarbon, for example, is less than the magnitude for the same hydrocarbon in gaseous form; and it is less by an amount equal to the latent enthalpy of vaporisation at the standard temperature To. Or to take another example, when the fuel contains hydrogen, the resulting H2 O in the products may be in the vapour or the liquid phase. This point will be considered again in the next section. The conventional way of conveying the data is to give the combustion equation to which the value of Atio or Ago is applicable. For example, the enthalpy of combustion at the standard temperature To = 25 °C for hydrogen burning to 336
Combustion Processes
[15.4]
water vapour is H2 +102 H2 0(vap); Ago = —241 830 kJ/kmol of H2 It may sometimes be more convenient to work in terms of mass units, and in such cases we find Duo and Oho are quoted per unit mass of fuel. Taking the exact value for molar mass of H2 , 61= 2.016 kg/kmol, then for the above reaction Oho = —119 960 kJ/kg of H2 . It is usual to make direct experimental determinations of Alio for solid and liquid fuels, and of Ago for gaseous fuels. Once either Au° or A/ has been determined experimentally, the other quantity can be calculated by making use of the following relation: Ako = HP0 —
HRO
= (UPO + 140140)  (IJR0 PRO VRO) = Alio +(PVP0 — P Vito)
For gaseous reactants and products we can write pV = niZT, and for solid and liquid constituents the pV terms are negligible compared with the internal energy term. The relation between Ago and Aso can therefore be written as
eF0 = erio + IITO (np — nR)gas where nR and np are the amountsofsubstance of gaseous reactants and products respectively. It follows that when n R for gaseous reactants is equal to np for the gaseous products, then Alio and Al o are equal. For most fuels the difference is quite small, as will be shown in the particular case dealt with in Example 15.8. It is evident from equations (15.9) and (15.10) that, in addition to values of Alio or Ago, we require a knowledge of the internal energies or enthalpies of the various reactants and products, or of heat capacities, as functions of temperature. Ref. 17 contains tables of molar internal energies and enthalpies, namely values of a and J, for most common gases and a representative selection of hydrocarbon fuels. These are tabulated against absolute temperature, and their use will be illustrated in Example 15.7. Ref. 17 also contains values of cp tabulated against absolute temperature, and their use will be illustrated in Example 15.6. Attention is drawn to the discussion in section 8.5.3 of the evaluation of mean specific heat capacities over a range of temperature T1 to T2 . There it is explained that using a value at, say, 1( T, + T2 ) will lead to inaccuracies unless c, varies linearly with T Since the temperature ranges met with in combustion processes are often large, c p tables used in this way can be much less accurate than a and g tables. It is worth emphasising that in tables of internal energy or enthalpy, one or other value must be put equal to zero at some arbitrary value of temperature. In Ref. 17 it is the enthalpy which is put equal to zero at To = 298.15 K. The tables can be used to find changes of internal energy and enthalpy only along paths which do not involve a chemical reaction, because no account is taken of the particular form of internal energy which changes when a reaction occurs. 337
Applications to Particular Fluids
Example 15.6
[15.4]
When all the products of the gaseous hydrocarbon engine (C2 H 6 ) are in the gaseous phase, the enthalpy of combustion at 25°C is —47 590 kJ/kg. Find (a) the corresponding internal energy of combustion, and (b) the enthalpy of combustion at 540°C. Calculate the heat transferred when 0.2 kg of ethane is burnt at constant pressure in a cylinder containing 4.0 kg of dry air, the temperature of the reactants and products being 40°C and 54°C respectively.
The relevant mean specific heat capacities at constant pressure, for the range 25°C to 540 °C, are found from Ref. 17 at the mean temperature 555 K to be C2 H6 2.800; 02 0.989; CO2 1.049; H2 O(vap) 1.987; N2 1.066 kJ/kg K And for the range 25°C to 40°C, C2 H6 1.788; 02 0.919; N2 1.040 kJ/kg K (a) Internal energy of combustion at 25 °C
The stoichiometric combustion equation is C2 H6 + 3402 2CO2 + 3H2 0(vap) There are 44 kmol of reactants and 5 kmol of products per kmol of ethane, so that in equation (15.11) we have (tip — nR)= kmol Since Ah25 is given in kJ/kg, and 1 kmol of ethane is equivalent to a mass of 30 kg, Au2, = —47 590 8.3145 x 298 = 47 630 kJ/kg of C2 H6 2 x 30
(b) Enthalpy of combustion at 540°C
From equation (15.10) we have Ah540 = (H P540 HR540 ) = (HP540 — Hp 25 ) Ah25 (Hp25 — 14540)
In terms of mass, the combustion equation is
30 kg C2 H6 + 112 kg 02 88 kg CO2 + 54 kg H2 O On the basis of 1 kg of C2 H6 , we have (14540 — HP25) =
mic,;(540 — 25)
515 = 30 {(88 x 1.049) + (54 x 1.987)} = 3247 kJ/kg of C2 H6 338
Combustion Processes
[15.4]
Similarly, mi cpi(25 540)
(HR25 HR540 ) — R
515 = —— 30 1(30 x 2.80) + (112 x 0.989)} = —3345 kJ/kg of C2 H6 Ah 540 = 3427 — 47 590 — 3345 = —47 510 kJ/kg of C2 H6
From (a) and (b) it should be noted that the difference between Oho and Duo is small, and that the values are not greatly affected by a change of reference temperature.
Constant pressure combustion In the constant pressure combustion, the products are not returned to the initial temperature and we must take account of the change in enthalpy of the nonreacting substances. The heat transferred is equal to the change of enthalpy if the expansion work can be regarded as $ p dv. Therefore Q = ( 14540 111140) = (Hp540 — HP25) + Ah 25 (HR25 HR4o)
The stoichiometric combustion equation for 0.2 kg of ethane is 0.2 kg C2 H6 + 0.747 kg 02 0.587 kg CO2 + 0.360 kg H2 O But 4 kg of air are provided, consisting of (4 x 0.233 kg 02 ) + (4 x 0.767 kg N2 ) = 0.932 kg 02 + 3.068 kg N2 Evidently there is some excess air, and the combustion equation for the specified mixture is 0.2 kg C2 H6 + 0.932 kg 02 + 3.068 kg N2 —+ 0.587 kg CO2 + 0.360 kg H2 O + 0.185 kg 02 + 3.068 kg N2 On the basis of 0.2 kg of ethane: ( 14540 — Hp25 ) = 515{(0.587 x 1.049) + (0.360 x 1.987)
+ (0.185 x 0.989) + (3.068 x 1.066)} = 2464 kJ (HR25 — HR4o) = —15{(0.2 x 1.788) + (0.932 x 0.919) + (3.068 x 1.040)1 = —66 kJ Therefore Q = 2464 — (0.2 x 47 590) — 66 = —7120 kJ 339
[15.4]
Applications to Particular Fluids
15.4.3 UT and HT diagrams
We have already noted that, during changes of state involving no chemical reaction (see the first and third terms on the righthand sides of equations (15.9) and (15.10)), the internal energies and enthalpies can be taken as functions of temperature only. Under these circumstances, U and H for the reactants and products can be plotted as single lines on U— T and H—T diagrams as shown in Fig. 15.6.* The only constraint is that the two lines must be separated by the correct amount. The vertical separation must, at T0, be equal to Au° in Fig. 15.6a and to Ago in Fig. 15.6b. For an exothermic reaction the products line must lie below the reactants line. The location of the two lines on the graph is otherwise arbitrary, because the datum state for either reactants or products can be chosen arbitrarily. During any combustion process 12 in a closed system, both work and heat may be transferred across the boundary in accordance with the nonflow energy equation Q+ W = Up2  U R,
There are two combustion processes of special interest. One is often referred to as the calorimeter process, 13, carried out at constant volume and with T3 = Tt . In this process the work is zero and the heat transferred is effectively equal to the internal energy of combustion at T1 . This process yields the maximum possible transfer of energy to surroundings at T, . The second process of special interest is adiabatic combustion at constant volume. Since both the heat and work transfers are zero, the internal energy remains constant. There is merely a redistribution of internal energy resulting in a rise of temperature, i.e. we may say that chemical energy is transformed into sensible internal energy. This process, 14 in Fig. 15.6a, results in the maximum possible rise of temperature for any given air/fuel ratio.
Fig. 15.6
H
U
U—T and H—T diagrams for combustion processes
To
(a)
T
To (b)
T
* One reservation must be mentioned: if the mixtures of reactants and products contain constituents that can change phase, then the ratio of vapour to liquid of such constituents must not change along 10 or 02. Otherwise a family of lines would be required to describe the U—T or H—T relations.
340
[15.4]
Combustion Processes
When considering steadyflow processes, it is appropriate to depict these on an H—T diagram (Fig. 15.6b). The steadyflow calorimeter process, in which the heat transferred is equal to the enthalpy of combustion, is represented by 15. Steadyflow adiabatic combustion, with zero work and no change of kinetic energy, is represented by 16; this process yields the maximum possible temperature rise for steadyflow combustion. In solving combustion problems, great care must always be taken with signs. Intelligent use of the diagrams, as illustrated in Example 15.7, can save one from this source of error.
Example 15.7
Liquid heptane ( C7H16) has an enthalpy of combustion of —4 465 300 kJ/ kmol at 298 K when the water in the products is in the vapour phase. This fuel is to be burnt adiabatically in a steadystream of air in stoichiometric proportions. If the initial temperature of the fuel and air is 288 K, estimate the temperature of the products. For liquid heptane "dp = 230 kJ /kmol K. The stoichiometric combustion equation, including the nitrogen introduced with the air, is 79 C7 H16(liq) + 1102 + —11N, 21
79 i 7CO2 + 8H2 0(vap) + — 111.4 2 21
The steadyflow energy equation reduces to HPT — H8288 = 0, where T refers to the products' absolute temperature. Expanding the equation, following the path of calculation indicated in Fig. 15.7, (HPT  Hp298) Ar1298 + (H8298  H8288) = 0
or
E
— ITP298) Ar1298
E ni(ER298 — gR288) = 0
The evaluation of this equation involves successive approximations because the values of hpr of the constituents of the products depend upon the unknown temperature T Guessing initially that T = 2200 K, it is possible to extract the
Fig. 15.7 Path of calculation
[kJ/kmol]
288 298
T/[1(] 341
[15.4]
Applications to Particular Fluids
following table of molar enthalpies F/[kJ/kmol] from Ref. 17:
T, = 288 K T, = 298 K T = 2200 K
02
N2
CO2
— 296 0 66 802
— 296 0 63 371
— 353 0 103 570
1120(Vap) — 339 0 83 036
Hence we can write, per kmol of C71116, 79 7(103 570 — 0) + 8(83 036 — 0) + — 11(63 371 —0) 21 + ( —4465 300) + {1 x 230(298 — 288)} 79 + 11{0 — ( —296)} + — 11{0 — ( —296) } = —435865 kJ 21 Clearly, the guess T = 2200 K was not correct, because the result is not equal to zero. Repeating with enthalpy values for T = 2400 K, the imbalance in the enthalpy equation becomes + 35 473 kJ. Linear interpolation between the imbalance terms of — 435 865 kJ and + 35 473 kJ yields a value for T of 2385 K. The temperature intervals in the molar tables of Ref. 17 are 200 K, while those in the original Janaf Thermochemical Tables [Ref. 37] from which they were abstracted are 100 K. The denser table would yield a somewhat more accurate result when the variation of with T is not linear in the relevant temperature interval. The adiabatic temperature rise can also be obtained directly from special charts, such as the Diagram of Temperature Rise versus Fuel—Air Ratio published in association with Ref. 17. This chart provides adiabatic temperature rises for any initial temperature of reactants and any air/fuel ratio. However, it applies strictly for only one particular fuel, in this instance one with a mass ratio of hydrogen to carbon of 13.92/86.08 and an enthalpy of reaction of —43 100 kJ/kg. The actual temperature of the products from the adiabatic combustion of a stoichiometric mixture would not be as high as the value calculated in the manner of the previous example. The combustion would in fact be incomplete, partly for the reasons already given in section 15.2, and partly because at high temperatures the products are unstable. Some of the molecules split into their constituents, usually with an accompanying absorption of energy. This phenomenon is known as dissociation, and the method of estimating the final temperature when dissociation occurs is discussed in section 15.7. Most fuels produce adiabatic combustion temperatures between 2200 and 2700 K when burnt stoichiometrically in air initially at atmospheric temperature. Higher temperatures can always be achieved, either by heating the air before combustion, or by enriching it with oxygen and so effectively reducing the mass of nitrogen present. The temperature will be increased in the latter case because the mass of the products, and hence their heat capacity, is reduced. The rise in temperature for a given release of chemical energy is therefore greater. It should be appreciated, however, that although very high temperatures may be desirable
342
[15.51
Combustion Processes
from a thermodynamic point of view, they cannot always be employed in power plant. lit a gas turbine, for example, where the highly stressed parts of the turbine are in a continuous stream of hot gaseous products, serious overheating would occur unless a large quantity of excess air were provided to reduce the temperature at exit from the combustion chamber.
15.5 Experimental determination of ACio and Ah0 and calorific values
For solid and liquid fuels it is the value of Afio with water in the products in the liquid phase which is found from experiments: we shall denote the value by Atio(liq). Values of Afio with water in the vapour phase, namely Aiio(vap), and corresponding values of Aho with water in either liquid or vapour phase, must be found by calculation from the value of Aiio(liq) and from the ultimate analysis of the fuel. Thus Atio(vap) —
= nH2o fifg
Aho(vap) — Aho(liq) =
n H20 fg
(15.12a) (15.12b)
The amountofsubstance of H 2 0 formed per unit amountofsubstance of fuel, n H 2O, can be deduced from the fuel analysis. The internal energy and enthalpy of evaporation, fifg and kg, must be taken at the standard temperature of 25 °C. The relation between Aito and AE0 has already been derived in section 15.4.2, equation (15.11). Calculations of the kind described above are illustrated, in mass units, in Example 15.8. The experimental value of Afi, is found by burning a measured quantity of fuel in a bomb calorimeter. This consists essentially of a gastight steel vessel, the 'bomb', which is immersed in a conventional water calorimeter. The 'water equivalent' of the calorimeter and bomb is found by conducting a preliminary experiment using an electrical resistance method of heating (or benzoic acid, whose value of Atiio(liq) is accurately known). The bomb is then charged with the fuel sample, and with oxygen at a high pressure to ensure complete combustion. A small quantity of water is placed in the bomb initially to saturate the volume, and any water formed by the combustion will therefore condense. Thus the value obtained will be that with water in the liquid phase. After ignition, the final steady temperature of the calorimeter is noted; it is arranged to be not more than about 3 K above an initial temperature of about 23.5 °C. Although the temperature of the products is not exactly equal to that of the reactants, or equal to the standard temperature of 25 °C, the value of Alio so obtained should be very close to that demanded by the definition. Example 15.6 showed that a large change in To had a small effect on Also, and this is true also of Ai10. The concept of internal energy of combustion was explained and defined in section 15.4 with the help of a 'paper' experiment involving a stoichiometric mixture of fuel and air. In the experiment just described pure oxygen is supplied, and moreover in excess of stoichiometric requirements. Does this matter? In principle it does not, because the initial and final temperatures are ideally the 343
Applications to Particular Fluids
[15.5]
same and there will therefore be no net change in internal energy of any nonreacting substance present. For example, excess oxygen and water in the bomb should have no effect other than to ensure complete combustion of the fuel and complete condensation of the water vapour in the products respectively. The presence (or in this case absence) of inert constituents of air should likewise have no effect on Azio(liq). Because in the actual experiment the temperature of the products is not exactly equal to that of the reactants, corrections have to be applied when obtaining precise values of Afio(liq) from the experimental results. Other corrections may also have to be made. For example, there may be heat released or absorbed when some of the gaseous products dissolve in the water in the bomb. A more fundamental correction, not necessarily larger in magnitude, arises from the fact that the pressure in the reaction vessel is not the standard pressure pe. We are seeking an internal energy change at pe, T0 ),, — (17 at pe, To)R while what we obtain from experiment, after all the above corrections have been applied, is 04 at pi ,
— (a at p2, To)R
Here pi is the pressure to which the bomb is charged, and this is very high; so too is the final pressure p2. In fact, p2 = p (ti p/ nR)gas. The corrections are of two kinds: those due to departures from perfect gas behaviour at high pressure, and those due to any difference between n, and nR. (The reader should satisfy himself that the second correction, obtainable from equation (9.13), is equal to npRT0 ln(np/nR). For gaseous fuels it is the value of AE0 (hq) which is found from experiment; Ailo(liq), Afio(vap) and AE0(vap) should be found by calculation from Arzo(liq) and the ultimate analysis of the fuel. The value of Ak (lig) is most conveniently measured by burning a mixed stream of gas and air at atmospheric pressure and temperature, under steadyflow conditions in a gas calorimeter. The gas—air mixture is saturated with water vapour. After burning, the hot products of combustion flow over cooling coils through which water flows steadily in the opposite direction. With this counterflow arrangement the products leave the calorimeter at approximately atmospheric temperature and all the water vapour produced is condensed. An approximate value of AE0 (liq) of the gas can be readily calculated from the mass flow and temperature rise of the cooling water. Certain corrections have to be applied to the results obtained, as had to be done to the results for Aiio(liq) from the bomb calorimeter. However, because the experiment is carried out at a pressure approximately equal to pe, and the pressures at inlet to and exit from the calorimeter are very nearly equal, corrections for effects due to high pressure and changes in amountsofsubstance do not arise.
Example 15.8
The value of Auo (liq) for liquid kerosene was found by experiment to be —46890 kJ/kg. The ultimate analysis of the kerosene was 86 per cent 344
Combustion Processes
[15.5]
carbon and 14 per cent hydrogen. Calculate the value of Auo (vap), and the corresponding values of Aho (liq) and Aho (vap).
First, 1 kg of fuel produces 0.86(44/12) = 3.15 kg of CO2 and 0.14(18/2) = 1.26 kgof H2 O. At 25 °C, ufg = 2304 kJ/kg and hfg = 2442 kJ/kg. So that Auo(vap) = Au0 (liq) + mH,o ufg = —46 890 + (1.26 x 2304) = —43 987 kJ/kg The combustion equation can be written as 1 kg fuel + 3.41 kg 02 4 1.26 kg H2 O + 3.15 kg CO2 The relation between Aho(liq) and Au0(liq) can be obtained from equation (15.11). Remembering that only gaseous reactants and products should be included, and given that the fuel is in liquid form, the equation becomes Ah0(liq) = Au0(liq) + RT0 ( E — P Mi
R mi
= —46 890 + {8.3145 x 298.15
gas
(3.15 3.41 )} 44 32
= —46890 — 87 = —46977 kJ/kg Ah0(vap) = Ah0(liq) + mH2o hfg = —46 977 + (1.26 x 2442) = —43 900 kJ/kg As a check, we can find Ah0(vap) from Au0(vap) using equation (15.11): Ah0(vap) = Au0(vap) +
RT0( E;i p Mi
R
Mi)gas
1.26 3.15 3.41)1 = —43 987 + {8.3145 x 298.151 — + 18 44 32 = — 43 900 kJ/kg Note that the difference between Au0(liq) and Au0(vap) is 6.2 per cent, whereas Au0 (liq) and Ah0 (liq) differ only by about 0.2 per cent. In any applications of combustion data, it is evidently more important to decide whether the H2 O in the products should be regarded as liquid or vapour than whether Au, or Alio data are appropriate.
When dealing with energy transfers in combustion processes, engineers have in the past commonly related these transfers to some calorific value of the fuel rather than to the properties Au, and Ah0 . Calorific values refer directly to quantities of heat liberated when unit mass of fuel is burnt completely in a calorimeter under specified conditions. Because calorific values are defined in terms of quantities of heat, the definition must specify not merely the end states 345
[15.6]
Applications to Particular Fluids
but also the details of the process connecting these end states. Provided standardised equipment is used and the specific conditions are adhered to, the results obtained will be accurately reproducible. The fact that the quantities are not identical with the more rigorously defined properties Duo and Oho is not important for such purposes as comparing the efficiency of power plant, or meeting statutory requirements for the heating value of a gas supply. The four calorific values that have been in common use are as follows, together with the values of Duo and Oho to which they correspond most closely: Gross (or higher) calorific value at constant volume: Net (or lower) calorific value at constant volume: .2net, = Gross (or higher) calorific value at constant pressure: Qua,= 42„ei,p= Net (or lower) calorific value at constant pressure:
—Au25 (liq) —4u25(vah) —Ah25(ltq) —4h25(vap)
Two points should be noted. First, while values of Auo and Oho for an exothermic reaction in accord with our sign convention are negative numbers, calorific values are always quoted as positive numbers. Secondly, gross (or higher) and net (or lower) refer to the phase of H2 O in the products, the former to liquid and the latter to vapour. 15.6 Efficiency of power plant and of combustion processes
The cycle efficiency of a heat engine is calculated without reference to the source of heat. When considering the efficiency of the power plant as a whole, however, we are also concerned with the efficiency of the means of producing the heat, i.e. whether the fuel is in fact being completely burnt under the most advantageous conditions. The overall thermal efficiency of a power plant can be suitably defined as the ratio of the work produced to the latent energy in the fuel supplied. The question arises as to how this latent energy should be assessed. Any power plant, considered as a whole, is an open system undergoing a steadyflow process—with air and fuel entering the system, and the products of combustion leaving it, at a steady rate. This is illustrated in Fig. 15.8a. The fuel and air enter at atmospheric temperature, and the largest quantity of energy that can be transferred to the surroundings will be produced if (a) the fuel is burnt completely, (b) the products leave at atmospheric temperature, and (c) any water in the products is in the liquid phase. The energy transferred under Fig. 15.8 Schematic combustion power plant
Fuel Air w
Fuel —FP Air
I JI
T,, T,
1✓ Q (a) 346
I *
Products
Combustion Processes
[15.6]
these conditions, per unit mass of fuel burnt, is Ahrn(liq), where 'a' and 'atm' refer to the ambient reference temperature and pressure respectively. To all intents and purposes Ahrn(liq) = Aho(liq). If Aho(liq) is regarded as the effective latent energy in the fuel, the efficiency of the power plant is suitably defined by (15.13)
Aho(liq)
where W is the work transfer per unit mass of fuel. Now the temperature of the products is never reduced to atmospheric temperature in practice, for this would entail an infinitely large heat exchange surface somewhere in the plant (e.g. in the economiser of a steam plant). Moreover, this condition is not even approached, if for no other reason than the undesirability of allowing water vapour to condense. Combustion products usually include a small quantity of sulphur dioxide which would dissolve in the water and form corrosive sulphuric acid (but note the reference to socalled `condensing boilers' in section 11.6). Considerations of this type have led many engineers to prefer to define thermal efficiency in terms of Aho(vap), i.e. =
(15.14)
Aho(vap)
This definition yields slightly higher values for the thermal efficiency because Aho(vap) is smaller in magnitude than Aho(liq). It is clear that power plant efficiencies are process efficiencies and, like all such efficiencies, they are comparisons between an achieved result and some arbitrary standard. It is most important always to state clearly which standard, Aho(liq) or Aho(vap), is being used. A more rational definition of power plant efficiency is discussed in section 17.5, from which it is apparent that, of the two arbitrary definitions presented here, definition (15.14) is to be preferred. It must be emphasised that the foregoing discussion applies equally to steam power plant and internalcombustion engines. For the former, Fig. 15.8a can be analysed further as in Fig. 15.8b; part A of the system is regarded as the boiler furnace and part B as the working fluid which is taken through a thermodynamic cycle. Most of the heat rejected Q2 passes out in the condenser cooling water. When the combustion process itself can be isolated from the rest of the plant, as in a steam boiler or gas turbine combustion chamber, it is necessary to have some measure of its efficiency so that the performance of different combustion systems can be compared. Combustion efficiency is most generally defined as the fraction of the latent energy input which is effectively utilised in the desired manner. The detailed definition will depend upon the method of designating the latent energy input and the effectively used output. In the case of a steam boiler, for example, the combustion is used to produce heat and so transform water into steam. The combustion efficiency can therefore be alternatively defined as rl —
—Aho(liq)
or
—Aho(vap)
(15.15) 347
[15.6]
Applications to Particular Fluids
where Q is the heat transferred to the water, i.e. the increase in enthalpy of the water per unit mass of fuel supplied. To take a second example, the object of the adiabatic combustion in a gas turbine combustion chamber is to increase the sensible enthalpy of the fluid flowing through it—so that this can be used to produce work in the turbine. The efficiency may be defined, therefore, as the ratio of the actual increase of sensible enthalpy per kilogram of fuel to the increase obtained when each kilogram of fuel is burnt completely. The energy equation is (Hp2 — HR1) = (142 —
+ Aho + (H • .R0
HR1) =
With complete combustion, the increase in sensible enthalpy is given by (142 —
— (HR1 —
= —M0
With incomplete combustion, the increase in sensible enthalpy will be {(H p2 — H p0 ) — (HR1 — H RO
actual = Aho —
E mi( —M 01)
The summation is of unburnt or partially burnt constituents; mi is the mass of constituent i per unit mass of fuel, and Aho, is its enthalpy of combustion. The choice of reference temperature T0 has little effect on the efficiency, but the phase of the H2 O in the products must be specified. The expression for combustion efficiency becomes 1=
1
{(Hp2 — Hpo) — (141 — — Oho
HRO)}actual
(15.16)
The enthalpy of combustion can be taken as either Aho(liq) or Aho(vap) according to convention. The numerator in equation (15.16) is best determined from the results of an experimental analysis of the products. A second definition of efficiency frequently employed is the fraction of the actual fuel used which would have been sufficient to achieve the actual products temperature with complete combustion. Further discussion of these and other ways of expressing gas turbine combustion efficiencies can be found in Ref. 26.
Example 15.9
Find the efficiency of the combustion process of Example 15.5 on the basis of Aho (vap) and the percentage of complete combustion attained. The following data can be assumed: = —24490 kJ/kg Aho(vap) of the coal = — 32 790 kJ/kg Aho of solid carbon Aho of carbon monoxide = —10110 kJ/kg
The efficiency may be expressed by —Aho(vap) — =
348
E m,( — Oho);
— Aho(vap)
[15.7]
Combustion Processes
From the solution of Example 15.5, the unburnt and partially burnt constituents in the products, per kg of coal burnt, are 0.17 kg of CO in the gaseous products 0.4 x 0.217 = 0.0868 kg of C in the refuse Therefore
Erni(Aha= (0.17 x 10110) + (0.0868 x 32790) = 4565 kJ/kg 24 490 — 4565 —
24 490
— 0.814
15.7 Dissociation
It was pointed out in section 15.4 that the maximum temperature reached in an adiabatic combustion process is limited by the phenomenon of dissociation. Consider, for example, the reaction CO + 102 CO2 When it proceeds in the direction indicated by the arrow it is accompanied by a release of energy. The reaction can be made to proceed in the reverse direction, however, if sufficient energy is supplied to molecules of CO2 . Some of the CO2 molecules in the combustion products do receive sufficient energy in collision for this to occur, i.e. some of the molecules undergo the reaction CO2 CO + 102 This possibility is symbolised by writing the equation as CO + 102 ,, 'CO2 The reversed reaction is accompanied by an absorption of energy, and it is termed an endothermic reaction. It is found that at any particular temperature and pressure the proportions of CO2 , CO and 02 adjust themselves until the two reactions proceed at the same rate, i.e. until the number of CO2 molecules being formed is equal to the number dissociating. A state of stable chemical equilibrium is then said to exist. The state of equilibrium is not a static one, because the two reactions are going on continuously and simultaneously. It is only at high temperatures, above about 1500 K, that a significant proportion of the CO2 molecules must dissociate to provide an equilibrium mixture. The preceding remarks apply equally to H2 O molecules in combustion products. It is now possible to appreciate why the adiabatic combustion temperature is less than that predicted by the simple calculation of Example 15.7. Evidently the products contain an equilibrium mixture of CO2 , CO and 02, and an equilibrium mixture of H2O, H 2 and 02 . The presence of CO and H2 indicates that not all the chemical energy in the fuel is released. The question arises as to how the states of chemical equilibria can be predicted. We shall proceed to show that a condition for equilibrium can be deduced from the Second Law of Thermodynamics. The first step is to visualise how a thermo349
Applications to Particular Fluids
[15.7]
dynamically reversible chemical reaction can be achieved, and the argument suggested by van't Hoff in 1887 will be used here. 15.7.1 The van't Hoff equilibrium box
Consider a stoichiometric reaction between CO and 02, each initially at the standard pressure pe and a temperature T, to form CO2 at the same pressure and temperature. This reaction can be carried out in many ways. In the gas calorimeter, for example, all the energy released is transferred as heat and the reaction is irreversible. When the reaction is made reversible, however, we shall find that some of the energy is transferred as work. Fig. 15.9 illustrates one conceivable steadyflow open system in which the reaction can proceed reversibly. The reaction itself occurs in the reaction chamber, or 'equilibrium box', which contains CO2, CO and 02 in such proportions that the reactions CO + 102 CO2 and CO2 —> CO + 102 are proceeding simultaneously at equal rates. The box is maintained at a constant temperature T by surrounding it with a reservoir at T Any heat exchanges will therefore take place reversibly. The total pressure in the box may have any arbitrary value p, which may be greater or smaller than pe, determined by the total mass of gas present. The CO, 02 and CO2 enter or leave the box through semipermeable membranes, the mass flows at entry and exit being equal. If these mass transfers are to take place reversibly (see section 14.3), the pressure of each constituent outside the box must be equal to its partial pressure inside the box (i.e. pco , pot or pco,), and the temperature of each constituent outside the box must be equal to T Since the pressure and temperature of the CO, 02 and CO2 are p° and T at the boundary, reversible isothermal compressors and expanders must be included in the system to maintain the respective pressures at Pco' Po, and pco, outside the semipermeable membranes. Imagine that CO and 02 are transported slowly into the reaction box at the steady molar flow rates of it and 2 respectively, and that the reaction proceeds Fig. 15.9 The
Surrounding reservoir at T
van't Hoff equilibrium
Wco Oco
box
Wo,
350
x.o2 [Drawn for the case where the net reaction proceeds according to CO +102— CO2 and any partial pressure > ]
Combustion Processes
[15.7]
in the normal direction. The equilibrium mixture will remain unchanged if CO2 is discharged at the steady molar flow rate of A. Only an infinitesimal change in the external conditions is needed to reverse the expanders and compressors and to cause the reaction to proceed in the opposite direction. All the quantities of heat and work transferred across the boundary then have the same magnitude but are reversed in sign. The whole isothermal steadyflow process can therefore be regarded as reversible. We shall proceed to show that the power output from this hypothetical reversible plant is the maximum attainable from this chemical reaction in surroundings at the temperature T In the course of so doing we shall find that the relative proportions of constituents in the equilibrium box, expressed in terms of mole fractions, depend upon a parameter K which is a function of T but not of p. For simplicity we shall assume here that the reaction involves only perfect gases, for which a mole fraction is proportional to the partial pressure, equation (14.17). 15.7.2 Maximum work of a chemical reaction and equilibrium constants
The rate of work transfer when a perfect gas undergoes a reversible isothermal steadyflow process is given by equation (10.6). When the gas flows at a molar rate of ri, it can be written as 14/ = riRTln P2 P The net power output from the system shown in Fig. 15.9 is therefore W I = riRT(ln Pco, + In + 1 In Pe Pe Pco 2 Po, = ART ln
(Pco,/Pe) (Pco/Pe)(Po2/P9)1"
(15.17a)
Now suppose that the pressure p in the reaction box is changed to p', but all other conditions remain unchanged. The new partial pressures will be p'co, p'02, and p'02,2 such that P'co + PO2 + P'co 2 = and the net power output becomes I 14/11 = ART In
(PiC°2/Pe) (P'co/Pe)(P62 /Pe)1/2
(15.17b)
Either IWI = IW'I or IWI IW' I. If the latter, the system producing the lesser power could be reversed and the two systems coupled together. The combined system will then operate in a cycle and produce a net amount of work while exchanging heat with a single reservoir of uniform temperature T This contradicts the Second Law, and so I W I must be equal to I W' I. The same argument would apply to any reversible system that can be conceived operating with the same boundary conditions of pe and T, and the power I W I is therefore 351
Applications to Particular Fluids
[15.7]
the maximum that can be obtained from this chemical reaction. When the process is irreversible, the power output will be less; in the calorimeter process it is zero. Since I W I = Oil, it follows that (Pico2 /Pe) (Pco2 /P8) 1/2 = (prcoipe)(p02/pe)112 (Pco/Pe)(P02/P1 Thus the combination of pressure ratios (pdpe) above is independent of the total pressure p in the equilibrium box. This combination, or parameter, is called the standard or thermodynamic equilibrium constant for the reaction considered. The symbol used is K 8, the superscript indicating that all partial pressures are normalised by the standard pressure IA Thus Ke —
(Pco2 /199) (Pco/Pe)(Po2 /P9)"2
(15.18a)
It is sometimes useful to gather all 138 terms together and rewrite equation (15.18a) as )(pe)1/2
Ke = (PCO, (PC0)(P02 )"2
( 15.18b )
(as is done in the table headings of Ref. 17 to save space). Although IC' is dimensionless, its numerical value will depend on the choice of p'. It is independent of IP only for reactions in which np = nR, when the net exponent of the IP term becomes zero.* In common with other chemicalthermodynamic data which have to be referred to a standard pressure (e.g. Aut, An), the standard pressure agreed upon internationally is 1 bar. There is nothing in the foregoing to suggest that 10 is independent of the temperature T of the mixture, and experiment shows that it varies strongly with temperature, as we shall see later. As anticipated earlier, we have not only shown that Ke f(p), but also derived the important result that equation (15.17a) expresses the maximum work I 147 Imax attainable from this particular reaction. The result can be generalised to apply to any other chemical reaction involving perfect gases for which the equilibrium constant 10 is known, and I Pi/ Lax can be related to 10 by I W Imax = ART ln K°
(15.19)
This result is discussed further in section 17.7 and, for the more advanced student, in section 7.9.3. In generalising the foregoing arguments to other chemical equations, let us * It used to be common practice to define the equilibrium constant in terms of partial pressures, e.g. in the case considered here as K„= (PCO2)/(PC0)(P02)112. The subscript p was added to imply the above mode of definition. K p would then in general not be dimensionless unless np = nR. Tables used to present values of log K„ (or In K p), an inadmissible practice because arguments of logarithms, or of any transcendental function, should always be dimensionless quantities. Why did this breach not lead to errors? It is easy to show that if the unit in which the partial pressures are measured is equal to the standard pressure adopted (it used to be 1 atm), then numerically K,, = K 8 and the breach is thus swept under the carpet.
352
Combustion Processes
[15.7]
consider any stoichiometric equation such as v1 kmol of A + 1'2 kmol of B v3 kmol of C + v4 kmol of D where v1 , v2 , v 3 and v4 are called the stoichiometric coefficients; the coefficients of the products are by convention taken as positive, and those of the reactants as negative. We would then arrive at the expression Ke
= (Pc/Per.3(PD/P9)''4 (PA
/Pe r (PB/PeY2
And this could be written even more generally as
K 9 = fl (pdpe)"
or In Ke = E ln(pdper
(15.20)
where FL means the product for all constituents i, and Ei is the sum of the logarithmic terms. Applying equation (15.20) to the reaction H2 + 102 ,='14 2 0, for example, we get for the equilibrium constant (Pii,o/P9)
(Pu2o)(P11/2
(15.21) (Pu,/Pe)(PolPe)1/2 (PH2)(P02)112 It should be clear that when tabulating experimentally determined values of K 8, it is necessary to specify the reaction. The equilibrium constant K9 would have different values if the reaction were written as, say, 2H 2 + 02 =2H2 O or H20 ± H2 + 102 . In the former case K9 would be the square of that given by equation (15.21), and in the latter it would be the reciprocal of it. Remembering that the partial pressures are proportional to the mole fractions as given by equation (14.17), it is evident that Ke is a measure of the amount of dissociation. A high value implies that the mixture contains a large proportion of undissociated products and so there is little dissociation. For exothermic reactions, such as those we have been considering, we would expect K 9 to decrease with increase of temperature because more molecules of products would Ke =
Fig. 15.10 Variation of equilibrium constant with temperature
50 40
•
N
(Values of K9 with pe = 1 bar)
30
_
20 In K°
•,.. .. 10 8
,..., 42 .i.
6
Cb
1 y,
4
0 1.,, .....z.
''''.::?b, •
%5 ,0 2,..
"...
\
00 ,
2
0
500
1000
1500
20(X)
2500
3000
Temperature/[K]
353
[15.7]
Applications to Particular Fluids
receive sufficient energy in collisions to dissociate. That 1q02 and 1q4,0 decrease strongly at very high temperatures is indicated in Fig. 15.10. It is usual to plot and tabulate values of In 10 rather than values of Ke. This is because graphs plotted logarithmically cope more easily with the wide range of variation of 10, and linear interpolation from tables of In IC° provides values which are closer to the true values than would be obtained from linear interpolation between values of IC'. Moreover, thermodynamic theory normally requires values of In IC' (see equation (15.19)). Values of In IC' for several reactions of importance in combustion are tabulated against temperature in Ref. 17. The following example illustrates the method of calculating the equilibrium constant when the percentage dissociation has been obtained by a products analysis, and also how this equilibrium constant can then be used to predict the percentage dissociation in other circumstances.
Example 15.10
The products from the combustion of a stoichiometric mixture of CO and 02 are at a pressure of 1 bar and a certain temperature. The products analysis shows that 35 per cent of each kmol of CO2 is dissociated. Determine the equilibrium constant for this temperature, and thence find the percentage dissociation when the products are at the same temperature but compressed to 10 bar.
The combustion equation for the reaction to products in equilibrium is CO + 102 (1 — a)CO2 + aCO + la02 where a is the fraction of CO2 dissociated. At 1 bar the products consist of 0.65 kmol CO2 + 0.35 kmol CO + 0.175 kmol 02 The total amount of substance of products is 1.175 kmol, and' the partial pressures of the constituents in bar are therefore Pco2 =
0.65
nco, n P
1.175
x 1 [bar] = 0.553 bar
ncp 0.35 x 1 [ bar] = 0.298 bar Pco = TP = I 1.175 no, P°2
=
0.175 x I [bar] = 0.149 bar = 1.175
Based on the equilibrium equation CO + 10 2 N.=  . CO2, Ke = (Pc°2"1112 =
(Pco)(Po2 )112
0.553 0.298(0.149)1/2
= 4.81
At any pressure p, the partial pressures will be Pco, — 354
1— a 1 + a/2
P, Pco =
a/2 a P P, Po = ' 1 + a/2 1 + a/2
Combustion Processes
[15.7]
And the equilibrium constant will be (1—a Ke =
p(r,e)1/2 + a/2) x ( a )( a/2 )1/2 p X p112 1 + a/2 1 + a/2
(15.22)
Since the temperature is unchanged, 10 will still equal 4.81. At 10 bar, therefore, 4.81 —
(1 — a)(2 + a)1/2
a 3/2
1 x 101/2
Squaring and simplifying, we have 230.4a 3 + 3a = 2 and the solution, by trial and error or graphical means, is a = 0.185. Thus the dissociation is 18.5 per cent of the CO2 . The preceding example illustrates the important point that although the
equilibrium constant is independent of the pressure of the reacting mixture, the actual fraction of the dissociated product usually varies with pressure. Inspection of equation (15.22) in the example shows that the term containing p only vanishes when the amountofsubstance of dissociating compound and of dissociated constituents is the same. We may now see how a knowledge of the equilibrium constants enables the combustion equation to be established, and the adiabatic combustion temperature to be predicted, for the reaction of Example 15.7. The reactants are liquid heptane and air in stoichiometric proportions. Assuming that some of the CO2 and H2 O molecules have dissociated, the combustion equation will be 79 Tx 79 C,H,6 + 11V2 + 112 0( + aCO2 + bH2 0 + cCO + d02 + er3.2 + —111'4 2 21 21 There are five unknowns: a, b, c, d and e. Three equations can be written down directly by equating the number of atoms of carbon, hydrogen and oxygen on each side of the equation:
a+c=7 2b + 2e = 16 2a + b + c + 2d = 22 The remaining equations can be formulated with the aid of the equilibrium constants, which establish the proportions in which CO2 , CO and 02 , and H2O, H2 and 02 , can exist in equilibrium. If n is the total amountofsubstance of products, given by 79 n=a+b+c+d+e+ —11 21 355
[15.7]
Applications to Particular Fluids
then the partial pressures are a Pco, = — P+ Pco = T P, etc. n I The two equations are therefore a (co + 402 ,=s co2)
(H2 + 1 1 02 726 H2 0)
p e )1/2
K—
c(d/n)112 p b 20 = p e(d/n)
Since p appears in these equations, the pressure at which the reaction occurs must be known. (In Example 15.7 this was irrelevant because the enthalpies can be assumed to be independent of pressure.) Assuming the pressure is specified, there is still the difficulty that the dissociation constants are functions of the unknown temperature. The method of solution is to assume a final temperature, obtain the appropriate values of Ke from tables, e.g. Ref. 17, and then solve the five simultaneous equations for a, b, c, d and e. Once the composition of the products is known, the final temperature can be computed from the energy equation. If this does not agree with the assumed temperature, a better approximation to the values of 10 can be obtained and the calculation repeated until the desired agreement is reached. The energy equation for the reaction in Example 15.7 must now be written more generally as (Hpr — Hp298 ) + AH298 + (HR298 — HR288 ) = 0 AH298 replaces AF298 because, although we are still relating the solution to 1 kmol of heptane, Ag288 must be modified to make allowance for the unburnt CO and H2 in the products; that is, I 6S298 1 must be decreased by the magnitudes of the enthalpies of combustion of c kmol of CO and e kmol of H2. The numerical solution of such a dissociation problem is too lengthy to be given here, but the reader can find some simple problems in Appendix B and a variety of worked examples in Ref. 7. When the fuel/air mixture is appreciably richer than stoichiometric, it will be found that the amountofsubstance d of oxygen in the products is negligible. A somewhat simpler treatment involving only one equilibrium constant can then be used. The argument rests on the fact that the oxygen produced by the dissociation of CO2 can be regarded as being wholly used in the combustion of H2 . The two reaction equations CO 1 f02 74 CO2 and H2 + ZO2 7'2 H2 O can then be combined to yield the socalled water—gas reaction CO2 + H2 7± CO 1 H2 0 With the 02 eliminated from the products, one fewer equation is required, and the water—gas equilibrium constant is all that is needed for the solution of the 356
Combustion Processes
[15.7]
simultaneous equations. Values of Ke =
(PH,o)(Pco)
(Pn2 )(Pco,) are also given in Ref. 17. The foregoing method of solution is for an adiabatic steadyflow process at a known constant pressure, such as occurs in a ram jet combustion chamber. (This type of process also occurs in gas turbine combustion chambers, but the temperatures are too low for dissociation to be significant.) In the cylinders of many reciprocating internalcombustion engines the reaction occurs at substantially constant volume and the final pressure is unknown. The following example deals with this case, using carbon monoxide as the fuel for simplicity.
Example 15.11
The analysis of the products obtained from the adiabatic combustion of a stoichiometric mixture of CO and air at constant volume showed that there were 0.808 kmol of CO2 , 0.192 kmol of CO and 0.096 kmol of 02, per kmol of CO in the reactants. The initial pressure and temperature of the reactants were 1 atm and 333 K, and the final temperature was found to be 2742 K. Check the accuracy of the results by an atom balance and by verifying that the equilibrium condition is satisfied.
The reactants for a stoichiometric mixture, per kmol of CO, are CO +
)1 + (79  N2 21 2
The combustion equation for the reaction is therefore CO + 0.5 02 + 1.881 N2 > 0.808 CO2 + 0.192 CO + 0.096 02 + 1.881 N2 Checking the atom balance we have (C) 0.808 + 0.192 = 1 (0) 1.616 + 0.192 + 0.192 = 2 The relevant partial pressures are 0.808 Pco, =
Pco =
0.192 n
Po, =
0.096
P
Since the reactants and products are assumed to he perfect gases, and the reaction occurs at constant volume, n, AT,
niZT
Pi where subscript 1 refers to the initial conditions. The amountofsubstance of reactants is n1 = 1 + 0.5 + 1.881 = 3.381 kmol 357
[15.7]
Applications to Particular Fluids
and pi = 1 atm = 1.013 25 bar and T1 = 333 K. Hence p
p, T
1.013 25[bar] x 2742[K]
n
n t Ti
3.381 [kmol]'x 333[K]
— 2.468
bar kmol
The equilibrium constant is Pco,
(nco, n
IC° — Pco)(Po2 )112 ( Pe Pe
nco P n
P
no2 np
112
0.808 [kmol] 0.192 [kmol; ( 2.468 [bar] 0.096 [kmol] y/ [kmol] 1 [bar]
2
=8.65
This is in good agreement with the linearly interpolated value obtained from Ref. 17, which is 8.64. The check can be completed by showing that the energy equation is For this adiabatic constant volume process, the energy equation will be satisfied. For // UP298) + A U2  (UR298 UR333) = AU25 is the internal energy of combustion of 0.808 kmol of CO, per kmol of CO supplied in the reactants.
The treatment of the combustion of hydrocarbon fuels in air given here requires some qualification. First, at high temperatures nitrogen is not the inert gas we have hither supposed it to be; some of it combines withoxygen to form nitric oxide according to the equation 102 + 11%1.2 NO. The combination is endothermic and causes a reduction in products temperature. Secondly, some of the molecules of water vapour dissociate not only into hydrogen and oxygen, but also into hydrogen and hydroxyl (1H2 + OH H2 0). And finally, some of the molecules of oxygen, nitrogen and hydrogen dissociate into their respective atoms. The dissociation constants for all these reactions are known, and their effect on the products temperature can be taken into account in more accurate calculations. It must be emphasised that dissociation does not affect the internal energies and enthalpies of combustion, which are determined at about atmospheric temperature. In general, if the products of combustion of a hydrocarbon fuel—air mixture are cooled below 1500 K before leaving the system, the chemical energy liberated is not much affected by dissociation. As the products of combustion are cooled, the dissociated products recombine and the combustion is effectively complete below 1500 K.* The efficiency of the combustion process itself is therefore not affected by any dissociation that may occur due to a high temperature reached at some intermediate stage. The efficiency of a power plant * When the products are cooled very rapidly, however, as when a sample is withdrawn through a watercooled sampling tube, the reaction rates may be reduced to such an extent that very little recombination takes place.
358
Combustion Processes
[15.8]
in which the combustion process occurs may be affected, however, because the heat transferred to the working fluid is now transferred at a lower average temperature—the maximum temperature reached being reduced by the dissociation. In other words, the quantity of energy liberated is the same as if there were no dissociation, but its effectiveness for producing work is diminished. For steam or gas turbine plants this point is of no importance owing to the use of relatively low maximum temperatures imposed by the metallurgical limit. The discussions in sections 17.4 and 18.4.2, however, indicate that dissociation is an important factor limiting the efficiency of reciprocating internalcombustion engines and rocket motors.
15.8 Tabulation of thermodynamic reaction data
It is worth emphasising that although this chapter has been concerned with the particular class of chemical reaction known as combustion, most of the theory presented applies equally to chemical reactions in general. The enthalpy of combustion, for example, is then referred to as the enthalpy of reaction. In this wider context, it is impracticable to tabulate the enthalpies of all reactions which a chemical compound may undergo with other substances. Instead it is the enthalpy of formation Alifo which is tabulated and, as will be shown, it is a simple matter to calculate the enthalpy of reaction Arlo in any particular case from the values of A, of the substances taking part in the reaction. The enthalpy of formation is defined as the increase in enthalpy when a compound is formed from its constituent elements in their natural forms and in a standard state. It is usually expressed in energy units per unit of amountofsubstance of compound, and is referred to the case where each of the reacting elements is at pe = 1 bar and To = 25 °C = 298.15 K and the product is at the same pressure and temperature. The qualification 'natural forms' implies that it is the enthalpy of formation of, say, gaseous hydrogen H2 , and not that of the dissociated monatomic gas H, which is put equal to zero. Of course some elements may exist in several 'natural forms' and only one can be used as a datum state; for example, for carbon it is graphite and not diamond which is used for this purpose. The enthalpies of formation of three compounds at To = 25 °C are as follows: C(graphite) + 2H2 CH4; (425)cii, = — 74 870 kJ/kmol of CH4 C(graphite) 02 CO2; (Arlf25)CO, = 393 520 kJ/kmol of CO2 H2 + 402 H2 0( vap);
(425)H2 0 = —241 830 kJ/kmol of H2 O
Since the change of enthalpy is independent of the process by which the end state is reached, we can view a reaction in two stages: a breaking up of the reactants into elements, followed by a recombination to form the products. Thus to find the enthalpy of reaction of methane and oxygen we can write CH4
202 C + 2H2 + 202 + CO2 + 2H2 0( yap) 359
Applications to Particular Fluids
[15.8]
and hence Aks = (Agus)co, + 2 (gr2s)u2 o — ( 4 k2s)cui4 — 2 (AE125)02 = ( —393 520) + 2( —241 830) — ( —74 870) — 0 = — 802 310 kJ/kmol of CH4 Two important points must be made here. First, the reader is reminded that Chapter 7 is intended to be studied on a second reading of the book. The same applies to the remainder of this chapter which requires an understanding, in particular, of section 7.9.3. Secondly, near the end of section 15.4.1 it was suggested that the superscript e, which refers to properties at the standard pressure p° = 1 bar, can safely be omitted. This was because we were going to assume that, in the absence of changes of phase, the properties U and H of reactants and products can be taken as independent of pressure. In the following we shall be dealing with two properties, namely the entropy S and the Gibbs function G (or their molar equivalents g and 0), and even for perfect gases these are strongly dependent on pressure. In view of this we shall revert to the more rigorous notation incorporating the superscript e for properties at standard pressure. For consistency the superscript will be attached not just to S and G, but also to U and H, although in the latter case we shall neglect variations with pressure where appropriate. We have seen in section 7.9.3 that data for enthalpy of reaction AR, change in Gibbs function An and equilibrium constant Kt are interchangeable. Thus from equations (7.72), (7.73) and (7.75), —Adt = —Aht + To(slo — Kilo) (15.23) In Kt = —Ago (15.24) R To By virtue of the Third Law (see section 7.9.1), which enables absolute entropies to be determined for the reactants and products relative to a common datum at absolute zero of temperature, the entropy term in equation (15.23) can be calculated. The Gibbs function of formation Ago can then be defined in an analogous manner to the value of AiiTo; and the values of e0T, for any reaction can be found by adding the formation values as for AR. Consequently it follows from equation (15.24) that it is also possible to define logarithms of the equilibrium constant of formation In K,90, from which the logarithm of the equilibrium constant Kt for any reaction can be calculated from a similar summation procedure.* A short compilation of various chemicalthermodynamic data from Refs 36 and 37 is given in Fig. 15.11; it contains values of Ah?0, * Because values of In KS) can be found from additions of the appropriate values of In Ka,, it follows that values of K?, can be found by multiplication of the Ka, values. This should also be clear from the definition of the equilibrium constant in section 15.7.2 since, by multiplication of suitable equilibrium constants and cancellation of partial pressure terms, any required equilibrium constant can be found.
360
Combustion Processes
[15.8] Fig. 15,11
at pe = 1 bar and To = 298.15 K
A selection of chemical thermodynamic data
th kg 1 L kmol _I
F C (graphite) C (diamond) C (gas) CH4 (gas) C2144 (gas) CO (gas) CO2 (gas) H (gas) H2 (gas) OH (gas) H2 O (liq) H2 O (vaP) N (gas) N2 (gas) NO (gas) 0 (gas) 02 (gas)
12.011 12.011 12.011 16.043 28.054 28.0105 44.010 1.008 2.016 17.005 18.0155 18.0155 14.0065 28.013 30.006 15.9995 31.999
Ara kJ 1 Lkmol i
r
0 1 900 714 990 74870 52 470 110530  393 520 217 990 0 39 710 285820 241830 472 650 0 90 290 249 170 0
r
A 0 ro kJ 1
Lkmoli
r ln K,%.
0 2 870 669 570 50810 68 350 137160 394390 203 290 0 35 010 237150  228 590 455 500 0 86 600 231 750 0
ape° kJ 1
LkmolKi
0 1.157 270.098 20.498 27.573 55.331 159.093 82.003 0 14.122 95.660 92.207 183.740 0  34.933 93.481 0
8.53 6.06 20.84 35.64 42.89 29.14 37.13 20.79 28.84 29.99 75.32 33.58 20.79 29.21 29.84 21.91 29.37
...e so kJ 1 kmol K i 5.69 2.44 158.10 186.26 219.33 197.65 213.80 114.71 130.68 183.61 70.00 188.83 153.30 191.61 210.76 161.06 205.14
and the absolute molar entropy In K lo and also of the molar heat capacity g7), all in the standard state of p° = 1 bar and To = 298.15 K. Both the enthalpy and the equilibrium constant for perfect gases are independent of pressure, and in practice the data for AFt% and In iqc, can be assumed to be constant for real gases and vapours over wide ranges of pressure. Similarly, these values are very nearly independent of pressure for liquids and solids. The Gibbs function, however, involves an entropy term which varies appreciably with pressure for gaseous substances (although not for liquids and solids), and this variation must be taken into account when any gaseous reactants or products are not at the standard pressure of 1 bar. A particular difficulty appears with regard to substances which cannot exist at the standard state. Thus H2 O vapour cannot exist at 1 bar at 25 °C, and H2 O in the standard state can exist only as a compressed liquid. The tables make use of a fictitious vapour at the standard state, obtained by assuming that the substance behaves as a perfect gas between the saturated vapour state at 25 °C (0.031 66 bar in the case of H2 O) and the standard state. This is permissible because we are interested only in using tabulated data to calculate changes in h or 0 . As an example, let us consider the differences between the tabulated liquid and vapour values for water. For the enthalpy of formation, omitting the subscript 25 for brevity, we have (Aiin,ap at 1 bar  (Ag?),Iq at 1 bar = {(4Envap at 1 bar  (AFf )Vap at 0.03166 bar} + (AFf)Vap at 0.03166 bar  (AXON at 0.03166 bar} ce p
+ {(Akf)iict at 0.031 66 bar  (gni:q at 1 bar} =0+ 43 990 kJ/kmol of H2 O + 0 =
361
[15.8]
Applications to Particular Fluids
The first and third terms are zero because the enthalpy of vapour and of liquid is taken as independent of pressure; the middle term represents the latent enthalpy of vaporisation per kmol of H2 O. Considering the Gibbs function of formation, again at 25 °C, we have (Aar)vap at 1 bar — (Adr)liq at 1 bar = {(6,0)„.p at 1 bar — (Ajf )„ at 0.031 66 bar}
+ {(4)„ at 0.03166 bar — ( NAN at 0.03166 bar} + {OM" at 0.03166 bar — (Agniq at 1 bar} = 8.3145 x 298.15
kmol
In
1 + 0 + 0 = 8559 kJ/kmol of H2 0 0.03166
The first term represents extrapolation to the fictitious vapour state using (15.23) and assuming that the vapour behaves as a perfect gas over that range. The second term is zero because the Gibbs function remains constant in an isothermal change of phase (see sections 7.7 and 7.9.1), and the third term is zero because the Gibbs function of a liquid is taken as independent of pressure. Finally, considering the entropy at 25 °C we can write (r)vap at 1 bar — (3e)liq at 1 bar = {(31,ap at 1 bar — (3), at 0.031 66 bar} •
{(§),,p ,
at 0.031 66 bar — (3"),i, at 0.031 66 bar}
+ {MN at 0.031 66 bar — (nog at 1 bar.} kJ + 43 990 [kJ/kmol] = —8.3145 [ 1 1n 1 +0 kmol K 298.15[K] 0.03166 = ( —28.71 + 147.54)[kJ/kmol K] = 118.83 kJ/kmol Or, since g = — Ts and the temperature is constant at To, the change in entropy can also be found from T,
Age (43 990 — 8559)[kJ/kmol] — 118.83 kJ/kmol K To — 298.15[K]
We conclude this brief explanation of the way thermodynamic reaction data are presented with an example illustrating their use to calculate the values of Ali, Ag and K for a reaction at .a specified temperature and pressure which differs from the standard state. Example 15.12
Calculate Ali, A# and In Ke at 298.15 K for the reaction CO2 + H 2 CO + H2 0 ( \tap)
where the total pressure of the reactants and products is 1 bar each. Use the data on Fig. 15.11 and check them for consistency. Also calculate the value of In 1(9 at T = 400 K, using first equation 362
Combustion Processes
[15.8]
( 15.24 ) and secondly equation (7.7 7 ); assume in each case that the molar heat capacities ep are constant over the temperature range considered. 298.15 K The enthalpy of reaction Ah398 when each constituent is at 1 bar is
Enthalpy, Gibbs function and equilibrium constant at
AE398 = {( — 110 530) + (241 830) — ( —393 520) — 0}[kJ] = +41160 kJ This will also be equal to tg298 for the specified pressure of each reactant and product (in this case 0.5 bar each), because the enthalpy can be taken as independent of pressure. The change of Gibbs function Q398 is given by 6,4398 = {( — 137 160) + (228 590) — (394 390) — 0} [kJ]
= + 28 640 kJ To find the change of Gibbs function for the reactants and products each at 0.5 bar, the Gibbs function of each term will have to be modified by nf?' To In(p°/ p), where p$ = 1 bar and p = 0.5 bar. It is obvious that these modifications (with appropriate signs) will cancel in this case and Ag298 = Ag398; there will be a net effect only when the reaction is such that the amountofsubstance of the gaseous products differs from that of the gaseous reactants. The equilibrium constant is In Ke = 55.331 + 92.207 — 159.093 — 0 = —11.555 To check for consistency,
let us first apply equation (15.23);
— AE298 = — 9298 — TO( E nA298 — EnA298
P
R
= —28640[kJ] — 298.15[K]{(1 x 197.65) +(1 x 188.83) — (1 x 213.80) — (1 x 130.684 k
kJ]
= { —28 640 — (298.15 x 42.00)}[kJ] = —41 160 kJ Also, from equation (15.24), In Ke =
A9298
RT0
=
28 640 — —11.553 8.3145 x 298.15
Equilibrium constant at 400 K To calculate the value of In 1(7, at T = 400 K using equation (15.24), we will first write equations for AhT and (SPT — SRT ) at T, taking the values of "el, from Fig. 15.11. From equation (15.10), '
AFT = {(1 x 29.14) + (1 x 33.584 kj ](T — 298.15[K]) + 41 160[K] i 363
[15.9]
Applications to Particular Fluids
+ {(1 x 37.13) + (1 x 28.84)1[]298.15[K] — T) = 41 160 — 3.25 ( T — 298.15) } [kJ] = ( 42 130 — 3.25 T —) kJ [K] [K] and remembering that the pressure terms cancel in this case, (SRT — SRT ) = E ni epi lri
TO
+ E nA298 P
= (42.00 — 3.251n
T° E niep, In —
E nigi298
1 kJ 298.15[K])K T
At T = 400 K, A4T =
AFT  T(spT — sRT)
= {42130 — ( 3.25 x 400)} — 400 ( 42.00 — 3.251n
400 ) [kJ] 298.15
= +24410 kJ and from (15.24), In K €7', —
24 410 — 8.3145 x 400
7.340
Alternatively, using equation (7.77) and treating Ah as a variable between T0 and T, T
.T
d(In KG) = 1 f Agd(1) 7, IT° R ro and hence, using the intermediate result for AFT above, ln KL0 — ln K398 =
8.3145 f
f T (42 130
3. 4[(]) [K]/T) T
To
1 42 130 8.3145 T/[1(]
1 ( 42 130 8.3145 400
3.25 In [IC] T 42 130 298.15
T
To
3.25 ln 2"'15 = +4.213 400
Thus, using In Ke = —11.555 at 298.15 K from the first part of the example, In K:00 = 4.213 — 11.555 = —7.342 which agrees closely with•the result obtained above. 15.9 Limitations of the thermodynamic analysis
In the previous chapter it was emphasised that the thermodynamic analysis of the processes occurring in condensers and airconditioning plant is limited to 364
[15.9]
Combustion Processes
the prediction of final states and energy tralisfers from a knowledge of the initial states and certain operating conditions. A more detailed analysis of the way in which heat is transferred must be undertaken before an actual plant can be designed. The thermodynamic analysis of combustion processes, given in this chapter, is limited in a similar way: it does not enable us to specify the conditions under which the process can actually be carried out in practice. For example, it cannot be used to predict the air/fuel ratio and initial temperature necessary for selfignition to occur. Nor has the simple thermodynamic treatment anything to say about the rate at which the process can be carried out; for example, it cannot predict flame speeds, or the conditions under which a stable flame is possible, or the delay periods experienced in internalcombustion engines. A great deal of empirical data has been amassed over the years to explain the detailed phenomena encountered in practical combustion systems such as coal and oil fired furnaces, gas burners, reciprocating engines, gas turbines, ramjets and rocket motors. The concepts necessary for a synthesis of this mass of data are now being formulated with the growth of the fundamental sciences of combustion kinetics and combustion wave theory. Quantitatively there is still a wide gap to be bridged before these sciences can be applied directly so that new combustion systems can be designed on the drawing board, but even now they can be used to aid consistent thinking and to reduce the amount of ad hoc development which is still required before a new design can be made to work efficiently. Ref. 30 provides an introduction to combustion kinetics and combustion wave theory.
365
Part Ill Work Transfer
Introduction
So far in this book we have been concerned mainly with relations between fluid properties and the quantities of work and heat which accompany changes of state. Before it is possible to design plant which will effect the desired changes of state, it is necessary to analyse the mechanisms of work and heat transfer in some detail; the former mode of energy transfer is discussed here and the latter in Part IV. This division is easily justified in such cases as steam plant, refrigeration plant and airconditioning plant, because the work and heat transfers are carried out in separate components. It is not so easily justified when considering reciprocating air compressors or internalcombustion engines. To cover these latter examples it may be said that Part III deals with those systems whose main purpose is the transfer of work and for which exchanges of heat with the surroundings are only incidental. Fundamentally, there are two types of machine used to perform the process of work transfer: (a) positive displacement machines, and (b) nonpositive displacement machines. The former comprise all reciprocating expanders and compressors and also some types of rotary compressor such as the Roots blower and the vane pump. The features common to class (a) are: these machines possess members (e.g. pistons and valves) which ensure positive admission and delivery of the working fluid and prevent any undesired reversal of flow within the machine; their operation is intermittent and they subject the fluid to nonflow processes; and work is transferred by virtue of a hydrostatic pressure force exerted on a moving boundary. In nonpositive displacement machines, which comprise axialflow and radialflow turbines and compressors, there are no means for preventing a reversal of flow in the machine; the processes are steadyflow processes; and work is transferred by virtue of the change in momentum of a stream of fluid flowing at a high speed over blades or vanes attached to a rotor. In all practical power plant, work is done during successive compressions and expansions of the working fluid. To obtain a net amount of work, it is essential to change the stage of the working fluid between the compression and expansion processes. So far we have mainly considered plant in which this change of state is brought about by external heat addition, e.g. steam power plant and closedcycle gas turbine plant. The one exception in Part II has been the opencycle gas turbine wherein the change of state is effected by a chemical 369
Introduction
reaction. In Part III we shall describe the reciprocating internalcombustion engine, where the compression, change of state by combustion, and subsequent expansion are all performed in a single component—the engine cylinder. Reciprocating internalcombustion engines fall within the class of positive displacement machines, as does the newer rotary type known as the Wankel engine which is also described briefly. The scheme of Part III may now be outlined. Chapter 16 deals with positive displacement compressors and expanders, with the reciprocating air compressor and steam engine discussed as important examples of each type. The following chapter describes the processes in positivedisplacement internalcombustion engines. The knowledge of nonflow processes already gained from a study of Parts I and II is adequate for the purposes of these two chapters. For a study of nonpositive displacement machines, however, the treatment of steadyflow processes given so far is insufficiently detailed; we need to know something about the nature of the flow within the open system. Chapter 18 analyses the simplest type of flow—onedimensional steady flow—and the results are then applied in Chapter 19 to the processes which occur in nonpositive displacement machines. When dealing with stationary power plant, the useful net work is always delivered by the engine as a torque in a rotating shaft. When the power plant is used for propelling a vehicle, this need not necessarily be the case. Admittedly in rail, road and ship propulsion the power is usually delivered via a shaft, but in the more recent developments of aircraft propulsion the force required to move an aircraft against atmospheric drag or gravitational pull is derived without the intermediary of shaft work. The analysis of the behaviour of jet power plant is basically a problem of onedimensional flow, and as such it is treated in Chapter 18. Finally, it should be realised that the major fraction of the total mechanical work produced by the world's power plant is utilised in the production of electrical power, i.e. it is used to drive electric generators. If the primary source of energy—whether chemical or nuclear—could be converted directly into electricity, both a higher efficiency and an overall simplification of plant might be attained. Part III closes with a chapter describing briefly the main devices which are being developed for direct conversion. The excuse for including this topic in a part entitled 'Work Transfer' is that in principle electrical and mechanical work are mutually convertible without loss and in this sense are equivalent.
370
16 Reciprocating Expanders and Compressors
The function of a compressor is to admit fluid from a lowpressure region, compress it, and deliver it to a highpressure region. An expander carries out the reverse processes with the object of producing work. Although this chapter is mainly concerned with reciprocating machines, of which the air compressor and steam engine are considered as typical examples, the last section deals with rotary positive displacement compressors. These are more akin to their reciprocating equivalent than they are to the nonpositive displacement compressors described in Chapter 19, even though the latter are rotary machines. The essential feature common to all positive displacement machines is that the fluid is prevented by a solid boundary from flowing back in the direction of the pressure gradient. All the compressors described here are therefore capable of producing large pressure ratios. As already pointed out, reciprocating machines can be regarded as open systems being steadily supplied with working fluid and transferring work and heat between the fluid and its surroundings at a uniform rate. Nevertheless the internal processes are intermittent, and this fact imposes an important limitation on reciprocating machines—the comparatively low rate at which machines of reasonable size can handle the working fluid.
16.1 Work transfer in reversible reciprocating machines
A reciprocating machine consists essentially of a cylinder and a piston, with the piston connected to a rotating shaft by a connecting rod and crank as shown in Fig. 16.1. Valves permit the fluid to flow into and out of the cylinder at appropriate times. The total piston travel is called the stroke, and the volume displaced is called the swept volume. There is always some minimum volume, the clearance volume, when the piston is at the end of the stroke. This is necessary to accommodate the valves and avoid contact of piston and cylinder head. The succession of events can best be explained with the aid of a diagram (Fig. 16.2a) showing how the pressure in the cylinder varies during one revolution of the crankshaft, i.e. during one complete machine cycle. The change in state of the fluid as it passes through the machine will be depicted on a p— v diagram (Fig. 16.2b). We shall refer explicitly to the operation of an expander, and bear 371
[16.1 ]
Work Transfer Piston rings
Fig. 16.1 The reciprocating
Crank
expander or compressor •e1/4 Valves
Connecting rod
Crankshaft
111
Clearance volume Swept volume
Am,.
Fig. 16.2
p—V and p—v diagrams
p
for an ideal expander
I
Anti p
d
Arne K
AM f
ejected V (a)
(b)
in mind the fact that in a compressor the machine cycle is traversed in the reverse direction. The following analysis refers to an idealised machine in which the processes are reversible, the state of the fluid at inlet and outlet remains constant with respect to time, and the kinetic energy at inlet and outlet is negligible. a—b The inlet valve is open, and a mass of fluid Amf in state 1 enters the cylinder without change of state. It mixes reversibly with a mass Am, already present in the clearance volume in the same state 1. b—c Both valves are closed and the mass (Amf + Am,) changes its state during the expansion to pressure p2. c—d The exhaust valve is open and a mass Amf is ejected from the cylinder without further change of state. d—a Both valves are closed and a mass Am, is compressed to the original state 1. It is important to note that although Fig. 16.2a represents the events during a machine cycle, it does not represent a thermodynamic cycle. Admittedly the mass Am, is carried through a thermodynamic cycle, although it consists merely of the traversing and retraversing of a single path of states as shown on the p—v diagram of Fig. 16.2b. But the mass Amf is not carried through a cycle at all, and simply has its state changed from state 1 to state 2. Before the work done can be estimated, the processes of expansion and compression between states 1 and 2 must be defined. Since the speed of flow 372
[16.1 ]
Reciprocating Expanders and Compressors
through the machine is not very great, these processes cannot be assumed to be adiabatic. A better approximation is to assume that they are polytropics, i.e. of the form pV" = constant. An expression for the work done can be derived in two ways: either by considering the forces on the piston during a complete machine cycle, or by applying the steadyflow energy equation between inlet and outlet of the machine. The same assumption of constant inlet and outlet conditions has to be made in both cases. That is, it must be assumed that there is sufficient intake and receiver volume for the intermittent working of the machine to make a negligible difference to the fluid properties at inlet and outlet.
16.1.1 Machine cycle analysis
The net work done per machine cycle is the algebraic sum of the work transfers in the four processes, each of which can be found from pA dL or I p dV. A is the area of the piston and L is the distance moved. Referring to Fg. 16.2, d a b c dW = — f pdV — f pdV — f pdV — f pdV = — pdV .. d a b c The magnitude of cf clW is evidently equal to the area of the p— V diagram. Carrying out the integration, making use of equation (3.12), we have dW= —pi (Vb — Va) +
=
n—1
{13
(P2 vc — Pi vb)
n—1
P2(vd ve) +
(Pi
v. — P2 Vd) n—1
— Vb) + P2(Vc K)}
The work done can be expressed in terms of the fluid properties at inlet and outlet by noting that Vb = (Am f + Ama )v,
Va = Amc v,,
= (Amf + Amc)lly, Vd = Ame ll2 We then have d W = Am f
n n—1
(lo2v 2 — Pivi)
(16.1)
The rate of work done is obtained by multiplying the net work done during the machine cycle by the number of cycles N per unit time. If the mass flow per unit time (NAmf ) is denoted by th, the rate of work done is = th
n—
(16.2)
1 (P2v2 — vi)
Equation (16.2) can be recast in terms of the pressure ratio as follows: 14/ =
v
n
p 2 v2
1)
n
373
[16.11
Work Transfer
and since v2 /v1 = (P1/P2)11n, W =
tripl y,
n p2 )( n "In n 1Rpi j
_
1
)
(16.3)
Identical expressions are obtained for the case where the machine cycle is carried out in the reverse direction as in a compressor; p2 is theri greater than Pi and W becomes a positive quantity. The exact path of the expansion and compression processes, i.e. the value of the polytropic index n, depends upon the heat flow through the cylinder walls. Ideally, heat is only transferred during the processes bc and da, because processes ab and cd are merely mass transfers to and from the cylinder without change of state. The heat transferred during the compression of Am, along da is equal and opposite to the heat transferred during its expansion from b to c. The net heat transfer per machine cycle is therefore that associated with the expansion of Amf along bc. Since the system is closed during this process, the appropriate energy equation is 2 dQ = Amf (u2  u1 ) + Amf f
p dv
1 , = Amf (u2  ui )  Amf n  02v2,  PILO 1 Since u = h  pv, this can also be written as dQ = Amf(h2  h i )  Amf
n 1 (p2v2  pi th) n
The rate of heat transfer per unit time is therefore = th(h2  hi)
n (p2 v2  p i v i ) mn  1
(16.4)
16.1.2 Steadyflow analysis The foregoing expressions for the work and heat transfers can also be obtained by applying the steadyflow energy equation, without the necessity for such a detailed analysis of the events which take place within the cylinder. The energy equation, neglecting the kinetic energy terms, has been shown in section 10.4 to lead to 2 1/V = rim f
V
(16.5)
dp
Making the further assumption that the reversible process is polytropic, as before, we can perform the integration and obtain 14/ 374
ril
n1
(P2 v2 
vi,)
[16.2]
Reciprocating Expanders and Compressors
Fig. 16.3 Effect of polytropic index on the work transfer
n decreasing
n decreasing
\ Ii
2
and hence also, from the steadyflow energy equation, = th(h2 — h1)
n (p2 v2 — p, v1 )
n—1
These equations are identical with equations (16.2) and (16.4).
There are two important points to be noted from the analysis of the reversible reciprocating machine. (a) If the machine is an expander then the magnitude of the work increases as the value of n decreases, while for a compressor it decreases as n decreases. There is no need to evaluate equation (16.2) to show this; it is evident from the p—v diagrams of Fig. 16.3. Equation (16.2) is represented by (rim x shaded area), i.e. by rhfl v dp, and the negative slope of a polytropic curve decreases with decrease of n (section 3.4). (b) Equation (16.1) indicates that the clearance volume has no effect on the work done per unit mass flow. The mass Am, in the clearance volume is expanded and recompressed along the same state path and no net work is done on or by it. The clearance volume does, however, affect the capacity of the machine, i.e. the mass Am.,. of fluid which a cylinder of given size can handle per machine cycle. The greater the clearance volume per unit swept volume, the smaller the amount of fluid that can be handled by the machine. This will be shown formally for an air compressor in section 16.3. 16.2 The indicator diagram
There is one important respect in which the actual p—V diagram of all real reciprocating machines differs from the ideal diagram of a reversible machine. Owing to the fact that valves take a finite time to open and close, the corners of the diagram are rounded and ill defined. When a valve port is only partly open, throttling occurs and there is a considerable pressure drop in the direction of flow. Even when the port is fully open, some pressure drop is inevitable due to fluid friction. Thus the real p—V diagrams for an expander and a compressor appear as in Fig. 16.4a and b. It must be remembered, too, that in the real machine the expansion and compression processes will not necessarily be exactly polytropic. Since the real processes are not reversible, the actual work and heat transfers 375
[16.2]
Work Transfer Fig. 16.4
p
Effect of valve loss on the
p—V diagram: (a) expander; ( b) compressor
V
(b) Compressor
(a) Expander
Fig. 16.5 Recording drum
The mechanical indicator
Cord
.. Indicator cylinder
11111
cannot be individually expressed in terms of the fluid properties at inlet and outlet as in equations (16.2) and (16.4). Nevertheless a good approximation to the actual work done can still be obtained from f (force on piston x dL) or f p d V, provided the variation of average pressure in the cylinder is plotted during the machine cycle. Strictly speaking it is the pressure on the piston face which should be measured, but this presents too difficult a problem of measurement for ordinary purposes. (The error can become significant when considerable turbulence is present as in highspeed compressionignition engines; see section 17.3.2.) The real p—V diagram is obtained by fitting an indicator to the machine. Fig. 16.5 illustrates a simple mechanical indicator suitable for machines of low rotational speed.* The main part of the indicator is itself a small cylinder and piston which can be put into communication with the cylinder of the machine. The volume of the indicator cylinder must be small compared with the clearance volume of the machine cylinder, otherwise the diagram will be altered appreciably when the indicator cock is opened. The indicator piston is spring loaded so that its movement is directly proportional to the pressure, and this movement is magnified by a link mechanism connecting the piston and a pencil. The spring is calibrated, the spring constant k being expressed as the number of units of * Descriptions of other indicators, e.g. electronic and optical types, can be found in the Proceedings of the Institution of Mechanical Engineers and in the Transactions of the Society of Automotive Engineers. Such indicators are more suitable for highspeed machines because the inertia of their moving parts is much less than that of the mechanical indicator described here.
376
Reciprocating Expanders and Compressors
[16.2]
Fig. 16.6 Finding the mean effective pressure
Indicator card (b)
pressure required to move the pencil point vertically through unit distance. The pencil point moves along the surface of a drum parallel to its axis, while the drum is rotated by a cord connected, via a reducing linkage, to the piston of the machine. Thus while the pencil moves along the drum a distance proportional to the pressure, the drum surface moves past the pencil a distance proportional to the engine piston stroke and in phase with it. In this way the p—V diagram can be recorded on an indicator card wrapped round the drum. When the chart is unwrapped the area of the diagram can be measured with a planimeter, this area being proportional to the net work transfer per machine cycle. In practice the constant of proportionality is not evaluated, and the work done is usually deduced by making use of the concept of mean effective pressure already introduced in section 12.8. Consider the p—V diagram of Fig. 16.6a. The net work transfer per machine cycle can be expressed by Vb
dW = — f (Pi — P2) dV = — (Pt P2)A dL 0
where A is the area of the piston and L is the stroke. This can be written as d W = pm AL
(16.6)
where IL
Pm =
0
(P — P2) di,
Conventionally, pm is always treated as a positive quantity. Thus pm is the height of a rectangle of the same area and length as the p—V diagram. pm is known as the indicated mean effective pressure, and it can be regarded as that constant pressure which, if it acted on the piston over one stroke, would do the same amount of work as is done in one machine cycle. Since the actual indicator card is drawn to a reduced scale (Fig. 16.6b), it is first necessary to find its mean height all, say in cm, and then deduce pm in bar by multiplying the mean
377
[16.2]
Work Transfer
height by the spring constant k in bar/cm, i.e. k
Pm _
a/[cm2]
[bar] [bar/em] l/[cm]
(16.7)
The work done per machine cycle can then be found from (16.6). If N is the rotational speed in rev/s, A is the piston area in m2 and L is the stroke in m, the numerical equation for the rate of work done becomes A L N — 102 pm [kW] [bar] [m2 ] [m] [rev/s] 147 I
() 16.8
The work so found is known as the indicated power (IP). The power of machines is still sometimes expressed in horsepower units, and it is then referred to as the indicated horsepower (IHP). The British and metric horsepower units are related to the kilowatt by the following equation, to four significant figures: 1 1 kW = 1 British hp — metric hp 0.7457 0.7355 The actual power produced at the shaft of an expander will be less than the IP because some work is dissipated by friction between piston and cylinder and in the bearings. The shaft power (SP) is measured by some type of dynamometer,* of, which the friction brake is a common example, and consequently it is often referred to as the brake power (BP). The ratio qmech —
BP p
SP
or —
(16.9)
IP
is called the mechanical efficiency of the expander. If the machine is a compressor, equation (16.8) gives the rate of work done on the fluid by the piston. In fact more work than this must be supplied to the shaft to overcome mechanical friction losses, and the mechanical efficiency is therefore defined in this case as IP Ilmech — SP
(16.10)
For reasons similar to those given in section 12.8, a machine cycle yielding a high indicated mean effective pressure is likely to provide the basis for a compressor or expander having a high mechanical efficiency. In this section we have concentrated on the essential differences which exist between all real and ideal reciprocating machines. There are other differences which are peculiar to particular types of machine and these will be brought out in the following sections. For brevity we shall consider one example of a compressor, the air compressor, and one example of an expander, the steam engine.
* A description of the more common types of dynamonieter can be found in textbooks on mechanics of machines.
378
[16.3]
Reciprocating Expanders and Compressors
16.3 Reciprocating air compressors
One special feature of a compressor is the use of springloaded, nonreturn valves which open and close automatically (Fig. 16.7). This considerable mechanical simplification is made possible by the fact that the fluid is forced in the direction opposing the pressure gradient. In an expander it is necessary to use mechanically operated valves, timed to open and close by some linkage from the crankshaft. Automatic springloaded valves tend to be less positive in their action and lead to greater throttling losses than mechanically operated valves, but the mechanical simplification is considered to be worth the small amount of additional compression work entailed. A typical pV diagram is shown in Fig. 16.7. The wavy lines during the suction and delivery processes are due to valve bounce, which arises because initially a rather large pressure difference is required across the valves to overcome their inertia. Apart from these peculiarities the actual indicator diagram follows the ideal p V diagram closely, and for the remainder of this section only the ideal diagram will be considered. When air is the working fluid, the equation of state for a perfect gas enables equations (16.2), (16.3) and (16.4) to be put in the following form: 14/  rit 14/ = th
n R(T2  T1 ) n1 n
n1
RTl
(16.11)
{(p2 )(n  "1" _ 1 } Pi )
= Incp(T2 
th
n1
(16.12)
R(T2  T1)
Since R = cv(y  1), the last equation reduces to Q=
tyci,
nn1
cu(y 
.yn cv(T2  T1) =m1  n
(T2  T1 )
(16.13)
Fig. 16.7 Selfacting valves for a compressor and their effect on the actual indicator diagram
Fr/A r41 IA 12 FA r/A F./
379
[16.3]
Work Transfer
In section 16.1 it was pointed out that the work done on the air decreases as the value of n decreases. For this reason the compressor cylinder is either water cooled, or finned and air cooled. Even with good cooling the value of n is usually between 1.2 and 1.3, whereas the compression work is a minimum when n = 1, i.e. for an isothermal compression. (If n < 1 the air is cooled below the inlet temperature, implying the use of refrigeration on which work would have to be expended.) These considerations give rise to the practice of quoting the performance of a compressor in terms of an isothermal efficiency defined by
1 1180 
isothermal work actual indicated work
(16.14)
If the mechanical friction losses are included, we have the overall isothermal efficiency defined as the ratio of the isothermal work to the actual brake work. The reversible isothermal work cannot be obtained by putting n = 1 in (16.11), since this would yield the indeterminate solution 0/0. The anomaly arises from the fact that f dv/v is a special case off dv/vn, for which the solution is In v. A repetition of the derivation of equation (16.2) for the special case n = 1 can be shown to yield
Wino =
.
In P2 — = mR Pi
ln P2 Pi
(16.15)
This is the quantity used as the numerator in the expression for the isothermal efficiency (16.14). When the air is compressed nonisothermally, i.e. when 1 < n < y, the extra work expended is not necessarily wasted. If the highpressure air were to be used directly in an expander with the same polytropic index as the compressor, all the extra work could ideally be recovered. There are two main reasons why recovery is not feasible in practical applications. First, for n to lie between 1 and y during an expansion, heat has to be supplied to the air. But this heat cannot be drawn from the cooler surroundings, and some means would have to be provided for transferring the heat rejected during the compression directly to the expander in a reversible manner. Secondly, the compressed air is normally used some distance away from the reciprocating compressor and it cools to atmospheric temperature in the delivery pipe. In fact the air is sometimes cooled deliberately immediately after compression, to condense the water vapour always present in atmospheric air and permit it to be drained off. This cooling has the incidental advantage of reducing the air viscosity and volume flow and hence the friction losses in the delivery pipe. One other point noted in section 16.1 was the importance of the clearance volume in so far as it limits the mass flow which can be passed by a machine of given cylinder volume and speed. This consideration gives rise to another quantity used to assess the performance of a compressor—the volumetric efficiency. The volumetric efficiency is defined as the ratio of the actual volume induced per cycle to the swept volume. In terms of easily measured quantities 380
Reciprocating Expanders and Compressors
[16.3]
it is given by tivoi =
?nth N 17a
The quantity rim, is known as the free air delivery; it is the rate of volume flow measured at inlet (e.g. atmospheric) pressure and temperature. An expression for the volumetric efficiency of a reversible compressor can be deduced as follows. With reference to Fig. 16.7, Vb — Va V + V„, — Va oI=
Vs
Vs Vd Va
P2 lm — 1. =+ — — = 1 — Vd {(—) VS Vd V Vs Pi
(16.16)
Evidently with a fixed value of Vd / Vs, called the clearance ratio, the volumetric efficiency decreases with increase of pressure ratio. This is also obvious from Fig. 16.8a. At some pressure ratio the flow will be zero, but even before this extreme value is reached it is more economical to split the compression into two or more stages, rather than simply increase the size of cylinder to obtain the desired flow. The p—V diagram for a reversible twostage machine is shown in Fig. 16.8b. Air is compressed to some intermediate pressure pi in the lowpressure cylinder and is then transferred to the highpressure cylinder for final compression to p2. The intermediate pressure pi is determined by the relative values of the swept volumes in the two stages and their respective clearance ratios (see Example 16.1). The volumetric efficiency is usually expressed in terms of the firststage swept volume Vs, i.e. (Vb — Va )/Vs. If the whole compression were accomplished in the ldwpressure cylinder, the dashed curve in Fig. 16.8b indicates that the volumetric efficiency would be reduced to ( Vb — V'a )/ Va . An improvement in volumetric efficiency is not the only benefit to be obtained by compounding the compression. Equation (16.12) indicates that the work required decreases as the inlet temperature T, decreases. If an intercooler is fitted between the stages, cooling the air leaving the first stage to T, before it
Fig. 16.8 The effect of multistage compression on volumetric efficiency
381
[16.3]
Work Transfer
P
Fig. 16.9 The effect of intercooling
2
Intercooler
r
on the work of a Pi
twostage compressor
P2
Pi
V
enters the second stage, the work required to drive the second stage is reduced. Fig. 16.9 illustrates this; the shaded area represents the saving in work. Intercooling brings the compression nearer to the ideal of isothermal compression. With an infinite number of stages this ideal would be reached, but in practice more than three stages are not used unless unusually high pressure ratios are required. The actual saving in work depends on the choice of intermediate pressure. It is easy to show that in the case of reversible polytropic compression the total work required is a minimum when the work is divided equally between the stages. This applies to any number of stages, but here it will only be proved for the twostage machine. With complete intercooling to T1 at constant pressure, the total work required in the two stages is W=
+ Wi2 n
(n — 1)/n
ri Pi
= di n RT,{ n—1
p2 (n — 1)/n — 1
1} + rii n RT n—1 1
{(
pi
Differentiating with respect to pi and equating the zero, n —1 n
(
1
(n  "I" 1 1 in
pi
n— 1
pi
, p
_ 1)/n pli —2n)/n = 0
2n
Or
Pi = V(P2P1)
(16.17)
It then follows that PiiPi
= P2/Pi and 14/1i = 147,2
(16.18)
Finally, it is worth noting two mechanical advantages of compounding which help to offset the additional complication and cost. First, only the small highpressure cylinder need be designed to withstand the delivery pressure. Secondly, a multicylinder arrangement provides a less difficult balancing problem and entails the use of a smaller flywheel. In the whole of the foregoing analysis of reciprocating machines it has been implied that the working fluid is only introduced to one side of the piston. The 382
[16.3]
Reciprocating Expanders and Compressors
Fig. 16.10 The doubleacting compressor
Piston rod
Connecting rod
Crosshead guide
work capacity of the machine can be very nearly doubled if both sides of the piston are used; the machine is then said to be double acting. The chief difference in construction between a single and a doubleacting machine is that the latter requires the addition of a piston rod and crosshead, as depicted in Fig. 16.10, because it is necessary to seal the 'open' end of the cylinder with a gland. The piston performs two complete machine cycles per revolution. To determine the indicated power of a doubleacting machine, it is necessary to take indicator diagrams from each end of the cylinder, and evaluate each diagram separately. It must be remembered that the effective piston area (A in equation (16.8)) is not the same in each case; the crosssectional area of the piston rod must be subtracted from the piston area when evaluating the indicated power associated with the crosshead side of the piston.
Example 16.1
A singleacting twostage compressor with complete intercooling delivers 6 kg/min of air at 16 bar. Assuming an intake state of 1 bar and 15°C, and that the compression and expansion processes are reversible and polytropic with n = 1.3, calculate the power required, the isothermal efficiency and the free air delivery. Also calculate the net heat transferred in each cylinder and in the intercooler. If the clearance ratios for the low and highpressure cylinders are 0.04 and 0.06 respectively, calculate the swept and clearance volumes for each cylinder. The speed is 420 rev/min. (See Fig. 16.11.)
The pressure ratio per stage is r = Pi = P2 = I( 16 —) = 4 1 P t Pi The work done in the two stages is 141 =
+ 1472 —
n—1
RT,
1)1" — 1}
= 2 x 6 x13 x 0.287 x 288(40.3/1.3 — 1) = 2 x 13.50 = 27.00 kW 60 0.3
383
[16.3]
Work Transfer
Fig. 16.11
P
P2 h/
Pi e\
T = T1 If
Pi V
The isothermal work is = ?MT,. In P Z = — 6 x 0.287 x 2881n16 = 22.92 kW 1 Pi 60 and the isothermal efficiency is 22.92 = — 84.9 per cent W 27.00
t;9. =
The free air delivery is th
R T,
=
6 x 0.287
Pi
x 288 — 4.96 m3 /min 100 x 1
The temperature at the exit of each stage is 7'c = 7; = To11)/" = 288 x
= 397K
Hence the net heat rejected from each cylinder is found from the energy equation = rhc p( 'T, — T1 ) —
=
p(Tg — T1) — 4V2
6 = —0 x 1.005(397 — 288) — 13.50 = —2.55 kW
6
and from the intercooler = iiicp(T1 — 71) =
60
x 1.005(288 — 397) = —10.95 kW
The volumetric efficiency for each stage is found from (16.16) as = 1 — 0.04(41/1.3 — 1) = 0.924 1.1,2 = 1 — 0.06(4 1/1• 3 — 1) = 0.887 384
Reciprocating Expanders and Compressors
[16.4]
Hence for the first stage the swept volume is Vb
Vd
free air delivery speed x
4.96 420 x 0.924
= 0.012 78 m3
and the clearance volume is
V, = 0.04( Vb — Vd ) = 0.000 51 m3 For the second stage the swept volume is Vf
Vb =
1 free air delivery 1 4.96 —X — 0.003 33 m 3 rP speed x t1„„1, 2 4 420 x 0.887
and the clearance volume is Vh =0.06(1'—
V„) = 0.000 20 m 3
It must be noted that points d and e need not coincide on the indicator diagram because they represent different states and different clearance masses Am„ and Arna. In this particular case Ve = vh rplin = 0.00020 x 41/1.3 = 0.000 58 m3 16.4 The steam engine
The reciprocating steam engine is a particular type of expander designed to produce work from steam expanding from a high to a low pressure. It is used as an alternative to a turbine in small steam plant (up to a few hundred kilowatts) where a turbine would be very inefficient, and where the inherent intermittent working of a reciprocating machine, which allows only moderate rates of flow and rotational speeds, is no disadvantage. (The reasons for the inefficiency of small turbines will become apparent after a reading of Chapter 19.) The range of expansion for the engine is governed by considerations of the thermodynamic cycle, and it will be remembered from Chapter 11 that a very wide range of pressure is required if a steam cycle is to be efficient. This requirement leads to multistage expansion in successive cylinders, but only the singlecylinder steam engine is described here in any detail. There are two features peculiar to the steam engine which result in its ideal indicator diagram being different from the ideal diagram of an expander shown in Fig. 16.2a. The first lies in the fact that the temperature of the working fluid is always much greater than the surroundings. Thus, although the work done increases as the index of expansion n decreases, the best that can be hoped for in practice is that the expansion shall be isentropic. An index of expansion less than the isentropic index would imply heat reception from the surroundings. The second peculiarity arises because with steam at low pressures there is a very rapid increase of specific volume as the pressure is decreased isentropically, i.e. — (dv/dp), is very large. With the pressure ranges employed in practice, this implies that a very long stroke would be required if the steam were to be expanded reversibly down to condenser pressure inside the engine cylinder. Such a long stroke is undesirable not only for structural reasons, but also 385
[16.4]
Work Transfer Steam chest
Fig. 16.12
77177///77/7/77/
A doubleacting steam
40
,
ideal p—V diagram
To slide valve eccentric
..
engine cylinder with an
Stuffing boxes
—)To crank via connecting rod
77///////
p 1
2
Steam chest pressure
3
5
4
Condenser pressure 3' V
because. it would reduce the mean effective pressure of the machine cycle and so increase the proportion of the indicated power expended in overcoming mechanical friction. That complete expansion entails a decrease in mean effective pressure should be evident from the p—V diagram of Fig. 16.12, the mean effective pressure of the additional area 433' being so small. Fig. 16.12 shows a sketch of a doubleacting steam engine fitted with a simple slide valve which is actuated by an eccentric on the crankshaft. As with all expanders, mechanically operated valves are necessary, and this feature makes possible the opening and closing of ports at any desired point in the machine cycle. The events on one side of the piston are as follows, those on the other side being similar but displaced in time by half a revolution of the crankshaft: 12
23 34
45 51
386
Admission When the piston is at outer dead centre the inlet port is opened, and a mass Ani f of highpressure steam is admitted by the time the inlet port is closed at the point of cutoff. The steam admitted mixes with a mass Am,. which remained in the clearance volume after completion of the previous cycle. Expansion The steam expands isentropically until the exhaust port is opened at the end of the stroke. Blowdown The pressure at the end of the expansion stroke p3 is higher than the condenser pressure p4. When the exhaust port opens, some of the steam 'blows down' into the condenser until the pressure in the cylinder is 134. Exhaust On its return stroke the piston displaces the steam left in the cylinder after the blowdown until the exhaust port closes at point 5. Compression or 'cushioning' The steam Anic left in the cylinder is compressed isentropically during the remainder of the stroke. Point 5
[16.4]
Fig.16.13
Reciprocating Expanders and Compressors
1,2
State path of steam in the cylinder + Am,)
3 (Arni + Ani..)— 1
45 S
may be so chosen that the final pressure is equal to pl , when Am, will mix reversibly with the next charge Am f . The state path of the steam in the cylinder is depicted in Fig. 16.13. Admission 12 occurs ideally with no change in state, and the ensuing expansion follows an isentropic path 23 up to the blowdown. Although the blowdown is an irreversible expansion process, it may be imagined to consist of two parts, one reversible and the other irreversible. First, the steam in the cylinder expands isentropically, displacing some steam into the condenser; the expelled steam acquires some kinetic energy in the process. The state of the steam remaining in the cylinder is represented by point 4. Secondly, the kinetic energy of the expelled steam is dissipated irreversibly in the condenser; this part of the process is not shown on the h—s diagram. During the exhaust process 45 the state of the steam in the cylinder is unchanged, though the displaced steam will mix with steam in the condenser irreversibly. Finally, the mass Am, in state 4,5 is returned isentropically to state 1,2. Owing to the blowdown, as well as for other reasons elaborated below, the expansion of the mass Amf passing through the cylinder is not isentropic. The overall enthalpy drop Am f(h, — h6 ) is less than the isentropic drop Amf (h, — h 5 ), if h6 denotes the enthalpy of the exhaust steam in the condenser space before it has rejected any heat to the cooling water. The ratio between the actual and the isentropic enthalpy drops is the isentropic efficiency of the engine. Example 16.2 shows how the effect of blowdown on the isentropic efficiency can be estimated.
Example 16.2
A steam engine cylinder has a swept volume of 0.03 m3 and a clearance volume of 0.001 m3. Cutoff is at 0.4 of the stroke. Saturated steam is admitted at 7 bar and expands isentropically to the blowdown. The mass which expands inside the cylinder during the blowdown may be assumed to do so isentropically. Cushioning is timed so that isentropic compression brings the clearance steam to the admission state. Calculate the work done per machine cycle and the isentropic efficiency when the engine exhausts at atmospheric pressure. 387
[16.4]
Work Transfer
Using the notation of Fig. 16.12, V1 = 0.001 m 3,
V3 = V4 = 0.031 m 3,
112 = V1 + 0.4( V, — V1 ) = 0.013 m 3 During the admission 12 the state is Pi = p2 = 7 bar, v1 = v2 = 0.2728 m 3 /kg u1 = u2 = 2573 kJ/kg,
h 1 = h 2 = 2764 kJ/kg,
si = s2 = 6.709 kJ/kg K During exhaust 45 the pressure is 1.013 bar, and the dryness fraction is found from s1 = s5 = s4 to be 0.893. Then v4 = v5 = 1.494 m 3 /kg, u4 = 115 = 2283 kJ/kg, h4 = 115 = 2434 kJ/kg At the beginning of the blowdown, state 3, the specific volume is V3 = 112
V 3 V2
=
0.2728 x
0 031 0.013
— 0.6505 m 3 /kg
By trial and error from tables, or more quickly from the h—s chart, we find that in state 3, defined by v3 = 0.6505 m 3/kg and s3 = s2 = 6.709 kJ/kg K, p3 = 2.6 bar and x3 = 0.939. Hence u 3 = 2417 kJ/kg. The masses of steam in the cylinder at the points 1 to 5 are = m5 = Vi /vi = 0.0037 kg tn2 = tn 3 = V2/ 11 2 = 173 /v3 = 0.0477 kg, tn,= V4/v4 = 0.0207 kg Cushioning must begin when V5 = in,v, = 0.0055 m 3 The total work done per machine cycle can now be found from five nonflow processes: W12 = W23 =
—p 1 (V2 — V1 )= —100 x 7 x 0.012 = 1112 (113 — u2 ) = —0.0477 x 156 =
W51 =
W
—7.44 kJ 0 kJ
W34 = W45 = — P4(
—8.40 kJ
V5 — V4 ) = 100 x 1.013 x 0.0255 = +2.58 kJ — u 5 ) = 0.0037 x 290 =
=
+ 1.07 kJ — 12.19 kJ
The isentropic work can be found in two ways. Assuming that full expansion is achieved by lengthening the stroke to 3', corresponding to the exhaust state 4,5, V3 = 1113 114 = 0.0713 m 3 388
Reciprocating Expanders and Compressors
[16.4]
Hence the total work is — 8.40 kJ
W12 =
0.0477 x 290 =
W23' — M2(u3 u2)
—13.83 kJ
W3, 5 = —p'3(1/5 — V'3 ) = 100 x 1.013 x 0.0658 = +6.67 kJ W5 —
+ 1.07 kJ
VVisen =
—14.49 kJ
We arrive at the same answer more easily using the steadyflow analysis. The flow steam per machine cycle is Am f = m 2 —
= 0.0477 — 0.0037 = 0.0440 kg
and, because from the h—s chart (h3 — h1 ) = — 330 kJ/kg, Wis. = Anif (W3 — h1 ) = — 0.0440 x 330 = —14.52 kJ The isentropic efficiency is W
—12.19
risen =
14.52
Wisen
= 0.84
Note that the mean effective pressure for the complete reversible expansion is 14.52 0.0703 2.07 bar
I Wlisen
(Pm)isen
/7
V1
100 x
and for the irreversible expansion is Pm =
I WI
12.19
V4 — V,
100 x 0.030
= 4.06 bar
Thus in practice, when mechanical friction is taken into account, the irreversible expansion would probably yield a greater brake power. It has already been mentioned that the ports may be opened and closed at any desired point in the cycle. The point of cutoff and the point where cushioning begins require special comment. If the cutoff is too early in the expansion stroke the work done per cycle will be unduly small, and if it is too late the additional work will not be commensurate with the additional amount of steam admitted (see Fig. 16.14a). The work done per machine cycle can also be increased by delaying the onset of cushioning (Fig. 16.14b), but again this will be at the expense of an increase in steam consumption. This is because the pressure of the clearance steam after cushioning is then below the steam main pressure and, when the inlet port is opened, steam rushes in to raise the cylinder pressure in an irreversible manner. The indicator diagram taken from an actual engine differs from the ideal diagram of Fig. 16.12 for a number of reasons. There are the usual differences already mentioned in section 16.3 associated with the finite time required for opening and closing valve ports and the pressure drops incurred by fluid friction as the steam enters and leaves the cylinder. There is another important difference
389
[16.4]
Work Transfer p
Fig. 16.14 The effect of varying (a) cutoff and (b) cushioning on the p—V diagram
V (a)
Fig. 16.15 Cyclic variation of temperature
V (b)
Inlet steam temperature Cylinder wall temperature (steam jacketed) Cylinder wall temperature (lagged)
—— Exhaust steam temperature
Crank revolutions
associated with the fact that it is not possible to eliminate heat transfers between the steam and the cylinder. The steam undergoes a considerable change in temperature during its passage through the machine but, owing to the resistance to heat flow between fluid and cylinder, the cylinder temperature fluctuates between much narrower limits; this is indicated in Fig. 16.15. Evidently the temperature difference between the steam and the cylinder varies in such a way that heat is rejected by the steam during admission and early expansion, while heat is received during the latter part of the expansion and during the exhaust process. Even if the cylinder is well lagged or steam jacketed, and the heat rejected to the surrounding atmosphere is small, the cylinder itself acts alternately as a sink and a source of heat. The effect of the heat exchanges is not very marked if superheated steam is being used, but it becomes very pronounced if the steam is only just dry at entry. Heat rejection during admission is then manifested by condensation of steam on the cylinder walls. Once condensation occurs there is a sudden and very large increase in the rate of heat transfer,* and hence the condensation process is accelerated. Heat transfer from the cylinder during the latter part of the expansion and exhaust stroke reevaporates some of the condensate, but too late for the resulting vapour to do much work. The main effect of the reevaporation is an increase in exhaust pressure due to the increased specific • * A condensing vapour exchanges heat with a surface at a rate which may be several hundred times larger than that for a dry vapour or gas; see Fig. 22.25.
390
Reciprocating Expanders and Compressors
[16.4]
volume of the steam flowing through the exhaust port. The net result of all these heat exchanges is an increase in steam consumption and a decrease of work output. Both the loss of work associated with the failure to expand down to condenser pressure in the cylinder, and that due to the heat transfers, become more pronounced as the pressure range is increased. More efficient operation can then be achieved by compounding, i.e. by carrying out the expansion in two or more stages. The large volume of lowpressure steam can be handled in a largediameter cylinder without the need for an excessively long stroke, and at the same time the range of temperature variation in each cylinder is only a fraction of the total temperature change of the steam. Sometimes, to keep the lowpressure cylinder within reasonable dimensions, the lowpressure steam is split between two cylinders in parallel. The expansion may be completed down to the condenser pressure if a turbine is added as a final stage. Even if the plant is of relatively low power output, a turbine can be quite efficient if it is called upon to deal with the steam at the lowpressure end where the volume flow is large. The combination of reciprocating engine and turbine was used for mediumsize marine plant before the oil engine began to supplant the steam engine. The power output of a steam engine can be controlled in one of two ways. From what has been said about the choice of the point of cutoff (Fig. 16.14a), it will be clear that one possibility is the use of a special valve gear which will permit the timing of the cutoff to be varied; this is called cutoff governing. The second method, throttle governing, consists of throttling the steam in a regulating valve before admission to the steam chest, thereby reducing the inlet pressure and effective enthalpy drop available from the expansion. The effect of both methods is illustrated in Fig. 16.16 for the simple case where the clearance volume is zero. In the cutoff governed engine the reduction in work is obtained by a reduction in the mass of steam admitted, and the ideal enthalpy drop per unit mass is unchanged. In the throttle governed engine the work is reduced by an irreversible reduction of steam chest pressure, which results in an appreciable reduction in available enthalpy drop per unit mass, and the mass of steam admitted is only slightly reduced by virtue of the fact that the specific volume of the steam is increased. The former is clearly the more efficient method of governing, and is always preferred for such applications as steam locomotives Throttle governing
Fig. 16.16 Cutoff and throttle governing
/3
Cutoff governing Main
Main
Loss of output (a)
Main p Chest p Condenser p
(b)
391
[16.5]
Work Transfer
where the engine is not speed governed. The heavy valve gear required for varying the point of cutoff is unsuitable for use with the normal type of speed governor, and where constant speed is required (e.g. for pumping plant) the ease with which a simple throttle valve can be operated by a governor outweighs considerations of fuel economy. Reference to Fig. 16.16a will indicate another reason why cutoff governing is used for traction engines. By operating the engine nonexpansively, a rectangular diagram is obtained. This provides the particularly large torques required for starting purposes, and the disproportionate increase in steam consumption is of no significance for such a short duration. 16.5 Rotary positive displacement compressors
In the type of compressor discussed earlier, the component which displaces the fluid from the low to the highpressure region performs a reciprocating motion. Here we shall discuss compressors in which the displacement is performed by a rotating component. The rotary machine can operate at high speeds and can therefore handle larger rates of flow than its reciprocating counterpart—or is smaller for a given flow. The processes are for this reason more nearly adiabatic than in reciprocating compressors, and the indicated isothermal efficiency will be lower. To some extent this is offset by the fact that the mechanical efficiency is usually higher than for reciprocating machines, thus giving similar overall isothermal efficiencies for both classes of compressor. Rotary compressors are particularly suitable as superchargers for internalcombustion engines and as vacuum pumps, and they are often arranged in stages. There are several distinct designs of rotary compressor, and one of the simplest and best known is the Roots blower shown in Fig. 16.17. Its essential parts are two rotors, each rotor having two or more lobes with profiles formed by complete epicycloids and hypocycloids. This geometric form ensures that at all angular
Fig, 16.17 The Roots blower To receiver
External gear drive
ni
392
Reciprocating Expanders and Compressors
[16.5] Fig. 16.18 Reciprocating analogue of Roots blower
Receiver
P2
„.Irreversible pressure rise I
due to backflow from receiver
Pi k
Pz
V
positions the highpressure space is sealed from the lowpressure space. One rotor is coupled to the source of power, the other being driven from it by gears external to the casing (not through the lobes). There is always a slight clearance between the meshing lobes to avoid wear at the sealing surfaces. The mode of action is as follows. In the position shown, a volume vs of air, at atmospheric pressure say, is being trapped between the lefthand rotor and the casing. Assuming adiabatic conditions, this trapped volume does not change its state until the space VS is opened to the highpressure region. At that instant some highpressure air will rush back from the receiver and mix irreversibly with the air in the lower until the pressure is equalised. The air is then displaced into the receiver. This happens four times per complete revolution, and the free air delivery of the compressor is thus LIK per revolution. The air flow into the receiver is intermittent, even though the rotors revolve with uniform speed. To see how the work done in this irreversible flow process may be calculated, let us consider the reciprocating compressor of Fig. 16.18 with no clearance and a swept volume of K. After air at atmospheric pressure Pt is drawn in, the inlet valve is closed and the delivery valve is opened immediately afterwards with the piston still at inner dead centre. Backflow from the receiver will equalise the pressure in the receiver and the cylinder by an irreversible process. We shall consider the receiver to be of infinite volume compared with the volume i.e. that the equalised pressure will be p2 , which is the steady pressure of the air leaving at section 2. This compressor performs the same process as a Roots blower with an infinite receiver.* The work required per four revolutions of the reciprocating machine, equivalent to that required per revolution of the Roots blower is, W = (P2 — P1)4 Vs
(16.19)
Note that this is greater than, the work required to drive a reversible adiabatic compressor. Fig. 16.19a shows a vane pump, whose mode of action differs slightly from that of the Roots blower. Volumes Va , Yb, Vd are trapped between the vanes * The analysis for the case of a finite receiver is complicated, and for this the reader is referred to Ref. 17.
393
[16.5]
Work Transfer
112
Fig. 16.19 The rotary vane compressor
2
Li
Receiver
1
Receiver
PI
PI
L
L —
Irreversible compression Reversible compression a
P
= —)
b
(b)
(a)
and the casing, the vanes sliding in slots in the eccentrically placed rotor. Consider the volume 17a of air which has just been trapped at atmospheric pressure pi . When it reaches the position of volume Vd, which is on the verge of being uncovered, it will have been reduced in size owing to the asymmetrical placing of the inlet and outlet ports; thus pd > p, assuming adiabatic conditions. In practical applications the pressure pd is normally less than the delivery pressure p2, and further compression is obtained by an irreversible backflow of air from the receiver as in the Roots blower. An idealised equivalent reciprocating compressor of swept volume vs equal to Va is shown in Fig. 16.19b. The initial part of the compression from p, to pd is reversible and, after the delivery valve is opened at d, further compression to p2 is achieved irreversibly. The total work per N revolutions, being equivalent to the work required per revolution by a vane pump with N vanes, is W=
N
pi Y
va
Pi
/Y )( 1) —
1}
N(P2
Pa) Vd
(16.20)
The vane compressor is said to have internal compression owing to the reduction in volume from Va to Vd , a feature which is absent in the Roots blower. By comparing the p—V diagrams in Figs 16.18 and 16.19, it is evident that internal compression reduces the work required. The Lysholm compressor, which is similar to the Roots blower but with helical lobes, possesses a high degree of internal compression: it is described fully in Ref. 9.
394
17 Reciprocating InternalCombustion Engines
There are two principal classes of reciprocating internalcombustion (or IC) engine. They are distinguished mainly by whether the combustion is initiated by a spark, or spontaneously by virtue of the rise in temperature during the compression process. Petrol and gas engines are in the former class and they will be referred to here as sparkignition (or SI) engines. The term compressionignition (or CI) engine will be used to refer to the second class, although the terms 'Diesel engine' and 'oil engine' are also common. After the modes of action of some typical SI and CI engines are described, suitable criteria of performance are discussed, and the factors which limit the performance of practical IC engines are outlined. This is followed by a comparison of the real processes of an IC engine with the equivalent airstandard cycle. The chapter ends with a brief discussion of the limits that are imposed by the laws of thermodynamics on the conversion of chemical energy into work.
17.1 The working of IC engines
Both SI and CI engines can be designed so that one complete cycle of events in the cylinder is completed during either four or two strokes of the piston. The main events occurring in a fourstroke petrol SI engine are illustrated in Fig. 17.1 and are as follows: 12
Induction stroke A mixture of air and petrol vapour is drawn into the cylinder, the pressure of the mixture being a little below atmospheric owing to friction in the induction pipe. The inlet valve closes just after the end of the stroke. 23 Compression stroke With both inlet and exhaust valves closed, the air—fuel mixture is compressed. Just before the piston reaches outer dead centre, ignition is effected by an electric spark. Combustion is not instantaneous, but occupies a finite period. Nevertheless much of it occurs at nearly constant volume because the piston is moving relatively slowly near dead centre. 34 Expansion or working stroke Combustion is nominally completed at the beginning of the expansion stroke, and the products expand until the 395
[17.1 ]
Work Transfer Fig. 17.1 The sparkignition SI
Throttle
engine Nominal end of combustion
Exhaust port opening
Swept volume Clearance volume
exhaust valve opens just before the end of the stroke. As the valve opens, the gases blow down the exhaust duct until the pressure in the cylinder has fallen to approximately atmospheric pressure. 41 Exhaust stroke The products which have not escaped from the cylinder during the blowdown are displaced by the piston. To provide the pressure difference necessary to overcome friction in the exhaust duct, the pressure in the cylinder is slightly above atmospheric. At the end of the stroke there will be some residual gases in the clearance volume, which will dilute the next charge drawn into the cylinder. The events in a fourstroke CI engine, illustrated in Fig. 17.2, differ from those in the SI engine in the following manner: 12 Induction stroke Air alone is admitted to the cylinder. 23 Compression stroke The air is compressed, and towards the end of the stroke liquid fuel is sprayed into the cylinder. The temperature of the air at the end of compression is sufficiently high for the droplets of fuel to vaporise and ignite as they enter the cylinder. 34 Expansion or working stroke Since the fuel is sprayed into the cylinder
Fig. 17.2 Fourstroke SI engine cycle
Nominal end of combustion Start of fuel injection
2 V
396
[17.1]
Reciprocating InternalCombustion Engines
Fig. 17.3
Spark plug or fuel injection nozzle
The twostroke engine
(a)
41
(b)
(c)
at a controlled rate, the pressure may remain fairly constant during combustion. In modern highspeed engines, however, there is often a rise in pressure during the initial stages of combustion. At some point in the expansion stroke the combustion is nominally complete and the pressure then falls steadily until the exhaust valve is opened and blowdown occurs. Exhaust stroke This follows as in the SI engine.
When the twostroke cycle is employed, the induction and exhaust strokes are eliminated. The piston stroke must be longer, because part of the compression and expansion strokes are used for the processes of exhaust and induction. Fig. 17.3 shows a section of a common type of twostroke engine. Apart from the selfacting springloaded valve on the crankcase, no valves are required, and the piston itself is used to open and close the inlet and exhaust ports. In Fig. 17.3a the piston is shown near the end of the compression stroke. The upward motion has decompressed the crank case and air has been admitted through the selfacting valve to the crankcase. During the expansion stroke the air in the crankcase is compressed, and near the end of this stroke the exhaust port is uncovered to allow the hot gases to blow down the exhaust duct. Further movement of the piston uncovers the inlet port, and compressed air from the crankcase flows into the cylinder. The exhaust and inlet ports are open simultaneously for a short period so that the incoming air can assist in clearing the cylinder of combustion products. The machine cycle is finally completed by compression of the air trapped in the cylinder. The twostroke engine can be built as an SI engine, with petrol vapour and air being admitted to the crankcase, or as a Cl engine. A full discussion of the relative merits of twostroke and fourstroke engines would be out of place here, but the following points are worth noting: (a) The twostroke engine does not require any mechanically operated valves. This implies not only considerable mechanical simplification, but also that the engine can be run in either direction. The twostroke CI engine has
397
Work Transfer
[17.1]
established itself in marine practice primarily because it eliminates the need for a reversing gear. (b) For the same rotational speed, the twostroke engine has twice the number of working strokes. The power output from an engine of given bulk and weight is therefore greater for a twostroke engine, although for a number of reasons it is not twice as great. The greater frequency of working strokes in the twostroke engine also implies a more uniform torque and a smaller flywheel. (c) The twostroke engine tends to have a higher fuel consumption than the fourstroke engine. Little time is available for induction and exhaust in the twostroke engine, so that the process of clearing the combustion products from the cylinder and recharging it is less complete. Moreover, less time is available for the fresh charge of air to cool the cylinder, and overheating may be a more serious problem. In twostroke SI engines some fuel may pass through the cylinder without combustion because of the necessary overlap of the periods when the inlet and exhaust ports are open. A description of the general working of IC engines would not be complete without the mention of a rotary variant, a recent design of which is known as the Wankel engine. It is akin to the twostroke engine in that it requires no valves. The diagrammatic sketch in Fig. 17.4 shows the principles of operation. The triangular rotor A, having internal teeth meshing with a central gear fixed to the engine casing, performs a planetary motion around this gear. An eccentric B, integral with the power output shaft, revolves in a recess of rotor A at three times its speed. The shape of the outer casing issuch that the apexes of the triangular rotor seal off three distinct spaces 1, 2 and 3. The shape of the curved surfaces of rotor A is unimportant, except in so far as it determines the maximum and minimum volumes of the sealed spaces, and therefore the compression ratio. The curved surfaces are recessed as shown, mainly to avoid `throttling' of the flame spreading from the spark plug through the combustion space. The sequence of events is not difficult to follow. Fig. 17.4a shows the situation where a charge is being induced into space 1, the preceding charge is fully compressed in space 2, and the combustion products are being exhausted from space 3. Fig. 17.4b represents the situation a little later, with the new charge occupying the maximum volume and about to be compressed in space 1, combustion gases expanding in space 2 to provide the 'working stroke', and space 3 being reduced in volume and thus exhausting the products through the outlet port. The rotary engine has one important feature in common with its reciprocating counterpart: it is a positive displacement machine, and the processes occur in a cyclic intermittent manner. We therefore consider it here for the same reason that the Roots blower and vane pump were considered in the chapter on reciprocating compressors. Its obvious advantages visàvis the reciprocating engine are that it is capable of handling fairly large mass flows for its size and 398
[17.1 ]
Fig. 17.4 The Wankel engine
Reciprocating InternalCombustion Engines
Cooling channel
thus has a larger power/weight ratio, and also that its rotor can be perfectly balanced by the addition of appropriate masses. Three disadvantages of the rotary design are apparent. First, because the processes occur in a sequence of positions around the casing, the surfaces near the spark plug are intermittently cooled by the compressed charge, whereas the reciprocating engine cylinder is intermittently cooled by the colder uncompressed charge. Furthermore, the casing surface adjacent to space 3 is permanently exposed to the expanding burnt gases. This implies the need for good local cooling arrangements. Although the problem is eased by the high surface/volume ratio of the combustion space, it does of course result in high heat losses. Secondly, the long narrow shape of the combustion space is not good from the point of view of using high compression ratios, as will become clear after the discussion of detonation in section 17.3.1. Thirdly—and this is the reason for the failure of many early attempts to develop a rotary engine—there is an inherently difficult sealing problem at the apexes and flat side faces of the rotor. After many years of development, and in spite of some degree of success, it now looks unlikely that the Wankel engine will displace the reciprocating engine
399
(17.2]
Work Transfer
from the numerous fields of application where the latter is well established. Certainly a CI version of the rotary design, possible in principle, will also have to be developed before the rotary engine can hope to capture a major part of the market. Further details of the Wankel engine can be found in Ref. 22.
17.2 Criteria of performances for IC engines
It was explained in section 15.6 that the overall efficiency of a power plant is usually expressed as
Aho(liq)
or
Aho(vap)
where W is the net work per unit mass of fuel supplied and Aho is the enthalpy of combustion of the fuel. The net output of an engine is called the brake power (BP) and for this reason the overall efficiency is termed the brake thermal efficiency lib. The BP is always treated as a positive quantity, and hence rib is defined by r1b
=
BP rhF( — Aho )
(17.1)
where tri. r is the rate of fuel consumption. The specific fuel consumption (SFC) is frequently used as an alternative criterion of performance. It is defined as the rate of fuel consumption per unit of brake power, i.e.
SFC =
(17.2)
BP
Evidently, for any given fuel the SFC is inversely proportional to rib. Most common hydrocarbon fuels have very similar enthalpies of combustion, and the SFC can therefore be used when comparing the economy of engines using different fuels. In a reciprocating engine an appreciable part of the loss is due to mechanical friction, and it is informative if the thermodynamic and mechanical friction losses are separated. The overall efficiency is therefore analysed as the product of the indicated thermal efficiency th and the mechanical efficiency th„,,. Thus
( rlb =
IP rh,( —Aho ))
BP IP )= r1i
►lmech
(17.3)
The indicated power (IP) is the actual rate of work done by the working fluid on the piston, and the difference between the IP and the BP is the power absorbed by mechanical friction (piston, bearings etc.). As its name implies, the IP can be determined from an indicator diagram. The procedure has been explained in section 16.3. The only point of difference here is that with a fourstoke engine the area of the small anticlockwise loop (Fig. 17.5) must be subtracted from the area of the main diagram when determining the indicated mean effective pressure (IMEP) pm . The work represented by the small loop is 400
Reciprocating InternalCombustion Engines
[17.2]
Fig. 17.5 Effect of pumping loss on the indicator diagram
termed the pumping loss; it is the result of viscous friction in the induction and exhaust strokes. The physical equation equivalent to (16.8) for the IP is (17.4)
IP = p,,,LAN
Here N is the number of machine cycles per unit time, namely half the rotational speed for a fourstroke engine, and the rotational speed for a twostroke engine. When an engine is run at constant speed, the variation of nb and n mech with load appears as in Fig. 17.6. At constant speed the power expended on mechanical friction—termed the friction power (FP)—is approximately constant. Therefore, as the BP is reduced the mechanical friction loss exercises an increasing influence on the efficiencies. At zero BP all the fuel is consumed in overcoming friction, and both t, and n,mech are zero. With an engine of good mechanical design, nmech should be between 80 and 90 per cent at full load. nb depends upon the type of engine, but at full load it is usually 2535 per cent for SI engines and 3040 per cent for CI engines. When discussing airstandard cycles for reciprocating engines it was suggested that the mean effective pressure provides a useful guide to the relative size of an engine. In practice it is usual to use the concept of brake mean effective pressure (BMEP) for this purpose. The BMEP, which may be denoted by pmb, is defined by an equivalent equation to (17.4), i.e. (17.5)
BP = pmb LAN
The BMEP may be regarded as that part of the IMEP which is imagined to Fig. 17.6 Variation of efficiency with load at constant speed
rimech
Constant speed test
401
Work Transfer
[17.3]
contribute to the BP, the remainder being used to overcome friction. An increase in BMEP implies that the cylinder volume LA can be smaller for a given output. As an illustration, the values of BMEP used in SI car engines have steadily increased through the years from 4.6 bar ( when the RAC rating was introduced) to approximately 10 bar. The corresponding BP obtained per litre of cylinder swept volume has increased from about 10 to 30 kW. This considerable reduction of specific engine size is not due solely to the increase in BMEP but is partly due to a simultaneous increase in permissible engine speed. In the following section we shall discuss the more important factors which limit the efficiency and BMEP of SI and CI engines. 17.3 Factors limiting the performance of IC engines
When discussing gas turbine power plant in section 12.2 it was pointed out that the performance was limited by the maximum gas temperature that can be permitted in the engine. This 'metallurgical limit' is imposed because the turbine is continuously exposed to high temperatures under conditions of severe stress. Provided that proper attention is paid to the cooling of the cylinder (particularly the cylinder head) and exhaust valves, no such limitation is encountered in reciprocating engines where the working stresses are much lower. The reason for this is indicated in Fig. 17.7, which shows qualitatively the temperature variation of the gas in an engine cylinder. The peak gas temperature may be as high as 2800 K, but this temperature is reached in intermittent combustion and is not due to a transfer of heat through the cylinder wall. The metal temperature therefore fluctuates between much narrower limits. Moreover, owing to cylinder cooling, and the insulating properties of a gas boundary layer and a film of lubricating oil which are adhering to the wall, the mean metal temperature is well below the mean gas temperature. There are several factors of a different nature limiting the performance of reciprocating engines and, as they differ for SI and CI engines, each type of engine will be considered separately. 17.3.1 The Si engine
The analysis of the airstandard Otto cycle showed that the cycle efficiency improves with increase of compression ratio. This is also true of the brake 9g. 17.7
I engine cycle d
Is.yclic variation of emperature
I
— Peak temperature
Uncooled cylinder wall Cooled cylinder wall — Atmospheric temperature Crank angle or time
402
Reciprocating InternalCombustion Engines
[17.3]
Controlled propagation of flame
Fig. 17.8
Combustion in an SI engine Spark plug Controlled combustion Region of controlled flame propagation Delay Spark plug
I
Detonation and selfignition
Selfignition Spark in 'end gas' 90°
0° ODC
90°
Crank angle or time thermal efficiency of SI engines. There is an upper limit to the compression ratio that can be employed, however, which has its origin in the fact that the liquid compressed in the cylinder is a mixture of fuel vapour and air. The temperature of the combustible mixture increases on compression, and if the compression ratio is too high it is possible for selfignition to occur before spark ignition. The onset of combustion at too early a point in the compression stroke would lead to a serious loss of power and must be avoided. Even a compression ratio sufficiently low to avoid preignition may be too high for efficient operation. This is due to the phenomenon of detonation. Although a considerable effort has been made to determine the exact nature of detonation in an engine cylinder, it is still a controversial topic. There are undoubtedly several phenomena involved, and such terms as 'knocking' and 'pinking' are often used in an attempt to distinguish between them. Here we can only give a very brief and oversimplified picture, with the aid of Fig. 17.8. Under normal conditions combustion begins near the spark plug after a short delay following the formation of the spark, and the flame spreads through the mixture with a rapid but finite velocity. The energy released by the spark is only small, and it sets off a relatively slow flameless reaction which occupies the delay period. Further energy is released at an accelerating rate by the reaction, until a proper flame front develops. (The delay period is very short— approximately 0.002 second—but it may correspond to an appreciable movement of the crank in a highspeed engine. For example, at 3000 rev/min the crank turns through 36 degrees in 0.002 second. This is the reason why the point of ignition is always well in advance of outer dead centre (ODC).) As the flame front spreads in a uniform manner across the combustion space, it compresses the unburnt part of the mixture before it. The temperature of the unburnt portion is raised by intense radiation from the flame as well as by the compression. If the initial pressure and temperature are too high, the unburnt portion appears to reach a critical condition resulting in selfignition at numerous points in the unburnt 'end gas'. A violent pressure rise is then produced which may result in a knocking noise. This phenomenon of selfignition 403
Work Transfer
[17.3]
in the end gas, though occurring after the spark, is akin to the phenomenon of preignition. It should not be confused with detonation proper. Strictly speaking, the term 'detonation' refers to phenomena associated with the sudden acceleration of a flame front. As the flame front progresses at a moderate rate through the mixture, a critical condition is sometimes reached at which a violent pressure wave, i.e. a shock wave, is formed. The violence of the shock wave so accelerates the rate of reaction that the flame front keeps pace with the shock wave and they traverse the cylinder together at a very high velocity. This rapidly moving front is termed a detonation wave, and it is reflected and rereflected by the cylinder walls. It results in a noise, though usually of a higher frequency than that produced by selfignition in the end gas.* The main objection to detonation of any kind is that it causes excessive turbulence which removes most of the insulating gas boundary layer. It therefore increases the rate of heat transfer between gas and cylinder wall and may result in serious overheating of the engine. Even if this is avoided, continuous detonation may cause the formation of local hot spots which eventually lead to preignition. Excessive turbulence also results in a reduction of power output. From the mechanical point of view, detonation may cause deterioration of the bearing surfaces in a lightly built engine. Lastly, the appearance of carbon in the exhaust gases when detonation occurs indicates that it results in incomplete combustion. For all these reasons a compression ratio sufficiently high to cause detonation must be avoided. Some fuels permit the use of a higher compression ratio than others,t and there are compounds (`dopes') which can be added to petrols to suppress the tendency to detonate. It is difficult to devise a measure of the detonating tendency of a fuel. One method is to compare the performance of a fuel with that of a heptaneoctane mixture in a special variable compressionratio engine. nheptane (C,H16 ) is a fuel liable to give detonation at low compression ratios, while isooctane (C81118 ) detonates at much higher ratios; different mixtures of the two provide a continuous octane number scale from 0 to 100 per cent in octane content. The compression ratio of the engine is raised until the fuel under test detonates, and the highest percentage of octane in a heptaneoctane mixture that produces detonation at the same compression ratio is called the octane number of the fuel. It should be emphasised, however, that the octane rating is an arbitrary measure, and it is possible to mix a fuel which is better than pure isooctane and which therefore has an octane rating greater than 100. The need for a test engine of agreed design arises from the fact that the size and shape of the combustion space and the location of the spark plug are also important factors governing detonation, because they determine the length of time during which the end gas is exposed to the advancing flame front. For the same reason, in an engine of given size a large number of small cylinders is preferable to a small number of large cylinders. Over the last fifty years, * A discussion of various theories can be found in Refs 10 and 21. t Fuel oils have a marked tendency to detonate and therefore cannot be used in SI engines. Apart from this, oils do not evaporate as readily as petrols and homogeneous combustible mixtures are not easily obtained.
404
Reciprocating InternalCombustion Engines
[17.3]
Fig. 17.9
BP
Effect of mixture strength on engine performance
Constan speed test 0,1
Stoichiometric, / mixture 18:1
= 16.5:1 Lean
Rich
developments in 'doped' fuels and combustion chamber design (Ref. 12) have succeeded in raising the permissible compression ratio of ordinary car engines from about 4.5 to 9. With the compression ratio fixed, the other factor limiting the performance is the rise in pressure obtainable during combustion. The IMEP increases with increase in peak pressure, and an increase in IMEP is desirable because it implies that the engine will be smaller for a given power output and that a relatively smaller share of the IP will be absorbed in overcoming mechanical friction. The peak pressure is fixed by the amount of fuel that can be burnt and hence by the amount of oxygen available. Theoretically it will be a maximum if a stoichiometric mixture is used. Stoichiometric air/fuel ratios by weight are nearly identical for all common liquid fuels, i.e. about 14.5: 1. In practice, maximum brake thermal efficiency is achieved with a slightly weak mixture giving complete combustion of the fuel, and maximum power with a slightly rich mixture giving complete combustion of the oxygen (Fig. 17.9). The variation of efficiency with load has already been mentioned in the previous section, and the method of regulating the power output deserves some mention here. At first sight it would seem that the work output could be reduced by weakening the mixture and thereby reducing the rise in pressure during combustion. Unfortunately, reliable ignition by a spark is only possible over a fairly narrow range of air/fuel ratio, 18 : 1 being about the weakest limit. It follows that variation of the air/fuel ratio is quite unsuitable as a method of governing SI engines. Instead, approximately stoichiometric ratios are used at all loads, and regulation is achieved by reducing the mass of mixture induced in each working cycle. This method is referred to as throttle or quantity governing. Throttling results in subatmospheric pressure in the cylinder during the induction stroke, and an increase in the 'pumping loss' (Fig. 17.10). Since the exhaust process always occurs at atmospheric pressure, the dilution of the fresh charge with residual products is more serious at part load. In fact, at very low loads, mixtures richer than stoichiometric must be supplied to ensure satisfactory 405
[17.3]
Work Transfer Fig. 17.10 Effect of throttle governing on the indicator diagram
p
Full load — Part load
V
ignition. Evidently throttle governing is an inefficient method, and the partload efficiency of SI engines is poor for this reason. The normal method of achieving the appropriate mixture of air and fuel is by means of a carburettor, which consists of a venturi throat in the induction manifold, and one or more fuel jets through which petrol can be introduced into the air stream at this section. The pressure depression at the throat, whose magnitude depends on the air flow, causes petrol to be sucked from the jets into the air stream. From what has been said previously it is clear that the normal requirement from a carburettor is an approximately stoichiometric mixture at most speeds and throttle settings in order to work near the point of maximum efficiency. But in addition a rich mixture is required (a) at full throttle to attain maximum power, and (b) at very low throttle settings when there is marked dilution by residual products. Carburettors usually satisfy these requirements only moderately well, and moreover it is found that they produce nonhomogeneous mixtures of air and fuel and uneven distribution to the various cylinders. Fitting a multicylinder engine with several carburettors may improve this situation, but such an arrangement requires frequent adjustment. Solutions giving more positive control have been sought, using injection pumps and nozzles capable of metering the correct amounts of petrol—preferably into individual cylinders. Direct petrol injection has been used successfully on several engines but, because of the high cost of injection equipment compared with that of carburettors, it has been restricted to the more expensive car engines. One way of overcoming our apparent inability to govern an SI engine by weakening the mixture is by charging the cylinder with a controlled nonuniform mixture. Part of the cylinder is filled with a layer of ignitable mixture, while the remainder is filled with. air. In this way ignition can be achieved with an average charge well below stoichiometric ratio. This method of filling a cylinder with a nonhomogeneous air—fuel mixture is called stratified charging. Although engines have been successfully governed in this way under laboratory conditions, few commercial engines using this principle have been produced. A successful engine of this type would provide a major breakthrough in improving the partload, and therefore overall, economy of SI engines. 406
[17.3]
Reciprocating InternalCombustion Engines
17.3.2 The CI engine
Because the fuel is introduced into the cylinder of a CI engine only when combustion is required, i.e. towards the end of the compression stroke, preignition cannot occur. Moreover, since the fuel is injected at a controlled rate, the simultaneous combustion of the whole quantity of fuel cannot occur, and the problem of detonation as in SI engines does not arise. It follows that the compression ratio can be much higher in CI engines, and in fact there is a lower limit of about 12 : 1 below which compression ignition of common fuel oils is not possible. In a CI engine most of the combustion occurs at substantially constant pressure, and the maximum pressure reached in the cylinder is largely determined by the compression ratio employed. The upper limit of the compression ratio is therefore fixed by the strength of the cylinder, the bearings, and other parts whose stresses are determined by the peak pressure forces. Evidently the designer must reach a compromise between high efficiency and low weight and cost. From the analysis of the airstandard Diesel cycle, summarised in Fig. 12.14, it is evident that compression ratios in excess of 20: 1 give diminishing returns, and this is in fact about the maximum value used in practical engines. A comparison of the airstandard efficiencies of the Diesel and Otto cycles (Fig. 12.14), when made at appropriate compression ratios, suggests that the CI engine will be the more efficient. This is borne out in practice, and in general CI engines are more efficient than SI engines. We must next consider a factor limiting the IMEP of CI engines. It is evident from the p— V diagram that the mean effective pressure increases with increase in the change of volume which occurs during the combustion at constant pressure (Fig. 17.2). This change in volume is a maximum when all the fuel that can be burnt in the oxygen available is injected into the cylinder. At first sight it appears that this implies the use of a stoichiometric air/fuel ratio (x 14.5: 1) as in SI engines. To see why this is not so, it is necessary to outline briefly the way in which combustion is accomplished in CI engines. Although the fuel is injected as a deeply penetrating spray of fine droplets, the fact that it is in liquid form means that the delay period between injection and initiation of combustion is appreciably longer than in SI engines. Each droplet must first partially evaporate until sufficient vapour diffuses into the surrounding air to form a layer having an air/fuel ratio which is combustible. This vaporisation cools the droplet and surrounding layer, and time is required for the necessary temperature to be reestablished. Combustion then begins simultaneously at many points in the combustion space, and there is an initial rapid and uncontrolled rise of pressure. As the cylinder fills with combustion products, the rate of reaction becomes more controlled and the pressure remains sensibly constant. If the delay period is too long, there is time for a large fraction of the charge to enter the cylinder and a rather violent initial combustion may occur, resulting in rough running and the socalled Diesel knock. Diesel knock is thus seen to be a function of the fuel, and it also depends on droplet size, the rate at which droplets are introduced into the cylinder, and the heat transferred between droplets and their environment. If the latter
407
[17.3]
Work Transfer Fig. 17.11 Methods of improving the mixing of fuel droplets and air
Direction of sprays
(a)
(b)
parameters are kept substantially constant, by using a standard engine as is done when measuring octane numbers, the Diesel knock tendency can be measured by matching the fuel with a twocomponent fueloil mixture. For this purpose cetane (C16 H34) and alphamethylnaphthalene (C11 H10 ) are used to establish the socalled cetane number scale. It is found, not surprisingly, that a high octane number implies a low cetane number and vice versa, and this is one of the principal reasons why petrols are unsuitable for CI engines. Apart from reducing the delay period to avoid Diesel knock, another difficulty, particularly in the later stages of injection, is to ensure that all the fuel molecules collide with oxygen molecules to complete the process of combustion. To assist the mixing process, some turbulence or swirl is deliberately stimulated by careful design of the inlet port and combustion chamber. The turbulence must not be excessive, otherwise the initial uncontrolled rise of pressure may be too violent, and the work in the expansion stroke may be reduced unduly. What is required, therefore, is a controlled movement of the bulk of the air, and not smallscale random turbulence. Ideally the spray of fuel should be carried with the air through one complete sector between successive sprays by the time combustion is completed (Fig. 17.11a). Unfortunately this approach requires several small fuel jets (which may become choked), and very high injection pressures to achieve good fuel 'atomisation'. Another way of solving this problem (Fig. 17.11b) is to have some kind of separate swirl chamber into which the fuel is sprayed in a relatively coarse spray. Breakup of the fuel and mixing with oxygen is achieved as a result of the intense vortex motion produced as the air is forced into the chamber during the compression stroke. In spite of much ingenuity expended on combustion chamber design (Ref. 14), it is not possible to burn all the fuel completely if stoichiometric ratios are used, and the minimum air/fuel ratio, corresponding to full load, usually lies between 18: 1 and 25: 1. Consequently the engine must be larger than would be the case were it to be capable of burning stoichiometric ratios. The swirl chamber design, while allowing the use of air/fuel ratios down to 18 : 1, also results in higher heat losses during combustion and a lower efficiency than direct injection. When comparing the size and weight of CI and SI engines, three main factors must be borne in mind: utilisation of air, cylinder peak pressure and thermal efficiency. The CI engine, being incapable of using stoichiometric ratios and 408
[17.3]
Reciprocating InternalCombustion Engines
working with high peak pressures, tends to be larger and heavier than an equivalent SI engine, although the former has a higher thermal efficiency. Turning to the question of governing, it is found that very weak mixtures can be ignited and burnt in a CI engine, so that it is possible to reduce the power output by reducing the fuel supply. Reduction of the fuel supply is equivalent to a reduction of the cutoff ratio re of the airstandard Diesel cycle, and Fig. 12.14 shows that this improves the cycle efficiency. In practice, although an improvement in the indicated thermal efficiency may be achieved at part load, the fall in mechanical efficiency more than outweighs this effect and the brake thermal efficiency always falls off. Nevertheless the reduction in efficiency with decrease of load is not so marked as in SI engines. Governing the power output by weakening the mixture is usually referred to as quality governing.
So far in our discussion of both SI and CI engines we have considered factors limiting the work done per complete cycle*—but the actual power output will also depend on the rotational speed. It would seem that, other things being equal, the power output of an engine can be raised by increasing the speed—at least up to the limit imposed by purely mechanical considerations of stress and piston sliding velocities. In practice, however, it is found that the maximum indicated work per engine cycle varies considerably with speed, and beyond a certain speed the IP may even fall with further increase in speed. Typical curves are shown in Fig. 17.12. The reduction in indicated work per cycle at high speeds is chiefly due to a reduction in the mass of the charge induced during each engine cycle. Theoretically, an unsupercharged engine should induce a mass equivalent to the swept volume at ambient pressure and temperature. As a result of fluid friction and expansion of the charge in the hot inlet manifold, considerably less is taken in at high engine speeds when gas velocities are high and the manifold is very hot. (This is only a rough generalisation, and whether or not the mass induced falls with increase in speed depends also upon the valve timing and the design of the inlet and exhaust manifolds.) The 'breathing' capacity of an engine is expressed in terms of a volumetric efficiency defined as volume of induced charge per induction stroke reckoned at a reference pressure and temperature swept volume of piston
(17.6)
The reference pressure and temperature should logically be taken as the ambient values prevailing when the volumetric efficiency is determined, but sometimes they are assumed to be at some arbitrary level such as 0 °C and 1 atm. When comparing volumetric efficiencies care should be taken to ensure that they are based on the same definition. Fig. 17.12 shows that the indicated work per engine cycle also falls at low * The wbrk done per engine cycle is, of course, proportional to the mean engine torque, i.e. it equals 4n x torque for the fourstoke engine and 2n x torque for the twostroke engine.
409
[17.3]
Work Transfer Fig. 17.12 Variation of indicated work with engine speed
IP if IMEP were constant and equal to the max. value Indicated work/cycle (or IMEP)
\r/
Constant throttle test
Engine speed
>
speeds. This is due partly to increased leakage past valves and piston for which more time is available at low speed. It is also due to reduced turbulence and the increased cooling time available, which make the combustion process less efficient. At very low speeds the combustion tends to be erratic, and below a certain speed the engine will not run at all. Other things being equal, the total power developed in an engine cylinder depends upon the mass of the charge induced, and from the earlier remarks it might be supposed that this is limited by the prevailing ambient pressure and temperature of the air. In SI engines the induction temperature is lowered slightly by the evaporative cooling effect of liquid fuels. This is the reason for the superiority of alcohol over petrol as a fuel: its latent enthalpy of vaporisation is about three times that of petrol and the improved volumetric efficiency is sufficient to outweigh the disadvantage of the magnitude of the enthalpy of combustion being only about half that of petrol. Sometimes a liquid of high latent enthalpy, such as methanol, is injected into the induction manifold to lower the temperature still further; this device has been used in some aircraft piston engines for short periods of thrust boosting. Finally, by utilising resonance effects in the inlet and exhaust manifolds a certain amount of pressure charging can be achieved at selected speeds. A much greater increase in charge density can be obtained, however, by precompressing the charge before induction with some type of supercharger. A Roots blower or a centrifugal compressor is commonly used for this purpose. The supercharger may be gear driven from the crankshaft, or its power may be derived from a turbine driven by the exhaust gases. Although the net increase in power obtained by supercharging can be very considerable, it has little effect on the brake thermal efficiency. The reason is that the fuel supply must be increased in proportion to the increase in air charge in order to maintain the required air/fuel ratio. Owing to its greater mechanical complexity, a supercharged engine is not always preferred to its larger and heavier unsupercharged equivalent. Nevertheless, supercharging has become established practice in three important fields. First, a reciprocating aircraft 410
[17.4]
Reciprocating InternalCombustion Engines
engine must be supercharged at high altitudes, as otherwise the power falls off owing to reduced atmospheric pressure. Secondly, twostroke CI engines are usually supercharged because there is the added advantage that the cylinders can be more effectively cleared—or scavenged—of combustion products. Thirdly, in recent years supercharging has established itself in CI engines for automobiles, enabling them, through sophisticated control systems, to achieve high thermal efficiencies throughout their power range. Engine mass can be kept low by this means, allowing such cars to compete in terms of acceleration with their SI counterparts.* High thermal efficiency is important not only because it reduces running costs but also because it implies a reduction of noxious exhaust emissions. Urban pollution has become of paramount importance in the last decade or so as our cities have become choked with road traffic. The main pollutants from SI engines are carbon monoxide, unburnt hydrocarbons and oxides of nitrogen. The first two are strongly dependent on air/fuel ratio, and are much reduced in leanburn' engines designed to run on a high air/fuel ratio over a wide range of power and speed. Another approach is to incorporate a 'catalytic converter' in the exhaust system. The main component is a ceramic honeycomb, or a bed of ceramic particles, impregnated with noble metals like platinum and palladium. Because lead attacks most catalysts of this kind, and is itself a toxic pollutant, the use of lead as a dope in petrol is being phased out. Although in general CI engines cause less pollution than SI engines, it should be remembered that all engines running on fossil fuel contribute to the increase in concentration of carbon dioxide in the atmosphere. This in turn may lead to a significant rise in ambient temperature owing to the 'greenhouse effect' (see section 23.5). There is little doubt that, as long as fossil fuel is used for, road transport, when all forms of pollution are considered the only satisfactory solution is a reduction in the size of automobiles and a greater use of public transport. Enough has been said to indicate the main factors which influence the design of an engine. In practice the design must be a compromise between thermodynamic and mechanical considerations which are closely interlinked, and for detailed discussions the reader is referred to specialised texts on the subject such as Refs 4, 21 and 27. A good discussion of combustion in SI and CI engines is presented in Ref. 19, and of pollution formation and control in Chapter 11 of Ref. 21.
17.4 Comparison of real IC engine processes with airstandard cycles
That an analogy exists between the processes in real IC engines and the equivalent airstandard Otto, Diesel or mixed cycles has been suggested in Chapter 12, but further explanation is required. The analogy rests on the fact that the p—v diagram for the airstandard cycle is similar in shape to the p—V * A useful survey of supercharging practice is given in Ref. 15, and more recent work specifically on turbocharging is described in Ref. 16.
411
[17.4]
Work Transfer
diagram obtained from the engine, i.e. that the MEP of the cycle is approximately equal to the IMEP of the engine. This implies that the indicated work W produced by an engine inducing a mass m of air is approximately equal to m W, where W is the net work per unit mass of air taken through the airstandard cycle. The energy of reaction made available for work, by burning a mass mF of fuel, is approximately mF( — Aho ). Ideally this is equal to the heat input mcv( T3 — T2 ) in the Otto cycle (see Fig. 12.13a) or mc p( T3 — T2 ) in the Diesel cycle (see Fig. 12.13b). It follows that the indicated thermal efficiency of the engine is approximately equal to the airstandard efficiency. For example, for the SI engine, =
I Hid
m I WI
mF( —Oho) mcv(T3 — T2 )
— Otto cycle efficiency
In practice this analogy is far less close than the comparable analogy between the processes in the opencycle gas turbine and the airstandard Joule cycle. The reasons for the poorer analogy in the case of the reciprocating engine are as follows: (a) Since the processes are carried out intermittently in a single component they are not so clearly defined. For example, the corners of the p— V diagram are rounded owing to the time taken for valves to open and close, and combustion does not occur precisely at constant volume (or constant pressure as the case may be). (b) The temperature changes involved in the expansion and compression are much larger than in gas turbines, and the consequent variation of specific heat capacities is appreciable. (c) The air/fuel ratios used in reciprocating engines are much smaller, so that the properties of the working fluid are markedly different from those of air. (d) The maximum temperature reached at the end of the combustion process is much higher than in gas turbines, and dissociation plays an important role. This implies that the chemical energy of the fuel is used much less effectively for the production of work. (e) Owing to the use of cylinder cooling and the relatively low mass flow per unit surface area in a reciprocating machine, the compression and expansion processes cannot be so nearly described as adiabatic. Nothing further need be said about item (a), but the remaining points require amplification. This will be done by considering the compression, combustion and expansion processes in turn. Compression process
The ratio of specific heat capacities y decreases with increase of temperature, and its mean value for the temperature range normally encountered in the compression process is appreciably less than 1.4 even if the gas is air. The mixing of the incoming charge with residual products of combustion results in a lower value for y for the mixture because the products contain CO2 and H2 O which individually have a relatively low value of y. In SI engines the gas compressed is an air—fuel mixture, and this too has a lower value of y than air. Finally, 412
Reciprocating InternalCombustion Engines
[17.4]
heat transfers from the cylinder to the gas in the early stages of the compression, and from the gas to the cylinder in the later stages, mean that the compression does not follow an isentropic path. The net result of all these effects is that the pressure and temperature at the end of the compression are appreciably less than the values predicted by airstandard calculations (see Example 17.1). Combustion process Owing to the high temperature reached in the combustion process there is an appreciable proportion of dissociated products at the nominal end of combustion. The result is that the full enthalpy of combustion of the fuel is not released and the actual temperature rise is less than would be predicted if dissociation were ignored. The calculation of the adiabatic temperature rise in a chemical reaction was discussed in sections 15.4 and 15.7. Expansion process As the temperature during the expansion falls, some of the dissociated molecules combine, and strictly speaking the combustion process still continues during the expansion. By the end of the expansion the temperature has fallen to a level where the proportion of dissociated products is very small, and the fuel can then be regarded as completely burnt. Evidently the unused part of the enthalpy of combustion is recovered to some extent, although the energy recovered in this way is not so effective for the production of work. This is because the increased pressures resulting from the completion of the reaction are available only over part of the stroke. The efficiency with which the chemical energy is converted into work is therefore decreased by the dissociation occurring in the early stages of combustion. The expansion is also markedly different from the isentropic expansion of air because the hot combustion products have a low value of y and the expansion is far from adiabatic. An appreciable quantity of energy is rejected as heat, particularly during the period of intense chemical activity when radiation from the burning gases to the cylinder wall plays an important role. The effect of all these factors on the p—V diagram of an SI engine is shown in Fig. 17.13. The net result is a considerable reduction in both mean effective Fig. 17.13 Effect of variation of y,
Reduction due to low y in compression
dissociation and heat loss on the airstandard cycle
Reduction due to dissociation
I\ Without recombination and heat loss
With recombination and heat loss
V
413
[17.4]
Work Transfer
pressure and efficiency. It is possible to analyse the processes in IC engines taking the more important of these factors into account, and thermodynamic charts enabling this to be done have been produced by Hottel et al. (Ref. 3). The airstandard cycle is a simple model adequate only for predicting the effect of compression ratio on the performance of an engine. ,The more complex models can predict the effect of other parameters such as the air/fuel ratio. Nevertheless, such calculations are more useful in showing the relative importance of the various 'losses' than for the prediction of an actual engine's performance. This is because other variables, such as the design of the induction system, or those mentioned in the first of the five points listed earlier, also play an important part in determining the performance. Example 17.1
A charge enters a SI engine at 330 K and 1 bar, and is compressed isentropically through a compression ratio of 7 :1. Estimate the temperature and pressure at the end of compression, taking the charge to be (a) pure air with constant specific heat capacities, (b) a stoichiometric mixture of air and octane (C8 H18 ) with variable specific heat capacities. (Neglect the effect of dilution with residual products of combustion.)
(a) With air, the temperature and pressure at the end of compression are given by T2 =T1 r
p2 = pi
= 330 x 70.4 = 719 K
v, T, 719 = 1 x 7 x — = 15.25 bar v2 Ti 330
(b) The combustion equation for octane is 79 C81118 + 12.502 + — 12.5N2 8CO2 + 9H2 0 + 3.76 x 12.5N2 21 Hence the air/fuel ratio by mass is (12.5 x 32) + (3.76 x 12.5 x 28) = 15.05 114 The value of y for the mixture will vary with temperature. Assuming that T2 found in (a) is approximately correct, a mean value of y for the compression can be found from the properties of the mixture at (330 + 719)/2 x 525 K. The value of the gas constant R is R = ( 16.05 x 0.287 ) + 16.05 x
.
x
8.314 114
0.274 kJ/kg K
At 525 K, c,, for air is 1.035 kJ/kg K and for octane 2.691 kJ/kg K. Hence for the mixture ( 15.05 x 1.035 c 1 x 2.691 = 1.138 kJ/kg K P 16.05 16.05
y= 414
c cP
—R
—
1.138 0.864
— 1.317
Reciprocating InternalCorVibustion Engines
[17.5]
The temperature and pressure after compression are therefore T2 =
330 x 7'7 = 612 K
• p2 = 1 x 7 x
330
13.0 bar
A better estimate can now be obtained by taking the properties of the constituents at the mean temperature of (330 + 612)/2 = 471 K, when for the mixture cp = 1.115 kJ/kg K and y = 1.326. T2 is then found to be 622 K and p2 13.2 bar. Evidently a further approximation is not necessary.
17.5 Maximum work of a chemical reaction
It has been seen that there are ',tactical limits to the work output which can be obtained from the combustion of a fuel in an internalcombustion engine in which the reaction is rapid and highly irreversible. Of rather more academic interest is the question of what is the maximum possible work that can be derived from any particular chemical reaction. Since the power is derived from a noncyclic process while heat is exchanged with a single reservoir (i.e. the surrounding atmosphere), and not from a cycle working between two reservoirs, the Carnot efficiency cannot be a guide in answering this question. In effect the question posed has been answered in section 15.7, but the following paragraphs discuss this problem more explicitly. For an efficient conversion of chemical energy into work it is essential for the reaction to be carried out reversibly. A hypothetical 'reversible IC plant has already been described in section 15.7.1—the van't Hoff equilibrium box. The particular van't Hoff box described therein performs the reaction CO + 102 CO2 reversibly while exchanging heat with one reservoir. In doing so it produces the maximum possible amount of work, and hence it rejects the least possible amount of heat. The reaction proceeds isothermally, indicating that a high temperature at some point in a combustion process is not essential for maximum work output. The reason why the efficiency of a real IC engine increases with increase of compression ratio, and hence of peak temperature, is therefore not obvious. It lies in the fact that in the hypothetical reversible engine the chemical energy is transformed directly into work, which is not the case in a conventional IC engine. The rapid combustion occurring in the latter results in the chemical energy being first of all transformed into random molecular energy (i.e. sensible internal energy) as manifested by the rise in temperature accompanying the combustion process. Apart from the chemical change of some of the constituents, this irreversible combustion has the same effect of increasing the sensible internal energy of the gases (mainly nitrogen) as an external heat addition at the appropriate temperatures. Once the intermediate transformation into sensible internal energy is accepted as inevitable, the analogy between the real process and the equivalent airstandard cycle has shown that the practical IC engine efficiency will improve with increase of peak temperature (i.e. compression ratio). It should not be forgotten, however, that a reversible isothermal reaction would 415
[17.5]
Work Transfer
result in a much high proportion of the chemical energy being transformed into work. A numerical example may be helpful. The expression for the maximum work which can be done in any reversible process by the reactants CO and 02, exchanging heat with a single reservoir at temperature T, was found in section 15.7.2, to be given by equation (15.19). The maximum work, per kmol of CO, therefore becomes innax = RT ln Ke The reactants are assumed to enter in stoichiometric proportions at standard pressure p° and temperature T, with the product CO2 leaving at the same pressure and temperature. For a temperature T = 298.15 K, the equilibrium constant is found from tables to be In Ke = 103.762. Hence, per kmol of CO, I Wimax = 8.3145 x 298.15 x 103.762 = 257 220 kJ Since the enthalpy of reaction Ari39, is — 282 990 kJ per kmol of CO, it is evident that I Win. ax is nearly equal to Ah2981• Neglecting kinetic energy terms, the heat transferred to the surroundings can be found from the steadyflow energy equation Q = Arz398 + I WI.
282 990 + 257 220 = — 25 770 kJ
The work I In.., need not necessarily be less than the negative of the enthalpy of reaction. If a similar calculation is carried out for the reversible combustion of a stoichiometric mixture of C and 02, it can be shown than I WImax is greater than ( — Ari398); in this case heat is received from the surroundings during the process. The definition of efficiency that is normally used for IC plant, whether W/Arialiq) of W/ArOvap), is therefore not logically sound because theoretically it can be greater than unity. A process efficiency should be defined as a ratio X/Xmax, where X and Xmax are the actual and maximum possible values of the physical quantities concerned in the process. A more rational definition therefore would be iWiii It is found that for hydrogen and the usual hydrocarbon fuels — 4R(vap) is numerically close to 1WI„,„„, while — Araiq) differs from I WImax by a much wider margin. Hence I WI W imax
1 WI
Arit(vap)
and this provides the principal argument in favour of defining thermal efficiencies by equation (15.14) rather than (15.13). It is interesting to note that the value of I WIrnax, unlike that of AR), does not depend on the phase of H2 O in the products of the fuel, and this is proved formally in section 7.9.3. One final comment: we have seen that there is no fundamental thermodynamic reason why the efficiency of an IC engine should not be 100 per cent, and therefore presentday utilisation of our fuel resources is far removed from the ultimate standard of perfection. Because an appreciable fraction of the work produced by the world's power plant is used for the production of electricity, 416
[17.5]
Reciprocating InternalCombustion Engines
an improvement in fuel utilisation would undoubtedly follow if we could convert chemical (and nuclear) energy directly into electrical energy in a reversible reaction. Although there are some chemical reactions which allow chemical —) electrical energy conversions with a high degree of reversibility, as in the leadacid accumulator and the hydrogenoxygen fuel cell (see section 20.4), no equally efficient device has yet been developed for common fuels and air. Any such device would almost certainly not permit high rates of energy transformation; the advantage of irreversible combustion at high temperature is that very high power outputs can be produced by relatively small power plant.
417
18 OneDimensional Steady Flow and Jet Propulsion
The steadyflow energy equation was deduced in Chapter 4 as a consequence of the First Law of Thermodynamics. The equation relates the heat and work transfers across the boundary of an open system, to the mechanical and thermodynamic properties of the fluid at the inlet and outlet where these properties can be assumed constant across the crosssection of flow. No assumption had to be made about whether the flow was frictionless or not, and the derivation did not require any knowledge of the flow within the open system. We have seen that this equation enables a useful range of problems to be solved. For example, when considering adiabatic flow in a nozzle, a knowledge of the initial enthalpy, initial velocity and final enthalpy enables the final velocity to be calculated. If the adiabatic flow is also assumed to be frictionless, the fact that the entropy is constant—a consequence of the Second Law of Thermodynamics—enables the final thermodynamic state to be predicted. The principle of conservation of mass—in the form of the continuity equation—then enables the inlet and outlet areas to be determined for any given mass flow. The foregoing analysis, however, has nothing to say about how the crosssectional area of the nozzle must change between inlet and outlet for the results to be physically possible. Before this kind of information can be obtained from the analysis, some knowledge of the flow within the open system is evidently necessary. This extension of the analysis is undertaken in the science of fluid dynamics. With the advent of highspeed flight, turbojet engines, ramjets and rockets, fluid dynamics has been enormously extended in recent years— particularly the branch dealing with compressible flow known as gas dynamics. Gas dynamics is now studied as a subject in its own right, and can no longer be adequately covered by a chapter in a book of this kind. All that will be attempted here is the consideration of a few special cases with the object of emphasising the point at which a simple thermodynamic analysis must be reinforced by a more complete treatment. Such a treatment (a) must involve some assumption about the flow within the open system, and (b) may involve explicitly Newton's Second Law of Motion. A case where item (a) is necessary and sufficient will be considered first before any attempt is made to explain what is meant by item ( b).
418
[18.1]
OneDimensional Steady Flow and Jet Propulsion
18.1 Isentropic flow in a duct of varying area
When a fluid flows through a duct with no work or heat transfer, the only factors which can cause a change in fluid properties are (i) a change in flow area, and (ii) frictional forces. In this section we shall assume that frictional forces are absent. The effect of variation in the crosssectional area of the duct may be determined if some assumption is made about the nature of the flow. The simplest type of flow conceivable is onedimensional steady flow. With reference to Fig. 18.1, the flow is said to be onedimensional if the following conditions are fulfilled: (a) Changes in area and curvature of the axis are gradual. (b) Thermodynamic and mechanical properties are uniform across planes normal to the axis of the duct. No real flow is truly onedimensional, but provided that there are no sudden changes in direction or area, and that average values of the properties at any crosssection are used in the analysis, the onedimensional treatment yields results which are sufficiently accurate for many purposes. When the flow is onedimensional, the properties are uniform over any crosssection of the flow within the open system—not merely at inlet and outlet. It is therefore possible to apply the energy equation to the flow between any two planes 1 and 2, and so, for given inlet conditions, to determine the properties at any section along the duct. Consider the case of isentropic flow in a nozzle (or diffuser). Given pi and Ti (or x1 if the fluid is a wet vapour), the thermodynamic properties at various values of p2 can be found using the equation of state (or tables of properties) together with the fact that s2 equals sl . Given also the initial velocity C1 , corresponding values of C2 can be found from the energy equation , h2 + — = n i + — 2 2 Finally, given the inlet crosssectional area A1, corresponding values of A2 can be found from the continuity equation A2 C2 = A1 C1 V2
V1
The variation of V2, C2 and A 2 with p2 can then be represented by curves of the form shown in. Fig. 18.2. Although the precise shape of the curves depends upon the equation of state of the fluid, all gases and vapours exhibit the same Fig. 18.1 Onedimensional' ducts
1
2
ezazzi eezelv 2 2 ./... . Mem/1a" I
I
419
[18.1 ]
Work Transfer
Fig. 18.2 Variation of v, C and A with pressure along a duct
general behaviour under these conditions. One point of interest is the very gradual change in specific volume v at low velocities. For some analyses of lowspeed gas flow it is possible to simplify the calculations without much loss of accuracy by assuming that the specific volume is constant. This realm of fluid dynamics is called incompressible flow and the treatment is then identical for liquids and gases. Fig. 18.2 can be interpreted as applying to either a nozzle or a diffuser. Moving from left to right on the diagram, the pressure p2 is falling and the duct acts as nozzle. Although both the specific volume and the velocity increase continuously during the expansion, the flow area decreases to a minimum and then increases. A glance at the continuity equation shows that this will happen if the rate of increase of specific volume is at first less than, and finally greater than, the rate of increase of velocity. Such behaviour is always exhibited by gases and vapours. The pressure ratio at which the minimum area is reached is called the critical pressure ratio; at this point the mass flow per unit area is a maximum. 18.1.1 Derivation of the basic equations
It is more informative if the foregoing stepbystep method of calculation is replaced by the analytical approach which follows. First it is necessary to arrive at equations expressing the First and Second Laws, and the principle of conservation of mass (continuity), in differential form. Applying the steadyflow energy equation between any two planes an infinitesimal distance apart, we arrive at the differential energy equation per unit mass: 2 dQ + dW = dh + d C' 2
(18.1)
When applied to the simple case of adiabatic flow in a nozzle or diffuser, (18.1) reduces to dh + c1( 420
2 =0
(18.2)
OneDimensional Steady Flow and Jet Propulsion
[18.1]
Applying the Second Law to the flow between planes an infinitesimal distance apart, we have the result that for a reversible process dQ = T ds We also have the general relation between properties, equation (6.13), which states that T ds = dh — v dp For an isentropic process, therefore, (18.3)
dh = v dp
The differential form of the continuity equation is most easily obtained by logarithmic differentiation. Thus we have log A + log C — log v = constant and differentiating, dA dC dv A + C v
n
(18.4)
Equations (18.2) to (18.4) can be used to find expressions for the changes in velocity and area with pressure in an isentropic process. Thus, combining (18.2) and (18.3), v dp + d( c2 ) = 0 2 For the flow between any two planes 1 and 2 we therefore have 2 12 (C22  C;) _ f v dp 1
(18.5)
(18.6)
For any given fluid there is a definite relation between p and v in an isentropic process, and when this is known in algebraic form the RHS of the equation can be evaluated. To find the change in area required to accommodate the flow, equation (18.5) can be substituted in (18.4) to yield 1 dA v, dv 1 dv — = — cap + — = v dp — + — A C2 C2 v 2 dp
(18.7)
It is shown in texts on fluid dynamics that the velocity of propagation of a small pressure wave through a fluid (i.e. a sound wave) is given by a 2 = — 1)2(410v),
(18.8)
The bracketed term is the rate of change of pressure with specific volume at constant entropy.* Since equation (18.7) refers to isentropic flow, (18.8) may * It is conventional to use the density p in place of v in fluid dynamics; the expression is therefore usually written as a 2 = (oplap),.
421
[18.1 ]
Work Transfer
be used to substitute for dv/dp to give 1 1) dA — = v dp — A C 2 a2
(18.9)
where a is the local velocity of sound in the fluid at the section in the flow where the pressure is p and the specific volume is v. Equation (18.9) may be interpreted directly without integration. Considering accelerated flow, decelerated flow and constant velocity flow in turn, the most important consequences are as follows: Accelerated flow (nozzle) dp must be negative so that: (a) When C < a, dA is negative, i.e. the duct must converge. (b) When C > a, dA is positive, i.e. the duct must diverge. Decelerated flow (diffuser) dp must be positive so that: (a) When C < a, dA is positive. (b) When C > a, dA is negative. Constant velocity flow dp is zero so that: (a) Whether C a, dA is zero. It follows immediately that if the flow is to be continuously accelerated from a subsonic to a supersonic velocity the duct must have a throat between the two regions, at which dA is zero and the velocity C is equal to the local sonic velocity a, as in Fig. 18.3a. The same remarks apply to a flow continuously decelerating from a supersonic to a subsonic velocity, as depicted in Fig. 18.3b. Fig. 18.3
Throat
Throat
Flow in a duct of varying area I I
I
C~C < a —or—C > a oi constant 1 C= a 1 I I
C,p lo—C > a —or,— C < p ot constant 1
p decreasing continuously
(b) Diffuser
Throat
I
k
1
p increasing continuously
(a) Nozzle
p falling I p rising )re C rising C falling
(c) Venturi
422
C = a
OneDimensional Steady Flow and Jet Propulsion
[18.1]
When there is not a continuous rise (or fall) of pressure, the presence of a throat does not necessarily imply that the velocity there is sonic: Fig. 18.3c illustrates the case of a venturi where a subsonic flow is accelerated and then decelerated without sonic velocity ever being reached. The condition at the throat is that of constant velocity flow with dp zero. One final point is worth noting from the foregoing analysis: it is that the critical pressure ratio is that pressure ratio which will accelerate the flow to a velocity equal to the local velocity of sound in the fluid, because this is the point in the flow where the area is a minimum and the mass flow per unit area a maximum. All these deductions have been made without reference to any particular fluid, and they apply equally to liquids and gases. The reason why it is never necessary in practice to use convergentdivergent nozzles or diffusers for liquids is that the velocity of sound in a liquid is about 1500 m/s. Such a velocity is quite outside the range of practicable velocities of flow in view of the friction which would be involved. The analysis can be carried further if we restrict our attention to certain types of fluid for which there is a simple algthraic relation between 'p and v in an isentropic process; equations (18.5) and (18.7) may then be integrated analytically. For a perfect gas we have the isentropic relation pvY = constant Although no such simple equation can be formulated for the isentropic expansion or compression of a vapour, it was pointed out in section 9.4 that a good approximation is provided by the same type of polytropic law, i.e. pun =
constant
When the vapour is steam, initially wet with a dryness fraction 0.7 < x < 1.0, then for an isentropic expansion n 1.035 + 0.1x (see section 9.4). Thus with x R., 1.0 and the whole expansion in the wet region, n 1.135. When the steam is initially sufficiently superheated for the whole of the expansion to lie within the superheat region, n 1.30. Consideration of what happens when the steam is initially only slightly superheated, so that condensation can be expected to occur inside the nozzle, must be left to section 18.2. To provide a uniform solution for gases and vapours, the symbol n will be used for the index of isentropic expansion. The resulting equations, however, will be exact only for perfect gases, i.e. for the case where n = y. To avoid obscuring the essentials by lengthy equations, we shall consider only the simple case of a continuous expansion from an initial state where the velocity may be considered negligible. Fig. 18.4 shows the nomenclature employed. Using the polytropic relation between p and v, and putting C1 equal to zero, equation (18.6) gives the velocity at any plane 2, whether in the convergent or the divergent part of the duct, as n , (P2v2 — Piv 1) 1—n
423
[18.1 ]
Work Transfer Fig. 18.4 Convergentdivergent nozzle
t
Cl = 01
and hence C2
f(p2 )(11— 1)1n
I 2n =
L 1 n
1/2
(18.10)
poi
Note that, for any given initial state, there is a maximum possible velocity which is achieved when the fluid is expanded to zero pressure. This maximum velocity is )1/2 ( 2n (18.11) Cnim POI n
1
The curve representing C2 in Fig. 18.2 does not, therefore, proceed to infinity. The required area at any plane 2 can be found by integrating (18.7), but it is more easily obtained by computing C2 and v2 and using the continuity equation directly. Thus, if th is the mass flow, we have m=
A2C2 A2
or
v2
v — 2 —
vi
(18.12)
iil C2 C2(P2/P1)1In
An expression for the mass flow per unit area can be found by taking the reciprocal of (18.12) and substituting for C2 from (18.10). This yields th
—
A2
2n pl [1 — n vl
p2 ("+ oi" p,
—
n _ 2/n 1 : 21
1/2
(18.13)
Pi
The mass flow per unit area is a maximum at the throat, and the pressure at the throat can therefore be found by differentiating (18.13) with respect to p2 and equating to zero. The result is that rh/A2 is a maximum when p
2
n/(n— 1)
2 =
P1
n+1
In this equation p2 is the throat pressure p„ and it is also referred to as the critical pressure pc. The critical pressure ratio is therefore 2 )111(n— 1) Pt = P. = — — (18.14) n+1 Pi Pi The following gives the critical pressure ratio for four values of n:
424
n
1.135 1.300 1.400 1.667
P./P1
0.577 0.546 0.528 0.487
OneDimensional Steady Flow and Jet Propulsion
[18.1]
The value of the maximum mass flow per unit area can be found by substituting (18.14) in (18.13), giving / 2 \(n + 1)/(n 4 1) 1 1/2 pi (18.15) —= n
A,
v,
(n + 1)
The general result, that the velocity at the throat will be sonic, has already been deduced from equation (18.9); it is easy to check this for the special case of fluids which expand isentropically according to the law pv" = constant. Thus substituting (18.14) in (18.10), the throat velocity is )1/2
= ( 2n
+ npiv
Using pi v", = pg in conjunction with (18.14), this can be transformed to (18.16)
C,= (nPivi) 112
Sonic velocity at the throat can be found,from (18.8), since by differentiating the isentropic relation pv" = constant we have
(ap) 8u 3
np v
and hence when p = p, and v = v„ a, = (np,v,)112 The required identity between C, and the local sonic velocity is thereby established. It must be emphasised once again that this analysis is for a continuous expansion. The pressure p, and velocity C„ given by the foregoing equations, are the minimum and maximum values respectively which can be achieved at the throat with the given initial conditions pi and v1. Higher values of p„ and lower values of C„ are possible in a venturi where the pressure increases after the throat. When the fluid is a perfect gas, we may substitute n = y and pu = RT in the previous equations to obtain
C2
2Y RT {( P2 )(r1"' — 1111/2 =[ 1 — Y Pi 2y
1 f (P2)(7 + 1"Y
A2 = Pi [ 1 — y RTI tp i Pi
2
P.
(18.17) )2/y 11/2
( P 2
(18.18)
P1 )
)),/(),  1)
Pi Pi (Y + 1 ) Ct =
th At
a, = (yR'T,)112 ( 2 vy + my 11/2
—PI
Y
RTi y + 1) 425
[18.1]
Work Transfer
A simple expression for the ratio T,/ T1 can also be formulated in this instance:
T = (Pt)(y10
2
p,
Y+ 1
1
(18.22)
Equations (18.17) to (18.22) can be deduced more easily and directly by using the energy equation in the form cp T, = cp T2 + 1C3 but this is left as an exercise for the student. Much of the preceding analysis has only been necessary to obtain an expression for the critical pressure ratio, equation (18.14). Most calculations on the design of nozzles are easily made from first principles once (18.14) has been established. The following example illustrates this.
Example 18.1
Determine the throat area, exit area and exit velocity for a steam nozzle to pass a mass flow of 0.2 kg /s when the inlet conditions are 10 bar and 250 °C and the final pressure is 2 bar. Assume that the expansion is isentropic and that the inlet velocity is negligible.
Ot Fig. 18.5 illustrates the process on an h—s diagram. Using n = 1.3 when finding the critical pressure ratio, we have from (18.14) 2 )1.3/0.3 Pt = 0.546 +1 and hence Pt = 0.546 x 10 = 5.46 bar Since the expansion is isentropic, st = s1 = 6.926 kJ/kg K The steam is still superheated at the throat because st is greater than the saturation value 6.794 kJ/kg K at the throat pressure of 5.46 bar. By a double interpolation in the superheat table, of which only the second step is
Fig. 18.5
h
426
OneDimensional Steady Flow and Jet Propulsion
[18.1]
given here, the enthalpy and specific volume at the throat are found to be
h, = 2753 + (2854 — 2753)
6.926 — 6.794 (at 5.46 bar) 7.018 — 6.794
= 2813 kJ/kg v, = 0.3476 + (0.3916 — 0.3476)
6.926 — 6.794 7.018 — 6.794
at 5.46 bar)
= 0.3735 m3 /kg Now from the energy equation with C1 = 0,
C, = {2(h,. — = {2 x 103(2944 — 2813)}1/ 2 = 511.9 m/s From the continuity equation, the required throat area is
A,—
du) 0.2 x 0.3735 [m2] = 1.46 cm' — C, 511.9
The dryness fraction at exit may be found from S2
= S1 = Sf2
x2 —
X2 Sfg2
6.926 — 1.530 — 0.964 5.597
Therefore
h2 = 505 + (0.964 x 2202) = 2628 kJ/kg v2 = 0.964 x 0.8856 = 0.8537 m3 /kg The exit velocity is therefore C2 =
{2 x 103(2944 — 2628)}1/2 = 795.0 m/s
and the exit area required is A 11. 2
0.2 x 0.8537 795.0
[m2] = 2.15 cm2
Note that the approximate expression pV1I3 = constant has been used only to determine the critical pressure ratio, and hence indirectly the throat area. The throat and exit velocities have been calculated from the correct isentropic enthalpy drop and not from Iv dp. Note also that such calculations are greatly simplified if values of the enthalpy drop and specific volume can be read directly from an h—s chart.
18.1.2 Phenomena in nozzles operating off the design pressure ratio
This section has so far been devoted to establishing the area changes necessary for a continuous isentropic expansion from a given initial state to a given final
427
[18.1]
Work Transfer
pressure. It is also of interest to know what happens to the flow in a nozzle of given dimensions when the downstream pressure differs from the value for which the nozzle is designed. In this respect the behaviour of convergent and convergentdivergent nozzles is different, and the two types must be considered separately. Convergent nozzle
Consider the experimental setup shown in Fig. 18.6. The inlet conditions are maintained constant and the downstream pressure pc is gradually reduced from the inlet pressure pi by opening the valve. When pe = pi there is no pressure drop and no flow, shown by curve (i). As pc is reduced, the axial pressure distribution takes the form of curve (ii), and the mass flow increases as shown in Fig. 18.6b. The pressure p2 in the plane of the nozzle exit is always equal to pc. This state of affairs continues until pe/p1 is reduced to the critical pressure ratio pc /p„ corresponding to curve (iii). At this operating condition the nozzle passes the maximum mass flow, given by equation (18.15), and p2 = pc = pc. Further reduction of pc cannot produce any change in the flow within the nozzle because we have seen that p2/pi cannot be less than the critical pressure ratio unless there is a throat upstream of plane 2. Consequently, for all values of pe less than pc, the pressure p2 in the plane of the exit remains constant at the critical pressure pc . There is therefore no further change in specific volume or velocity at plane 2 and no change in mass flow. The mass flow remains at the maximum value, as shown in Fig. 18.6b, and the nozzle is said to be choked. On leaving plane 2 the fluid undergoes an unrestrained and irreversible expansion to pc, as illustrated by curve (iv), and the flow is no longer amenable to simple onedimensional treatment. What happens is that the pressure Fig. 18.6 Flow in a convergent nozzle with varying back pressure
/
IP > Pe 44J/1 10%%.. ,  I
//////////// ////////////
4
.4424(4,4 Pc
< Pe
l Pe < Pc ) ic
1
Pe/P1 (b)
0
OneDimensional Steady Flow and Jet Propulsion
[18.1] Fig. 18.7 Flow in a convergentdivergent nozzle with varying back pressure
1 (ii)
2
(iii) P2 = Pc
P
(iv) )1( (V) P2 > Pe
Distance along axis (a)
Distance along axis (b)
oscillates around Pe, as shown in Fig. 18.6c, and the supersonic velocity achieved in the initial divergence of the stream is rapidly reduced by viscous friction. Convergentdivergent nozzle
Fig. 18.7 shows a similar setup with a convergentdivergent nozzle. When operating at the design pressure ratio, appropriate to the throat and exit areas of the nozzle, the flow accelerates continuously from a subsonic to a supersonic velocity. The axial pressure and velocity distributions are then represented by curves (iv) in Figs 18.7a and b. Now consider what happens as pc is slowly reduced from pi to the design exit pressure. At first the duct acts as a subsonic nozzle followed by a subsonic diffuser, i.e. as a venturi, and the pressure distribution appears as curve (i). The mass flow increases during this range of pe until the conditions are such that the throat pressure p, is equal to the critical pressure pc, shown by curve (ii). The mass flow is then a maximum and the nozzle is choked. Further reduction of pc cannot alter the conditions at the throat and the mass flow thereafter remains constant. If pc is reduced below the value giving rise to curve (ii), the process of acceleration followed by diffusion can no longer continue in the same manner as before. This is because once the stream has acquired a supersonic velocity, a converging duct is necessary for an isentropic diffusion process. Evidently the normal type of continuous isentropic flow process can no longer exist under these conditions. Mathematically speaking, the equations expressing the constancy of energy, mass and entropy cannot be satisfied simultaneously in the given duct. The energy and continuity equations are fundamental and must be satisfied; it is the assumption of isentropic flow which must be discarded. What happens is that a discontinuity—known as a shock wave—is formed in the flow. A shock wave involves a rise of pressure, an increase of entropy, and 429
Work Transfer
[18.2]
a deceleration from a supersonic to a subsonic velocity.* These events occur suddenly in a very short distance, and the resulting subsonic stream is then diffused normally in the remaining length of the divergent duct to satisfy the condition that p2 equals pe. The pressure distribution then corresponds to curve (iii). As Pe is reduced towards the design value, the shock wave moves down the divergent part towards the exit. When it reaches the exit, the shock wave changes its character and becomes inclined to the direction of flow, and the downstream velocity can then remain supersonic. Finally, if pe is reduced below the design value, the pressure p2 remains constant at the design value and an uncontrolled expansion to pe occurs outside the nozzle in a manner similar to that already described for the convergent nozzle. 18.2 Metastable flow of vapours
Before leaving the subject of flow in nozzles, it is necessary to describe a phenomenon peculiar to the rapid expansion of a vapour. The ideal case of isentropic expansion of a superheated vapour to a state in the wet region is depicted on the T—s diagram in Fig. 18.8a. At the point in the expansion where the pressure is /32 a change of phase should begin to occur. At this point the random kinetic energy of the molecules has fallen to a level which is insufficient to overcome the attractive forces of the molecules, and some of the slower moving molecules coalesce to form tiny droplets of condensate. Now this process, although rapid, does not have time to occur in a nozzle where the flow velocity is very great. The achievement of equilibrium between the liquid and vapour phases is therefore delayed, and the vapour continues to expand in a dry state. If the constant pressure line p3 in the superheat region is extended into the wet region, the final state could be represented by point 3 in Fig. 18.8b. Between pressures p2 and p3 the vapour is said to be supersaturated or supercooled. The latter term owes its origin to the fact that at any pressure between p2 and p3 the temperature of the vapour is always less than the saturation temperature corresponding to that pressure. The path of the process between 2 and 3 is shown dashed in Fig. 18.8b because these states are not states of stable equilibrium; they are called metastable states. The type of equilibrium established is certainly not stable because a disturbance, such as the introduction of a measuring instrument, can bring about condensation and a restoration of the stable state of equilibrium between liquid and vapour. Neither can the state be regarded as unstable, because this term is only applied to states for which any infinitesimal disturbance will cause a major change of state. An infinitesimal disturbance, such as the formation of a tiny droplet, is insufficient to bring about general condensation. When designing steam nozzles, it may be assumed that the supersaturated vapour expands according to the laws of the superheated vapour. As steam * A onedimensional treatment can still be used to analyse flow involving some types of shock wave, but for this the student must turn to texts on fluid dynamics, e.g. Ref. 5 or the useful summary in Appendix A of Ref. I.
430
[18.2]
Fig. 18.8
OneDimensional Steady Flow and Jet Propulsion
T
T
(P1
Metastable states
1
•
3
P3
[4(2
,\ 3 S
S (b)
(a)
tables do not normally extend the stable superheat range into the metastable supersaturated region, extrapolation of property values is most easily carried out by reference to approximate property relations for superheated steam. The simplest equation which can be used for this purpose is equation (9.8), which led to the following two useful relations for an isentropic process: pv1• 3 = constant and p/T1• 3/°•3 = constant These equations enable the final state and the isentropic enthalpy drop to be predicted. Thus in practice, owing to the phenomenon of supersaturation, the value of 1.3 should be used for n even if the steam is only just superheated initially and most of the expansion occurs in the 'wet region'. The following example shows that the mass flow through a nozzle is increased by supersaturation. In early experiments on nozzle flow it was noticed that the measured mass flow was often greater than the value estimated on the assumption of a normal expansion with phase equilibrium, and it was this fact that drew the attention of engineers to the phenomenon of supersaturation. Example 18.2
Dry saturated steam at 2.8 bar is expanded in a simple convergent nozzle to a pressure of 1.7 bar. The throat area is 3 cm 2 and the inlet velocity is negligible. Estimate the exit velocity and mass flow (a) if phase equilibrium is assumed throughout the expansion and (b) if the steam is assumed to be supersaturated. (a)
Assuming isentropic expansion, the dryness fraction at the exit is given by Sl
= S2 = St 2 + X25152
7.015 = 1.475 + x2 5.707 and hence x2 = 0.971 Hence h1 — h2 = 2722 — {483 + (0.971 x 2216)} = 87 kJ/kg C2 = {2(h1 h2 )1112 = (2 x 103 x 87)1/2 = 417 m/s v2 = X2 Vg2 = 0.971 x 1.031 = 1.001 m3 /kg — (b)
A 2 C2 v2
3x417 = 0.125 kg/s 104 x 1.001
Assuming the supersaturated expansion to conform to pv1 •3 = constant, 431
[18.2]
Work Transfer
and using (18.10), we have C2 —
n (n1)/n }11/2 [ 2n —1 pl y, {(" ) 1—n P
v1 is 0.6462 m3 /kg from tables, so that [2 x 1.3 C2
0.3 10
Pi v2 = v (—
)1/n
5 x 2.8 x 0.6462 11 —
1.7
2.8
= 413 m/s
.8 )1/1.3 = 0.6462 ( 2 = 0.949 m3 /kg
P2 ph _
1 3 x 413 = 0.131 kg/s 104 x 0.949
Note that part (b) may be solved using equation (9.11) to find ( h2 — h1) and hence C2 , and (9.10) to find v2. Provided that the vapour remains supersaturated up to the outlet of the nozzle, the method used in the previous example is adequate because, in the absence of friction, the process within the nozzle can be considered reversible and therefore isentropic. The restoration of equilibrium is an irreversible process, however, and if this occurs at some point within the nozzle the prediction of the final state is difficult. The supersaturated condition cannot continue indefinitely; the delay in condensation leads to a buildup of molecular cohesive forces which finally results in sudden condensation at many points in the vapour. Much work has been done to determine the minimum pressure to which steam may be expanded before condensation occurs, and a description of some of these experiments is given in Refs 7 and 8. It has been found that even if the steam is only just superheated at the beginning of the expansion, the condensation pressure is less than the critical pressure. Thus the irreversible restoration of stable equilibrium always occurs after the throat of a steam nozzle, and an estimate of the mass flow for a given throat area can always be made in the manner indicated by Example 18.2b. The difficulty arises in predicting the conditions at the outlet of convergentdivergent nozzles of large pressure drop. Experiments have shown that the condensation occurs suddenly with an increase of both entropy and pressure. Fig. 18.9 Restoration of equilibrium
OneDimensional Steady Flow and Jet Propulsion
[18.31
Fig. 18.9 illustrates a frictionless expansion of this kind on the h—s diagram. When designing nozzles in practice, it is always necessary to introduce a `coefficient' or 'efficiency' to allow for the increase of entropy due to friction, and this factor, being experimentally determined, will automatically take into account the increase in entropy due to the condensation process. The prediction of the final state by such means will be made clearer in the next section when the effects of friction are discussed. 18.3 The momentum equation It is now appropriate to explain what was meant in the introduction to this chapter by the statement that it is sometimes necessary to invoke explicitly Newton's Second Law of Motion. It may seem surprising that we have been able to solve any problem concerned with motion without reference to this fundamental principle. The fact is, however, that so far we have been concerned with problems for which the Second Law of Motion is expressed implicitly in the energy equation. This point may be appreciated if we think for a moment of how the energy equation is deduced for a purely mechanical system. The starting point is Newton's Second Law, that the force acting on a body is equal to the rate of change of momentum in the direction of the force, i.e.
F=
d(mC) dt
(18.23)
Equation (18.23) is the simplest form of momentum equation. If a body of constant mass m is moved a distance dx by the force F, we can write dC F dx = m(— ) dx dt And since dx = C dt, this becomes F dx = mC dC which on integration yields 2
F dx = 2 — The LHS can be integrated directly if there exists a function of x, which we may denote by P, such that dP/dx = —F. We then have f 2 —dP =
2
—
Or
P1 + fincl = P2 + fmci
(18.24)
In these circumstances there is a quantity (P + mC2 /2) which remains constant during the motion; it is called the energy of the body. mC2 /2 is the kinetic energy and P the potential energy. If the force is simply that due to gravity, 433
[18.3]
Work Transfer
F = constant = —mg, and the change in potential energy is P2 — P 1 = Ing(x 2 — x1 ) Or again, if the force is the restoring force of an extended spring, F = —kx where k is the spring stiffness, and P2 — PI = — (xi xi) 2 The integrated equation (18.24), which is an equation of mechanical energy, is equivalent to the equation of momentum and the two are interchangeable. It is often more convenient to use the energy equation because it relates scalar quantities; the momentum equation, on the other hand, relates vector quantities. The simplest energy equation for a purely mechanical system is only another form of the momentum equation because it has been deduced from it without further reference to empirical data. But this energy equation applies only to frictionless systems. Friction forces are not simple functions of position (i.e. we cannot write dP/dx = — F), and they involve the transformation of mechanical forms of energy into other quite different forms (e.g. internal energy) with which classical mechanics is not concerned. A more comprehensive energy equation can be formulated only when the additional generalisation of the First Law of Thermodynamics has been introduced. Then the energy equation rests upon its own empirical ground and applies to any system whether frictionless or not and whether adiabatic or not; it is no longer simply another form of the momentum equation. We should not be surprised, however, if the energy and momentum equations appear to be identical when friction forces are assumed to be absent and the process is adiabatic. Conversely, when these conditions are not fulfilled, we can usefully employ both the general energy equation and the momentum equation, because they are no longer identical but express different fundamental principles. It is now necessary to apply Newton's Second Law of Motion to fluid flow. The deduction of the most general form of this momentum equation is left to texts on fluid dynamics; we shall restrict our attention to onedimensional steady flow. Heat may be transferred to the fluid provided that it changes the fluid properties uniformly across the crosssection of flow. Consider the open system between planes 1 and 2 in Fig. 18.10. In time dt the mass between 1 and 2 plus the mass equal to dm moves to the right. Newton's law states that the vector sum EF of all the external forces acting on dm Fig. 18.10
Force on a duct due to fluid flow
/
After time dt C2
C2
Clx
12 Sign convention:
\1 Fy and Cy positive F, and C, positive
434
OneDimensional Steady Flow.and Jet Propulsion
[18.3] Fig. 18.11 Pressure forces on an element of a straight duct
0 A + dA k C + dC
A30 C
v + du
p + dp 1
Rotor blade h2
Stator blade Stator diaphragm
(b) Gland
blades (which are then often referred to as nozzle blades) and the stage is called an impulse stage. In a 50 per cent reaction design the pressure ratios across the stator and rotor blades are approximately equal. This will be referred to here simply as a reaction stage because we shall not be considering the use of other values of A. The mode of action of the turbine can best be studied by following the path of the fluid through a single stage at the mean radius of the annulus, as in Fig. 19.3. We shall adopt the practice, now commonly used for both turbines and compressors, of measuring all blade and fluid flow angles from the axial direction. The fluid enters the stage with velocity Co at pressure po and is expanded to pi in the stator blades. It leaves these blades with a velocity C1 , in a direction
Fig. 19.3 Velocity triangles for a turbine stage w Positive directions 1
a
Rotor blades al.1.
C2„,
454
Stator blades (or nozzle blades) U V1
Rotary Expanders and Compressors
[19.2] Fig. 19.4 Velocity diagrams of a turbine stage
(6)
making an angle a t with the axial direction. C1 must satisfy the energy equation 1 2(C2 1
 C20) 0 1
(19.6)
The velocity of the fluid relative to the moving blades can be found by subtracting vectorially the blade speed U. This is easily accomplished by drawing the inlet velocity triangle. To avoid a multiplicity of indices, relative velocities will be denoted by V, and the relative velocity at inlet to the rotor blades is therefore V1 . V1 makes an angle fil with the axial direction, and if the fluid is to flow smoothly into the blade passages without undue disturbance, the inlet angle of the blades must be made approximately equal to If the outlet angle of the rotor blades is )2, the direction of the relative velocity at outlet V2 will also be approximately 132 . Applying the energy equation to the flow relative to the rotor blades, it follows that 4(11 — = h1 — h2 (19.7) because no work is done in the frame of reference of the moving blades. V2 must satisfy this equation. Vectorial addition of the blade speed then gives the absolute velocity C2 and the direction oz2. Usually, if this is one stage of a multistage turbine, C2 will be made equal to Co and oc2 equal, to oco; the fluid can then pass on to another similar stage. Equation (19.4a) gives the rate of work done, i.e. I Pfr I = rriU(Ci ,„ — C2,,„) = ritUAC„, Note that the whirl component of the absolute outlet velocity C2,„ is negative in the case depicted in Fig. 19.3. It is usually convenient to combine the inlet and outlet velocity triangles to give the velocity diagram of Fig. 19.4a. It is then easy to see that the algebraic difference of C,„„ and C2,4, is equal to the algebraic difference of the whirl components of the relative velocities at inlet and outlet. Thus* 114,1 = thUAC„ = rhUAV„,
(19.8)
The axial thrust can be obtained from equation (19.1). For an axialflow stage the areas A 1 and A 2 are normal to the axial direction, and consequently (19.1)
* The interchangeability of ,6,C„, and LIV„ is to be expected because, as we have already pointed out in section 18.4.1, the momentum equation upon which (19.8) is based applies in any inertial frame of reference and we are here treating the rotating blade passages as if they are moving linearly with a uniform absolute velocity U.
455
[19.2]
Work Transfer
becomes (19.9)
Ra = th(Cia — C2a) + (p1 Al— P2 A2)
Evidently the term rh(C 1. — C2a) is negative for the particular case shown in Fig. 19.4a. It must be pointed out that equation (19.9) does not necessarily give the total thrust exerted on the shaft bearings. In addition to R. there may be a net pressure thrust acting on the solid rotor disk, of area Ad say, equal to Ad (Pi — p2 ). In impulse turbines p2 is equal to pi , and if Al = A2 as in Fig. 19.2, the thrust due to the pressure terms is zero. Thus only small thrust bearings are required. To reduce the thrust in multistage reaction turbines, the fluid is sometimes introduced at the midpoint of the casing and allowed to expand in opposite axial directions; the machine is then called a doubleflow turbine.
As an alternative to equation (19.8), an expression for the work done can be found in terms of the fluid velocities by eliminating the enthalpy term from the energy equation. Thus, applying the energy equation between planes 1 and 2 of Fig. 19.2a, we have IWI = ph ((h i — h2 ) +
— C3)}
Absolute velocities are used here (i.e. velocities relative to the turbine casing) so that the work term must be included. No work is done in the stator row and YV is therefore the rate of work done in the stage. Using (19.7), the enthalpy term can be eliminated to give (19.10)
=— 61 {(C? — C3) + (V3 — V?)} 2
I
Equation (19.10) can be shown to be identical with (19.8) by considering the geometry of the velocity triangles. Thus =
+ U2 + 21/1 U sin Pi
CZ = V z + U2 — 2V2 U sin #2
Subtracting, —
= V? — V3 + 2U (V, sin /31 +
V2 sin )62 )
But A Vw = V1 sin /31 +
V2 sin )32
and therefore Ilk I =
AV„ = — 1.11 {(C? — 2
+ (11. — VD}
The agreement between the two derivations is not surprising because the energy equation contains implicitly the laws of motion. Once the thermodynamic properties are eliminated, the energy equation should yield the same result as an equation derived from purely mechanical considerations. So far we have concentrated on what happens in an individual stage, and 456
Rotary Expanders and Compressors
[19.2]
we must now briefly consider the turbine as a whole. The chief aim in the design of a turbine is to utilise the available isentropic enthalpy drop with the least possible friction loss and in the smallest number of stages. It should be clear from equation (19.8) that the work done per stage increases with the blade speed U, but consideration of the centrifugal stresses in the rotating parts leads to a maximum permissible blade speed. With the blade speed fixed, an attempt to use a small number of stages (and hence a large enthalpy drop per stage) may mean that a smaller fraction of the enthalpy drop is converted into work and that a larger fraction remains as kinetic energy in the stream leaving the rotor blades. This should be clear from Fig. 19.4b. Furthermore, high fluid velocities lead to large friction losses. A useful criterion which indicates the effectiveness of energy abstraction in a stage is the diagram efficiency rid (sometimes called the utilisation factor). This is defined as ?id —
work calculated from velocity diagram energy available to rotor blades
The denominator is the kinetic energy at inlet to the rotor blades, MC?/2, plus the energy rii( VI — Vi)/2 made available by any expansion in the rotor. From equation (19.10) it is apparent that the difference between the denominator and the numerator is the rejected kinetic energy diCi/2. It must be emphasised that although a low diagram efficiency indicates the probability of large friction losses, (1 — rid) does not itself necessarily represent a loss. This is because the kinetic energy leaving one stage can be used in the following state. The total work done by an expansion in a multistage turbine can be found by summing the individual stage outputs. That is, per unit mass flow we have 114/121
=(h1 — h2) +
1 147231
=
C3)
— h3) + 2(C2 — C3)
114/„,„,11=0„ h,,+1)+1(c, c!+1) = (h1  h„ +1 )+2(c1 E Here subscripts 12, 23 etc. refer to the inlet and outlet of each complete stage. Evidently the interstage velocities are irrelevant except in so far as they affect the friction losses. Even the kinetic energy at outlet from the last stage, or leaving loss, can be utilised to some extent by fitting a diffuser (usually in the form of a volute) to the turbine exhaust. The effect of the diffuser is to increase the pressure drop across the turbine as illustrated in Fig. 19.5. In the figure the diffusion process is depicted as being isentropic, but in practice friction only permits part of the leaving loss to be recovered in this way. The various relations derived in the foregoing paragraphs will now be applied to particular stage designs. 457
[19.2]
Work Transfer Expansion without diffuser
Fig. 19.5 Effect of a diffuser at turbine exit
19.2.1 Impulse stage
In an impulse stage, where nominally all the enthalpy drop occurs in the stator blade row, it is usual to refer to these blades as nozzle blades or simply as nozzles. With no enthalpy drop across the rotor blades, there would be no change in relative velocity of the fluid as it passes through the rotor blade passages. In the absence of friction there would also be no change in pressure or specific volume across the rotor blades, and the continuity equation then requires the area at right angles to the direction of flow to be the same at inlet and outlet. With reference to Fig. 19.6, these areas are I,np cos II, at inlet and I2 np cos [ 2 at outlet', n is the number of blades in the row, p is the pitch, and I is the height of the blade. The simplest method of obtaining equal areas is to maintain the blade height constant and make fl2 equal to fl,. If this is done the velocity diagram for the impulse stage* appears as in Fig. 19.6. In practice, friction will occur in the passages, and if the blade passages have equal inlet and outlet areas there will be a small pressure and enthalpy drop resulting in a slight acceleration of the fluid relative to the blades.t In the following analysis friction in the rotor blade passages will be neglected. Expressions for the work done by the stage and the diagram efficiency can be found as follows. With reference to Fig. 19.6, for the case where V2 = V1 and P2 = PI , evidently AV,, = 2V, sin 31 = 2(C, sin a, — U) Hence 11411
= riAJAV,„= 2thU(C, sin a, — U)
(19.12)
With an impulse stage the only energy available to the rotor blades is mC?/2. The diagram efficiency is therefore qd =
2thU(C, sin a, — riiCP2:
U)
—4
U( U) sin a, — — C, C,
(19.13)
The ratio U/C, is called the blade speed ratio. In steam turbine practice it is customary to refer to a singlestage impulse turbine as a de Laval turbine, and a turbine consisting of a number of such stages in series as a Rateau turbine. t This effect of friction is not obvious, but all that can be done here is to refer the reader to the wellknown Fanno lines of fluid mechanics.
458
[19.2]
Rotary Expanders and Compressors
Fig. 19.6 Impulse stage
Other things being equal, equation (19.12) indicates that the work output increases with increase in nozzle outlet angle a,. An increase in al , however, implies a reduced axial velocity (C1 cos a,) and hence an increase in annulus area if the same mass flow is to be passed through the stage. The nozzle blade surface area over which the fluid flows is therefore increased, and this in turn implies an increase in nozzle friction loss. Considerations of this kind lead to the use of nozzle outlet angles of between 60 and 75 degrees. If a, is assumed to be fixed, equation (19.13) can be differentiated with respect to the blade speed ratio, and the result can be equated to zero to find the value of U/C1 which yields a maximum value of rid . Thus d(ld)
d(U/C,)
— 4 sin a t — 8 — C1
which equals zero when
U C,
sin a,
(19.14)
2
It will be seen by inspection of the velocity diagram that this optimum blade speed ratio corresponds to the case where the outlet velocity is axial, i.e. when the outlet kinetic energy is a minimum. Substituting (19.14) in (19.13) we have (rid)max =
(19.15)
sin 2 a,
Similarly, the power output at optimum blade speed ratio becomes I 14/ I = 2rhU2
(19.16)
The variation of rid with U/C1 is shown in Fig. 19.7. Fig. 19.7 Variation of ryd with blade speed ratio for an impulse stage
U/C,
[19.2]
Work Transfer
The maximum permissible blade speed that can be used depends upon the temperature of the working fluid, the strength of the heatresisting alloys available, and the life required of the turbine; blade speeds of about 250 m/s are common, but speeds as high as 370 m/s are sometimes used. When the rotational speed at which the turbine is required to operate is low, the blade speed is often chosen well below the permissible limit. It is then determined by the need to use a wellproportioned annulus; too high a blade speed at low rotational speed implies an annulus of large mean diameter and small height (for a given mass flow and therefore fixed annulus area). This might involve the use of unduly short blades, particularly at the highpressure end of the turbine where the specific volume of the fluid is small. Irrespective of how the blade speed is determined, once it is fixed equation (19.14) can be used to determine C1, and hence the stage enthalpy drop or number of stages for a given overall enthalpy drop. This procedure is illustrated by the following example. Example 19.1
A multistage gas turbine is to be designed with impulse stages, and is to operate with an inlet pressure and temperature of 6 bar and 900 K, and an outlet pressure of 1 bar. The isentropic efficiency of the turbine is likely to be 85 per cent. All the stages are to have a nozzle outlet angle of 75 degrees, equal inlet and outlet rotor blade angles, a mean blade speed of 250 m/s, and equal inlet and outlet gas velocities. Estimate the number of stages required. Assume cp = 1.15 kJ/kg K and y = 1.333.
The final temperature, assuming isentropic expansion, is
T'
900 (6/1)0.333/1.333 — 575 K
Hence the actual overall temperature drop is 0.85(900 — 575) = 276.3 K The energy equation for the flow through any nozzle row is 1(C? + C1) = c p(To — If the optimum blade speed ratio is to be used, C1 is given by C, =
2U 2 x 250 — — 517.6 m/s sin a, 0.966
Co is to be equal to C2, and with 12 = P I we have C2 = C1 cos a, = 517.6 x 0.259 = 134.1 m/s Hence To —
517.62 — 134.12 — 108.7 K 2 x 103 x 1.15
Since there is no expansion in the rotor blades, (T, — T1 ) will also be the stage 460
[19.2]
Rotary Expanders and Compressors
temperature drop, and therefore the number of stages becomes 276.3 — 2.54 108.7 Evidently three stages are required. The blade speed ratio used will be greater than the optimum, and the required expansion will be obtained with slightly lower gas velocities. 19.2.2 Velocitycompounded impulse stage
Before considering reaction designs it is necessary to mention an important modification to the simple impulse stage. Sometimes it is desirable to carry out a large enthalpy drop in one stage, in which case the fluid velocities are very high and, owing to the blade speed limitation, the U/C1 ratio is low and the work output is consequently a low fraction of the available enthalpy drop. The work output can be increased by velocity compounding, even though still using a low blade speed ratio. The method is illustrated in Fig. 19.8, which shows a tworow velocitycompounded stage. A velocitycompounded stage is known as a Curtis stage. The flow through the nozzles and the first moving row is similar to the flow. through a simple impulse stage, except that the ratio U/C, is much smaller. The fluid leaves the first row of rotor blades with a high velocity C2 at an angle a2 and enters a row of fixed guide blades having an inlet angle a2. No further expansion takes place and these blades merely turn the stream into the direction required for entry to a second row of rotor blades, i.e. C3 equals C2 . The guide blades are often made symmetrical, with the outlet angle a3 equal to the inlet angle a2, and the blade height will then be the same at inlet and outlet to give Fig. 19.8 Velocitycompounded impulse stage
Guide blades
C2
4 AV„,,
1
461
[19.2]
Work Transfer
equality of areas. The geometry of the velocity triangles then fixes the magnitude V3 and direction /33 of the relative velocity at inlet to the second moving row. If these blades are also symmetrical, 134 is equal to 163 and V4 is equal to V3 . The velocity diagrams are then determined, and the work done is W i = rhU(AV,,, + AV,,2 )
(19.17)
where subscripts 1 and 2 refer to the first and second rows of moving blades. With the foregoing assumptions about symmetrical moviniand guide blades, and unchanged relative velocities in the moving and guide blade passages, it is easy to show that for a given value of a, the diagram efficiency is a maximum when U C1
sin a 4
(19.18)
The leaving velocity C4 is then axial. It can also be shown that with this optimum value of U/C1 the diagram efficiency is the same as for the simple impulse stage, i.e. (fld)max = s1n 2 al but that the work done becomes I W I = 6rizU2 + 2rriU2 = 8thU2
(19.19)
Thus, for any given blade speed, a tworow stage can utilise four times the enthalpy drop of a simple impulse stage without any reduction in diagram efficiency. The velocities are of course high in the nozzles and first rotor row, and friction losses may be rather large. One important use of a velocitycompounded stage is mentioned in section 19.2.4.
Example 19.2
The nozzles of a tworow velocitycompounded stage have outlet angles of 68 degrees and utilise an isentropic enthalpy drop of 200 kJ per kg of steam. All moving and guide blades are symmetrical, and the mean blade speed is 150 m/s. Assuming an isentropic efficiency for the nozzles of 90 per cent, find all the blade angles and calculate the specific power output produced by the stage. The velocity at inlet to the stage can be neglected.
Since the inlet velocity may be assumed zero, the outlet velocity from the nozzles is given by
iCi
= thjAh'
C1 = (2 x 103 x 0.90 x 200)1/2 = 600 m/s The velocity diagram for the first row can now be drawn as in Fig. 19.9, from which /31 = /32 = 61.0 0, a2 = 48.7°, AV,„i = 812 m/s With C3 = C2 and a3 = oc2 , the velocity diagram for the second row can also 462
Rotary Expanders and Compressors
[19.2]
Fig. 19.9
132 =
150
a 812 First row
211 )1 Second row
be drawn, from which 133
= )34 = 25.2°,
V02 = 211 m/s
The specific power, i.e. the work output per kg/s of steam, is therefore WI = U(AV„, + AV,„2 )=
150(812 + 211) = 153.5 kW 1 03
Note that even with the comparatively low blade speed used in the foregoing example, the relative velocity at entry to the first row of rotor blades is very high. If it is too near the local velocity of sound in the fluid, losses will be incurred by the formation of shock waves in the blade passages. For this reason the tworow impulse stage is not suitable for use with high blade speeds—and for this reason also, threerow stages, which have an even lower optimum U/C1 ratio, are seldom used. It is worth noting that sonic velocity, given by — v2 (ap/Dv),}1/2 in general or (yRT)112 for a perfect gas (see section 18.1.1), is higher at the highpressure end of an expansion. It follows that higher fluid velocities relative to the blade are permissible in the first few stages of a multistage turbine and therefore that this might be where a tworow impulse stage can be used without incurring losses from shock waves. We shall see in section 19.2.4 that there are in fact good reasons for choosing this type of stage for the highpressure end of a turbine. 19.2.3 Reaction stage Before considering the special case of 50 per cent reaction, it is convenient to derive a general expression for the degree of reaction in terms of the main variables. This is most easily done when the velocities at inlet and outlet of the stage are equal and when the axial velocity remains constant throughout the stage. Both these conditions are commonly used in reaction designs because they enable the same blade shapes to be used in successive stages. In general the degree of reaction is A
hi — h2 110 — h2
Since the velocities are to be the same at inlet and outlet of the stage, the energy equation, per unit mass flow, reduces to IIj'I= ho — h2
463
[19.2]
Work Transfer
Therefore from equation (19.8), and using the nomenclature of Fig. 19.3, h0 — h2 = UAVW = UCa(tan /31 + tan $2 ) Also, applying the energy equation to the flow relative to the rotor blades, h i — h2 =
— 171)
= ICRsec2 /32 — sec2 /30 = ICa2 (tan2 N2 — tang /3k) It follows that (19.20)
A= °(tan,q2 — tan igi) 2U
Putting A= 0 in (19.20) yields the impulse stage with /3, =. /32, and putting A= 0.5 we have the reaction stage with (19.21)
— = tan /32 — tan Pi Ca From the geometry of the velocity triangles we also have the equation U = Ca(tan ai — tan /11 ) = Ca(tan 112 — tan a2 ) Comparing this with (19.21) we get al = $2 and a2 = /31
Also, from the initial assumptions that C2 = Co and Ca = Co cos ao = C2 cos C{2, it follows that = Evidently, for a 50 per cent reaction design the stator and rotor blades have the same shape, and the velocity diagram is symmetrical as shown in Fig. 19.10a. (Note that the rotor blades also act as nozzles in a reaction design. This is the reason why the first row of blades is referred to as a stator row rather than a nozzle row.) The optimum blade speed ratio for the reaction stage can be found as follows. From the symmetry of Fig. 19.10a, AK, = 2C, sin a, — U
Fig. 19.10 Velocity diagrams for a reaction stage /32 = al = /31
AVW (a)
464
(b)
[19.2]
Rotary Expanders and Compressors
and therefore, per unit mass flow, 114/I=U
= U(2C1 sin a, — U)
(19.22)
Since there is an enthalpy drop in the rotor blades, the energy available to the rotor blades per unit mass flow is C? 2 And since
— 2
V2 =
C1 this becomes
C? — 11/1 Furthermore, — 2C, U sin a,
= C? +
and therefore the energy available is 2(C1 — Uz + 2C1 U sin a l ) It follows that =
2U(2C1 sin a, — U) (C1  U 2 + 2C, U sin ai) U 2 U (2 sina, C1 z 1 — U ) + 2( U ) sin a l CI CI
(
(19.23)
Differentiating (19.23) with respect to U/C1 and equating to zero we have the optimum blade speed ratio given by U Cl
= sin a,
(19.24)
When the optimum blade speed ratio is used, the velocity diagram appears as in Fig. 19.10b. Substituting (19.24) in (19.22), the work done for a rate of flow Its becomes
w
= thu2
(19.25)
and substituting (19.24) in (19.23) yields 2 sin 2 a l (11d )max
1 + sin2 a,
(19.26)
Fig. 19.11 shows the variation of diagram efficiency with U/C1 for the three types of stage described. The significance of these curves will be discussed in the next subsection. 465
[19.2]
Work Transfer Fig. 19.11 Comparison of ryd for different types of stage
d
sin2cti
2 sin2 al/(1 + sin2 al ) —— Reaction Simple impulse
19.2.4 Multistage turbines and internal losses
The overall enthalpy drop across a turbine, particularly in steam turbine plant, is usually great enough to require the use of a large number of stages in series. As many as fifty stages may be required. Assuming that optimum blade speed ratios are used in each case, the power output per stage for the three types considered has been shown to be Tworow impulse:
13iii U 2
Simple impulse:
2thU 2
Reaction:
rriU 2
It might therefore be supposed that it is advantageous to use a succession of tworow impulse stages, since this would result in the least number of blade rows for a given overall enthalpy drop. However, it is also important to utilise the given isentropic enthalpy drop with the minimum loss, and when losses are taken into account the order of merit is not so obvious. The losses in a turbine may be divided conveniently into two groups. There will be external losses due to bearing friction and the power required to drive auxiliaries. These losses will be similar for all types of turbine and will not be considered here. The second and major group, the internal losses, may be dealt with under two heads as follows.
Blading friction losses The fluid friction in the nozzle and rotor blade passages results in the actual enthalpy drop being less than the isentropic enthalpy drop. These friction losses are proportional to the square of the average relative velocity through the blading, and the surface area. of blading swept by the fluid; they also depend on the nature of the flow. In general, for the same surface area and average relative velocity, the friction incurred by flow in a curved passage is less when the flow is accelerating, as in reaction blading, than it is when the velocity is substantially constant as in impulse blading. The reason for this is as follows. Most of the friction occurs in a boundary layer where there is a steep velocity gradient, and it is much less in a laminar boundary layer than in a turbulent
466
Rotary Expanders and Compressors
[19.2]
Fig. 19.12 Comparative velocity diagrams, using optimum U/Ci ratios and same
Reaction
values of U and al Singlerow impulse
Tworow impulse
boundary layer.* The boundary layer on a blade is normally turbulent over the concave surface, but on the convex surface it is initially laminar and only becomes turbulent at some distance from the leading edge. The effect of having a falling pressure gradient in the direction of flow is to cause the desirable laminar condition to prevail over a great part of the blade surface. A comparison of the velocity diagrams for the three types of stage (Fig. 19.12) shows that the average velocity through the stator and rotor blading is less for the reaction stage than for either of the others. This fact, coupled with the beneficial pressure gradient across the reaction rotor blades, is sufficient to outweigh the effect of the greater surface area incurred by the larger number of stages in a reaction design. The net result is that friction losses are least in a multistage reaction turbine. Leakage losses
Turbine rotor blading is carried either on a series of disks or on a drum, as shown in Figs 19.13a and b. Because clearance is needed between the moving and stationary parts, some fluid passes through the turbine without doing its full complement of work on the blading. Losses incurred in this way are called leakage losses and, since they involve a form of throttling, they contribute to the irreversible increase of entropy which occurs during the expansion. The leakage flow area between the stator diaphragm and the rotor shaft in Fig. 19.13a is obviously much less than that between the stator tips and the rotor drum in Fig. 19.13b. The disk construction is therefore always used for impulse stages, because the pressure difference across a stator row is comparatively large. On the other hand, the drum construction is usually preferred for reaction stages where the pressure drop across a stator row is not so great, because this type of construction does avoid the inevitable friction loss incurred by any disk spinning in a fluid. * The concept of a boundary layer is described in section 22.1.
467
[19.2]
Work Transfer Fig. 19.13 Disk and drum construction
Stator diaphragm
(a)
(b)
The leakage past the tips of the rotor blades will clearly be greater in a reaction stage, owing to the pressure drop which is absent in any impulse design. In general, therefore, the total leakage losses are rather greater in a reaction design than in an impulse design. This is particularly true at the highpressure end of a turbine where, owing to the high density of fluid, the annulus area required is small and the tip clearance is a relatively large proportion of the blade height. Summing up, we have seen that there are two main sources of loss to consider: (a) Blading friction losses, which are least for a reaction design (b) Leakage losses, which are least for an impulse design. A glance at the expansion on a p—v diagram (Fig. 19.14) will emphasise the fact that when the work is divided equally between the stages (i.e. when approximately equal stage pressure ratios are used), the pressure differences causing leakage are greatest at the highpressure end of a turbine. Furthermore, these pressure differences are particularly large in turbines of high pressure ratio (inlet/outlet). As a general rule, the leakage losses predominate over the friction losses at the highpressure end of high pressureratio turbines (e.g. most steam turbines), whereas .at the lowpressure end, or throughout low pressureratio turbines (e.g. gas turbines), the friction losses predominate. Taken together, the points made in the previous paragraph explain why reaction blading is invariably used for gas turbines, and why steam turbines normally have impulse stages at the highpressure end. The choice of stages in steam turbines varies widely with the range of steam conditions employed and the relative importance of capital cost and turbine efficiency. Generally speaking, turbine isentropic efficiency is the primary consideration because, apart from Fig. 19.14 Pressure differences
468
[19.2]
Rotary Expanders and Compressors
the saving in fuel, a lower steam consumption implies a smaller boiler and condenser which together account for the largest fraction of the capital cost of the whole plant. In high pressureratio steam turbines it is usual to use at least two turbines in series: a highpressure turbine with impulse stages followed by a lowpressure reaction turbine. The first impulse stage is commonly a tworow velocitycompounded design, because with the pressures and superheats used in modern plant it is important to achieve a large enthalpy drop in the first row of nozzles. Not only does this avoid exposing the turbine casing and rotor to the extreme steam conditions, but it also appreciably increases the volume flow before the steam reaches the first row of rotor blades. Without this increase in volume the blades might otherwise be too small for good efficiency. Even with an initial tworow impulse stage, it is sometimes necessary to use partial admission to avoid too small a blade height; the required flow area is obtained with a reasonable annulus height by blanking off sectors of the row of nozzles. It is of interest to note that the power output of steam turbines is commonly controlled by varying the inlet area in this way. After this brief discussion of the sources of loss in a turbine, it can now be explained why small turbines (i.e. turbines of low mass flow and small work output) have poorer efficiencies than large turbines. When the blades are very small, both the fluid friction loss and the leakage loss become a large proportion of the work done: the former because the boundary layer occupies a relatively large portion of the passage, and the latter because clearances between stationary and moving parts cannot be reduced proportionately. We opened this subsection with a comparison of the three types of stage on the basis of number of stages required, and went on to show that, when losses are considered, reaction designs are usually preferred in spite of the relatively large number of stages they involve. The position as regards number of stages is not quite as poor as our simple analysis has indicated, however, because the optimum blade speed ratio need not necessarily be used. Fig. 19.11 indicates that the curve of diagram efficiency for a reaction stage is fairly flat near the optimum U/C1 ratio, and it is possible to use a lower value of U/C1 (i.e. a larger enthalpy drop per stage) without an appreciable loss in efficiency. It must be remembered, however, that the diagram efficiency is only a rough guide to the probable susceptibility of a stage to friction losses, and the true optimum blade speed ratio for maximum isentropic efficiency (Ah/Ah isen) is not necessarily the nominal optimum value we have been deducing. The true optimum can only be found from a more complete analysis which makes use of friction data obtained from tests on rows of blades in 'cascade tunnels'.* Although this cannot be entered into here, we shall consider qualitatively the likely effect of using higher and lower values of the U/C1 ratio in a reaction stage. Fig. 19.15 shows the velocity diagrams for blade speed ratios less than, equal to and greater than the nominal optimum value. The blade speed U and the stator blade outlet angle a, have been assumed the same in each case. It will
* The type of analysis used for gas turbines can be found in Ref. 13.
469
(19.2;
Work Transfer Fig. 19.15 Reaction stage with low and high values of U/Ci (same U and ai U/C1 = sin a t
U/Cl < sin a i
U/C1 > sin al
be seen that the use of a low U/C1 ratio involves (a) Higher fluid velocities (b) Decrease in surface area swept by the fluid. The surface area is reduced both because of the smaller number of stages required, and because the higher axial velocity implies that a smaller annulus area is required to pass the given mass flow. Item (b) partially offsets (a) but, since the friction is proportional to the square of the fluid velocity, item (a) predominates and there is a decrease in isentropic efficiency of the stage. The use of a high U/C1 ratio involves (a) Lower fluid velocities (b) Increase in surface area, owing to the greater number of stages and lower axial velocity. In this case there may even be a slight rise in isentropic efficiency as the U/C1 ratio is increased from the nominal optimum value, and the eventual fall in efficiency is more gradual. Fig. 19.16 shows a typical curve of isentropic efficiency versus U/C1 ratio. It follows that a rather greater sacrifice in efficiency may be incurred by attempting to use a smaller number of stages (i.e. lower U/C1 ratio) than might be supposed from simple consideration of the variation in diagram efficiency. To close this discussion of losses, one form of loss peculiar to steam turbines must be mentioned. It was suggested in section 11.3 that it is undesirable for much of the expansion to occur in the wet region. It seems that liquid in the steam flow appears in three places, namely as a film running along the casing, as a fine mist suspended in the steam, and as a film on the surface of the stator blades (a liquid film does not form on the rotor blades because any moisture is flung off by centrifugal effects). The film on the stator blades detaches itself in relatively large droplets at velocities well below the mean velocity of the vapour, although sufficiently high to cause erosion damage at the leading edges
Fig. 19.16 Approx. 90%
Isentropic efficiency of reaction stage
I
U/Ca = sin al
(.1/C,
470
Rotary Expanders and Compressors
[19.2]
Fig. 19.17 Effect of a wet vapour
of the rotor blades, as indicated by the dashed arrows in Fig. 19.17. The turbine efficiency is also reduced. An annular collecting slot in the casing is often used to reduce erosion, but clearly this does not remove the moisture which does the damage. More recently, slots in the trailing edges of hollow stator blades through which the liquid film is sucked away have been tried on an experimental scale (see Ref. 20). Provided that the liquid from the trailing edge can be removed, the 0.88 lower limit for dryness fraction suggested in section 11.3 might not represent the absolute limit it has been thought to be. 19.2.5 Stage efficiency, overall efficiency, reheat factor and polytropic efficiency
Both the isentropic efficiency of a stage, and the overall isentropic efficiency of a turbine, can be defined in various ways depending on whether it is desired to take account of the whole, or a particular part, of the losses incurred. We have seen that the work done on the blading is less than can be expected from the isentropic enthalpy drop because of blading friction loss and leakage loss. Both these forms of loss increase the entropy of the expanding fluid and lead to a reduced actual enthalpy drop. Before the work done on the blading reaches the shaft, some of it will be dissipated in overcoming the disk friction loss when disk construction is employed. This loss also contributes to the increase in entropy and the reduction in enthalpy drop. All these internal losses affect the state of the fluid flowing through the stage or turbine. Efficiencies defined in terms of the internal work delivered to the shaft are called internal efficiencies. Finally, the work delivered by the shaft, or shaft work, is even smaller by reason of the external losses (e.g. bearing friction) which do not affect the state of the fluid; efficiencies based upon the shaft work may be called external efficiencies. We shall here be concerned solely with the internal efficiency of a stage or turbine. The internal work done during the expansion of unit mass flow from state 1 to state 2 is I W I = (h, — h2) +
— Ci)
In a multistage turbine the interstage velocities are equal, or nearly so, and for our purposes we can simply write I
= (h1 — h2 ) = Ah
The internal work is a maximum when the expansion between the given pressures is isentropic, i.e. I
= (hi — hZ) = 471
[19.2]
Work Transfer Fig. 19.18
h
The reheat factor
Defining the efficiency always as 147I/1 Wlmax, we arrive at the following definitions of the isentropic efficiency of a stage q, and overall isentropic efficiency of a turbine Ah Aho =and II. = Ohs; The following argument may be used to show that rh, is always greater than qs. For simplicity, we shall consider a fourstage turbine with each stage having the same efficiency rys. The expansion is shown on an h—s diagram in Fig. 19.18. The dashed curve indicates the average state of the fluid during the actual expansion; in steam turbine practice it is called the line of condition. The total work can be expressed either in terms of the overall isentropic enthalpy drop as
or in terms of the isentropic stage enthalpy drops as ;is(
+ Ales2 + Ah;3 + Ah54) = nS Eehs
Equating these expressions, we have no = no
ZAh; — r/sg2 Ak,
(19.27)
EAh;, called the cumulative enthalpy drop, is evidently greater than Ah'„, because the vertical height between any pair of constant pressure lines increases with increase of entropy. The ratio gP of the cumulative enthalpy drop to the isentropic enthalpy drop is called the reheat factor, and it is always greater than unity. The physical interpretation of this result is that the internal losses in any stage (except the last) are partially recoverable in subsequent stages owing to the 'reheating' effect of friction. It follows that it is more important to use highefficiency stages at the lowpressure end of a turbine than at the highpressure end. It should also be evident from the foregoing analysis that the difference between ;lc, and ry, increases as the overall pressure ratio of the turbine is increased. For this reason, turbines of high pressure ratio tend to be more efficient than those of low pressure ratio. 472
Rotary Expanders and Compressors
[19.2]
Example 19.3
Twelve successive stages of a reaction steam turbine have blades with effective inlet and outlet angles of 10° and 70° respectively. The mean diameter of the blade rows is 1.2 m and the speed of rotation is 3000 rev/ min. If the axial velocity is constant throughout the stages, estimate the specific enthalpy drop per stage. The steam inlet conditions are 10 bar and 250 °C, and the outlet pressure is 0.2 bar. Assuming a reheat factor of 1.04, estimate the stage efficiency (defined without reference to the kinetic energy term). Determine the approximate blade height at the outlet of the sixth stage, if the twelve stages are to develop 7500 kW. Assume the line of condition to be straight on the h—s diagram.
The mean blade speed is U = TEM —
it
x 1.2 x 3000
60
— 188.5 m/s
The velocity diagram can now be drawn to scale as in Fig. 19.19a, or the required velocities can be calculated as follows: sin 20 sin 60
hence Ili = 74.4 m/s
From symmetry, A V,„ = U + 2171 sin 10 = 214.3 m/s Therefore WI = UA V,, =
188.5 x 214.3 = 40.4 kJ/kg 10'
Since there is no change of kinetic energy between inlet and outlet, the specific enthalpy drop per stage must also be 40.4 kJ/kg. The actual enthalpy drop for the 12 stages is 12 x 40.4 = 48.4 kJ/kg. Using the h—s chart for steam, as illustrated in Fig. 19.19b, the initial enthalpy is found to be 2944 kJ/kg, and after isentropic expansion to 0.2 bar the enthalpy is 2281 kJ/kg, i.e. there is an isentropic drop of 663 kJ/kg. The overall efficiency
10 bar 2944
Fig. 19.19
/ 1.02 m3/kg
co 484.8/2 ap
80° 70° — 10°
.14
V1 = 74.4
(a)
(b)
473
[19.2]
Work Transfer
is therefore 484.8_0.731 — 0.731 g° = 663 If the reheat factor is 1.04, the stage efficiency must be ns
0.731 — 0.703 1.04
The assumed line of condition can be located on the h—s diagram since the actual final enthalpy is 2944 — 484.8 = 2459 kJ/kg. After the sixth stage, half of the actual enthalpy drop has occurred, i.e. the enthalpy is 2944 — 242.4 = 2702 kJ/kg. At this point the steam is still superheated and the pressure is 1.75 bar. By interpolation in the tables at this pressure and h = 2702 kJ/kg, the specific volume is found to be v = 1.02 m3 /kg. The power output required is 7500 kW (or kJ/s), so that the mass flow of steam must be 7500 — 15.47 kg/s 484.8 The axial velocity, from the velocity diagram, is Vli, = V1 cos 10 = 73.27 m/s and therefore the annulus area required is A—
thy V10
—
15.47 x 1.02 73.27
0.215 m2
If the mean diameter is d and the blade height 1, A = ncll and hence /=
0.215 = 0.0570 m = 5.70 cm it x 1.2
We have seen that the overall isentropic efficiency of a turbine increases as the overall pressure ratio (p,/p2 ) increases. When carrying out a series of cycle calculations to determine the optimum pressure ratio, as in section 12.2 for example, it is clearly misleading to assume a constant value for the overall turbine efficiency rh, over the range of pressure ratio. For such purposes the smallstage or polytropic efficiency n. is a more useful concept. It can be arrived at by taking the argument leading to equation (19.27) a step further. There we assumed the expansion to be carried out in several stages, each having the isentropic efficiency ?h. The polytropic efficiency is identical with ris when the number of stages is infinite, i.e. it is the isentropic efficiency of an infinitesimal step in the expansion which is assumed constant throughout the whole expansion. Thus it is defined by dh tho = — = constant dh' 474
(19.28)
Rotary Expanders and Compressors
[19.3]
where — dh and — dh' are respectively the actual and isentropic enthalpy drops over the pressure drop — dp. That the relation between goo and no is simple when the fluid is a perfect gas can be shown as follows. For an isentropic expansion we have T / p(Y  = constant, which on differentiation becomes dT' y — 1 dp T y p Combining this with (19.28), and remembering that for a perfect gas dh = cp dT and dh' = c p dT', we get dT y — 1 dp — 11. T Y P and on integration, rico being constant by definition,
72__ p2 '(''"' ( T,
(19.29)
p
Finally, from the definition of q„ we have T1 — T2 no =
T1 — T'2
1
T2/T1) —
)
n
1 — (P2/Pl) '(V— I)/Y 1 — (P2/P1
YY1)/7
(19.30)
This equation enables the variation of no with pressure ratio to be determined for any given value of ri oo . Note that if we write ncoey —
= (n — 1 )/n
equation (19.29) is the relation between p and T for a polytropic process undergone by a perfect gas. Thus the definition of go, implies the assumption that this nonisentropic process is polytropic, and hence the origin of the term `polytropic efficiency'. Note also that the concepts of polytropic efficiency and reheat factor are alternative ways of accounting for the 'reheating' effect of friction; the former has been found the more useful for gas turbine calculations and the latter for steam turbine calculations.
19.3 Axialflow compressors
We have already noted in the introduction to this chapter that, from the point of view of the exchange of energy between the fluid and the rotor, the compressor can be regarded as a reversed turbine. An axial compressor stage is therefore always thought of as a row of rotor blades followed by a row of stator blades, as in Fig. 19.20a. The velocity triangles are usually depicted as in Fig. 19.20b. The processes undergone by the fluid as it passes through the stage at the mean diameter of the annulus are as follows. The fluid approaches the rotor blades with absolute velocity Co at an angle oco . The relative velocity at inlet V0 is obtained by vectorial subtraction of the blade speed U. If Vo is found to be in the direction So, the rotor blade inlet 475
[19.3]
Work Transfer Fig. 19.20 An axialflow compressor stage
0 1 2 Diyek•gent passage
(b)
(a)
angle must also be approximately equal to 130 for the fluid to flow over the blade without interference. The rotor blade passage is made divergent and the flow is diffused, the fluid leaving with a reduced relative velocity V, at an angle fl„ Vectorial addition of the blade speed gives the absolute velocity C, at outlet from the rotor and its direction a l ; C, is larger than Co owing to the work done on the fluid by the rotor. The inlet angle of the stator blade is made approximately equal to a„ and the fluid is diffused in the stator passage. The velocity is reduced to C2 , and the stream leaves in the direction a2 . If the fluid is to leave the stage in a condition suitable for entry to another similar stage, C2 and a2 must be made equal to Co and ao . The work done in the stage, given by equation (19.4) but with the notation of Fig. 19.20, is W = ritU(C", — Cow ) It is evident from the velocity triangles that this is a positive quantity, in agreement with our sign convention for work. If the two velocity triangles are combined as in Fig. 19.21a it is convenient to write the equation as YV = ritUOCw
(19.31)
where AC,„ is (C,,„ — Cow). U
Fig. 19.21
U
Velocity diagrams for a compressor stage
(a) 476
(b)
Rotary Expanders and Compressors
[19.3]
In the stage just described, some increase of enthalpy, and therefore of pressure, is obtained in both rotor and stator rows. The concept of degree of reaction is also useful here, and for compressors it is defined as the ratio of the enthalpy rise in the rotor to the enthalpy rise in the stage, i.e. A=
h i ho h 2 — ho
The losses associated with fluid friction and blade tip clearance are found to be a minimum when the pressure rise is approximately equally divided between the rotor and the stator, and therefore a 50 per cent reaction design is normally used. By a similar analysis to that employed in section 19.2.3, it can be shown that with equal inlet and outlet velocities, and a constant axial velocity through the stage, 50 per cent reaction implies that the rotor and stator blades are identical in shape, i.e. = a l and )61 = ao The velocity diagram is then symmetrical as in Fig. 19.21b. This is the only type of stage design that will be considered here. When a value for the isentropic efficiency is available, the stage pressure ratio can be deduced as follows. Since axial compressors are used exclusively for compressing gases (normally air), the perfect gas relations may be introduced. With equal inlet and outlet velocities, the steadyflow energy equation applied to the whole stage is simply YV = thc p( T2 — To )
and hence c p(T2 — To ) = U AC ,,,
(19.32)
If the isentropic efficiency of the stage gs is defined as the ratio of the isentropic temperature rise ( T'2 — To ) to the actual temperature rise ( T2 — T0 ), we have (
— To ) = s(T2 — To )
T2 T=
(T2 — To) s To
Consequently, P2
Po
=
T2 WO— 1) (T2 — To ) — { 1 + Is To ( o
1() "
(19.33)
Substituting equation (19.32) in (19.33) we get finally p2 = (1 ± Po
U4C,,y(Y 1) ns
cp To
(19.34)
Equation (19.33) may also be used to obtain the overall pressure ratio of a multistage compressor if the overall isentropic efficiency is substituted for ris and the subscripts 0 and 2 refer to the inlet and outlet of the whole compressor. 477
[19.3]
Work Transfer Fig. 19.22
Polytropic efficiency
Arsa
Aro Al;, Ars2
A T:i
The overall temperature rise is the sum of the stage temperature rises, and if the same work is done in each of N stages it is simply NAT. By a similar argument to that used when deducing the reheat factor for turbines, in conjunction with Fig. 19.22, it is easy to show that the overall isentropic efficiency of a compressor is less than the stage efficiency, and that this difference increases as the pressure ratio of a compressor is increased by adding more stages. The concept of polytropic efficiency is useful here also; for a compression it is defined as dh' dh For a perfect gas, by repeating the argument used in deriving equation (19.29), we have the actual outlet temperature given by T2 (P2r ,),. "
=
Ti
Pi
We must now discuss briefly the factors which limit the pressure rise that can be obtained efficiently in one stage. Before doing so it is necessary to emphasise the essential difference between a compressor and a turbine, namely that the flow in the rotor and stator passages of a compressor is diffusing, whereas it is accelerating in a turbine (Fig. 19.23). It is always more difficult to arrange for an efficient deceleration of flow than for an efficient acceleration. In a diffusion process there is a natural tendency for the fluid to break away from the wall of the diverging passage, reverse its direction, and flow back in the direction of the falling pressure gradient. This will occur if the rate of divergence of the passage is too great, and the tendency is particularly marked when the passage is curved. The difference between the nature of the flow in a compressor and a turbine has a number of important consequences. First, the blade design is much more critical in a compressor. Whereas turbine blade profiles can be constructed quite satisfactorily of circular arcs and straight lines, compressor blades must be of aerodynamic shape, i.e. of aerofoil section. A less obvious
478
Rotary Expanders and Compressors
[19.3] Fig. 19.23 Comparison of turbine and compressor blades
Diffusing too rapidly
Turbine blades
Compressor blades
consequence is that the work done in a compressor stage cannot actually be estimated from equation (19.31) as it stands. The result of trying to induce a flow in a direction opposing the pressure gradient is that the axial velocity distribution across the annulus settles down after the first few stages into the peaky profile shown in Fig. 19.24. The effect of this is that the onedimensional treatment of this chapter is not nearly so adequate for compressors as it is for turbines, and the work done on unit mass of fluid depends to a greater extent than in a turbine on the radius at which the fluid is flowing through the annulus. In order to obtain an estimate of the average work done from onedimensional considerations it has been found necessary to multiply equation (19.31) by an empirical coefficient, called the work done factor. A typical value, except for the first few stages where it is nearer unity, is 0.86. The work done factor expresses a limitation upon the work that can be put into a stage. It should not be confused with the isentropic efficiency, which indicates how much of this actual work is usefully employed in raising the pressure and how much is dissipated by friction. The other most important factor limiting the work which can be put into a stage is the permissible rate of divergence of the blade passage. Fig. 19.23 shows that this will be a function of the angle through which the fluid is deflected, i.e. (#0 — /30 for the rotor and (a, — a2 ) for the stator. For the 50 per cent reaction design we are considering, equation (19.31) can be expressed as W = rhUCa(tan — tan /3t ) In this form it is clear that a limitation on (/30 — ) is reflected in a limitation on the work that can be put into a stage, and hence on the pressure ratio that can be obtained. With the blade speed limited by stressing considerations, and Outer wall
Fig. 19.24 Axial velocity distributions
Profile at entry Compressor annulus
Ca
After first few stages
I. Inner wall
479
Work Transfer
[19.4]
the axial velocity Ca limited by the need to keep the gas velocities relative to the blading below the sonic value and so avoid losses due to the formation of shock waves, any attempt to obtain a stage pressure ratio much in excess of 1.2 is accompanied by a serious drop in isentropic efficiency. We are now in a position to explain an important difference between the operating characteristics of positive displacement and nonpositive displacement compressors. Assuming the compressor to be running at a constant rotational speed, the delivery pressure of a positive displacement compressor is increased steadily by throttling the outlet and reducing the mass flow. This process can be continued until the mass flow is zero. With the nonpositive displacement rotary compressor there is only a restricted range of mass flow, at any given speed, within which the compressor can operate. If the mass flow is reduced beyond a certain point, the directions of the velocities relative to the blading are so widely different from the blade angles that the flow breaks down completely. The compressor is then said to surge. Even within the restricted range of operation the efficiency varies considerably, and it can only be maintained at a high value by varying the rotational speed and mass flow simultaneously in such a way that the velocity triangles maintain the same shape. 19.4 Radialflow turbines
The axialflow turbine is nearly always preferred to its radialflow counterpart. There are, however, a few special applications for which the radialflow turbine is sometimes used and it deserves a brief mention here. There are two possibilities to be considered: outward flow and inward flow. 19.4.1 Outwardflow turbines
When the pressure ratio is large, as with steam turbines, it is essential to use outward radial flow rather than inward radial flow. This is because the increase in volume as the expansion proceeds can be partly accommodated by the increase in flow area associated with increase in diameter. The Ljungstrom steam turbine is the only commercial outwardflow turbine. Briefly, it consists of concentric rows of blades, similar in shape to those of an axialflow reaction turbine, attached to the opposing faces of two rotor disks, as in Fig. 19.25. The axial crosssection of the rotor exhibits a flow path of a convergentdivergent character. At first the increase in flow area with diameter is rather greater than is required to accommodate the increase in volume flow, but later the reverse applies and the blades must be increased in length. The disks rotate in opposite directions, each shaft driving a generator. Thus each row of blades produces a share of the work output, and the work output per pair of rows is thereby larger than in an axialflow machine where half the rows are stationary. (There is no theoretical reason why the 'stator' rows should not be allowed to rotate in an axialflow turbine but the mechanical difficulties are rather greater.) The velocity triangles for any row are similar to those for an axialflow reaction stage, the main difference being that the blade velocity is 480
[19.4]
Rotary Expanders,'and Compressors
Fig. 19.25 Rotor fora Ljungstram turbine
greater at outlet than at inlet. The work done on any blade row is found from the rate of change of angular momentum in the usual way, using equation (19.3a). The Ljungstrom turbine has the advantage that it is very short in length, and this reduces the difficulties due •to differential expansion on starting. It can in fact be started from cold in a matter of minutes, and it is this feature which made it popular as a power plant for 'standby' or 'peakload' electrical generation—a requirement now frequently fulfilled by gas turbine sets. 19.4.2 Inwardflow turbines
When the turbine pressure ratio is comparatively small, as in gas turbine plant, it is possible to obtain the required increase in flow area with an inwardflow arrangement such as that shown in Fig. 19.26. This type of turbine is similar to the Francis hydraulic turbine. The gas enters the turbine via a volute and flows through a row of fixed nozzles situated around the periphery of the rotor. The highvelocity stream then flows inward between vanes attached to the side
Fig. 19.26 Inward radialflow turbine
481
[19.4]
Work Transfer Fig. 19.27 Velocity triangles for an inwardflow turbine
/71(////(4 v U C2
J2 V2
Section at mean radius of exit r2
of the rotor, and the passages are so shaped that the flow finally exhausts in an axial direction. Straight radial vanes are generally used, partly for ease of manufacture, but mainly because centrifugal forces would produce undesirable bending stresses in curved vanes. With radial vanes, the velocity of the gas relative to the rotor at entry must be in the radial direction if the gas is to enter the passages smoothly. The inlet velocity triangle therefore appears as in Fig. 19.27. For a given rotor tip speed U1 , nozzle angle a, and absolute velocity. C1 , the relative velocity will be V,. The whirl component Of the absolute velocity C1,, is equal to U1 . A crosssection through the 'eye' of the rotor, at the mean radius of the exit annulus, is also shown in Fig. 19.27. If the outlet velocity C2 is to be truly axial, the outlet velocity triangle shows that the relative velocity V2 must make an angle /32 with the axial direction. The rotor vanes must therefore be bent into this direction at the exit. Since there is no angular momentum at the outlet, equation (19.3a) becomes simply 1W1 = rhUi CI. And since C1„ is equal to U1 , this reduces to I
=
(19.35)
tUi
A simple expression for the pressure ratio required to produce this work can be deduced when (a) The fluid is a perfect gas (b) The velocities at inlet and outlet of the turbine are equal (c) A value is assumed for the overall isentropic efficiency of the turbine no The steadyflow energy equation applied to the whole turbine, with inlet conditions denoted by subscript 0, is then IWI=
To — T2 ) = riic pqj To — T2 )
where T2 is the temperature after an isentropic expansion to the final pressure. This equation can be written as I gi I = 482
rilCp
To {
( P 2 )(Y 1)/Y Po
Rotary Expanders and Compressors
[19.5]
Fig. 19.28 Twostage radial turbine
Equating this to (19.35) we have P2 = Po
U21)Y/(Y flo c, To
(19.36)
The permissible rotor tip speed depends upon the gas temperature; it is not likely to be much greater than 460 m/s when the gas inlet temperature is 1200 K. Using these values of U1 and To, an isentropic efficiency of 85 per cent, and typical values of c p and y for combustion gases of 1.15 kJ/kg K and 1.333, the pressure ratio becomes 1.333/0.333 1 4602 P2 = =' 103 x 1.15 x 0.85 x 1200 2.22 Po It is apparent that if inlet/outlet pressure ratios of much more than 2 are required, more than one stage is necessary. Unfortunately the ducting arrangements necessary for compounding radial turbines involve a rather tortuous flow path, as illustrated in Fig. 19.28. The additional friction loss associated with this does not arise in axialflow machines where the multiplication of stages presents no problem. For this reason the axialflow turbine is always preferred when the pressure ratio is such that more than one radial stage would be required. Even when only low pressureratio turbines of the two types are compared, the axial machine normally has the higher efficiency. A radial design only becomes competitive for small turbines of low mass flow because then, as was pointed out in section 19.2.4, the axialflow turbine becomes very inefficient.
19.5 Radialflow compressors
Although the inward radialflow turbine has so far been little used, its opposite number, the centrifugal compressor, has been used extensively both in small sizes as superchargers and in large sizes as compressors for gas turbine plant. Centrifugal compressors have lower isentropic efficiencies than axial compressors, but other compensating advantages have proved to be important for some applications. In appearance the centrifugal compressor is very similar to the radial turbine shown in Fig. 19.26. The rotor, or impeller, is driven in the opposite direction, so increasing the angular momentum of the fluid (normally air). There is also a pressure rise due to centrifugal effects. The fluid leaves the impeller with a 483
[1C.5]
Work Transfer Fig. 19.29 Velocity triangles for a centrifugal compressor
c
yo U0
Section at mean radius
of inlet r,
high velocity and flows through fixed diffuser passages in which the remaining pressure rise is obtained. The velocity triangles at the inlet and outlet of the impeller are shown in Fig. 19.29, for the normal case where the absolute inlet velocity is axial. Ideally the fluid should be ejected from the periphery of the impeller at such a velocity that the whirl component C bs, is equal to the impeller tip speed U1 . Owing to the inertia of the air trapped between the impeller vanes, C1,, is always less than U1 , the difference depending upon the number of vanes. The power input, from equation (19.3), is W = thU I C I„, Introducing the overall isentropic efficiency, and assuming equal inlet and outlet velocities for the compressor as a whole, the energy equation becomes ( 7 2 — To )
14/ = 110
Hence the pressure ratio is given by yl(' 1) (
P2 = ( Po
= 1 I
To
r2 
TO
= (1 4. ii o U ICI w vi(Y  1)
cp To
(19.37)
For an air compressor, the maximum permissible peripheral speed would be about 460 m/s because, although not subject to high temperatures, the impeller is normally made of light alloy. With the usual number of impeller vanes, C1,, is about 0.9 U1. Using these figures, together with ci, = 1.005 kJ/kg K, y = 1.4, T0 = 288 K and no = 0.8, the pressure ratio becomes 0.8 x 0.9 x 460 2 1.4/0.4 P2 = ( 1 + = 4.39 10' x 1.005 x 288 Po Impellers made from titanium permit higher tip speeds to be used, and pressure ratios of between 6 and 7 are then possible. As with radial turbines, the losses associated with compounding usually mean that the axialflow machine is preferred when more than one radial stage would be required. Centrifugal compressors producing pressure ratios much greater than 6 are therefore not 484
[19.5]
Rotary Expanders and Compressors
used when high efficiency and low weight are important requirements. When size and weight are unimportant, a high efficiency can be obtained from multistage radial compressors if intercoolers are fitted between the stages. This chapter provides the briefest possible introduction to the study of, rotary expanders and compressors. A more detailed introduction, but one which still employs an integrated approach to the subject of turbomachinery as a whole, is provided by Ref. 6. For more practical details the reader must turn to specialised books on each type of machine, such as Ref. 1 for gas turbines and Ref. 2 for axialflow turbines.
485
20 Direct Conversion
Often the production of mechanical work from a source of energy is merely an intermediate step in the production of electricity. It might be expected that if this intermediate step were eliminated the conversion of chemical or nuclear energy into electrical energy could be made with smaller and lighter equipment or perhaps with greater efficiency. Devices for direct conversion which are receiving most attention at present can be classified as follows: (1)
Thermionic converters
(2) (3)
Thermoelectric converters
(4)
Magnetohydrodynamic generators
(5)
Fuel cells
Photovoltaic generators
It ' is much too early to say which of these has the greatest potential for development or what are the applications for which each type is most suited. Broadly, the first three are likely to be suitable as sources of auxiliary power, the fourth for largescale power generation and the fifth for medium power outputs such as are required for road vehicles. The theories on which the design of these systems are based are likewise at an early stage of development. An understanding of them demands a knowledge of thermodynamics, electromagnetics, fluid mechanics and solidstate physics which is beyond the scope of this book.' All we shall attempt here is a brief description of the main features of each type of device, with an indication of the points at which thermodynamics plays a part in the theory. It is hoped that this introduction to the topic will stimulate interest and encourage the engineering student to pay greater attention to supporting science courses. Such is the pace of change that subjects of study which are now peripheral may well become central in his or her lifetime. The performance of four of the devices listed above is limited by thermodynamic considerations, as will be apparent later. Thermionic and thermoelectric converters are heat engines, even if unconventional forms, Ref. 24 is recommended as an attempt to present a coherent introduction to the subject of direct conversion in a single volume, as opposed to books, comprising collections of papers by specialists.
486
[20.1]
Direct Conversion in which electrons acting as the 'working fluid' can be said to be taken through a cycle. The maximum efficiency of such converters is therefore limited to the Carnot value (T1 — T2 )/ T1 , based on the temperatures of the source and sink between which they are operating. On the other hand, magnetohydrodynamic generators and fuel cells are essentially open systems, drawing on steady supplies of reactants at ambient conditions which ideally could leave as products at ambient conditions. The ambient conditions can in practice be taken to be the standard state (pe, To ), and the work output is therefore limited to the maximum work of reaction as explained in section 17.5 (and is also equal to the change in Gibbs function Agt as shown in section 7.9.3). Photovoltaic generators are the exception, because here electromagnetic radiation is converted directly to electricity without the intermediate step of a conversion to heat or a chemical reaction. It is worth pointing out that the laws of thermodynamics, and the energy equation Q W = AU, apply to more complex systems than those with which this book is primarily concerned. For example, they apply equally to systems involving electric and magnetic effects. The concept of work has to be widened, however, to embrace other than mere mechanical work, and more than two properties may have to be specified to fix the state of the system. Consider for example a system comprising an electrolytic cell, with an external circuit through which flows a quantity of electricity or charge SY impelled by a potential difference lc. If the external circuit consists of a simple resistance, the energy flow If SY will be dissipated as ohmic heating; this is analogous to the situation where mechanical work done by a system is dissipated by friction. But in principle it is possible to pass 82° through a perfect electric motor (i.e. one with no copper, iron and windage losses) which will do mechanical work equal to "K 8.2°. Any mode of energy transfer which can in principle be converted into mechanical work without loss can be included in the work term of the energy equation. Wthen becomes a symbol for a more generalised concept of thermodynamic work. If the operation of the electrolytic cell involves the liberation of gases, there may be work transfer due to a change in volume also. Thus for a reversible cell the energy equation could be written as dla = dU + p dV + d.t.' It would be found that in this case the internal energy U is a function of three properties, e.g. p, T and f". Before turning to books on direct conversion such as Ref. 24, the student will find it helpful to obtain this kind of background material from Ref. 8 of Part I.
20.1 Thermionic converters
Thermionic devices make use of the fact that when a metal plate is heated some of the free electrons are emitted from the surface. The distribution of energy among the free electrons, and the binding forces which exist at the surface, are such that only the faster moving electrons are emitted. The number emitted 487
[20.1]
Work Transfer Fig. 20.1
AGapIq2 41 0—, • 0—, T2 T1 ^/c • Load
A diode converter
°
(a)
a 0
Cathode
Anode (b)
increases when the general energy level is raised by increasing the temperature of the metal. The simplest form of thermionic device is the vacuum diode shown in Fig. 20.1, in which two opposing plates are maintained at different temperatures T1 and T2 . Since the current density (Aim') emitted from the surface is a function of temperature, there will be a net flow of electrons from the hightemperature electrode (cathode) to the lowtemperature electrode (anode), returning to the cathode via an external circuit. The retarding potential barrier which the electrons leaving the cathode must overcome is illustrated in Fig. 20.1b as + 42 + r — 01 ). 01 and 02 are the potential barriers for electrons within the material of the cathode and anode respectively; in solidstate physics (/) is referred to as the work function of the material, and its value varies greatly with the state of the metal surface. S is the retarding potential due to the cloud of electrons in the space between the electrodes, and is called the space charge barrier. 'V is the output voltage. Using electromagnetic theory to calculate the number of electrons per unit area which have sufficient energy to overcome the barrier, a relation may be deduced for the net current density /,from cathode and the temperatures T1 and T2 . The net power to anode in terms of 0, S, output is then /lc per unit area of emissive surface. It is possible to apply the steadyflow energy equation to an open system containing the cathode, with inlet and outlet planes across the conductor leading to the cathode and the space between the electrodes. The rate of heat flow 41 required to maintain unit area of cathode at T1 is equal to the algebraic sum of the energy of the electrons flowing across the gap and in the conducting lead, the thermal radiation from the plate, and the conduction of heat in the lead. An expression can thereby be obtained for d i , and hence finally for the efficiency of conversion "VA,. With presentday materials, reasonable efficiencies can be achieved only if the space charge barrier c5 is kept to a minimum. And with a vacuum diode this can be done only by maintaining a very small gap between the electrodes ( < 0.025 mm), which is difficult at the high temperatures required ( T1 > 1600 K). Another approach is to introduce an ionising agent into the gap to neutralise the space charge. It is expected that, with further development, power densities of up to 300 kW/m2 will be achieved with an efficiency of about 15 per cent. 488
[20.2] Fig. 20.2
Possible nuclear application
Direct Conversion
Nuclear fuel Coolant Anode Vacuum Cathode
If we view the system with its external leads and load as a whole, we can see that the electrons pass through a cycle of states while heat is supplied and rejected at the cathode and anode respectively. The maximum efficiency is therefore limited to (T1 — T2)/ Ti . As there are no highly stressed parts, very high temperatures can be used. But the inevitably high rate of irreversible heat transfer by radiation to the anode prohibits the use of large temperature differences and the efficiency obtainable cannot be very high. Thermionic converters are likely to be used either as a source of auxiliary power in space applications, where small size and low weight are important, or as 'topping' devices in conjunction with conventional power plant to make use of the hitherto unused temperature drop between available combustion temperatures and permissible boiler operating temperatures. In the latter case, the electrons would be the hightemperature working fluid in a binary cycle. Experiments are proceeding on these lines in the nuclear power field, by incorporating the converter into nuclear fuel elements as shown in Fig. 20.2. The tubular sheath around the fuel rod is the cathode, and the coolant, which is the heat source for the conventional power plant, flows along the outside of the tubular anode. 20.2 Thermoelectric converters
When the junctions of a loop of two wires of dissimilar metal are maintained at different temperatures, an electric current is produced in the circuit; this is the net result of the Peltier and Seebeck effects. The opencircuit potential difference produced, per unit temperature difference between the junctions, is called the Seebeck coefficient or thermoelectric power a (see Fig. 20.3a). With pairs of ordinary metals the value of a is only of the order of a few µV/K; this is adequate for use as thermocouples but much too low to be of interest for direct conversion. The development of semiconductors, however, which have thermoelectric powers in the region of mV/K, has now made thermoelectric converters a practical possibility. Useful power outputs can be obtained by connecting a large number of pairs in series. The Seebeck effect in metals is due to the diffusion of electrons along the temperature gradient from the hot to the cold junction. If this is greater in one metal than the other there will be a net flow of electrons around the circuit. In semiconductors the rate of diffusion is much greater, and furthermore the effect in each limb of the pair can be additive for the following reason. In some types 489
[20.2]
Work Transfer Fig. 20.3 Thermoelectric converter
Copper conductors
a = cl'K/dT
Load (b)
(a)
of semiconductor the charge carriers are electrons as in ordinary metals; these are referred to as ntype materials. But in others, ptype materials, the charge carriers are positive and can be regarded as 'holes' vacated by electrons. The current produced in a pair of n and ptype materials is in effect equal to the sum of the rates of diffusion of negative and positive charge carriers. A high thermoelectric power a is not the only criterion of importance in the choice of material for a thermoelectric converter. Fig. 20.3b shows a typical arrangement with hot junctions at T1 and cold junctions at T2 . It should be clear that a low thermal conductivity k is necessary to keep the heat flow by conduction across the elements to a minimum, and a low electrical resistivity p is required to reduce the internal ohmic (52 M) losses. Semiconductors are also good in these respects, because they are essentially materials of low thermal and electrical conductivity with the latter alone improved by the addition of impurities. a, k and p are temperature dependent and, when arriving at what is called the figure of merit M for a pair of n and ptype materials, it has been found convenient to include the temperature range which it is intended to employ. The figure of merit commonly used is M—
a2 (Ti + T2 ) kp 2
(20.1)
The thermoelectric converter is like the thermionic variety in that it is a heat engine with a flow of charge carriers as the working fluid. The maximum possible efficiency is therefore (T1 — T2 ) . This could be achieved only if the figure of merit were infinite, i.e. if there were no irreversibilities due to thermal conduction or ohmic loss between the hot and cold junctions. A thermodynamic analysis can be used to show that the practical ideal efficiency of conversion for a given value of M is given by T1 — T2 ( 1  F M )1 1 2 — 1
T1
(1 + M)112 + (T2/Ti )
(20.2)
A not very rigorous derivation of this equation can be found in Ref. 24. Since we are here dealing with essentially irreversible processes, the relatively new science of irreversible thermodynamics is necessary for a rigorous treatment (see the chapter by Hatsopoulos and Keenan in Ref. 25). With presentday materials, M is about unity and T1 and T2 might be about 600 °C and 200 °C 490
[20.3]
Direct Conversion
respectively. The corresponding ideal efficiency from equation (20.2) is thus about 10 per cent. Various losses not taken into account in deriving (20.2), such as those due to thermal contact resistance between the elements and the heat source and sink, result in actual efficiencies being nearer 5 per cent. Unless new semiconductor materials can be developed which are capable of operating at high temperatures, thermoelectric converters are likely to be used as `bottomers' rather than 'toppers' in binary cycles. They are especially suitable for waste heat recovery, perhaps using the exhaust gases of gas turbines as a source of heat, or the heat generated by a radioactive source as in the American Snap III generator designed for space applications. Thermoelectric generators using paraffin heating have been used in the USSR as a power source for radio receivers in rural areas. Thermoelectric devices can also be run in reverse; by supplying a current from an external source they act as refrigerators. The coefficient of performance is quite low, about 0.6, but the simplicity of the device makes it useful for some applications. 20.3 Photovoltaic generators
Electricity can be produced directly by exposing pn junctions to electromagnetic radiation. The conversion is due to quantum interactions between individual photons of radiation and the electronic structure of the cell material, which take place when the photon energy ( = he/A) exceeds a certain threshold value (h is Planck's constant, c the velocity of light and A the wavelength). The two most important types of energy source are (a) radioactive materials, which yield radiations of very short wavelength 10 12 m), and (b) sunlight whose wavelength ranges around 10 6 m. Photovoltaic cells designed to use sunlight have received the most attention. Photovoltaic effects in a solid were first observed in 1877 by Adams and Day who worked with selenium. The work led to the development of photographic exposure meters, but they convert no more than 0.8 per cent of the incident radiation into electrical energy. With the introduction of n and ptype semiconductors in the 1950s, conversion efficiencies of about 6 per cent were obtained and it was possible to think of using photovoltaic cells as a power source. Efficiencies of 15 per cent are now obtained with silicon pn junctions. Energy is produced by photons of radiation, creating free electrons and holes. To achieve a high efficiency it is necessary to produce electronhole pairs very close to the pn interface. Those far from the junction recombine without contributing to the cell's output. Furthermore, the internal resistance must be small. For these reasons cells consist of a very thin layer ( 10 ' mm thick) of ntype material on a wafer of ptype material ( 0.5 mm thick). Unwanted surface recombination of electronhole pairs is minimised by chemically etching the surface of the cell to leave it in a highly polished state, and reflection losses are reduced by using antireflection coatings. By considering the various losses inherent in the collecting and conversion processes, it can be shown by solidstate theory as in Ref. 24 that the theoretical maximum efficiency of a silicon cell is about 20 per cent, and with other possible materials such as gallium arsenide 491
[20.4]
Work Transfer
or cadmium telluride it is about 25 per cent. At present the actual efficiency of cells made of the theoretically better materials is lower than that of silicon cells. Because the source of energy is free, the factor limiting the use of photovoltaic cells as a power source is not so' much the conversion efficiency as the high cost of production. So far this has limited their use largely to space applications, such as communication satellites, where the cost of the cells is a small proportion of the total cost of the system. Now that costs are falling towards a more commercial level, the efficiency has become more important because it determines the number of solar cells (still costly) required for a given power, output. The power produced per unit surface area of cell might be increased by concentrating the radiation with lenses or reflectors. Unfortunately the conversion efficiency of present materials is reduced as the temperature of the cell increases, so that the net effect is small. Cooling the cell is no answer; the result would simply be a thermoelectric system. Another possibility is the construction of multilayer cells of different materials, matching their electronic characteristics to the energy spectra of the radiation in such a way that a greater proportion of the wavelength range can be used. Efficiencies of over 30 per cent might then be possible. 20.4 Magnetohydrodynamic generators Strictly speaking, it is doubtful whether the magnetohydrodynamic (MHD) generator can be called a direct conversion device; certainly there is no direct conversion of heat into electrical energy as in thermionic and thermoelectric converters. A gas at high pressure and temperature is still required as in conventional plant, but instead of using this via a turbine to drive metallic conductors through a magnetic field as in a conventional generator, the gas itself acts as a moving conductor (see Fig. 20.4). At very high temperatures a gas is ionised and the degree of ionisation can be enhanced by 'seeding' the gas with a small quantity of another substance such as caesium or potassium. Such ionised gases are referred to as plasmas. This conducting fluid is accelerated in a nozzle and passed at high velocity through a rectangular duct across which a magnetic field is applied at right angles to the direction of flow. An EMF is thereby generated in the fluid, which can be utilised by placing electrodes along the sides of the duct. The flow in the duct is governed by the momentum and energy equations, Fig. 20.4 Magnetohydrodynamic duct vishvis the conventional generator
Magnetic field
Velocity C
492
Electrode
Direct Conversion
[20.4]
which in this case must include electrical force and energy terms. A simple derivation of these equations for onedimensional frictionless adiabatic flow is given in Ref. 24, where they are shown to be: Momentum equation:
dp dC — + C— dx dx
= — via
C d — — (h + 4C 2) = — Pff v dx
Energy equation:
Here a' is the magnetic flux density, '•/7. the potential difference across the electrodes, b the distance between electrodes, and of the current density given by
where a is the electrical conductivity of the fluid. From these equations it is possible to deduce such useful performance criteria as the rate at which enthalpy is converted into electrical energy, the ratio of actual to isentropic enthalpy drop, and the power produced per unit volume of duct. It can be shown that the last of these, the power density, is proportional to aC2.42. The velocity of flow C is much higher than the speed at which a solid conductor can be rotated in a conventional generator, and this partially offsets the inherent disadvantage that a (even for a seeded gas at 3000 K) is only about 100 (() m) compared with 107 (SI m)' for solid copper. The overall efficiency will depend on the way in which the MHD duct is incorporated in the complete plant. Because sufficient ionisation can be achieved only at temperatures of 2500 °C or greater, the MHD generator is essentially a hightemperature device. Furthermore, the temperature must still be very high at outlet from the duct, so that to obtain a reasonable overall efficiency it must be used as a 'topper' in conjunction with a conventional cycle. A typical opencycle scheme is shown in Fig. 20.5; it would be possible to use a completely closed cycle if the combustion chamber was replaced by a nuclear reactor, but the temperatures required for adeqt, ate ionisation are well beyond those at present possible in reactors. Considering the opencycle plant shown, the MHD
Fig. 20.5 Possible MHD generator plant
Combustion chamber
IA Air preheater Steam boiler
Fuel
Exhaust
Air compressor Steam turbine Al
Condenser Feed pump
493
[20.5]
Work Transfer
portion to the left of the dashed line AA is an open system for which the efficiency might be expressed as net electrical work I — I compressor work I — Alio The net electrical output is the gross output less the power supplied to the electromagnetics producing the field M, and Aho is the enthalpy of combustion. (Those who have studied section 7.9.3 will appreciate that the denominator should strictly be the change in Gibbs function — Ago.) For the plant as a whole, the numerator becomes the net electrical output, including that from the steam cycle, minus the fOd pump work. The major sources of lo0 are fluid friction, heat loss through the walls of the duct, and internal elpc rical resistance. These losses can be made a small fraction of the output ori by using large ducts and high flow rates. It appears that the MHD generator p unlikely to be used for powers below the megawatt range. This is a case where little useful experimental work can be done on a small scale and thus development costs are very high. Several pilot plants have been built in the Soviet Union, and 1000 MW commercial units are now being designed using superconducting magnets and natural gas as the fuel.
20.5 Fuel cells
A fuel cell is a practical method of achieving a near reversible chemical reaction in which there is a conversion of chemical energy into electrical energy without even the intermediate step of conversion into random molecular energy (i.e. sensible internal energy). Thus, whereas the thermionic and thermoelectric forms of direct converter are essentially heat engines and subject to the Carnot limitation on efficiency, the fuel cell is not. Theoretically, the maximum work of a chemical reaction discussed in section 17.5 (and section 7.9.3) could be made available as electrical energy. The development of such a device, if capable of operating with hydrocarbon fuels or cheap derivatives such as carbon monoxide, would be a great step forward in the efficient utilisation of fuel resources. The fuel cell (Fig. 20.6) is an electrochemical device consisting basically of an electrolyte and two nonconsumable electrodes (often porous plates through which the fuel and oxidant diffuse). The electrodes play a catalytic role in facilitating the ionising reactions. In a simple type of hydrogenoxygen fuel cell the reactions might be written as Anode:
H2 > 2H + 2e 
Cathode:
2e + 2H + 102 > H2O
The opencircuit EMF can be related to a function of the enthalpy and entropy of the reactants and products (in fact to the change in the Gibbs function — Aga and the effect of temperature and pressure on the EMF can be determined by chemical thermodynamic analysis (see Ref. 26). The ideal 494
Direct Conversion
[20.5]
Fig. 20.6 Hydrogenoxygen fuel cell
Anode
— 0, H2O Electrolyte
maximum work for the reaction is not made available in practice because of internal losses. These include inhibiting effects due to absorption of molecules on the surface of the electrodes, uneven concentration of the electrolyte when current is flowing, changes in the conductivity of the electrolyte near the electrodes, and ohmic heating (52 a loss) due to the resistance of the electrolyte. Depending on the fuel and oxidant employed, the EMF produced is between 0.5 V and 1.5 V, and any required output voltage can be obtained by connecting cells in series as in the ordinary electric battery. Current densities of up to 400 Aim' have been achieved. Before about 1960, research in this field had been done by only a few individuals and mostly on the hydrogenoxygen cell. The picture has been transformed since then, and now a large number of laboratories and research teams are actively engaged in this development. The result has been not only a marked increase in performance—in power density and efficiency—but also such a bewildering variety of types of cell that classification is difficult. Attempts have been made to classify them on the basis of operating temperature or pressure, and type of electrolyte, fuel, oxidant or electrode, but no neat picture has emerged. There is little doubt that fuel cells will find a place for special military and space applications, but whether they will come into more general use depends on finding means of using cheap fuel and extending their working life.
495
Part IV Heat Transfer
Introduction
Heat is energy in transition under the motive force of a temperature difference, and the study of heat transfer deals with the rate at which such energy is transferred. When discussing thermodynamic processes, time is never considered a limiting factor, and ideal processes can be conceived during which heat is transferred by virtue of an infinitesimally small temperature difference. In actual processes some of the available temperature drop, which might be used for the production of work, must be sacrificed to ensure that the required quantity of heat is transferred in a reasonable time across a surface of reasonable size. Two types of problem are frequently of interest; the first, met in the design of boilers and heat exchangers, is concerned with the promotion of the required rate of heat transfer with the minimum possible surface area and temperature difference; the other is concerned with the prevention of heat transfer, i.e. with thermal insulation. Three modes of heat transfer may be distinguished, but the fact that a temperature difference is necessary is common to all. One mode of heat transfer is that of conduction, discussed in Chapter 21, in which energy is transferred on a molecular scale with no movement of macroscopic portions of matter relative to one another. Fourier's law forms the basis of all calculations of heat transfer by conduction. A second mode of heat transfer occurs when temperature differences exist between a fluid and a solid boundary. Here the redistribution of energy is partly due to conduction and partly due to transport of enthalpy by the motion of the fluid itself. Such motion can be due to a pump, as in the case of a fluid passing through the tubes of a heat exchanger, and this mode of heat transfer is called forced convection. On the other hand, the motion may be entirely due to density gradients in the fluid, caused by the temperature gradients—as when a stove heats the air in a room—and this is called free or natural convection. Convection is far more difficult to analyse than conduction because it is a combined problem of heat flow and fluid flow. The rate of heat transfer is influenced by all the fluid properties that can affect both heat and fluid flow, such as velocity, thermal conductivity, viscosity, density and thermal expansion. In finding an exact solution to any particular problem, it is essential to satisfy the equation of motion (Newton's Second Law), the equation of energy and the equation of continuity of flow, in addition to Fourier's law. The differential
499
Introduction
equations governing convection are complicated and exact solutions can be given in only a few simple cases. Some approximate analytical methods are given in Chapter 22, together with a description of an empirical approach using dimensional analysis. The third mode of heat transfer is radiation, and this mode does not depend upon the existence of an intervening medium. All matter at temperatures above absolute zero emits energy in the form of electromagnetic waves. Gases at low pressure emit waves of particular frequencies only, which are the natural frequencies of vibration of the gas molecules. In gases at high pressure, or liquids and solids, the molecular vibrations are more damped, and the emission of energy is over wide frequency bands. It is impossible here to go into the mechanism of radiation, and from the engineer's point of view it is usually sufficient to know the total quantities of energy emitted and absorbed by matter at various temperatures. The calculation of radiation heat transfer, discussed in Chapter 23, is based mainly on the StefanBoltzmann, Kirchhoff, and Lambert Laws. Often all three forms of heat transfer are involved simultaneously. It is then usual to calculate the rate of heat transfer by each mode separately, adding the separate effects to provide an estimate of the total rate of heat transfer. In this way a complex problem can be resolved, and the relative importance of the various modes of heat transfer can be assessed. A few simple examples are given in Chapter 24. The final result may not be exact, however, because a certain amount of interaction usually exists between the different modes. In the study of heat transfer it is usual to talk about the flow of heat, and of heat being contained in a material, as if heat were something tangible. Although in thermodynamics we permit outselves to talk loosely about the flow of heat, we are always careful to distinguish between the energy in transition (heat) and the energy residing in the material (internal energy). This distinction is necessary because the change in internal energy can be due to either work or heat crossing the boundary of a system. Normally this distinction is unnecessary in heat transfer because we are considering processes during which the change in internal energy is due solely to a flow of heat, and we are not concerned with transformations of one form of energy into another. In heat transfer problems involving flowing fluids, some of the kinetic energy is transformed into random molecular energy by viscous forces, and greater care is needed in the use of the term 'heat'. Nevertheless, for low velocities of flow the quantities of kinetic energy involved are usually small compared with the rate at which heat is transferred to or from the fluid, so that again no harm is done by the loose usage of the term. In highspeed flow, however, when the dissipation of kinetic energy into random molecular energy may be considerable, the thermodynamic view of the concept of heat must be retained.
500
21 Conduction
When temperature differences are present in any matter, heat flows from the hot to the cold regions until the temperatures are equalised. This occurs even when the movement of macroscopic portions of matter is prevented as in solids. The actual mechanism is complicated, but a brief explanation is as follows. In solids the conduction of heat is partly due to the impact of adjacent molecules vibrating about their mean positions, and partly due to internal radiation. When the solid is a metal, there are also large numbers of mobile electrons which can easily move through the matter, passing from one atom to another, and they contribute to the redistribution of energy in the metal. Indeed the contribution of the mobile electrons predominates in metals, thus explaining the relation which is found to exist between the thermal and electrical conductivity of such materials.' In liquids, single molecules may make large excursions with frequent collisions, even when largescale motion (convection) of the fluid is completely suppressed, and such movement assists the conduction of heat. Although the mobility of individual molecules is even greater in gases, the conductivity is appreciably lower than that of liquids and solids owing to the relatively long 'mean free path' in gases and hence the comparatively infrequent impact between the molecules. The detailed analysis of the mechanism of conduction is not discussed in this chapter. The first sections deal with Fourier's law of conduction, and its application to onedimensional steadyflow problems. The general equation for unsteady threedimensional heat flow is then derived. In the course of introducing relaxation methods, a twodimensional steadyflow problem is solved. Finally, onedimensional unsteady (transient) problems are considered with the aid of a numerical method. For a brief discussion of the status of Fourier's law, visàvis the laws of thermodynamics, the reader may turn to the end of section 6.7.
21.1 Fourier's law of heat conduction Fourier's law of conduction is based on the empirical observation of onedimensional steady heat flow through a solid. Onedimensional flow implies that * A fairly easy but comprehensive modern explanation is given by J. D. Eshelby in Ref. 35, p. 267. 501
[21.1 ]
Heat Transfer
Isothermal surfaces
Fig. 21.1 Onedimensional steady heat conduction through a planeparallel wall
k increases with T k constant
Temperature profile k decreases 'with T
the temperature is uniform over surfaces perpendicular to the direction x of heat conduction (Fig. 21.1a), and such surfaces are called isothermal surfaces. Steady flow implies that the temperature at any point does not vary with time. It follows from considerations of continuity that in onedimensional steady flow the rate of heat flow through successive surfaces is constant. Consider a plane layer of thickness dx, with one face maintained at a temperature T and the other at (T + dT). The rate of heat flow Q is found to be proportional to the area of flow A and to the temperature difference of dT across the layer, and inversely proportional to the thickness dx. This is Fourier's law, and it can be expressed by the equation = —kA(
dx
)
(21.1)
The constant of proportionality k is called the thermal conductivity of the material. The negative sign indicates that the heat flow is positive in the direction of temperature fall while treating k as a positive quantity. Steady onedimensional conduction demands that Q be constant through successive layers of the wall; if this were not so, the temperature in any layer dx with unequal inflow and outflow would vary with time. It follows that Q is not a function of x. Equation (21.1) therefore implies that if k is constant then (dT/dx) must also be constant, and thus the temperature profile is linear. Equation (21.1) can be integrated between limits x, and x2, to enable the heat flow to be expressed in terms of the surface temperatures T, and T2 by Q=
kA
T, — T, x12
(21.2)
When Q is in kW (or kJ/s), A in m 2, and the temperature gradient (dT/dx) in K/m, the units of k become kW/m K. Fig. 21.2 indicates that more convenient numbers are obtained if k is expressed in W/m K, and this smaller unit will often be used. 502
Conduction
[21.1 ] Fig. 21.2 Some values of thermal conductivity kl [Wlm K]
T/[K]
250
300
400
500
600
800
Aluminium Copper Steel (0.5% C)
208 393 57
202 386 55
209 377 52
222 372 48
234 367 45
277 357 38
Glass Building brick Concrete Asbestos Mercury, liquid Sodium, liquid Water (sat.) Steam (sat.) Steam (low p) Hydrogen Air Carbon dioxide
0.81.1 0.350.7 0.91.4 0.163 7.5 135 (sol.) 2.22 (ice)
0.0156 0.0223 0.0129
8.1 135 (sol.) 0.614
0.194
0.206
9.4 86 0.687
10.7 80 0.642
0.0184 0.0188 0.182 0.0262 0.0166
0.0275 0.0266 0.228 0.0337 0.0246
0.0432 0.0357 0.272 0.0404 0.0335
12.8 74
0.0463 0.315 0.0466 0.0431
13.7 6.3
0.0708 0.402 0.0577 0.0560
Fig. 21.2 gives some representative values of thermal conductivity for various materials, and it will be seen that the thermal conductivity varies with temperature. However, if the temperature difference ( T2  TO between the outside faces of the slab in Fig. 21.1a is small, a mean value of k may be chosen and assumed constant. When the temperature difference across the slab is large, due account must be taken of the variation of thermal conductivity with temperature. Typical temperature profiles for variable conductivities are shown in Fig. 21.1b. Unless otherwise stated, k will be assumed constant, but the method of calculating the heat transfer when k is a function of temperature is illustrated in the following example. Example 21.1
The conductivity of a planeparallel wall is not constant, but can be expressed with sufficient accuracy as a linear function of temperature, k = aT + b. Show that equation (21.2) can be used to calculate the rate of heat flow, if the arithmetic mean of the conductivities k1 and k2, at the temperatures 7.1 and T2 respectively, is substituted for k. Considering unit area of wall, and writing 4 = 01 A, equation (21.1) becomes q=
dx
\ d T) = (aT + b)(dx
For onedimensional steady flow 4 is independent of x and hence, by integration between x, and x2 (Fig. 21.1a), we have 4( )C2 xl) =
i• 51 (T1  Ti)  b(T2  T1)
or
q=  t c (T2 + Ti ) + 1)1 7'2 Ti 2
x12
503
[21.2]
Heat Transfer
But the mean conductivity is k2 + ki (aT2 + 6) + (aT, + b) = T,_ 1 (12 2 2 — (2
TO + b}
and hence equation (21.2) can be applied in the manner suggested. That there is some similarity between the flow of heat and that of electricity becomes apparent when equation (21.2) is compared with Ohm's law, .1 = The temperature difference, responsible for the heat conduction, plays an analogous part to the potential difference or voltage in the conduction of electricity. The current can then be compared to the heat flow per unit area 4, and the resistance a to the value of x12 /k (see Fig. 21.1a). The practical value of this electrical analogy will become clear in the next section.
r
21.2 Onedimensional steady conduction through a composite wall
A wall built up of three different materials is shown in Fig. 21.3. The surface temperatures of the wall are T1 and T4, and the temperatures of the interfaces are T2 and T3. For steady flow through the wall, the heat flow through successive slabs must be the same for reasons of continuity, and hence 4=
ki2
T2
T, x12
= k 23
T3 — T2 x23

T4 — T3 k34
(21.3)
x34
It follows from (21.3) that — ( T2 — T1 ) — (T3
T2) — (T4 — T3) = — (T4 — T1) X23 X34) = q. (x12 + + ki2 k23
Fig. 21.3 Heat conduction through a composite wall
504
(21.4)
[21.2]
Conduction
For the complete wall as a whole we can write
4 = U(T4 
(21.5)
where U is an overall heat transfer coefficient for the wall, defined by (21.5). It follows from (21.4) and (21.5) that 1 = x12 x23 x34
U
k12 k23
k34
or in general for any number of layers 1 U
v Ax
(21.6)
k
Here 1/U is the overall resistance to heat flow, and it is equal to the sum of the individual resistances x12 /k12 etc. in series. This might be expected from the electrical analogy illustrated in Fig. 21.3. The approach by way of equations (21.5) and (21.6) makes it possible to find the heat flow through a composite wall in terms of the surface temperatures, without calculating the interface temperatures. We have assumed, however, that there is no contact resistance between the layers; poor contact will lead to a temperature discontinuity at the interfaces and may result in a marked reduction in the rate of heat transfer because of the very low conductivity of air. Frequently it is required to calculate the heat flow through a wall separating two fluids of known temperature, when the surface temperatures of the wall are unknown. A typical temperature distribution in a fluid near a wall is shown in Fig. 21.4. Most of the temperature drop occurs very near the wall in a relatively stagnant boundary layer which adheres to the wall. Some distance from the wall the heat transfer is assisted by convection, and the temperature drop becomes more gradual until in practice it vanishes completely. The heat flow in the fluid boundary layer could theoretically be calculated from Fourier's law dT
4 = kf(
(21.7)
dx
where (dT/dx)w is the temperature gradient in the fluid immediately adjacent to the wall, and kf is the thermal conductivity of the fluid film at the wall. But
Fig. 21.4 Temperature profile in a fluid boundary layer
Solid
Fluid lc( Temperature profile
dT dx 505
[21.2]
Heat Transfer
(dT/dx),,, is a quantity which cannot easily be measured in practice, and it is more usual to express the heat flow from the wall to a fluid by an equation of the form (21.8)
4 = —0c.(7; — T)
where a, is a convection heat transfer coefficient or film coefficient, and Ts is the uniform fluid temperature so—te distance from the wall, referred to as the freestream temperature. To make the sign convention and general appearance of equation (21.8) consistent with that of Fourier's equation (21.7), we have introduced the negative sign in (21.8). The temperature change (Ts — 7) in the xdirection must always be written in the correct order to make 4 positive in the direction of temperature fall. Comparing (21.7) and (21.8), it is evidently possible to think of a stagnant fluid layer of thickness 5 = k,/a, which has the same resistance to heat flow as the actual fluid. The heat flow calculated from ( 21.8 ) includes the combined effects of conduction and convection in the fluid, and the two cannot be separated. The value of a, is difficult to calculate, and methods of evaluating it will be considered in Chapter 22. It is a function of numerous variables, such as the fluid viscosity and density and the fluid velocity relative to the wall; it is not a physical constant valid for a particular fluid under all conditions of convective heat transfer. For the time being it will merely be assumed that a, can be found. In addition to heat transfer by convection from the wall surface to its surroundings, the wall may also lose or gain heat by radiation. It is again convenient to express this heat transfer by the equation (21.9)
4 = —cer(Ts — T.)
where a, is a radiation heat transfer coefficient. In this case Ts is the temperature of the surface with which the wall is exchanging heat by radiation. a, is a function of several variables, such as the temperatures, emissivities and absorptivities of the radiating surfaces. The evaluation of a, is considered in Chapter 23, and here it is merely assumed that its value can be found. Let us now consider a composite wall which separates two fluids at temperatures Ts and Tb (Fig. 21.5). For simplicity, it is assumed that the surfaces with which the wall is exchanging heat by radiation have the same temperature as the intervening fluid. The total heat flow to the wall is given by 4 = — aca(Ti —
=—
) — ra
— 7'a )
ca + ara )( — 7;,)
Similarly the heat flow from the wall is 4=
c b + , b ) ( Tb —
T4 )
An overall heat transfer coefficient U can now be defined by 4 = —u(T,,— Ta )
506
[21.3]
Conduction
Fig. 21.5 Heat exchange between two fluids through a composite wall
It then follows from (21.3), (21.10), (21.11) and (21.12) that 1
1 U
OCca
x12 x23 x34
+ + + + ara k1 2 k23 k34 C(cb
1 arb
or in general 1
1
Ax E — U = 1ac + a r + k
(21.13)
Again considering the electrical analogy, the overall resistance to heat flow 1/U is equal to the sum of the individual resistances 1 /fa 1 x 12, /k12 etc. Here s ca + a  rao 1/aaa and 1 / ara are two resistances in parallel. 1
21.3 Radial steady conduction through the wall of a tube When the inner and outer surfaces of a long tube are each at a uniform temperature, heat flows radially through the tube wall. Owing to symmetry, any cylindrical surface concentric with the axis of the tube is an isothermal surface, and the direction of heat flow is normal to such a surface. To calculate the steady rate of conduction through the wall, it will be found convenient to consider unit length of tube rather than unit surface area. Continuity considerations indicate that the radial heat flow per unit length of the tube through successive layers must be constant if the flow is steady. Thus, since the area of successive layers increases with radius, the temperature gradient must decrease with radius. The temperature distribution will therefore appear as in Fig. 21.6a. Consider any elemental cylindrical tube of thickness dr. The area of flow per unit length of tube is 2itr, and the temperature gradient normal to this tube is 507
[21.3]
Heat Transfer
T,
Fig. 21.6 Radial flow through a thick tube and a composite tube
profile Cylindrical isothermal surfaces
dT
Temperature
ab
Fluid temp.
Lines of heat flow
Tb
(b)
(a)
(dT/dr). The heat flow is, according to Fourier's law, Q = —k2nr( dT ) dr Hence, since 0 is independent of r, we obtain by integration Qlnr2 =2nk(T2 —T1 ) r, and thus the heat flow per unit length of tube is 2Tck(T2 — —
(21.14)
ln(r2 /r,)
Considering a compound tube of n concentric layers, with fluid flowing through it and around it (Fig. 21.6b), it is possible to derive an expression for the overall heat transfer coefficient per unit length of tube U', analogous to equation (21.13) for the plane parallel wall. If T. and Tb are the temperatures of the fluids inside and outside the wall respectively, the rate of heat flow per unit length of tube is = — U'(Tb — 'T.) And using the same argument as in the previous section for deriving (21.13), it may be shown that U' is given by the expression 1
1
U'
2Tcro a.
+
/r,_ ,) E ln(ri27tki
1 27crn ab
(21.15)
Here as and ab are the respective total surface heat transfer coefficients, i.e. (a.. + ara) and (acb Ccb).* * It will be apparent after reading Chapter 23 that, unless the internal fluid is radiating, be zero.
508
must
Conduction
[21.4]
In the case of a single thin tube of thickness tx, for which the inner and outer radii are nearly equal, (21.15) reduces to 1
1
U'
2nraa
+
Ax
1
2itrk
27tra,
Hence the overall heat transfer coefficient per unit area of tube wall is 1 1 tx 1 — = a, U aa k which is identical with the 'expression for a flat plate. 21.4 The differential equation of threedimensional conduction
In the previous sections only onedimensional steady conduction has been considered, i.e. when the temperature only varies in the direction of heat flow and is uniform over any plane surface normal to the direction of flow. To calculate the heat flow through a conductor of any arbitrary shape, it will be shown that the problem reduces to one of finding the temperature distribution in the conductor, and once this is known the problem is effectively solved. A threedimensional equation will be derived which is applicable to both steady and unsteady conduction. In subsequent sections it will be applied first to steady and then to unsteady conduction. 'Steady' implies that the temperature at any point does not change with time. Consider a solid body having a plan view of the shape shown in Fig. 21.7. To get a picture of the temperature distribution, points of equal temperature can be joined to form isothermal surfaces (Fig. 21.7 shows these only in two dimensions). The picture of the temperature distribution is called the temperature field. Here we shall consider only materials which are homogeneous and isotropic: Isothermals
Fig. 21.7 Heat flow in the corner of a wall
Lines of heat flow
Surfaces at Ti
T varies from 7'i to T,
Surfaces at T,
on;
bA4 6,4 3 OA, °A
509
[21.4]
Heat Transfer
homogeneous because their density, specific heat and thermal conductivity are the same everywhere in the temperature field; isotropic because the thermal conductivity at any point is the same in all directions. For such materials the flow of heat is in the direction of maximum temperature gradient, i.e. at right angles to the isothermal surfaces. The lines of heat flow, which therefore cut the isothermal surfaces orthogonally, are also shown in Fig. 21.7. Consider any elemental area dA; the heat flow through this element during a time interval dt is given by Fourier's law as
aT on
dQ = —k dA(— )dt or the rate of heat flow is given by (21.16)
dQ = — k dA
where (aT/an) is the temperature gradient normal to dA. The following procedure may be adopted for calculating the total rate of heat flow through the conductor once the temperature distribution, or temperature field, is known. An isothermal surface is selected and divided into elemental areas SA 1 , SA 2 etc., and the normal gradient is found for each element. For steady flow, any isothermal surface may be chosen because the total rate of heat flow is the same for all such surfaces. Thus the rate of heat flow through dA, is
i = — k SA ,C T a where (aT/an), is the temperature gradient normal to the isothermal surface at SA,. The total rate of heat flow through the material can be found by integrating this equation over the whole area A of the isothermal surface, and hence = 
E
i=i
k
aT On ) i
(21.17)
The main problem lies in the prior determination of the temperature distribution in the field, and for this it is necessary to solve the differential equation that governs the conduction of heat. Consider any volume element (dx dy dz) of the conducting material in Cartesian coordinates with its edges parallel to the coordinates (Fig. 21.8). The basic idea in establishing the differential equation is to satisfy the continuity of flow in any region of the temperature fluid. To do this, we shall proceed in three stages to take account of the following energy terms during an infinitesimal time interval dt: (a) The net heat conduction dQ, into the volume element (b) The net energy (or 'internal heat') generation dQg within the volume element (c) The energy (or 'heat') stored dQ5 within the element as a result of a temperature rise d T.
510
Conduction
[21.4] Fig. 21.8 Derivation of the differential equation of conduction
z
x All three can be positive or negative, but energy conservation demands that dQs = dQ, + dQg Let us proceed by first thinking of the volume element (dx dy dz) in steady flow without internal heat generation. The heat inflow must be equal to the heat outflow, otherwise the temperature of the element will change with time. The rate of heat inflow through the lefthand face (dy dz), i.e. in the xdirection, is / dQx = —k(dy dz)— aT ax and the outflow from the righthand face (dy dz) is dOx + dx
k(dy dz)
T + (7 ) dx x
= — k(dy dz) (L T + ( 2T 2 dx ax Ox Similar equations can be written down for the y and zdirections. The net rate of heat inflow by conduction is thus dOc = (dOx — dOx+dx) + (dOy — 02 T
= k(dx dy dz)( For steady flow dOe = 0, hence az T 02 7, 02 T + Or 2 0 ox 2 +— 0y 2
0 2n
02 T
+ ax e
dOy+dy) (dOz dOz dz)
y
2
+
OZ 2
(21.18)
There may be energy generating sources inside the conducting material as the result, for example, of nuclear fission, or of a flow of electric current and the ohmic heating of the material. If 4g is the rate of the heat generated per unit volume, the total rate of heat generated in the volume element (dx dy dz) is dQg = 4g(dx dy dz) For steady flow with internal energy generation, dOs + dQg = 0 and hence 2 T 02 T 0 2 T k(dx dy dz)( 0x2 a + 3,2 + az 2 + 4g (dx dy dz) = 0 511
[21.4]
Heat Transfer Fig. 21.9
Some values of thermal diffusivity K
k I pcp 10 6 [m 2 Is]
T/[K]
250
300
400
500
600
800
Aluminium Copper Steel (0.5% C)
96.5 114
93.7 112 15
97.0 107
103 103
107 99.4
128 94.2
7.3 66
8.0 60
62.7 529 75.4 44.8
120 892 119.1 71.5
0.350.5 0.250.5 0.50.8
Glass Building brick Concrete Mercury liquid Sodium liquid Water (sat.) Steam (sat.) Steam (1 atm) H2 (1 atm) Air (1 atm) CO2 (1 atm)
or a
3.9 117 (sol.) 1.24 (ice)
4.3 114 (sol.) 0.147 382
113 15.7 7.60
155 22.2 11.0
2 T a2 v 1327
ax 2 ay 2
az 2
6.0 68 0.165
5.2 68 0.172 9.39 25.2 257 37.6 19.5
0.962 41.5 382 55.6 30.8
h
(21.19)
k =0
f(x, y, z), but for steady flow The term qg may be a function of position, i.e. it cannot be a function of time. Finally, in unsteady conduction, energy may be stored by (or drained from) the element. If the temperature of the element rises at a rate of (aT/ at), the rate of energy storage* amounts to 4g =
) a,
( ail= (heat capacity) (
= pcp(dx dy dz)(T aT )= ( PcP )k(dx dy di) (
aT
k
An energy balance then prescribes that dOs = dOc + dQg and hence h a2T a2T 2 1 (aT  ) =  II+1 ' kg K at ax 2 ay aazT
(21.20)
where K = k/ pc, is a dimensional group called the thermal diffusivity of the material; the dimensions are [length]2 /[time] and typical values are given in Fig. 21.9. We shall meet K again, not only in unsteady conduction but also in convection. * It is more correct to say that the net inflow of heat is equal to the increase of internal energy of the layer plus the work done against adjacent layers in expansion or contraction. If the pressure in the wall and outside is constant, the relevant specific heat capacity is c,, as used here.
512
Conduction
[21.4]
Equation (21.20) is normally referred to as the general conduction equation in Cartesian coordinates. It is not completely general, however, because it is restricted to isotropic and homogeneous materials as explained at the beginning of this section. Analytical solutions of equation (21.20) are possible only for relatively simple shapes of conductors. The following example of steady onedimensional heat flow with internal heat generation illustrates how the boundary conditions are applied to the solution of the differential equation. Example 21.2
An electric current of 34 000 A flows along a flat steel plate 1.25 cm thick and 10 cm wide. The temperature of one surface of the plate is 80 °C and that of the other is 95 °C. Find the temperature distribution across the plate, and the value and position of the maximum temperature. Also calculate the total amount of heat generated per metre length of plate and the flow of heat from each surface of the plate. The end effects along the short sides of the plate may be neglected, i.e. it may be assumed that no heat flows across these surfaces. It may also be assumed that the ohmic heating is generated uniformly across the section. The resistivity of the steel is p = 12 x 10 6 ohm cm, and its thermal conductivity is k = 54 W/m K. This is essentially a onedimensional problem with uniform heat generation
throughout the conductor. The governing differential equation is a2 t qg Dx 2 k
=0
The heat generated per unit volume given by i—
34000[A] 1.25 x 10[cm2 ]
48
is pi', where i is the current density
— 2720 A/cm 2
Hence
4g = pi' = 12 x 10 '[S1 cm] x 27202 [A 2 /cm 4 ] = 88 780 kW/m3 The differential equation therefore becomes
02T 8x2
82 T — 0 or — + 1 664 000[K/m 2 ] = 0 0.054[kW/m K] 8x2 88 78[kW/m3 ]
Integrating this equation, we obtain
T = —822 000[K1m 2 ]x 2 + Ax + B where A and B are constants to be determined from the boundary conditions. Choosing the origin of the xcoordinate at the 95 °C surface of the plate (Fig. 21.10), we can write for x 0 m 95°C = B and for x = 0.0125 m 80[°C] = —822000(0.0125)2 [K] + A(0.0125)[m] + B 513
[21.4]
Heat Transfer Fig. 21.10
61 95 °C
Hence the equation for the temperature variation with x becomes* T = —822 000[K/m2 ]x2 + 9075[K/m]x + 95[°C] The temperature distribution is therefore parabolic. Differentiating with respect to x and equating to zero, we find the position of the maximum temperature, i.e. dT
dx
= — 1 644 000 [K/m2 ]x + 9075 [K/rn] = 0
and x = 0.005 52 m = 0.552 cm The value of the maximum temperature is Lax = { — 822 000(0.005 52)2 + 9075(0.005 52) + 95 } [°C]
= 120 °C The heat flow from the plate across the 95 °C surface per metre length of bar is 0 / = kA (_ d T ) = {0.054 x 10 x 1 x 9075} [kW] d x .=.0 100 = 49.0 kW or kJ/s The heat flow from the plate across the 80 °C surface is 02 = —kA(dd: x=0.0125
I
=
—0.054 x
10 x 1 00
( 11 480)} [kW] = 62.0 kW or kJ/s
The sum of 01 and 02 which is equal to 111 kW must be equal to the total heat generated per unit length of plate by ohmic heating, i.e. (volume/metre length). Thus 4g
Qg = 88 780[kW/m3] x (1 x 0.0125 x 0.1)[m 3] = 111 kW * Here it is clear from the context that T is a Celsius temperature. The equation involves the addition of two increments of temperature change, correctly expressed in K, to the boundary condition given as a Celsius temperature.
514
Conduction
[21.4]
In the next section a numerical method of solution is introduced which can be applied to complicated shapes, and this method is applied to a twodimensional example. A good survey of mathematical methods used for the solution of conduction problems is given in Ref. 10. One other approach is via the electrical analogy. It is essentially an experimental approach, but it is easier to arrange for a flow of electricity than for a flow of heat, and to measure potential differences and currents rather than temperature differences and heat flows. The method makes use of the fact that the steady flow of electricity in a threedimensional conductor is governed by the equation a217. + a2„/„. + =o az2 ax2 ay2
a2
where ./t is the potential distribution if = f(x, y, z) throughout the conductor. This equation is clearly similar to equation (21.19). The current SA flowing through any elemental area SA , in a direction normal to SA , is 5~1 = —
m 71
l Can ame
)
i
where p is the resistivity of the material. Summing over the whole of an isopotential surface, the total current is given by =—
1 ( ail E7, —SA; );
= p
which is similar to equation (21.17). Thus potentials can be related to temperatures, and currents to heat flows. Thinking of the twodimensional corner of Fig. 21.7, a simple electrical analogue can be produced from a sheet of metallised paper of uniform and relatively high resistivity, cut to the appropriate shape, with copper strips placed along the boundaries. The low resistivity of the copper strips ensures that any voltages 'V, and 'ff2 applied to them will be uniform and analogous to the isothermal boundaries T1 and T2 . The potential at any point in the field can be measured by a simple probe and voltmeter, and the corresponding temperature found from 17. — T2 Yri  "r2 Once the temperature distribution has been obtained, the heat flow can be calculated using equation (21.17). More sophisticated analogues, capable of handling threedimensional problems, can be built using an electrolytic solution in a tank with conducting sides of appropriate shape. For a detailed treatment the reader can turn to Ref. 40. 515
[21.5]
Heat Transfer
21.5 Numerical solution of twodimensional steady conduction
It has been explained in the previous section that the solution of a multidimensional conduction problem consists essentially of finding the temperature distribution in the conducting material. This involves the solution of the differential equation (21.20), which may be extremely difficult except for a few simple shapes.* To solve this equation it is necessary to know the boundary conditions of the temperature field, e.g. the temperature distribution at the edge of the region considered, and the distribution of the internal heat sources if any. It can be proved (Ref. 9) that, for any given shape and boundary conditions, there is only the one solution to (21.20), i.e. there is only one possible temperature distribution. This section describes an approximate numerical method for solving twodimensional steady conduction problems. For such problems equation (21.20) reduces to a 2 T 02 7, 4 (21.21) + + g= 0 Dx2 ay2 k The object of the numerical method is to find values of the temperature in the conducting material at a limited number of points. It is most convenient to cover the region considered by a square net, and to find the temperature at the mesh points (Fig. 21.11). Whereas a general analytic solution gives the values of the temperature everywhere in the field as a function T = (1)(x, y), the numerical method merely finds numerical values of the temperature at the mesh T
Fig. 21.11 Relaxation method applied to twodimensional conduction
3
0
.41111111111\h,
T2 To
T4
2 a)
.11111111
111111111114x NIP NMI"—a 111111, IMEN0".
E
E,
* For analytical methods see Refs 3 and 19. 516
T1
Tempera ure profile in xdirection T known all round boundary
A
T