An Introduction to the Theory of the BOLTZMANN EQUATION Stewart Harris Stewart Harris (1937-2004) was a faculty member in the Department of Mechanical Engineering at Stony Brook University from 1966 until his death. He served as chairman of the department from 1978 to 1981 and was the dean of the College of Engineering from 1981 to 1992. Professor Harris held many visiting appointments in the U.S. and in Europe; these included positions at Princeton University, Imperial College (London), the Materials Directorate at Wright Patterson Air Force Base, and Columbia University. Dr. Harris received a B.S.E. from Case Institute of Technology (1959) and an M.S. (I960) and Ph.D. (1964) from Northwestern University, followed by postdoctoral work at the Courant Institute from 1964 to 1966. His research focused on the theory of transport processes at the microscopic level and on molecular beam epitaxy— the growth of atomically precise metal and semiconductor crystal structures. Dr. Harris,s research interests encom passed a number of distinct areas related to the study of reaction-diffusion systems; most recently these included the dispersal of genes and organisms, including early human populations. Copyright Copyright © 1971 by Holt, Rinehart and Winston, Inc. Copyright © renewed 1999 by Stewart Harris All rights reserved. Bibliographical Note This Dover edition, first published in 2004, is an unabridged republication of the work originally published by Holt, Rinehart and Winston, Inc., New York, in 1971. Library of Congress Cataloging-in-Publication Data Harris, Stewart. An introduction to the theory of the Boltzmann equation / Stewart Harris, p. cm. Originally published: New York : Holt, Rinehart, and Winston, 1971. Includes bibliographical references and index. ISBN 0-486-43831-7 (pbk.) 1. Transport theory. I. Title. QC175.2.H33 2004 530.13'8—dc22 2004050198 Manufactured in the United States of America Dover Publications, Inc., 31 East 2nd Street, Mineola, N.Y. 11501 43831702 To My Parents, Seymour and Goldie And My Wife, Helen Faith is a fine invention For gentlemen who see; But microscopes are prudent In an emergency I Emily Dickinson Preface The past twenty years have seen the steady maturation of the theory of the Boltzmann equation. In this period the Boltzmann equation has gone from a rather formidable mathematical curiosity with a limited but distinguished following, to a much used methodology having wide spread application. With the advent of modern high-speed flight through the rarefied regions of the outer atmosphere Boltzmann's equation has taken on a particular practical significance. However, it is no longer the exclusive property of the fluid physicist. One finds Boltzmann's equation, or Boltzmann-like equations, extensively used in such disparate fields as laser scattering, solid-state physics, nuclear transport, and even outside the conventional boundaries of physics and engineering in the fields of cellular proliferation and automobile traffic flow. It is especially significant that at a time when the method of time correlation functions seemed to be usurping much of the Boltzmann equation's earlier domain of transport theory such a veritable cornucopia of new uses for this equation should arise. Many of the advances which have been made in the theory of Boltz- mann's equation since the publishing, some thirty years ago, of Chapman and Cowling's now classic monograph are contained in the Handbuch article of Grad, who is himself responsible for much of this work. There exist two other outstanding expositions on the theory of the Boltzmann equation, the book by Carleman, and the Handbuch article by Wald mann一neither, unfortunately, are at present available in English. The above-mentioned sources are intended for a relatively sophisticated audience and for that reason are not basically suitable for use as a text in vii viii PREFACE an introductory graduate level course on the theory of Boltzmann's equa tion; in fact, strangely enough, there seems to be no book at the present time which satisfies this need: (Shorter, less complete accounts of the theory of Boltzmann's equation appear as an isolated chapter or two in books mainly devoted to equilibrium statistical mechanics.) This situation has been evident to me for some time, both as a graduate student and as a teacher of graduate students, and I have finally become emboldened enough to attempt to remedy what I consider to be a serious void in text book literature. In this book I have attempted to present in some detail the basic modern theory of Boltzmann's equation, and to include representative applications using both Boltzmann's equation and the model Boltzmann equations which are developed in the text. It is hoped that adherence to detail will enable this book to also serve as a reference source for research workers using the Boltzmann equation. The book is primarily intended for use in a graduate level course on the theory of the Boltzmann equation for physicists and engineers, and to this end I have tended to emphasize the physical aspects of the theory. The problems following each chapter are intended as learning examples, and these have quite often been used to extend and generalize the text material. This book has been the direct product of a course on the "Theory of the Boltzmann EquationM which I have taught at Stony Brook for the past few years. The point of view represents a distillation and, hopefully, a coherent synthesis of ideas presented to me from several sources. In particular, courses by Professors I. M. Krieger, M. B. Lewis, I. Prigogine, and G. E. Uhlenbeck, and the books by Chapman and Cowling, and by Carleman have been especially stimulating. A special debt must be acknowledged to Professor H. Grad who, through both the spoken and written word, has taught me much of what I know about the Boltzmann equation. Any successes which this book may enjoy are due in part to the above men; its failures must be my own. Stony Brook, New York Stewart Harris April 1971 Historical Introduction In the Foreword to Part 2 of his Lectures on Gas Theory, written in 1898, Boltzmann comments on the increasing attack which was being mounted by the so-called "school of energetics^ on all theories based on the atomic model of matter. It is unfortunate that it was only after Boltzmann^ untimely death, eight years later, that the atomic theory of matter became universally accepted by the scientific community, and the twentieth century began for physics and chemistry. The idea that matter is composed of atoms arose to conflict with the earth, water, air, and fire theory sometime in the fifth century b.c., and is usually credited to the Greek philosophers Leucippus and Democritus. Although discredited by Aristotle, the idea survived somehow until the first century a.d., when it was championed by the Roman poet-philoso pher Lucretius. In the Middle Ages the ideas of Aristotle became firmly established as Church dogma, and atomism was relegated to the list of heresies. For this, among other heresies, the ex-monk and philosopher Giordano Bruno fell victim to the flames of the Inquisition in 1600. Ideas cannot be killed as easily as men, however, and in. the seventeenth century, in a somewhat more tolerant atmosphere, the atomic theory was again taken up by Gassendi, and then by Boyle and Newton. Finally, in 1738, Daniel Bernoulli used the atomic model as the basis for postulating the first kinetic theory of gases. After another century of inactivity, Herapath, Waterson, Clausius, and finally the masters, Alaxwell and Boltzmann, formulated and developed a rigorous kinetic theory of gases. Herapath and Waterson found their ideas rejected by the scientific establishment of their country (they were English), although Waterson^ paper on the ix X HISTORICAL INTRODUCTION subject was finally published in 1891 by Lord Rayleigh, eight years after Waterson's death and forty-five years after he first submitted it to the Royal Society. Clausius, Maxwell, and Boltzmann, however, were important scientists in their countries, and although they were swimming against the scientific current of their day, they were able to publish their results. The work of Maxwell and Boltzmann, especially, can be con sidered as forming the basis of the modern kinetic theory of rarefied gases which we will consider in this book. Contents Preface vii Historical Introduction ix Chapter 1 Statistical Mechanical Preliminaries 1 11- The Microscopic Description 3 12- Relationship Between Microscopic and Macroscopic Descriptions 4 13- The Gibbs Ensemble 5 14- The Liouville Equation 6 1- 5 Proof of Lionville's Theorem 8 References 9 Problems 10 Chapter 2 Contraction of the Statistical Mechanical Description 13 2- 1 Reduced Distribution Functions 15 22- Reduction of the First BBGKY Equation to the Boltzmann Equation 19 23- The Moments of f 23 24- The Hydro dynamical Equations 26 References 27 Problems 28 xi xii CONTENTS Chapter 3 Description of Binary Collisions 31 31- General Formulation 33 32- An Alternate Representation of the Collision Integral 38 33- Hard Sphere Molecules Ifi 34- General Intermolecular Potentials 41 35- Power Law Potentials 站 3- 6 The Collision Cross Section 46 References 50 Problems 50 Chapter 4 Properties of the Collision Term 53 4- 1 Symmetry Properties of J(/) 55 42- The Summational Invariants 56 43- The Linearized Collision Term, L(g) 59 44- An Alternate Representation of L(g) 61 4- 5 The Eigentheory of L(g) 62 References 63 Problems 64 Chapter 5 The H Theorem and Irreversibility 67 5- 1 Spatially Homogeneous Systems 69 52- The H Theorem for a Nonuniform System 71 5- 3 Irreversibility and Boltzmann's Equation 74 References 77 Problems 77 Chapter 6 Normal Solutions of Boltzmann^ Equation 79 6- 1 The Fredholm Theorems 81 62- Hilbert's Uniqueness Theorem 82 63- The Chapman-Enskog Procedure 86 64- The First-Order Chapman-Enskog Solution 90 65- The Second-Order Chapman-Enskog Solution 90 66- Expressions for the Thermal Conductivity and Viscosity 93 67- Calculation of the Transport Coefficients 96 68- Validity of the Chapman-Enskog Results 99 References 100 Problems 101