Cartesian Tensors: An Introduction
By G. Temple
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Cartesian Tensors - G. Temple
INTRODUCTION
CARTESIAN TENSORS
AN INTRODUCTION
G. TEMPLE, F. R. S.
Sedleian Professor of Natural Philosophy in the University of Oxford
DOVER PUBLICATIONS, INC.
Mineola, New York
Bibliographical Note
This Dover edition, first published in 2004, is an unabridged republication of the work published by Methuen & Co., Ltd., London, and John Wiley & Sons, Inc., New York, 1960.
Library of Congress Cataloging-in-Publication Data
Temple, George Frederick James, 1901-
Cartesian tensors : an introduction / G. Temple.
p. cm.
Includes index.
Originally published: London : Methuen ; New York : Wiley, c1960, in series: Methuen’s monographs on physical subjects.
eISBN 13: 978-0-486-15454-1
1. Calculus of tensors. I. Title.
QA433.T4 2004
515'.63—dc22
2004049370
Manufactured in the United States of America
Dover Publications, Inc., 31 East 2nd Street, Mineola, N.Y 11501
Contents
Preface
IVECTORS, BASES AND ORTHOGONAL TRANSFORMATIONS
1.1 Introduction
1.2 The geometrical theory of vectors
1.3 Bases
1.4 The summation convention
1.5 The components of a vector
1.6 Transformations of base
1.7 Properties of the transformation matrix T
1.8 The orthogonal group
1.9 Examples
IITHE DEFINITION OF A TENSOR
2.1 Introduction
2.2 Geometrical examples of multilinear functions of direction
2.3 Examples of multilinear functions of direction in rigid dynamics
2.4 The stress tensor in continuum dynamics
2.5 Formal definition of a tensor
2.6 The angular velocity tensor
IIITHE ALGEBRA OF TENSORS
3.1 Introduction
3.2 Addition and scalar multiplication
3.3 Outer multiplication
3.4 Spherical means of tensors and contraction
3.5 Symmetry and antisymmetry
3.6 Antisymmetric tensors of rank 2
3.7 Products of vectors
3.8 The Chapman-Cowling notation
IVTHE CALCULUS OF TENSORS
4.1 Introduction
4.2 The differentiation of tensors
4.3 Derived tensors
4.4 The strain tensor
4.5 The rate of strain tensor
4.6 The momentum equations for a continuous medium
VTHE STRUCTURE OF TENSORS
5.1 Introduction
5.2 Projection operators
5.3 Definition of eigenvalues and eigenvectors
5.4 Existence of eigenvalues and eigenvectors
5.5 The secular equation
VIISOTROPIC TENSORS
6.1 Introduction
6.2 Definition of isotropic tensors
6.3 Isotropic tensors in two dimensions
6.4 Isotropic tensors of rank 2 in three dimensions
6.5 Isotropic tensors of rank 3 in three dimensions
6.6 Isotropic tensors of rank 4 in three dimensions
6.7 The stress-strain relations for an isotropic elastic medium
6.8 The constitutive equations for a viscous fluid
VIISPINORS
7.1 Introduction
7.2 Isotropic vectors
7.3 The isotropic parameter
7.4 Spinors
7.5 Spinors and vectors
7.6 The Clifford algebra
7.7 The inner automorphisms of the Clifford algebra
7.8 The spinor manifold
VIIITENSORS IN ORTHOGONAL CURVILINEAR COORDINATES
8.1 Introduction
8.2 Curvilinear orthogonal coordinates
8.3 Curvilinear components of tensors
8.4 Gradient, divergence and curl in orthogonal curvilinear coordinates
8.5 The strain tensor in orthogonal curvilinear coordinates
8.6 The three index symbols
8.7 The divergence of the stress tensor in curvilinear coordinates
INDEX
Preface
The purpose of this book is to provide an introduction to the theory of Cartesian tensors for first-year students pursuing an Honours course in Mathematics or Physics.
Tensor analysis was first forced upon the attention of theoretical physicists by the publication of Sir Arthur Eddington’s ‘Report on the Relativity Theory of Gravitation’.* In that report, however, tensor analysis was inevitably deployed on what was then the strange terrain of Riemannian geometry. In 1931 Sir Harold Jeffreys† had the happy idea of displaying tensor analysis on the familiar stage of three-dimensional Euclidean space. In this setting tensor analysis is freed from all irrelevant complications and is manifested in all its simplicity and power.
The excuse for writing another book on Cartesian tensors is that in the last thirty years the subject has been developed in a number of different directions which are of interest and importance to theoretical physicists.
The original definition of a tensor as a set of variables which are transformed cogrediently with the coordinate system with which they are associated has been replaced by the simpler and deeper definition now codified in the work of Bourbaki.‡ I have somewhat domesticated the native abstraction of this definition while preserving (I trust) its spirit and utility. Thus tensors are here defined as multilinear functions of direction, and this definition is found to simplify many theorems and to give a new unity to the subject.
The analysis of the structure of tensors (especially those of the second rank) in terms of spectral sets of projection operators is part of the very substance of quantum theory and therefore requires at least an elementary discussion.
The subject of isotropic tensors (whose components are the same in all orthogonal bases), always of fundamental importance in elasticity and hydrodynamics, has received new vigour from developments of the theory of group-representations and of abstract invariant theory.*
The development of spinor analysis, both as an algebraic discipline and as an integral part of quantum theory, appears to demand an introductory account, even in a work restricted to three-dimensional space.
I have therefore attempted to provide some initiation into these topics without quitting the confines of Euclidean space. I have, however, resisted the temptation to trespass too deeply into the territory of the hydrodynamicist and elastician, the quantum theorist and the relativist. For physicists the theory of tensors in a space-time manifold is so intimately associated with the special theory of relativity, and the theory of tensors in a Riemarmian manifold with the