DOCSLIB.ORG

A General Exact Solution of the Einstein–Dirac Equations with The

Total Page：16

File Type：pdf, Size：1020Kb

Download full-text PDF Read full-text
A General Exact Solution of the Einstein–Dirac Equations with The Journal of Experimental and Theoretical Physics, Vol. 98, No. 4, 2004, pp. 619–628. Translated from Zhurnal Éksperimental’noÏ i TeoreticheskoÏ Fiziki, Vol. 125, No. 4, 2004, pp. 707–716. Original Russian Text Copyright © 2004 by Zhelnorovich. GRAVITATION, ASTROPHYSICS A General Exact Solution of the Einstein–Dirac Equations with the Cosmological Constant in Homogeneous Space V. A. Zhelnorovich Institute of Mechanics, Moscow State University, Vorob’evy gory, Moscow, 119992 Russia e-mail: [email protected] Received May 29, 2003 Abstract—We have obtained a general exact solution of the system of Einstein–Dirac equations with the cos- mological constant in homogeneous Riemannian space of the first type according to the Bianchi classification. © 2004 MAIK “Nauka/Interperiodica”. 1. INTRODUCTION ant way. Using this gauge allows the number of unknown functions in the Einstein–Dirac equations to We face two problems when integrating the Ein- be reduced by six, while keeping the equations invari- stein–Dirac equations. ant under transformation of the observer’s coordinate The first, purely technical problem stems from the system. fact that the Einstein–Dirac equations constitute a com- plex system of nonlinear partial differential equations With the tetrad gauge used here, all of the equations of the second order for 24 unknown functions. Previ- can be written as equations of the first order only for ously, some of the particular exact solutions [1–6] to two invariants of the spinor field and the Ricci rotation the Einstein–Dirac equations in homogeneous space symbols of the proper vector bases determined by the have been obtained only for diagonal metrics of the spinor field. The tetrad gauge transforms the Dirac Riemannian event space. equations to equations for the Ricci rotation symbols and for the spinor field invariants, with the Ricci rota- The second problem is fundamental in nature and tion symbols in the Dirac equations being linear and ψ stems from the fact that the spinor field functions in without derivatives. Therefore, the Dirac equations in the Riemannian event space can be determined only in homogeneous Riemannian space close the system of certain nonholonomic orthonormal bases (tetrads) Einstein equations for the Ricci rotation symbols with- which that must be specified, or a tetrad gauge is said to out using additional equations. In this case, we can first be needed. A large number of such gauges are known, integrate the first-order equations for the Ricci rotation and different authors have suggested various gauges. symbols and the spinor field invariants and then inte- All of these are either noninvariant under transforma- grate the first-order equations for the tetrad (Lamé) tion of the variables of the observer’s coordinate system coefficients. or are written in the form of differential equations, which complicates the initial system of equations. These two factors—the reduction in the number of unknown functions by six and the possibility of inte- Physically, all gauges are equivalent, because the grating the second-order equations in two steps — con- Einstein–Dirac equations are invariant under the choice siderably simplify the Einstein–Dirac equations. As a of tetrads. Mathematically, however, using a bad gauge result, it becomes possible to obtain new exact solu- (i.e., additional equations that close the Einstein–Dirac tions of these equations. equations) can greatly complicate the equations, while using a good gauge can significantly simplify them. A general exact solution of the Einstein–Dirac equa- tions in homogeneous Riemannian space of the first In many respects, the problem of choosing a reason- type according to the Bianchi classification was able tetrad gauge stems from the fact that the solutions obtained in [7–9]. Recently, new papers in which the of the Einstein–Dirac equations have previously been authors discuss models described by the Einstein equa- obtained only for diagonal metrics. Since the basis vec- tions with the cosmological constant (including those tors of a holonomic coordinate system for such metrics with the spinor fields) have appeared. In this paper, we are orthogonal, the tetrads associated with the orthogo- obtain a general exact solution to the system of Ein- nal holonomic basis of the Riemannian space can be stein–Dirac equations with the cosmological constant chosen naturally. in homogeneous Riemannian space in connection with In this paper, we use a new tetrad gauge [7] that is increasing interest in studying the role of the cosmolog- algebraic and, at the same time, is formed in an invari- ical constant. 1063-7761/04/9804-0619 $26.00 © 2004 MAIK “Nauka/Interperiodica” 620 ZHELNOROVICH 2. THE SPINOR FIELDS complex conjugation; the invariant spinor of the second IN FOUR-DIMENSIONAL RIEMANNIAN SPACE rank β is given by the equations Let V be the four-dimensional Riemannian space γ T βγ β–1 β˙ T β with metric signature (+, +, +, –) referred to a coordi- ˙ a ==– a , . (4) nate system with variables xi and with a holonomic vec- tor basis Ji (i = 1, 2, 3, 4). We specify the metric tensor In general, the four-component spinor field ψ has of space V in basis Ji by the covariant components gij; two real invariants, ρ and η, that can be determined by the connectivity is defined by the Christoffel symbols using the equation Γs . In space V, we introduce a smooth field of ij + + 5 i ρexp()iη = ψ ψ + iψ γ ψ, (5) orthonormal bases (tetrads) ea(x ) (a = 1, 2, 3, 4) in the form where i a ea ==ha Ji, Ji hi ea, (1) γ 5 1 εabcdγ γ γ γ = ------ a b c d, a i 24 where hi and ha are the scale factors. Below, we denote the indices of the tensor components calculated εabcd are the components of the four-dimensional Levi– in basis Ji by the Latin letters i, j, k, …, and the indices Civita pseudotensor, ε1234 = –1. Using the spinor field ψ of the tensor components calculated in the orthonormal and the conjugate spinor field ψ+ in Riemannian space bases ea by the first Latin letters a, b, c, d, e, and f. V, we can determine the proper orthonormal vector The differential of the vectors of the orthonormal basis e˘ of the spinor field: i a basis ea(x ) is defined by the Ricci rotation symbols b i i i i i de = ∆ , e dx , which can be expressed in terms of the π ξ σ a ia b ˘e1 ====Ji, ˘e2 Ji, e˘ 3 Ji, e˘4 u Ji. scale factors The vector components πi, ξi, σi, and ui are specified by ∆ 1[ j ()∂ ∂ the relations [7, 10] iac, = --- hc ih ja – jhia 2 (2) j ()∂ ∂ b j s ()]∂ ∂ ρπi ==Im()ψT Eγ iψ , ρξi Re()ψT Eγ iψ , – ha ih jc – jhic + hi hahc jhsb – sh jb . (6) ρσi ψ+γ iγ 5ψ ρ i ψ+γ iψ ∂ ∂ ∂ i ==, u i , Here, i = / x . i Let us define the spinor field of the first rank, y(x ), in which the spin tensors γ i = hi γ a satisfy the equation in Riemannian space V specified by the contravariant a components ψA(xi) (A = 1, 2, 3, 4) in the orthonormal i j j i ij i γ γ γ γ bases ea(x ). The spinor indices are juggled by using the +2= g I. ψA ABψ ψ ψB formulas = e B and A = eAB . In these formulas, || || –1 || AB|| ˘ i E = eAB and E = e are the covariant and contra- Clearly, the scale factors ha that correspond to the variant components of the metric spinor, respectively, proper basis e˘ are defined by the matrix given by the equations a γ T γ –1 T 1 1 1 1 a ==–E aE , E –E. (3) π ξ σ u 2 2 2 2 γ i π ξ σ Here, T is the transposition symbol; a are the four- ˘ u ha = . (7) dimensional Dirac matrices, which, by definition, sat- π3 ξ3 σ3 u3 isfy the equation π4 ξ4 σ4 u4 γ γ γ γ a b +2b a = gabI, γ β || || If the spintensors a, E, and are specified as where I is a unit four-dimensional matrix; and gab = diag(1, 1, 1, –1) are the covariant components of the metric tensor in the orthonormal basis ea. 000i 00 01 Let us also define the conjugate spinor field by the γ = 00i 0 , γ = 00–0 1 , ψ+ ψ+ 1 2 covariant components = A using the relation 0 –00i 01–00 ψ+ = ψ˙ T β , in which the dot above the letter means –000i 10 00 JOURNAL OF EXPERIMENTAL AND THEORETICAL PHYSICS Vol. 98 No. 4 2004 A GENERAL EXACT SOLUTION OF THE EINSTEIN–DIRAC EQUATIONS 621 the covariant derivatives for the partial derivatives. 00i 0 00i 0 Eqs. (11) are identically valid by the definition of ρ, η, γ 000–i γ 000i and ∆˘ , . 3 = , 4 = , (8) sij –000i i 000 0 i 00 0 i 00 3. THE EINSTEIN–DIRAC EQUATIONS WITH THE COSMOLOGICAL CONSTANT 0100 0010 Let us consider the system of equations E ==–0001 , β 0001 , γ a∇ ψ ψ 0001– 1000 a +0,m = 0010 0100 1 R – ---Rg + λg = κT , ab 2 ab ab ab then the components of the spinor ψ calculated in the (13) ˘ ρ η 1[∇ψ+γ ψ proper basis ea are defined by the invariants and as T ab = --- a b follows [7, 10]: 4 ()γ∇ ψ+ ψψ+γ ∇ ψ∇()γψ+ ψ] – b a + b a – a b . 1 2 1 i ψ˘˘==0, ψ i ---ρexp ---η , 2 2 Here, ψ is the four-component spinor field in four- (9) dimensional Riemannian event space V specified in the 3 4 1 i λ κ ψ˘˘==0, ψ i ---ρexp –---η .
Load more

Recommended publications
  • Differentiable Manifolds
    Gerardo F. Torres del Castillo Differentiable Manifolds ATheoreticalPhysicsApproach Gerardo F. Torres del Castillo Instituto de Ciencias Universidad Autónoma de Puebla Ciudad Universitaria 72570 Puebla, Puebla, Mexico [email protected] ISBN 978-0-8176-8270-5 e-ISBN 978-0-8176-8271-2 DOI 10.1007/978-0-8176-8271-2 Springer New York Dordrecht Heidelberg London Library of Congress Control Number: 2011939950 Mathematics Subject Classification (2010): 22E70, 34C14, 53B20, 58A15, 70H05 © Springer Science+Business Media, LLC 2012 All rights reserved. This work may not be translated or copied in whole or in part without the written permission of the publisher (Springer Science+Business Media, LLC, 233 Spring Street, New York, NY 10013, USA), except for brief excerpts in connection with reviews or scholarly analysis. Use in connection with any form of information storage and retrieval, electronic adaptation, computer software, or by similar or dissimilar methodology now known or hereafter developed is forbidden. The use in this publication of trade names, trademarks, service marks, and similar terms, even if they are not identified as such, is not to be taken as an expression of opinion as to whether or not they are subject to proprietary rights. Printed on acid-free paper Springer is part of Springer Science+Business Media (www.birkhauser-science.com) Preface The aim of this book is to present in an elementary manner the basic notions related with differentiable manifolds and some of their applications, especially in physics. The book is aimed at advanced undergraduate and graduate students in physics and mathematics, assuming a working knowledge of calculus in several variables, linear algebra, and differential equations.
    [Show full text]
  • Tensor Calculus and Differential Geometry
    Course Notes Tensor Calculus and Differential Geometry 2WAH0 Luc Florack March 10, 2021 Cover illustration: papyrus fragment from Euclid’s Elements of Geometry, Book II [8]. Contents Preface iii Notation 1 1 Prerequisites from Linear Algebra 3 2 Tensor Calculus 7 2.1 Vector Spaces and Bases . .7 2.2 Dual Vector Spaces and Dual Bases . .8 2.3 The Kronecker Tensor . 10 2.4 Inner Products . 11 2.5 Reciprocal Bases . 14 2.6 Bases, Dual Bases, Reciprocal Bases: Mutual Relations . 16 2.7 Examples of Vectors and Covectors . 17 2.8 Tensors . 18 2.8.1 Tensors in all Generality . 18 2.8.2 Tensors Subject to Symmetries . 22 2.8.3 Symmetry and Antisymmetry Preserving Product Operators . 24 2.8.4 Vector Spaces with an Oriented Volume . 31 2.8.5 Tensors on an Inner Product Space . 34 2.8.6 Tensor Transformations . 36 2.8.6.1 “Absolute Tensors” . 37 CONTENTS i 2.8.6.2 “Relative Tensors” . 38 2.8.6.3 “Pseudo Tensors” . 41 2.8.7 Contractions . 43 2.9 The Hodge Star Operator . 43 3 Differential Geometry 47 3.1 Euclidean Space: Cartesian and Curvilinear Coordinates . 47 3.2 Differentiable Manifolds . 48 3.3 Tangent Vectors . 49 3.4 Tangent and Cotangent Bundle . 50 3.5 Exterior Derivative . 51 3.6 Affine Connection . 52 3.7 Lie Derivative . 55 3.8 Torsion . 55 3.9 Levi-Civita Connection . 56 3.10 Geodesics . 57 3.11 Curvature . 58 3.12 Push-Forward and Pull-Back . 59 3.13 Examples . 60 3.13.1 Polar Coordinates in the Euclidean Plane .
    [Show full text]
  • Lecture Note on Elementary Differential Geometry
    Lecture Note on Elementary Differential Geometry Ling-Wei Luo* Institute of Physics, Academia Sinica July 20, 2019 Abstract This is a note based on a course of elementary differential geometry as I gave the lectures in the NCTU-Yau Journal Club: Interplay of Physics and Geometry at Department of Electrophysics in National Chiao Tung University (NCTU) in Spring semester 2017. The contents of remarks, supplements and examples are highlighted in the red, green and blue frame boxes respectively. The supplements can be omitted at first reading. The basic knowledge of the differential forms can be found in the lecture notes given by Dr. Sheng-Hong Lai (NCTU) and Prof. Jen-Chi Lee (NCTU) on the website. The website address of Interplay of Physics and Geometry is http: //web.it.nctu.edu.tw/~string/journalclub.htm or http://web.it.nctu. edu.tw/~string/ipg/. Contents 1 Curve on E2 ......................................... 1 2 Curve in E3 .......................................... 6 3 Surface theory in E3 ..................................... 9 4 Cartan’s moving frame and exterior differentiation methods .............. 31 1 Curve on E2 We define n-dimensional Euclidean space En as a n-dimensional real space Rn equipped a dot product defined n-dimensional vector space. Tangent vector In 2-dimensional Euclidean space, an( E2 plane,) we parametrize a curve p(t) = x(t); y(t) by one parameter t with re- spect to a reference point o with a fixed Cartesian coordinate frame. The( velocity) vector at point p is given by p_ (t) = x_(t); y_(t) with the norm Figure 1: A curve. p p jp_ (t)j = p_ · p_ = x_ 2 +y _2 ; (1) *Electronic address: [email protected] 1 where x_ := dx/dt.
    [Show full text]
  • 2 a Patch of an Open Friedmann-Robertson-Walker Universe
    Total Mass of a Patch of a Matter-Dominated Friedmann-Robertson-Walker Universe by Sarah Geller B.S., Massachusetts Institute of Technology (2013) Submitted to the Department of Physics in partial fulfillment of the requirements for the degree of Masters of Science in Physics at the MASSACHUSETTS INSTITUTE OF TECHNOLOGY June 2017 Massachusetts Institute of Technology 2017. All rights reserved. j A I A A Signature redacted Author ... Department of Physics May 31, 2017 Signature redacted C ertified by ....... ...................... Alan H. Guth V F Weisskopf Professor of Physics and MacVicar Faculty Fellow Thesis Supervisor Accepted by ..... Signature redacted Nergis Mavalvala MASSACHUETT INSTITUTE Associate Department Head of Physics OF TECHNOLOGY (0W JUN 2 7 2017 r LIBRARIES 2 Total Mass of a Patch of a Matter-Dominated Friedmann-Robertson-Walker Universe by Sarah Geller Submitted to the Department of Physics on May 31, 2017, in partial fulfillment of the requirements for the degree of Masters of Science in Physics Abstract In this thesis, I have addressed the question of how to calculate the total relativistic mass for a patch of a spherically-symmetric matter-dominated spacetime of nega- tive curvature. This calculation provides the open-universe analogue to a similar calculation first proposed by Zel'dovich in 1962. I consider a finite, spherically- symmetric (SO(3)) spatial region of a Friedmann-Robertson-Walker (FRW) universe surrounded with a vacuum described by the Schwarzschild metric. Provided that the patch of FRW spacetime is glued along its boundary to a Schwarzschild spacetime in a sufficiently smooth manner, the result is a spatial region of FRW which transitions smoothly to an asymptotically flat exterior region such that spherical symmetry is preserved throughout.
    [Show full text]
  • Catalogue of Spacetimes
    Catalogue of Spacetimes e2 e1 x2 = 2 x = 2 q ∂x2 1 x2 = 1 ∂x1 x1 = 1 x1 = 0 x2 = 0 M Authors: Thomas Müller Visualisierungsinstitut der Universität Stuttgart (VISUS) Allmandring 19, 70569 Stuttgart, Germany [email protected] Frank Grave formerly, Universität Stuttgart, Institut für Theoretische Physik 1 (ITP1) Pfaffenwaldring 57 //IV, 70550 Stuttgart, Germany [email protected] URL: http://go.visus.uni-stuttgart.de/CoS Date: 21. Mai 2014 Co-authors Andreas Lemmer, formerly, Institut für Theoretische Physik 1 (ITP1), Universität Stuttgart Alcubierre Warp Sebastian Boblest, Institut für Theoretische Physik 1 (ITP1), Universität Stuttgart deSitter, Friedmann-Robertson-Walker Felix Beslmeisl, Institut für Theoretische Physik 1 (ITP1), Universität Stuttgart Petrov-Type D Heiko Munz, Institut für Theoretische Physik 1 (ITP1), Universität Stuttgart Bessel and plane wave Andreas Wünsch, Institut für Theoretische Physik 1 (ITP1), Universität Stuttgart Majumdar-Papapetrou, extreme Reissner-Nordstrøm dihole, energy momentum tensor Many thanks to all that have reported bug fixes or added metric descriptions. Contents 1 Introduction and Notation1 1.1 Notation...............................................1 1.2 General remarks...........................................1 1.3 Basic objects of a metric......................................2 1.4 Natural local tetrad and initial conditions for geodesics....................3 1.4.1 Orthonormality condition.................................3 1.4.2 Tetrad transformations...................................4
    [Show full text]
  • Cambridge University Press 978-1-108-47122-0 — Mathematics for Physicists Alexander Altland , Jan Von Delft Index More Information
    Cambridge University Press 978-1-108-47122-0 — Mathematics for Physicists Alexander Altland , Jan von Delft Index More Information Index δ-function basis Gaussian representation, 273 definition, 30 qualitative discussion, 272 local, 418 ǫ–δ criterion, 208 orientation, 96 ∃, there exists, 7 orthonormal, 43, 50 ∀, for all,7 bilinear form, 156 ´ , symbol, 217 bin, 218 n-tuple, 34 bit, 8 Abel, Nils Henrik, 8 calculus, 205 absolute value, 17 canonical, 32 action principle, 334 Cantor, Georg Ferdinand Ludwig Philipp, 13 affine space Cartesian product, 13 definition, 26 Cauchy theorem, 344 Euclidean, 26 Cauchy, Augustin-Louis, 339 point, 25 Cauchy–Schwarz inequality, 40 chaos algebra definition, 325 definition, 71 fractal dimension, 325 Grassmann, 161 Lyapunov exponent, 325 alternating form strange attractor, 325 exterior product, 161 characteristic polynomial, 101 maximal degree, 158 closure of degree p, 157 group operation, 7 one-form, 150 interval, 17 pullback, 163 set, 17 top-form, 158 co- and contravariant transformation, 152 volume form, 165 commutator, 183 wedge product, 161 completeness Ampère’s law, 457 relation, 134 analysis, 205 vectors, 30 angle complex conjugate, 15 azimuthal, 423 complex function between vectors, 40 analytic, 338 polar, 423 branch cut, 356 angular momentum, 152 branch point, 356 ansatz, 42 contour integral, 342 anti-derivative, 220 definition, 338 antisymmetric symbol, 12 extended singularity, 346 area element holomorphic, 338 definition, 245 meromorphic, 347 polar coordinates, 246 pole, 347 asymptotic expansion, 267 singularity,
    [Show full text]
  • Arxiv:0907.0934V2
    ON THE POINCARE GAUGE THEORY OF GRAVITATION S. A. Ali1, C. Cafaro2, S. Capozziello3, Ch. Corda4 1Department of Physics, State University of New York at Albany, 1400 Washington Avenue, Albany, NY 12222, USA 2Dipartimento di Fisica, Universit`adi Camerino, I-62032 Camerino, Italy 3Dipartimento di Scienze Fisiche, Universit`adi Napoli “Federico II” and INFN Sez. di Napoli, Compl. Univ. di Monte S. Angelo, Edificio G, Via Cinthia, I-80126, Napoli, Italy 4Associazione Scientifica Galileo Galilei,Via Pier Cironi 16, I-59100 Prato, Italy We present a compact, self-contained review of the conventional gauge theoretical approach to gravitation based on the local Poincar´egroup of symmetry transformations. The covariant field equations, Bianchi identities and conservation laws for angular momentum and energy-momentum are obtained. PACS numbers: Gravity (04.); Gauge Symmetry (11.10.-z); Riemann-Cartan Geometry (02.40.-k). I. INTRODUCTION From the viewpoint of Classical physics, our spacetime is a four-dimensional differential manifold. In special relativity, this manifold is Minkwoskian spacetime M4. In general relativity, the underlying spacetime is curved so as to describe the effect of gravitation. Utiyama (1956) [1] was the first to propose that general relativity can be seen as a gauge theory based on the local Lorentz group SO(3, 1) in much the same manner Yang-Mills gauge theory (1954) [2] was developed on the basis of the internal isospin gauge group SU(2). In this formulation, the Riemannian connection is obtained as the gravitational counterpart of the Yang-Mills gauge fields. While SU(2) in the Yang-Mills theory is an internal symmetry group, the Lorentz symmetry represents the local nature of spacetime rather than internal degrees of freedom.
    [Show full text]
  • Spacetime Is a Manifold That Is Continuous and Differentiable. This
    I. GENERAL RELATIVITY { A SUMMARY A. Pseudo-Riemannian manifolds Spacetime is a manifold that is continuous and differentiable. This means that we can define scalars, vectors, 1-forms and in general tensor fields and are able to take derivatives at any point. A differential manifold is an primitive amorphous collection of points (events in the case of spacetime). Locally, these points are ordered as points in a Euclidian space. Next, we specify a distance concept by adding a metric g, which contains information about how fast clocks proceed and what are the distances between points. −−! On the surface of the Earth we can determine a metric by drawing small vectors ∆P on the surface. We state that the length of the vector is given by the inner product −−! −−! −−! −−! ∆P· ∆P ≡ ∆P2 = (length of ∆P)2; (1.1) and use a ruler to determine its value. We now have a definition for the inner vector product for a small vector with itself. We use linearity to extend this to macroscopic vectors. Next, we can obtain a definition for the inner product of two different vectors by writing 1 h i A~ · B~ = (A~ + B~ )2 − (A~ − B~ )2 : (1.2) 4 In summary, when one has a distance concept (a ruler on the surface of the Earth), then one can define an inner product, and from this the metric follows (since it is nothing but g(A;~ B~ ) ≡ (A~ · B~ ) = g(B;~ A~). The metric tensor is symmetric.). A differentiable manifold with a metric as additional structure, is termed a (pseudo-)Riemannian manifold.
    [Show full text]
  • On the Structure of Geometries with Spinor
    ON THE STRUCTURE OF GEOMETRIES WITH SPINOR-TYPE CONNEXION M. c. Cullinan A dissertation presented in partial fulfilment of requirements for the degree of Doctor of Philosphy universitj of New South Wal~s C March 1975 .... .,,..-,·-,; ..,. ., I am indebted to Professor G. Szekeres for his constant help and guidance during the writing of this thesis. I would also like to thank Ms. Helen Cook for her careful and expert typing, and Dr. H.A. Cohen for many stimulating conversations. In addition it gives me great pleasure to acknowledge the continued support of my family and friends during the preparation of this thesis; without them this research could not have been completed. Abstract The aim of this thesis is to present a synthesis, using standard techniques of algebra and of differential geometry, of some of the principal ideas and structures of the classical field­ theoretic description of spinor fields in curved space-time. A geometric model for spinor fields in curved space-time is described which is based upon properties of so-called tangent Clifford algebras. The tangent Clifford algebra to a space-time manifold at a certain point is the quotient space of the algebra of covariant tensors at the point by a certain two-sided ideal, and is uniquely defined once the metric structure of the space-time manifold is given. Minimal left ideals of each tangent Clifford algebra are identified with spaces of four component spinors at the point. This model therefore features a direct method for synthesizing spinor fields from vector and tensor fields on a space­ time manifold.
    [Show full text]
  • Ryder Lewis Introductionto General Relativity.Pdf
    This page intentionally left blank Introduction to General Relativity A student-friendly style, over 100 illustrations, and numerous exercises are brought together in this textbook for advanced undergraduate and beginning graduate students in physics and mathematics. Lewis Ryder develops the theory of General Relativity in detail. Covering the core topics of black holes, gravitational radiation and cosmology, he provides an overview of General Relativity and its modern ramifications. The book contains a chapter on the connections between General Relativity and the fundamental physics of the microworld, explains the geometry of curved spaces and contains key solutions of Einstein’s equations – the Schwarzschild and Kerr solutions. Mathematical calculations are worked out in detail, so students can develop an intuitive understanding of the subject, as well as learn how to perform calculations. Password- protected solutions for instructors are available at www.cambridge.org/Ryder. Lewis Ryder is an Honorary Senior Lecturer in Physics at the University of Kent, UK. His research interests are in geometrical aspects of particle theory and its parallels with General Relativity. Introduction to General Relativity Lewis Ryder University of Kent, UK CAMBRIDGE UNIVERSITY PRESS Cambridge, New York, Melbourne, Madrid, Cape Town, Singapore, São Paulo, Delhi, Dubai, Tokyo Cambridge University Press The Edinburgh Building, Cambridge CB2 8RU, UK Published in the United States of America by Cambridge University Press, New York www.cambridge.org Information on this title: www.cambridge.org/9780521845632 © L. Ryder 2009 This publication is in copyright. Subject to statutory exception and to the provision of relevant collective licensing agreements, no reproduction of any part may take place without the written permission of Cambridge University Press.
    [Show full text]
  • Special Bases for Derivations of Tensor Algebras
    Special bases for derivations of tensor algebras II. The case along paths Bozhidar Z. Iliev 1 Published: Communication JINR, E5-92-508, Dubna, 1992 http://www.arXiv.org e-Print archive No. math.DG/0304157 2000 MSC numbers: 57R25, 53B05, 53B99, 53C99, 83C99 2003 PACS numbers: 02.40.Ma, 02.40.Vh, 04.20.Cv, 04.90.+h The LATEX 2ε source file of this paper was produced by converting a ChiWriter 3.16 source file into ChiWriter 4.0 file and then converting the latter file into a LATEX 2.09 source file, which was manually edited for correcting numerous errors and for improv- ing the appearance of the text. As a result of this procedure, some errors in the text may exist. Abstract The existence of local bases in which the components of derivations of tensor algebras over a differentiable manifold vanish along paths is proved. The holonomicity of these bases is investigated. The obtained results are applied to the case of linear connections. Some relations with the equivalence principle are shown. I. INTRODUCTION The existence of local coordinates in which the components of symmetric linear connections [1] vanish along a smooth path without selfintersections is a known classical result [2, 3]. In connection with the intensive use of nonsym- arXiv:math/0304157v1 [math.DG] 12 Apr 2003 metric linear connections [1, 2] in different physical theories it is natural these results to be generalized to the case of nonvanishing torsion. This paper investigates the mentioned problem from the more general view- point of arbitrary derivations of the tensor algebra over a differentiable manifold 1 Permanent address: Laboratory of Mathematical Modeling in Physics, Institute for Nu- clear Research and Nuclear Energy, Bulgarian Academy of Sciences, Boul.
    [Show full text]
  • GAUGE TORSION GRAVITY, STRING THEORY, and ANTISYMMETRIC TENSOR INTERACTIONS a Dissertation Submitted to the Graduate Faculty Of
    GAUGE TORSION GRAVITY, STRING THEORY, AND ANTISYMMETRIC TENSOR INTERACTIONS A Dissertation Submitted to the Graduate Faculty of the North Dakota State University of Agriculture and Applied Science By Terry Glenn Pilling In Partial Fulfillment of the Requirements for the Degree of DOCTOR OF PHILOSOPHY Major Department: Physics April 2002 Fargo, North Dakota Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. UMI Number: 3103621 UMI UMI Microform 3103621 Copyright 2003 by ProQuest Information and Learning Company. All rights reserved. This microform edition is protected against unauthorized copying under Title 17, United States Code. ProQuest Information and Learning Company 300 North Zeeb Road P.O. Box 1346 Ann Arbor, Ml 48106-1346 Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. North Dakota State University Graduate School Title GAUGE TORSION GRAVITY. STRING THEORY. AMD ANTISYMMETRIC TENSOR INTERACTIONS By TERRY GLENN PILLING The Supervisory Committee certifies that this disquisition complies with North Dakota State University’s regulations and meets the accepted standards for the degree of DOCTOR OF PHILOSOPHY SUPERVISORY COMMITTEE: J l k Approved by Department Chair: Date Signature Reproduced with permission of the copyright owner. Further reproduction prohibited without permission. ABSTRACT Pilling, Terry Glenn, Ph.D., Department of Physics, College of Science and Mathemat­ ics, North Dakota State University, April 2002. Gauge Torsion Gravity, String Theory, and Antisymmetric Tensor Interactions. Major Professor: Dr. Patrick F. Kelly. The antisymmetric tensor field is derived in the context of general relativity with torsion as well as the context of string theory. The interaction between antisymmetric tensor fields and fermion fields is examined.
    [Show full text]