General Physics G General Relativity: Basics and Beyond familiarizes you with the basic features of the theory of general relativity as well as some of its more advanced aspects. e Relativity Employing the pedagogical style of a textbook, it includes essential ideas and just n enough background material needed for you to appreciate the issues and current research. e The first five chapters form the core of an introductory course on general relativity. r The author traces Einstein’s arguments and presents examples of space-times a Basics and Beyond corresponding to different types of gravitational fields. He discusses the adaptation l of dynamics in a Riemannian geometry framework, the Einstein equation and its elementary properties, and different phenomena predicted or influenced by general R relativity. e Moving on to more sophisticated features of general relativity, the book presents l the physical requirements of a well-defined deterministic framework for non- a gravitational dynamics and describes the characterization of asymptotic space- times. After covering black holes, gravitational waves, and cosmological space- t i times, the book examines the evolutionary interpretation for the class of globally v hyperbolic space-times, explores numerical relativity, and discusses approaches i that address the challenges of general relativity. t Features y • Emphasizes the physical ideas and motivations of the theory while refraining from exhaustive details • Covers the mathematical aspects that are important in understanding the scope and limitations of the theory, such as the mathematical model for space-time and basic physical quantities related to space-time measurements • Explores current research topics, including the quasi-local generalization of black holes, the challenge of directly detecting gravitational waves, and the nature of cosmological singularities D • Discusses an emergent gravity viewpoint and the main approaches to a a quantum theory of gravity t • Provides the necessary background information, including differential e geometry Ghanashyam Date K15233 www.crcpress.com K15233_cover.indd 1 10/2/14 2:10 PM General Relativity Basics and Beyond General Relativity Basics and Beyond Ghanashyam Date The Institute of Mathematical Sciences Chennai, India CRC Press Taylor & Francis Group 6000 Broken Sound Parkway NW, Suite 300 Boca Raton, FL 33487-2742 © 2015 by Taylor & Francis Group, LLC CRC Press is an imprint of Taylor & Francis Group, an Informa business No claim to original U.S. Government works Version Date: 20141007 International Standard Book Number-13: 978-1-4665-5272-2 (eBook - PDF) This book contains information obtained from authentic and highly regarded sources. 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Visit the Taylor & Francis Web site at http://www.taylorandfrancis.com and the CRC Press Web site at http://www.crcpress.com Contents Preface ix I The Basics 1 1 From Newton to Einstein: Synthesis of General Relativity 3 1.1 Space, Time, Observers . . . . . . . . . . . . . . . . . . . . . 3 1.2 General Relativity and Space-Time Arenas . . . . . . . . . . 7 2 Examples of Space-Times 11 2.1 No Gravity (Minkowski Space-Time) . . . . . . . . . . . . . 18 2.2 Uniform Gravity (Rindler Space-Time) . . . . . . . . . . . . 19 2.3 Centrifugal Gravity (Uniformly Rotating Platform) . . . . . 21 2.4 Spherical Gravity (The Schwarzschild Space-Time) . . . . . . 23 2.5 Cosmological Gravity (Robertson–Walker Space-Times) . . . 25 2.6 Undulating Gravity (Gravitational Waves) . . . . . . . . . . 27 3 Dynamics in Space-Time 29 3.1 Particle Motion Including Spin . . . . . . . . . . . . . . . . . 29 3.2 Wave Motion . . . . . . . . . . . . . . . . . . . . . . . . . . . 31 4 Dynamics of Space-Time 37 4.1 Einstein Equation . . . . . . . . . . . . . . . . . . . . . . . . 37 4.2 Elementary Properties and Peculiarities . . . . . . . . . . . 40 4.3 The Stress Tensor and Fluids . . . . . . . . . . . . . . . . . 42 4.4 Operational Determination of the Metric . . . . . . . . . . . 46 5 Elementary Phenomenology 49 5.1 Geodesics and the Classic Tests . . . . . . . . . . . . . . . . 49 5.1.1 Geodesics . . . . . . . . . . . . . . . . . . . . . . . . . 52 5.1.2 Deflection of Light . . . . . . . . . . . . . . . . . . . . 53 5.1.3 Precession of Perihelia . . . . . . . . . . . . . . . . . 55 5.2 Relativistic Cosmology . . . . . . . . . . . . . . . . . . . . . 56 5.2.1 Friedmann–Lamaitre–Robertson–Walker Cosmologies 58 5.2.2 Digression on Big-Bang Cosmology: Thermal History 62 5.2.3 Cosmic Microwave Background Radiation . . . . . . . 68 5.3 Gravitational Waves . . . . . . . . . . . . . . . . . . . . . . 72 5.3.1 Plane Waves . . . . . . . . . . . . . . . . . . . . . . . 73 v vi Contents 5.3.2 Gravitational Radiation . . . . . . . . . . . . . . . . . 75 5.3.3 Radiated Energy and the Quadrupole Formula . . . . 78 5.4 Black Holes—Elementary Aspects . . . . . . . . . . . . . . . 83 5.4.1 Static Black Holes . . . . . . . . . . . . . . . . . . . . 83 5.4.1.1 Schwarzschild Black Hole . . . . . . . . . . . 83 5.4.1.2 The Reissner–Nordstrom Black Hole . . . . . 86 5.4.2 Stationary (Non-Static) Black Holes . . . . . . . . . . 88 5.4.2.1 Kerr–Newman Black Holes . . . . . . . . . . 88 5.4.3 Observational Status . . . . . . . . . . . . . . . . . . 90 5.5 Stars in GR . . . . . . . . . . . . . . . . . . . . . . . . . . . 91 II The Beyond 95 6 The Space-Time Arena 97 6.1 Preliminary Notions and Results . . . . . . . . . . . . . . . 98 6.2 Causality . . . . . . . . . . . . . . . . . . . . . . . . . . . . 103 6.3 Determinism and Global Hyperbolicity . . . . . . . . . . . . 105 6.4 Geodesics and Congruences . . . . . . . . . . . . . . . . . . 108 6.5 Singularity Theorems . . . . . . . . . . . . . . . . . . . . . . 117 7 Asymptotic Structure 123 7.1 Vicinity of the Null Infinity . . . . . . . . . . . . . . . . . . . 128 7.2 Vicinity of the Spatial Infinity . . . . . . . . . . . . . . . . . 136 8 Black Holes 139 8.1 Examples of Extended Black Hole Solutions . . . . . . . . . 139 8.2 General Black Holes and Uniqueness Theorems . . . . . . . 144 8.3 Black Hole Thermodynamics . . . . . . . . . . . . . . . . . . 147 8.4 Quasi-Local Definitions of Horizons . . . . . . . . . . . . . . 150 9 Cosmological Space-Times 159 10 Gravitational Waves 167 10.1 Conceptual Issues . . . . . . . . . . . . . . . . . . . . . . . . 167 10.2 Observational Issues . . . . . . . . . . . . . . . . . . . . . . 169 11 Field Equation: Evolutionary Interpretation 173 11.1 The 3 + 1 Decomposition . . . . . . . . . . . . . . . . . . . 173 11.2 Initial Value Formulation . . . . . . . . . . . . . . . . . . . . 176 11.3 Hamiltonian Formulation (ADM) . . . . . . . . . . . . . . . 179 12 Numerical Relativity 185 Contents vii 13 Into the Quantum Realm 191 13.1 Gravity Is “Emergent” . . . . . . . . . . . . . . . . . . . . . 192 13.2 The Quantum Gravity Paradigm . . . . . . . . . . . . . . . 194 13.2.1 String Theory: The Unification Paradigm . . . . . . . 195 13.2.2 LoopQuantumGravity:TheBackgroundIndependence Demand . . . . . . . . . . . . . . . . . . . . . . . . . 196 14 Mathematical Background 199 14.1 Basic Differential Geometry . . . . . . . . . . . . . . . . . . 199 14.2 Sets, Metric Spaces and Topological Spaces . . . . . . . . . 199 14.3 Manifolds and Tensors . . . . . . . . . . . . . . . . . . . . . 202 14.4 Affine Connection and Curvature . . . . . . . . . . . . . . . 207 14.5 Metric Tensor and Pseudo–Riemannian Geometry . . . . . . 211 14.6 Summary of Differential Geometry . . . . . . . . . . . . . . . 212 14.7 Theorems on Initial Value Problem . . . . . . . . . . . . . . 232 14.8 Petrov Classification . . . . . . . . . . . . . . . . . . . . . . . 234 Epilogue 237 Bibliography 239 Index 251 Preface It fills me with a sense of joy and humility to present this book on the eve of the centenary year of the publication of Albert Einstein’s General Theory of Relativity. When general relativity arrived, it had an aura of mystery due to its sophisticated view of space, time and gravitational phenomena. From the early phase when primary elaboration of the theory was mathematical in nature,ithasevolvedintoaphasewhereitisbeingconfrontedbyincreasingly sophisticatedexperimentsthathavebeensuccessfulsofar.Studentsareoften attracted to the theory and want to know what yet can be done with it. The book is envisaged as an attempt to familiarize students and prospective researcherswiththebasicfeaturesofthetheoryandofferaperspectiveonits more advance features. There are many excellent textbooks from the classics by Misner–Thorne– Wheeler, Weinberg and Wald to the more recent ones by Sean Carroll, James HartleandThanuPadmanabhan,withdifferingstylesandemphasisandthere are excellent review articles on frontline topics. The idea here is to combine the ‘textbook’ and ‘the review’. Thus, I have tried to adopt the pedagogical styleofatextbookwhileavoidinganemphasisondetailedtreatments,andat thesametime,triedtopresenttheessentialideasandjustenoughbackground material needed for students to appreciate the issues and current research. There was also a conscious effort to emphasize the physical ideas and motivations, contrasting the mathematical idealizations which are important inappreciatingthescopeandlimitationsofthetheory.Consequently,requisite mathematical background of differential geometry is summarized in the last chapter while the main text emphasizes the physical aspects. The first five chapters usually form the core of an introductory course on General Relativity (GR) and constitute the “Basics” part of the book. The first chapter traces Einstein’s arguments and informally motivates the mathematical model for space-time. In the second chapter, we first discuss the basic physical quantities related to space-time measurements and their relation to a metric in an arbitrary coordinate system. This is followed by examplesofspace-timescorrespondingtodifferenttypesofgravitationalfields. Some of these are revisited subsequently for further elaboration. Chapter 3 discussesadaptationof dynamicsinaRiemanniangeometryframeworkwhile the next chapter presents the Einstein equation together with its elementary properties. The fifth chapter discusses different phenomena either predicted ix