GRAVITATIONAL COLLAPSE AND RELATIVITY
|
|
|
- Buck Short
- 5 years ago
- Views:
Transcription
1 Proceedings of Yamada Conference XIV GRAVITATIONAL COLLAPSE AND RELATIVITY KYOTO INTERNATIONAL CONFERENCE HALL, JAPAN 7-11 APRIL 1986 EDITED BY HUMITAKA SATO TAKASHI NAKAMURA UNIVERSITATSBIBLIOTHEK HANNOVER TEC HN ISC HE INFORM ATiONSBIBLIOTHEK Wortd Scientific
2 CONTENTS XI Preface v Welcome address vii Yamada Science Foundation and the Scope of Yamada Conference ix Advisers and Organizing Committee x H. Sato Opening Address 1 J. Ehlers Summary 4 DISCOURSES K. S. Thorne The membrane paradigm and black-hole 13 thermodynamics S. Hayakasa Black hole candidates in X-ray binaries 20 R. Penrose Gravitational field mass 43 CLASSICAL RELATIVITY T. Damour On the propagation problem in gravitational 63 radiation theory F. I. Cooperstock The new formula for gravitational radiation energy 74 and P. H. Lim loss and its applications T. Futamase The strong field point particle limit and the 81 quadrupole formula in the binary pulsar system J. N. Goldberg Surface integrals associated with the canonical 88 formalism on a null surface W. Israel The third law 96
3 XII D. C. Chern and J. M. Nester M. Sasaki Positive energy and Poincare gauge theory 106 Gauge-invariant cosmological density perturbations 114 EXACT SOLUTION M. A. H. MacCallum F. J. Ernst M. Yamazaki S. M. Scott C. Hoenselaers F. B. Estabrook M. Jimbo, T. Miwa and M. Okado M. Gurses F. J. Chinea J. Winicour S.W.Kim and B. H. Cho S. Antoci Computer-aided classification of exact solutions in general relativity Derivation of Nutku-Halil colliding plane wave solution from isotropic Kasner metric using double-harrison transformation Black holes and monopoles Analysis of a directional singularity On multipole moments in general relativity Frame bundles: Covariance, invariant forms and exterior differential systems for Ricci-flat solutions Solvable lattice models and the elliptic theta functions Some linear prolongations of the vacuum gravitational field equations Clifford algebras in general relativity Exact solutions, numerical relativity and gravitational radiation Bianchi type-l solutions in Brans-Dicke theory with torsion An interpretation of the Hermitian theory of relativity COMPUTER-AIDED RELATIVITY R. F. Stark and T. Pi ran Gravitational radiation from rotating gravitational collapse 249
4 J. A. Marck and T. Piran S. M. Miyama, M. Nagasawa and T. Nakamura T. Nakamura K. Oohara Y. Kojima J. B. Hartle M. R. Dubai B. F. Schutz H. Komatsu, Y. Eriguchi and I. Hachisu F. de Felice and L. Sigalotti S. L. Shapiro and S. A. Teukolsky 3-D relativistic hydrodynamics around a Kerr 276 black hole Gravitational radiation in the 3-D processes such 282 as fragmentation and collision of fluids Gravitational radiation and 3D numerical 295 relativity Apparent horizon of initial data for black hole- 313 collision Gravitational radiation from a Kerr black hole 320 Numerical quantum gravity 329 Regge calculus in numerical relativity 339 Hubble's constant from gravitational wave 350 observations Rapidly rotating general relativistic polytropes 369 The value of the a/m ratio in binary systems 377 Computer simulations of relativistic star clusters 387 xin COSMOLOGY AND OTHER TOPICS A. Tomimatsu Are extra dimensions visible near the event 417 horizon? Black holes coupled to scalar fields K. Maeda C. H. Lee and H. K. Lee The Einstein gravity as an attractor in higher- 426 dimensional theories Higher dimensional cosmology 434
5 XIV H. Ishihara Higher dimensional solutions of modified Einstein equations with curvature square terms 443 K. V. Kuchar and M. P. Ryan Jr. SWada T. Azuma R. Balbinot Y. Fujii A. Krasinski Can mini-superspace quantization be justified? 451 Who decides boundary conditions for the wave 465 function of the universe? Cosmological solutions of the Einstein equation 474 with the backreaction effect of quantized conformally invariant fields Quantum effects in nonstatic black hole space- 482 times Nonzero effect of the Eotvds experiment? 491 Inhomogeneous generalizations of the Robertson- 500 Walker cosmological models Conference program 509 List of participants 511
Classical Field Theory
April 13, 2010 Field Theory : Introduction A classical field theory is a physical theory that describes the study of how one or more physical fields interact with matter. The word classical is used in
Black Hole Physics. Basic Concepts and New Developments KLUWER ACADEMIC PUBLISHERS. Valeri P. Frolov. Igor D. Nbvikov. and
Black Hole Physics Basic Concepts and New Developments by Valeri P. Frolov Department of Physics, University of Alberta, Edmonton, Alberta, Canada and Igor D. Nbvikov Theoretical Astrophysics Center, University
Tensor Calculus, Relativity, and Cosmology
Tensor Calculus, Relativity, and Cosmology A First Course by M. Dalarsson Ericsson Research and Development Stockholm, Sweden and N. Dalarsson Royal Institute of Technology Stockholm, Sweden ELSEVIER ACADEMIC
Relativity, Gravitation, and Cosmology
Relativity, Gravitation, and Cosmology A basic introduction TA-PEI CHENG University of Missouri St. Louis OXFORD UNIVERSITY PRESS Contents Parti RELATIVITY Metric Description of Spacetime 1 Introduction
2.5.1 Static tides Tidal dissipation Dynamical tides Bibliographical notes Exercises 118
ii Contents Preface xiii 1 Foundations of Newtonian gravity 1 1.1 Newtonian gravity 2 1.2 Equations of Newtonian gravity 3 1.3 Newtonian field equation 7 1.4 Equations of hydrodynamics 9 1.4.1 Motion of
Modern Geometric Structures and Fields
Modern Geometric Structures and Fields S. P. Novikov I.A.TaJmanov Translated by Dmitry Chibisov Graduate Studies in Mathematics Volume 71 American Mathematical Society Providence, Rhode Island Preface
INTRODUCTION TO GENERAL RELATIVITY
INTRODUCTION TO GENERAL RELATIVITY RONALD ADLER Instito de Fisica Universidade Federal de Pemambuco Recife, Brazil MAURICE BAZIN Department of Physics Rutgers University MENAHEM SCHIFFER Department of
Richard A. Mould. Basic Relativity. With 144 Figures. Springer-Verlag New York Berlin Heidelberg London Paris Tokyo Hong Kong Barcelona Budapest
Richard A. Mould Basic Relativity With 144 Figures Springer-Verlag New York Berlin Heidelberg London Paris Tokyo Hong Kong Barcelona Budapest Contents Preface vii PARTI 1. Principles of Relativity 3 1.1
RELG - General Relativity
Coordinating unit: Teaching unit: Academic year: Degree: ECTS credits: 2017 230 - ETSETB - Barcelona School of Telecommunications Engineering 749 - MAT - Department of Mathematics 748 - FIS - Department
Lecture Notes on General Relativity
Lecture Notes on General Relativity Matthias Blau Albert Einstein Center for Fundamental Physics Institut für Theoretische Physik Universität Bern CH-3012 Bern, Switzerland The latest version of these
Colliding scalar pulses in the Einstein-Gauss-Bonnet gravity
Colliding scalar pulses in the Einstein-Gauss-Bonnet gravity Hisaaki Shinkai 1, and Takashi Torii 2, 1 Department of Information Systems, Osaka Institute of Technology, Hirakata City, Osaka 573-0196, Japan
Second-order gauge-invariant cosmological perturbation theory: --- Recent development and problems ---
Second-order gauge-invariant cosmological perturbation theory: --- Recent development and problems --- Kouji Nakamura (NAOJ) with Masa-Katsu Fujimoto (NAOJ) References : K.N. Prog. Theor. Phys., 110 (2003),
COSMOLOGY The Origin and Evolution of Cosmic Structure
COSMOLOGY The Origin and Evolution of Cosmic Structure Peter COLES Astronomy Unit, Queen Mary & Westfield College, University of London, United Kingdom Francesco LUCCHIN Dipartimento di Astronomia, Universita
Chapters of Advanced General Relativity
Chapters of Advanced General Relativity Notes for the Amsterdam-Brussels-Geneva-Paris doctoral school 2014 & 2016 In preparation Glenn Barnich Physique Théorique et Mathématique Université Libre de Bruxelles
Supplement to Lesson 9: The Petrov classification and the Weyl tensor
Supplement to Lesson 9: The Petrov classification and the Weyl tensor Mario Diaz November 1, 2015 As we have pointed out one of unsolved problems of General Relativity (and one that might be impossible
Quantum gravity and aspects of relativity
Quantum gravity and aspects of relativity Branislav Nikolic Institute for Theoretical Physics, University of Cologne Bonn-Cologne Graduate School in Physics and Astronomy who are we??? Gravitation and
A Summary of the Black Hole Perturbation Theory. Steven Hochman
A Summary of the Black Hole Perturbation Theory Steven Hochman Introduction Many frameworks for doing perturbation theory The two most popular ones Direct examination of the Einstein equations -> Zerilli-Regge-Wheeler
Relativity SPECIAL, GENERAL, AND COSMOLOGICAL SECOND EDITION. Wolfgang Rindler. Professor of Physics The University of Texas at Dallas
Relativity SPECIAL, GENERAL, AND COSMOLOGICAL SECOND EDITION Wolfgang Rindler Professor of Physics The University of Texas at Dallas OXPORD UNIVERSITY PRESS Contents Introduction l 1 From absolute space
PRINCIPLES OF PHYSICS. \Hp. Ni Jun TSINGHUA. Physics. From Quantum Field Theory. to Classical Mechanics. World Scientific. Vol.2. Report and Review in
LONDON BEIJING HONG TSINGHUA Report and Review in Physics Vol2 PRINCIPLES OF PHYSICS From Quantum Field Theory to Classical Mechanics Ni Jun Tsinghua University, China NEW JERSEY \Hp SINGAPORE World Scientific
Emergent Universe by Tunneling. Pedro Labraña, ICC, Universidad de Barcelona and Facultad de Ciencias, Universidad del Bío-Bío, Chile.
Emergent Universe by Tunneling Pedro Labraña, ICC, Universidad de Barcelona and Facultad de Ciencias, Universidad del Bío-Bío, Chile. The Emergent Universe scenario Is Eternal Inflation, past eternal?
Overview and Innerview of Black Holes
Overview and Innerview of Black Holes Kip S. Thorne, Caltech Beyond Einstein: From the Big Bang to Black Holes SLAC, 14 May 2004 1 Black Hole Created by Implosion of a Star Our Focus: quiescent black hole
The Chronology Protection Conjecture and the Formation of the Kerr Black Hole through Gravitational Collapse
The Chronology Protection Conjecture and the Formation of the Kerr Black Hole through Gravitational Collapse Moninder Singh Modgil 1 Abstract Exterior of the Kerr black hole is considered as the likely
Modern Cosmology / Scott Dodelson Contents
Modern Cosmology / Scott Dodelson Contents The Standard Model and Beyond p. 1 The Expanding Universe p. 1 The Hubble Diagram p. 7 Big Bang Nucleosynthesis p. 9 The Cosmic Microwave Background p. 13 Beyond
Non-existence of time-periodic dynamics in general relativity
Non-existence of time-periodic dynamics in general relativity Volker Schlue University of Toronto University of Miami, February 2, 2015 Outline 1 General relativity Newtonian mechanics Self-gravitating
Theory. V H Satheeshkumar. XXVII Texas Symposium, Dallas, TX December 8 13, 2013
Department of Physics Baylor University Waco, TX 76798-7316, based on my paper with J Greenwald, J Lenells and A Wang Phys. Rev. D 88 (2013) 024044 with XXVII Texas Symposium, Dallas, TX December 8 13,
Index. Cambridge University Press A First Course in General Relativity: Second Edition Bernard F. Schutz. Index.
accelerated particle, 41 acceleration, 46 48 absolute, 2 of the universe, 351 353 accretion disk, 317 active gravitational mass, 197, 202, 355 adiabatic, 103 affine parameter, 161, 166, 175 angular diameter
DARK MATTER IN UNIVERSE. edited by. John Bahcall Institute for Advanced Study, Princeton, USA. Tsvi Piran The Hebrew University, Israel
DARK MATTER IN UNIVERSE n d edited by John Bahcall Institute for Advanced Study, Princeton, USA Tsvi Piran The Hebrew University, Israel Steven Weinberg University of Texas, Austin, USA TECHNiSCHE INFORMATIONSBIBLIOTHEK
Stephen Blaha, Ph.D. M PubHsMtw
Quantum Big Bang Cosmology: Complex Space-time General Relativity, Quantum Coordinates,"Dodecahedral Universe, Inflation, and New Spin 0, 1 / 2,1 & 2 Tachyons & Imagyons Stephen Blaha, Ph.D. M PubHsMtw
Gravitational radiation from compact binaries in scalar-tensor gravity
Gravitational radiation from compact binaries in scalar-tensor gravity Ryan Lang University of Florida 10th International LISA Symposium May 23, 2014 Testing general relativity General relativity has withstood
An Introduction to General Relativity and Cosmology
An Introduction to General Relativity and Cosmology Jerzy Plebariski Centro de Investigacion y de Estudios Avanzados Instituto Politecnico Nacional Apartado Postal 14-740, 07000 Mexico D.F., Mexico Andrzej
Relativistic theory of surficial Love numbers
Department of Physics, University of Guelph APS April Meeting 2013, Denver Newtonian tides 1 In Newtonian theory, the tidal environment of a body of mass M and radius R is described by the tidal quadrupole
Graceful exit from inflation for minimally coupled Bianchi A scalar field models
Graceful exit from inflation for minimally coupled Bianchi A scalar field models Florian Beyer Reference: F.B. and Leon Escobar (2013), CQG, 30(19), p.195020. University of Otago, Dunedin, New Zealand
Bibliography. Introduction to General Relativity and Cosmology Downloaded from
Bibliography Abbott, B. P. et al. (2016). Observation of gravitational waves from a binary black hole merger, Phys. Rev. Lett. 116, 061102. Ade, P. A. R. et al. (2015). Planck 2015 results. XIII. Cosmological
Black holes in loop quantum gravity
Black holes in loop quantum gravity Javier Olmedo Physics Department - Institute for Gravitation & the Cosmos Pennsylvania State University Quantum Gravity in the Southern Cone VII March, 31st 2017 1 /
A loop quantum multiverse?
Space-time structure p. 1 A loop quantum multiverse? Martin Bojowald The Pennsylvania State University Institute for Gravitation and the Cosmos University Park, PA arxiv:1212.5150 Space-time structure
A GENERAL RELATIVITY WORKBOOK. Thomas A. Moore. Pomona College. University Science Books. California. Mill Valley,
A GENERAL RELATIVITY WORKBOOK Thomas A. Moore Pomona College University Science Books Mill Valley, California CONTENTS Preface xv 1. INTRODUCTION 1 Concept Summary 2 Homework Problems 9 General Relativity
Black-hole binary inspiral and merger in scalar-tensor theory of gravity
Black-hole binary inspiral and merger in scalar-tensor theory of gravity U. Sperhake DAMTP, University of Cambridge General Relativity Seminar, DAMTP, University of Cambridge 24 th January 2014 U. Sperhake
Gravity and action at a distance
Gravitational waves Gravity and action at a distance Newtonian gravity: instantaneous action at a distance Maxwell's theory of electromagnetism: E and B fields at distance D from charge/current distribution:
Quantum Gravity and Black Holes
Quantum Gravity and Black Holes Viqar Husain March 30, 2007 Outline Classical setting Quantum theory Gravitational collapse in quantum gravity Summary/Outlook Role of metrics In conventional theories the
IoP. An Introduction to the Science of Cosmology. Derek Raine. Ted Thomas. Series in Astronomy and Astrophysics
Series in Astronomy and Astrophysics An Introduction to the Science of Cosmology Derek Raine Department of Physics and Astronomy University of Leicester, UK Ted Thomas Department of Physics and Astronomy
Pedagogical Strategy
Integre Technical Publishing Co., Inc. Hartle November 18, 2002 1:42 p.m. hartlemain19-end page 557 Pedagogical Strategy APPENDIX D...as simple as possible, but not simpler. attributed to A. Einstein The
An introduction to General Relativity and the positive mass theorem
An introduction to General Relativity and the positive mass theorem National Center for Theoretical Sciences, Mathematics Division March 2 nd, 2007 Wen-ling Huang Department of Mathematics University of
The Cosmic Barber: Counting Gravitational Hair in the Solar System and beyond. Clifford Will Washington University, St. Louis
The Cosmic Barber: Counting Gravitational Hair in the Solar System and beyond Clifford Will Washington University, St. Louis Testing GR with Astrophysical Systems May 17, 2012 Counting Gravitational Hair
General Relativity (2nd part)
General Relativity (2nd part) Electromagnetism Remember Maxwell equations Conservation Electromagnetism Can collect E and B in a tensor given by And the charge density Can be constructed from and current
Lecture 1 General relativity and cosmology. Kerson Huang MIT & IAS, NTU
A Superfluid Universe Lecture 1 General relativity and cosmology Kerson Huang MIT & IAS, NTU Lecture 1. General relativity and cosmology Mathematics and physics Big bang Dark energy Dark matter Robertson-Walker
So the question remains how does the blackhole still display information on mass?
THE ZERO POINT NON-LOCAL FRAME AND BLACKHOLES By: Doctor Paul Karl Hoiland Abstract: I will show that my own zero point Model supports not only the no-hair proposals, but also the Bekenstein bound on information
Perturbed Einstein field equations using Maple
Perturbed Einstein field equations using Maple arxiv:gr-qc/0304008v2 9 Jun 2003 M.de Campos () February 7, 2008 Abstract We obtain the perturbed components of affine connection and Ricci tensor using algebraic
How black holes get their kicks! Gravitational radiation recoil from binary inspiral and plunge into a rapidly-rotating black hole.
How black holes get their kicks! Gravitational radiation recoil from binary inspiral and plunge into a rapidly-rotating black hole. Marc Favata (Cornell) Daniel Holz (U. Chicago) Scott Hughes (MIT) The
Contents Part I The General Theory of Relativity Introduction Physics in External Gravitational Fields
Contents Part I The General Theory of Relativity 1 Introduction... 3 2 Physics in External Gravitational Fields... 7 2.1 Characteristic Properties of Gravitation... 7 2.1.1 Strength of the Gravitational
Fundamental Theories of Physics in Flat and Curved Space-Time
Fundamental Theories of Physics in Flat and Curved Space-Time Zdzislaw Musielak and John Fry Department of Physics The University of Texas at Arlington OUTLINE General Relativity Our Main Goals Basic Principles
Gauge-invariant quantity. Monday, June 23, 2014
Gauge-invariant quantity U Topics that will be covered Gauge-invariant quantity, U, (reciprocal of the red-shift invariant, z), the 1 st order (in mass-ratio) change in u t. For eccentric orbits it can
First structure equation
First structure equation Spin connection Let us consider the differential of the vielbvein it is not a Lorentz vector. Introduce the spin connection connection one form The quantity transforms as a vector
General Relativity in AdS
General Relativity in AdS Akihiro Ishibashi 3 July 2013 KIAS-YITP joint workshop 1-5 July 2013, Kyoto Based on work 2012 w/ Kengo Maeda w/ Norihiro Iizuka, Kengo Maeda - work in progress Plan 1. Classical
Geometry of SpaceTime Einstein Theory. of Gravity II. Max Camenzind CB Oct-2010-D7
Geometry of SpaceTime Einstein Theory of Gravity II Max Camenzind CB Oct-2010-D7 Textbooks on General Relativity Geometry of SpaceTime II Connection and curvature on manifolds. Sectional Curvature. Geodetic
Introduction to Numerical Relativity
APCTP Winter School, January 17-18, 2003 Introduction to Numerical Relativity RIKEN Institute, Computational Science Division, Hisaaki Shinkai 1. Subjects for Numerical Relativity Why Numerical Relativity?
Tidal deformation and dynamics of compact bodies
Department of Physics, University of Guelph Capra 17, Pasadena, June 2014 Outline Goal and motivation Newtonian tides Relativistic tides Relativistic tidal dynamics Conclusion Goal and motivation Goal
Nonsingular big-bounce cosmology from spin and torsion
Nonsingular big-bounce cosmology from spin and torsion Nikodem J. Popławski Department of Physics, Indiana University, Bloomington, IN 22 nd Midwest Relativity Meeting University of Chicago, Chicago, IL
Stability and Instability of Black Holes
Stability and Instability of Black Holes Stefanos Aretakis September 24, 2013 General relativity is a successful theory of gravitation. Objects of study: (4-dimensional) Lorentzian manifolds (M, g) which
The initial value problem in general relativity
LC Physics Colloquium, Spring 2015 Abstract In 1915, Einstein introduced equations describing a theory of gravitation known as general relativity. The Einstein equations, as they are now called, are at
Charles Keeton. Principles of Astrophysics. Using Gravity and Stellar Physics. to Explore the Cosmos. ^ Springer
Charles Keeton Principles of Astrophysics Using Gravity and Stellar Physics to Explore the Cosmos ^ Springer Contents 1 Introduction: Tools of the Trade 1 1.1 What Is Gravity? 1 1.2 Dimensions and Units
Electromagnetic spikes
Electromagnetic spikes Ernesto Nungesser (joint work with Woei Chet Lim) Trinity College Dublin ANZAMP, 29th of November, 2013 Overview Heuristic picture of initial singularity What is a Bianchi spacetime?
1 The role of gravity The view of physics that is most generally accepted at the moment is that one can divide the discussion of the universe into
1 The role of gravity The view of physics that is most generally accepted at the moment is that one can divide the discussion of the universe into two parts. First, there is the question of the local laws
PRIMORDIAL COSMOLOGY
PRIMORDIAL COSMOLOGY Giovanni Montani ENEA - C.R. Frascati, ICFtANet and Dipartimento di Fisica, Universita di Roma "Sapienza", Italy Marco Valerio Battisti Dipartimento di Fisica, Universita di Roma "Sapienza",
Non-gravitating waves
Non-gravitating waves D C Robinson Mathematics Department King s College London Strand London WC2R 2LS United Kingdom email: david.c.robinson@kcl.ac.uk October 6, 2005 Abstract: It is pointed out that
5.5 Energy-momentum tensor
5.5 Energy-momentum tensor components of stress tensor force area of cross section normal to cross section 5 Special Relativity provides relation between the forces and the cross sections these are exerted
2.1 Basics of the Relativistic Cosmology: Global Geometry and the Dynamics of the Universe Part I
1 2.1 Basics of the Relativistic Cosmology: Global Geometry and the Dynamics of the Universe Part I 2 Special Relativity (1905) A fundamental change in viewing the physical space and time, now unified
Dynamics of star clusters containing stellar mass black holes: 1. Introduction to Gravitational Waves
Dynamics of star clusters containing stellar mass black holes: 1. Introduction to Gravitational Waves July 25, 2017 Bonn Seoul National University Outline What are the gravitational waves? Generation of
Contents. Preface to the second edition. Preface to the first edition. Part I Introduction to gravity and supergravity 1
Table of Preface to the second edition page xxi Preface to the first edition xxv Part I Introduction to gravity and supergravity 1 1 Differential geometry 3 1.1 World tensors 3 1.2 Affinely connected spacetimes
GRAVITATIONAL COLLAPSE
GRAVITATIONAL COLLAPSE Landau and Chandrasekhar first realised the importance of General Relativity for Stars (1930). If we increase their mass and/or density, the effects of gravitation become increasingly
COSMOLOGY IN HIGHER DIMENSIONS
COSMOLOGY IN HIGHER DIMENSIONS 1. Introduction 2. Overview of Higher Dimensional Cosmology 3. Cosmology in Higher Dimensions 4. String Frame 5. Summary Kei-ichi MAEDA Waseda University 1. INTRODUCTION
Black-hole binaries in Einstein-dilaton Gauss Bonnet gravity
Black-hole binaries in Einstein-dilaton Gauss Bonnet gravity Helvi Witek Theoretical Particle Physics and Cosmology Department of Physics, King s College London work in progress with L. Gualtieri, P. Pani,
Black Hole Universe with Rotation Chan Park KAIST
Black Hole Universe with Rotation 2016.01.02. Chan Park KAIST Motivation FLRW cosmology Highly symmetric assumption : spatial homogeneity and isotropy Metric ds 2 = dt 2 + a 2 t a t : scale factor Friedmann
arxiv:gr-qc/ v4 4 Oct 2004
PRAMANA c Indian Academy of Sciences Vol. 53, No. 6 journal of December 1999 physics pp. 1 12 Gravitational collapse and naked singularities Tomohiro Harada Astronomy Unit, School of Mathematical Sciences,
A873: Cosmology Course Notes. II. General Relativity
II. General Relativity Suggested Readings on this Section (All Optional) For a quick mathematical introduction to GR, try Chapter 1 of Peacock. For a brilliant historical treatment of relativity (special
The BKL proposal and cosmic censorship
- 1 - The BKL proposal and cosmic censorship Lars Andersson University of Miami and Albert Einstein Institute (joint work with Henk van Elst, Claes Uggla and Woei-Chet Lim) References: Gowdy phenomenology
Norihiro Tanahashi (Kavli IPMU)
Norihiro Tanahashi (Kavli IPMU) in collaboration with James Lucietti, Keiju Murata, Harvey S. Reall based on arxiv:1212.2557 Classical stability of 4D Black holes Stable (mostly) Power-law decay of perturbations
EXCISION TECHNIQUE IN CONSTRAINED FORMULATIONS OF EINSTEIN EQUATIONS
EXCISION TECHNIQUE IN CONSTRAINED FORMULATIONS OF EINSTEIN EQUATIONS Journée Gravitation et Physique Fondamentale Meudon, 27 May 2014 Isabel Cordero-Carrión Laboratoire Univers et Théories (LUTh), Observatory
Advanced Study, 9 Adela Court, Mulgrave, Victoria 3170, Australia
A CLASSIFICATION OF QUANTUM PARTICLES Vu B Ho Advanced Study, 9 Adela Court, Mulgrave, Victoria 3170, Australia Email: vubho@bigpond.net.au Abstract: In this work, by summarising our recent works on the
Questions for Black Hole evaporation from Quantum Statistical Mechanics
Questions for Black Hole evaporation from Quantum Statistical Mechanics David Wallace Philosophy Department, University of Southern California Black Hole Initiative, May 9 th 2017 Thermally Typical Black
Nature of Singularities in (n+2)-dimensional Gravitational Collapse of Vaidya Space-time in presence of monopole field.
Nature of Singularities in (n+2)-dimensional Gravitational Collapse of Vaidya Space-time in presence of monopole field. 1 C. S. Khodre, 2 K. D.Patil, 3 S. D.Kohale and 3 P. B.Jikar 1 Department of Mathematics,
Introduction to Numerical Relativity I. Erik Schnetter, Pohang, July 2007
Introduction to Numerical Relativity I Erik Schnetter, Pohang, July 2007 Lectures Overview I. The Einstein Equations (Formulations and Gauge Conditions) II. Analysis Methods (Horizons and Gravitational
BLACKHOLE WORMHOLE THEORY
BLACKHOLE WORMHOLE THEORY By - ASHU PRAKASH Black hole, a name which has infinite knowledge to define, but very difficult to define. What is a black hole? In general, a black hole is a gravitationally
Covariant Equations of Motion of Extended Bodies with Mass and Spin Multipoles
Covariant Equations of Motion of Extended Bodies with Mass and Spin Multipoles Sergei Kopeikin University of Missouri-Columbia 1 Content of lecture: Motivations Statement of the problem Notable issues
Konstantin E. Osetrin. Tomsk State Pedagogical University
Space-time models with dust and cosmological constant, that allow integrating the Hamilton-Jacobi test particle equation by separation of variables method. Konstantin E. Osetrin Tomsk State Pedagogical
Fluid/Gravity Correspondence for general non-rotating black holes
Fluid/Gravity Correspondence for general non-rotating black holes Xiaoning Wu Institute of Mathematics, AMSS, CAS 2013. 7. 30, @Max Planck Institute for Physics, Munich Joint work with Y. Ling, Y. Tian,
The Quadrupole Moment of Rotating Fluid Balls
The Quadrupole Moment of Rotating Fluid Balls Michael Bradley, Umeå University, Sweden Gyula Fodor, KFKI, Budapest, Hungary Current topics in Exact Solutions, Gent, 8- April 04 Phys. Rev. D 79, 04408 (009)
HOMEWORK 10. Applications: special relativity, Newtonian limit, gravitational waves, gravitational lensing, cosmology, 1 black holes
General Relativity 8.96 (Petters, spring 003) HOMEWORK 10. Applications: special relativity, Newtonian limit, gravitational waves, gravitational lensing, cosmology, 1 black holes 1. Special Relativity
Topics in Relativistic Astrophysics
Topics in Relativistic Astrophysics John Friedman ICTP/SAIFR Advanced School in General Relativity Parker Center for Gravitation, Cosmology, and Astrophysics Part I: General relativistic perfect fluids
General Relativity Lecture 20
General Relativity Lecture 20 1 General relativity General relativity is the classical (not quantum mechanical) theory of gravitation. As the gravitational interaction is a result of the structure of space-time,
Cosmological Implications of Spinor-Torsion Coupling
Cosmological Implications of Spinor-Torsion Coupling Nikodem J. Popławski Department of Physics, Indiana University, Bloomington, IN Astrophysics-Relativity Seminar Department of Physics and Astronomy
PoS(HEP2005)010. Spontaneously Induced Gravity: From Rippled Dark Matter to Einstein Corpuscles. Aharon Davidson and Ilya Gurwich
Spontaneously Induced Gravity: From Rippled Dark Matter to Einstein Corpuscles and Ilya Gurwich Ben-Gurion University, Israel E-mail: davidson@bgu.ac.il Suppose General Relativity, provocatively governed
Jose Luis Blázquez Salcedo
Jose Luis Blázquez Salcedo In collaboration with Jutta Kunz, Francisco Navarro Lérida, and Eugen Radu GR Spring School, March 2015, Brandenburg an der Havel 1. Introduction 2. General properties of EMCS-AdS
String Theory in a Nutshell. Elias Kiritsis
String Theory in a Nutshell Elias Kiritsis P R I N C E T O N U N I V E R S I T Y P R E S S P R I N C E T O N A N D O X F O R D Contents Preface Abbreviations xv xvii Introduction 1 1.1 Prehistory 1 1.2
Jose Luis Blázquez Salcedo
Physical Review Letters 112 (2014) 011101 Jose Luis Blázquez Salcedo In collaboration with Jutta Kunz, Eugen Radu and Francisco Navarro Lérida 1. Introduction: Ansatz and general properties 2. Near-horizon
CMB Polarization in Einstein-Aether Theory
CMB Polarization in Einstein-Aether Theory Masahiro Nakashima (The Univ. of Tokyo, RESCEU) With Tsutomu Kobayashi (RESCEU) COSMO/CosPa 2010 Introduction Two Big Mysteries of Cosmology Dark Energy & Dark
Theoretical Aspects of Black Hole Physics
Les Chercheurs Luxembourgeois à l Etranger, Luxembourg-Ville, October 24, 2011 Hawking & Ellis Theoretical Aspects of Black Hole Physics Glenn Barnich Physique théorique et mathématique Université Libre
Intrinsic Time Quantum Geometrodynamics (ITQG)
Intrinsic Time Quantum Geometrodynamics (ITQG) Assistant Professor Eyo Ita Eyo Eyo Ita Physics Department LQG International Seminar United States Naval Academy Annapolis, MD 27 October, 2015 Outline of
Toward Binary Black Hole Simulations in Numerical Relativity
Toward Binary Black Hole Simulations in Numerical Relativity Frans Pretorius California Institute of Technology BIRS Workshop on Numerical Relativity Banff, April 19 2005 Outline generalized harmonic coordinates
Crossing the Event Horizon Presented by Nassim Haramein
Crossing the Event Horizon Presented by Nassim Haramein Part 1: The Untold Physics Chapter 5: Concept of Black Holes In order to understand the concept of atoms, planets, galaxies and stars as all having
Curved Spacetime III Einstein's field equations
Curved Spacetime III Einstein's field equations Dr. Naylor Note that in this lecture we will work in SI units: namely c 1 Last Week s class: Curved spacetime II Riemann curvature tensor: This is a tensor