Analogue Gravity
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Universal Thermodynamics in the Context of Dynamical Black Hole
universe Article Universal Thermodynamics in the Context of Dynamical Black Hole Sudipto Bhattacharjee and Subenoy Chakraborty * Department of Mathematics, Jadavpur University, Kolkata 700032, West Bengal, India; [email protected] * Correspondence: [email protected] Received: 27 April 2018; Accepted: 22 June 2018; Published: 1 July 2018 Abstract: The present work is a brief review of the development of dynamical black holes from the geometric point view. Furthermore, in this context, universal thermodynamics in the FLRW model has been analyzed using the notion of the Kodama vector. Finally, some general conclusions have been drawn. Keywords: dynamical black hole; trapped surfaces; universal thermodynamics; unified first law 1. Introduction A black hole is a region of space-time from which all future directed null geodesics fail to reach the future null infinity I+. More specifically, the black hole region B of the space-time manifold M is the set of all events P that do not belong to the causal past of future null infinity, i.e., B = M − J−(I+). (1) Here, J−(I+) denotes the causal past of I+, i.e., it is the set of all points that causally precede I+. The boundary of the black hole region is termed as the event horizon (H), H = ¶B = ¶(J−(I+)). (2) A cross-section of the horizon is a 2D surface H(S) obtained by intersecting the event horizon with a space-like hypersurface S. As event the horizon is a causal boundary, it must be a null hypersurface generated by null geodesics that have no future end points. In the black hole region, there are trapped surfaces that are closed 2-surfaces (S) such that both ingoing and outgoing congruences of null geodesics are orthogonal to S, and the expansion scalar is negative everywhere on S. -
Dynamics of the Four Kinds of Trapping Horizons & Existence of Hawking
Dynamics of the four kinds of Trapping Horizons & Existence of Hawking Radiation Alexis Helou1 AstroParticule et Cosmologie, Universit´eParis Diderot, CNRS, CEA, Observatoire de Paris, Sorbonne Paris Cit´e Bˆatiment Condorcet, 10, rue Alice Domon et L´eonieDuquet, F-75205 Paris Cedex 13, France Abstract We work with the notion of apparent/trapping horizons for spherically symmetric, dynamical spacetimes: these are quasi-locally defined, simply based on the behaviour of congruence of light rays. We show that the sign of the dynamical Hayward-Kodama surface gravity is dictated by the in- ner/outer nature of the horizon. Using the tunneling method to compute Hawking Radiation, this surface gravity is then linked to a notion of temper- ature, up to a sign that is dictated by the future/past nature of the horizon. Therefore two sign effects are conspiring to give a positive temperature for the black hole case and the expanding cosmology, whereas the same quantity is negative for white holes and contracting cosmologies. This is consistent with the fact that, in the latter cases, the horizon does not act as a separating membrane, and Hawking emission should not occur. arXiv:1505.07371v1 [gr-qc] 27 May 2015 [email protected] Contents 1 Introduction 1 2 Foreword 2 3 Past Horizons: Retarded Eddington-Finkelstein metric 4 4 Future Horizons: Advanced Eddington-Finkelstein metric 10 5 Hawking Radiation from Tunneling 12 6 The four kinds of apparent/trapping horizons, and feasibility of Hawking radiation 14 6.1 Future-outer trapping horizon: black holes . 15 6.2 Past-inner trapping horizon: expanding cosmology . -
The Flexibility of Optical Metrics
Home Search Collections Journals About Contact us My IOPscience The flexibility of optical metrics This content has been downloaded from IOPscience. Please scroll down to see the full text. 2016 Class. Quantum Grav. 33 165008 (http://iopscience.iop.org/0264-9381/33/16/165008) View the table of contents for this issue, or go to the journal homepage for more Download details: IP Address: 128.220.159.5 This content was downloaded on 08/05/2017 at 21:52 Please note that terms and conditions apply. You may also be interested in: Induced optical metric in the non-impedance-matched media S A Mousavi, R Roknizadeh and S Sahebdivan Lux in obscuro: photon orbits of extremal black holes revisited Fech Scen Khoo and Yen Chin Ong Hidden geometries in nonlinear theories: a novel aspect of analogue gravity E Goulart, M Novello, F T Falciano et al. Black holes and stars in Horndeski theory Eugeny Babichev, Christos Charmousis and Antoine Lehébel Singularities in GR coupled to nonlinearelectrodynamics M Novello, S E Perez Bergliaffa and J M Salim Parity horizons in shape dynamics Gabriel Herczeg Numerical methods for finding stationary gravitational solutions Óscar J C Dias, Jorge E Santos and Benson Way Static spherically symmetric solutions in mimetic gravity: rotation curves and wormholes Ratbay Myrzakulov, Lorenzo Sebastiani, Sunny Vagnozzi et al. Supersymmetric solutions of N = (2, 0) topologically massive supergravity Nihat Sadik Deger and George Moutsopoulos Classical and Quantum Gravity Class. Quantum Grav. 33 (2016) 165008 (14pp) doi:10.1088/0264-9381/33/16/165008 -
Negative Frequency at the Horizon Theoretical Study and Experimental Realisation of Analogue Gravity Physics in Dispersive Optical Media Springer Theses
Springer Theses Recognizing Outstanding Ph.D. Research Maxime J. Jacquet Negative Frequency at the Horizon Theoretical Study and Experimental Realisation of Analogue Gravity Physics in Dispersive Optical Media Springer Theses Recognizing Outstanding Ph.D. Research Aims and Scope The series “Springer Theses” brings together a selection of the very best Ph.D. theses from around the world and across the physical sciences. Nominated and endorsed by two recognized specialists, each published volume has been selected for its scientific excellence and the high impact of its contents for the pertinent field of research. For greater accessibility to non-specialists, the published versions include an extended introduction, as well as a foreword by the student’s supervisor explaining the special relevance of the work for the field. As a whole, the series will provide a valuable resource both for newcomers to the research fields described, and for other scientists seeking detailed background information on special questions. Finally, it provides an accredited documentation of the valuable contributions made by today’s younger generation of scientists. Theses are accepted into the series by invited nomination only and must fulfill all of the following criteria • They must be written in good English. • The topic should fall within the confines of Chemistry, Physics, Earth Sciences, Engineering and related interdisciplinary fields such as Materials, Nanoscience, Chemical Engineering, Complex Systems and Biophysics. • The work reported in the thesis must represent a significant scientific advance. • If the thesis includes previously published material, permission to reproduce this must be gained from the respective copyright holder. • They must have been examined and passed during the 12 months prior to nomination. -
Phase Transition of Quantum-Corrected Schwarzschild Black Hole in Rainbow Gravity
Physics Letters B 784 (2018) 6–11 Contents lists available at ScienceDirect Physics Letters B www.elsevier.com/locate/physletb Phase transition of quantum-corrected Schwarzschild black hole in rainbow gravity Md. Shahjalal Department of Mathematics, Shahjalal University of Science and Technology, Sylhet-3114, Bangladesh a r t i c l e i n f o a b s t r a c t Article history: The thermodynamic phase transition of Schwarzschild black hole, after employing a quantum correction Received 30 May 2018 to the space–time metric, in the gravity’s rainbow is explored. The rainbow gravity-inspired Hawking Received in revised form 15 July 2018 temperature of the quantum-corrected rainbow Schwarzschild black hole is calculated initially, and then Accepted 16 July 2018 the entropy, the local temperature, and the local energy of the black hole in an isothermal cavity Available online 20 July 2018 are derived. The off-shell free energy is calculated to further investigate the critical behavior, the Editor: B. Grinstein thermodynamic stability, and the phase transition of the black hole. It is evident that the rainbow gravity Keywords: determines the late fate of the black hole as leading to a remnant, the findings of this letter also show Rainbow gravity that a quantum correction to the metric reduces the remnant mass of the Schwarzschild black hole in Black hole thermodynamics comparison with the usual rainbow Schwarzschild black hole. Phase transition © 2018 The Author(s). Published by Elsevier B.V. This is an open access article under the CC BY license (http://creativecommons.org/licenses/by/4.0/). -
Light Rays, Singularities, and All That
Light Rays, Singularities, and All That Edward Witten School of Natural Sciences, Institute for Advanced Study Einstein Drive, Princeton, NJ 08540 USA Abstract This article is an introduction to causal properties of General Relativity. Topics include the Raychaudhuri equation, singularity theorems of Penrose and Hawking, the black hole area theorem, topological censorship, and the Gao-Wald theorem. The article is based on lectures at the 2018 summer program Prospects in Theoretical Physics at the Institute for Advanced Study, and also at the 2020 New Zealand Mathematical Research Institute summer school in Nelson, New Zealand. Contents 1 Introduction 3 2 Causal Paths 4 3 Globally Hyperbolic Spacetimes 11 3.1 Definition . 11 3.2 Some Properties of Globally Hyperbolic Spacetimes . 15 3.3 More On Compactness . 18 3.4 Cauchy Horizons . 21 3.5 Causality Conditions . 23 3.6 Maximal Extensions . 24 4 Geodesics and Focal Points 25 4.1 The Riemannian Case . 25 4.2 Lorentz Signature Analog . 28 4.3 Raychaudhuri’s Equation . 31 4.4 Hawking’s Big Bang Singularity Theorem . 35 5 Null Geodesics and Penrose’s Theorem 37 5.1 Promptness . 37 5.2 Promptness And Focal Points . 40 5.3 More On The Boundary Of The Future . 46 1 5.4 The Null Raychaudhuri Equation . 47 5.5 Trapped Surfaces . 52 5.6 Penrose’s Theorem . 54 6 Black Holes 58 6.1 Cosmic Censorship . 58 6.2 The Black Hole Region . 60 6.3 The Horizon And Its Generators . 63 7 Some Additional Topics 66 7.1 Topological Censorship . 67 7.2 The Averaged Null Energy Condition . -
Arxiv:Gr-Qc/0304042V1 9 Apr 2003
Do black holes radiate? Adam D Helfer Department of Mathematics, Mathematical Sciences Building, University of Missouri, Columbia, Missouri 65211, U.S.A. Abstract. The prediction that black holes radiate due to quantum effects is often considered one of the most secure in quantum field theory in curved space–time. Yet this prediction rests on two dubious assumptions: that ordinary physics may be applied to vacuum fluctuations at energy scales increasing exponentially without bound; and that quantum–gravitational effects may be neglected. Various suggestions have been put forward to address these issues: that they might be explained away by lessons from sonic black hole models; that the prediction is indeed successfully reproduced by quantum gravity; that the success of the link provided by the prediction between black holes and thermodynamics justifies the prediction. This paper explains the nature of the difficulties, and reviews the proposals that have been put forward to deal with them. None of the proposals put forward can so far be considered to be really successful, and simple dimensional arguments show that quantum–gravitational effects might well alter the evaporation process outlined by Hawking. arXiv:gr-qc/0304042v1 9 Apr 2003 Thus a definitive theoretical treatment will require an understanding of quantum gravity in at least some regimes. Until then, no compelling theoretical case for or against radiation by black holes is likely to be made. The possibility that non–radiating “mini” black holes exist should be taken seriously; such holes could be part of the dark matter in the Universe. Attempts to place observational limits on the number of “mini” black holes (independent of the assumption that they radiate) would be most welcome. -
Field Theory Aspects of Cosmology and Black Holes
FIELD THEORY ASPECTS OF COSMOLOGY AND BLACK HOLES Thesis submitted for the degree of Doctor of Philosophy (Science) of Jadavpur University, Kolkata August 2009 arXiv:1011.6570v1 [hep-th] 30 Nov 2010 Kulkarni Shailesh Gajanan Satyendra Nath Bose National Centre for Basic Sciences JD Block, Sector 3, Salt Lake, Kolkata 700098, India Certificate from the supervisor This is to certify that the thesis entitled \Field theory aspects of cosmology and black holes" submitted by Sri. Kulkarni Shailesh Gajanan, who got his name registered on October 8, 2007 for the award of Ph.D. (Science) degree of Jadavpur University, is absolutely based upon his own work under the supervision of Professor Rabin Banerjee at S.N. Bose National Centre for Basic Sciences, Kolkata, India, and that neither this thesis nor any part of it has been submitted for any degree/diploma or any other academic award anywhere before. Rabin Banerjee Professor S.N. Bose National Centre for Basic Sciences JD Block, Sector 3, Salt Lake Kolkata 700098, India TO MY MOT HER Acknowledgements This thesis is the culminative outcome of five years work, which has been made possible by the blessings and support of many individuals. I take this opportunity to express my sincere gratitude to all of them. First and foremost, I would like to thank Prof. Rabin Banerjee, my thesis supervisor. His uncanny ability to select a particular problem, a keen and strategic analysis of it and deep involvement among the students makes him something special. Thank you Sir for giving me all that could last my entire life. -
New Journal of Physics the Open–Access Journal for Physics
New Journal of Physics The open–access journal for physics Relativistic Bose–Einstein condensates: a new system for analogue models of gravity S Fagnocchi1,2, S Finazzi1,2,3, S Liberati1,2, M Kormos1,2 and A Trombettoni1,2 1 SISSA via Beirut 2-4, I-34151 Trieste, Italy 2 INFN, Sezione di Trieste, Italy E-mail: [email protected], fi[email protected], [email protected], [email protected] and [email protected] New Journal of Physics 12 (2010) 095012 (19pp) Received 20 January 2010 Published 30 September 2010 Online at http://www.njp.org/ doi:10.1088/1367-2630/12/9/095012 Abstract. In this paper we propose to apply the analogy between gravity and condensed matter physics to relativistic Bose—Einstein condensates (RBECs), i.e. condensates composed by relativistic constituents. While such systems are not yet a subject of experimental realization, they do provide us with a very rich analogue model of gravity, characterized by several novel features with respect to their non-relativistic counterpart. Relativistic condensates exhibit two (rather than one) quasi-particle excitations, a massless and a massive one, the latter disappearing in the non-relativistic limit. We show that the metric associated with the massless mode is a generalization of the usual acoustic geometry allowing also for non-conformally flat spatial sections. This is relevant, as it implies that these systems can allow the simulation of a wider variety of geometries. Finally, while in non-RBECs the transition is from Lorentzian to Galilean relativity, these systems represent an emergent gravity toy model where Lorentz symmetry is present (albeit with different limit speeds) at both low and high energies. -
Observation of Quantum Hawking Radiation and Its Entanglement in an Analogue Black Hole
ARTICLES PUBLISHED ONLINE: 15 AUGUST 2016 | DOI: 10.1038/NPHYS3863 Observation of quantum Hawking radiation and its entanglement in an analogue black hole Je Steinhauer We observe spontaneous Hawking radiation, stimulated by quantum vacuum fluctuations, emanating from an analogue black hole in an atomic Bose–Einstein condensate. Correlations are observed between the Hawking particles outside the black hole and the partner particles inside. These correlations indicate an approximately thermal distribution of Hawking radiation. We find that the high-energy pairs are entangled, while the low-energy pairs are not, within the reasonable assumption that excitations with dierent frequencies are not correlated. The entanglement verifies the quantum nature of the Hawking radiation. The results are consistent with a driven oscillation experiment and a numerical simulation. ifty years ago, Bekenstein discovered the field of black hole where n.x/ is the one-dimensional (1D) density of the condensate 1 thermodynamics . This field has vast and deep implications, forming the black hole, and nout and nin are the average densities far beyond the physics of black holes themselves. The most outside and inside the black hole, respectively. The positionp x is F 2,3 important prediction of the field is that of Hawking radiation . By in units of the shortest length scale of the condensate ξ ≡ ξoutξin, making an approximation to the still-unknown laws of quantum where ξout and ξin are the healing lengths outside and inside the gravity, Hawking predicted that the horizon of the black hole should black hole, respectively, and ξi D hN=mci, where ci is the speed emit a thermal distribution of particles. -
Gravity As an Emergent Phenomenon: Fundamentals and Applications
Gravity as an emergent phenomenon: fundamentals and applications Ra´ulCarballo Rubio Universidad de Granada Programa de Doctorado en F´ısicay Matem´aticas Escuela de Doctorado de Ciencias, Tecnolog´ıase Ingenier´ıas Granada, 2016 Editor: Universidad de Granada. Tesis Doctorales Autor: Raúl Carballo Rubio ISBN: 978-84-9125-879-7 URI: http://hdl.handle.net/10481/43711 Gravity as an emergent phenomenon: fundamentals and applications Ra´ulCarballo Rubio1 In Partial Fulfillment of the Requirements for the Degree of Doctor of Philosophy Under the supervision of: Carlos Barcel´oSer´on1 Luis Javier Garay Elizondo2;3 1 Instituto de Astrof´ısicade Andaluc´ıa(IAA-CSIC), Glorieta de la Astronom´ıa,18008 Granada, Spain 2 Departamento de F´ısicaTe´oricaII, Universidad Complutense de Madrid, 28040 Madrid, Spain 3 Instituto de Estructura de la Materia (IEM-CSIC), Serrano 121, 28006 Madrid, Spain Consejo Superior de Investigaciones Cient´ıficas Estructuraci´onde contenidos en la memoria Los contenidos exigidos en una tesis doctoral en la Universidad de Granada para los pro- gramas de doctorado regulados por el RD99/2011 se encuentran en la presente memoria estructurados en las siguientes secciones: T´ıtulo Portada Compromiso de respeto de derechos de autor Compromiso de respeto de derechos de autor Resumen Resumen Introducci´on Introduction Objetivos Introduction, Secs. 1.1, 2.1, 3.1 and 4.1 Metodolog´ıa Secs. 1.2, 1.3, 2.2, 4.2, 4.3 and 4.4 Resultados Secs. 1.4, 1.5, 1.6, 2.3, 2.4, 2.5, 3.2, 3.3, 4.5 and 4.6 Conclusiones Secs. 1.7, 2.6, 3.4 and 4.7; Main conclusions and future directions Bibliograf´ıa Bibliography Resumen En esta tesis se ha realizado un estudio de distintos aspectos de la aproximaci´ona la construcci´onde una teor´ıade gravedad cu´antica conocida como gravedad emergente, con el objetivo de analizar preguntas fundamentales en el marco de este programa de investi- gaci´on,as´ıcomo posibles aplicaciones a problemas actuales de la f´ısicate´oricagravitacional. -
Quantum Wave Mechanics 3Rd Ed
Geometrical description of photons, electrons and composite particles. Dimensional analysis of electrical charge. Quantum gravity, gravitational frequency spectrum, mass oscillator synchronization, spectral energy density modulation and phase conjugation. Origin of charge, fine structure constant and inertia. Prospects for wave-based EM propulsion. Quantum Wave Mechanics by Larry Reed Order the complete book from the publisher Booklocker.com https://www.booklocker.com/p/books/10176.html?s=pdf or from your favorite neighborhood or online bookstore. To my parents who never knew the result of their great experiment Copyright © 2019, 2020 by Larry J. Reed All rights reserved. No part of this publication may be reproduced, stored in a retrieval system, or transmitted in any form or by any means, electronic, mechanical, recording or otherwise, without the prior written permission of the author. Printed on acid-free paper. Library of Congress Control Number: 2018901065 ISBN: 978-1-63492-964-6 paperback To order additional copies of this book, contact: www.booklocker.com CONTENTS Preface ........................................................................................................................... ix SECTION 1 – LIGHT 1. Photon model ................................................................................................................. 1 2. Quantum vacuum ......................................................................................................... 13 3. Electromagnetic 4-Potential .......................................................................................