Appendix: a Simple Numerical Toy Model
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Toy Models for Black Hole Evaporation
UCSBTH-92-36 hep-th/9209113 Toy Models for Black Hole Evaporation∗ Steven B. Giddings† Department of Physics University of California Santa Barbara, CA 93106-9530 Abstract These notes first present a brief summary of the puzzle of information loss to black holes, of its proposed resolutions, and of the flaws in the proposed resolutions. There follows a review of recent attempts to attack this problem, and other issues in black hole physics, using two-dimensional dilaton gravity theories as toy models. These toy models contain collapsing black holes and have for the first time enabled an explicit semiclassical treatment of the backreaction of the Hawking radiation on the geometry of an evaporating black hole. However, a complete answer to the information conundrum seems to require physics beyond the semiclassical approximation. Preliminary attempts to make progress arXiv:hep-th/9209113v2 11 Nov 1992 in this direction, using connections to conformal field theory, are described. *To appear in the proceedings of the International Workshop of Theoretical Physics, 6th Session, String Quantum Gravity and Physics at the Planck Energy Scale, 21 – 28 June 1992, Erice, Italy. † Email addresses: [email protected], [email protected]. Since the discovery of black holes, physicists have been faced with the possibility that they engender a breakdown of predictability. At the classical level this breakdown arises at the singularity. Classically we do not know how to evolve past it. Inclusion of quantum effects may serve as a remedy, allowing predictable evolution, by smoothing out the singularities of general relativity. However, as suggested by Hawking [1,2], quantum effects also present another sharp challenge to predictability through the mechanism of Hawking evaporation. -
Quantum Vacuum Energy Density and Unifying Perspectives Between Gravity and Quantum Behaviour of Matter
Annales de la Fondation Louis de Broglie, Volume 42, numéro 2, 2017 251 Quantum vacuum energy density and unifying perspectives between gravity and quantum behaviour of matter Davide Fiscalettia, Amrit Sorlib aSpaceLife Institute, S. Lorenzo in Campo (PU), Italy corresponding author, email: [email protected] bSpaceLife Institute, S. Lorenzo in Campo (PU), Italy Foundations of Physics Institute, Idrija, Slovenia email: [email protected] ABSTRACT. A model of a three-dimensional quantum vacuum based on Planck energy density as a universal property of a granular space is suggested. This model introduces the possibility to interpret gravity and the quantum behaviour of matter as two different aspects of the same origin. The change of the quantum vacuum energy density can be considered as the fundamental medium which determines a bridge between gravity and the quantum behaviour, leading to new interest- ing perspectives about the problem of unifying gravity with quantum theory. PACS numbers: 04. ; 04.20-q ; 04.50.Kd ; 04.60.-m. Key words: general relativity, three-dimensional space, quantum vac- uum energy density, quantum mechanics, generalized Klein-Gordon equation for the quantum vacuum energy density, generalized Dirac equation for the quantum vacuum energy density. 1 Introduction The standard interpretation of phenomena in gravitational fields is in terms of a fundamentally curved space-time. However, this approach leads to well known problems if one aims to find a unifying picture which takes into account some basic aspects of the quantum theory. For this reason, several authors advocated different ways in order to treat gravitational interaction, in which the space-time manifold can be considered as an emergence of the deepest processes situated at the fundamental level of quantum gravity. -
Spacetime Geometry from Graviton Condensation: a New Perspective on Black Holes
Spacetime Geometry from Graviton Condensation: A new Perspective on Black Holes Sophia Zielinski née Müller München 2015 Spacetime Geometry from Graviton Condensation: A new Perspective on Black Holes Sophia Zielinski née Müller Dissertation an der Fakultät für Physik der Ludwig–Maximilians–Universität München vorgelegt von Sophia Zielinski geb. Müller aus Stuttgart München, den 18. Dezember 2015 Erstgutachter: Prof. Dr. Stefan Hofmann Zweitgutachter: Prof. Dr. Georgi Dvali Tag der mündlichen Prüfung: 13. April 2016 Contents Zusammenfassung ix Abstract xi Introduction 1 Naturalness problems . .1 The hierarchy problem . .1 The strong CP problem . .2 The cosmological constant problem . .3 Problems of gravity ... .3 ... in the UV . .4 ... in the IR and in general . .5 Outline . .7 I The classical description of spacetime geometry 9 1 The problem of singularities 11 1.1 Singularities in GR vs. other gauge theories . 11 1.2 Defining spacetime singularities . 12 1.3 On the singularity theorems . 13 1.3.1 Energy conditions and the Raychaudhuri equation . 13 1.3.2 Causality conditions . 15 1.3.3 Initial and boundary conditions . 16 1.3.4 Outlining the proof of the Hawking-Penrose theorem . 16 1.3.5 Discussion on the Hawking-Penrose theorem . 17 1.4 Limitations of singularity forecasts . 17 2 Towards a quantum theoretical probing of classical black holes 19 2.1 Defining quantum mechanical singularities . 19 2.1.1 Checking for quantum mechanical singularities in an example spacetime . 21 2.2 Extending the singularity analysis to quantum field theory . 22 2.2.1 Schrödinger representation of quantum field theory . 23 2.2.2 Quantum field probes of black hole singularities . -
Closed Timelike Curves, Singularities and Causality: a Survey from Gödel to Chronological Protection
Closed Timelike Curves, Singularities and Causality: A Survey from Gödel to Chronological Protection Jean-Pierre Luminet Aix-Marseille Université, CNRS, Laboratoire d’Astrophysique de Marseille , France; Centre de Physique Théorique de Marseille (France) Observatoire de Paris, LUTH (France) [email protected] Abstract: I give a historical survey of the discussions about the existence of closed timelike curves in general relativistic models of the universe, opening the physical possibility of time travel in the past, as first recognized by K. Gödel in his rotating universe model of 1949. I emphasize that journeying into the past is intimately linked to spacetime models devoid of timelike singularities. Since such singularities arise as an inevitable consequence of the equations of general relativity given physically reasonable assumptions, time travel in the past becomes possible only when one or another of these assumptions is violated. It is the case with wormhole-type solutions. S. Hawking and other authors have tried to save the paradoxical consequences of time travel in the past by advocating physical mechanisms of chronological protection; however, such mechanisms remain presently unknown, even when quantum fluctuations near horizons are taken into account. I close the survey by a brief and pedestrian discussion of Causal Dynamical Triangulations, an approach to quantum gravity in which causality plays a seminal role. Keywords: time travel; closed timelike curves; singularities; wormholes; Gödel’s universe; chronological protection; causal dynamical triangulations 1. Introduction In 1949, the mathematician and logician Kurt Gödel, who had previously demonstrated the incompleteness theorems that broke ground in logic, mathematics, and philosophy, became interested in the theory of general relativity of Albert Einstein, of which he became a close colleague at the Institute for Advanced Study at Princeton. -
Black Holes and Gravitational Waves in Models of Minicharged Dark Matter
Home Search Collections Journals About Contact us My IOPscience Black holes and gravitational waves in models of minicharged dark matter This content has been downloaded from IOPscience. Please scroll down to see the full text. JCAP05(2016)054 (http://iopscience.iop.org/1475-7516/2016/05/054) View the table of contents for this issue, or go to the journal homepage for more Download details: IP Address: 62.210.105.116 This content was downloaded on 28/06/2016 at 17:13 Please note that terms and conditions apply. ournal of Cosmology and Astroparticle Physics JAn IOP and SISSA journal Black holes and gravitational waves in models of minicharged dark matter JCAP05(2016)054 Vitor Cardoso,a;b Caio F.B. Macedo,a Paolo Pania;c and Valeria Ferraric aCENTRA, Departamento de F´ısica,Instituto Superior T´ecnico| IST, Universidade de Lisboa | UL, Avenida Rovisco Pais 1, 1049 Lisboa, Portugal bPerimeter Institute for Theoretical Physics, 31 Caroline Street North Waterloo, Ontario N2L 2Y5, Canada cDipartimento di Fisica, \Sapienza" Universit`adi Roma and Sezione INFN Roma1, Piazzale A. Moro 5, 00185, Roma, Italy E-mail: [email protected], [email protected], [email protected], [email protected] Received April 29, 2016 Revised May 16, 2016 Accepted May 17, 2016 Published May 23, 2016 Abstract. In viable models of minicharged dark matter, astrophysical black holes might be charged under a hidden U(1) symmetry and are formally described by the same Kerr- Newman solution of Einstein-Maxwell theory. These objects are unique probes of minicharged dark matter and dark photons. -
Quantum Time Machines Are Expectation Values of the Scalar field Squared and Stress- Quantum-Mechanically Stable
Quantum time machine Pedro F. Gonz´alez-D´ıaz Centro de F´ısica “Miguel Catal´an”, Instituto de Matem´aticas y F´ısica Fundamental, Consejo Superior de Investigaciones Cient´ıficas, Serrano 121, 28006 Madrid (SPAIN) (December 6, 1997) The continuation of Misner space into the Euclidean region is seen to imply the topological re- striction that the period of the closed spatial direction becomes time-dependent. This restriction results in a modified Lorentzian Misner space in which the renormalized stress-energy tensor for quantized complex massless scalar fields becomes regular everywhere, even on the chronology hori- zon. A quantum-mechanically stable time machine with just the sub-microscopic size may then be constructed out of the modified Misner space, for which the semiclassical Hawking’s chronology protection conjecture is no longer an obstruction. PACS number(s): 04.20.Gz, 04.62.+v I. INTRODUCTION some attempts intended to violate it [14,15], this con- jecture has survived rather forcefully [16]. However, the After the seminal papers by Morris, Thorne and Yurt- realm where chronology protection holds is semiclassical sever [1], the notion of a time machine has jumped from physics, as it is for all hitherto proposed time machines. the pages of science fiction books to those of scientific Actually, because spacetime foam [17] must entail strong journals, giving rise to a recent influx of papers [2-7] violations of causal locality everywhere, one would expect and books [8,9] on the subject. Several potentially use- the Hawking’s conjecture to be inapplicable in the frame- ful models for time machines have since been proposed, work of quantum gravity proper, and that the divergences including the wormhole of Thorne et al. -
Asymptotically Flat Boundary Conditions for the U(1)3 Model for Euclidean Quantum Gravity
universe Article Asymptotically Flat Boundary Conditions for the U(1)3 Model for Euclidean Quantum Gravity Sepideh Bakhoda 1,2,* , Hossein Shojaie 1 and Thomas Thiemann 2,* 1 Department of Physics, Shahid Beheshti University, Tehran 1983969411, Iran; [email protected] 2 Institute for Quantum Gravity, FAU Erlangen—Nürnberg, Staudtstraße 7, 91058 Erlangen, Germany * Correspondence: [email protected] (S.B.); [email protected] (T.T.) 3 Abstract: A generally covariant U(1) gauge theory describing the GN ! 0 limit of Euclidean general relativity is an interesting test laboratory for general relativity, specially because the algebra of the Hamiltonian and diffeomorphism constraints of this limit is isomorphic to the algebra of the corresponding constraints in general relativity. In the present work, we the study boundary conditions and asymptotic symmetries of the U(1)3 model and show that while asymptotic spacetime translations admit well-defined generators, boosts and rotations do not. Comparing with Euclidean general relativity, one finds that the non-Abelian part of the SU(2) Gauss constraint, which is absent in the U(1)3 model, plays a crucial role in obtaining boost and rotation generators. Keywords: asymptotically flat boundary conditions; classical and quantum gravity; U(1)3 model; asymptotic charges Citation: Bakhoda, S.; Shojaie, H.; 1. Introduction Thiemann, T. Asymptotically Flat In the framework of the Ashtekar variables in terms of which General Relativity (GR) Boundary Conditions for the U(1)3 is formulated as a SU(2) gauge theory [1–3], attempts to find an operator corresponding to Model for Euclidean Quantum the Hamiltonian constraint of the Lorentzian vacuum canonical GR led to the result [4] that Gravity. -
Quantum Fluctuations and Thermodynamic Processes in The
Quantum fluctuations and thermodynamic processes in the presence of closed timelike curves by Tsunefumi Tanaka A thesis submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy in Physics Montana State University © Copyright by Tsunefumi Tanaka (1997) Abstract: A closed timelike curve (CTC) is a closed loop in spacetime whose tangent vector is everywhere timelike. A spacetime which contains CTC’s will allow time travel. One of these spacetimes is Grant space. It can be constructed from Minkowski space by imposing periodic boundary conditions in spatial directions and making the boundaries move toward each other. If Hawking’s chronology protection conjecture is correct, there must be a physical mechanism preventing the formation of CTC’s. Currently the most promising candidate for the chronology protection mechanism is the back reaction of the metric to quantum vacuum fluctuations. In this thesis the quantum fluctuations for a massive scalar field, a self-interacting field, and for a field at nonzero temperature are calculated in Grant space. The stress-energy tensor is found to remain finite everywhere in Grant space for the massive scalar field with sufficiently large field mass. Otherwise it diverges on chronology horizons like the stress-energy tensor for a massless scalar field. If CTC’s exist they will have profound effects on physical processes. Causality can be protected even in the presence of CTC’s if the self-consistency condition is imposed on all processes. Simple classical thermodynamic processes of a box filled with ideal gas in the presence of CTC’s are studied. If a system of boxes is closed, its state does not change as it travels through a region of spacetime with CTC’s. -
"What Is Space?" by Frank Wilczek
What is Space? 30 ) wilczek mit physics annual 2009 by Frank Wilczek hat is space: An empty stage, where the physical world of matter acts W out its drama; an equal participant, that both provides background and has a life of its own; or the primary reality, of which matter is a secondary manifestation? Views on this question have evolved, and several times changed radically, over the history of science. Today, the third view is triumphant. Where our eyes see nothing our brains, pondering the revelations of sharply tuned experi- ments, discover the Grid that powers physical reality. Many loose ends remain in today’s best world-models, and some big myster- ies. Clearly the last word has not been spoken. But we know a lot, too—enough, I think, to draw some surprising conclusions that go beyond piecemeal facts. They address, and offer some answers to, questions that have traditionally been regarded as belonging to philosophy, or even theology. A Brief History of Space Debate about the emptiness of space goes back to the prehistory of modern science, at least to the ancient Greek philosophers. Aristotle wrote that “Nature abhors a vacuum,” while his opponents the atomists held, in the words of their poet Lucretius, that All nature, then, as self-sustained, consists Of twain of things: of bodies and of void In which they’re set, and where they’re moved around. At the beginning of the seventeenth century, at the dawn of the Scientific Revolution, that great debate resumed. René Descartes proposed to ground the scientific description of the natural world solely on what he called primary qualities: extension (essentially, shape) and motion. -
The Quantum Physics of Chronology Protection
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by CERN Document Server The quantum physics of chronology protection Matt Visser Physics Department, Washington University, Saint Louis, Missouri 63130-4899, USA. 2 April 2002; LATEX-ed April 8, 2002 Abstract: This is a brief survey of the current status of Stephen Hawking’s “chronol- ogy protection conjecture”. That is: “Why does nature abhor a time machine?” I’ll discuss a few examples of spacetimes containing “time ma- chines” (closed causal curves), the sorts of peculiarities that arise, and the reactions of the physics community. While pointing out other possibilities, this article concentrates on the possibility of “chronology protection”. As Stephen puts it: It seems that there is a Chronology Protection Agency which prevents the appearance of closed timelike curves and so makes the universe safe for historians. To appear in: The future of theoretical physics and cosmology; Proceedings of the conference held in honour of Stephen Hawking on the occasion of his 60’th birthday. (Cambridge, 7–10 January 2002.) E-mail: [email protected] Homepage: http://www.physics.wustl.edu/~visser Archive: gr-qc/0204022 Permanent address after 1 July 2002: School of Mathematics and Computer Science, Victoria University, PO Box 600, Wellington, New Zealand. [email protected] 1 The quantum physics of chronology protection Simply put, chronology protection is the assertion that nature abhors a time machine. In the words of Stephen Hawking [1]: It seems that there is a Chronology Protection Agency which prevents the appearance of closed timelike curves and so makes the universe safe for historians. -
Parallel Worlds
www.Ael.af Kaku_0385509863_4p_all_r1.qxd 10/27/04 7:07 AM Page i PARALLEL WORLDS www.Ael.af Kaku_0385509863_4p_all_r1.qxd 10/27/04 7:07 AM Page ii www.Ael.af Kaku_0385509863_4p_all_r1.qxd 10/27/04 7:07 AM Page iii Also by Michio Kaku Beyond Einstein Hyperspace Visions Einstein’s Cosmos www.Ael.af Kaku_0385509863_4p_all_r1.qxd 10/27/04 7:07 AM Page iv MICHIO KAKU DOUBLEDAY New York London Toronto Sydney Auckland www.Ael.af Kaku_0385509863_4p_all_r1.qxd 10/27/04 7:07 AM Page v PARALLEL WORLDS A JOURNEY THROUGH CREATION, HIGHER DIMENSIONS, AND THE FUTURE OF THE COSMOS www.Ael.af Kaku_0385509863_4p_all_r1.qxd 10/27/04 7:07 AM Page vi published by doubleday a division of Random House, Inc. doubleday and the portrayal of an anchor with a dolphin are regis- tered trademarks of Random House, Inc. Book design by Nicola Ferguson Illustrations by Hadel Studio Library of Congress Cataloging-in-Publication Data Kaku, Michio. Parallel worlds : a journey through creation, higher dimensions, and the future of the cosmos/Michio Kaku.—1st ed. p. cm. Includes bibliographical references 1. Cosmology. 2. Big bang theory. 3. Superstring theories. 4. Supergravity. I. Title. QB981.K134 2004 523.1—dc22 2004056039 eISBN 0-385-51416-6 Copyright © 2005 Michio Kaku All Rights Reserved v1.0 www.Ael.af Kaku_0385509863_4p_all_r1.qxd 10/27/04 7:07 AM Page vii This book is dedicated to my loving wife, Shizue. www.Ael.af Kaku_0385509863_4p_all_r1.qxd 10/27/04 7:07 AM Page viii www.Ael.af Kaku_0385509863_4p_all_r1.qxd 10/27/04 7:07 AM Page ix CONTENTS acknowledgments xi -
Scrambling and Decoding the Charged Quantum Information
Scrambling and decoding the charged quantum information Junyu Liua;b aWalter Burke Institute for Theoretical Physics, California Institute of Technology, Pasadena, California 91125, USA bInstitute for Quantum Information and Matter, California Institute of Technology, Pasadena, California 91125, USA Abstract: Some deep conjectures about quantum gravity are closely related to the role of symmetries in the gravitational background, especially for quantum black holes. In this paper, we systematically study the theory of quantum information for a charged, chaotic system. We show how the quantum information in the whole system has been represented by its charge sectors, using the theory of quantum chaos and quantum error correction, with concrete examples in the context of the complex SYK model. We discuss possible implications for black hole thought experiments and conjectures about quantum gravity in the dynamical setup. We believe this work will have poten- tial applications from theories of quantum gravity to quantum simulation in quantum devices. arXiv:2003.11425v3 [quant-ph] 13 Oct 2020 Contents 1 Overview1 2 Preliminaries4 3 Chaos 13 3.1 Form factor 14 3.1.1 General result 14 3.1.2 Haar randomness 16 3.2 OTOCs 16 3.2.1 General result 16 3.2.2 Haar randomness 18 3.2.3 k-invariant subspace 19 3.3 Frame potential 21 3.3.1 General result 21 3.3.2 Haar randomness 22 3.3.3 k-invariant subspace 23 3.4 Decoupling 24 4 Example: the complex SYK model 26 5 Codes 30 5.1 Quantum error correction for the Haar randomness 31 5.2 Error correction in