On the Axioms of Causal Set Theory
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Symmetry and Gravity
universe Article Making a Quantum Universe: Symmetry and Gravity Houri Ziaeepour 1,2 1 Institut UTINAM, CNRS UMR 6213, Observatoire de Besançon, Université de Franche Compté, 41 bis ave. de l’Observatoire, BP 1615, 25010 Besançon, France; [email protected] or [email protected] 2 Mullard Space Science Laboratory, University College London, Holmbury St. Mary, Dorking GU5 6NT, UK Received: 05 September 2020; Accepted: 17 October 2020; Published: 23 October 2020 Abstract: So far, none of attempts to quantize gravity has led to a satisfactory model that not only describe gravity in the realm of a quantum world, but also its relation to elementary particles and other fundamental forces. Here, we outline the preliminary results for a model of quantum universe, in which gravity is fundamentally and by construction quantic. The model is based on three well motivated assumptions with compelling observational and theoretical evidence: quantum mechanics is valid at all scales; quantum systems are described by their symmetries; universe has infinite independent degrees of freedom. The last assumption means that the Hilbert space of the Universe has SUpN Ñ 8q – area preserving Diff.pS2q symmetry, which is parameterized by two angular variables. We show that, in the absence of a background spacetime, this Universe is trivial and static. Nonetheless, quantum fluctuations break the symmetry and divide the Universe to subsystems. When a subsystem is singled out as reference—observer—and another as clock, two more continuous parameters arise, which can be interpreted as distance and time. We identify the classical spacetime with parameter space of the Hilbert space of the Universe. -
What Can We Learn from Shape Dynamics? International Loop Quantum Gravity Seminar
What can we learn from shape dynamics? International Loop Quantum Gravity Seminar Tim A. Koslowski University of New Brunswick, Fredericton, NB, Canada November 12, 2013 Tim A. Koslowski (UNB) What can we learn from shape dynamics? November 12, 2013 1 / 19 Outline 1 Motivation from 2+1 diemsnional qunatum gravity to consider conformal evolution as fundamental 2 Conformal evolution is different from spacetime (i.e. abandon spacetime) 3 Generic dynamical emergence of spacetime in the presence of matter (i.e. regain spacetime) Tim A. Koslowski (UNB) What can we learn from shape dynamics? November 12, 2013 2 / 19 Introduction and Motivation Tim A. Koslowski (UNB) What can we learn from shape dynamics? November 12, 2013 3 / 19 Motivation Canonical metric path integral in 2+1 (only known metric path integral) ab p necessary: 2+1 split and CMC gauge condition gabπ − t g = 0 R 2 ab R ab a pπ c i dtd x(_gabπ −S(N)−H(ξ)) Z = [dgab][dπ ][dN][dξ ]δ[ g − t]δ[F ] det[FP ]e R 2 A R A i dtd x(_τAp −Vo(τ;p;t)) = [dτA][dp ]e [Carlip: CQG 12 (1995) 2201, Seriu PRD 55 (1997) 781] where: τA are Teichm¨ullerparameters, Vo(τ; p; t) denotes on-shell volume, which depends explicitly on time t ) QM on Teichm¨ullerspace, phys. Hamilt. Vo(τ; p; t) [Moncrief: JMP 30 (1989) 2907] Fradkin-Vilkovisky theorem: [cf. Henneaux/Teitelboim: \Quantization of Gauge Systems"] \Partition function depends on gauge fixing cond. only through the gauge equivalence class of gauge fixing conditions." for a discussion and some examples of non-equivalence [see Govaerts, Scholtz: J.Phys. -
Jhep09(2019)100
Published for SISSA by Springer Received: July 29, 2019 Accepted: September 5, 2019 Published: September 12, 2019 A link that matters: towards phenomenological tests of unimodular asymptotic safety JHEP09(2019)100 Gustavo P. de Brito,a;b Astrid Eichhornc;b and Antonio D. Pereirad;b aCentro Brasileiro de Pesquisas F´ısicas (CBPF), Rua Dr Xavier Sigaud 150, Urca, Rio de Janeiro, RJ, Brazil, CEP 22290-180 bInstitute for Theoretical Physics, University of Heidelberg, Philosophenweg 16, 69120 Heidelberg, Germany cCP3-Origins, University of Southern Denmark, Campusvej 55, DK-5230 Odense M, Denmark dInstituto de F´ısica, Universidade Federal Fluminense, Campus da Praia Vermelha, Av. Litor^anea s/n, 24210-346, Niter´oi,RJ, Brazil E-mail: [email protected], [email protected], [email protected] Abstract: Constraining quantum gravity from observations is a challenge. We expand on the idea that the interplay of quantum gravity with matter could be key to meeting this challenge. Thus, we set out to confront different potential candidates for quantum gravity | unimodular asymptotic safety, Weyl-squared gravity and asymptotically safe gravity | with constraints arising from demanding an ultraviolet complete Standard Model. Specif- ically, we show that within approximations, demanding that quantum gravity solves the Landau-pole problems in Abelian gauge couplings and Yukawa couplings strongly con- strains the viable gravitational parameter space. In the case of Weyl-squared gravity with a dimensionless gravitational coupling, we also investigate whether the gravitational con- tribution to beta functions in the matter sector calculated from functional Renormalization Group techniques is universal, by studying the dependence on the regulator, metric field parameterization and choice of gauge. -
Shape Dynamics
Shape Dynamics Tim A. Koslowski Abstract Barbour’s formulation of Mach’s principle requires a theory of gravity to implement local relativity of clocks, local relativity of rods and spatial covariance. It turns out that relativity of clocks and rods are mutually exclusive. General Relativity implements local relativity of clocks and spatial covariance, but not local relativity of rods. It is the purpose of this contribution to show how Shape Dynamics, a theory that is locally equivalent to General Relativity, implements local relativity of rods and spatial covariance and how a BRST formulation, which I call Doubly General Relativity, implements all of Barbour’s principles. 1 Introduction A reflection on Mach’s principle lead Barbour to postulate that rods and spatial frames of reference should be locally determined by a procedure that he calls “best matching,” while clocks should be locally determined by what he calls “objective change.” (For more, see [1].) More concretely, Barbour’s principles postulate lo- cal time reparametrization invariance, local spatial conformal invariance and spatial covariance. The best matching algorithm for spatial covariance and local spatial conformal invariance turns out to be equivalent to the imposition of linear diffeo- morphism and conformal constraints Z Z 3 ab 3 H(x) = d xp (Lx g)ab; C(r) = d xr p; (1) S S Tim A. Koslowski Perimeter Institute for Theoretical Physics, 31 Caroline St. N, Waterloo, Ontario, Canada New address: Department of Mathematics and Statistics, University of New Brunswick Fredericton, New Brunswick E3B 5A3, Canada e-mail: [email protected] 1 2 Tim A. -
Annual Report 2013 NARODOWE CENTRUM BADAŃ JĄDROWYCH NATIONAL CENTRE for NUCLEAR RESEARCH
Annual Report 2013 NARODOWE CENTRUM BADAŃ JĄDROWYCH NATIONAL CENTRE FOR NUCLEAR RESEARCH ANNUAL REPORT 2013 PL-05-400 Otwock-Świerk, POLAND tel.: 048 22 718 00 01 fax: 048 22 779 34 81 e-mail: [email protected] http://www.ncbj.gov.pl Editors: N. Keeley K. Kurek Cover design: S. Mirski Secretarial work and layout: G. Swiboda ISSN 2299-2960 Annual Report 2013 3 CONTENTS FOREWORD ............................................................................................................................................................ 5 I. GENERAL INFORMATION ................................................................................................... 7 1. LOCATIONS ...................................................................................................................... 7 2. MANAGEMENT OF THE INSTITUTE ............................................................................ 7 3. SCIENTIFIC COUNCIL ..................................................................................................... 8 4. MAIN RESEARCH ACTIVITIES ................................................................................... 11 5. SCIENTIFIC STAFF OF THE INSTITUTE .................................................................... 13 6. VISITING SCIENTISTS .................................................................................................. 15 7. PARTICIPATION IN NATIONAL CONSORTIA AND SCIENTIFIC NETWORKS .. 23 8. DEGREES ........................................................................................................................ -
Does Time Differ from Change? Philosophical Appraisal of the Problem of Time in Quantum Gravity and in Physics
Studies in History and Philosophy of Modern Physics 52 (2015) 48–54 Contents lists available at ScienceDirect Studies in History and Philosophy of Modern Physics journal homepage: www.elsevier.com/locate/shpsb Does time differ from change? Philosophical appraisal of the problem of time in quantum gravity and in physics Alexis de Saint-Ours Université Paris Diderot – CNRS, Laboratoire SPHERE, UMR 7219, Bâtiment Condorcet, case 7093, 5 rue Thomas Mann, 75205 Paris cedex 13, France article info abstract Article history: After reviewing the problem of time in Quantum Gravity, I compare from a philosophical perspective, Received 16 December 2013 both Carlo Rovelli's and Julian Barbour's (before Shape Dynamics) understanding of time in Quantum Received in revised form Gravity and in dynamics in general, trying to show that those two relational understandings of time 10 March 2015 differ. Rovelli argues that there is change without time and that time can be abstracted from any change Accepted 15 March 2015 whereas Barbour claims that some motions are better than others for constituting duration standards Available online 27 October 2015 To my father and that time is to be abstracted from all change in the universe. I conclude by a few remarks on Bergson's criticism of physics in the light of those debates trying to show that both Rovelli and Barbour Keywords: give surrationalist (as Bachelard understood it) answers to the critique of spatialized time in Physics. Time & 2015 Elsevier Ltd. All rights reserved. Change Barbour Rovelli Bergson Lautman When citing this paper, please use the full journal title Studies in History and Philosophy of Modern Physics 1. -
The Multiple Realizability of General Relativity in Quantum Gravity
The multiple realizability of general relativity in quantum gravity Rasmus Jaksland∗ Forthcoming in Synthese† Abstract Must a theory of quantum gravity have some truth to it if it can recover general rela- tivity in some limit of the theory? This paper answers this question in the negative by indicating that general relativity is multiply realizable in quantum gravity. The argu- ment is inspired by spacetime functionalism – multiple realizability being a central tenet of functionalism – and proceeds via three case studies: induced gravity, thermodynamic gravity, and entanglement gravity. In these, general relativity in the form of the Ein- stein field equations can be recovered from elements that are either manifestly multiply realizable or at least of the generic nature that is suggestive of functions. If general relativity, as argued here, can inherit this multiple realizability, then a theory of quantum gravity can recover general relativity while being completely wrong about the posited microstructure. As a consequence, the recovery of general relativity cannot serve as the ultimate arbiter that decides which theory of quantum gravity that is worthy of pursuit, even though it is of course not irrelevant either qua quantum gravity. Thus, the recovery of general relativity in string theory, for instance, does not guarantee that the stringy account of the world is on the right track; despite sentiments to the contrary among string theorists. Keywords quantum gravity, general relativity, spacetime functionalism, entanglement, emergent gravity, multiple realizability, string theory ∗Department of Philosophy and Religious Studies, NTNU – Norwegian University of Science and Technology, Trondheim, Norway. Email: [email protected] †This is a post-peer-review, pre-copyedit version of an article published in Synthese. -
Redalyc.Big Extra Dimensions Make a Too Small
Brazilian Journal of Physics ISSN: 0103-9733 [email protected] Sociedade Brasileira de Física Brasil Sorkin, Rafael D. Big extra dimensions make A too Small Brazilian Journal of Physics, vol. 35, núm. 2A, june, 2005, pp. 280-283 Sociedade Brasileira de Física Sâo Paulo, Brasil Available in: http://www.redalyc.org/articulo.oa?id=46435212 How to cite Complete issue Scientific Information System More information about this article Network of Scientific Journals from Latin America, the Caribbean, Spain and Portugal Journal's homepage in redalyc.org Non-profit academic project, developed under the open access initiative 280 Brazilian Journal of Physics, vol. 35, no. 2A, June, 2005 Big Extra Dimensions Make L too Small Rafael D. Sorkin Perimeter Institute, 31 Caroline Street North, Waterloo ON, N2L 2Y5 Canada and Department of Physics, Syracuse University, Syracuse, NY 13244-1130, U.S.A. Received on 23 February, 2005 I argue that the true quantum gravity scale cannot be much larger than the Planck length, because if it were then the quantum gravity-induced fluctuations in L would be insufficient to produce the observed cosmic “dark energy”. If one accepts this argument, it rules out scenarios of the “large extra dimensions” type. I also point out that the relation between the lower and higher dimensional gravitational constants in a Kaluza-Klein theory is precisely what is needed in order that a black hole’s entropy admit a consistent higher dimensional interpretation in terms of an underlying spatio-temporal discreteness. Probably few people anticipate that laboratory experiments in L far too small to be compatible with its observed value. -
What Is Time in Some Modern Physics Theories: Interpretation Problems
Ivan A. Karpenko WHAT IS TIME IN SOME MODERN PHYSICS THEORIES: INTERPRETATION PROBLEMS BASIC RESEARCH PROGRAM WORKING PAPERS SERIES: HUMANITIES WP BRP 124/HUM/2016 This Working Paper is an output of a research project implemented at the National Research University Higher School of Economics (HSE). Any opinions or claims contained in this Working Paper do not necessarily reflect the views of HSE. Ivan A. Karpenko1 WHAT IS TIME IN SOME MODERN PHYSICS THEORIES: INTERPRETATION PROBLEMS2 The article deals with the problem of time in the context of several theories of modern physics. This fundamental concept inevitably arises in physical theories, but so far there is no adequate description of it in the philosophy of science. In the theory of relativity, quantum field theory, Standard Model of particle physics, theory of loop quantum gravity, superstring theory and other most recent theories the idea of time is shown explicitly or not. Sometimes, such as in the special theory of relativity, it plays a significant role and sometimes it does not. But anyway it exists and is implied by the content of the theory, which in some cases directly includes its mathematical tools. Fundamental difference of space-time processes in microcosm and macrocosm is of particular importance for solving the problem. In this regard, a need to understand the time in the way it appears in modern physics, to describe it in the language of philosophy arises (satisfactory for time description mathematical tools also do not exist). This will give an opportunity to get closer to the answer on question of time characteristics. -
Manifoldlike Causal Sets
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by eGrove (Univ. of Mississippi) University of Mississippi eGrove Electronic Theses and Dissertations Graduate School 2019 Manifoldlike Causal Sets Miremad Aghili University of Mississippi Follow this and additional works at: https://egrove.olemiss.edu/etd Part of the Physics Commons Recommended Citation Aghili, Miremad, "Manifoldlike Causal Sets" (2019). Electronic Theses and Dissertations. 1529. https://egrove.olemiss.edu/etd/1529 This Dissertation is brought to you for free and open access by the Graduate School at eGrove. It has been accepted for inclusion in Electronic Theses and Dissertations by an authorized administrator of eGrove. For more information, please contact [email protected]. Manifoldlike Causal Sets A Dissertation presented in partial fulfillment of requirements for the degree of Doctor of Philosophy in the Department of Physics and Astronomy The University of Mississippi by Miremad Aghili May 2019 Copyright Miremad Aghili 2019 ALL RIGHTS RESERVED ABSTRACT The content of this dissertation is written in a way to answer the important question of manifoldlikeness of causal sets. This problem has importance in the sense that in the continuum limit and in the case one finds a formalism for the sum over histories, the result requires to be embeddable in a manifold to be able to reproduce General Relativity. In what follows I will use the distribution of path length in a causal set to assign a measure for manifoldlikeness of causal sets to eliminate the dominance of nonmanifoldlike causal sets. The distribution of interval sizes is also investigated as a way to find the discrete version of scalar curvature in causal sets in order to present a dynamics of gravitational fields. -
Dimension and Dimensional Reduction in Quantum Gravity
March 2019 Dimension and Dimensional Reduction in Quantum Gravity S. Carlip∗ Department of Physics University of California Davis, CA 95616 USA Abstract If gravity is asymptotically safe, operators will exhibit anomalous scaling at the ultraviolet fixed point in a way that makes the theory effectively two- dimensional. A number of independent lines of evidence, based on different approaches to quantization, indicate a similar short-distance dimensional reduction. I will review the evidence for this behavior, emphasizing the physical question of what one means by “dimension” in a quantum spacetime, and will dis- cuss possible mechanisms that could explain the universality of this phenomenon. For proceedings of the conference in honor of Martin Reuter: “Quantum Fields—From Fundamental Concepts to Phenomenological Questions” September 2018 arXiv:1904.04379v1 [gr-qc] 8 Apr 2019 ∗email: [email protected] 1. Introduction The asymptotic safety program offers a fascinating possibility for the quantization of gravity, starkly different from other, more common approaches, such as string theory and loop quantum gravity [1–3]. We don’t know whether quantum gravity can be described by an asymptotically safe (and unitary) field theory, but it might be. For “traditionalists” working on quantum gravity, this raises a fundamental question: What does asymptotic safety tell us about the small-scale structure of spacetime? So far, the most intriguing answer to this question involves the phenomenon of short-distance dimensional reduction. It seems nearly certain that, near a nontrivial ultraviolet fixed point, operators acquire large anomalous dimensions, in such a way that their effective dimensions are those of operators in a two-dimensional spacetime [4–6]. -
Arxiv:Gr-Qc/9510063V1 31 Oct 1995
STRUCTURAL ISSUES IN QUANTUM GRAVITYa C.J. Isham b Blackett Laboratory, Imperial College of Science, Technology and Medicine, South Kensington, London SW7 2BZ A discursive, non-technical, analysis is made of some of the basic issues that arise in almost any approach to quantum gravity, and of how these issues stand in relation to recent developments in the field. Specific topics include the applicability of the conceptual and mathematical structures of both classical general relativity and standard quantum theory. This discussion is preceded by a short history of the last twenty-five years of research in quantum gravity, and concludes with speculations on what a future theory might look like. 1 Introduction 1.1 Some Crucial Questions in Quantum Gravity In this lecture I wish to reflect on certain fundamental issues that can be expected to arise in almost all approaches to quantum gravity. As such, the talk is rather non-mathematical in nature—in particular, it is not meant to be a technical review of the who-has-been-doing-what-since-GR13 type: the subject has developed in too many different ways in recent years to make this option either feasible or desirable. The presentation is focussed around the following prima facie questions: 1. Why are we interested in quantum gravity at all? In the past, different researchers have had significantly different motivations for their work— and this has had a strong influence on the technical developments of the subject. arXiv:gr-qc/9510063v1 31 Oct 1995 2. What are the basic ways of trying to construct a quantum theory of gravity? For example, can general relativity be regarded as ‘just another field theory’ to be quantised in a more-or-less standard way, or does its basic structure demand something quite different? 3.