Renormalization and Coarse-Graining of Loop Quantum Gravity Christoph Charles

Total Page:16

File Type:pdf, Size:1020Kb

Renormalization and Coarse-Graining of Loop Quantum Gravity Christoph Charles Renormalization and Coarse-graining of Loop Quantum Gravity Christoph Charles To cite this version: Christoph Charles. Renormalization and Coarse-graining of Loop Quantum Gravity. General Rela- tivity and Quantum Cosmology [gr-qc]. Université de Lyon, 2016. English. NNT : 2016LYSEN053. tel-01429887 HAL Id: tel-01429887 https://tel.archives-ouvertes.fr/tel-01429887 Submitted on 9 Jan 2017 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Numéro National de Thèse : 2016LYSEN053 THESE de DOCTORAT DE L’UNIVERSITE DE LYON opérée par l’Ecole Normale Supérieure de Lyon Ecole Doctorale N° 52 Physique et astrophysique de Lyon Discipline : Physique Soutenue publiquement le 25/11/2016, par : Christoph CHARLES Renormalization and Coarse-graining of Loop Quantum Gravity Renormalisation et coarse-graining de la gravitation quantique à boucle Devant le jury composé de : Noui, Karim Maître de conférences Université de Tours Rapporteur Dittrich, Bianca Faculty member Perimeter Institute Rapporteur Freidel, Laurent Faculty member Perimeter Institute Président Speziale, Simone Chargé de recherche Université d’Aix-Marseille Examinateur Samtleben, Henning Professeur ENS de Lyon Examinateur Livine, Etera Directeur de recherche ENS de Lyon Directeur de thèse christoph charles RENORMALIZATIONANDCOARSE-GRAININGOF LOOP QUANTUM GRAVITY RENORMALIZATIONANDCOARSE-GRAININGOFLOOP QUANTUM GRAVITY christoph charles November 2016 Christoph Charles: Renormalization and Coarse-graining of Loop Quan- tum Gravity, , © November 2016 “Together, or not at all” — Amy Pond To my parents to whom I owe nearly everything. To my wife who has always been supportive. ABSTRACT The continuum limit of loop quantum gravity is still an open problem. Indeed, no proper dynamics in known to start with and we still lack the mathematical tools to study its would-be continuum limit. In the present PhD dissertation, we will investigate some coarse-graining methods that should become helpful in this enterprise. We concen- trate on two aspects of the theory’s coarse-graining: finding natural large scale observables on one hand and studying how the dynamics of varying graphs could be cast onto fixed graphs on the other hand. To determine large scale observables, we study the case of hyper- bolic tetrahedra and their natural description in a language close to loop quantum gravity. The surface holonomies in particular play an important role. This highlights the structure of double spin networks, which consist in a graph and its dual, which seems to also appear in works from Freidel et al. To solve the problem of varying graphs, we consider and define loopy spin networks. They encode the local curvature with loops around an effective vertex and allow to describe different graphs by hidding them in a coarse-graining process. More- over, their definition gives a natural procedure for coarse-graining allowing to relate different scales. Together, these two results constitute the foundation of a coarse- graining programme for diffeomorphism invariant theories. vii RÉSUMÉ Le problème de la limite continue de la gravitation quantique à boucle est encore ouvert. En effet, la dynamique précise n’est pas connue et nous ne disposons pas des outils nécessaires à l’étude de cette limite le cas échéant. Dans cette thèse, nous étudions quelques méthodes de coarse-graining (étude à gros grains) qui devraient contribuer à cette entreprise. Nous nous concentrons sur deux aspects du flot: la détermination d’observables naturelles à grandes échelles d’un côté et la manière de s’abstraire du problème de la dynamique à graphe variable en la projetant sur des graphes fixes de l’autre. Pour déterminer les observables aux grandes distances, nous étu- dions le cas des tétraèdres hyperboliques et leur description naturelle dans un langage proche de celui de la gravitation quantique à boucle. Les holonomies de surface en particulier jouent un rôle important. Cela dégage la structure des double spin networks constitués d’un graphe et de son dual, structure qui semble aussi apparaître dans les travaux de Freidel et al. Pour résoudre le problème des graphes variables, nous considérons et définissons les loopy spin networks. Ils encodent par des boucles la courbure locale d’un vertex effectif et permettent ainsi de décrire différents graphes en les masquant via le processus de coarse-graining. De plus, leur définition donne un procédé naturel systématique de coarse-graining pour passer d’une échelle à une autre. Ensemble, ces deux principaux résultats posent le fondement d’un programme de coarse-graining pour les théories invariantes sous dif- féomorphismes. viii PUBLICATIONS [1] Christoph Charles and Etera R. Livine. “Ashtekar-Barbero holon- omy on the hyperboloid: Immirzi parameter as a cutoff for quantum gravity.” In: D92.12 (2015), p. 124031. doi: 10.1103/ PhysRevD.92.124031. eprint: 1507.00851. [2] Christoph Charles and Etera R. Livine. “Closure constraints for hyperbolic tetrahedra.” In: 32.13 (2015), p. 135003. doi: 10. 1088/0264-9381/32/13/135003. eprint: 1501.00855. [3] Christoph Charles and Etera R. Livine. “The closure constraint for the hyperbolic tetrahedron as a Bianchi identity.” In: (2016). eprint: 1607.08359. [4] Christoph Charles and Etera R. Livine. “The Fock Space of Loopy Spin Networks for Quantum Gravity.” In: 48.8 (2016), p. 113. doi: 10.1007/s10714-016-2107-5. eprint: 1603.01117. ix ACKNOWLEDGMENTS I was told this is the hardest part to write. It is certainly most difficult not to forget someone as so many have helped in one way or another. The order of mention should not be taken to represent anything and certainly does not reflect the amount of work these people provided. First and foremost, I want to give a very special thanks to my ad- visor, doctor Etera Livine, who has mentored me, taught me and guided me during the whole thesis. Etera, it took some time to adapt to each other but in the end, I’m grateful. I’m grateful for learning to work with people with different approaches but I’m more especially grateful for all the sacrifices you made and the help you provided as a mental support, most notably in the end. You have introduced the world of research to me and taught me to love it enough to continue. I discovered quantum gravity and more specifically loop quantum gravity thanks to you. For all this, I want to say thank you. Thank you also to all of the defense committee members, doctor Laurent Freidel, doctor Henning Samtleben, doctor Bianca Dittrich, doctor Karim Noui and doctor Simone Speziale. All of you have been kind enough to answer every e-mail, to wait when I had some trouble getting all the information in time and have been flexible enough to accommodate all the difficulties. Thank you also for the help you gave when I had administrative issues. I also want to thank the administrative team of the ENS of Lyon, which is one of the most effective I have ever met. But most impor- tantly, I am always impressed by their willingness to help, their kind- ness and the support they provide. I must thank most particularly Myriam Friat who has borne with me for at least two weeks in the last run for the Ph.D. defense and helped me at every step of the process. My labmates have been of tremendous help too and it is difficult not to omit someone. I want to thank all of them for welcoming me in the first place, for all the discussions about nearly everything, but also for all the support and the encouragement they provided. Thank you to Michel Fruchart, David Lopes Cardozo, to Daniele Malpetti and to Baptiste Pezelier. A particular thank you must be addressed to Michel who have taken the trouble of listening to me talking for hours about quantum gravity just to help me clarify my ideas. His help cannot be overstated. I also want to thank Christophe Göller whose internship I had the chance to oversee. He encouraged me a lot, allowed some very interesting conversations and made the summer work a bit more xi lifeful. I want to thank him more specifically for the help he provided on some quite lengthy computations. I want to thank all my close friends who have been an incredible and inexhaustible source of courage and joy, namely, Chérif Adouama, Ivan Bannwarth, Dimitri Cobb, Siméon Giménez and Cyril Philippe. Thank you for all the discussions. Thank you Cyril for our talks on epistemology guiding my research. Thank you Dimitri for your help in math, where your knowledge is quickly exceeding mine. Thank you Ivan and Chérif for all the discussions about the Ph.D. life and your attentive ear. Thank you Siméon for the numerous conversations, the way too many jokes and the galaxy savings. I am also thinking about my flatmates though this group inter- sects with the previous one. Thank you Nathanaël Dobé and Mar- jorie Dobé, thank you Cyril Philippe, thank you Siméon Giménez, thank you Dimitri Cobb, thank you Maxime Kristanek and thank your Alexandre Drouin. Thank you for all the time playing, sharing meals and talking. Thank you for the good food and wine we shared and thank you for the less good burgers and coke we shared. I also want to thank people from church who have always been keen to ask for news and have been of great support: Gilles and Yvette Campoy, Denis and Maïlys Blum, Jonah and Amy Haddad, Alexandre and Suzanne Sarran.
Recommended publications
  • Effective Field Theory from Spin Foam Models :3D Example
    Effective field theory from spin Foam models :3d example Laurent Freidel Pennstate 2007 Background independent Loop Quantum Gravity in a nutshell Background independence: what the quantum geometry is at Planck scale cannot be postulated its needs to be determined dynamically •Hamiltonian quantisation: gravity is a gauge theory 2 SU(2) Yang-mills phase space (A,E) + constraints i1 (Γ, j , i ) (15) •Kinematical Hilbert space is spannede v by j1 j5 j2 spin network: graph colored by su(2) rep j6 j4 i4 Wave function i3 Ψ(Γ,je,iv)(A) i2 j3 (16) •Eigenstates of Geometrical operators, Area, Vol = trj(h (A)) (17) discrete spectra quantized space◦ geometry s’ 2 •Dynamics:Area !encodedΨΓ,je,i vin= spin8πγ foamlP modelsje(j eallowing+ 1) ΨΓ ,jthee,iv (18) e R Γ + ... computation of transition amplitudes∈!∪ "between Spin networks states: quantum spacetime geometry s 2 Area!Ψ(Γ,je,iv) = 8πγlP je(je + 1) Ψ(Γ,je,iv) (19) # e R Γ ( ∈!∪ " $ %& ' 3 2 VolΨΓ,je,iv = 8πγlP vje,iv ΨΓ,je,iv (20) # v R Γ ( * ∈!∪ ) F (A) E (21) ∝ Area(! H) = A (22) H = tr([E, E]F (A)) (23) Hj(i) (24) i ! i S(g) Dg e lP (25) + K (j) k (l d ) (26) F ∝ F P j ! k [Xi , Xj] = ilP #ijkX (27) m sin(κm)/κ (28) → S3 SU(2) (29) ∼ X ∂ (30) ∼ P 2 (Γ, je, iv) (15) Ψ(Γ,je,iv)(A) (16) v v Ue Pe + [Ωe, Pe] = 0 (0.32) = trj(h (A)) (17) ◦ ∂!e=v 2 S = tr(XeGe) (0.33) Area!ΨΓ,je,iv = 8πγlP je(je +T1ra)nsΨitioΓn,jaem,ipvlitudes between spin network state(1s a8)re defined by e e R Γ s, s! = A[ ], (11) ∈ ∪ ! "phys F ! " ! F:s→s! v v ! δXe = Ue Φwhvere the[nΩotaeti,onΦanvtic]ip=ates t0he interpretation of such amplitudes as defining the physical (0.34) scala−r product.
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • On the Axioms of Causal Set Theory
    On the Axioms of Causal Set Theory Benjamin F. Dribus Louisiana State University [email protected] November 8, 2013 Abstract Causal set theory is a promising attempt to model fundamental spacetime structure in a discrete order-theoretic context via sets equipped with special binary relations, called causal sets. The el- ements of a causal set are taken to represent spacetime events, while its binary relation is taken to encode causal relations between pairs of events. Causal set theory was introduced in 1987 by Bombelli, Lee, Meyer, and Sorkin, motivated by results of Hawking and Malament relating the causal, conformal, and metric structures of relativistic spacetime, together with earlier work on discrete causal theory by Finkelstein, Myrheim, and 't Hooft. Sorkin has coined the phrase, \order plus number equals geometry," to summarize the causal set viewpoint regarding the roles of causal structure and discreteness in the emergence of spacetime geometry. This phrase represents a specific version of what I refer to as the causal metric hypothesis, which is the idea that the properties of the physical universe, and in particular, the metric properties of classical spacetime, arise from causal structure at the fundamental scale. Causal set theory may be expressed in terms of six axioms: the binary axiom, the measure axiom, countability, transitivity, interval finiteness, and irreflexivity. The first three axioms, which fix the physical interpretation of a causal set, and restrict its \size," appear in the literature either implic- itly, or as part of the preliminary definition of a causal set. The last three axioms, which encode the essential mathematical structure of a causal set, appear in the literature as the irreflexive formula- tion of causal set theory.
    [Show full text]
  • The Black Hole Information Paradox and Relative Locality Arxiv
    The black hole information paradox and relative locality Lee Smolin∗ Perimeter Institute for Theoretical Physics, 31 Caroline Street North, Waterloo, Ontario N2J 2Y5, Canada October 24, 2018 Abstract We argue that the recently proposed principle of relative locality offers a new way to resolve the black hole information puzzle. Contents 1 Introduction 2 2 A possible resolution of the BH information paradox 5 2.1 The usual statement of the black hole information paradox . 5 2.2 The point of view of an observer at the formation of the black hole . 6 2.3 The point of view of the observer at the final evaporation . 7 arXiv:1108.0910v1 [gr-qc] 3 Aug 2011 3 Conclusion 8 ∗[email protected] 1 1 Introduction The black hole information paradox1 has challenged theorists of quantum gravity since first proposed by Hawking[1]. One much discussed view has been that some kind of non- locality is required to resolve the puzzle[4]. A recently proposed framework for quantum gravity phenomenology, called relative locality[5, 6, 7, 8] does feature a very controlled form of non-locality. We argue here that the kind and scale of non-locality implied by relative locality is sufficient to resolve the black hole information paradox. Whatever the quantum theory of gravity that describes nature is, we have good reason to suspect that it involves a dissolving of the usual notion of locality in spacetime. It is therefore of interest to characterize exactly how non-locality first appears in physical phenomena in experimental regimes where one of the Planck scales becomes evident.
    [Show full text]
  • 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 ........................................................................................................................
    [Show full text]
  • At the Corner of Space and Time
    At the Corner of Space and Time by Barak Shoshany A thesis presented to the University of Waterloo in fulfillment of the thesis requirement for the degree of Doctor of Philosophy in Physics Waterloo, Ontario, Canada, 2019 c Barak Shoshany 2019 Examining Committee Membership The following served on the Examining Committee for this thesis. The decision of the Examining Committee is by majority vote. External Examiner: Karim Noui Associate Professor University of Tours Supervisors: Laurent Freidel Faculty Perimeter Institute for Theoretical Physics Robert Myers Faculty Perimeter Institute for Theoretical Physics Internal Members: Robert Mann Professor University of Waterloo John Moffat Professor Emeritus University of Toronto Internal-External Member: Florian Girelli Associate Professor University of Waterloo ii Author’s Declaration This thesis consists of material all of which I authored or co-authored: see Statement of Contributions included in the thesis. This is a true copy of the thesis, including any required final revisions, as accepted by my examiners. I understand that my thesis may be made electronically available to the public. iii Statement of Contributions This thesis is based on the papers [1], co-authored with Laurent Freidel and Florian Girelli, the papers [2, 3], of which I am the sole author, and additional unpublished material, of which I am the sole author. iv Abstract We perform a rigorous piecewise-flat discretization of classical general relativity in the first-order formulation, in both 2+1 and 3+1 dimensions, carefully keeping track of curvature and torsion via holonomies. We show that the resulting phase space is precisely that of spin networks, the quantum states of discrete spacetime in loop quan- tum gravity, with additional degrees of freedom called edge modes, which control the gluing between cells.
    [Show full text]
  • Redalyc.Physics of Deformed Special Relativity: Relativity Principle Revisited
    Brazilian Journal of Physics ISSN: 0103-9733 [email protected] Sociedade Brasileira de Física Brasil Girelli, Florian; Livine, Etera R. Physics of deformed special relativity: relativity principle revisited Brazilian Journal of Physics, vol. 35, núm. 2B, junio, 2005, pp. 432-438 Sociedade Brasileira de Física Sâo Paulo, Brasil Available in: http://www.redalyc.org/articulo.oa?id=46415793011 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 432 Brazilian Journal of Physics, vol. 35, no. 2B, June, 2005 Physics of Deformed Special Relativity: Relativity Principle Revisited Florian Girelli and Etera R. Livine Perimeter Institute, 31 Caroline Street North Waterloo, Ontario Canada N2L 2Y5 Received on 23 December, 2004 In many different ways, Deformed Special Relativity (DSR) has been argued to provide an effective limit of quantum gravity in almost-flat regime. Unfortunately, DSR is up to now plagued by many conceptual problems (in particular how it describes macroscopic objects) which forbids a definitive physical interpretation and clear predictions. Here we propose a consistent framework to interpret DSR. We extend the principle of relativity: the same way that Special Relativity showed us that the definition of a reference frame requires to specify its speed, we show that DSR implies that we must also take into account its mass. We further advocate a 5- dimensional point of view on DSR physics and the extension of the kinematical symmetry from the Poincare´ group to the Poincare-de´ Sitter group (ISO(4; 1)).
    [Show full text]
  • 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.
    [Show full text]
  • 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.
    [Show full text]
  • Quantum Gravity Past, Present and Future
    Quantum Gravity past, present and future carlo rovelli vancouver 2017 loop quantum gravity, Many directions of investigation string theory, Hořava–Lifshitz theory, supergravity, Vastly different numbers of researchers involved asymptotic safety, AdS-CFT-like dualities A few offer rather complete twistor theory, tentative theories of quantum gravity causal set theory, entropic gravity, Most are highly incomplete emergent gravity, non-commutative geometry, Several are related, boundaries are fluid group field theory, Penrose nonlinear quantum dynamics causal dynamical triangulations, Several are only vaguely connected to the actual problem of quantum gravity shape dynamics, ’t Hooft theory non-quantization of geometry Many offer useful insights … loop quantum causal dynamical gravity triangulations string theory asymptotic Hořava–Lifshitz safety group field AdS-CFT theory dualities twistor theory shape dynamics causal set supergravity theory Penrose nonlinear quantum dynamics non-commutative geometry Violation of QM non-quantized geometry entropic ’t Hooft emergent gravity theory gravity Several are related Herman Verlinde at LOOP17 in Warsaw No major physical assumptions over GR&QM No infinity in the small loop quantum causal dynamical Infinity gravity triangulations in the small Supersymmetry string High dimensions theory Strings Lorentz Violation asymptotic Hořava–Lifshitz safety group field AdS-CFT theory dualities twistor theory Mostly still shape dynamics causal set classical supergravity theory Penrose nonlinear quantum dynamics non-commutative geometry Violation of QM non-quantized geometry entropic ’t Hooft emergent gravity theory gravity Discriminatory questions: Is Lorentz symmetry violated at the Planck scale or not? Are there supersymmetric particles or not? Is Quantum Mechanics violated in the presence of gravity or not? Are there physical degrees of freedom at any arbitrary small scale or not? Is geometry discrete i the small? Lorentz violations Infinite d.o.f.
    [Show full text]
  • 2+1D Loop Quantum Gravity on the Edge,” Phys
    2+1D Loop Quantum Gravity on the Edge Laurent Freidel∗ and Barak Shoshany† Perimeter Institute for Theoretical Physics, 31 Caroline Street North, Waterloo, Ontario, Canada, N2L 2Y5 Florian Girelli‡ Department of Applied Mathematics, University of Waterloo, 200 University Avenue West, Waterloo, Ontario, Canada, N2L 3G1 April 3, 2020 Abstract We develop a new perspective on the discretization of the phase space structure of gravity in 2+1 dimensions as a piecewise-flat geometry in 2 spatial dimensions. Starting from a subdivision of the continuum geometric and phase space structure into elementary cells, we obtain the loop gravity phase space coupled to a collection of effective particles carrying mass and spin, which measure the curvature and torsion of the geometry. We show that the new degrees of freedom associated to the particle-like elements can be understood as edge modes, which appear in the decomposition of the continuum theory into subsystems and do not cancel out in the gluing of cells along codimension 2 defects. These new particle-like edge modes are gravitationally dressed in an explicit way. This provides a detailed explanation of the relations and differences between the loop gravity phase space and the one deduced from the continuum theory. Contents 1 Introduction 2 arXiv:1811.04360v4 [gr-qc] 1 Apr 2020 2 Piecewise-DG-Flat Manifolds in Two Dimensions 6 2.1 TheCellularDecomposition . ........... 6 2.2 TheDGConnectionInsidetheCells . ........... 7 2.3 The DG Connection Inside the Disks . ........... 8 2.4 Continuity Conditions Between Cells . ............. 12 2.5 Continuity Conditions Between Disks and Cells . ............... 13 2.6 Summary......................................... ..... 14 2.7 The Chern-Simons Symplectic Potential .
    [Show full text]