Quantum Theory of Geometry I: Area Operators

Total Page:16

File Type:pdf, Size:1020Kb

Quantum Theory of Geometry I: Area Operators The Erwin Schrodinger International Boltzmanngasse ESI Institute for Mathematical Physics A Wien Austria Quantum Theory of Geometry I Area Op erators Abhay Ashtekar Jerzy Lewandowski Vienna Preprint ESI August Supp orted by Federal Ministry of Science and Research Austria Available via httpwwwesiacat Quantum Theory of Geometry I Area Op erators Abhay Ashtekar and Jerzy Lewandowski August Center for Gravitational Physics and Geometry Physics Department Penn State University Park PA USA Institute of Theoretical Physics Warsaw University ul Hoza Warsaw Poland Max Planck Institut fur Gravitationphysik Schlaatzweg Potsdam Germany Abstract A new functional calculus develop ed recently for a fully nonp erturbative treatment of quantum gravity is used to b egin a systematic construction of a quantum theory of geometry Regulated op erators corresp onding to areas of surfaces are intro duced and shown to b e selfadjoint on the underlying kinematical Hilb ert space of states It is shown that their sp ectra are purely discrete indicating that the underlying quantum geometry is far from what the continuum picture might suggest Indeed the fundamental excitations of quantum geometry are dimensional rather like p olymers and the dimensional continuum geometry emerges only on coarse graining The full Hilb ert space admits an orthonormal decomp osition into nite dimensional subspaces which can b e interpreted as the spaces of states of spin systems Using this prop erty the complete sp ectrum of the area op erators is evaluated The general framework constructed here will b e used in a subsequent pap er to discuss dimensional geometric op erators eg the ones corresp onding to volumes of regions It is a pleasure to dedicate this article to Professor Andrzej Trautman who was one of the rst to recognize the deep relation b etween geometry and the physics of gauge elds which lies at the heart of this investigation Intro duction In his celebrated inaugural address Riemann suggested that geometry of space may b e more than just a ducial mathematical entity serving as a passive stage for physical phenomena and may in fact have a direct physical meaning in its own right General relativity proved this vision to b e correct Einsteins equations put geometry on the same fo oting as matter Now the physics of this century has shown us that matter has constituents and the dimensional ob jects we p erceive as solids in fact have a discrete underlying structure The continuum description of matter is an approximation which succeeds brilliantly in the macroscopic regime but fails hop elessly at the atomic scale It is therefore natural to ask if the same is true of geometry Do es geometry also have constituents at the Planck scale What are its atoms Its elementary excitations Is the spacetime continuum only a coarsegrained approximation If so what is the nature of the underlying quantum geometry To prob e such issues it is natural to lo ok for hints in the pro cedures that have b een successful in describing matter Let us b egin by asking what we mean by quantization of physical quantities Let us take a simple example the hydrogen atom In this case the answer is clear while the basic observables energy and angular momentum take on a continuous range of values classically in quantum mechanics their sp ectra are discrete So we can ask if the same is true of geometry Classical geometrical observables such as areas of surfaces and volumes of regions can take on continuous values on the phase space of general relativity Are the sp ectra of corresp onding quantum op erators discrete If so we would say that geometry is quantized Thus it is rather easy to p ose the basic questions in a precise fashion Indeed they could have b een formulated so on after the advent of quantum mechanics An swering them on the other hand has proved to b e surprisingly dicult The main reason it seems is the inadequacy of the standard techniques More precisely the traditional approach to quantum eld theory has b een p erturbative where one begins with a continuum background geometry It is then dicult to see how discreteness would arise in the sp ectra of geometric op erators To analyze such issues one needs a fully nonp erturbative approach geometric op erators have to b e constructed ab initio without assuming any background geometry To prob e the nature of quantum geometry we can not b egin by assuming the validity of the continuum picture We must let quantum gravity itself decide whether this picture is adequate at the Planck scale the theory itself should lead us to the correct microscopic picture of geometry In this pap er we will use the nonp erturbative canonical approach to quantum gravity based on connections to prob e these issues Over the past three years this approach has b een put on a rm mathematical fo oting through the development of a new functional calculus on the space of gauge equivalent connections This calculus do es not use any background elds such as a metric and is therefore wellsuited to a fully nonp erturbative treatment The purp ose of this pap er is to use this framework to explore the nature of quantum geometry In section we recall the relevant results from the new functional calculus and outline the general strategy In section we present a regularization of the area op erator Its prop erties are discussed in section in particular we exhibit its entire sp ectrum Our analysis is carried out in the connection representation and the discussion is selfcontained However at a nontechnical level there is a close similarity b etween the basic ideas used here and those used in discussions based on the lo op representation Indeed the development of the functional calculus which underlies this analysis itself was motivated in a large measure by the pioneering work on lo op representation by Rovelli and Smolin The relation b etween various approaches will discussed in section The main result of this pap er should have ramications on the statistical me chanical origin of the entropy of black holes along the lines of This issue is b eing investigated Preliminaries This section is divided into three parts In the rst we will recall the basic structure of the quantum conguration space and in the second that of the Hilb ert space of kinematic quantum states The overall strategy will b e summarized in the third part Quantum conguration space In general relativity one can regard the space AG of SU connections mo dulo gauge transformations on a spatial manifold as the classical conguration space For systems with only a nite numb er of degrees of freedom the classical conguration space also serves as the domain space of quantum wave functions ie as the quantum conguration space For systems with an innite numb er of degrees of freedom on the other hand this is not true generically the quantum conguration space is an enlargement of the classical In free eld theory in Minkowski space as well as exactly solvable mo dels in low spacetime dimensions for example while the classical conguration space can b e built from suitably smo oth elds the quantum conguration space includes all temp ered distributions This is an imp ortant p oint b ecause typically the classical conguration spaces are of zero measure wave functions with supp ort only on smo oth congurations have zero norm The overall situation is the same in general relativity The quantum conguration AG is a certain completion of AG space AG inherits the quotient structure of AG ie AG is the quotient The space of the space A of generalized connections by the space G of generalized gauge trans formations To see the nature of the generalization involved recall rst that each R A smo oth connection denes a holonomy along paths in h A P exp p p Generalized connections capture this notion That is each A in A can b e dened as a map which assigns to each oriented path p in an element Ap of SU such that i Ap Ap and ii Ap p Ap Ap where p is obtained from p by simply reversing the orientation p p denotes the comp osition of the two paths obtained by connecting the end of p with the b eginning of p and Ap Ap is the comp osition in SU A generalized gauge transformation is a map g which assigns to each p oint v of an SU element g x in an arbitrary p ossibly discontinuous fashion It acts on A in the exp ected manner at the end p oints of paths Ap g v Ap g v where v and v are resp ectively the b eginning and the end p oint of p If A happ ens to b e a smo oth connections say A we have Ap h A However in general Ap can not b e expressed as a path p ordered exp onential of a smo oth form with values in the Lie algebra of SU Similarly in general a generalized gauge transformation can not b e represented by a smo oth group valued function on A G and AG seem to o large to b e mathematically At rst sight the spaces controllable However they admit three characterizations which enables one to in tro duce dierential and integral calculus on them We will conclude this subsection by summarizing the characterization as suitable limits of the corre sp onding spaces in lattice gauge theory which will b e most useful for the main b o dy of this pap er We b egin with some denitions An edge is an oriented dimensional submanifold of with two b oundary p oints called vertices which is analytic everywhere including the vertices A graph in is a collection of edges such that if two distinct edges meet they do so only at vertices In the physics
Recommended publications
  • Emergence of Time in Loop Quantum Gravity∗
    Emergence of time in Loop Quantum Gravity∗ Suddhasattwa Brahma,1y 1 Center for Field Theory and Particle Physics, Fudan University, 200433 Shanghai, China Abstract Loop quantum gravity has formalized a robust scheme in resolving classical singu- larities in a variety of symmetry-reduced models of gravity. In this essay, we demon- strate that the same quantum correction which is crucial for singularity resolution is also responsible for the phenomenon of signature change in these models, whereby one effectively transitions from a `fuzzy' Euclidean space to a Lorentzian space-time in deep quantum regimes. As long as one uses a quantization scheme which re- spects covariance, holonomy corrections from loop quantum gravity generically leads to non-singular signature change, thereby giving an emergent notion of time in the theory. Robustness of this mechanism is established by comparison across large class of midisuperspace models and allowing for diverse quantization ambiguities. Con- ceptual and mathematical consequences of such an underlying quantum-deformed space-time are briefly discussed. 1 Introduction It is not difficult to imagine a mind to which the sequence of things happens not in space but only in time like the sequence of notes in music. For such a mind such conception of reality is akin to the musical reality in which Pythagorean geometry can have no meaning. | Tagore to Einstein, 1920. We are yet to come up with a formal theory of quantum gravity which is mathematically consistent and allows us to draw phenomenological predictions from it. Yet, there are widespread beliefs among physicists working in fundamental theory regarding some aspects of such a theory, once realized.
    [Show full text]
  • The EPRL Intertwiners and Corrected Partition Function Wojciech Kamiski, Marcin Kisielowski, Jerzy Lewandowski
    The EPRL intertwiners and corrected partition function Wojciech Kamiski, Marcin Kisielowski, Jerzy Lewandowski To cite this version: Wojciech Kamiski, Marcin Kisielowski, Jerzy Lewandowski. The EPRL intertwiners and corrected partition function. Classical and Quantum Gravity, IOP Publishing, 2010, 27 (16), pp.165020. 10.1088/0264-9381/27/16/165020. hal-00616260 HAL Id: hal-00616260 https://hal.archives-ouvertes.fr/hal-00616260 Submitted on 21 Aug 2011 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. Confidential: not for distribution. Submitted to IOP Publishing for peer review 31 May 2010 The EPRL intertwiners and corrected partition function Wo jciech Kami´nski, Marcin Kisielowski, Jerzy Lewandowski Instytut Fizyki Teoretycznej, Uniwersytet Warszawski, ul. Ho˙za 69, 00-681 Warszawa (Warsaw), Polska (Poland) Abstract Do the SU(2) intertwiners parametrize the space of the EPRL solutions to the sim- plicity constraint? What is a complete form of the partition function written in terms of this parametrization? We prove that the EPRL map is injective in the general n-valent vertex case for the Barbero-Immirzi parameter less then 1. We find, however, that the EPRL map is not isomet- ric.
    [Show full text]
  • On the Consistency of the Constraint Algebra in Spin Network Quantum
    SU-GP-97/10-2 On the consistency of the constraint algebra in spin network quantum gravity Rodolfo Gambini∗ Instituto de F´ısica, Facultad de Ciencias, Tristan Narvaja 1674, Montevideo,CGPG-97-10/1 Uruguay gr-qc/9710018 Jerzy Lewandowski† Max-Planck-Institut f¨ur Gravitationsphysik Schlaatzweg 1 D-14473 Potsdam, Germany Donald Marolf Physics Department, Syracuse University, Syracuse, NY 13244-1130 Jorge Pullin Center for Gravitational Physics and Geometry, Department of Physics, 104 Davey Lab, The Pennsylvania State University, University Park, PA 16802 Abstract We point out several features of the quantum Hamiltonian constraints re- arXiv:gr-qc/9710018v1 2 Oct 1997 cently introduced by Thiemann for Euclidean gravity. In particular we dis- cuss the issue of the constraint algebra and of the quantum realization of the ab object q Vb, which is classically the Poisson Bracket of two Hamiltonians. I. INTRODUCTION In a remarkable series of papers [1–4] by Thiemann, the loop approach to the quantiza- tion of general relativity reached a new level. Using ideas related to those of Rovelli and ∗Associate member of ICTP. †On leave from Instytut Fizyki Teoretycznej, Uniwersytet Warszawski, ul. Ho˙za 69, 00-681 Warszawa, Poland 1 Smolin [8], Thiemann proposed a definition of the quantum Hamiltonian (Wheeler-DeWitt) constraint of Einstein-Hilbert gravity which is a densely defined operator on a certain Hilbert space and which is (in a certain sense [1]) anomaly free on diffeomorphism invariant states. The fact that the proposed constraints imply the existence of a self-consistent, well defined theory is very impressive. However, it is still not clear whether the resulting theory is con- nected with the physics of gravity.
    [Show full text]
  • Loop Quantum Gravity
    QUANTUM GRAVITY Loop gravity combines general relativity and quantum theory but it leaves no room for space as we know it – only networks of loops that turn space–time into spinfoam Loop quantum gravity Carlo Rovelli GENERAL relativity and quantum the- ture – as a sort of “stage” on which mat- ory have profoundly changed our view ter moves independently. This way of of the world. Furthermore, both theo- understanding space is not, however, as ries have been verified to extraordinary old as you might think; it was introduced accuracy in the last several decades. by Isaac Newton in the 17th century. Loop quantum gravity takes this novel Indeed, the dominant view of space that view of the world seriously,by incorpo- was held from the time of Aristotle to rating the notions of space and time that of Descartes was that there is no from general relativity directly into space without matter. Space was an quantum field theory. The theory that abstraction of the fact that some parts of results is radically different from con- matter can be in touch with others. ventional quantum field theory. Not Newton introduced the idea of physi- only does it provide a precise mathemat- cal space as an independent entity ical picture of quantum space and time, because he needed it for his dynamical but it also offers a solution to long-stand- theory. In order for his second law of ing problems such as the thermodynam- motion to make any sense, acceleration ics of black holes and the physics of the must make sense.
    [Show full text]
  • Loop Gravity 2
    Loop Quantum Gravity∗ Hanno Sahlmann Institute for Theoretical Physics, Karlsruhe University Karlsruhe Institute for Technology Preprint KA-TP-19-2009 Abstract In this article we review the foundations and the present status of loop quantum gravity. It is short and relatively non-technical, the emphasis is on the ideas, and the flavor of the techniques. In particular, we describe the kinematical quantization and the implementation of the Hamilton constraint, as well as the quantum theory of black hole horizons, semiclassical states, and matter propagation. Spin foam models and loop quantum cosmology are mentioned only in passing, as these will be covered in separate reviews to be published alongside this one. 1 Introduction Loop quantum gravity is non-perturbative approach to the quantum theory of gravity, in which no classical background metric is used. In particular, its starting point is not a linearized theory of gravity. As a consequence, while it still operates according to the rules of quantum field theory, the details are quite different of those for field theories that operate on a fixed classical background space-time. It has considerable successes to its credit, perhaps most notably a quantum theory of spatial geometry in which quan- tities such as area and volume are quantized in units of the Planck length, and a cal- culation of black hole entropy for static and rotating, charged and neutral black holes. But there are also open questions, many of them surrounding the dynamics (“quantum Einstein equations”) of the theory. In contrast to other approaches such as string theory, loop quantum gravity is rather modest in its aims.
    [Show full text]
  • Volume and Quantizations
    Volume and Quantizations Jerzy Lewandowski ∗ August 30, 2018 Abstract The aim of this letter is to indicate the differences between the Rovelli-Smolin quantum volume operator and other quantum volume operators existing in the literature. The formulas for the operators are written in a unifying notation of the graph projective framework. It is clarified whose results apply to which operators and why. ∗Institute of Theoretical Physics, Warsaw University, ul Hoza 69, 00-681 Warsaw, Poland and Max-Planck-Institut f¨ur Gravitationsphysik, Schlaatzweg 1, 14473 Potsdam, Germany arXiv:gr-qc/9602035v1 17 Feb 1996 1 It should be emphasized at the very beginning that the letter has been motivated by very nice calculations made recently by Loll [1] in connection with the lattice quantization of the volume and by the work of Pietri and Rovelli [2] who studied the Rovelli-Smolin volume operator [3]. In the full continuum theory, there is still one more candidate for the quantum volume operator proposed in [4, 5, 6] which will be referred to as the ‘projective limit framework’ volume operator. The misunderstanding which we indicate here is that in [1, 7] the lattice operator tends to be considered as the restriction of the Rovelli-Smolin as well as the projective limit framework volume op- erators. In fact, the first lattice volume, that of [1], corresponds to neither of them. The corrected lattice volume operator of [7], on the other hand, has been modified to agree with the graph projective framework volume op- erator. However this is still different then the Rovelli-Smolin operator.
    [Show full text]
  • Properties of the Rovelli-Smolin-Depietri Volume
    Properties of the Rovelli-Smolin-DePietri volume operator in the spaces of monochromatic intertwiners Marcin Kisielowski National Centre for Nuclear Research, Pateura 7, 02-093 Warsaw, Poland Abstract. We study some properties of the Rovelli-Smolin-DePietri volume operator in loop quantum gravity, which significantly simplify the diagonalization problem and shed some light on the pattern of degeneracy of the eigenstates. The operator is defined by its action in the spaces of tensor products j1 ... jN of the irreducible SU(2) H ⊗ ⊗ H 1 N representation spaces ji ,i = 1,...,N, labelled with spins ji . We restrict to H ∈ 2 spaces of SU(2) invariant tensors (intertwiners) with all spins equal j1 = ... = jN = j. We call them spin j monochromatic intertwiners. Such spaces are important in the study of SU(2) gauge invariant states that are isotropic and can be applied to extract the cosmological sector of the theory. In the case of spin 1/2 we solve the eigenvalue problem completely: we show that the volume operator is proportional to identity and calculate the proportionality factor. arXiv:2104.11010v2 [gr-qc] 27 Apr 2021 Rovelli-Smolin-DePietri volume operator for monochromatic intertwiners 2 1. Introduction The idea that isotropic states in loop quantum gravity should be described by monochromatic intertwiners appeared in the literature a couple of times. In spin-foam cosmology the conditions of homogeneity and isotropy are imposed on the coherent states [1]. The coherent states are linear combinations of spin-network states for different spins but the main contribution comes from states with all spins equal.
    [Show full text]
  • Black Holes in Loop Quantum Gravity Alejandro Perez
    Black Holes in Loop Quantum Gravity Alejandro Perez To cite this version: Alejandro Perez. Black Holes in Loop Quantum Gravity. Rept.Prog.Phys., 2017, 80 (12), pp.126901. 10.1088/1361-6633/aa7e14. hal-01645217 HAL Id: hal-01645217 https://hal.archives-ouvertes.fr/hal-01645217 Submitted on 17 Apr 2018 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. Black Holes in Loop Quantum Gravity Alejandro Perez1 1 Centre de Physique Th´eorique,Aix Marseille Universit, Universit de Toulon, CNRS, UMR 7332, 13288 Marseille, France. This is a review of the results on black hole physics in the framework of loop quantum gravity. The key feature underlying the results is the discreteness of geometric quantities at the Planck scale predicted by this approach to quantum gravity. Quantum discreteness follows directly from the canonical quantization prescription when applied to the action of general relativity that is suitable for the coupling of gravity with gauge fields and specially with fermions. Planckian discreteness and causal considerations provide the basic structure for the understanding of the thermal properties of black holes close to equilibrium. Discreteness also provides a fresh new look at more (at the mo- ment) speculative issues such as those concerning the fate of information in black hole evaporation.
    [Show full text]
  • Book of Abstracts
    The 5th Conference of the Polish Society on Relativity 24 - 27 September 2018 BOOK OF ABSTRACTS WEBPAGE: http://ift.uni.wroc.pl/~potor5/ MAIL: [email protected] List of participants Giovanni Amelino-Camelia (Naples) Wojciech Kulczycki (Cracow) Michał Artymowski (Cracow & Warsaw) Sofya Labazova (Moscow) Paolo Aschieri (Alessandria) Taejin Lee (Kangwon) Abhay Ashtekar (Pennsylvania) Jerzy Lewandowski (Warsaw) Eric Bergshoeff (Groningen) Jerzy Lukierski (Wroclaw) Krzysztof Bolejko (Sydney) Patryk Mach (Cracow) Gioele Botta (Warsaw) Shahn Majid (London) Iwo Białynicki-Birula (Warsaw) Edward Malec (Cracow) Arkadiusz Błaut (Wroclaw) Tomáš Málek (Prague) Andrzej Borowiec (Wroclaw) Przemysław Małkiewicz (Warsaw) Lennart Brocki (Wroclaw) Michal Marvan (Opava) Bernd Brügmann (Jena) Lionel Mason (Oxford) Piotr Chruściel (Vienna) Jerzy Matyjasek (Lublin) Adam Chudecki (Lodz) Jakub Mielczarek (Cracow & Marseille) Ewa Czuchry (Warsaw) Djordje Minic (Virginia) Marcin Daszkiewicz (Wroclaw) Sergey Odintsov (Barcelona) Denis Dobkowski-Ryłko (Warsaw) Andrzej Odrzywołek (Cracow) Remigiusz Durka (Wroclaw) Marcello Ortaggio (Prague) Polina Dyadina (Moscow) Tomasz Pawłowski (Warsaw) Filip Ficek (Cracow) Michał Piróg (Cracow) Laurent Freidel (Waterloo) Istvan Racz (Budapest & Warsaw) Andrzej Frydryszak (Wroclaw) Marek Rogatko (Lublin) Jakub Gizbert-Studnicki (Cracow) Giacomo Rosati (Cagliari) Krzysztof Głód (Cracow) Szymon Sikora (Cracow) Giulia Gubitosi (Nijmegen) Andrzej Sitarz (Cracow) Zbigniew Haba (Wroclaw) Tomasz Smołka (Warsaw) Orest Hrycyna (Warsaw)
    [Show full text]
  • 1 the Inverted Big-Bang Our Universe Appears to Have Been Created Not
    The Inverted Big-Bang Our universe appears to have been created not out of nothing but from a strange space-time dust of quantum geometry By Rüdiger Vaas ________________________________________________________________________ Summary: • Quantum geometry makes it possible to avoid the ominous beginning of our universe with its physically unrealistic – infinite – curvature, extreme temperature, and energy density. It could be the long sought after explanation of the big-bang. • It perhaps even opens a window into a time before the big-bang – space itself may have come from an earlier collapsing universe that turned inside out or inverted and began to expand again. With the help of one equation, Martin Bojowald tries to look into a time that no one has ever seen – into a time before time, into the time before the big-bang. If this equation is correct, the big-bang was not the beginning of everything but merely a transition – the end of a previous universe collapsing into itself and at the same time turning inside out into a new universe expanding out. The young physicist at Max-Planck-Institute for gravitational physics in Potsdam cannot yet say what happened exactly before the big-bang. But his results are already so promising, that he has received high recognition and collaboration from renowned physicists worldwide. Obviously equations are not telescopes or time machines that permit us to really peer into this presumed precursor-universe. Yet mathematical intuition and physical genius can help us leap into this fantasy. A quantum leap in viewpoint is also urgently needed to solve perhaps the biggest mystery of physics: the origin of the universe.
    [Show full text]
  • Quantum Theory of Geometry: I. Area Operators
    Class. Quantum Grav. 14 (1997) A55–A81. Printed in the UK PII: S0264-9381(97)77957-7 Quantum theory of geometry: I. Area operators Abhay Ashtekar and Jerzy Lewandowski y zx Center for Gravitational Physics and Geometry, Physics Department, Penn State, University y Park, PA 16802-6300, USA Institute of Theoretical Physics, Warsaw University, ul Hoza 69, 00-681 Warsaw, Poland z Max Planck Institut fur¨ Gravitationphysik, Schlaatzweg 1, 14473 Potsdam, Germany x Abstract. A new functional calculus, developed recently for a fully non-perturbative treatment of quantum gravity, is used to begin a systematic construction of a quantum theory of geometry. Regulated operators corresponding to areas of 2-surfaces are introduced and shown to be self- adjoint on the underlying (kinematical) Hilbert space of states. It is shown that their spectra are purely discrete, indicating that the underlying quantum geometry is far from what the continuum picture might suggest. Indeed, the fundamental excitations of quantum geometry are one dimensional, rather like polymers, and the three-dimensional continuum geometry emerges only on coarse graining. The full Hilbert space admits an orthonormal decomposition into finite- dimensional subspaces which can be interpreted as the spaces of states of spin systems. Using this property, the complete spectrum of the area operators is evaluated. The general framework constructed here will be used in a subsequent paper to discuss three-dimensional geometric operators, e.g. the ones corresponding to volumes of regions. PACS numbers: 0460, 0240 It is a pleasure to dedicate this paper to Professor Andrzej Trautman, who was one of the first to recognize the deep relationship between geometry and the physics of gauge fields [1, 2] which lies at the heart of this investigation.
    [Show full text]
  • Statistical Equilibrium in Quantum Gravity
    PAPER • OPEN ACCESS Related content - Emergent Friedmann dynamics with a Statistical equilibrium in quantum gravity: Gibbs quantum bounce from quantum gravity condensates Daniele Oriti, Lorenzo Sindoni and Edward states in group field theory Wilson-Ewing - Topical Review To cite this article: Isha Kotecha and Daniele Oriti 2018 New J. Phys. 20 073009 Abhay Ashtekar and Jerzy Lewandowski - Group field theory as the second quantization of loop quantum gravity Daniele Oriti View the article online for updates and enhancements. This content was downloaded from IP address 188.184.3.52 on 13/07/2018 at 16:14 New J. Phys. 20 (2018) 073009 https://doi.org/10.1088/1367-2630/aacbbd PAPER Statistical equilibrium in quantum gravity: Gibbs states in group field OPEN ACCESS theory RECEIVED 13 February 2018 Isha Kotecha1,2 and Daniele Oriti1,3 REVISED 1 Max Planck Institute for Gravitational Physics (Albert Einstein Institute), Am Mühlenberg 1, D-14476 Potsdam-Golm, Germany 30 May 2018 2 Institute for Physics, Humboldt-Universität zu Berlin, Newtonstraße 15, D-12489 Berlin, Germany ACCEPTED FOR PUBLICATION 3 II Institute for Theoretical Physics, University of Hamburg, Luruper Chaussee 149, D-22761 Hamburg, Germany 11 June 2018 PUBLISHED E-mail: [email protected] and [email protected] 4 July 2018 Keywords: quantum gravity, background independence, statistical equilibrium, deparametrization, Gibbs states Original content from this work may be used under the terms of the Creative Abstract Commons Attribution 3.0 licence. Gibbs states are known to play a crucial role in the statistical description of a system with a large Any further distribution of number of degrees of freedom.
    [Show full text]