Amplitudes in the Spin Foam Approach to Quantum Gravity
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Quantum Simplicial Geometry in the Group Field Theory Formalism
Quantum simplicial geometry in the group field theory formalism: reconsidering the Barrett-Crane model Aristide Baratin∗1 and Daniele Oriti†2 1Centre de Physique Th´eorique, CNRS UMR 7644, Ecole Polytechnique F-9112 Palaiseau Cedex, France 2Max-Planck-Institut f¨ur Gravitationsphysik Albert Einstein Institute Am M¨uhlenberg 2, 14476, Golm, Germany, EU A dual formulation of group field theories, obtained by a Fourier transform mapping functions on a group to functions on its Lie algebra, has been proposed recently. In the case of the Ooguri model for SO(4) BF theory, the variables of the dual field variables are thus so(4) bivectors, which have a direct interpretation as the discrete B variables. Here we study a modification of the model by means of a constraint operator implementing the simplicity of the bivectors, in such a way that projected fields describe metric tetrahedra. This involves a extension of the usual GFT framework, where boundary operators are labelled by projected spin network states. By construction, the Feynman amplitudes are simplicial path integrals for constrained BF theory. We show that the spin foam formulation of these amplitudes corresponds to a variant of the Barrett-Crane model for quantum gravity. We then re-examin the arguments against the Barrett-Crane model(s), in light of our construction. Introduction Group field theories (GFT) represent a second quantized framework for both spin networks and simplicial geometry [6, 7, 9], field theories on group manifolds (or Lie algebras) producing Feynman amplitudes which can be equivalently expressed as simplicial gravity path integrals [5] or spin foam models [10], in turn covariant formulations of spin networks dynamics [1]3. -
The Feynman Propagator for Quantum Gravity: Spin Foams, Proper Time, Orientation, Causality and Timeless-Ordering
Brazilian Journal of Physics, vol. 35, no. 2B, June, 2005 481 The Feynman Propagator for Quantum Gravity: Spin Foams, Proper Time, Orientation, Causality and Timeless-Ordering D. Oriti Department of Applied Mathematics and Theoretical Physics, Centre for Mathematical Sciences, University of Cambridge, Wilberforce Road, Cambridge CB3 0WA, UK, EU Received on 19 December, 2004 We discuss the notion of causality in Quantum Gravity in the context of sum-over-histories approaches, in the absence therefore of any background time parameter. In the spin foam formulation of Quantum Gravity, we identify the appropriate causal structure in the orientation of the spin foam 2-complex and the data that characterize it; we construct a generalised version of spin foam models introducing an extra variable with the interpretation of proper time and show that different ranges of integration for this proper time give two separate classes of spin foam models: one corresponds to the spin foam models currently studied, that are independent of the underlying orientation/causal structure and are therefore interpreted as a-causal transition amplitudes; the second corresponds to a general definition of causal or orientation dependent spin foam models, interpreted as causal transition amplitudes or as the Quantum Gravity analogue of the Feynman propagator of field theory, implying a notion of ”timeless ordering”. 1 Introduction emerge only in a semiclassical approximation [3]. Regarding the issue of causality, there seem to be two basic attitude one This paper discusses the issue of causality in non-perturbative can take: one can hold that we cannot speak of causality in quantum gravity, and more precisely in the spin foam formu- absence of time and therefore just as time itself also a notion lation of the theory. -
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. -
Dimensional Topological Quantum Field Theory from a Tight-Binding Model of Interacting Spinless Fermions
This is a repository copy of (3+1)-dimensional topological quantum field theory from a tight-binding model of interacting spinless fermions. White Rose Research Online URL for this paper: http://eprints.whiterose.ac.uk/99993/ Version: Accepted Version Article: Cirio, M, Palumbo, G and Pachos, JK (2014) (3+1)-dimensional topological quantum field theory from a tight-binding model of interacting spinless fermions. Physical Review B, 90 (8). 085114. ISSN 2469-9950 https://doi.org/10.1103/PhysRevB.90.085114 Reuse Unless indicated otherwise, fulltext items are protected by copyright with all rights reserved. The copyright exception in section 29 of the Copyright, Designs and Patents Act 1988 allows the making of a single copy solely for the purpose of non-commercial research or private study within the limits of fair dealing. The publisher or other rights-holder may allow further reproduction and re-use of this version - refer to the White Rose Research Online record for this item. Where records identify the publisher as the copyright holder, users can verify any specific terms of use on the publisher’s website. Takedown If you consider content in White Rose Research Online to be in breach of UK law, please notify us by emailing [email protected] including the URL of the record and the reason for the withdrawal request. [email protected] https://eprints.whiterose.ac.uk/ (3+1)-dimensional topological quantum field theory from a tight-binding model of interacting spinless fermions Mauro Cirio,1 Giandomenico Palumbo,2 and Jiannis K. Pachos2 1Centre for Engineered Quantum Systems, Department of Physics and Astronomy, Macquarie University, North Ryde, NSW 2109, Australia 2School of Physics and Astronomy, University of Leeds, Leeds, LS2 9JT, United Kingdom (Dated: July 15, 2014) Currently, there is much interest in discovering analytically tractable (3 + 1)-dimensional models that describe interacting fermions with emerging topological properties. -
Construction and Examples of Higher Gauge Theories∗
Construction and examples of higher gauge theories∗ Tijana Radenkovi´cy Institute of Physics, University of Belgrade, Pregrevica 118, 11080 Belgrade, Serbia Marko Vojinovi´cz Institute of Physics, University of Belgrade, Pregrevica 118, 11080 Belgrade, Serbia Abstract We provide several examples of higher gauge theories, constructed as gener- alizations of a BF model to 2BF and 3BF models with constraints. Using the framework of higher category theory, we introduce appropriate 2-groups and 3- groups, and construct the actions for the corresponding constrained 2BF and 3BF theories. In this way, we can construct actions which describe the correct dynamics of Yang-Mills, Klein-Gordon, Dirac, Weyl, and Majorana fields coupled to Einstein-Cartan gravity. Each action is naturally split into a topological sector and a sector with simplicity constraints. The properties of the higher gauge group structure opens up a possibility of a nontrivial unification of all fields. 1. Introduction The quantization of the gravitational field is one of the fundamental open problems in modern physics. There are various approaches to this prob- lem, some of which have developed into vast research frameworks. One of such frameworks is the Loop Quantum Gravity approach, which aims to establish a nonperturbative quantization of gravity, both canonically and covariantly [1, 2, 3]. The covariant approach is slightly more general, and ∗ This work was supported by the project ON171031 of the Ministry of Education, Sci- ence and Technological Development (MPNTR) of the Republic of Serbia, and partially by the bilateral scientific cooperation between Austria and Serbia through the project \Causality in Quantum Mechanics and Quantum Gravity - 2018-2019", no. -
Loop Quantum Cosmology, Modified Gravity and Extra Dimensions
universe Review Loop Quantum Cosmology, Modified Gravity and Extra Dimensions Xiangdong Zhang Department of Physics, South China University of Technology, Guangzhou 510641, China; [email protected] Academic Editor: Jaume Haro Received: 24 May 2016; Accepted: 2 August 2016; Published: 10 August 2016 Abstract: Loop quantum cosmology (LQC) is a framework of quantum cosmology based on the quantization of symmetry reduced models following the quantization techniques of loop quantum gravity (LQG). This paper is devoted to reviewing LQC as well as its various extensions including modified gravity and higher dimensions. For simplicity considerations, we mainly focus on the effective theory, which captures main quantum corrections at the cosmological level. We set up the basic structure of Brans–Dicke (BD) and higher dimensional LQC. The effective dynamical equations of these theories are also obtained, which lay a foundation for the future phenomenological investigations to probe possible quantum gravity effects in cosmology. Some outlooks and future extensions are also discussed. Keywords: loop quantum cosmology; singularity resolution; effective equation 1. Introduction Loop quantum gravity (LQG) is a quantum gravity scheme that tries to quantize general relativity (GR) with the nonperturbative techniques consistently [1–4]. Many issues of LQG have been carried out in the past thirty years. In particular, among these issues, loop quantum cosmology (LQC), which is the cosmological sector of LQG has received increasing interest and has become one of the most thriving and fruitful directions of LQG [5–9]. It is well known that GR suffers singularity problems and this, in turn, implies that our universe also has an infinitely dense singularity point that is highly unphysical. -
Aspects of Loop Quantum Gravity
Aspects of loop quantum gravity Alexander Nagen 23 September 2020 Submitted in partial fulfilment of the requirements for the degree of Master of Science of Imperial College London 1 Contents 1 Introduction 4 2 Classical theory 12 2.1 The ADM / initial-value formulation of GR . 12 2.2 Hamiltonian GR . 14 2.3 Ashtekar variables . 18 2.4 Reality conditions . 22 3 Quantisation 23 3.1 Holonomies . 23 3.2 The connection representation . 25 3.3 The loop representation . 25 3.4 Constraints and Hilbert spaces in canonical quantisation . 27 3.4.1 The kinematical Hilbert space . 27 3.4.2 Imposing the Gauss constraint . 29 3.4.3 Imposing the diffeomorphism constraint . 29 3.4.4 Imposing the Hamiltonian constraint . 31 3.4.5 The master constraint . 32 4 Aspects of canonical loop quantum gravity 35 4.1 Properties of spin networks . 35 4.2 The area operator . 36 4.3 The volume operator . 43 2 4.4 Geometry in loop quantum gravity . 46 5 Spin foams 48 5.1 The nature and origin of spin foams . 48 5.2 Spin foam models . 49 5.3 The BF model . 50 5.4 The Barrett-Crane model . 53 5.5 The EPRL model . 57 5.6 The spin foam - GFT correspondence . 59 6 Applications to black holes 61 6.1 Black hole entropy . 61 6.2 Hawking radiation . 65 7 Current topics 69 7.1 Fractal horizons . 69 7.2 Quantum-corrected black hole . 70 7.3 A model for Hawking radiation . 73 7.4 Effective spin-foam models . -
Loop and Spin Foam Quantum Gravity: a Brief Guide for Beginners
AEI-2006-004 hep-th/0601129 January 18th, 2006 Loop and Spin Foam Quantum Gravity: A Brief Guide for Beginners Hermann Nicolai and Kasper Peeters Max-Planck-Institut f¨ur Gravitationsphysik Albert-Einstein-Institut Am M¨uhlenberg 1 14476 Golm, GERMANY hermann.nicolai, [email protected] Abstract: We review aspects of loop quantum gravity and spin foam models at an introductory level, with special attention to questions frequently asked by non-specialists. arXiv:hep-th/0601129 v2 16 Feb 2006 Contributed article to “An assessment of current paradigms in the physics of fundamental interactions”, ed. I. Stamatescu, Springer Verlag. 1. Quantum Einstein gravity ics approach [7], addresses several aspects of the problem that are currently outside the main focus The assumption that Einstein’s classical theory of of string theory, in particular the question of back- gravity can be quantised non-perturbatively is at the ground independence and the quantisation of geom- root of a wide variety of approaches to quantum etry. Whereas there is a rather direct link between gravity. The assumption constitutes the basis of sev- (perturbative) string theory and classical space-time eral discrete methods [1], such as dynamical tri- concepts, and string theory can therefore rely on fa- angulations and Regge calculus, but it also implic- miliar notions and concepts, such as the notion of a itly underlies the older Euclidean path integral ap- particle and the S-matrix, the task is harder for LQG, proach [2, 3] and the somewhat more indirect ar- as it must face up right away to the question of what guments which suggest that there may exist a non- an observable quantity is in the absence of a proper trivial fixed point of the renormalisation group [4–6]. -
Arxiv:1108.1178V2 [Gr-Qc]
Quantum simplicial geometry in the group field theory formalism: reconsidering the Barrett-Crane model Aristide Baratin∗1 and Daniele Oriti†2 1Centre de Physique Th´eorique, CNRS UMR 7644, Ecole Polytechnique F-9112 Palaiseau Cedex, France 2Max-Planck-Institut f¨ur Gravitationsphysik Albert Einstein Institute Am M¨uhlenberg 2, 14476, Golm, Germany, EU A dual formulation of group field theories, obtained by a Fourier transform mapping functions on a group to functions on its Lie algebra, has been proposed recently. In the case of the Ooguri model for SO(4) BF theory, the variables of the dual field variables are thus so(4) bivectors, which have a direct interpretation as the discrete B variables. Here we study a modification of the model by means of a constraint operator implementing the simplicity of the bivectors, in such a way that projected fields describe metric tetrahedra. This involves a extension of the usual GFT framework, where boundary operators are labelled by projected spin network states. By construction, the Feynman amplitudes are simplicial path integrals for constrained BF theory. We show that the spin foam formulation of these amplitudes corresponds to a variant of the Barrett-Crane model for quantum gravity. We then re-examin the arguments against the Barrett-Crane model(s), in light of our construction. Introduction Group field theories (GFT) represent a second quantized framework for both spin networks and simplicial geometry [6, 7, 9], field theories on group manifolds (or Lie algebras) producing Feynman amplitudes which can be equivalently expressed as simplicial gravity path integrals [5] or spin foam models [10], in turn covariant formulations of spin networks dynamics [1]3. -
De-Sheng Li. Pati-Salam Model in Curved Space-Time from Square Root Lorentz Manifold
Physical Science & Biophysics Journal MEDWIN PUBLISHERS ISSN: 2641-9165 Committed to Create Value for Researchers Pati-Salam Model in Curved Space-Time from Square Root Lorentz Manifold De-Sheng Li1,2,3* Review Article 1College of Physics, Mechanical and Electrical Engineering, Jishou University, China Volume 5 Issue 2 2Interdisciplinary Center for Quantum Information, National University of Defense Technology, Received Date: July 07, 2021 China Published Date: August 11, 2021 3 Institute of High Energy Physics, Chinese Academy of Sciences, China DOI: 10.23880/psbj-16000186 *Corresponding author: De-Sheng Li, College of Physics, Mechanical and Electrical Engineering, Jishou University, Jishou 416000, P. R. China, Email: [email protected] Abstract There is a UU(4') × (4) -bundle on four-dimensional square root Lorentz manifold. Then a Pati-Salam model in curved space-time (Lagrangian) and a gravity theory (Lagrangian) are constructed on square root Lorentz manifold based on self-parallel transportation principle. An explicit formulation of Sheaf quantization on this square root Lorentz manifold is shown. Sheaf quantization is based on superposition principle and construct a linear Sheaf space in curved space-time. The in Standard Model (SM) of particle physics and Einstein gravity are found in square root metric and the connections of bundle. transition amplitude in path integral quantization is given which is consistent with Sheaf quantization. All particles and fields ±c Thegravity interactions theory is betweenEinstein-Cartan particles/fields kind with are torsion. described There by are Lagrangian new particles, explicitly. right There handed are neutrinos, few new physics dark photon, in this Fiona,model. TheX 01212 and YYYYY,,,,**. -
Quantum Gravity, Field Theory and Signatures of Noncommutative Spacetime
HWM–09–5 EMPG–09–10 Quantum Gravity, Field Theory and Signatures of Noncommutative Spacetime1 Richard J. Szabo Department of Mathematics Heriot-Watt University Colin Maclaurin Building, Riccarton, Edinburgh EH14 4AS, U.K. and Maxwell Institute for Mathematical Sciences, Edinburgh, U.K. Email: [email protected] Abstract A pedagogical introduction to some of the main ideas and results of field theories on quantized spacetimes is presented, with emphasis on what such field theories may teach us about the problem of quantizing gravity. We examine to what extent noncommutative gauge theories may be regarded as gauge theories of gravity. UV/IR mixing is explained in detail and we describe its relations to renormalization, to gravitational dynamics, and to deformed dispersion relations arXiv:0906.2913v3 [hep-th] 5 Oct 2009 in models of quantum spacetime of interest in string theory and in doubly special relativity. We also discuss some potential experimental probes of spacetime noncommutativity. 1Based on Plenary Lecture delivered at the XXIX Encontro Nacional de F´ısica de Part´ıculas e Campos, S˜ao Louren¸co, Brasil, September 22–26, 2008. Contents 1 Introduction 1 2 Spacetime quantization 3 2.1 Snyder’sspacetime ............................... ...... 3 2.2 κ-Minkowskispacetime. .. .. .. .. .. .. .. .. .. ... 4 2.3 Three-dimensional quantum gravity . .......... 5 2.4 Spacetime uncertainty principle . ........... 6 2.5 Physicsinstrongmagneticfields . ......... 7 2.6 Noncommutative geometry in string theory . ........... 8 3 Field theory on quantized spacetimes 9 3.1 Formalism....................................... ... 9 3.2 UV/IRmixing ..................................... 10 3.3 Renormalization ................................. ..... 12 4 Noncommutative gauge theory of gravity 14 4.1 Gaugeinteractions ............................... ...... 14 4.2 Gravity in noncommutative gauge theories . -
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.