Dimensional Topological Quantum Field Theory from a Tight-Binding Model of Interacting Spinless Fermions
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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. -
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. -
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. -
Lecture 9 Sine-Gordon Model and Thirring Model Consider the Action
Lecture 9 Sine-Gordon model and Thirring model Consider the action of the sine-Gordon model in the general form Z (@ ')2 S ['] = d2x µ + 2µ cos β' : (1) sG 16π Here the action depends on two parameters: β and µ. Thep parameter β is dimensionless. We may consider it as the square root of the Planck constant: β = ~. Indeed, let u(x) = β'(x). Then the action is 1 Z (@ u)2 S = d2x µ + 2µβ2 cos u : sG β2 16π For β 1 the square of mass of the lightest excitation is m2 = 16πµβ2. If we keep it finite, the only place β enters is the prefactor, which must be ~−1 in the quantum case. We will consider the sine-Gordon theory as a perturbation of a free massless boson. The perturbation operator :cos β': has the scaling dimension 2β2. Hence, the dimension of the parameter µ is 2 − 2β2. Since this is the only dimensional parameter, masses of all particles in the theory must be proportional 2 to µ1=(2−2β ). In the limit β ! 0 we have m / µ1=2 as expected. The behavior of the model depends of the value of β. There are three cases 1. β2 < 1. The dimension of µ is positive, the perturbation is relevant. It means that the interaction decreases with decreasing scale. The short-range correlation functions behave like those in the massless free field theory. It makes the sine-Gordon theory well-defined and superrenormalizable. But the large-distance behavior strikingly differs from the short-distance one. It is described by a system of massive particles, whose mass spectrum essentially depends on the parameter β. -
Braids, 3-Manifolds, Elementary Particles: Number Theory and Symmetry in Particle Physics
S S symmetry Article Braids, 3-Manifolds, Elementary Particles: Number Theory and Symmetry in Particle Physics Torsten Asselmeyer-Maluga German Aeorspace Center, Rosa-Luxemburg-Str. 2, 10178 Berlin, Germany; [email protected]; Tel.: +49-30-67055-725 Received: 25 July 2019; Accepted: 2 October 2019; Published: 15 October 2019 Abstract: In this paper, we will describe a topological model for elementary particles based on 3-manifolds. Here, we will use Thurston’s geometrization theorem to get a simple picture: fermions as hyperbolic knot complements (a complement C(K) = S3 n (K × D2) of a knot K carrying a hyperbolic geometry) and bosons as torus bundles. In particular, hyperbolic 3-manifolds have a close connection to number theory (Bloch group, algebraic K-theory, quaternionic trace fields), which will be used in the description of fermions. Here, we choose the description of 3-manifolds by branched covers. Every 3-manifold can be described by a 3-fold branched cover of S3 branched along a knot. In case of knot complements, one will obtain a 3-fold branched cover of the 3-disk D3 branched along a 3-braid or 3-braids describing fermions. The whole approach will uncover new symmetries as induced by quantum and discrete groups. Using the Drinfeld–Turaev quantization, we will also construct a quantization so that quantum states correspond to knots. Particle properties like the electric charge must be expressed by topology, and we will obtain the right spectrum of possible values. Finally, we will get a connection to recent models of Furey, Stoica and Gresnigt using octonionic and quaternionic algebras with relations to 3-braids (Bilson–Thompson model). -
Effective Field Theories for Interacting Boundaries of 3D Topological
www.nature.com/scientificreports OPEN Efective feld theories for interacting boundaries of 3D topological crystalline insulators through bosonisation Patricio Salgado‑Rebolledo1*, Giandomenico Palumbo2 & Jiannis K. Pachos1 Here, we analyse two Dirac fermion species in two spatial dimensions in the presence of general quartic contact interactions. By employing functional bosonisation techniques, we demonstrate that depending on the couplings of the fermion interactions the system can be efectively described by a rich variety of topologically massive gauge theories. Among these efective theories, we obtain an extended Chern–Simons theory with higher order derivatives as well as two coupled Chern–Simons theories. Our formalism allows for a general description of interacting fermions emerging, for example, at the gapped boundary of three‑dimensional topological crystalline insulators. Time-reversal-invariant topological insulators are among the most well studied topological phases of matter. In three dimensions, they are characterised by suitable topological numbers in the bulk that guarantee the existence 1,2 of topologically protected massless Dirac fermions on the boundary . Although the topological invariant is a Z2 number, on the slab geometry, it has been shown that robust surface states are given by an odd number of Dirac fermions per boundary3. Te situation changes in the case of three-dimensional topological crystalline insula- tors (TCIs), namely topological insulators characterised by further crystalline symmetries, such as mirror and rotation symmetries4–11. In particular, for three-dimensional TCIs protected by a single mirror symmetry, one can defne the so called mirror Chern number nM on a given two-dimensional plane, which is invariant under 5 the mirror symmetry. -
VARIATIONAL ANALYSIS of the THIRRING MODEL* Sidney
SLAC-PUB-1999 August 1977 (T) FERMION FIELD THEORY ON A LATTICE: VARIATIONAL ANALYSIS OF THE THIRRING MODEL* Sidney D. Drell, Benjamin Svetitsky**, and Marvin Weinstein Stanford Linear Accelerator Center Stanford University, Stanford, California 94305 Abstract We extend variational techniques previously described to study the two-dimensional massless free fermion field and the Thirring model on a spatial lattice, The iterative block spin procedure of con- structing an effective lattice Hamiltonian, starting ,by dissecting the lattice into Z-site blocks, is shown to be successful in producing results known for the continuum Thirring model. Submitted to Phys . Rev. *Work supported by the Energy Research and Development Administration, **National Science Foundation Graduate Fellow in absentia from Princeton University. -2- 1. INTRODUCTION I,n this paper we continue the development and application of techniques for finding the ground state and spectrum of low-lying physical states of field the- ories without recourse to either weak or strong coupling expansioas. Following 1 our earlier papers we study lattice Hamiltonians by means of a constructive variational procedure. The methods, which in our preceding paper (Paper III) were described and applied to free field theory of bosons in oae space dimension and to the one-dimensional Ising model with a transverse applied mag.netic field, are now applied to two fermion theories in lx - It dimensions: massless free 2-5 fermions and the Thirring .model. Our aim in this paper is to demonstrate that these methods are easily applied to fermion theories and that our simple con- structive approach reproduces results known to hold in soluble continuum models. -
Amplitudes in the Spin Foam Approach to Quantum Gravity
Amplitudes in the Spin Foam Approach to Quantum Gravity by Lin-Qing Chen 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, 2017 c Lin-Qing Chen 2017 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 Jesus Fernando Barbero Gonzalez Prof. Supervisor Lee Smolin Prof. Co-supervisor Laurent Freidel Prof. Internal Member Niayesh Afshordi Prof. Committee Member Bianca Dittrich Prof. Internal-external Examiner Eduardo Martin-Martinez Prof. ii This thesis consists of material all of which I authored or co-authored: see Statement of Con- tributions 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 The construction of the holomorphic Spin Foam model and the calculation of Pachner Moves have been done in collaboration with Andrzej Banburski and Jeff Hnybida, which was supervised by Laurent Freidel. The asymptotics is based on work in collaboration with Andrzej Banburski. The rest of the original results are based solely on my own work. The publications related with this thesis: L. Q. Chen, “Bulk amplitude and degree of divergence in 4d spin foams,” Phys. Rev. D 94, no. 10, 104025 (2016) A. Banburski and L. Q. Chen, “Simpler way of imposing simplicity constraints,” Phys. Rev. D 94, no. 10, 104003 (2016) A. -
Towards a Bulk Description of Higher Spin SYK
Prepared for submission to JHEP TUW–18–02 Towards a bulk description of higher spin SYK Hern´anA. Gonz´alez,Daniel Grumiller, and Jakob Salzer Institute for Theoretical Physics, TU Wien, Wiedner Hauptstr. 8-10/136, A-1040 Vienna, Austria E-mail: hgonzale@, grumil@, [email protected] Abstract: We consider on the bulk side extensions of the Sachdev{Ye{Kitaev (SYK) model to Yang{Mills and higher spins. To this end we study generalizations of the Jackiw{ Teitelboim (JT) model in the BF formulation. Our main goal is to obtain generalizations of the Schwarzian action, which we achieve in two ways: by considering the on-shell action supplemented by suitable boundary terms compatible with all symmetries, and by applying the Lee{Wald{Zoupas formalism to analyze the symplectic structure of dilaton gravity. We conclude with a discussion of the entropy (including log-corrections from higher spins) and a holographic dictionary for the generalized SYK/JT correspondence. Keywords: two-dimensional dilaton gravity, asymptotically anti-de Sitter, Jackiw{Teitelboim model, Poisson sigma model, Sachdev{Ye{Kitaev model, generalized Schwarzian action, higher spin theories, Einstein-dilaton{Yang{Mills gravity arXiv:1802.01562v2 [hep-th] 12 Feb 2018 Contents 1 Introduction2 2 Dilaton gravity as generalized BF-theory4 2.1 Bulk action and equations of motion5 2.2 Observables5 2.3 Action principle7 3 Jackiw{Teitelboim model8 3.1 Boundary and integrability conditions8 3.2 Action principle and on-shell action9 3.3 Boundary action from Casimir 10 4 Yang{Mills -
Topological Gravity on (D, N)−Shift Superspace Formulation
Topological Gravity on (D, N)−Shift Superspace Formulation J. A. Louren¸coa,b,d, J. A. Helay¨el Netob, W. Spalenzab,c,d a Universidade Federal do Esp´ırito Santo, Campus S˜ao Mateus (UFES) Brazil. b Centro Brasileiro de Pesquisas F´ısicas (CBPF) Brazil. c Instituto Federal do Esp´ırito Santo, Campus Cariacica (IFES) Brazil. d Grupo de Pesquisa em F´ısica Te´orica (GPFT-IFES). E-mails: [email protected], [email protected], [email protected] Abstract In this contribution, we re-assess the subject of topological gravity by following the Shift Supersymmetry formalism. The gauge-fixing of the theory goes under the Batallin-Vilkovisky (BV) prescription based on a diagram that contains both ghost and anti-ghost superfields, associated to the super-vielbein and the super-Lorentz connection. We extend the formulation of the topological gravity action to an arbitrary number of dimensions of the shift superspace by adopting a formulation based on the gauge-fixing for BF-type models. 1 Introduction Topological field theories have been introduced by Witten [1] and soon after applied in several areas that describe quantum-mechanical and quantum field-theoretical systems. Over the recent years, they have been applied to study non-perturbative quantum gravity [2], the issues of topo- logical phases, spin foam, Loop Quantum Gravity, a topological approach to the cosmological constant and a number of other relevant applications. One of the basic topics for the construction of Topological Gravity are the topological Yang-Mills theories, by now fairly-well discussed and understood. However, on the other hand, the complexity of the symmetry groups and Lagrangians in topological gravity renders difficult the comparison between the results obtained by using dif- ferent formalisms.