Search results for "Loop quantum gravity"

showing 10 items of 16 documents

U(N) tools for loop quantum gravity: the return of the spinor

2011

We explore the classical setting for the U(N) framework for SU(2) intertwiners for loop quantum gravity (LQG) and describe the corresponding phase space in terms of spinors with appropriate constraints. We show how its quantization leads back to the standard Hilbert space of intertwiner states defined as holomorphic functionals. We then explain how to glue these intertwiners states in order to construct spin network states as wave-functions on the spinor phase space. In particular, we translate the usual loop gravity holonomy observables to our classical framework. Finally, we propose how to derive our phase space structure from an action principle which induces non-trivial dynamics for the…

High Energy Physics - TheoryPhysics and Astronomy (miscellaneous)FOS: Physical sciencesLoop quantum gravityGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciencesGeneral Relativity and Quantum Cosmologysymbols.namesake0103 physical sciences010306 general physicsWave functionMathematical PhysicsMathematical physicsPhysicsSpinor010308 nuclear & particles physicsHilbert spaceObservableMathematical Physics (math-ph)High Energy Physics - Theory (hep-th)Phase spacePhysical Sciencessymbols[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Quantum gravitySpin network
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Computing black hole entropy in loop quantum gravity from a conformal field theory perspective

2009

Motivated by the analogy proposed by Witten between Chern-Simons and conformal field theories, we explore an alternative way of computing the entropy of a black hole starting from the isolated horizon framework in loop quantum gravity. The consistency of the result opens a window for the interplay between conformal field theory and the description of black holes in loop quantum gravity.

High Energy Physics - TheoryPhysics010308 nuclear & particles physicsConformal field theoryAstrophysics::High Energy Astrophysical PhenomenaGravityFOS: Physical sciencesAstronomy and AstrophysicsConformal mapGeneral Relativity and Quantum Cosmology (gr-qc)Loop quantum gravity01 natural sciencesGeneral Relativity and Quantum CosmologyBlack holeQuantum black holesHigh Energy Physics::TheoryGeneral Relativity and Quantum CosmologyTheoretical physicsHigh Energy Physics - Theory (hep-th)0103 physical sciences010306 general physicsBlack hole thermodynamicsEntropy (arrow of time)Journal of Cosmology and Astroparticle Physics
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Quantum geometry and microscopic black hole entropy

2006

9 pages, 6 figures.-- PACS nrs.: 04.60.Pp, 04.70.Dy.-- ISI Article Identifier: 000242448900013.-- Published online on Nov 28, 2006.

High Energy Physics - TheoryPhysicsQuantum geometryPhysics and Astronomy (miscellaneous)LogarithmEntropy (statistical thermodynamics)Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Loop quantum gravityGeneral Relativity and Quantum CosmologyBlack holeGeneral Relativity and Quantum Cosmologysymbols.namesakeHigh Energy Physics - Theory (hep-th)[PACS] Quantum aspects of black holes evaporation thermodynamicssymbolsPlanckBlack hole thermodynamicsQuantum[PACS] Loop quantum gravity quantum geometry spin foamsMathematical physics
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Statistical Thermodynamics of Polymer Quantum Systems

2011

Polymer quantum systems are mechanical models quantized similarly as loop quantum gravity. It is actually in quantizing gravity that the polymer term holds proper as the quantum geometry excitations yield a reminiscent of a polymer material. In such an approach both non-singular cosmological models and a microscopic basis for the entropy of some black holes have arisen. Also important physical questions for these systems involve thermodynamics. With this motivation, in this work, we study the statistical thermody- namics of two one dimensional polymer quantum systems: an ensemble of oscillators that describe a solid and a bunch of non-interacting particles in a box, which thus form an ideal…

Length scaleHigh Energy Physics - TheoryCanonical quantizationThermodynamicsFOS: Physical sciencesLoop quantum gravityGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyQuantization (physics)canonical quantizationQuantum mechanicsstatistical thermodynamicsQuantumBlack hole thermodynamicsMathematical PhysicsCondensed Matter - Statistical MechanicsPhysicsQuantum geometryQuantitative Biology::BiomoleculesStatistical Mechanics (cond-mat.stat-mech)loop quantum gravitylcsh:Mathematics82B30 81S05 81Q65 82B20 83C45lcsh:QA1-939Ideal gasCondensed Matter::Soft Condensed MatterClassical mechanicsHigh Energy Physics - Theory (hep-th)Geometry and TopologyAnalysis
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New solutions of the hamiltonian and diffeomorphism constraints of quantum gravity from a highest weight loop representation

1991

Abstract We introduce a highest weight type representation of the Rovelli-Smolin algebra of loop observables for quantum gravity. In terms of this representation, new solutions of the hamiltonian and diffeomorphism constraints are given. Assuming the locality of the quantum hamiltonian constraint we show that any functional depending on the generalized link class of the disjoint union of arbitrary simple loops is a solution. Finally we argue that this is the general solution in the irreducible representation space.

PhysicsGeneral Relativity and Quantum CosmologyNuclear and High Energy PhysicsPure mathematicsHamiltonian constraintQuantum mechanicsIrreducible representationTrivial representationWheeler–DeWitt equationQuantum gravityLoop quantum gravityCanonical quantum gravityDiffeomorphism constraintPhysics Letters B
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The Quantum Scalar Field in Spherically Symmetric Loop Quantum Gravity

2013

We consider the quantization of a spherically symmetric gravitational system coupled to a massless scalar field within the loop quantum gravity framework. Our results rely on the uniform discretizations method developed during the last years. We minimize the associated discrete “master constraint” using a trial state whose gravitational part is peaked around the classical Schwarzschild solution.

PhysicsGeneral Relativity and Quantum CosmologyQuantization (physics)Quantum geometryClassical mechanicsSpin foamQuantum gravitySemiclassical gravityLoop quantum gravityScalar fieldLoop quantum cosmology
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Revisiting the quantum scalar field in spherically symmetric quantum gravity

2012

We extend previous results in spherically symmetric gravitational systems coupled with a massless scalar field within the loop quantum gravity framework. As starting point, we take the Schwarzschild spacetime. The results presented here rely on the uniform discretization method. We are able to minimize the associated discrete master constraint using a variational method. The trial state for the vacuum consists of a direct product of a Fock vacuum for the matter part and a Gaussian centered around the classical Schwarzschild solution. This paper follows the line of research presented by Gambini, Pullin and Rastgoo and a comparison between their result and the one given in this work is made.

PhysicsGravitationGeneral Relativity and Quantum CosmologyVariational methodPhysics and Astronomy (miscellaneous)Schwarzschild metricQuantum gravityLoop quantum gravityScalar fieldSchwarzschild radiusGeneral Relativity and Quantum CosmologyFock spaceMathematical physics
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Super-entropic black hole with Immirzi hair

2020

In the context of $f(R)$ generalizations to the Holst action, endowed with a dynamical Immirzi field, we derive an analytic solution describing asymptotically anti--de Sitter black holes with hyperbolic horizon. These exhibit a scalar hair of the second kind, which ultimately depends on the Immirzi field radial behavior. In particular, we show how the Immirzi field modifies the usual entropy law associated to the black hole. We also verify that the Immirzi field boils down to a constant value in the asymptotic region, thus restoring the standard loop quantum gravity picture. We finally prove the violation of the reverse isoperimetric inequality, resulting in the superentropic nature of the …

PhysicsHigh Energy Physics - TheoryField (physics)HorizonScalar (mathematics)FOS: Physical sciencesContext (language use)Loop quantum gravityGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyBlack holeGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)Isoperimetric inequalityEntropy (arrow of time)Mathematical physics
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Generalized Ashtekar variables for Palatini f(R) models

2021

We consider special classes of Palatini f(R) theories, featured by additional Loop Quantum Gravity inspired terms, with the aim of identifying a set of modified Ashtekar canonical variables, which still preserve the SU(2) gauge structure of the standard theory. In particular, we allow for affine connection to be endowed with torsion, which turns out to depend on the additional scalar degree affecting Palatini f(R) gravity, and in this respect we successfully construct a novel Gauss constraint. We analyze the role of the additional scalar field, outlining as it acquires a dynamical character by virtue of a non vanishing Immirzi parameter, and we describe some possible effects on the area ope…

PhysicsHigh Energy Physics - TheoryNuclear and High Energy Physics010308 nuclear & particles physicsImmirzi parameterGaussScalar (mathematics)FOS: Physical sciencesLoop quantum gravityGeneral Relativity and Quantum Cosmology (gr-qc)Affine connection01 natural sciencesGeneral Relativity and Quantum CosmologyAshtekar variablessymbols.namesakeGeneral Relativity and Quantum CosmologyHigh Energy Physics - Theory (hep-th)0103 physical sciencessymbolslcsh:QC770-798lcsh:Nuclear and particle physics. Atomic energy. RadioactivityEinstein010306 general physicsScalar fieldMathematical physics
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Loop quantum gravity and Planck-size black hole entropy

2007

The Loop Quantum Gravity (LQG) program is briefly reviewed and one of its main applications, namely the counting of black hole entropy within the framework is considered. In particular, recent results for Planck size black holes are reviewed. These results are consistent with an asymptotic linear relation (that fixes uniquely a free parameter of the theory) and a logarithmic correction with a coefficient equal to -1/2. The account is tailored as an introduction to the subject for non-experts.

PhysicsHistoryLogarithmFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Loop quantum gravityLinear-quadratic-Gaussian controlGeneral Relativity and Quantum CosmologyComputer Science ApplicationsEducationsymbols.namesakeTheoretical physicsGeneral Relativity and Quantum CosmologysymbolsLinear relationPlanckBlack hole thermodynamicsFree parameter
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