0000000000380727

AUTHOR

Alejandro Corichi

0000-0001-8196-6066

showing 3 related works from this author

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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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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Black Hole Entropy Quantization

2006

Ever since the pioneer works of Bekenstein and Hawking, black hole entropy has been known to have a quantum origin. Furthermore, it has long been argued by Bekenstein that entropy should be quantized in discrete (equidistant) steps given its identification with horizon area in (semi-)classical general relativity and the properties of area as an adiabatic invariant. This lead to the suggestion that black hole area should also be quantized in equidistant steps to account for the discrete black hole entropy. Here we shall show that loop quantum gravity, in which area is {\it not} quantized in equidistant steps can nevertheless be consistent with Bekenstein's equidistant entropy proposal in a s…

High Energy Physics - TheoryHolographic principlePhysicsWhite holeBlack hole information paradoxBekenstein boundFOS: Physical sciencesGeneral Physics and AstronomyGeneral Relativity and Quantum Cosmology (gr-qc)General Relativity and Quantum CosmologyGeneral Relativity and Quantum CosmologyTheoretical physicsClassical mechanicsHigh Energy Physics - Theory (hep-th)Extremal black holeBlack hole thermodynamicsBlack hole complementarityHawking radiationPhysical Review Letters
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