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Semiclassical Loop Quantum Gravity and Black Hole Thermodynamics

Vernadsky National Library of Ukraine

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Title Semiclassical Loop Quantum Gravity and Black Hole Thermodynamics
 
Creator Dasgupta, A.
 
Description In this article we explore the origin of black hole thermodynamics using semiclassical states in loop quantum gravity. We re-examine the case of entropy using a density matrix for a coherent state and describe correlations across the horizon due to SU(2) intertwiners. We further show that Hawking radiation is a consequence of a non-Hermitian term in the evolution operator, which is necessary for entropy production or depletion at the horizon. This non-unitary evolution is also rooted in formulations of irreversible physics.
 
Date 2019-02-19T18:58:05Z
2019-02-19T18:58:05Z
2013
 
Type Article
 
Identifier Semiclassical Loop Quantum Gravity and Black Hole Thermodynamics / A. Dasgupta // Symmetry, Integrability and Geometry: Methods and Applications. — 2013. — Т. 9. — Бібліогр.: 43 назв. — англ.
1815-0659
2010 Mathematics Subject Classification: 83C57; 81Q35; 81T20
DOI: http://dx.doi.org/10.3842/SIGMA.2013.013
http://dspace.nbuv.gov.ua/handle/123456789/149217
 
Language en
 
Relation Symmetry, Integrability and Geometry: Methods and Applications
 
Publisher Інститут математики НАН України