Semiclassical Loop Quantum Gravity and Black Hole Thermodynamics

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 ra...

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Дата:2013
Автор: Dasgupta, A.
Формат: Стаття
Мова:English
Опубліковано: Інститут математики НАН України 2013
Назва видання:Symmetry, Integrability and Geometry: Methods and Applications
Онлайн доступ:http://dspace.nbuv.gov.ua/handle/123456789/149217
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Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Цитувати:Semiclassical Loop Quantum Gravity and Black Hole Thermodynamics / A. Dasgupta // Symmetry, Integrability and Geometry: Methods and Applications. — 2013. — Т. 9. — Бібліогр.: 43 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
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spelling irk-123456789-1492172019-02-20T01:29:09Z Semiclassical Loop Quantum Gravity and Black Hole Thermodynamics Dasgupta, A. 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. 2013 Article 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 en Symmetry, Integrability and Geometry: Methods and Applications Інститут математики НАН України
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
language English
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.
format Article
author Dasgupta, A.
spellingShingle Dasgupta, A.
Semiclassical Loop Quantum Gravity and Black Hole Thermodynamics
Symmetry, Integrability and Geometry: Methods and Applications
author_facet Dasgupta, A.
author_sort Dasgupta, A.
title Semiclassical Loop Quantum Gravity and Black Hole Thermodynamics
title_short Semiclassical Loop Quantum Gravity and Black Hole Thermodynamics
title_full Semiclassical Loop Quantum Gravity and Black Hole Thermodynamics
title_fullStr Semiclassical Loop Quantum Gravity and Black Hole Thermodynamics
title_full_unstemmed Semiclassical Loop Quantum Gravity and Black Hole Thermodynamics
title_sort semiclassical loop quantum gravity and black hole thermodynamics
publisher Інститут математики НАН України
publishDate 2013
url http://dspace.nbuv.gov.ua/handle/123456789/149217
citation_txt Semiclassical Loop Quantum Gravity and Black Hole Thermodynamics / A. Dasgupta // Symmetry, Integrability and Geometry: Methods and Applications. — 2013. — Т. 9. — Бібліогр.: 43 назв. — англ.
series Symmetry, Integrability and Geometry: Methods and Applications
work_keys_str_mv AT dasguptaa semiclassicalloopquantumgravityandblackholethermodynamics
first_indexed 2023-05-20T17:32:15Z
last_indexed 2023-05-20T17:32:15Z
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