Thermodynamics in Loop Quantum Cosmology

Loop quantum cosmology (LQC) is very powerful to deal with the behavior of early universe. Moreover, the effective loop quantum cosmology gives a successful description of the universe in the semiclassical region. We consider the apparent horizon of the Friedmann-Robertson-Walker universe as a therm...

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Main Authors: Li-Fang Li, Jian-Yang Zhu
Format: Article
Language:English
Published: Wiley 2009-01-01
Series:Advances in High Energy Physics
Online Access:http://dx.doi.org/10.1155/2009/905705
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author Li-Fang Li
Jian-Yang Zhu
author_facet Li-Fang Li
Jian-Yang Zhu
author_sort Li-Fang Li
collection DOAJ
description Loop quantum cosmology (LQC) is very powerful to deal with the behavior of early universe. Moreover, the effective loop quantum cosmology gives a successful description of the universe in the semiclassical region. We consider the apparent horizon of the Friedmann-Robertson-Walker universe as a thermodynamical system and investigate the thermodynamics of LQC in the semiclassical region. The effective density and effective pressure in the modified Friedmann equation from LQC not only determine the evolution of the universe in LQC scenario but also are actually found to be the thermodynamic quantities. This result comes from the energy definition in cosmology (the Misner-Sharp gravitational energy) and is consistent with thermodynamic laws. We prove that within the framework of loop quantum cosmology, the elementary equation of equilibrium thermodynamics is still valid.
format Article
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institution Kabale University
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publishDate 2009-01-01
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series Advances in High Energy Physics
spelling doaj-art-b9286d2cdfc64fb9a4817fdbe028c9222025-02-03T01:20:49ZengWileyAdvances in High Energy Physics1687-73571687-73652009-01-01200910.1155/2009/905705905705Thermodynamics in Loop Quantum CosmologyLi-Fang Li0Jian-Yang Zhu1Department of Physics, Beijing Normal University, Beijing 100875, ChinaDepartment of Physics, Beijing Normal University, Beijing 100875, ChinaLoop quantum cosmology (LQC) is very powerful to deal with the behavior of early universe. Moreover, the effective loop quantum cosmology gives a successful description of the universe in the semiclassical region. We consider the apparent horizon of the Friedmann-Robertson-Walker universe as a thermodynamical system and investigate the thermodynamics of LQC in the semiclassical region. The effective density and effective pressure in the modified Friedmann equation from LQC not only determine the evolution of the universe in LQC scenario but also are actually found to be the thermodynamic quantities. This result comes from the energy definition in cosmology (the Misner-Sharp gravitational energy) and is consistent with thermodynamic laws. We prove that within the framework of loop quantum cosmology, the elementary equation of equilibrium thermodynamics is still valid.http://dx.doi.org/10.1155/2009/905705
spellingShingle Li-Fang Li
Jian-Yang Zhu
Thermodynamics in Loop Quantum Cosmology
Advances in High Energy Physics
title Thermodynamics in Loop Quantum Cosmology
title_full Thermodynamics in Loop Quantum Cosmology
title_fullStr Thermodynamics in Loop Quantum Cosmology
title_full_unstemmed Thermodynamics in Loop Quantum Cosmology
title_short Thermodynamics in Loop Quantum Cosmology
title_sort thermodynamics in loop quantum cosmology
url http://dx.doi.org/10.1155/2009/905705
work_keys_str_mv AT lifangli thermodynamicsinloopquantumcosmology
AT jianyangzhu thermodynamicsinloopquantumcosmology