Quantum spectrum and statistic entropy of black hole

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dc.creatorRen, Zhao
dc.creatorHuaifan, Li
dc.creatorShengli, Zhang
dc.date2006-10-16
dc.date.accessioned2026-07-07T07:28:01Z
dc.date.available2026-07-07T07:28:01Z
dc.descriptionTaking the horizon surface of the black hole as a compact membrane and solving the oscillation equation of this membrane by Klein-Gordon equation, we derive the frequencies of oscillation modes of the horizon surface, which are proportional to the radiation temperature of the black hole. However, the frequencies of oscillation modes are not equidistant. Using the distribution of obtained frequencies of oscillation mode we compute the statistic entropy of the black hole and obtain that the statistic entropy of the black hole is proportional to the area of the horizon. Therefore, it is proven that the quantum statistic entropy of the black hole is consistent with Bekenstein-Hawking entropy.
dc.description7 pages
dc.identifierhttps://arxiv.org/abs/gr-qc/0610077
dc.identifierhttp://arxiv.org/abs/gr-qc/0610077
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/117581
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleQuantum spectrum and statistic entropy of black hole
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