The Bekenstein-Hawking Entropy of Higher-Dimensional Rotating Black Holes

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dc.creatorMa, Zheng Ze
dc.date2005-12-12
dc.date2006-05-24
dc.date.accessioned2026-07-07T10:45:27Z
dc.date.available2026-07-07T10:45:27Z
dc.descriptionA black hole can be regarded as a thermodynamic system described by a grand canonical ensemble. In this paper, we study the Bekenstein-Hawking entropy of higher-dimensional rotating black holes using the Euclidean path-integral method of Gibbons and Hawking. We give a general proof demonstrating that ignoring quantum corrections, the Bekenstein-Hawking entropy is equal to one-fourth of its horizon area for general higher-dimensional rotating black holes.
dc.description9 pages, Latex, v2: arxiv-id for the references supplemented, v3: accepted for publication by Progress of Theoretical Physics
dc.identifierhttps://arxiv.org/abs/hep-th/0512130
dc.identifierhttp://arxiv.org/abs/hep-th/0512130
dc.identifierProg.Theor.Phys.115:863-871,2006
dc.identifierdoi:10.1143/PTP.115.863
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/182920
dc.subjectHigh Energy Physics - Theory
dc.titleThe Bekenstein-Hawking Entropy of Higher-Dimensional Rotating Black Holes
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