Logarithmic correction to the Bekenstein-Hawking entropy

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dc.creatorKaul, Romesh K.
dc.creatorMajumdar, Parthasarathi
dc.date2000-02-10
dc.date2000-06-14
dc.date.accessioned2026-07-07T10:31:53Z
dc.date.available2026-07-07T10:31:53Z
dc.descriptionThe exact formula derived by us earlier for the entropy of a four dimensional non-rotating black hole within the quantum geometry formulation of the event horizon in terms of boundary states of a three dimensional Chern-Simons theory, is reexamined for large horizon areas. In addition to the {\it semiclassical} Bekenstein-Hawking contribution to the area obtained earlier, we find a contribution proportional to the logarithm of the area together with subleading corrections that constitute a series in inverse powers of the area.
dc.description4 pages in Revtex format, one eps figure; version published in Physical Review Letters
dc.identifierhttps://arxiv.org/abs/gr-qc/0002040
dc.identifierhttp://arxiv.org/abs/gr-qc/0002040
dc.identifierPhys.Rev.Lett.84:5255-5257,2000
dc.identifierdoi:10.1103/PhysRevLett.84.5255
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/178573
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleLogarithmic correction to the Bekenstein-Hawking entropy
dc.typetext

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