Area law corrections from state counting and supergravity

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dc.creatorCardoso, Gabriel Lopes
dc.creatorde Wit, Bernard
dc.creatorMohaupt, Thomas
dc.date1999-10-22
dc.date.accessioned2026-07-07T10:34:27Z
dc.date.available2026-07-07T10:34:27Z
dc.descriptionModifications of the Bekenstein-Hawking area law for black holes are crucial in order to find agreement between the microscopic entropy based on state counting and the macroscopic entropy based on an effective field theory computation. We discuss this and related issues for the case of four-dimensional N=2 supersymmetric black holes. We also briefly comment on the state counting for N=4 and N=8 black holes.
dc.description10 pages, LaTeX; submitted to Proceedings of Strings 99
dc.identifierhttps://arxiv.org/abs/hep-th/9910179
dc.identifierhttp://arxiv.org/abs/hep-th/9910179
dc.identifierClass.Quant.Grav.17:1007-1015,2000
dc.identifierdoi:10.1088/0264-9381/17/5/310
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/179476
dc.subjectHigh Energy Physics - Theory
dc.titleArea law corrections from state counting and supergravity
dc.typetext

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