Entropy of Extremal Black Hole Solutions of String Theory

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dc.creatorGhosh, A.
dc.creatorMitra, P.
dc.date1995-09-15
dc.date1995-09-29
dc.date.accessioned2026-07-07T09:04:06Z
dc.date.available2026-07-07T09:04:06Z
dc.descriptionFor extremal black holes, the thermodynamic entropy is not proportional to the area. The general form allowed by thermodynamics is worked out for three classes of extremal black hole solutions of string theory and shown to be consistent with the entropy calculated from the density of elementary string states. On the other hand, the entanglement entropy does not in general agree with these results.
dc.description12 pages, harvmac (minor errors corrected)
dc.identifierhttps://arxiv.org/abs/hep-th/9509090
dc.identifierhttp://arxiv.org/abs/hep-th/9509090
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/149252
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleEntropy of Extremal Black Hole Solutions of String Theory
dc.typetext

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