Entropy and topology for manifolds with boundaries

dc.creatorLiberati, Stefano
dc.creatorPollifrone, Giuseppe
dc.date1995-09-15
dc.date1995-09-19
dc.date.accessioned2026-07-07T09:04:06Z
dc.date.available2026-07-07T09:04:06Z
dc.descriptionIn this work a deep relation between topology and thermodynamical features of manifolds with boundaries is shown. The expression for the Euler characteristic, through the Gauss- Bonnet integral, and the one for the entropy of gravitational instantons are proposed in a form which makes the relation between them self-evident. A generalization of Bekenstein-Hawking formula, in which entropy and Euler characteristic are related in the form $S=χA/8$, is obtained. This formula reproduces the correct result for extreme black hole, where the Bekenstein-Hawking one fails ($S=0$ but $A \neq 0$). In such a way it recovers a unified picture for the black hole entropy law. Moreover, it is proved that such a relation can be generalized to a wide class of manifolds with boundaries which are described by spherically symmetric metrics (e.g. Schwarzschild, Reissner-Nordström, static de Sitter).
dc.description19 pages, phyzzx, no figures
dc.identifierhttps://arxiv.org/abs/hep-th/9509093
dc.identifierhttp://arxiv.org/abs/hep-th/9509093
dc.identifierNucl.Phys.Proc.Suppl. 57 (1997) 197-200
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/149253
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleEntropy and topology for manifolds with boundaries
dc.typetext

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