On the Entropy of Quantum Fields in Black Hole Backgrounds

dc.creatorde Alwis, S. P.
dc.creatorOhta, N.
dc.date1994-12-03
dc.date1994-12-15
dc.date.accessioned2026-07-07T09:03:52Z
dc.date.available2026-07-07T09:03:52Z
dc.descriptionWe show that the partition function for a scalar field in a static spacetime background can be expressed as a functional integral in the corresponding optical space, and point out that the difference between this and the functional integral in the original metric is a Liouville type action. A general formula for the free energy is derived in the high temperature approximation and applied to various cases. In particular we find that thermodynamics in the extremal Reissner-Nordström space has extra singularities that make it ill-defined.
dc.description10 pages, phyzzx (added references)
dc.identifierhttps://arxiv.org/abs/hep-th/9412027
dc.identifierhttp://arxiv.org/abs/hep-th/9412027
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/149174
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleOn the Entropy of Quantum Fields in Black Hole Backgrounds
dc.typetext

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