Mapping Hawking into Unruh Thermal Properties

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dc.creatorDeser, S.
dc.creatorLevin, Orit
dc.date1998-09-21
dc.date.accessioned2026-07-07T11:48:13Z
dc.date.available2026-07-07T11:48:13Z
dc.descriptionBy globally embedding curved spaces into higher dimensional flat ones, we show that Hawking thermal properties map into their Unruh equivalents: The relevant curved space detectors become Rindler ones, whose temperature and entropy reproduce the originals. Specific illustrations include Schwarzschild, Schwarzschild-(anti)deSitter, Reissner-Nordstrom and BTZ spaces.
dc.description10 pages
dc.identifierhttps://arxiv.org/abs/hep-th/9809159
dc.identifierhttp://arxiv.org/abs/hep-th/9809159
dc.identifierPhys.Rev.D59:064004,1999
dc.identifierdoi:10.1103/PhysRevD.59.064004
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/202845
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleMapping Hawking into Unruh Thermal Properties
dc.typetext

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