Covariant path integrals and black holes

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dc.creatorVendrell, F.
dc.creatorOrtiz, M. E.
dc.date1997-10-08
dc.date.accessioned2026-07-07T03:31:50Z
dc.date.available2026-07-07T03:31:50Z
dc.descriptionThe thermal nature of the propagator in a collapsed black-hole spacetime is shown to follow from the non-trivial topology of the configuration space in tortoise coordinates by using the path integral formalism.
dc.description5 pages, Revtex, 1 figure. To appear in the proceedings of the Eighth Marcel Grossmann Meeting on General Relativity. (Jerusalem, Israel, June 1997)
dc.identifierhttps://arxiv.org/abs/gr-qc/9710050
dc.identifierhttp://arxiv.org/abs/gr-qc/9710050
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/36010
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleCovariant path integrals and black holes
dc.typetext

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