Black Holes in Non-flat Backgrounds: the Schwarzschild Black Hole in the Einstein Universe

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dc.creatorNayak, K. Rajesh
dc.creatorMacCallum, M. A. H.
dc.creatorVishveshwara, C. V.
dc.date2000-06-12
dc.date2000-10-24
dc.date.accessioned2026-07-07T11:46:15Z
dc.date.available2026-07-07T11:46:15Z
dc.descriptionAs an example of a black hole in a non-flat background a composite static spacetime is constructed. It comprises a vacuum Schwarzschild spacetime for the interior of the black hole across whose horizon it is matched on to the spacetime of Vaidya representing a black hole in the background of the Einstein universe. The scale length of the exterior sets a maximum to the black hole mass. To obtain a non-singular exterior, the Vaidya metric is matched to an Einstein universe. The behaviour of scalar waves is studied in this composite model.
dc.description8 pages, 3 postscript figures, minor corrections Journal Ref: accepted for Physical Review D
dc.identifierhttps://arxiv.org/abs/gr-qc/0006040
dc.identifierhttp://arxiv.org/abs/gr-qc/0006040
dc.identifierPhys.Rev.D63:024020,2001
dc.identifierdoi:10.1103/PhysRevD.63.024020
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/202157
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleBlack Holes in Non-flat Backgrounds: the Schwarzschild Black Hole in the Einstein Universe
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