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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3088
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dc.contributor.authorNayak, R. K-
dc.contributor.authorMacCallum, M. A-
dc.contributor.authorVishveshwara, C. V-
dc.date.accessioned2008-08-12T09:23:04Z-
dc.date.available2008-08-12T09:23:04Z-
dc.date.issued2001-01-
dc.identifier.citationPhysical Review D, Vol. 63, No. 2, pp. 024020en
dc.identifier.issn0556-2821-
dc.identifier.urihttp://hdl.handle.net/2248/3088-
dc.description.abstractAs 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 onto 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 behavior of scalar waves is studied in this composite model.en
dc.format.extent68688 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherThe American Physical Societyen
dc.relation.urihttp://link.aps.org/abstract/PRD/v63/e024020en
dc.subjectBlack Holeen
dc.subjectScalar Waves, Einstein Universeen
dc.titleBlack holes in nonflat backgrounds: The Schwarzschild black hole in the Einstein universeen
dc.typeArticleen
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