Black holes in nonflat backgrounds: The Schwarzschild black hole in the Einstein universe

dc.contributor.author	Nayak, R. K
dc.contributor.author	MacCallum, M. A
dc.contributor.author	Vishveshwara, C. V
dc.date.accessioned	2008-08-12T09:23:04Z
dc.date.available	2008-08-12T09:23:04Z
dc.date.issued	2001-01
dc.identifier.citation	Physical Review D, Vol. 63, No. 2, pp. 024020	en
dc.identifier.issn	0556-2821
dc.identifier.uri	http://hdl.handle.net/2248/3088
dc.description.abstract	As 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.extent	68688 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	The American Physical Society	en
dc.relation.uri	http://link.aps.org/abstract/PRD/v63/e024020	en
dc.subject	Black Hole	en
dc.subject	Scalar Waves, Einstein Universe	en
dc.title	Black holes in nonflat backgrounds: The Schwarzschild black hole in the Einstein universe	en
dc.type	Article	en