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DC Field | Value | Language |
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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 |
Appears in Collections: | IIAP Publications |
Files in This Item:
File | Description | Size | Format | |
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Nayak R. K.pdf | 67.08 kB | Adobe PDF | View/Open |
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