Scattering by black holes: a simulated potential approach

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2978

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DC Field	Value	Language
dc.contributor.author	Aguirregabiria, J. M	-
dc.contributor.author	Vishveshwara, C. V	-
dc.date.accessioned	2008-08-04T10:15:28Z	-
dc.date.available	2008-08-04T10:15:28Z	-
dc.date.issued	1996-01	-
dc.identifier.citation	Physics Letters A, Vol. 210, No. 4 - 5, pp. 251 - 254	en
dc.identifier.issn	0375-9601	-
dc.identifier.uri	http://hdl.handle.net/2248/2978	-
dc.description	Restricted Access	-
dc.description.abstract	The effective potential appearing in the scattering of scalar, electromagnetic and gravitational waves by a Schwarzschild black hole is replaced with potentials for which the exact analytical solutions are known. It is shown that the simulated potentials provide an easy way to obtain some results (the reflection coefficient, or the shape of scattered wave packets, for instance) that compare well with those that can be obtained by numerical integration of the exact potential. Some results pertaining to quasinormal modes are also discussed.	en
dc.format.extent	3894 bytes	-
dc.format.mimetype	application/pdf	-
dc.language.iso	en	en
dc.publisher	Elsevier B.V	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1996PhLA..210..251A	en
dc.subject	Black Holes: scattering	en
dc.title	Scattering by black holes: a simulated potential approach	en
dc.type	Article	en
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