Physical effects in the Vaidya Einstein Kerr spacetime

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3597

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DC Field	Value	Language
dc.contributor.author	Ramachandra, B. S	-
dc.contributor.author	Vishveshwara, C. V	-
dc.date.accessioned	2008-09-12T15:43:04Z	-
dc.date.available	2008-09-12T15:43:04Z	-
dc.date.issued	2003-12	-
dc.identifier.citation	Classical and Quantum Gravity, Vol. 20, No. 24, pp. 5253 - 5273	en
dc.identifier.uri	http://hdl.handle.net/2248/3597	-
dc.description	Restricted Access	-
dc.description.abstract	We investigate some physical effects in the Vaidya Einstein Kerr (VEK) spacetime which represents the spacetime of the Kerr black-hole in the background of the non-flat Einstein universe. We have chosen for our study the nature of circular geodesics and the phenomenon of gyroscopic precession in the VEK spacetime. We show that the nature of the circular geodesics is radically altered by the presence of the background. Turning to gyroscopic precession we show that a novel feature emerges in that the background affects the precession in two different ways, one by coupling to rotation and another in a direct manner. We investigate also several special cases of general precession.	en
dc.language.iso	en	en
dc.publisher	Institute of Physics	en
dc.relation.uri	http://www.iop.org/EJ/abstract/0264-9381/20/24/002	en
dc.subject	Vaidya Einstein Kerr Spacetime	en
dc.subject	Einstein Universe	en
dc.title	Physical effects in the Vaidya Einstein Kerr spacetime	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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