Electromagnetic fields in space-times with local rotational symmetry

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1254

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DC Field	Value	Language
dc.contributor.author	Dhurandhar, S.V.	-
dc.contributor.author	Vishveshwara, C.V.	-
dc.contributor.author	Cohen, J.M.	-
dc.date.accessioned	2006-05-16T10:14:14Z	-
dc.date.available	2006-05-16T10:14:14Z	-
dc.date.issued	1980-05-15	-
dc.identifier.citation	Physical Review D, 1980, Vol.21, 2794-2804	en
dc.identifier.issn	1550-7998	-
dc.identifier.uri	http://hdl.handle.net/2289/1254	-
dc.description.abstract	The Debye-potential formalism is applied to perfect-fluid space-times with local rotational symmetry which form a subclass of the generalized Goldberg-Sachs space-times. A decoupled equation for the potentials is obtained. It is seen that this equation yields a considerable amount of information in its general form without specializing to any example of the subclass. Finally some particular space-times, namely, Kantowski-Sachs universes, Taub space, and anisotropic spatially homogeneous cosmological models, are discussed in detail.	en
dc.format.extent	1486786 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/v21/p2794	en
dc.rights	(1980) by the American Physical Society	en
dc.title	Electromagnetic fields in space-times with local rotational symmetry	en
dc.type	Article	en
Appears in Collections:	Research Papers (TP)

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