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Electromagnetic fields in space-times with local rotational symmetry

dc.contributor.authorDhurandhar, S V
dc.contributor.authorVishveshwara, C V
dc.contributor.authorCohen, J M
dc.date.accessioned2006-05-16T10:14:14Z
dc.date.available2006-05-16T10:14:14Z
dc.date.issued1980-05-15
dc.description.abstractThe 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.extent1486786 bytes
dc.format.mimetypeapplication/pdf
dc.identifier.citationPhysical Review D, 1980, Vol.21, 2794-2804en
dc.identifier.issn1550-7998
dc.identifier.urihttp://hdl.handle.net/2289/1254
dc.language.isoenen
dc.publisherThe American Physical Societyen
dc.relation.urihttp://link.aps.org/abstract/PRD/v21/p2794en
dc.rights(1980) by the American Physical Societyen
dc.titleElectromagnetic fields in space-times with local rotational symmetryen
dc.typeArticleen

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