Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/3249
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dc.contributor.authorDhurandhar, S.V.-
dc.contributor.authorVishveshwara, C.V.-
dc.contributor.authorCohen, J.M.-
dc.date.accessioned2007-07-12T05:59:36Z-
dc.date.available2007-07-12T05:59:36Z-
dc.date.issued1984-01-
dc.identifier.citationClassical and Quantum Gravity, 1984, Vol.1, p61-69en
dc.identifier.issn0264-9381-
dc.identifier.urihttp://hdl.handle.net/2289/3249-
dc.descriptionRestricted Access.en
dc.description.abstractThe Hertz-Debye superpotential formalism has been applied to study the behaviour of the perturbative zero rest-mass fields, namely, the electromagnetic, massless neutrino and gravitational fields in the rotationally symmetric Kasner Universe. The formalism yields a single decoupled equation for the superpotential in each of the three cases. A considerable amount of information is obtained from these equations themselves and the equations are subjected to various methods of solution. The effects of anisotropy of the Kasner space-time on the superposed fields are analysed. The relative behaviour of the three fields is studied with the similarities and differences in their evolution being highlighted. Finally in the geometric optics approximation the propagation of the fields is compared with the null geodesics.en
dc.format.extent406659 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherIOP Publishing Ltden
dc.relation.urihttp://dx.doi.org/10.1088/0264-9381/1/1/009en
dc.rights1984 IOP Publishing Ltd.en
dc.titleElectromagnetic, neutrino and gravitational fields in the Kasner space-time with rotational symmetryen
dc.typeArticleen
Appears in Collections:Research Papers (TP)

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