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Some anisotropic spatially-homogeneous cosmological models with electromagnetic field

dc.contributor.authorSingh T.; Srivastava R.S.
dc.date.accessioned2025-05-24T09:55:33Z
dc.description.abstractConsidering Bianchi type-I metric, cosmological models of a perfect fluid with an electromagnetic field have been obtained, using a supplementary condition between the metric potentials. The four-current is either zero or space-like. The model has expanding and shearing but non-rotating fluid flow which is also geodetic. The requirement of positive conductivity imposes an additional restriction on the model. Various physical and mathematical properties of the model have been discussed. © 1989 Kluwer Academic Publishers.
dc.identifier.doihttps://doi.org/10.1007/BF00640484
dc.identifier.urihttp://172.23.0.11:4000/handle/123456789/19942
dc.relation.ispartofseriesAstrophysics and Space Science
dc.titleSome anisotropic spatially-homogeneous cosmological models with electromagnetic field

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