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An anisotropic cosmological model in Brans-Dicke theory

dc.contributor.authorSingh T.; Rai L.N.
dc.date.accessioned2025-05-24T09:56:26Z
dc.description.abstractSolutions of Brans-Dicke field equations are obtained when the source of the gravitational field is a perfect fluid with pressure equal to energy density and the metric is cylindrically symmetric of Marder-type. Various physical and geometrical properties of the model have been discussed. Finally the solutions have been transformed to the original form of Brans-Dicke (1961) theory and then through unit transformation to a general form. © 1983 D. Reidel Publishing Company.
dc.identifier.doihttps://doi.org/10.1007/BF00661944
dc.identifier.urihttp://172.23.0.11:4000/handle/123456789/21018
dc.relation.ispartofseriesAstrophysics and Space Science
dc.titleAn anisotropic cosmological model in Brans-Dicke theory

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