Tilted Bianchi Type I Cosmological Models Filled with Disordered Radiation in General Relativity Revisited
نویسندگان
چکیده
General Relativity describes the state in which radiation concentrates around a star. Klein (1948) worked on it and obtained an approximate solution to Einsteinian field equations in spherical symmetry for a distribution of diffused radiation. Many other researchers (Singh and Abdussattar, 1973; Roy and Bali, 1977) have worked on this topic and obtained exact static spherically and cylindrically symmetric solutions of Einstein’s field equations with exception as well. Roy and Singh (1977) have obtained a non-static plane symmetric spacetime filled with disordered radiation. Teixeira, Wolk and Som (1977) investigated a model filled with source free disordered distribution of electromagnetic radiation in Einstein’s general relativity.
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