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Tilted Bianchi Type I Cosmological Models Filled with Disordered Radiation in General Relativity Revisited

Anirudh Pradhan·Abha Rai
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Abstract

Tilted Bianchi type I cosmological models filled with disordered radiation in presence of a bulk viscous fluid and heat flow are investigated. The coefficient of bulk viscosity is assumed to be a power function of mass density. Some physical and geometric properties of the models are also discussed.

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Anirudh Pradhan, Abha Rai. 2002-12-26. Tilted Bianchi Type I Cosmological Models Filled with Disordered Radiation in General Relativity Revisited. https://doi.org/10.1023/a%3A1026301915781

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