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Tilted Bianchi Type V Bulk Viscous Cosmological Models in General Relativity

Anirudh Pradhan·Abha Rai
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Abstract

Conformally flat tilted Bianchi type V cosmological models 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 aspects of the models are also discussed.

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Anirudh Pradhan, Abha Rai. 2003-07-10. Tilted Bianchi Type V Bulk Viscous Cosmological Models in General Relativity. https://doi.org/10.1023/b%3Aastr.0000032069.58003.b4

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