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Bianchi Type V Universes with Bulk Viscosity in General Relativity

Anirudh Pradhan·Vandana Rai·R. S. Singh
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Abstract

Bianchi type V bulk viscous fluid cosmological models are investigated. Using a generation technique (Camci {\it et al.}, 2001), it is shown that the Einstein's field equations are solvable for any arbitrary cosmic scale function. The viscosity coefficient of bulk viscous fluid is assumed to be a power function of mass density. Solutions for particular forms of cosmic scale functions are also obtained. Some physical and geometric aspects of the models are also discussed.

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Anirudh Pradhan, Vandana Rai, R. S. Singh. 2007-04-03. Bianchi Type V Universes with Bulk Viscosity in General Relativity. https://arxiv.org/abs/gr-qc/0612185

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