Anirudh Pradhan, Sudhir Kumar Srivastava
Abstract
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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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.
Key concepts: Physics, Volume viscosity, Viscous liquid, Viscosity, Type (biology), Cosmological model, General relativity, Power function