Abstract
In the present paper we investigate Bianchi type-I Cosmological model with inhomogeneous equation of state (EoS) in the presence of variable bulk viscous fluid(ζ) in the framework of general theory of relativity. In order to find exact solutions of the Einstein’s field equations, we have assumed a special law of variation for Hubble parameter H i. e. . The nature of model is discussed for α ≠ 0 and α = 0. Some physical and kinematical aspects of model are also discussed for both the conditions.
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