Abstract

The paper devotes to dynamical investigations of spatially homogeneous Bianchi type-I space-time filled with wet dark fluid, which is a candidate for dark energy in the framework of gravity. The equation of state parameter modeled on in the form of wet dark fluid for the dark energy component of the universe. Solutions to the corresponding field equations are obtained towards power and exponential volumetric law of expansion. The geometrical and physical parameters for both the models are studied in details. PACS numbers: 98.80.Es; 14.65.q; 04.60.m; 04.50.Kd.

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