Dynamics Of Anisotropic Bianchi Universe With Bulk Viscous

We have considered a innovative class of Bianchi type-III anisotropic cosmological models in which source of matter is bulk viscous fluid. To get the conclusive model of the universe, we have supposed that the coefficient of bulk viscosity is a power function of mass density. The exact solutions of the Einstein’s field equations are achieved which represent an expanding, shearing, and anisotropic model of the universe. The models offered are tested for physically acceptable cosmologies by using constancy. In view of the accelerated expansion of the current universe, the dynamical and physical properties of the models have been analyzed.