Axially Symmetric Bianchi Type-I Bulk Viscous Cosmological Model with Lyra Geometry

We have discussed in this paper spatially homogeneous and anisotropic axially symmetric Bianchi type-I cosmological model with Lyra geometry in the presence of bulk viscous fluid. Here we have considered the coefficient of bulk viscosity as a quadratic function of Hubble parameter (i, e), Where, , are constant. The physical and kinematical properties of the models are discussed.