Some Bianchi Type-IX Viscous Fluid Cosmological Models in General Relativity

In this paper we have considered Bianchi Type – IX viscous fluid cosmological model in General Relativity and to solve the field equations, we have assumed judicious relations between metric potential A and B. Further we have taken   where  is the co-efficient of shear viscosity and  is the scalar of expansion in the model. We have also taken co-efficient of bulk viscosity  to be constant. Various physical geometrical properties of the model have been also discussed and it is found that the model does not approach isotropy for large values of T in the absence of viscosity.