Anisotropic bulk viscous string cosmological models with heat flux

Abstract

Bulk viscosity coupled with cosmic string for Bianchi type VI0 cosmological model is investigated in the context of Self creation theory of gravitation. Field equations are solved for two different cases by considering relation between metric potentials. It is assumed that scalar function is proportional to the scale factor. It is found that the universe is anisotropic and stable. The early universe is highly heated. Some physical parameters are also discussed in details.