  The irrotational Bianchi V cosmological model under the influence of both
shear and bulk viscosity, together with heat flux, has been studied. Exact
solutions for the model are obtained with three physically viable assumptions.
The first two relate the matter density, shear scalar, and expansion scalar and
the third is a barotropic equation of state, connecting the matter density and
thermodynamic pressure. The properties of the solutions are studied and the
temperature distribution is also presented explicitly. It has been observed
that along with the viscosity, heat flux further adds to the rate of entropy
increase.
