The general class of Bianchi cosmological models in f(R, T) gravity with dark energy in viscous cosmology

The general class of Bianchi cosmological models in f ( R , T ) gravity with dark energy in the form of standard and modified Chaplygin gas and bulk viscosity have been considered. We have discussed three types of average scale factor by using a special law for deceleration parameter which is linear in time with negative slope. The model describes an accelerating universe for large value of time t , wherein the effective negative pressure induced by Chaplygin gas and bulk viscous pressure are driving the acceleration.