Early cosmological models with bulk viscosity in Brans-Dicke theory

Abstract

The effect of time dependent bulk viscosity on the evolution of Friedmann models with zero curvature in Brans-Dicke theory is studied. The solutions of the field equations with 'gamma-law' equation of state p = (γ - 1) ρ, where γ varies continuously as the Universe expands, are obtained by using the power-law relation φ = bRn, which lead to models with constant deceleration parameter. We obtain solutions for the inflationary period and radiation dominated era of the universe. The physical properties of cosmological solutions are also discussed.