  In this paper, we investigate inhomogeneous viscous fluid cosmology for
inflation. Several toy models are presented in the attempt to analyze how
inflation can be realized according with cosmological data by making use of an
inhomogeneous EoS parameter for the fluid and/or by introducing a viscosity to
have a graceful exit from inflation. The results will be compared with the ones
of scalar field representation and discussed. We will pay attention on the
possibility to recover the reheating and therefore the Friedmann universe.
