  Though entropy production is forbidden in standard FRW Cosmology, Berman and
Som presented a simple inflationary model where entropy production by bulk
viscosity, during standard inflation without ad hoc pressure terms can be
accommodated with Robertson-Walker's metric, so the requirement that the early
Universe be anisotropic is not essential in order to have entropy growth during
inflationary phase, as we show. Entropy also grows due to shear viscosity, for
the anisotropic case. The intrinsically inflationary metric that we propose can
be thought of as defining a polarized vacuum, and leads directly to the desired
effects without the need of introducing extra pressure terms.
