  We present a simple model for slow-rollover inflation where the vacuum energy
that drives inflation is of the order of $G_F^{-2}$; unlike most models, the
conversion of vacuum energy to radiation (``reheating'') is moderately
efficient. The scalar field responsible for inflation is a standard-model
singlet, develops a vacuum expectation value of the order of $4\times
10^6\GeV$, has a mass of order $1\GeV$, and can play a role in electroweak
phenomena.
