  We present a novel scenario for baryogenesis in a hybrid inflation model at
the electroweak scale, in which the Standard Model Higgs field triggers the end
of inflation. One of the conditions for successful baryogenesis, the departure
from thermal equilibrium, is naturally achieved at the stage of preheating
after inflation. The inflaton oscillations induce large occupation numbers for
long-wavelength configurations of Higgs and gauge fields, which leads to a
large rate of sphaleron transitions. We estimate this rate during the first
stages of reheating and evaluate the amount of baryons produced due to a
particular type of higher dimensional CP violating operator. The universe
thermalizes through fermion interactions, at a temperature below critical,
$T_{rh} < 100$ GeV, preventing the wash-out of the produced baryon asymmetry.
Numerical simulations in (1+1) dimensions support our theoretical analysis.
