  The process of baryogenesis through the evaporation of black holes formed at
the end of inflation phase is considered. The increase of black hole mass due
to accretion from the surrounding radiation after the reheating is taken into
account. It is shown that the influence of the accretion on the baryogenesis is
important only in the case when the initial values of black hole mass are
larger than $\sim 10^{4}{g}$. The behavior of calculated baryon asymmetry, as a
function of model parameters, is studied.
