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The process of baryogenesis through the evaporation of black holes formed atthe end of inflation phase is considered. The increase of black hole mass dueto accretion from the surrounding radiation after the reheating is taken intoaccount. It is shown that the influence of the accretion on the baryogenesis isimportant only in the case when the initial values of black hole mass arelarger than $\sim 10^{4}{g}$. The behavior of calculated baryon asymmetry, as afunction of model parameters, is studied.Comment: 5 pages (including 6 .eps files

Baryon asymmetry of the universe from evaporation of primordial black holes