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We study the Affleck-Dine (AD) baryogenesis in the inflating curvatonscenario, when the curvaton is a moduli field with O($10-10^2$TeV) mass. Amoduli field with such mass is known to be free from the Polonyi problem, andfurthermore its decay products can explain the present cold dark matterabundance. In our scenario, it further explains the primordial curvatureperturbation and the present baryon density all together. The currentobservational bound on the baryon isocurvature perturbation, which severelyconstrains the AD baryogenesis with the original oscillating moduli curvatonscenario, is shown to put practically negligible constraint if we replace theoscillating curvaton with the inflating curvaton.

Affleck-Dine baryogenesis in inflating curvaton scenario with O($10-10^2$TeV) mass moduli curvaton