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In hybrid inflation and running mass inflation models it is possible that theinflaton field will fragment into non-topological solitons, resulting in ahighly inhomogeneous post-inflation era prior to reheating. In supersymmetricmodels with a conventional homogeneous post-inflation era, the dynamics of flatdirection scalars are determined by cH^{2} corrections to the mass squaredterms, coming from the energy density of the Universe combined withPlanck-scale suppressed interactions. Here we reconsider the cH^{2} correctionsfor a Universe dominated by inflatonic non-topological solitons. We show thatthe dynamics in this case are typically equivalent to the case c = 0, even inthe vicinity of the non-topological solitons. Thus Affleck-Dine baryogenesiswill proceed as in the original c = 0 Affleck-Dine scenario.Comment: 16 pages LaTeX, additional discussion, conclusions unchange

Flat direction dynamics in a non-topological soliton-dominated universe