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We consider the B-ball cosmology of the MSSM in the context of D-terminflation models where the reheating temperature is determined by theAffleck-Dine mechanism to be of the order of 1 GeV. We show that such a lowreheating temperature can arise quite naturally as the result of a symmetrywhich is required to maintain the flatness of the inflaton potential. In thiscase the B-balls will decay well after the freeze-out temperature of the LSP,allowing baryons and cold dark matter to originate primarily from B-balldecays.Comment: 12 pages LaTeX. Final published version (Phys.Rev.Lett. 81 (1998)  3071

physical review letters

Supersymmetric<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi mathvariant="italic">D</mml:mi></mml:math>-Term Inflation and<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mi mathvariant="italic">B</mml:mi></mml:math>-Ball Baryogenesis

SupersymmetricD-Term Inflation andB-Ball Baryogenesis