We conducted an investigation into Affleck-Dine baryogenesis within the
context of D-term inflation, specifically focusing on its relationship with a
recent reheating formalism. It was found that by considering a specific
reheating temperature, the observed baryon asymmetry can be accounted through
Affleck-Dine baryogenesis. Additionally, the majority of gravitinos are
inferred to be generated from the decay of the next-to-lightest supersymmetric
particle, with Q-balls potentially serving as a source of gravitinos via NSP
decay. The temperature at which decay occurs depends on the charge of the
Q-balls, which is determined by the fragmentation of the Affleck-Dine
condensate. Remarkably, the gravitino mass required for dark matter aligns
naturally with the theoretical gravitino mass.Comment: 11 pages, 4 figure