  We investigate the Affleck-Dine baryogenesis after D-term inflation with a
positive Hubble-induced mass term for a B-L flat direction. It stays at a large
field value during D-term inflation, and just after inflation ends it starts to
oscillate around the origin of the potential due to the positive Hubble-induced
mass term. The phase direction is kicked by higher-dimensional Kahler
potentials to generate the B-L asymmetry. The scenario predicts nonzero
baryonic isocurvature perturbations, which would be detected by future
observations of CMB fluctuations. We also provide a D-term inflation model
which naturally explain the coincidence of the energy density of baryon and
dark matter.
