  We present a model of partially interacting dark matter (PIDM) within the
framework of supersymmetry with gauge mediated symmetry breaking. Dark sector
atoms are produced through Affleck-Dine baryogenesis in the dark sector while
avoiding the production of Q-ball relics. We discuss the astrophysical
constraints relevant for this model and the possibility of dark galactic disk
formation. In addition, jet emission from rotating black holes is discussed in
the context of this class of models.
