Supersymmetric Partially Interacting Dark Matter

Understand

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.