Supersymmetric Partially Interacting Dark Matter
Willy Fischler, Dustin Lorshbough, Walter Tangarife
TL;DR
This paper introduces a supersymmetric model of partially interacting dark matter, exploring its formation, astrophysical constraints, and potential for dark galactic disk creation, along with jet emission from black holes.
Contribution
It proposes a novel supersymmetric PIDM model with unique dark sector atom production and discusses astrophysical implications and black hole jet phenomena.
Findings
Dark sector atoms can form via Affleck-Dine baryogenesis without Q-ball relics.
Astrophysical constraints limit the properties of the dark matter model.
Potential for dark galactic disk formation and black hole jet emission within this framework.
Abstract
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.
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