Super-Resonant Dark Matter
Csaba Cs\'aki, Andrew Gomes, Yonit Hochberg, Eric Kuflik, Kevin, Langhoff, Hitoshi Murayama

TL;DR
This paper proposes a supersymmetric QCD-based model of dark matter with resonant self-interactions that vary with velocity, potentially solving small-scale structure issues, and predicts a dark matter mass around 3-4 MeV.
Contribution
It introduces a novel super-resonant dark matter model with velocity-dependent self-interactions derived from supersymmetric QCD, explaining small-scale structure puzzles.
Findings
Dark matter mass predicted around 3-4 MeV
Self-interactions are resonantly enhanced and velocity-dependent
Model accommodates small-scale structure observations
Abstract
We introduce Super-Resonant Dark Matter, a model of self-interacting dark matter based on the low energy effective theory of supersymmetric QCD. The structure of the theory ensures a resonant enhancement of the self-interactions of the low energy mesons, since their mass ratio is set by the number of colors and flavors. The velocity dependence of the resonantly enhanced self-interactions allows such theories to accommodate puzzles in small scale structure that arise from dark matter halos of different sizes. The dark matter mass is then predicted to be around 3-4 MeV, with its abundance set by freeze-in via a kinetically mixed dark photon.
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Scientific Research and Discoveries · Cold Atom Physics and Bose-Einstein Condensates
