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arXiv 2008.00529hep-ph
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Self-interacting hidden sector dark matter, small scale galaxy structure anomalies, and a dark force

Amin Aboubrahim, Wan-Zhe Feng, Pran Nath, Zhu-Yao Wang

英文摘要:

The short distance behavior of dark matter (DM) at galaxy scales exhibits several features not explained by the typical cold dark matter (CDM) with velocity-independent cross-section. We discuss a particle physics model with a hidden sector interacting feebly with the visible sector where a dark fermion self-interacts via a dark force with a light dark photon as the mediator. We study coupled Boltzmann equations involving two temperatures, one for each sector. We fit the velocity-dependent DM cross-section to the data from scales of dwarf galaxies to clusters consistent with relic density constraint.

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