Boosted dark matter signals uplifted with self-interaction
arXiv:1411.6632 · doi:10.1016/j.physletb.2015.02.057
Abstract
We explore detection prospects of a non-standard dark sector in the context of boosted dark matter. We focus on a scenario with two dark matter particles of a large mass difference, where the heavier candidate is secluded and interacts with the standard model particles only at loops, escaping existing direct and indirect detection bounds. Yet its pair annihilation in the galactic center or in the Sun may produce boosted stable particles, which could be detected as visible Cherenkov light in large volume neutrino detectors. In such models with multiple candidates, self-interaction of dark matter particles is naturally utilized in the {\it assisted freeze-out} mechanism and is corroborated by various cosmological studies such as N-body simulations of structure formation, observations of dwarf galaxies, and the small scale problem. We show that self-interaction of the secluded (heavier) dark matter greatly enhances the capture rate in the Sun and results in promising signals at current and future experiments. We perform a detailed analysis of the boosted dark matter events for Super-Kamiokande, Hyper-Kamiokande and PINGU, including notable effects such as evaporation due to self-interaction and energy loss in the Sun.
24 pages, 8 figures; discussion on the boosted DM flux from the Earth, references added, typos corrected; published in PLB
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- Boosted Dark Matter in IceCube and at the Galactic Center
- On the Direct Detection of Dark Matter Annihilation
- Monochromatic dark neutrinos and boosted dark matter in noble liquid direct detection
- Multi-component Dark Matter through a Radiative Higgs Portal
- Updated Constraints on Self-Interacting Dark Matter from Supernova 1987A
- Boosting (In)direct Detection of Dark Matter