Expected sensitivity of phonon-based light dark matter detectors varies by a factor of 2-3 depending on which Gaia-inspired dark matter substructure is assumed, because anharmonic crystal effects depend on the dark matter velocity distribution.
Probing Light DM through Migdal Effect with Spherical Proportional Counter
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abstract
Owing to its low electronic noise and flexible target materials, the Spherical Proportional Counter (SPC) with a single electron detection threshold can be utilized to search for sub-GeV dark matter (DM). In this work, we investigate the prospects for light DM direct detection through the DM-nucleus Migdal effect in the DARKSPHERE detector. We consider the different DM velocity distributions and momentum-transfer effects. For Xenon and Neon targets, we find that the DM mass $m_{DM}$ can be probed down to as low as $m_{DM} \sim \mathcal{O}$(10) MeV, and the derived bounds on the DM-nucleus scattering cross section $\bar{\sigma}_{n}$ are sensitive to the high-velocity tails of the DM velocity distribution, which can be altered by orders of magnitude for the different DM velocity distributions in the region $m_{DM} < 10$ MeV.
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Halo-dependent Anharmonic Effects in Collective Excitation for Light Dark Matter Direct Detection
Expected sensitivity of phonon-based light dark matter detectors varies by a factor of 2-3 depending on which Gaia-inspired dark matter substructure is assumed, because anharmonic crystal effects depend on the dark matter velocity distribution.