Constraints on Dark Matter with a moderately large and velocity-dependent DM-nucleon cross-section
M. Shafi Mahdawi, Glennys R. Farrar

TL;DR
This paper derives constraints on velocity-dependent dark matter-nucleon cross sections across a broad mass range using multiple experiments, highlighting the importance of recoil energy thermalization efficiency and its impact on detection limits.
Contribution
It introduces new limits on velocity-dependent DM-nucleon interactions, emphasizing the role of thermalization efficiency and analyzing implications for the EDGES 21 cm anomaly.
Findings
Limits on cross sections for velocity dependencies with n in {-4,-2,-1,0,1,2}
Identification of a potential gap in constraints for 0.2-2 GeV mass range due to thermalization uncertainties
Exclusion of much of the parameter space relevant to the EDGES 21 cm anomaly for milli-charged dark matter
Abstract
We derive constraints on a possible velocity-dependent DM-nucleon scattering cross section, for Dark Matter in the 10 MeV -- 100 GeV mass range, using the XQC, DAMIC, and CRESST 2017 Surface Run experiments. We report the limits on cross sections of the form , for a range of velocity dependencies with . We point out the need to measure the efficiency with which nuclear recoil energy in the sub-keV range thermalizes, rather than being stored as Frenkel pairs in the semi-conductor lattice. The possibility of a significant inefficiency leaves open a considerable `hole' in the limits for mass in the 0.2 -- 2 GeV range, which XQC and CRESST can potentially fill when the thermalization efficiency is measured. We call attention to the asymmetry between a conventional lower limit cross section and the `upper-reach cross section' imposed by…
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