http://arxiv.org/abs/2012.09751
Migdal effect provides a new way to search for sub-GeV dark matter. However, due to the limitation of the energy of ionization and/or de-excitation of the intrinsic atomic electron state, the current limits on light DM exist in the mass range of ${\cal O}(10)~{\rm MeV}< m_\chi < {\cal O}(1)~{\rm GeV}$. On the other hand, since the ionization form factor in Migdal effects can be enhanced by large momentum transfer, the resulting event rate of S2 signal may be increased for fast-moving DM, and then improves the bounds on light DM. As a proof-of concept, we consider a fast-moving sub-GeV DM, namely atmospheric DM (ADM), which is produced by the interaction between high energy cosmic rays (CRs) and the atmosphere. With Xenon1T data, we find that there will be nearly three orders of magnitude improvement on the DM-nucleus scattering cross section by including Migdal effect.
V. Flambaum, L. Su, L. Wu, et. al.
Fri, 18 Dec 20
38/78
Comments: 7 pages, 4 figures
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