1. Shining dark matter in XENON1T
- Author
-
Michele Tammaro, Alexey A. Petrov, Gil Paz, and Jure Zupan
- Subjects
Physics ,Photon ,Annihilation ,010308 nuclear & particles physics ,Scattering ,Dark matter ,FOS: Physical sciences ,Electron ,01 natural sciences ,Nuclear physics ,symbols.namesake ,High Energy Physics - Phenomenology ,High Energy Physics - Phenomenology (hep-ph) ,Recoil ,0103 physical sciences ,symbols ,Neutrino ,Rayleigh scattering ,010306 general physics - Abstract
We point out that a non-relativistic $\sim 2 $ GeV dark matter (DM) which interacts with visible matter through higher dimensional Rayleigh operators could explain the excess of "electron recoil" events recently observed by the Xenon1T collaboration. A DM scattering event results in a few keV photon that on average carries most of the deposited energy, while the nuclear recoil energy is only a subleading correction. Since the Xenon1T detector does not discriminate between electrons and photons, such events would be interpreted as excess of the keV electrons. Indirect constraints from dark matter annihilation are avoided for light mediators of ${\mathcal O}(10~{\rm MeV})$ that have sizable couplings to neutrinos. One loop induced spin-independent scattering in dark matter may soon lead to a confirmation signal or already excludes regions of viable parameter space for the Rayleigh DM model, depending on what the exact values of the unknown nonperturbative nuclear matrix elements are., 5 pages, 5 figures, discussion shortened, typos corrected
- Published
- 2021