paper

Dark Matter and the XENON1T electron recoil excess

arXiv:2006.10735 · doi:10.1103/PhysRevD.102.095002

Abstract

We show that the electron recoil excess around 2 keV claimed by the Xenon collaboration can be fitted by DM or DM-like particles having a fast component with velocity of order . Those particles cannot be part of the cold DM halo of our Galaxy, so we speculate about their possible nature and origin, such as fast moving DM sub-haloes, semi-annihilations of DM and relativistic axions produced by a nearby axion star. Feasible new physics scenarios must accommodate exotic DM dynamics and unusual DM properties.

5 pages, 3 figures, published version

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