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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- Implications of the XENON1T Excess on the Dark Matter Interpretation
- Shedding New Light on Sterile Neutrinos from XENON1T Experiment
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- The Spectrum of Dark Radiation as a Probe of Reheating
- Canonical seesaw implication for two-component dark matter
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- Decoding Dark Matter Substructure without Supervision
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- Deep learning the astrometric signature of dark matter substructure
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- Terrestrial Probes of Electromagnetically Interacting Dark Radiation
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- Connecting Low scale Seesaw for Neutrino Mass to Inelastic sub-GeV Dark Matter with Abelian Gauge Symmetry
- Models for Self-resonant Dark Matter
- Asymmetric matter from symmetry breaking
- Dark Fluxes from Accreting Black Holes and Direct Detections
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- Milky Way Satellite Census. IV. Constraints on Decaying Dark Matter from Observations of Milky Way Satellite Galaxies