Dark Matter, Muon Anomalous Magnetic Moment and the XENON1T Excess

Abstract

A very economic scenario with just three extra scalar fields beyond the Standard Model is invoked to explain the muon anomalous magnetic moment, the requisite relic abundance of dark matter as well as the Xenon-1T excess through the inelastic down-scattering of the dark scalar.

arXiv comment7 pages, 4 figures; matches published version

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Cited by in corpus (16)

• A Next-Generation Liquid Xenon Observatory for Dark Matter and Neutrino Physics
• The Neutrino Magnetic Moment Portal: Cosmology, Astrophysics, and Direct Detection
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• Bounds on boosted dark matter from direct detection: The role of energy-dependent cross sections
• Self-interacting Inelastic Dark Matter in the light of XENON1T excess
• Pushing the frontier of WIMPy inelastic dark matter: journey to the end of the periodic table
• Blazar boosted Dark Matter -- direct detection constraints on ${\sigma }_{e\chi }$ : Role of energy dependent cross sections
• Canonical seesaw implication for two-component dark matter
• Boosted Self-Interacting Dark Matter and XENON1T Excess
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• Terrestrial Probes of Electromagnetically Interacting Dark Radiation
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• Explorations of pseudo-Dirac dark matter having keV splittings and interacting via transition electric and magnetic dipole moments
• Dark Fluxes from Accreting Black Holes and Direct Detections
• Inelastic dark matter, small scale problems, and the XENON1T excess
• Anomalous gauge couplings vis-$\grave{a}$-vis $(g-2{)}_{\mu }$ and flavor observables