Direct detection of freeze-in inelastic dark matter
arXiv:2006.15672 · doi:10.1016/j.physletb.2021.136408
Abstract
We show that the current sensitivities of direct detection experiments have already reached the interesting parameter space of freeze-in dark matter models if the dark sector is in the inelastic dark matter framework and the excited dark matter state is cosmologically stable. Using results recently presented by the XENON1T experiment, we present constraints on these models. We also show that these models can explain the reported excess in the electron recoil signals if the mass gap between the ground state and the excited state is at keV scale.
7 pages, 7 figures
References in corpus (8)
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Cited by in corpus (23)
- A Next-Generation Liquid Xenon Observatory for Dark Matter and Neutrino Physics
- XENON1T excess in local DM models with light dark sector
- Earth-bound Milli-charge Relics
- An Active-to-Sterile Neutrino Transition Dipole Moment and the XENON1T Excess
- The ups and downs of inelastic dark matter: Electron recoils from terrestrial upscattering
- Self-interacting Inelastic Dark Matter in the light of XENON1T excess
- Endothermic self-interacting dark matter in Milky Way-like dark matter haloes
- Implications of the XENON1T Excess on the Dark Matter Interpretation
- Spin-dependent sub-GeV Inelastic Dark Matter-electron scattering and Migdal effect: (I). Velocity Independent Operator
- Pushing the frontier of WIMPy inelastic dark matter: journey to the end of the periodic table
- Constraints on electron-scattering interpretation of XENON1T excess
- Canonical seesaw implication for two-component dark matter
- Boosted Self-Interacting Dark Matter and XENON1T Excess
- Detection of Inelastic Dark Matter via Electron Recoils in SENSEI
- Solar Active-Sterile Neutrino Conversion with Atomic Effects at Dark Matter Direct Detection Experiments
- Probing feebly interacting dark matter with monojet searches
- Testing freeze-in with axial and vector bosons
- Terrestrial Probes of Electromagnetically Interacting Dark Radiation
- Explaining The XENON1T Excess With Light Goldstini Dark Matter
- Unlocking the Inelastic Dark Matter Window with Vector Mediators
- 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