Collider Constraints on a Dark Matter Interpretation of the XENON1T Excess
arXiv:2006.13161 · doi:10.1140/epjc/s10052-020-08652-x
Abstract
In light of the excess in the low-energy electron recoil events reported by XENON1T, many new physics scenarios have been proposed as a possible origin of the excess. One possible explanation is that the excess is a result of a fast moving dark matter (DM), with velocity and mass between 1 MeV and 10 GeV, scattering off an electron. Assuming the fast moving DM-electron interaction is mediated by a vector particle, we derive collider constraints on the said DM-electron interaction. The bounds on DM-electron coupling is then used to constrain possible production mechanisms of the fast moving DM. We find that the preferred mass of the vector mediator is relatively light ( 1 GeV) and the coupling of the vector to the electron is much smaller than the coupling to the fast moving DM.
6 pages, 5 figures, references added, CMB constraints included, low-energy bounds updated, conclusion unchanged
References in corpus (16)
- Search for a dark photon in e+e- collisions at BABAR
- LEP Shines Light on Dark Matter
- Dark Matter Search Results from the Complete Exposure of the PICO-60 CF Bubble Chamber
- Upper Bound on the Dark Matter Total Annihilation Cross Section
- Model Independent Bounds on Magnetic Moments of Majorana Neutrinos
- Solar axions cannot explain the XENON1T excess
- Search for one large extra dimension with the DELPHI detector at LEP
- Explaining the XENON1T excess with Luminous Dark Matter
- Inelastic Dark Matter Electron Scattering and the XENON1T Excess
- Neutrino self-interactions and XENON1T electron recoil excess
- Light vector mediators facing XENON1T data
- XENON1T Anomaly and its Implication for Decaying Warm Dark Matter
- Hidden Photon Dark Matter in the Light of XENON1T and Stellar Cooling
- Shining dark matter in Xenon1T
- Sun Heated MeV-scale Dark Matter and the XENON1T Electron Recoil Excess
- Galactic Origin of Relativistic Bosons and XENON1T Excess
Cited by in corpus (23)
- New limits on dark photons from solar emission and keV scale dark matter
- Exploring New Physics with O(keV) Electron Recoils in Direct Detection Experiments
- Re-examining the Solar Axion Explanation for the XENON1T Excess
- Electric But Not Eclectic: Thermal Relic Dark Matter for the XENON1T Excess
- XENON1T excess in local DM models with light dark sector
- One-loop running of dimension-six Higgs-neutrino operators and implications of a large neutrino dipole moment
- Global fits of axion-like particles to XENON1T and astrophysical data
- An Active-to-Sterile Neutrino Transition Dipole Moment and the XENON1T Excess
- Probing the relaxed relaxion and Higgs-portal with S1 & S2
- Solar Neutrino Scattering with Electron into Massive Sterile Neutrino
- Implications of the XENON1T Excess on the Dark Matter Interpretation
- XENON1T solar axion and the Higgs boson emerging from the dark
- Dark Matter, Muon Anomalous Magnetic Moment and the XENON1T Excess
- Impact of loop-induced processes on the boosted dark matter interpretation of the XENON1T excess
- Constraints on electron-scattering interpretation of XENON1T excess
- EFT Approach of Inelastic Dark Matter for Xenon Electron Recoil Detection
- Canonical seesaw implication for two-component dark matter
- XENON1T Excess: Some Possible Backgrounds
- Probing sub-GeV leptophilic dark matter at Belle II and NA64
- Explaining The XENON1T Excess With Light Goldstini Dark Matter
- Dark Fluxes from Accreting Black Holes and Direct Detections
- Dequantization of electric charge: Probing scenarios of cosmological multi-component dark matter
- Lepton Number Violating Electron Recoils in a Model with Non-Standard Interactions