Self-interacting Inelastic Dark Matter in the light of XENON1T excess
arXiv:2101.06472 · doi:10.1103/PhysRevD.103.095018
Abstract
We propose a self-interacting inelastic dark matter (DM) scenario as a possible origin of the recently reported excess of electron recoil events by the XENON1T experiment. Two quasi-degenerate Majorana fermion DM interact within themselves via a light hidden sector massive gauge boson and with the standard model particles via gauge kinetic mixing. We also consider an additional long-lived singlet scalar which helps in realising correct dark matter relic abundance via a hybrid setup comprising of both freeze-in and freeze-out mechanisms. While being consistent with the required DM phenomenology along with sufficient self-interactions to address the small scale issues of cold dark matter, the model with GeV scale DM can explain the XENON1T excess via inelastic down scattering of heavier DM component into the lighter one. All these requirements leave a very tiny parameter space keeping the model very predictive for near future experiments.
34 pages, 14 figures, version accepted for publication in PRD
References in corpus (18)
- A direct empirical proof of the existence of dark matter
- A Theory of Dark Matter
- Search for a dark photon in e+e- collisions at BABAR
- Cores in Dwarf Galaxies from Dark Matter with a Yukawa Potential
- Is dark matter with long-range interactions a solution to all small-scale problems of ΛCDM cosmology?
- Searching for low-mass dark matter particles with a massive Ge bolometer operated above-ground
- First results from the NEWS-G direct dark matter search experiment at the LSM
- Candidates for Inelastic Dark Matter
- Self-Scattering for Dark Matter with an Excited State
- Self-Interacting Dark Matter through the Higgs Portal
- Inelastic Dark Matter Electron Scattering and the XENON1T Excess
- Self-interacting inelastic dark matter: A viable solution to the small scale structure problems
- Self-interacting Dark Matter Without Direct Detection Constraints
- Common Origin of Neutrino Mass and Dark Matter from Anomaly Cancellation Requirements of a Model
- Astrophysical probes of inelastic dark matter with a light mediator
- Pseudo-Dirac Dark Matter in XENON1T
- Xenon-1T excess as a possible signal of a sub-GeV hidden sector dark matter
- Verifiable type-II seesaw and dark matter in a gauged model
Cited by in corpus (17)
- A Next-Generation Liquid Xenon Observatory for Dark Matter and Neutrino Physics
- Direct detection of dark energy: the XENON1T excess and future prospects
- Non-thermal Origin of Asymmetric Dark Matter from Inflaton and Primordial Black Holes
- Self-interacting freeze-in dark matter in a singlet doublet scenario
- Self-interacting Dark Matter via Right Handed Neutrino Portal
- Gravitational waves from a dark phase transition in the light of NANOGrav 12.5 yr data
- Heating Neutron Stars with Inelastic Dark Matter and Relativistic Targets
- Pushing the frontier of WIMPy inelastic dark matter: journey to the end of the periodic table
- Asymmetric self-interacting dark matter with a canonical seesaw model
- Asymmetric Self-interacting Dark Matter via Dirac Leptogenesis
- Solar Active-Sterile Neutrino Conversion with Atomic Effects at Dark Matter Direct Detection Experiments
- Unified Origin of Dark Matter Self-Interactions and Low Scale Leptogenesis
- Inelastic Dark Matter from Dark Higgs Boson Decays at FASER
- Explorations of pseudo-Dirac dark matter having keV splittings and interacting via transition electric and magnetic dipole moments
- Inelastic dark matter, small scale problems, and the XENON1T excess
- Revisiting Puffy Dark Matter with Novel Insights: Partial Wave Analysis
- Singlet-Doublet Self-interacting Dark Matter and Radiative Neutrino Mass