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Published on: September 6, 2012
Electric But Not Eclectic: Thermal Relic Dark Matter for the XENON1T Excess
Joseph Bramante1, Ningqiang Song1
1The McDonald Institute and Department of Physics, Engineering Physics, and Astronomy, Queen's University, Kingston, Ontario, K7L 2S8, Canada and Perimeter Institute for Theoretical Physics, Waterloo, Ontario, N2L 2Y5, Canada.
A new dark matter model explains excess electronic recoil events detected by the XENON1T experiment. This inelastic dark matter comprises sub-GeV Dirac fermions and a dark photon, offering insights into dark matter particle physics.
Area of Science:
- Particle Physics
- Cosmology
- Astrophysics
Background:
- The nature of dark matter remains one of the most significant unsolved problems in physics.
- Experiments like XENON1T aim to directly detect dark matter particles through their interactions with ordinary matter.
- XENON1T recently observed an excess of electronic recoil events, prompting theoretical explanations.
Purpose of the Study:
- To investigate a potential dark matter model that can explain the observed excess electronic recoil events in the XENON1T experiment.
- To propose a specific particle physics model for dark matter that accounts for the XENON1T anomaly.
- To explore the implications of inelastic dark matter interactions for direct detection experiments.
Main Methods:
- Utilizing a straightforward model of inelastic dark matter produced via early Universe thermal freeze-out annihilation.
- Modeling sub-GeV mass Dirac fermion dark matter coupled to a lighter dark photon kinetically mixed with the standard model photon.
- Incorporating a scalar field to provide mass for the dark photon and split fermion state masses.
Main Results:
- The proposed inelastic dark matter model successfully accounts for the excess electronic recoil events reported by the XENON1T Collaboration.
- The model predicts dark matter particles with sub-GeV masses, interacting inelastically with electrons and nuclei.
- The model involves a dark photon and a scalar field, offering a specific particle physics framework for dark matter.
Conclusions:
- Inelastic dark matter, specifically a sub-GeV Dirac fermion coupled to a dark photon, provides a compelling explanation for the XENON1T excess.
- This model highlights the importance of considering inelastic interactions in dark matter searches.
- The findings suggest new avenues for exploring dark matter properties through direct detection experiments.
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