Solar-reflected inelastic dark matter produces detectable signals in xenon and semiconductor detectors, enabling new constraints on MeV-scale dark matter parameter space.
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Boosted sub-GeV dark matter from atmospheric cosmic ray bremsstrahlung can be probed by direct detection and neutrino experiments, with enhanced sensitivity near vector mediator resonances.
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Solar Reflection of Inelastic Dark Matter
Solar-reflected inelastic dark matter produces detectable signals in xenon and semiconductor detectors, enabling new constraints on MeV-scale dark matter parameter space.
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Sub-GeV dark matter from cosmic ray bremsstrahlung in the atmosphere
Boosted sub-GeV dark matter from atmospheric cosmic ray bremsstrahlung can be probed by direct detection and neutrino experiments, with enhanced sensitivity near vector mediator resonances.
- Primordial black holes as cosmic accelerators of light dark matter: Novel direct detection constraints