Combining cosmic-ray and supernova-neutrino boosts yields the strongest constraints to date on sub-GeV dark matter scattering with electrons, nucleons, and neutrinos.
Calculations of Relic Densities in the Early Universe,
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Boosted Dark Matter Driven by Cosmic Rays and Diffuse Supernova Neutrinos
Combining cosmic-ray and supernova-neutrino boosts yields the strongest constraints to date on sub-GeV dark matter scattering with electrons, nucleons, and neutrinos.