Speaker
Description
Sub-MeV cold dark matter (DM) particles are unable to produce electronic recoil in the XENONnT experiment above the detector threshold. The mechanism of boosted dark matter (BDM) scenario comes into picture to constrain the parameter space of such low mass dark matter from direct detection experiments. We consider the effect of the leading components of cosmic rays to boost the cold DM. To present a concrete example, we choose to work on a model consisting of a Dirac fermion
Secondary category for the parallel session (optional) | Astroparticle Physics |
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