Speaker
Pedro Pasquini
(Shanghai University)
Description
Solar neutrino scattering with electron via a light mediator, either scalar or vector can be searched in Xenon-based Dark Matter experiments. A keV sterile neutrino instead of an active neutrino can appear in the final state for the recoil electron. Such a scenario is difficult to probe in other types of experiments and can be used to obtain stringent bounds on new interactions. Moreover, a sterile neutrino with mass at the 100 keV allows the explanation of the Xenon1T excess. We also briefly discuss the case of sterile neutrino final state with light
Authors
Mr
Jie Sheng
(Shanghai Jiao Tong University)
Pedro Pasquini
(Shanghai University)
Shao-Feng Ge
(TDLI-SJTU)
