Speaker
Dr
Chung-Lin Shan
Description
In this talk, we will present our numerical simulation results of 3D recoil distributions of coherent elastic Solar B-8 neutrino-nucleus scattering events, which could be observed by future directional direct Dark Matter detectors. These results are achieved by our 3D Monte Carlo scattering-by-scattering simulation package, built originally for 3D elastic WIMP-nucleus scattering events. Dependence on detector material, laboratory location as well as annual/diurnal observation period will be discussed.
Primary author
Dr
Chung-Lin Shan
