The existence of dark matter as evidenced by numerous indirect observations is one of the
most important indications that there must be physics beyond the Standard Model of particle …

The nature of dark matter and properties of neutrinos are among the most pressing issues in
contemporary particle physics. The dual-phase xenon time-projection chamber is the …

The neutrino floor is a theoretical lower limit on WIMP-like dark matter models that are
discoverable in direct detection experiments. It is commonly interpreted as the point at which …

Abstract Weakly Interacting Massive Particles (WIMPs) are among the best-motivated dark
matter candidates. No conclusive signal, despite an extensive search program that …

We measured the cross section of coherent elastic neutrino-nucleus scattering (CEvNS)
using a CsI [Na] scintillating crystal in a high flux of neutrinos produced at the Spallation …

Predicting signals in experiments to directly detect dark matter (DM) requires a form for the
local DM velocity distribution. Hitherto, the standard halo model (SHM), in which velocities …

The SuperCDMS experiment is designed to directly detect weakly interacting massive
particles (WIMPs) that may constitute the dark matter in our Galaxy. During its operation at …

A bstract We calculate coherent elastic neutrino-nucleus scattering cross sections on spin-0
nuclei (eg 40 Ar and 28 Si) at energies below 100 MeV within the Standard Model and …

Above a critical dark matter-nucleus scattering cross section any terrestrial direct detection
experiment loses sensitivity to dark matter, since the Earth crust, atmosphere, and potential …

This report summarizes the present status of neutrino non-standard interactions (NSI). After
a brief overview, several aspects of NSIs are discussed, including connection to neutrino …