Searches for dark matter–induced recoils have made impressive advances in the last few
years. Yet the field is confronted by several outstanding problems. First, the inevitable …

Cosmological observations indicate that most of the matter in the Universe is Dark Matter.
Dark Matter in the form of Weakly Interacting Massive Particles (WIMPs) can be detected …

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 …

Data from the Gaia satellite show that the solar neighborhood of the Milky Way's stellar halo
is imprinted with substructure from several accretion events. Evidence of these events is …

The recently discovered S1 stream passes through the Solar neighborhood on a low
inclination, counterrotating orbit. The progenitor of S1 is a dwarf galaxy with a total mass …

Coherent scattering of solar, atmospheric, and diffuse supernovae neutrinos creates an
irreducible background for direct dark matter experiments with sensitivities to WIMP-nucleon …

The measurement of the direction of WIMP-induced nuclear recoils is a compelling but
technologically challenging strategy to provide an unambiguous signature of the detection of …

Next-generation dark matter (DM) detectors searching for weakly interacting massive
particles (WIMPs) will be sensitive to coherent scattering from solar neutrinos, demanding an …

There is a worldwide effort toward the development of a large time projection chamber
devoted to directional dark matter detection. All current projects are being designed to fulfill …

Recoil imaging entails the detection of spatially resolved ionization tracks generated by
particle interactions. This is a highly sought-after capability in many classes of detector, with …