LAUSR

Despite strong evidence for the existence of large amounts of dark matter (DM) in our Universe, there is no direct indication of its presence in our own solar system. All estimates of the local DM density, crucial for all direct DM searches, rely on extrapolating estimates on much larger scales. We demonstrate for the first time the possibility of measuring the local DM density with a direct detection experiment. It relies on the assumption that incoming DM particles frequently scatter on terrestrial nuclei prior to detection, inducing an additional time-dependence of the signal. We show that for sub-GeV DM, with a spin-independent DM-proton cross section $\sim10^{-32}\,\text{cm}^2$, future direct detection experiments should be able to reconstruct the local DM density with 20% uncertainty.