Kavli Affiliate: Lina Necib | Summary:The majority of terrestrial direct detection experiments for Dark Matter (DM) rely on the Standard Halo Model (SHM), which assumes the local DM velocity distribution follows a Maxwell-Boltzmann distribution. However, galaxy mergers can deposit DM that remains kinematically clustered today, inducing deviations from the smooth SHM prediction. Previous studies have […]
Continue.. Set the Night on FIRE: Building an Empirical Local Dark Matter Velocity Distribution