Kavli Affiliate: Lina Necib | Summary:The dark matter flux in a direct detection experiment depends on its local speed distribution. This distribution has been inferred from simulations of Milky Way-like galaxies, but such models serve only as proxies, given that no simulation directly captures the detailed evolution of our own Galaxy. This motivates alternative approaches […]
Continue.. How to Build an Empirical Speed Distribution for Dark Matter in the Solar Neighborhood