Venue: Stanford Linear Accelerator (SLAC) Building 48
Friday, 11/18/22
A Path to Detecting Self-Interacting Dark Matter using Astrophysical Sub-StructureDark matter self interactions can leave distinctive signatures on the properties of satellite galaxies around Milky Way-like hosts. By analyzing a number of Milky Way dwarf galaxies, we were able to place new constraints on models of self-interacting dark matter which interact via a Yukawa potential. The results push the theory ...
