Conveners
DM Indirect Detection
- Jose Maria Diego Rodriguez (IFCA)
ΛCDM predicts light dark matter (DM) subhalos (SHs), not massive enough to retain baryons and become visible. If DM is composed of Weakly Interacting Massive Particles (WIMPs), we expect them to annihilate in SHs, producing gamma rays which can be detected with the Large Area Telescope (LAT) on the Fermi satellite, appearing as unidentified sources (unIDs) in the gamma-ray sky. We characterize...
We show that the mere observation of the first stars (Pop~III stars) in the universe can be used to place tight constraints on the strength of the interaction between dark matter and regular, baryonic matter. We apply this technique to a candidate Pop~III stellar complex discovered with the Hubble Space Telescope at $z\sim7$ and find some of the deepest bounds to-date for both spin-dependent...