Kavli Affiliate: Lina Necib | Summary:The nature of dark matter sets the shape of galactic halos: collisionless cold dark matter (CDM) predicts triaxial halos, while scattering in self-interacting dark matter (SIDM) rounds them toward sphericity. We show that a large catalog of projected stellar stream tracks can statistically constrain halo shapes, and therefore the particle […]
Continue.. When Streams Curve Away: a Test of Dark Matter from Extragalactic Stellar Stream Populations