Speaker
Juan Urrutia
Description
As the number of event that gravitational wave detector detect increases the probability of finding lensed events gets bigger, with estimations of 0(100)/year for 3G detectors. The number and nature of this events is going to be a powerful prove on dark matter substructures. We will show recent developments on lensing by primordial black holes, dark stars and dark matter halos and how they offer a complementary tool to microlensing of light.
