Speaker
Mr.
Pablo-Miravé Martínez
(IFIC)
Description
Primordial black holes (PBHs) are potential dark matter candidates whose masses can span over many orders of magnitude. If they have masses in the 1015−1017 g range, they can emit sizeable fluxes of MeV neutrinos through evaporation via Hawking radiation. We explore the possibility of detecting light (non-)rotating PBHs with future neutrino experiments. We show that future neutrino experiments like DUNE and THEIA will be able to set constraints on PBH dark matter, thus providing complementary probes in a part of the PBH parameter space currently constrained mainly by photon data.
