Speaker
Valentina De Romeri
(IFIC (CSIC-Univ Valencia))
Description
Primordial black holes (PBHs) are a potential dark matter candidate whose masses can span over many orders of magnitude. If they have masses in the 10^15 − 10^17 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 DUNE and THEIA. We will show that they will be able to set competitive constraints on PBH dark matter, thus providing complementary probes in a part of the PBH parameter space currently constrained mainly by photon data.
Primary authors
Valentina De Romeri
(IFIC (CSIC-Univ Valencia))
Pablo Martínez-Miravé
(IFIC (CSIC - Universitat de Valencia))
Mariam Tórtola
(IFIC (CSIC-Univ. Valencia))
