  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. We focus
on two next generation facilities: the Deep Underground Neutrino Experiment
(DUNE) and THEIA. We simulate the expected event spectra at both experiments
assuming different PBH mass distributions and spins, and we extract the
expected 95% C.L. sensitivities to these scenarios. Our analysis shows that
future neutrino experiments like DUNE and THEIA 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.
