  The primordial black holes (PBHs) play as a novel source to radiate light
elementary particles of energies in the region of a few hundred MeV. We explore
the possibility that the axion-like particles (ALPs) with mass less than 1 MeV
are produced from PBH evaporation. The absorption of light ALPs in the
underground detector targets then induces energetic photoelectron signatures in
current and future neutrino experiments. Utilizing the PBH ALP event rate, we
place general exclusion limits on the axion couplings at Super-K and Hyper-K.
We also translate these limits into the upper bound on the fraction of DM
composed of PBHs $f_{\rm PBH}$.
