  Primordial black holes (PBHs) are the plausible candidates for the
cosmological dark matter. Theoretically, PBHs with masses $M_{\rm PBH}$ in the
range of $4\times10^{14}\sim 10^{17}\,{\rm g}$ can emit sub-GeV electrons and
positrons through Hawking radiation. Some of these particles could undergo
diffusive reacceleration during propagation in the Milky Way, potentially
reaching energies up to the GeV level observed by AMS-02. In this work, we
utilize AMS-02 data to constrain the PBH abundance $f_{\rm PBH}$ by employing
the reacceleration mechanism. Under the assumption of a monochromatic PBH mass
distribution, our findings reveal that the limit is stricter than that derived
from Voyager 1 data. This difference is particularly pronounced when $M_{\rm
PBH}\lesssim10^{15}\,{\rm g}$, exceeding an order of magnitude. The constraints
are even more robust in a more realistic scenario involving a log-normal mass
distribution of PBHs. Moreover, we explore the impact of varying propagation
parameters and solar modulation potential within reasonable ranges, and find
that such variations have minimal effects on the final results.
