Dark matter (DM) is a major constituent of the Universe. However, no definite evidence of DM particles (denoted as "χ") has been found in DM direct detection (DD) experiments to date. There is a novel concept of detecting χ from evaporating primordial black holes (PBHs). We search for χ emitted from PBHs by investigating their interaction with target electrons. The examined PBH masses range from 1×10 15 to 7×10 16 g under the current limits of PBH abundance fP BH . Using 205.4 kg•day data obtained from the CDEX-10 experiment conducted in the China Jinping Underground Laboratory, we exclude the χ-electron (χ-e) elastic-scattering cross section σχe ∼ 5 × 10 −29 cm 2 for χ with a mass mχ ≲ 0.1 keV from our results. If (mχ, σχe) can be determined in the future, DD experiments are expected to impose strong constraints on fP BH for large MP BH s.