Sub-MeV cold dark-matter particles are unable to produce electronic recoil in conventional
dark-matter direct detection experiments such as XENONnT and LUX-ZEPLIN above the detector
threshold. The mechanism of boosted dark matter comes into picture to constrain the parameter
space of such low mass dark matter from direct detection experiments. We consider the effect of
the leading components of cosmic rays to boost the cold dark matter, which results in significant
improvements on the exclusion limits compared to the existing ones. To present concrete study
results, we choose to work on models consisting of a dark-matter particle χ with an
additional U(1)' gauge symmetry including the secluded dark photon, U(1)B-L, and
U(1)L
e-L
μ
. We find that the energy dependence of the scattering cross section plays a
crucial role in improving the constraints. In addition, we systematically estimate the Earth
shielding effect on boosted dark matter in losing energy while traveling to the underground
detector through the Earth.