  In our galaxy, the white dwarfs (WDs) will inevitably capture the dark matter
(DM) particles streaming through them, if there exist interactions between DM
particles and nuclei/electrons. At the same time, these DM particles can also
be evaporated by the nuclei/electrons in a WD if they have proper mass and the
WD is not too cold. The evaporation of DM particles will lead to a faster
cooling evolution than that predicted by the stellar evolution theory. In this
work, we ascribe the faster cooling evolution of three observed WDs to the
capture and evaporation of DM particles, and get the possible DM particle's
mass and DM-electron cross section as follows: for $F(q) = 1$, $40\
\mathrm{MeV}/c^{2} \lesssim m_{\chi} \lesssim 70\ \mathrm{MeV}/c^{2}$ and
$10^{-57} \mathrm{cm}^{2} \lesssim \sigma_{\chi,e} \lesssim 10^{-55}
\mathrm{cm}^{2}$; for $F(q) = (\alpha m_{e})^{2}/q^{2}$, $30\
\mathrm{MeV}/c^{2} \lesssim m_{\chi} \lesssim 60\ \mathrm{MeV}/c^{2}$ and
$10^{-53} \mathrm{cm}^{2} \lesssim \sigma_{\chi,e} \lesssim 10^{-51}
\mathrm{cm}^{2}$. These results are beyond the detection capabilities of
current direct detection experiments and should be cross checked by more novel
scenarios in the future.
