  We probe dark matter-electron scattering using high-energy neutrino
observations from the Sun. Dark matter (DM) interacting with electrons can get
captured inside the Sun. These captured DM may annihilate to produce different
Standard Model (SM) particles. Neutrinos produced from these SM states can be
observed in IceCube and DeepCore. Although there is no excess of neutrinos from
the Solar direction, we find that the current data-sets of IceCube and DeepCore
set the strongest constraint on DM-electron scattering cross section in the DM
mass range $10\,$GeV to $10^5\,$GeV. Our work implies that future observations
of the Sun by neutrino telescopes have the potential to discover DM-electron
interaction.
