  We present a new multi-component dark matter model with a novel experimental
signature that mimics neutral current interactions at neutrino detectors. In
our model, the dark matter is composed of two particles, a heavier dominant
component that annihilates to produce a boosted lighter component that we refer
to as boosted dark matter. The lighter component is relativistic and scatters
off electrons in neutrino experiments to produce Cherenkov light. This model
combines the indirect detection of the dominant component with the direct
detection of the boosted dark matter. Directionality can be used to distinguish
the dark matter signal from the atmospheric neutrino background. We discuss the
viable region of parameter space in current and future experiments.
