  We propose the first experimental test of the inelastic boosted dark matter
hypothesis, capitalizing on the new physics potential with the imminent data
taking of the ProtoDUNE detectors. More specifically, we explore various
experimental signatures at the cosmic frontier, arising in boosted dark matter
scenarios, i.e., relativistic, inelastic scattering of boosted dark matter
often created by the annihilation of its heavier component which usually
comprises of the dominant relic abundance. Although features are unique enough
to isolate signal events from potential backgrounds, vetoing a vast amount of
cosmic background is rather challenging as the detectors are located on the
ground. We argue, with a careful estimate, that such backgrounds nevertheless
can be well under control by performing dedicated analyses after data
acquisition. We then discuss some phenomenological studies which can be
achieved with ProtoDUNE, employing a dark photon scenario as our benchmark
dark-sector model.
