Solar Neutrino Constraints on Inelastic Dark Matter Scattering in Light of Recent LUX-ZEPLIN Observations

Solar Neutrino Constraints on Inelastic Dark Matter Scattering in Light of Recent LUX-ZEPLIN Observations

A single 248 keV nuclear recoil in LUX-ZEPLIN leads far beyond an underground xenon detector. Inelastic dark matter that can scatter with nuclei on Earth may also be captured inside the Sun, where subsequent annihilation could leave a very different signature: high-energy neutrinos reaching IceCube. Connecting these two experimental environments creates an unusually broad test of dark matter masses, mass splittings, nuclear interactions, and possible annihilation channels.

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