Abstract

Multi-messenger astronomy can be a relevant tool for getting information about neutrino masses and their ordering using the measurement of the time lapses between the arrival of neutrinos and the other light messenger, e.g. the graviton, emitted in astrophysical catastrophes. We elucidate the experimental reach and challenges for planned neutrino detectors such as Hyper-Kamiokande as well as future several megaton detectors.

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