Presupernova neutrino signals as potential probes of neutrino mass hierarchy.

We assess the potential of using presupernova neutrino signals at the Jiangmen Underground Neutrino Observatory (JUNO) to probe the yet-unknown neutrino mass hierarchy. Using models for stars of 12, 15, 20, and 25 M ⊙ , we find that if the ν ¯ e signals from such a star can be predicted precisely and the star is within ≈440–880 pc, the number of ν ¯ e + p → n + e + events detected within one day of its explosion allows to determine the hierarchy at the ≳ 95 % confidence level. For determination at this level using such signals from Betelgeuse, which is at a distance of ≈222 pc, the uncertainty in the predicted number of signals needs to be ≲14–30%. In view of more realistic uncertainties, we discuss and advocate a model-independent determination using both ν e and ν ¯ e signals from Betelgeuse. This method is feasible if the cosmogenic background for ν - e scattering events can be reduced by a factor of ∼2.5–10 from the current estimate. Such reduction might be achieved by using coincidence of the background events, the exploration of which for JUNO is highly desirable. [ABSTRACT FROM AUTHOR]