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Inverted Hierarchy of Neutrino Masses Disfavored by Supernova 1987A

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We discuss the flavor conversion of supernova neutrinos in the three-flavor mixing scheme of neutrinos. We point out that by neutrino observation from supernova one can discriminate the inverted hierarchy of neutrino masses from the normal one if s_{13}^2 \gsim a few \times 10^{-4}, irrespective of which oscillation solution to the solar neutrino problem is realized in nature. We perform an analysis of data of SN1987A and obtain a strong indication that the inverted mass hierarchy is disfavored unless s_{13}^2 \lsim a few \times 10^{-4}.

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  • The flux of electron antineutrinos from supernova SN1987A data hep-ph · 2025-01-16 · conditional · none · ref 50 · internal anchor

    A refined fit of the SN1987A antineutrino data finds accretion at about 99% confidence and a small, theory-compatible neutron fraction, closing a tension in older analyses.