In magnetorotational stellar collapses, neutrinos undergo resonant flavor conversion in matter plus magnetic-moment-driven chirality flipping for Majorana neutrinos, producing orientation-dependent event rates at detectors that peak 400-600 ms after bounce.
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Superposition of neutrino helicity states creates azimuthal asymmetry in recoil momenta for scattering on electrons, protons, and nuclei, offering a way to observe spin oscillations with directional detection.
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Matter- and magnetically-driven flavor conversion of neutrinos in magnetorotational collapses
In magnetorotational stellar collapses, neutrinos undergo resonant flavor conversion in matter plus magnetic-moment-driven chirality flipping for Majorana neutrinos, producing orientation-dependent event rates at detectors that peak 400-600 ms after bounce.
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The potential of directional neutrino detection to observe neutrino spin oscillations
Superposition of neutrino helicity states creates azimuthal asymmetry in recoil momenta for scattering on electrons, protons, and nuclei, offering a way to observe spin oscillations with directional detection.