Distinguishing Dirac and Majorana Neutrinos: Resonant Spin-Flavor Precession of GeV-Scale Astrophysical Transients
This paper proposes a unified formalism using Resonant Spin-Flavor Precession of GeV-scale neutrinos from solar flares and supernovae to distinguish between Dirac and Majorana neutrinos and probe magnetic moments down to , overcoming previous constraints by shifting resonance conditions to regions with specific magnetic field configurations.