It is shown that at a sufficiently strong longitudinal magnetic field there may arise resonant amplification of neutrino oscillations. The resonance width does not decrease with decreasing vacuum mixing angle, and the resonance condition does not depend on the energy of neutrinos. The phenomenon under consideration may take place in the vicinity of collapsing stars provided neutrinos are highly degenerate in mass.
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Akhmedov et al. (1988) studied this question.
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