Derives Coriolis-coupled neutrino-driven MHD waves and resonant instabilities in rotating magnetoplasmas with two-flavor oscillations, finding magnetosonic growth rates higher than Alfvén and instability times of 0.09-0.14 s relevant to protoneutron-star surfaces.
Serbeto, Physics Letters A296, 217 (2002)
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Coupling of neutrino beam-driven MHD waves and resonant instabilities in rotating magnetoplasmas with neutrino two-flavor oscillations
Derives Coriolis-coupled neutrino-driven MHD waves and resonant instabilities in rotating magnetoplasmas with two-flavor oscillations, finding magnetosonic growth rates higher than Alfvén and instability times of 0.09-0.14 s relevant to protoneutron-star surfaces.