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arxiv: 1110.5572 · v1 · pith:TPR25SRUnew · submitted 2011-10-25 · 🌌 astro-ph.SR · hep-ph

Flavor stability analysis of supernova neutrino fluxes compared with simulations

classification 🌌 astro-ph.SR hep-ph
keywords analysisstabilityfluxeslinearizedmodelsneutrinosupernovaaccretion-phase
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We apply a linearized stability analysis to simplified models of accretion-phase neutrino fluxes streaming from a supernova. We compare the results with recent numerical studies and find excellent agreement. This provides confidence that a linearized stability analysis can be further applied to more realistic models.

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