Flavor stability analysis of supernova neutrino fluxes compared with   simulations
  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. 
Srdjan Sarikas and Georg Raffelt
astro-ph.SR hep-ph