Flavor stability analysis of supernova neutrino fluxes compared with simulations
Solar and Stellar Astrophysics
2011-10-26 v1 High Energy Physics - Phenomenology
Abstract
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.
Keywords
Cite
@article{arxiv.1110.5572,
title = {Flavor stability analysis of supernova neutrino fluxes compared with simulations},
author = {Srdjan Sarikas and Georg Raffelt},
journal= {arXiv preprint arXiv:1110.5572},
year = {2011}
}
Comments
Contribution to the Proceedings of HANSE 2011 workshop, 4 pages, 2 figures