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• W2009225178 abstract "The dense neutrino flux streaming from a core-collapse supernova can undergo self-induced flavor conversion caused by neutrino-neutrino refraction. Numerical studies of these nonlinear effects are challenging because representing the neutrino radiation field by discrete energy and angle bins can easily lead to unphysical solutions. In particular, if the number of angle bins ${N}_{a}$ is too small, flavor conversion begins too deep and produces completely spurious results. At the same time, ${N}_{a}=1$ (single-angle approximation) can be a good proxy for the ${N}_{a}ensuremath{rightarrow}ensuremath{infty}$ limit. Based on a linearized stability analysis, we explain some of the puzzling effects of discrete angle distributions." @default.
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• W2009225178 date "2012-12-11" @default.
• W2009225178 modified "2023-10-18" @default.
• W2009225178 title "Spurious instabilities in multiangle simulations of collective flavor conversion" @default.
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• W2009225178 doi "https://doi.org/10.1103/physrevd.86.125020" @default.
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