Matter gradients slow but do not suppress neutrino-mass-induced flavor instabilities, so flavomon ray tracing is required instead of local stability analysis alone.
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Small initial flavor perturbations in an inhomogeneous neutrino distribution exhibit chaotic divergence at small scales while domain-averaged density matrices stay stable.
Core collapse supernova models have demonstrated the neutrino shock reheating mechanism in three dimensions but require substantially more rigorous treatments of neutrino kinetics, fluid instabilities, magnetic fields, strong gravity, and nuclear physics to achieve quantitative predictive power.
citing papers explorer
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Flavomon ray tracing in matter gradients
Matter gradients slow but do not suppress neutrino-mass-induced flavor instabilities, so flavomon ray tracing is required instead of local stability analysis alone.
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Chaos in Inhomogeneous Neutrino Fast Flavor Instability
Small initial flavor perturbations in an inhomogeneous neutrino distribution exhibit chaotic divergence at small scales while domain-averaged density matrices stay stable.
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Core Collapse Supernova Modeling: The Next Ten Years
Core collapse supernova models have demonstrated the neutrino shock reheating mechanism in three dimensions but require substantially more rigorous treatments of neutrino kinetics, fluid instabilities, magnetic fields, strong gravity, and nuclear physics to achieve quantitative predictive power.