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.
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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.