Neutrino rates in proto-neutron-star matter differ by up to an order of magnitude with the Sky3s Skyrme parametrization versus SLy4, and beta equilibrium is less violated at finite temperature.
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Charged current neutrino processes in hot nuclear matter with a recent Skyrme parametrization constrained by microscopic calculations
Neutrino rates in proto-neutron-star matter differ by up to an order of magnitude with the Sky3s Skyrme parametrization versus SLy4, and beta equilibrium is less violated at finite temperature.