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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Skyrme SV calculations give |M^{2ν}| values of 0.069, 0.040, and 0.22 MeV^{-1} for 76Ge 2νββ decay depending on g9/2 occupancy and triaxiality, with one matching the empirical 0.204 value.
citing papers explorer
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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.
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Skyrme SV density-functional analysis of the $2\nu\beta\beta$ decay in $^{76}$Ge
Skyrme SV calculations give |M^{2ν}| values of 0.069, 0.040, and 0.22 MeV^{-1} for 76Ge 2νββ decay depending on g9/2 occupancy and triaxiality, with one matching the empirical 0.204 value.