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$Δ(1232)$ isobars and weak-interaction bulk viscosity in neutron-star merger matter
Binary neutron star mergers probe nuclear matter at densities of a few times nuclear saturation density and temperatures of tens of MeV, conditions under which heavier baryons such as the $Δ(1232)$ isobars may appear. Previous calculations of the bulk viscosity of merger matter have considered nucle
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