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$Δ(1232)$ isobars and neutrino opacities in hot dense matter
high-energy-astrophysical-phenomenahigh-energy-physics-phenomenologyhigh-energy-physics-theorynuclear-theory
We calculated the diffusion mean free paths of electron neutrinos and antineutrinos in hot, neutrino-trapped matter containing $Δ(1232)$ isobars, as found in proto-neutron stars and neutron star merger remnants. We included charged-current absorption with the $NΔ$ weak vertex of weak pion production
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