Preprint
Oct 2026
An updated model of neutrino emission from proto-neutron stars
We present an improved parametric model for neutrino emission from core-collapse supernovae that directly connects neutrino luminosity and average energy to stellar properties during emission. Our model incorporates two critical physical processes: convection within the proto-neutron star and the evolution of the neutr...
M. Ballelli, F. Pompa, C. Ternes et al.
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