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  1. Modern CCSN models (O'Connor et al. 2018) have commonly predicted the existence of the so-called neutronization neutrino burst with a peak luminosity ∼4 × 10 53 erg s −1, which emerges during the first ∼25 ms after the core bounce as a result of sudden breakout of a flood of neutrinos freshly produced in shock-heated matter (and some νe produced previously that have diffused to the neutrinosphere) when the bounce shock penetrates the neutrinosphere and reaches the neutrino-transparent regime at sufficiently low densities.
    iopscience.iop.org/article/10.3847/2041-8213/ac4014
    iopscience.iop.org/article/10.3847/2041-8213/ac4014
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