Adding microscopic beta-decay rates to supernova simulations makes the pre-bounce antineutrino signal orders of magnitude brighter than positron-capture-only models.
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Enhanced antineutrino emission from $\beta$ decay in core-collapse supernovae with self-consistent weak decay rates
Adding microscopic beta-decay rates to supernova simulations makes the pre-bounce antineutrino signal orders of magnitude brighter than positron-capture-only models.