Varying mass loss and overshooting in RSG models shows core contraction and heating interrupted by silicon burning, shifting pre-SN neutrino flux to higher energies and beta-process dominance hours before collapse.
Davies, Red supergiants as supernova progenitors, Philosophical Transactions of the Royal Society of Lon- don Series A375, 20160270 (2017)
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The Effect of Mass Loss and Convective Overshooting on the Pre-Collapse Structure, Composition, and Neutrino Emission of Red Supergiants
Varying mass loss and overshooting in RSG models shows core contraction and heating interrupted by silicon burning, shifting pre-SN neutrino flux to higher energies and beta-process dominance hours before collapse.