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.
Herwig, The evolution of agb stars with convective over- shoot, Astron
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The helium flash produces a neutrino burst with a 1.7 MeV line detectable up to almost 3 pc in future facilities, but asteroseismology remains the practical probe for now.
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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.
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Detection horizon for the neutrino burst from the stellar helium flash
The helium flash produces a neutrino burst with a 1.7 MeV line detectable up to almost 3 pc in future facilities, but asteroseismology remains the practical probe for now.