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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Future MeV telescopes could constrain axion-photon couplings to 1.61 × 10^{-13} GeV^{-1} for ALP masses below 10^{-9} eV using signals from galactic supernovae.
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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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Unveiling axion signals in galactic supernovae with future MeV telescopes
Future MeV telescopes could constrain axion-photon couplings to 1.61 × 10^{-13} GeV^{-1} for ALP masses below 10^{-9} eV using signals from galactic supernovae.