After calibrating the neutrino-process yields to the observed 11B/10B ratio, the model predicts that AGB stars, not the neutrino process, supply most of the present-day fluorine in the galaxy.
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Constraining $\nu$-Process Production of Fluorine through Cosmic Ray Nucleosynthesis
After calibrating the neutrino-process yields to the observed 11B/10B ratio, the model predicts that AGB stars, not the neutrino process, supply most of the present-day fluorine in the galaxy.