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Neutrino nucleosynthesis: An overview
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abstract
Neutrinos produced during a supernova explosion induce reactions on abundant nuclei in the outer stellar shells and contribute in this way to the synthesis of the elements in the Universe. This neutrino nucleosynthesis process has been identified as an important contributor to the origin of $^7$Li, $^{11}$B,$^{19}$F, $^{138}$La, and $^{180}$Ta, but also to the long-lived radionuclides $^{22}$Na and $^{26}$Al, which are both key isotopes for $\gamma$-ray astronomy. The manuscript summarizes the recent progress achieved in simulations of neutrino nucleosynthesis.
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Cited by 1 Pith paper
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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.
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