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O-17(p,alpha)N-14 reaction measurement at astrophysical energies

Abstract : The O-17(p,alpha)N-14 reaction is of paramount importance for the nucleosynthesis in a number of stellar sites, including red giants (RG), asymptotic giant branch (AGB) stars, massive stars and classical novae. We report on the indirect study of the O-17(p,alpha)N-14 reaction via the Trojan Horse Method by applying the approach recently developed for extracting the resonance strength of narrow resonance in the ultra-low energy region.
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http://hal.in2p3.fr/in2p3-01165516
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Submitted on : Friday, June 19, 2015 - 12:14:38 PM
Last modification on : Wednesday, September 16, 2020 - 5:45:24 PM

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L. Sergi M., C. Spitaleri, G. Pizzone R., . Burjan S. V., S. Cherubini, et al.. O-17(p,alpha)N-14 reaction measurement at astrophysical energies. SEVENTH EUROPEAN SUMMER SCHOOL ON EXPERIMENTAL NUCLEAR ASTROPHYSICS, Sep 2013, Santa Tecla, Italy. pp.208-210, ⟨10.1063/1.4875312⟩. ⟨in2p3-01165516⟩

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