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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Communication dans un congrès
SEVENTH EUROPEAN SUMMER SCHOOL ON EXPERIMENTAL NUCLEAR ASTROPHYSICS, Sep 2013, Santa Tecla, Italy. AIP Conference Proceedings, 1595, pp.208-210, 2014, 〈10.1063/1.4875312〉
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http://hal.in2p3.fr/in2p3-01165516
Contributeur : Emilie Bonnardel <>
Soumis le : vendredi 19 juin 2015 - 12:14:38
Dernière modification le : jeudi 11 janvier 2018 - 06:26:31

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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. AIP Conference Proceedings, 1595, pp.208-210, 2014, 〈10.1063/1.4875312〉. 〈in2p3-01165516〉

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