O-17(p,alpha)N-14 reaction measurement at astrophysical energies
- Sergi M., L.
- Spitaleri, C.
- Pizzone R., G.
- Burjan S. V., .
- Cherubini, S.
- Coc, A.
- Gulino, M.
- Hammache, F.
- Hons, Z.
- Irgaziev, B.
- Kiss G., G.
- Kroha, V.
- La Cognata, M.
- Lamia, L.
- Mukhamedzhanov, A.
- Puglia, S.M.R.
- Rapisarda G., G.
- Romano, S.
- De Sereville, N.
- Somorjai, E.
- Tumino, A.
DOIAbstract
International audienceThe 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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