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

Proceedings article published in 2013 by L. Sergi M., C. Spitaleri, G. Pizzone R., S. Burjan, S. Cherubini, A. Coc, M. Gulino, F. Hammache ORCID, Z. Hons, B. Irgaziev, Kroha, Rg G. Pizzone, M. La Cognata ORCID, G. Kiss G., N. de Sereville and other authors.
This paper was not found in any repository; the policy of its publisher is unknown or unclear.
This paper was not found in any repository; the policy of its publisher is unknown or unclear.

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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.