The bare-nucleus astrophysical S-factor for the (15)N(p, alpha)(12)C reaction is extracted down to zero energy by means of the Trojan-Horse Method. A fair agreement is found down to 70 keV, while the low-energy behavior of the S-factor provides a smaller rate than reported in the literature.

Astrophysical S-factor of the (15)N(p, alpha)(12)C reaction at sub-Coulomb energies via the Trojan-Horse method

Romano S;CHERUBINI, SILVIO;Pizzone, RG;Sergi ML;TUDISCO, SALVATORE;
2007-01-01

Abstract

The bare-nucleus astrophysical S-factor for the (15)N(p, alpha)(12)C reaction is extracted down to zero energy by means of the Trojan-Horse Method. A fair agreement is found down to 70 keV, while the low-energy behavior of the S-factor provides a smaller rate than reported in the literature.
2007
978-1-58381-318-8
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.11769/254927
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