Astrophysical S-factor of the 15N(p,α)12C Reaction at sub-Coulomb Energies via the Trojan-Horse Method

Details Astrophysical S-factor of the 15N(p,α)12C Reaction at sub-Coulomb Energies via the Trojan-Horse Method Astrophysical S-factor of the 15N(p,α)12C Reaction at sub-Coulomb Energies via the Trojan-Horse Method

Nov 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..378..125l&link_type=abstract

Why Galaxies Care About AGB Stars: Their Importance as Actors and Probes. ASP Conference Series, Vol. 378, proceedings of the co

Astronomy and Astrophysics

Astrophysics

Scientific paper

The bare-nucleus astrophysical S-factor for the 15N
(p,α)12C 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.

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