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S-factor of14N(p,γ)15O at astrophysical energies⋆

✍ Scribed by G. Imbriani; H. Costantini; A. Formicola; A. Vomiero; C. Angulo; D. Bemmerer; R. Bonetti; C. Broggini; F. Confortola; P. Corvisiero; J. Cruz; P. Descouvemont; Z. Fülöp; G. Gervino; A. Guglielmetti; C. Gustavino; Gy. Gyürky; A. P. Jesus; M. Junker; J. N. Klug; A. Lemut; R. Menegazzo; P. Prati; V. Roca; C. Rolfs; M. Romano; C. Rossi-Alvarez; F. Schümann; D. Schürmann; E. Somorjai; O. Straniero; F. Strieder; F. Terrasi; H. P. Trautvetter

Book ID
111618632
Publisher
Springer
Year
2005
Tongue
English
Weight
407 KB
Volume
25
Category
Article
ISSN
1434-601X

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The 14N(p,γ)15O low-energy S-factor
The 14N(p,γ)15O low-energy S-factor
✍ C. Angulo; P. Descouvemont 📂 Article 📅 2001 🏛 Elsevier Science 🌐 English ⚖ 176 KB

The 14 N(p,γ ) 15 O low-energy S-factor is analyzed using the R-matrix model. We find that the g.s. contribution is less than previously reported. The S-factor is mainly given by the 6.79 MeV state contribution which is determined by its asymptotic normalization constant (ANC). Consequently, the S-f