# S-factor of 14N(p,γ)15O at astrophysical energies⋆

@article{Imbriani2005SfactorO1,
title={S-factor of 14N(p,$\gamma$)15O at astrophysical energies⋆},
author={Gianluca Imbriani and Heide Costantini and Alba Formicola and Alberto Vomiero and Carmen Angulo and Daniel Bemmerer and Roberto Bonetti and Carlo Broggini and Federica Confortola and Pietro Corvisiero and J. Cruz and Pierre Descouvemont and Zs. F{\"u}l{\"o}p and Gianpiero Gervino and Alessandra Guglielmetti and C Gustavino and Gy. Gy{\"u}rky and A. P. Jesus and Markus Junker and J. N. Klug and Alberto Lemut and R. Menegazzo and Paolo Prati and Vincent Roca and Claus E. Rolfs and Mario R. Romano and C. Rossi-Alvarez and F. Schuemann and D. Sch{\"u}rmann and E. Somorjai and Oscar Straniero and Frank Strieder and Filippo Terrasi and H. P. Trautvetter},
journal={The European Physical Journal A - Hadrons and Nuclei},
year={2005},
volume={25},
pages={455-466}
}
Abstract.The astrophysical S(E) factor of 14N(p,γ)15O has been measured for effective center-of-mass energies between Eeff = 119 and 367 keV at the LUNA facility using TiN solid targets and Ge detectors. The data are in good agreement with previous and recent work at overlapping energies. R-matrix analysis reveals that due to the complex level structure of 15O the extrapolated S(0) value is model dependent and calls for additional experimental efforts to reduce the present uncertainty in S(0… Expand
107 Citations
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