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Astrophysical S-factor of 14N(p,g)15O

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arxiv nucl-ex/0312015 v2 pith:ZKNIXS4Z submitted 2003-12-12 nucl-ex astro-ph

the LUNA Collaboration: A. Formicola , G. Imbriani , H. Costantini This is my paper · ORCID
classification nucl-exastro-ph
keywords s-factorfindstatetotaltransitionacceleratoraccountsanalysis
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We report on a new measurement of the 14N(p,g)15O capture cross section at E_p = 140 to 400 keV using the 400 kV LUNA accelerator facility. The uncertainties have been reduced with respect to previous measurements and their analysis. We have analyzed the data using the R-matrix method and we find that the ground state transition accounts for about 15 % of the total S-factor. The main contribution to the S-factor is given by the transition to the 6.79 MeV state. We find a total S(0) = 1.7+/-0.2 keV b.

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  1. Background in $\gamma$-ray detectors and carbon beam tests in the Felsenkeller shallow-underground accelerator laboratory

    nucl-ex 2019-08 conditional novelty 4.0 of 10

    The Felsenkeller shallow-underground laboratory achieves gamma-ray backgrounds low enough, and carbon beam currents high enough, to make a sensitive measurement of carbon-12(alpha,gamma)oxygen-16 appear feasible.

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