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  • Author(s):
    Michael Wiescher, de Boer, R.J. , Bardayan, D.W., Go¨rres, J.

    Background: The slowest reaction in the first CNO cycle is 14N(p,γ ) 15O, therefore its rate determines the overall energy production efficiency of the entire cycle. The cross section presents several strong resonance contributions, especially for the ground-state transition. Some of the properties of the corresponding levels in the 15O compound nucleus remain uncertain, which affects the uncertainty in extrapolating the capture cross section to the low energy range of astrophysical interest….

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