Asymptotic normalization coefficients for 14N+p -> O-15 and the astrophysical S factor for N-14(p, gamma)O-15
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The [Formula Presented] reaction, which controls energy production in the CNO cycle, has contributions from both resonance and direct captures to the ground and excited states. The overall normalization of the direct captures is defined by the corresponding asymptotic normalization coefficients (ANCs). Especially important is the ANC for the subthreshold state in [Formula Presented] at [Formula Presented] since direct capture through this state dominates the reaction rate at stellar energies. In order to determine the ANCs for [Formula Presented] the [Formula Presented] proton transfer reaction has been measured at an incident energy of 26.3 MeV. Angular distributions for proton transfer to the ground and five excited states were obtained. ANCs were then extracted from comparison to both distorted-wave Born approximation and coupled-channels Born approximation calculations. Using these ANCs, we calculated the astrophysical factor and reaction rates for [Formula Presented] Our analysis favors a low value for the astrophysical factor. 2003 The American Physical Society.
author list (cited authors)
Mukhamedzhanov, A. M., Bem, P., Brown, B. A., Burjan, V., Gagliardi, C. A., Kroha, V., ... Vincour, J.
complete list of authors
Mukhamedzhanov, AM||Bem, P||Brown, BA||Burjan, V||Gagliardi, CA||Kroha, V||Novak, J||Nunes, FM||Paskor, S||Pirlepesov, F||Simeckova, E||Tribble, RE||Vincour, J