Study of the N-13(d,N) O-14 Reaction Cross-section and its Astrophysical Implications for the N-13 Proton Capture Reaction
(1993) Physical Review C (Nuclear Physics) — Vol. 48, n° 4, p. 2057-2067 (1993)
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- Abstract
- The total cross section for the N-13(d, n)O-14g.s. reaction has been measured with N-13 radioactive beams at laboratory energies of 8.2, 12.0, 16.2, and 28.5 MeV. A spectroscopic factor of 0.9 is obtained from a distorted-wave Born approximation analysis of this transfer reaction. The astrophysical S factor for the N-13(p,gamma)O-14 reaction is calculated using the experimentally known resonance parameters for the resonant contribution and the direct-capture model with the experimental spectroscopic factor for the non-resonant contribution.
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Decrock, P., Gaelens, M., Huyse, M., Reusen, G., Vancraeynest, G., Vanduppen, P., Wauters, J., Delbar, T., Galster, W., Leleux, P., Licot, I., Lienard, E., Lipnik, P., Michotte, C., Vervier, J., & Oberhummer, H. (1993). Study of the N-13(d,N) O-14 Reaction Cross-section and its Astrophysical Implications for the N-13 Proton Capture Reaction. Physical Review C (Nuclear Physics), 48(4), 2057-2067. https://doi.org/10.1103/PhysRevC.48.2057 (Original work published 1993)