Study of the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mmultiscripts><mrow><mi mathvariant="normal">N</mi></mrow><mprescripts></mprescripts><mrow></mrow><mrow><mn>13</mn></mrow><mrow></mrow><mrow></mrow></mmultiscripts></mrow></math>(d,n<math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><msup><mrow><mo>)</mo></mrow><mrow><mn>14</mn></mrow></msup></mrow></math>O reaction cross section and its astrophysical implications for the <math xmlns="http://www.w3.org/1998/Math/MathML" display="inline"><mrow><mmultiscripts><mrow><mi mathvariant="normal">N</mi></mrow><mprescripts></mprescripts><mrow></mrow><mrow><mn>13</mn></mrow><mrow></mrow><mrow></mrow></mmultiscripts></mrow></math> proton capture reaction

P. Decrock; M. Gaelens; M. Huyse; G. Reusen; G. Vancraeynest; P. Van Duppen; J. Wauters; Th. Delbar; W. Galster; P. Leleux; I. Licot; E. Liénard; P. Lipnik; C. Michotte; J. Vervier; H. Oberhummer

doi:10.1103/PhysRevC.48.2057

Study of the ${}^{13}N$ (d,n $)^{14}$ O reaction cross section and its astrophysical implications for the ${}^{13}N$ proton capture reaction

P. Decrock, M. Gaelens, M. Huyse, G. Reusen, G. Vancraeynest, P. Van Duppen, J. Wauters, Th. Delbar, W. Galster, P. Leleux, I. Licot, E. Liénard, P. Lipnik, C. Michotte, J. Vervier, and H. Oberhummer

Phys. Rev. C 48, 2057 – Published 1 October 1993

Abstract

The total cross section for the ${}^{13}N$ (d,n $)^{14}$ $O_{g . s .}$ reaction has been measured with ${}^{13}N$ 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 ${}^{13}N$ (p,γ $)^{14}$ O 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 nonresonant contribution.