Determination of the N13(p)14O reaction cross section using a N13 radioactive ion beam

P. Decrock, Th. Delbar, P. Duhamel, W. Galster, M. Huyse, P. Leleux, I. Licot, E. Liénard, P. Lipnik, M. Loiselet, C. Michotte, G. Ryckewaert, P. Van Duppen, J. Vanhorenbeeck, and J. Vervier
Phys. Rev. Lett. 67, 808 – Published 12 August 1991
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Abstract

The cross section for the astrophysically important N13(p)14O reaction has been measured directly with an intense (3×108 particles/s) and pure (>99%) 8.2-MeV N13 radioactive ion beam. The average value, for the 5.8–8.2-MeV N13 energy range, is 106(30) μb. The partial γ width of the resonance which occurs in this reaction at a center-of-mass energy of 0.545 MeV has been deduced to be 3.8(1.2) eV. It is compared with theoretical predictions and indirect determinations.

  • Received 2 May 1991

DOI:https://doi.org/10.1103/PhysRevLett.67.808

©1991 American Physical Society

Authors & Affiliations

P. Decrock, Th. Delbar, P. Duhamel, W. Galster, M. Huyse, P. Leleux, I. Licot, E. Liénard, P. Lipnik, M. Loiselet, C. Michotte, G. Ryckewaert, P. Van Duppen, J. Vanhorenbeeck, and J. Vervier

  • Institut de Physique Nucléaire and Centre de Recherches du Cyclotron, Université Catholique de Louvain, B-1348 Louvain-la-Neuve, Belgium
  • Instituut voor Kern- en Stralingsfysika, Katholieke Universiteit Leuven, B-3001 Leuven, Belgium
  • Institut d’Astronomie et d‘Astrophysique, Université Libre de Bruxelles, B-1050 Bruxelles, Belgium

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Vol. 67, Iss. 7 — 12 August 1991

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