par Decrock, Patrick;Delbar, Th;Duhamel, Paul 
;Galster, Wilfried;Huyse, Mark;Leleux, Pol;Licot, I.;Liénard, Etienne;Lipnik, Peter;Loiselet, Marc;Michotte, C.;Ryckewaert, Guido;Van Duppen, Piet;Vanhorenbeeck, Jean ;Vervier, Jean
Référence Physical review letters, 67, 7, page (808-811)
Publication Publié, 1991
;Galster, Wilfried;Huyse, Mark;Leleux, Pol;Licot, I.;Liénard, Etienne;Lipnik, Peter;Loiselet, Marc;Michotte, C.;Ryckewaert, Guido;Van Duppen, Piet;Vanhorenbeeck, Jean ;Vervier, JeanRéférence Physical review letters, 67, 7, page (808-811)
Publication Publié, 1991
Article révisé par les pairs
| Résumé : | The cross section for the astrophysically important 13N(p, γ) 14O reaction has been measured directly with an intense (3 × 108 particles/s) and pure (> 99%) 8.2-MeV 13N radioactive ion beam. The average value, for the 5.8-8.2-MeV 13N 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. |
