Comparison of low--energy resonances in 15N(alpha,gamma)19F and 15O(alpha,gamma)19Ne and related uncertainties
F. de Oliveira, A. Coc, P. Aguer, G. Bogaert, J. Kiener, A. Lefebvre, V. Tatischeff, J. -P. Thibaud, S. Fortier, J. M. Maison, L. Rosier, G. Rotbard, J. Vernotte, S. Wilmes, P. Mohr, V. Kölle, G. Staudt
Abstract
A disagreement between two determinations of Gammaalpha of the astro- physically relevant level at Ex=4.378 MeV in 19F has been stated in two recent papers by Wilmes et al. and de Oliveira et al. In this work the uncertainties of both papers are discussed in detail, and we adopt the value Gammaalpha=(1.5+1.5-0.8)10-9eV for the 4.378 MeV state. In addition, the validity and the uncertainties of the usual approximations for mirror nuclei Gammagamma(19F) approx Gammagamma(19Ne), theta2alpha(19F) approx theta2alpha(19Ne) are discussed, together with the resulting uncertainties on the resonance strengths in 19Ne and on the 15O(alpha,gamma)19Ne rate.
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