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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
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Abstract

A disagreement between two determinations of Gamma_alpha of the astro- physically relevant level at E_x=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 Gamma_alpha=(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 Gamma_gamma(19F) approx Gamma_gamma(19Ne), theta^2_alpha(19F) approx theta^2_alpha(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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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. 1997-03-17. Comparison of low--energy resonances in 15N(alpha,gamma)19F and 15O(alpha,gamma)19Ne and related uncertainties. https://doi.org/10.1103/physrevc.55.3149

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