par Katsuma, Masahiro
Référence AIP Conference Proceedings, 1012, page (365-367)
Publication Publié, 2008
Article révisé par les pairs
Résumé : The astrophysical S-factors of the 13C(α,n) 16O17O(α,n) 20Ne21Ne(α,n) 24Mg and 25Mg(α,n) 28Si reactions are analyzed with DWBA. The gross structures of the experimental data are reproduced by the DWBA calculations. The resulting reaction rates are compared with those in the CF88 and NACRE compilations.