par Wanajo, Shinya;Itoh, Naoki;Goriely, Stéphane 
;Samyn, Mathieu ;Ishimaru, Yuhri
Référence Nuclear physics. A, 758, 1-4 SPEC. ISS., page (671c-674c)
Publication Publié, 2005-07
;Samyn, Mathieu ;Ishimaru, YuhriRéférence Nuclear physics. A, 758, 1-4 SPEC. ISS., page (671c-674c)
Publication Publié, 2005-07
Article révisé par les pairs
| Résumé : | We examine the effects of the newly-derived microscopic Hartree-Fock-Bogoliubov (HFB) mass formulae on the r-process nucleosynthesis and analyse to what extent a solar-like r-abundance distribution can be obtained. The r-process calculations with the HFB-2 mass formula are performed, adopting the parametrized model of the prompt explosion from a collapsing O-Ne-Mg core for the physical conditions. The result is compared with those obtained with the HFB-7 and droplet-type mass formulae. © 2005 Elsevier B.V. All rights reserved. |
