par Fantina, Anthea ;Khan, Elias;Colò, Gianluca;Paar, Nils;Vretenar, Dario
Référence EPJ web of conferences, 66, page (02035)
Publication Publié, 2014-03-20
Référence EPJ web of conferences, 66, page (02035)
Publication Publié, 2014-03-20
Article révisé par les pairs
Résumé : | In this work, electron-capture rates on nuclei for stellar conditions are calculated for Ni isotopes, using a self-consistent microscopic model based on the finite temperature Skyrme Hartree-Fock plus finite-temperature charge-exchange random phase approximation approach. The results of the calculations show that electron-capture rates obtained either with different Skyrme sets or with different available models can differ by up to a few orders of magnitude. |