par Ryssens, Wouter ;Scamps, Guillaume ;Grams, Guilherme ;Kullmann, Ina ;Bender, Michaël ;Goriely, Stéphane
Editeur scientifique Azaiez, Faiçal;Wiedeking, M.
Référence INPC2022(28: 11/09/2022 - 16/09/2022: Cape Town, South Africa), 28th International Nuclear Physics Conference, Journal of physics. Conference series (Online) (2586), 012097
Publication Publié, 2023-09-25
Publication dans des actes
Résumé : Accurate estimates of the binding energy of nuclei far from stability that cannot be produced in the laboratory are crucial to our understanding of nuclear processes in astrophysical scenarios. Models based on energy density functionals have shown that they are capable of reproducing all known masses with root-mean-square error better than 800 keV, while retaining a firm microscopic foundation. However, it was recently pointed out in [M. Hukkanen et al., arXiv:2210.10674] that the recent BSkG1 model fails to account for a contribution to the binding energy that is specific to odd-odd nuclei, and which can be studied by using appropriate mass difference formulas. We analyse here the (lacking) performance of three recent microscopic mass models with respect to such formulas and examine possibilities to remedy this deficiency in the future.