par Pearson, Michael J.;Goriely, Stéphane 
;Chamel, Nicolas
Référence International journal of mass spectrometry, 349, 1, page (57)
Publication Publié, 2013-09-01
;Chamel, Nicolas Référence International journal of mass spectrometry, 349, 1, page (57)
Publication Publié, 2013-09-01
Article révisé par les pairs
| Résumé : | We review the various microscopic mass models based on effective interactions that have been developed in recent years, primarily with a view to extrapolation from the mass data to the highly neutron-rich environments that are encountered in various astrophysical contexts but that are experimentally inaccessible. All these models are based on the Hartree-Fock-Bogoliubov method, and use either Skyrme-type or Gogny-type effective interactions; they are likewise all constrained by many-body calculations on neutron matter with realistic nucleonic interactions. © 2013 Elsevier B.V. All rights reserved. |
