Statut | Confirmé |
Série | NUC-THEO |
Domaines | nucl-th |
Date | Mardi 21 Mars 2017 |
Heure | 11:30 |
Institut | IPN |
Salle | IPN, Bâtiment 100, salle A 015 |
Nom de l'orateur | Sagawa |
Prenom de l'orateur | Hiroyuki |
Addresse email de l'orateur | |
Institution de l'orateur | RIKEN Nishina Center, Wako, Japan |
Titre | Nuclear collective excitations and EoS |
Résumé | EoS (equations of states) is one of the most important ingredients for the study of neutron stars and supernova explosions. I will discuss the constrains on EoS from nuclear structure information. First, the isoscalar giant monopole resonances (ISGMR) are calculated by self-consistent HF+RPA or HF+BCS+QRPA and compared with available experimental data of closed shell and open-shell nuclei. A difference between empirical incompressibility between closed and open-shell nuclei is critically examined. Furthermore, the isotope dependence of ISGMR is studied in relation with the symmetry energy expansion terms J, L and Ksym. The symmetry energy coefficient constrains from other collective excitations and mass models are also mentioned |
Numéro de preprint arXiv | |
Commentaires | $$ |
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