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Statut |
Confirmé |
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Série |
IPN-THEO |
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Domaines |
nucl-th |
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Date |
Mardi 21 Mars 2017 |
|
Heure |
11:30 |
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Institut |
IPN |
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Salle |
IPN, Bâtiment 100, salle A 015 |
|
Nom de l'orateur |
Sagawa |
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Prenom de l'orateur |
Hiroyuki |
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Addresse email de l'orateur |
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Institution de l'orateur |
RIKEN Nishina Center, Wako, Japan |
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Titre |
Nuclear collective excitations and EoS |
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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 |
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Numéro de preprint arXiv |
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Commentaires |
$$ |
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Fichiers attachés |
- 2017_03_21_H_Sagawa.pdf (206701 bytes)
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