|
Statut |
Confirmé |
|
Série |
NUC-THEO |
|
Domaines |
nucl-ex,nucl-th |
|
Date |
Vendredi 23 Mars 2018 |
|
Heure |
11:00 |
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Institut |
IPN |
|
Salle |
Bâtiment 100, Salle A018 (Bibliothèque) |
|
Nom de l'orateur |
Fantina |
|
Prenom de l'orateur |
A. |
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Addresse email de l'orateur |
|
|
Institution de l'orateur |
GANIL |
|
Titre |
Nuclear physics inputs for core-collapse supernova and neutron-star physics |
|
Résumé |
Compact stars such as neutron stars and supernovae are unique
laboratories to probe matter in extreme conditions. Nuclear physics
experiments, in tandem with astrophysical observations, can give
valuable insight in to the properties of dense matter encountered in
these stellar objects.
In this seminar, I will discuss the importance of some nuclear physics
inputs in the description of these compact stars. In particular, the
impact of nuclear masses of neutron-rich nuclei for the compact-star
modelling will be discussed. Moreover the dense matter found in
neutron stars and supernovae being very neutron rich, a correct
description of the symmetry-energy contribution to the nuclear energy
is of great importance. The role of the symmetry energy on some
properties of the neutron-star structure and composition will be
addressed. |
|
Numéro de preprint arXiv |
|
|
Commentaires |
$ $ |
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Fichiers attachés |
- 2018_03_23_A_Fantina-commun.pdf (1180594 bytes)
|
