par Chamel, Nicolas 
;Pearson, Michael J.M.;Potekhin, Alexander Yu;Fantina, Anthea ;Ducoin, Camille;Dutta, April Kumar;Goriely, Stéphane ;Perot, Loïc
Référence AIP Conference Proceedings, 2127, 020021
Publication Publié, 2019-07-01
;Pearson, Michael J.M.;Potekhin, Alexander Yu;Fantina, Anthea ;Ducoin, Camille;Dutta, April Kumar;Goriely, Stéphane ;Perot, Loïc Référence AIP Conference Proceedings, 2127, 020021
Publication Publié, 2019-07-01
Article révisé par les pairs
| Résumé : | The role of the symmetry energy on the internal constitution and the global structure of a cold nonaccreted neutron star is studied using a set of unified equations of state. Based on the nuclear energy-density functional theory, these equations of state provide a thermodynamically consistent treatment of all regions of the star and were calculated using the four different Brussels-Montreal functionals BSk22, BSk24, BSk25 and BSk26. Our predictions are compared to various constraints inferred from astrophysical observations including the recent detection of the gravitational wave signal GW170817 from a binary neutron-star merger. |
