par Perot, Loïc ;Chamel, Nicolas
Référence 56th Rencontres de Moriond(56: 30 juin - 6 février 2022: La Thuile, Aosta Valley, Italie), 2022 Gravitation, Proceedings of the 56th Rencontres de Moriond, ARISF, page (25-28)
Publication Publié, 2022-10-28
Publication dans des actes
Résumé : The role of the dense matter properties on the tidal deformability and gravitational waveforms of binary neutron stars is studied using a set of unified equations of state. Based on the nuclear energy-density functional theory, these equations of state provide a thermodynamicallyconsistent treatment of all regions of the stars and were calculated using functionals that were precision fitted to experimental and theoretical nuclear data.