par Chamel, Nicolas ;Pavlov, Rossen;Mihailov, L.M.;Velchev, Ch. J.;Stoyanov, Zh. K.;Mutafchieva, Y. D.;Ivanovich, M. D.;Fantina, Anthea ;Pearson, Michael J.;Goriely, Stéphane
Référence IAU Symposium 291: Neutron Stars and Pulsars: Challenges and Opportunities after 80 years(20-31 August, 2012: Beijing, China), Proceedings of the International Astronomical Union, Cambridge University Press, Vol. 8, page (359-361)
Publication Publié, 2013-03-20
Publication dans des actes
Résumé : We have recently developed a set of equations of state based on the nuclear energy density functional theory providing a unified description of the different regions constituting the interior of neutron stars and magnetars. The nuclear functionals, which were constructed from generalized Skyrme effective nucleon-nucleon interactions, yield not only an excellent fit to essentially all experimental atomic mass data but were also constrained to reproduce the neutron-matter equation of state as obtained from realistic many-body calculations.