Neutron-star matter within the energy-density functional theory and neutron-star structure
Journal Article
·
· AIP Conference Proceedings
- Institut d'Astronomie et d'Astrophysique, CP226, Université Libre de Bruxelles (ULB), 1050 Brussels (Belgium)
- Dépt. de Physique, Université de Montréal, Montréal (Québec), H3C 3J7 (Canada)
In this lecture, we will present some nucleonic equations of state of neutron-star matter calculated within the nuclear energy-density functional theory using generalized Skyrme functionals developed by the Brussels-Montreal collaboration. These equations of state provide a consistent description of all regions of a neutron star. The global structure of neutron stars predicted by these equations of state will be discussed in connection with recent astrophysical observations.
- OSTI ID:
- 22391016
- Journal Information:
- AIP Conference Proceedings, Vol. 1645, Issue 1; Conference: Carpathian Summer School of Physics 2014, Sinaia (Romania), 13-26 Jul 2014; Other Information: (c) 2015 AIP Publishing LLC; Country of input: International Atomic Energy Agency (IAEA); ISSN 0094-243X
- Country of Publication:
- United States
- Language:
- English
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