{
  "id": "1301.2438",
  "version": "v1",
  "published": "2013-01-11T09:56:38.000Z",
  "updated": "2013-01-11T09:56:38.000Z",
  "title": "Unified description of dense matter in neutron stars and magnetars",
  "authors": [
    "N. Chamel",
    "R. L. Pavlov",
    "L. M. Mihailov",
    "Ch. J. Velchev",
    "Zh. K. Stoyanov",
    "Y. D. Mutafchieva",
    "M. D. Ivanovich",
    "A. F. Fantina",
    "J. M. Pearson",
    "S. Goriely"
  ],
  "comment": "Proceedings of IAUS 291 \"Neutron Stars and Pulsars: Challenges and Opportunities after 80 years\", J. van Leeuwen (ed.); 3 pages",
  "categories": [
    "astro-ph.HE",
    "nucl-th"
  ],
  "abstract": "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.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2013-01-11T09:56:38.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "neutron stars",
      "unified description",
      "dense matter",
      "nuclear energy density functional theory",
      "experimental atomic mass data"
    ],
    "tags": [
      "journal article"
    ],
    "publication": {
      "doi": "10.1017/S1743921312024118"
    },
    "note": {
      "typesetting": "TeX",
      "pages": 3,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 1210394,
      "adsabs": "2013IAUS..291..359C"
    }
  }
}