{
  "id": "nucl-th/9604041",
  "version": "v1",
  "published": "1996-04-25T09:57:45.000Z",
  "updated": "1996-04-25T09:57:45.000Z",
  "title": "Superfluidity in beta-stable neutron star matter",
  "authors": [
    "Oe. Elgaroey",
    "L. Engvik",
    "M. Hjorth-Jensen",
    "E. Osnes"
  ],
  "comment": "7 pages, RevTex latex style, 3 figs included",
  "journal": "Phys.Rev.Lett.77:1428-1431,1996",
  "doi": "10.1103/PhysRevLett.77.1428",
  "categories": [
    "nucl-th"
  ],
  "abstract": "In this work we present results for pairing gaps in $\\beta$--stable neutron star matter with electrons and muons using a relativistic Dirac--Brueckner--Hartree--Fock approach, starting with modern meson--exchange models for the nucleon--nucleon interaction. Results are given for superconducting $^1S_0$ protons and $^3P_2$ and $^1D_2$ neutron superfluids. A comparison is made with recent non--relativistic calculations and the implications for neutron star cooling are discussed.",
  "revisions": [
    {
      "version": "v1",
      "updated": "1996-04-25T09:57:45.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "beta-stable neutron star matter",
      "superfluidity",
      "relativistic dirac-brueckner-hartree-fock approach",
      "neutron superfluids",
      "nucleon-nucleon interaction"
    ],
    "tags": [
      "journal article"
    ],
    "publication": {
      "publisher": "APS",
      "journal": "Phys. Rev. Lett."
    },
    "note": {
      "typesetting": "RevTeX",
      "pages": 7,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 418023
    }
  }
}