{
  "id": "0808.0233",
  "version": "v2",
  "published": "2008-08-02T07:09:22.000Z",
  "updated": "2008-11-18T20:25:38.000Z",
  "title": "Cluster formation in compact stars: relativistic versus Skyrme models",
  "authors": [
    "Camille Ducoin",
    "Constança Providência",
    "Alexandro M. Santos",
    "Lucilia Brito",
    "Philippe Chomaz"
  ],
  "comment": "Accepted for publication",
  "journal": "Phys.Rev.C78:055801,2008",
  "doi": "10.1103/PhysRevC.78.055801",
  "categories": [
    "nucl-th",
    "astro-ph"
  ],
  "abstract": "We present various properties of nuclear and compact-star matter, comparing the predictions from two kinds of phenomenological approaches: relativistic models (both with constant and density-dependent couplings) and non-relativistic Skyrme-type interactions. We mainly focus on the liquid-gas instabilities that occur at sub-saturation densities, leading to the decomposition of the homogeneous matter into a clusterized phase. Such study is related to the description of neutron-star crust (at zero temperature) and of supernova dynamics (at finite temperature).",
  "revisions": [
    {
      "version": "v2",
      "updated": "2008-11-18T20:25:38.000Z"
    }
  ],
  "analyses": {
    "subjects": [
      "21.65.-f",
      "24.10.Jv",
      "26.60.-c",
      "95.30.Tg"
    ],
    "keywords": [
      "compact stars",
      "skyrme models",
      "cluster formation",
      "non-relativistic skyrme-type interactions",
      "zero temperature"
    ],
    "tags": [
      "journal article"
    ],
    "publication": {
      "publisher": "APS",
      "journal": "Physical Review C",
      "year": 2008,
      "month": "Nov",
      "volume": 78,
      "number": 5,
      "pages": "055801"
    },
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 792168,
      "adsabs": "2008PhRvC..78e5801D"
    }
  }
}