{
  "id": "1304.4007",
  "version": "v2",
  "published": "2013-04-15T07:25:52.000Z",
  "updated": "2013-07-22T15:25:28.000Z",
  "title": "Compressed Baryonic Matter of Astrophysics",
  "authors": [
    "Yanjun Guo",
    "Renxin Xu"
  ],
  "comment": "10 pages, Contribution for the Conference Proceedings of the Compact Stars in the QCD Phase Diagram III (CSQCD III), December 12-15, 2012, Guaruj\\'a, Brazil. http://www.astro.iag.usp.br/~foton/CSQCD3",
  "categories": [
    "astro-ph.HE",
    "astro-ph.SR",
    "hep-ph",
    "nucl-th"
  ],
  "abstract": "Baryonic matter in the core of a massive and evolved star is compressed significantly to form a supra-nuclear object, and compressed baryonic matter (CBM) is then produced after supernova. The state of cold matter at a few nuclear density is pedagogically reviewed, with significant attention paid to a possible quark-cluster state conjectured from an astrophysical point of view.",
  "revisions": [
    {
      "version": "v2",
      "updated": "2013-07-22T15:25:28.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "compressed baryonic matter",
      "astrophysics",
      "significant attention paid",
      "supra-nuclear object",
      "cold matter"
    ],
    "tags": [
      "conference paper"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 10,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 1228291,
      "adsabs": "2013arXiv1304.4007G"
    }
  }
}