{
  "id": "nucl-th/0508062",
  "version": "v3",
  "published": "2005-08-29T13:06:41.000Z",
  "updated": "2005-11-14T23:50:08.000Z",
  "title": "Quark Matter 2005 -- Theoretical Summary",
  "authors": [
    "Berndt Müller"
  ],
  "comment": "Final version containing multiple modifications in response to comments received on the draft version",
  "categories": [
    "nucl-th",
    "hep-ph"
  ],
  "abstract": "This is a review of the latest developments in the theory of superdense nuclear matter, formed in relativistic heavy ion collisions or in the core of collapsed stars, as they were reported and discussed at the Quark Matter 2005 conference in Budapest (Hungary).",
  "revisions": [
    {
      "version": "v3",
      "updated": "2005-11-14T23:50:08.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "quark matter",
      "theoretical summary",
      "relativistic heavy ion collisions",
      "superdense nuclear matter",
      "latest developments"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 690982,
      "adsabs": "2005nucl.th...8062M"
    }
  }
}