{
  "annotation_id": "aaf0e263-6532-4546-b70d-02edd1534a3b",
  "date_created": "2026-03-02T18:00:21.651000Z",
  "date_modified": "2026-03-02T18:00:21.651000Z",
  "file_hash": "d144a446001a640480879773fe3e5a22fd41a6a00e06c53f818986f74db0862b",
  "private": false,
  "record": {
    "abstract": "We explore the consequences of an equation of state (EOS) obtained in a\nconfining Dyson-Schwinger equation model of QCD for the structure and stability\nof nonstrange quark stars at finite-T, and compare the results with those\nobtained using a bag-model EOS. Both models support a temperature profile that\nvaries over the star\u0027s volume and the consequences of this are model\nindependent. However, in our model the analogue of the bag pressure is\n(T,mu)-dependent, which is not the case in the bag model. This is a significant\nqualitative difference and comparing the results effects a primary goal of\nelucidating the sensitivity of quark star properties to the form of the EOS.",
    "arxiv_id": "nucl-th/9801060",
    "authors": [
      "D. Blaschke",
      "H. Grigorian",
      "G. Poghosyan",
      "C. D. Roberts",
      "S. Schmidt"
    ],
    "categories": [
      "nucl-th",
      "astro-ph",
      "hep-ph"
    ],
    "doi": "10.1016/S0370-2693(99)00007-6",
    "journal_ref": "Phys.Lett.B450:207-214,1999",
    "title": "A dynamical, confining model and hot quark stars",
    "url": "https://arxiv.org/abs/nucl-th/9801060"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "1b661ebc-0dd7-4349-a7f4-df9043038c13",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}