{
  "annotation_id": "5013fb73-29b3-4069-a305-5d8ca20354a1",
  "date_created": "2026-03-02T18:00:01.137000Z",
  "date_modified": "2026-03-02T18:00:01.137000Z",
  "file_hash": "2f76c0bcda86c70ca92b4d713c4d38733ecdfdc05c2bb44f0968aacfcce7d5d3",
  "private": false,
  "record": {
    "abstract": "We study the hadron-quark phase transition in the interior of neutron stars\n(NS). For the hadronic sector, we use a microscopic equation of state (EOS)\ninvolving nucleons and hyperons derived within the Brueckner-Bethe-Goldstone\nmany-body theory, with realistic two-body and three-body forces. For the\ndescription of quark matter, we employ both the MIT bag model with a density\ndependent bag constant, and the color dielectric model. We calculate the\nstructure of NS interiors with the EOS comprising both phases, and we find that\nthe NS maximum masses are never larger than 1.7 solar masses, no matter the\nmodel chosen for describing the pure quark phase.",
    "arxiv_id": "nucl-th/0404089",
    "authors": [
      "C. Maieron",
      "M. Baldo",
      "G. F. Burgio",
      "H. -J. Schulze"
    ],
    "categories": [
      "nucl-th",
      "astro-ph",
      "hep-ph"
    ],
    "doi": "10.1103/PhysRevD.70.043010",
    "journal_ref": "Phys.Rev. D70 (2004) 043010",
    "title": "Hybrid stars with the color dielectric and the MIT bag models",
    "url": "https://arxiv.org/abs/nucl-th/0404089"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "464296c5-3939-4f93-afab-049376335da4",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}