{
  "annotation_id": "4902ca92-cde4-448d-bd28-6159b0387fa4",
  "date_created": "2026-03-02T18:00:00.610000Z",
  "date_modified": "2026-03-02T18:00:00.610000Z",
  "file_hash": "e6d212c6ca417c97389cd704c7a216401538a4130589ed5d12523eca55145a19",
  "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-Hartree-Fock\napproach. For the quark sector, we employ the MIT bag model, as well as the\nNambu--Jona-Lasinio (NJL) and the Color Dielectric (CD) models, and find that\nthe NS maximum masses lie in the interval between 1.5 and 1.8 solar masses.",
    "arxiv_id": "nucl-th/0410040",
    "authors": [
      "G. F. Burgio"
    ],
    "categories": [
      "nucl-th",
      "astro-ph",
      "hep-ph"
    ],
    "doi": "10.1016/j.nuclphysa.2004.12.064",
    "journal_ref": "Nucl.Phys. A749 (2005) 337-340",
    "title": "The hadron-quark phase transition in neutron stars",
    "url": "https://arxiv.org/abs/nucl-th/0410040"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "36af0e07-b11d-4db7-a3e7-11c626f25657",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}