{
  "annotation_id": "b12fa380-3877-4e3d-bf65-a89131d36464",
  "date_created": "2026-03-02T18:00:15.352000Z",
  "date_modified": "2026-03-02T18:00:15.352000Z",
  "file_hash": "6f269fd385a89efbbe09f0d1552aa41425808ff8ae91a2c102a6fdbd8c975d3d",
  "private": false,
  "record": {
    "abstract": "Using the Color-Dielectric model to describe quark confinement, including\nstrange quarks and accounting for beta--equilibrium, we get masses for a static\nneutron star in the range $1.3\\leq M/M_{\\odot}\\leq 1.54 $ for a radius\n$R\\approx 9$ km. Rapid cooling through the direct URCA mechanism is obtained.\nThe implications for the composition of neutron stars is discussed.",
    "arxiv_id": "nucl-th/9505037",
    "authors": [
      "A. Drago",
      "U. Tambini",
      "M. Hjorth-Jensen"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1016/0370-2693(96)00479-0",
    "journal_ref": "Phys. Lett. B380 (1996) 13",
    "title": "Neutron Stars and Massive Quark Matter",
    "url": "https://arxiv.org/abs/nucl-th/9505037"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "05388837-5770-4408-874a-750a755ac860",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}