{
  "annotation_id": "c65e4344-e124-4927-a031-a794c33ae483",
  "date_created": "2026-03-02T18:00:01.367000Z",
  "date_modified": "2026-03-02T18:00:01.367000Z",
  "file_hash": "d2561107396e3a7fe6b03935d6eebb57637e222568876cfcb4e17ff3edc71e68",
  "private": false,
  "record": {
    "abstract": "We show that if color superconducting quark matter forms in hybrid or quark\nstars it is possible to satisfy most of recent observational boundaries on\nmasses and radii of compact stellar objects. An energy of the order of\n$10^{53}$ erg is released in the conversion from a (metastable) hadronic star\ninto a (stable) hybrid or quark star in presence of a color superconducting\nphase. If the conversion occurs immediately after the deleptonization of the\nproto-neutron star, the released energy can help Supernovae to explode. If the\nconversion is delayed the energy released can power a Gamma Ray Burst. A delay\nbetween the Supernova and the subsequent Gamma Ray Burst is possible, in\nagreement with the delay proposed in recent analysis of astrophysical data.",
    "arxiv_id": "nucl-th/0401052",
    "authors": [
      "A. Drago",
      "A. Lavagno",
      "G. Pagliara"
    ],
    "categories": [
      "nucl-th",
      "astro-ph",
      "hep-ph"
    ],
    "doi": "10.1103/PhysRevD.69.057505",
    "journal_ref": "Phys.Rev. D69 (2004) 057505",
    "title": "Effects of color superconductivity on the structure and formation of   compact stars",
    "url": "https://arxiv.org/abs/nucl-th/0401052"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "05f62fc8-54ba-47cd-8fc6-0da3b2681ad1",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}