{
  "annotation_id": "897690fc-1bf3-4c91-8e11-5a6e5542c611",
  "date_created": "2026-03-02T17:59:57.646000Z",
  "date_modified": "2026-03-02T17:59:57.646000Z",
  "file_hash": "a2a75b6743f16e808a0edc31efdd8ff77ad26470ef7f99c70f9bd154b36c9b86",
  "private": false,
  "record": {
    "abstract": "We study the effects of color superconductivity on the structure and\nformation of compact stars. We show that it is possible to satisfy most of\nrecent observational boundaries on masses and radii if a diquark condensate\nforms in a hybrid or a quark star. Moreover, we find that a huge amount of\nenergy, of the order of $10^{53}$ erg, can be released in the conversion from a\n(metastable) hadronic star into a (stable) hybrid or quark star, if the\npresence of a color superconducting phase is taken into account. Accordingly to\nthe scenario proposed in Astrophys.J.586(2003)1250, the energy released in this\nconversion can power a Gamma Ray Burst. This mechanism can explain the recent\nobservations indicating a delay, of the order of days or years, between a few\nSupernova explosions and the subsequent Gamma Ray Burst.",
    "arxiv_id": "nucl-th/0304026",
    "authors": [
      "A. Drago",
      "A. Lavagno",
      "G. Pagliara"
    ],
    "categories": [
      "nucl-th",
      "astro-ph",
      "hep-ph"
    ],
    "doi": "10.1063/1.1810878",
    "title": "Color Superconductivity in Compact Stars and Gamma Ray Bursts",
    "url": "https://arxiv.org/abs/nucl-th/0304026"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "0211eea9-1b24-4d3c-9d76-53b1793e53e0",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}