{
  "annotation_id": "39560919-39f1-47c0-8458-bcdca87c538f",
  "date_created": "2026-03-02T18:00:10.822000Z",
  "date_modified": "2026-03-02T18:00:10.822000Z",
  "file_hash": "6f9c5eb624e4f5282d4a05ba1f4d33146dc2df2700137f6e7abdaf9c02d13ae3",
  "private": false,
  "record": {
    "abstract": "We investigate the phase transition to a deconfined phase and the\nconsequences in the formation of neutron stars. We use the recently proposed\neffective field theory motivated relativistic mean field theory for hadron and\nthe MIT Bag model and color-flavor locked (CFL) phase for the quark matter in\norder to get the appropriate equation of state. The properties of star are then\ncalculated. The differences between unpaired and CFL quark matter are\ndiscussed.",
    "arxiv_id": "nucl-th/0611039",
    "authors": [
      "B. K. Sharma",
      "P. K. Panda",
      "S. K. Patra"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1103/PhysRevC.75.035808",
    "journal_ref": "Phys.Rev.C75:035808,2007",
    "title": "Phase transition and properties of compact star",
    "url": "https://arxiv.org/abs/nucl-th/0611039"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "cb18e2db-07ee-48d9-a207-c7a82269e653",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}