{
  "annotation_id": "a7783c54-39b6-464c-8bdd-f8e2039f76d6",
  "date_created": "2026-03-02T18:00:11.141000Z",
  "date_modified": "2026-03-02T18:00:11.141000Z",
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  "record": {
    "abstract": "A hybrid equation of state for dense matter is presented that satisfies\nphenomenological constraints from modern compact star observations which\nindicate high maximum masses of about 2 M_sun and large radii of R\u003e 12 km. The\ncorresponding isospin symmetric equation of state is consistent with flow data\nanalyses of heavy-ion collisions. The transition from nuclear to two-flavor\ncolor superconducting quark matter at n approximately 0.55 fm^{-3} is almost a\ncrossover.",
    "arxiv_id": "nucl-th/0611078",
    "authors": [
      "T. Klahn"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1016/j.ppnp.2006.12.015",
    "journal_ref": "Prog.Part.Nucl.Phys.59:196-198,2007",
    "title": "Modern compact star observations and the quark matter EoS",
    "url": "https://arxiv.org/abs/nucl-th/0611078"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "8b958673-ea41-4f70-9755-6f4df043d9a0",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}