{
  "annotation_id": "24b12f38-08ed-4414-95f1-b45d02d1045e",
  "date_created": "2026-03-02T18:00:08.640000Z",
  "date_modified": "2026-03-02T18:00:08.640000Z",
  "file_hash": "afcc107516c514aac7f44f336007e9dbb5d9f06a0c17ea7d790d64627f148d3e",
  "private": false,
  "record": {
    "abstract": "By constructing an Ising analogue of compact-star matter at sub-saturation\ndensity we explored the effect of Coulomb frustration on the nuclear liquid-gas\nphase transition. Our conclusions is twofold. First, the range of temperatures\nwhere inhomogeneous phases form expands with increasing Coulomb-field strength.\nSecond, within the approximation of uniform electron distribution, the limiting\npoint upon which the phase-coexistence region ends does not exhibit any\ncritical behaviour. Possible astrophysics consequences and thermodynamical\nconnections are discussed.",
    "arxiv_id": "nucl-th/0609063",
    "authors": [
      "P. Napolitani",
      "Ph. Chomaz",
      "F. Gulminelli",
      "K. H. O. Hasnaoui"
    ],
    "categories": [
      "nucl-th",
      "cond-mat.stat-mech"
    ],
    "doi": "10.1103/PhysRevLett.98.131102",
    "journal_ref": "Phys.Rev.Lett.98:131102,2007",
    "title": "Ising analogue to compact-star matter",
    "url": "https://arxiv.org/abs/nucl-th/0609063"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "de238fe8-a6b1-4806-b202-b1d43551755f",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}