{
  "annotation_id": "081e0e5a-5162-4b1d-937e-e8222f7e8375",
  "date_created": "2026-03-02T18:00:07.624000Z",
  "date_modified": "2026-03-02T18:00:07.624000Z",
  "file_hash": "de959a4dd5483b13b00714727edcdab653c4188e9904409e6dd19d2d328e582c",
  "private": false,
  "record": {
    "abstract": "We review our recent works about ``pasta\u0027\u0027 structures following the\nfirst-order phase transition in dense matter, which correspond to the\nstructured mixed phases with geometrical symmetries. Three kinds of phase\ntransitions at different density ranges are examined as the stages of pasta\nstructures: liquid-gas phase transition at subnuclear density, kaon\ncondensation and hadron-quark phase transition at high density. Charge density\nas well as particle density is non-uniform there. A consistent treatment of the\nCoulomb potential and the particle densities is presented and a peculiar role\nof the Coulomb potential is elucidated: the physical picture of the Maxwell\nconstruction will be effectively recovered. It largely influences the density\nregime of pasta structures by the charge screening effect.",
    "arxiv_id": "nucl-th/0605075",
    "authors": [
      "Toshiki Maruyama",
      "Toshitaka Tatsumi",
      "Tomoki Endo",
      "Satoshi Chiba"
    ],
    "categories": [
      "nucl-th"
    ],
    "journal_ref": "RecentRes.Devel.Phys.7:1-57,2006",
    "title": "Pasta structures in compact stars",
    "url": "https://arxiv.org/abs/nucl-th/0605075"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "fee8cf69-e06e-4904-b296-94d9c31bc51f",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}