{
  "annotation_id": "844663c2-de62-496e-b9ea-ad1d2509cedc",
  "date_created": "2026-03-02T18:00:18.795000Z",
  "date_modified": "2026-03-02T18:00:18.795000Z",
  "file_hash": "a66e9c5ab76fc37a3d98e1e2d1652bf3bf8cb9422a730e5167ff8be5a7553fe9",
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  "record": {
    "abstract": "The modern nucleon-nucleon interaction of Myers and Swiatecki, adjusted to\nthe properties of finite nuclei, the parameters of the mass formula, and the\nbehavior of the optical potential is used to calculate the properties of\n$\\beta$--equilibrated neutron star matter, and to study the impact of this\nequation of state on the properties of (rapidly rotating) neutron stars and\ntheir cooling behavior. The results are in excellent agreement with the outcome\nof calculations performed for a broad collection of sophisticated\nnonrelativistic as well as relativistic models for the equation of state.",
    "arxiv_id": "nucl-th/9705043",
    "authors": [
      "Klaus Strobel",
      "Fridolin Weber",
      "Manfred K. Weigel",
      "Christoph Schaab"
    ],
    "categories": [
      "nucl-th",
      "astro-ph"
    ],
    "doi": "10.1142/S0218301397000329",
    "journal_ref": "Int.J.Mod.Phys. E6 (1997) 669-692",
    "title": "Neutron star properties in the Thomas-Fermi model",
    "url": "https://arxiv.org/abs/nucl-th/9705043"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "5ecc49e7-919c-403e-845d-de5b7ba37586",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}