{
  "annotation_id": "c240358f-d330-441a-86e2-650a2842a1b6",
  "date_created": "2026-03-02T18:00:18.945000Z",
  "date_modified": "2026-03-02T18:00:18.945000Z",
  "file_hash": "fc693c4d46a512d1671113eb7ca34fa36c2517c8f1d953f3f71ab6a2e882e2af",
  "private": false,
  "record": {
    "abstract": "The shell structure of superheavy nuclei is investigated within various\nparametrizations of relativistic and nonrelativistic nuclear mean field models.\nThe heaviest known even-even nucleus 264Hs is used as a benchmark to estimate\nthe predictive value of the models. From that starting point, doubly magic\nspherical nuclei are searched in the region Z=110-140 and N=134-298. They are\nfound at (Z=114, N=184), (Z=120, N=172), or at (Z=126, N=184), depending on the\nparametrization.",
    "arxiv_id": "nucl-th/9610032",
    "authors": [
      "K. Rutz",
      "M. Bender",
      "T. Buervenich",
      "T. Schilling",
      "P. -G. Reinhard",
      "J. A. Maruhn",
      "W. Greiner"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1103/PhysRevC.56.238",
    "journal_ref": "Phys.Rev.C56:238-243,1997",
    "title": "Superheavy nuclei in selfconsistent nuclear calculations",
    "url": "https://arxiv.org/abs/nucl-th/9610032"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "0715226b-b981-4d2b-972c-c353c031d352",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}