{
  "annotation_id": "0c8756f7-b79c-4c9b-9b9d-2c5af328c67b",
  "date_created": "2026-03-02T18:00:04.575000Z",
  "date_modified": "2026-03-02T18:00:04.575000Z",
  "file_hash": "b733a82b97aaf5fa4e530875e9c465db2bcf353a02b547dd5a68a0b544e144cd",
  "private": false,
  "record": {
    "abstract": "Nilsson parameters kappa and mu have been studied in the framework of the\nrelativistic mean field (RMF) models. They are used to investigate the reason\nthat the RMF models give a relatively well prediction of the spin-orbit\nsplitting, but fail to reproduce the placement of the states with different\norbital angular momenta. Instead of the relatively small effective mass M*, the\nindependence of M* from the angular momentum l is found to be the reason.",
    "arxiv_id": "nucl-th/0502014",
    "authors": [
      "A. Sulaksono",
      "T. Mart",
      "C. Bahri"
    ],
    "categories": [
      "nucl-th",
      "hep-ph"
    ],
    "doi": "10.1103/PhysRevC.71.034312",
    "journal_ref": "Phys.Rev. C71 (2005) 034312",
    "title": "Nilsson parameters kappa and mu in the relativistic mean field models",
    "url": "https://arxiv.org/abs/nucl-th/0502014"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "996f86e2-427e-4300-999c-73ef11f2bd11",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}