{
  "annotation_id": "6addbd7b-201a-48d6-bc30-cc37edbb9ce7",
  "date_created": "2026-03-02T18:00:18.466000Z",
  "date_modified": "2026-03-02T18:00:18.466000Z",
  "file_hash": "e7af1e6f70b51a4ac2c086add7e44ae8f89e9afa65fe198da4d753e97b685da1",
  "private": false,
  "record": {
    "abstract": "The isospin dependence of the spin-orbit interaction in light neutron rich\nnuclei is investigated in the framework of relativistic mean field theory. The\nmagnitude of the spin-orbit potential is considerably reduced in drip line\nnuclei, resulting in smaller energy splittings between spin-orbit partners. The\neffect does not depend on the parametrization of the effective Lagrangian. The\nresults are compared with corresponding calculations in the non-relativistic\nSkyrme model.",
    "arxiv_id": "nucl-th/9709020",
    "authors": [
      "G. A. Lalazissis",
      "D. Vretenar",
      "W. Poeschl",
      "P. Ring"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1016/S0370-2693(97)01473-1",
    "journal_ref": "Phys.Lett. B418 (1998) 7-12",
    "title": "Reduction of the spin-orbit potential in light drip-line nuclei",
    "url": "https://arxiv.org/abs/nucl-th/9709020"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "828d097f-6d98-4c9e-af81-06a5e6441a6e",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}