{
  "annotation_id": "442f795a-179a-431c-8bf5-c3fc9d3ba368",
  "date_created": "2026-03-02T18:00:07.891000Z",
  "date_modified": "2026-03-02T18:00:07.891000Z",
  "file_hash": "51eb26405461218bd5b2a77c58e1efe5cb3abdf6e25331e7d13bba0515b649be",
  "private": false,
  "record": {
    "abstract": "The spin-orbit (SO) interaction, emerging naturally from the Relativistic\nMean Field (RMF) theory is examined critically in the light of the recently\nmeasured excitation energy differences between the terminating states built on\ntwo different configurations for nuclei belonging to the lower pf shell. The\ncalculations are carried out using the cranked RMF framework. To further probe\nthe iso-vector dependence of the spin-orbit potential, the energy spacing\nbetween the g_{7/2} and h_{11/2} states in the Sb-chain is compared to\nexperiment. It is found that the calculation at the quantitative level deviates\nstrongly from the experiment. In particular the balance of the iso-scalar and\niso-vector strengths of the effective one body SO potential indicates that\nadditional terms like tensor couplings may be needed to account for the\nexperimental data.",
    "arxiv_id": "nucl-th/0605009",
    "authors": [
      "A. Bhagwat",
      "R. Wyss",
      "W. Satula",
      "J. Meng",
      "Y. K. Gambhir"
    ],
    "categories": [
      "nucl-th"
    ],
    "title": "Critical Survey of Isoscalar and Isovector Contributions to the Spin   Orbit Potential in Relativistic Mean Field Theory",
    "url": "https://arxiv.org/abs/nucl-th/0605009"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "fa555657-63c1-430c-9361-e6f5c0d2e287",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}