{
  "annotation_id": "4b40d934-ae94-4176-933e-224b1bb06ba3",
  "date_created": "2026-03-02T18:00:19.114000Z",
  "date_modified": "2026-03-02T18:00:19.114000Z",
  "file_hash": "cde46a8776deeba49415026d2ac537e87cbdab57ab61cea2bf19c63c949c2c8b",
  "private": false,
  "record": {
    "abstract": "We demonstrate the feasibility of realistic Shell-Model Monte Carlo (SMMC)\ncalculations spanning multiple major shells, using a realistic interaction\nwhose bad saturation and shell properties have been corrected by a newly\ndeveloped general prescription. Particular attention is paid to the approximate\nrestoration of translational invariance. The model space consists of the full\nsd-pf shells. We include in the study some well-known T=0 nuclei and several\nunstable neutron-rich ones around N=20,28. The results indicate that SMMC can\nreproduce binding energies, B(E2) transitions, and other observables with an\ninteraction that is practically parameter free. Some interesting insight is\ngained on the nature of deep correlations. The validity of previous studies is\nconfirmed.",
    "arxiv_id": "nucl-th/9708039",
    "authors": [
      "D. J. Dean",
      "M. T. Ressell",
      "M. Hjorth-Jensen",
      "S. E. Koonin",
      "K. Langanke",
      "A. P. Zuker"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1103/PhysRevC.59.2474",
    "journal_ref": "Phys.Rev. C59 (1999) 2474-2486",
    "title": "Shell Model Monte Carlo studies of neutron-rich nuclei in the   1s-0d-1p-0f shells",
    "url": "https://arxiv.org/abs/nucl-th/9708039"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "b69cbf81-0dd6-4392-bbf4-40907c6fc548",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}