{
  "annotation_id": "2797b8db-b331-4ff3-b96a-5cf229f69ea0",
  "date_created": "2026-03-02T18:00:18.342000Z",
  "date_modified": "2026-03-02T18:00:18.342000Z",
  "file_hash": "5f846e14a6eead4d02a6665b526abfb7b0df54e23fa7fbc0b8bedab2a7a6773f",
  "private": false,
  "record": {
    "abstract": "For a $Q \\cdot Q$ interaction the energy weighted sum rule for isovector\norbital magnetic dipole transitions is proportional to the difference $\\sum\nB(E2, isoscalar) - \\sum B(E2, isovector)$, not just to $\\sum B(E2, physical)$.\nThis fact is important in ensuring that one gets the correct limit as one goes\nto nuclei, some of which are far from stability, for which one shell (neutron\nor proton) is closed. In $0p$ shell calculations for the even-even Be isotopes\nit is shown that the Fermion SU(3) model and Boson SU(3) model give different\nresults for the energy weighted scissors mode strengths.",
    "arxiv_id": "nucl-th/9702017",
    "authors": [
      "Y. Y. Sharon",
      "L. Zamick",
      "M. S. Fayache",
      "G. Rosensteel"
    ],
    "categories": [
      "nucl-th"
    ],
    "title": "Comparison of Fermion SU(3) and Boson SU(3) models for scissors mode   excitations",
    "url": "https://arxiv.org/abs/nucl-th/9702017"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "604ce2b6-7f7f-4ba2-bd2f-c5dab715e050",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}