{
  "annotation_id": "caec9d98-032e-4525-b1d3-d43b57434ca8",
  "date_created": "2026-03-02T18:00:04.212000Z",
  "date_modified": "2026-03-02T18:00:04.212000Z",
  "file_hash": "af2bf63c9918886653b54126ed972eab14c0ce0c67bbca2d1ce651ec807952b9",
  "private": false,
  "record": {
    "abstract": "The rotational band built on the high-K multi-quasiparticle state can be\ninterpreted as a multi-phonon band of the precession mode, which represents the\nprecessional rotation about the axis perpendicular to the direction of the\nintrinsic angular momentum. By using the axially symmetric limit of the\nrandom-phase-approximation (RPA) formalism developed for the nuclear wobbling\nmotion, we study the properties of the precession modes in $^{178}$W; the\nexcitation energies, B(E2) and B(M1) values. We show that the excitations of\nsuch a specific type of rotation can be well described by the RPA formalism,\nwhich gives a new insight to understand the wobbling motion in the triaxial\nsuperdeformed nuclei from a microscopic view point.",
    "arxiv_id": "nucl-th/0412074",
    "authors": [
      "Yoshifumi R. Shimizu",
      "Masayuki Matsuzaki",
      "Kenichi Matsuyanagi"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1103/PhysRevC.72.014306",
    "journal_ref": "Phys.Rev. C72 (2005) 014306",
    "title": "High-K Precession modes: Axially symmetric limit of wobbling motion",
    "url": "https://arxiv.org/abs/nucl-th/0412074"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "421e8735-a52f-4b52-b44c-2d2dc2ab585d",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}