{
  "annotation_id": "4c86529d-b273-4460-8d9d-bac92ff5ab9d",
  "date_created": "2026-03-02T18:00:12.046000Z",
  "date_modified": "2026-03-02T18:00:12.046000Z",
  "file_hash": "f2d2d9b2d76278c7fa0bde1cb91bfd49fd26970b8a1d6373b8cb75c6ebf08d1a",
  "private": false,
  "record": {
    "abstract": "Pauli-projected random gaussians are used as a representation to solve the\nshell model equations. The elements of the representation are chosen by a\nvariational procedure. This scheme is particularly suited to describe cluster\nformation and cluster decay in nuclei. It overcomes the basis-size problem of\nthe ordinary shell model and the technical difficulties of the\ncluster-configuration shell model. The model reproduces the $\\alpha$-decay\nwidth of $^{212}$Po satisfactorily.",
    "arxiv_id": "nucl-th/9403016",
    "authors": [
      "K. Varga",
      "R. J. Liotta"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1103/PhysRevC.50.R1292",
    "journal_ref": "Phys.Rev.C50:1292-1295,1994",
    "title": "Shell model on a random gaussian basis",
    "url": "https://arxiv.org/abs/nucl-th/9403016"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "a5c46499-b87c-45a6-8e61-fe8a3c6d2934",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}