{
  "annotation_id": "9779c70a-8e86-41d8-8a96-18d34298e5da",
  "date_created": "2026-03-02T18:00:14.165000Z",
  "date_modified": "2026-03-02T18:00:14.165000Z",
  "file_hash": "3710e0c11016449b92cb5dae50cea421d362fe36392d4663043687f86c28bc80",
  "private": false,
  "record": {
    "abstract": "A simple method for calculating the asymptotic $D$ state observables for\nlight nuclei is suggested. The method exploits the dominant clusters of the\nlight nuclei. The method is applied to calculate the $^4He$ asymptotic $D$ to\n$S$ normalization ratio $\\rho^\\alpha$ and the closely related $D$ state\nparameter $D_2^\\alpha$. The study predicts a correlation between $D_2^\\alpha$\nand $B_\\alpha$, and between $\\rho^\\alpha$ and $B_\\alpha$, where $B_\\alpha$ is\nthe binding energy of $^4He$. The present study yields $\\rho^\\alpha \\simeq\n-0.14$ and $D_2^\\alpha \\simeq -0.12$ fm$^2$ consistent with the correct\nexperimental $\\eta^D$ and the binding energies of the deuteron, triton, and the\n$\\alpha$ particle, where $\\eta^d$ is the deuteron $D$ state to $S$ state\nnormalization ratio.",
    "arxiv_id": "nucl-th/9405019",
    "authors": [
      "Sadhan K. Adhikari",
      "T. Frederico",
      "I. D. Goldman",
      "S. S. Sharma"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1103/PhysRevC.50.822",
    "journal_ref": "Phys.Rev.C50:822-830,1994",
    "title": "Model for asymptotic $D$-state parameters of light nuclei: Application   to $^4He$",
    "url": "https://arxiv.org/abs/nucl-th/9405019"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "28b6aa83-3172-48b0-8f6f-3107fe17dd4d",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}