{
  "annotation_id": "c094a2a7-e525-4f8c-ac0a-ec731706e201",
  "date_created": "2026-03-02T18:00:25.533000Z",
  "date_modified": "2026-03-02T18:00:25.533000Z",
  "file_hash": "782d9bb12108c8c1ff02896a05ad0115dc586fe9a5e91faec549d3f97e5818bd",
  "private": false,
  "record": {
    "abstract": "Allowed weak interaction rates for sd-shell nuclei in stellar environment are\ncalculated using a generalized form of proton-neutron quasiparticle RPA model\nwith separable Gamow-Teller forces. Twelve different weak rates are calculated\nfor each nucleus as a function of temperature and density. This project\nconsists of calculation of weak rates for a total of 709 nuclei with masses\nranging from A = 18 to 100. This paper contains calculated weak rates for\nsd-shell nuclei. The calculated capture and decay rates take into consideration\nthe latest experimental energy levels and ft value compilations. The results\nare also compared with earlier works. Particle emission processes from excited\nstates, previously ignored, are taken into account, and are found to\nsignificantly affect some beta decay rates.",
    "arxiv_id": "nucl-th/9907106",
    "authors": [
      "J. -U. Nabi",
      "H. V. Klapdor-Kleingrothaus"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1006/adnd.1998.0801",
    "journal_ref": "Atom.Data Nucl.Data Tabl. 71 (1999) 149-345",
    "title": "Weak Interaction Rates Of sd-Shell Nuclei In Stellar Environment   Calculated in the Proton-Neutron Quasiparticle Random Phase Approximation",
    "url": "https://arxiv.org/abs/nucl-th/9907106"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "41c9c48e-aa67-43e2-a53c-de2a067c50fb",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}