{
  "annotation_id": "162db698-2793-4c31-a194-c26739c228da",
  "date_created": "2026-03-02T18:00:18.510000Z",
  "date_modified": "2026-03-02T18:00:18.510000Z",
  "file_hash": "959296ad9bef425c234e9556e85a432b996e759668e8b2902781f9bf275b7371",
  "private": false,
  "record": {
    "abstract": "Coulomb energy differences between mirror nuclei with $A \\le 70$ are\ncalculated within the framework of the nuclear shell model using an effective\nCoulomb plus isovector and isotensor interaction. Absolute binding energies for\nproton-rich nuclei are predicted by adding the calculated Coulomb shifts to\nexperimentally measured binding energies for the neutron-rich mirror. The\nlocation of the proton drip-line is investigated, as well as candidates for the\nexotic decay mode known as di-proton emission. Taking into account the\nlifetimes of competing decay modes and limits imposed by experimental setups,\nit is concluded that the best candidates for the observation of correlated\ndi-proton emission are $^{45}$Fe, $^{48}$Ni, and $^{63}$Se.",
    "arxiv_id": "nucl-th/9701002",
    "authors": [
      "W. E. Ormand"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1103/PhysRevC.55.2407",
    "journal_ref": "Phys.Rev.C55:2407-2417,1997",
    "title": "Mapping the proton drip-line up to A=70",
    "url": "https://arxiv.org/abs/nucl-th/9701002"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "bcd20c3f-2dc5-464e-88c3-38255d8f2e83",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}