{
  "annotation_id": "221cad32-3537-48f1-9ce5-6a8748c64c08",
  "date_created": "2026-03-02T18:00:18.470000Z",
  "date_modified": "2026-03-02T18:00:18.470000Z",
  "file_hash": "518a7efc5a95143272ff25eea9ac48d2cba2c65c76bea25438be4c05032343f1",
  "private": false,
  "record": {
    "abstract": "We have carried out a study of superheavy nuclei in the framework of the\nRelativistic Mean-Field theory. Relativistic Hartree-Bogoliubov (RHB)\ncalculations have been performed for nuclei with large proton and neutron\nnumbers. A finite-range pairing force of Gogny type has been used in the RHB\ncalculations. The ground-state properties of very heavy nuclei with atomic\nnumbers Z=100-114 and neutron numbers N=154-190 have been obtained. The results\nshow that in addition to N=184 the neutron numbers N=160 and N=166 exhibit an\nextra stability as compared to their neighbors. For the case of protons the\natomic number Z=106 is shown to demonstrate a closed-shell behavior in the\nregion of well deformed nuclei about N=160. The proton number Z=114 also\nindicates a shell closure. Indications for a doubly magic character at Z=106\nand N=160 are observed. Implications of shell closures on a possible synthesis\nof superheavy nuclei are discussed.",
    "arxiv_id": "nucl-th/9608005",
    "authors": [
      "G. A. Lalazissis",
      "M. M. Sharma",
      "P. Ring",
      "Y. K. Gambhir"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1016/0375-9474(96)00273-4",
    "journal_ref": "Nucl.Phys. A608 (1996) 202-226",
    "title": "Superheavy Nuclei in the Relativistic Mean Field Theory",
    "url": "https://arxiv.org/abs/nucl-th/9608005"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "bc925c7a-4239-45f0-9e73-c6487465df6a",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}