{
  "annotation_id": "938e284e-527c-4298-8b7a-265e03ed8e35",
  "date_created": "2026-03-02T18:00:29.351000Z",
  "date_modified": "2026-03-02T18:00:29.351000Z",
  "file_hash": "767cb85652c51b12974d8246d7789cf42058c83b3518a19fd1a49261065a815f",
  "private": false,
  "record": {
    "abstract": "Nuclei with large neutron-to-proton ratios have neutron skins, which manifest\nthemselves in an excess of neutrons at distances greater than the radius of the\nproton distribution. In addition, some drip-line nuclei develop very extended\nhalo structures. The neutron halo is a threshold effect; it appears when the\nvalence neutrons occupy weakly bound orbits. In this study, nuclear skins and\nhalos are analyzed within the self-consistent Skyrme-Hartree-Fock-Bogoliubov\nand relativistic Hartree-Bogoliubov theories for spherical shapes. It is\ndemonstrated that skins, halos, and surface thickness can be analyzed in a\nmodel-independent way in terms of nucleonic density form factors. Such an\nanalysis allows for defining a quantitative measure of the halo size. The\nsystematic behavior of skins, halos, and surface thickness in even-even nuclei\nis discussed.",
    "arxiv_id": "nucl-th/9911062",
    "authors": [
      "S. Mizutori",
      "J. Dobaczewski",
      "G. A. Lalazissis",
      "W. Nazarewicz",
      "P. -G. Reinhard"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1103/PhysRevC.61.044326",
    "journal_ref": "Phys.Rev. C61 (2000) 044326",
    "title": "Nuclear Skins and Halos in the Mean-Field Theory",
    "url": "https://arxiv.org/abs/nucl-th/9911062"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "1a83a8b5-fc8e-4bd4-924c-d5e34267e386",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}