{
  "annotation_id": "230eca4b-cc4e-43ce-9021-61e717876884",
  "date_created": "2026-03-02T18:00:25.832000Z",
  "date_modified": "2026-03-02T18:00:25.832000Z",
  "file_hash": "2a3693a1e0a69e0b47b8de3d219488e774bf65aa1515b08239f31863e4f5afd1",
  "private": false,
  "record": {
    "abstract": "We consider the Parity Nonconserving (PNC) mixing in the ground state of\nexotic (halo) nuclei caused by the PNC weak interaction between outer neutron\nand nucleons within nuclear interior. For the nucleus $^{11}Be$ as an example\nof typical nucleus with neutron halo, we use analytical model for the external\nneutron wave functions to estimate the scale of the PNC mixing. The amplitude\nof the PNC mixing in halo state is found to be an order of magnitude bigger\nthan that of typical PNC mixing between the ``normal\u0027\u0027 nuclear states in nearby\nnuclei. The enhanced PNC mixing in halo cloud is proportional to the neutron\nweak PNC potential constant $g^W_n$ only.",
    "arxiv_id": "nucl-th/9908047",
    "authors": [
      "M. S. Hussein",
      "A. F. R. de Toledo Piza",
      "O. K. Vorov",
      "A. K. Kerman"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1103/PhysRevC.60.064615",
    "journal_ref": "Phys.Rev. C60 (1999) 064615",
    "title": "Enhancement of parity violating mixing in halo nuclei and the problem of   neutron weak parity nonconserving potential constant",
    "url": "https://arxiv.org/abs/nucl-th/9908047"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "6b36cef4-652e-4531-bac1-a21c46343e48",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}