{
  "annotation_id": "06d033b6-fadd-4405-91d2-7fd698730514",
  "date_created": "2026-03-02T18:00:04.209000Z",
  "date_modified": "2026-03-02T18:00:04.209000Z",
  "file_hash": "56371e1c8b7807486dd938dc20668a1d15c139d0c62fdd1b6efa7f3cb3b5310a",
  "private": false,
  "record": {
    "abstract": "Nuclear mass data provide EMPIRICAL evidence of: 1. Clustering of nucleons;\n2. Attractive n-p interactions; and 3. Repulsive but symmetric n-n and p-p\ninteractions after correcting for the repulsive Coulomb interactions between\npositive nuclear charges. These findings suggest a possible source of energy in\nneutron stars, in stars which formed on them, and demonstrate the need for a\nTheoretical understanding of 1. Interactions between nucleons; 2. Clustering of\nnucleons; and 3. Neutron-emission by penetration of the gravitational barrier\nsurrounding a neutron star.",
    "arxiv_id": "nucl-th/0412073",
    "authors": [
      "O. Manuel"
    ],
    "categories": [
      "nucl-th"
    ],
    "title": "Nuclear Clustering and Interactions Between Nucleons",
    "url": "https://arxiv.org/abs/nucl-th/0412073"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "a21a3bf8-5b14-438e-b119-b77245b915b8",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}