{
  "annotation_id": "a737e003-43a4-4de2-afec-d11721880430",
  "date_created": "2026-03-02T18:00:29.429000Z",
  "date_modified": "2026-03-02T18:00:29.429000Z",
  "file_hash": "1767901a2084f90a3270119e9a2ee24d392675ee1b06246de06e2f3e93bf4129",
  "private": false,
  "record": {
    "abstract": "The effective field theory of NN interactions in nuclear matter is\nconsidered. Due to the Pauli principle the effective NN amplitude is not\naffected by the shallow bound states. We show that the next-to-leading order\nterms in the chiral expansion of the effective NN potential can be interpreted\nas corrections so the expansion is systematic. The value of potential energy\nper particle is calculated and some issues concerning the chiral effective\ntheory of nuclear matter are outlined.",
    "arxiv_id": "nucl-th/9910072",
    "authors": [
      "B. Krippa"
    ],
    "categories": [
      "nucl-th",
      "hep-ph"
    ],
    "title": "Chiral NN interaction in nuclear matter",
    "url": "https://arxiv.org/abs/nucl-th/9910072"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "c1c66a50-5179-4f99-8640-b1081bd7c3e4",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}