{
  "annotation_id": "d38a6ff5-0018-4bcc-bc5e-d438f70fe387",
  "date_created": "2026-03-02T18:00:28.040000Z",
  "date_modified": "2026-03-02T18:00:28.040000Z",
  "file_hash": "7282e8eb898a8f91387f85d444c2f6665793226993159dcd71d5a940dc241362",
  "private": false,
  "record": {
    "abstract": "Effects of the Dirac sea on the excitation energy of the giant monopole\nstates are investigated in an analytic way within the $\\sigma-\\omega$ model.\nThe excitation energy is determined by the relativistic Landau-Migdal\nparameters, $F_0$ and $F_1$. Their analytic expressions are derived in the\nrelativistic random phase approximation(RRPA) without the Dirac sea, with the\nPauli blocking terms and with the full Dirac sea. It is shown that in the RRPA\nbased on the mean field approximation the Pauli blocking terms should be\nincluded in the configuration space, according to the relativistic Landau\ntheory. In the renormalized RRPA, the incompressibility coefficient becomes\nnegative, if N$\\nbar$ excitations are neglected.",
    "arxiv_id": "nucl-th/9909042",
    "authors": [
      "Haruki Kurasawa",
      "Toshio Suzuki"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1016/S0370-2693(00)00046-0",
    "journal_ref": "Phys.Lett. B474 (2000) 262-268",
    "title": "Effects of the Dirac Sea on the Giant Monopole States",
    "url": "https://arxiv.org/abs/nucl-th/9909042"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "8ce1480d-16ee-4d17-99dc-c4163269c4bd",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}