{
  "annotation_id": "d6e8a78e-6d00-4a10-a54a-02574a1ed0da",
  "date_created": "2026-03-02T18:00:12.043000Z",
  "date_modified": "2026-03-02T18:00:12.043000Z",
  "file_hash": "12745fc90c0f2acd7b531b05aaa9f420d25e1d3b406993b1d9aed3d11b023e27",
  "private": false,
  "record": {
    "abstract": "We use the modified quark-meson coupling and the quantum hadrodynamics models\nto study the properties of neutron star. Coupling constants of both models are\nadjusted to reproduce the same saturation properties. The onset of kaon\ncondensation in neutron star matter is studied in detail over a wide range of\nkaon optical potential values. Once the kaon condensation takes place, the\npopulation of kaons increases very rapidly, and kaons become the dominant\ncomponent, possibly making the neutron star matter a kaonic matter if the kaon\noptical potential is large.",
    "arxiv_id": "nucl-th/0702028",
    "authors": [
      "S. W. Hong",
      "C. H. Hyun",
      "C. Y. Ryu"
    ],
    "categories": [
      "nucl-th"
    ],
    "title": "Kaon condensation in neutron star using relativistic mean field models",
    "url": "https://arxiv.org/abs/nucl-th/0702028"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "50b00585-e497-43d4-b7b0-d4db022a3c9b",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}