{
  "annotation_id": "82ebf5ad-7362-4f06-8731-499d9488d4b2",
  "date_created": "2026-03-02T18:00:18.455000Z",
  "date_modified": "2026-03-02T18:00:18.455000Z",
  "file_hash": "1658fc95bfc276b0e223a5fd82abfe7daadc230a811b1f02becaedeb42b6ec6f",
  "private": false,
  "record": {
    "abstract": "We discuss the equation of state of neutron stars in the dense interior\nconsidering hyperons and the possible onset of kaon condensation within the\nrelativistic mean field model. We find that hyperons are favoured in dense\nmatter and that their appearance make the existence of a kaon condensed phase\nquite unlikely. Implications for the recent measurements of kaons in heavy ion\ncollisions at subthreshold energy are also given.",
    "arxiv_id": "nucl-th/9607019",
    "authors": [
      "J. Schaffner",
      "J. Bondorf",
      "I. N. Mishustin"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1007/BF03155624",
    "journal_ref": "Heavy Ion Phys.4:293-300,1996",
    "title": "Hyperon-rich Matter and Kaons in Matter",
    "url": "https://arxiv.org/abs/nucl-th/9607019"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "ad500808-3756-4d57-9a0e-3df7771f0e25",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}