{
  "annotation_id": "a900483b-b622-48b4-b14a-cd08b9f570be",
  "date_created": "2026-03-02T18:00:25.366000Z",
  "date_modified": "2026-03-02T18:00:25.366000Z",
  "file_hash": "7dea53b833a0fc5eeb3643f983443ac51258199468992258148e9a986fe3b0c0",
  "private": false,
  "record": {
    "abstract": "We investigate the thermal kaon process,in which kaons are thermally produced\nvia nucleon-nucleon collisions.This process is relevant to nonequilibrium\ndynamics of kaon condensation inside neutron stars.The reaction rates for these\nprocesses are calculated, and their temperature and density dependences are\ncompared with those of other reaction rates.It is shown that the thermal kaon\nprocess is dominant over other relevant weak reactions throughout the\nnonequilibrium process, such as the kaon-induced Urca and the modified Urca\nreactions, and may control the entire evolution of the kaon condensate. The\ncharacteristic role of the soft and hard kaons during the evolution is\nexplained, and implications for astrophysical phenomena are briefly discussed.",
    "arxiv_id": "nucl-th/9906024",
    "authors": [
      "Takumi Muto",
      "Toshitaka Tatsumi",
      "Naoki Iwamoto"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1103/PhysRevD.61.063001",
    "journal_ref": "Phys.Rev. D61 (2000) 063001",
    "title": "Nonequilibrium Weak Processes in Kaon Condensation I --- Reaction rate   for the thermal kaon process ---",
    "url": "https://arxiv.org/abs/nucl-th/9906024"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "007607b8-702c-450e-8607-60c7513386c6",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}