{
  "annotation_id": "96b3c61e-6718-4487-8344-a12ccc5efcdd",
  "date_created": "2026-03-02T18:00:24.587000Z",
  "date_modified": "2026-03-02T18:00:24.587000Z",
  "file_hash": "227b4c93f485922d85eb90d3ffcef5f6e719b3d7ead8fe7e79ecc5e279c0ff6f",
  "private": false,
  "record": {
    "abstract": "We investigate the effect of neutrino trapping on kaon condensation process\nand Equation of State (EOS) in a newly formed neutron star which is less than\nseveral seconds old. Using nonlinear relativistic mean field model, we find\nthat the presence of neutrino shifts the threshold for kaon condensation and\nmuon production to much higher density. We also studied the energy density and\npressure of the syst under trapped neutrino condition and found that it\nstiffens the EOS of the system which may be responsible for the delayed\nexploision mechanism of supernovae.",
    "arxiv_id": "nucl-th/9812058",
    "authors": [
      "R. Dutta"
    ],
    "categories": [
      "nucl-th"
    ],
    "title": "The role of trapped neutrino in dense stelllar matter and kaon   condensation",
    "url": "https://arxiv.org/abs/nucl-th/9812058"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "dbdb8c32-be64-4dc0-9d16-a11e3b1ef2be",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}