{
  "annotation_id": "8a097ad7-30d2-492c-8ce6-851ac1ae565e",
  "date_created": "2026-03-02T18:00:08.194000Z",
  "date_modified": "2026-03-02T18:00:08.194000Z",
  "file_hash": "e6d34c1c430fb80dc3620885445701bfa9317a4fac94df6f68dec642287f30fc",
  "private": false,
  "record": {
    "abstract": "We investigate the composition and the equation of state of the kaon\ncondensed phase in neutrino-free and neutrino-trapped star matter within the\nframework of the Brueckner-Hartree-Fock approach with three-body forces. We\nfind that neutrino trapping shifts the onset density of kaon condensation to a\nlarger baryon density, and reduces considerably the kaon abundance. As a\nconsequence, when kaons are allowed, the equation of state of neutrino-trapped\nstar matter becomes stiffer than the one of neutrino free matter. The effects\nof different three-body forces are compared and discussed. Neutrino trapping\nturns out to weaken the role played by the symmetry energy in determining the\ncomposition of stellar matter, and thus reduces the difference between the\nresults obtained by using different three-body forces.",
    "arxiv_id": "nucl-th/0610037",
    "authors": [
      "A. Li",
      "G. F. Burgio",
      "U. Lombardo",
      "W. Zuo"
    ],
    "categories": [
      "nucl-th",
      "astro-ph"
    ],
    "doi": "10.1103/PhysRevC.74.055801",
    "journal_ref": "Phys.Rev.C74:055801,2006",
    "title": "Microscopic three-body forces and kaon condensation in cold   neutrino-trapped matter",
    "url": "https://arxiv.org/abs/nucl-th/0610037"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "6f94d6ae-517e-480f-bdb6-e7f0b8e46fbe",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}