{
  "annotation_id": "6faf0754-78c4-4143-8a56-6f3e63c6c252",
  "date_created": "2026-03-02T18:00:08.017000Z",
  "date_modified": "2026-03-02T18:00:08.017000Z",
  "file_hash": "be496c66e957046744cbe55b9942d34b0e10554c8c1fc29073a925387ab09c14",
  "private": false,
  "record": {
    "abstract": "Ab inito calculations for the nuclear many-body problem make predictions for\nthe density and isospin dependence of the nuclear equation-of-state (EOS) far\naway from the saturation point of nuclear matter. I compare predictions from\nmicroscopic and phenomenological approaches. Constraints on the EOS derived\nfrom heavy ion reactions, in particular from subthreshold kaon production, as\nwell as constraints from neutron stars are discussed.",
    "arxiv_id": "nucl-th/0610038",
    "authors": [
      "Christian Fuchs"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1142/9789812770417_0025",
    "title": "The Nuclear Equation of State at high densities",
    "url": "https://arxiv.org/abs/nucl-th/0610038"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "77aa2b0d-290a-4a91-977d-d7f05fcf6043",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}