{
  "annotation_id": "c0e0acbb-ed52-437f-8f5d-cb886d3c1b4f",
  "date_created": "2026-03-02T18:00:07.758000Z",
  "date_modified": "2026-03-02T18:00:07.758000Z",
  "file_hash": "7e280261ae78f5b0d5381ce8cae0cf5dce77d26d3080743a37d8510cb2613deb",
  "private": false,
  "record": {
    "abstract": "Characteristics of the nuclear equation of state (EOS) and its importance, in\nparticular for astrophysics, are discussed. Selected observables in nuclear\ncollisions are sensitive to the EOS and can be used to constrain it. For\ncentral collisions, these include collective flow asymmetries, subthreshold\nkaon yields and isospin diffusion. Comparisons between the data and transport\ntheory suggest an energy per nucleon that rises relatively slowly with density\nfor symmetric matter and symmetry energy that rises relatively quickly around\nthe normal nuclear density.",
    "arxiv_id": "nucl-th/0512009",
    "authors": [
      "P. Danielewicz"
    ],
    "categories": [
      "nucl-th"
    ],
    "title": "Nuclear Equation of State: Picture from Medium Energy Heavy Ion   Collisions",
    "url": "https://arxiv.org/abs/nucl-th/0512009"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "a55f5a2b-714a-4b02-a1c3-0400b2acff6f",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}