{
  "annotation_id": "341c4afb-4e71-4736-a3ae-acce1e0bfe30",
  "date_created": "2026-03-02T18:00:12.033000Z",
  "date_modified": "2026-03-02T18:00:12.033000Z",
  "file_hash": "1c7179eb57f284c7e9dbecbf66529800c35b116455f8b1c960c6d57db43221d5",
  "private": false,
  "record": {
    "abstract": "A central issue in the theory of astrophysical compact objects and heavy ion\nreactions at intermediate and relativistic energies is the Nuclear Equation of\nState (EoS). On one hand, the large and expanding set of experimental and\nobservational data is expected to constrain the behaviour of the nuclear EoS,\nespecially at density above saturation, where it is directly linked to\nfundamental processes which can occur in dense matter. On the other hand,\ntheoretical predictions for the EoS at high density can be challenged by the\nphenomenological findings. In this topical review paper we present the\nmany-body theory of nuclear matter as developed along different years and with\ndifferent methods. Only nucleonic degrees of freedom are considered. We compare\nthe different methods at formal level, as well as the final EoS calculated\nwithin each one of the considered many-body schemes. The outcome of this\nanalysis should help in restricting the uncertainty of the theoretical\npredictions for the nuclear EoS.",
    "arxiv_id": "nucl-th/0703004",
    "authors": [
      "M. Baldo",
      "C. Maieron"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1088/0954-3899/34/5/R01",
    "journal_ref": "J.Phys.G34:R243,2007",
    "title": "Equation of State of Nuclear Matter at high baryon density",
    "url": "https://arxiv.org/abs/nucl-th/0703004"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "23377c23-a6ff-4b56-b413-2acd5149a09c",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}