{
  "annotation_id": "2abfdfdd-65fc-4997-91e4-2214023bc70d",
  "date_created": "2026-03-02T18:00:22.407000Z",
  "date_modified": "2026-03-02T18:00:22.407000Z",
  "file_hash": "556cf6076321ca047f5ea8a294178970396f0b37044c39231a721d281ed7341e",
  "private": false,
  "record": {
    "abstract": "The properties of hot matter are studied in the frame of the relativistic\nBrueckner-Hartree-Fock theory. The equations are solved self-consistently in\nthe full Dirac space. For the interaction we used the potentials given by\nBrockmann and Machleidt. The obtained critical temperatures are smaller than in\nmost of the nonrelativistic investigations. We also calculated the\nthermodynamic properties of hot matter in the relativistic Hartree--Fock\napproximation, where the force parameters were adjusted to the outcome of the\nrelativistic Brueckner--Hartree--Fock calculations at zero temperature. Here,\none obtains higher critical temperatures, which are comparable with other\nrelativistic calculations in the Hartree scheme.",
    "arxiv_id": "nucl-th/9803026",
    "authors": [
      "H. Huber",
      "F. Weber",
      "M. K. Weigel"
    ],
    "categories": [
      "nucl-th",
      "astro-ph"
    ],
    "doi": "10.1103/PhysRevC.57.3484",
    "journal_ref": "Phys.Rev.C57:3484-3487,1998",
    "title": "Symmetric and asymmetric nuclear matter in the relativistic approach at   finite temperatures",
    "url": "https://arxiv.org/abs/nucl-th/9803026"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "9448b379-dd03-4cae-b46b-45f8f98c27b1",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}