{
  "annotation_id": "afd57c82-5be9-46dd-8501-9690f6e3529d",
  "date_created": "2026-03-02T18:00:01.355000Z",
  "date_modified": "2026-03-02T18:00:01.355000Z",
  "file_hash": "d47776085d931aa63014a9fe61cdf091e414e8a14d18a00cc360c7a68bd81c2d",
  "private": false,
  "record": {
    "abstract": "Extending the concepts of light-front field theory to quantum statistics\nprovides a novel approach towards nuclear matter under extreme conditions. Such\nconditions exist, e.g., in neutron stars or in the early stage of our universe.\nThey are experimentally expected to occur in heavy ion collisions, e.g., at\nRHIC and accelerators to be build at GSI and CERN. Light-front field theory is\nparticularly suited, since it is based on a relativistic Hamiltonian approach.\nIt allows us to treat the perturbative as well as the nonperturbative regime of\nQCD and also correlations that emerge as a field of few-body physics and is\nimportant for hadronization. Last but not least the Hamiltonian approach is\nuseful for nonequilibrium processes by utilizing, e.g., the formalism of\nnonequilibrium statistical operators.",
    "arxiv_id": "nucl-th/0410004",
    "authors": [
      "Michael Beyer"
    ],
    "categories": [
      "nucl-th",
      "hep-th"
    ],
    "doi": "10.1007/s00601-004-0076-9",
    "journal_ref": "Few Body Syst. 36 (2005) 23-28",
    "title": "Light-front field theory of hot and dense quark matter",
    "url": "https://arxiv.org/abs/nucl-th/0410004"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "391c7782-2562-478a-9b73-edff8b26db2d",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}