{
  "annotation_id": "bfea8f92-b10d-4167-adfa-53c969b227ed",
  "date_created": "2026-03-02T18:00:08.197000Z",
  "date_modified": "2026-03-02T18:00:08.197000Z",
  "file_hash": "60c2bde5126ce078a02e29f10937dcd3fe7633b0ef4e6bded7397f675c17efa7",
  "private": false,
  "record": {
    "abstract": "The effects of strong magnetic fields on neutron star matter are investigated\nin the quark-meson coupling (QMC) model. The QMC model describes a nuclear\nmany-body system as nonoverlapping MIT bags in which quarks interact through\nself-consistent exchange of scalar and vector mesons in the mean-field\napproximation. The results of the QMC model are compared with those obtained in\na relativistic mean-field (RMF) model. It is found that quantitative\ndifferences exist between the QMC and RMF models, while qualitative trends of\nthe magnetic field effects on the equation of state and composition of neutron\nstar matter are very similar.",
    "arxiv_id": "nucl-th/0610049",
    "authors": [
      "P. Yue",
      "H. Shen"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1103/PhysRevC.74.045807",
    "journal_ref": "Phys.Rev.C74:045807,2006",
    "title": "Neutron star matter in the quark-meson coupling model in strong magnetic   fields",
    "url": "https://arxiv.org/abs/nucl-th/0610049"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "86be5065-dc6e-478b-bf5c-9439e31ecd24",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}