{
  "annotation_id": "662f753f-047d-4c50-b6ae-7e8a62cfbc28",
  "date_created": "2026-03-02T18:01:46.037000Z",
  "date_modified": "2026-03-02T18:01:46.037000Z",
  "file_hash": "ad9ff2c25957efee839e4c91aaf11cc11f56055ce1f6fd8df3cb15d04cb60181",
  "private": false,
  "record": {
    "abstract": "We discuss corrections to the Casimir effect at finite temperature and\neffective field theory. Recently, it has been shown that effective field\ntheories can reproduce radiative corrections to the Casimir energy calculated\nin full QED. We apply effective field theory methods at finite temperature and\nreproduce the Casimir free energy. We show that the system undergoes\ndimensional reduction at high temperature and that it can be described by an\neffective three-dimensional field theory.",
    "arxiv_id": "quant-ph/0108009",
    "authors": [
      "Jens O. Andersen"
    ],
    "categories": [
      "quant-ph",
      "hep-ph",
      "hep-th"
    ],
    "title": "Effective Field Theories for the Casimir Effect at Finite Temperature",
    "url": "https://arxiv.org/abs/quant-ph/0108009"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "3daf5e10-a418-47f0-9ac9-d1b105f2641c",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}