{
  "annotation_id": "58718ec7-d941-471f-87e5-68c841b030f4",
  "date_created": "2026-03-02T18:01:45.458000Z",
  "date_modified": "2026-03-02T18:01:45.458000Z",
  "file_hash": "3178432cd0d65c26b0105feb713bd9476ff37a6f2fba5e3689e8c6210edd3abf",
  "private": false,
  "record": {
    "abstract": "The existence of irreducible field fluctuations in vacuum is an important\nprediction of quantum theory. These fluctuations have many observable\nconsequences, like the Casimir effect which is now measured with good accuracy\nand agreement with theory, provided that the latter accounts for differences\nbetween real experiments and the ideal situation considered by Casimir. But the\nvacuum energy density calculated by adding field mode energies is much larger\nthan the density observed around us through gravitational phenomena. This\n``vacuum catastrophe\u0027\u0027 is one of the unsolved problems at the interface between\nquantum theory on one hand, inertial and gravitational phenomena on the other\nhand. It is however possible to put properly formulated questions in the\nvicinity of this paradox. These questions are directly connected to observable\neffects bearing upon the principle of relativity of motion in quantum vacuum.",
    "arxiv_id": "quant-ph/0105053",
    "authors": [
      "Serge Reynaud",
      "Astrid Lambrecht",
      "Cyriaque Genet",
      "Marc-Thierry Jaekel"
    ],
    "categories": [
      "quant-ph",
      "gr-qc"
    ],
    "doi": "10.1016/S1296-2147(01)01270-7",
    "journal_ref": "C. R. Acad. Sci. Paris, 2-IV (2001) p.1287-1298",
    "title": "Quantum vacuum fluctuations",
    "url": "https://arxiv.org/abs/quant-ph/0105053"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "d29802b3-d240-4192-8e11-8bc8c6fbe38b",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}