{
  "annotation_id": "5c9aa0c2-743e-4a15-9d73-2ec1b385d7a4",
  "date_created": "2026-03-02T18:01:42.017000Z",
  "date_modified": "2026-03-02T18:01:42.017000Z",
  "file_hash": "810783bf5f22eeef38d81a54a4003e69e102943eb7d61b1d2397b2df4ecabc92",
  "private": false,
  "record": {
    "abstract": "A mirror in the vacuum is submitted to a radiation pressure exerted by\nscattered fields. It is known that the resulting mean force is zero for a\nmotionless mirror, but not for a mirror moving with a non-uniform acceleration.\nWe show here that this force results from a motional modification of the field\nscattering while being associated with the fluctuations of the radiation\npressure on a motionless mirror. We consider the case of a scalar field in a\ntwo-dimensional spacetime and characterize the scattering upon the mirror by\nfrequency dependent transmissivity and reflectivity functions obeying\nunitarity, causality and high frequency transparency conditions. We derive\ncausal expressions for dissipation and fluctuations and exhibit their relation\nfor any stationary input. We recover the known damping force at the limit of a\nperfect mirror in vacuum. Finally, we interpret the force as a mechanical\nsignature of the squeezing effect associated with the mirror\u0027s motion.",
    "arxiv_id": "quant-ph/0101068",
    "authors": [
      "Marc-Thierry Jaekel",
      "Serge Reynaud"
    ],
    "categories": [
      "quant-ph"
    ],
    "doi": "10.1088/0954-8998/4/1/005",
    "journal_ref": "Quant.Opt. 4 (1992) 39",
    "title": "Fluctuations and dissipation for a mirror in vacuum",
    "url": "https://arxiv.org/abs/quant-ph/0101068"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "343e59de-757b-47e5-a636-93238501f343",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}