{
  "annotation_id": "0843f0aa-9005-4bf8-84a3-1a9307999576",
  "date_created": "2026-03-02T18:00:42.214000Z",
  "date_modified": "2026-03-02T18:00:42.214000Z",
  "file_hash": "c9344427452075b9aa2bffadb87ffd02d966c1ed8aba622e62ad43335aef0622",
  "private": false,
  "record": {
    "abstract": "We solve the problem of formulating Brownian motion in a relativistically\ncovariant framework in 1+1 and 3+1 dimensions. We obtain covariant\nFokker-Planck equations with (for the isotropic case) a differential operator\nof invariant d\u0027Alembert form. Treating the spacelike and timelike fluctuations\nseparately, we show that it is essential to take into account the analytic\ncontinuation of \"unphysical\" fluctuations in order to achieve these results.",
    "arxiv_id": "physics/0212036",
    "authors": [
      "O. Oron",
      "L. P. Horwitz"
    ],
    "categories": [
      "physics.class-ph",
      "hep-ph",
      "hep-th",
      "physics.gen-ph"
    ],
    "journal_ref": "Rel.Grav.Cosmol. 1 (2004) 109-122",
    "title": "Relativistic Brownian Motion",
    "url": "https://arxiv.org/abs/physics/0212036"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "64352916-4e0d-4328-9708-728838e4f3ac",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}