{
  "annotation_id": "58e89132-68f8-4e65-9695-f5d9a7129486",
  "date_created": "2026-03-02T18:00:39.170000Z",
  "date_modified": "2026-03-02T18:00:39.170000Z",
  "file_hash": "d9468d1d5c0d3feb380dbf083f14418dad72f72d0ddc9d0f7ce24e19f46a1c4f",
  "private": false,
  "record": {
    "abstract": "A monochromatic linear source of light is rotated with certain angular\nfrequency and when such light is analysed after reflection then a change of\nfrequency or wavelength may be observed depending on the location of the\nobserver. This change of frequency or wavelength is different from the\nclassical Doppler effect [1] or relativistic Doppler effect [2]. The reason\nbehind this shift in wavelength is that a certain time interval observed by an\nobserver in the rotating frame is different from that of a stationary observer.",
    "arxiv_id": "physics/0208034",
    "authors": [
      "Amit Halder"
    ],
    "categories": [
      "physics.optics"
    ],
    "title": "Rotational Doppler Effect",
    "url": "https://arxiv.org/abs/physics/0208034"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "df2838d6-2c80-4ce2-995f-122f67788c49",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}