{
  "annotation_id": "a98798fa-b46b-4f28-932b-6a1b599706a5",
  "date_created": "2026-03-02T18:00:53.733000Z",
  "date_modified": "2026-03-02T18:00:53.733000Z",
  "file_hash": "153d8adb938f5a8b36078edd708277087a463e005b8986b396f7647d8a885761",
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  "record": {
    "abstract": "A new derivation of the relativistic aberration formula for a plane-polarized\nlight wave is presented that does not require any use of the Lorentz\ntransformation. The method is based on a modification of the Huygens-Fresnel\nprinciple to include the relativistic effects introduced by the relative motion\nbetween the observer and the emitter. The derivation clearly shows that the\naberration formula is a direct consequence of the relative simultaneity.",
    "arxiv_id": "physics/0409013",
    "authors": [
      "Aleksandar Gjurchinovski"
    ],
    "categories": [
      "physics.optics",
      "astro-ph",
      "physics.class-ph"
    ],
    "doi": "10.1088/0143-0807/27/4/002",
    "journal_ref": "Eur.J.Phys. 27 (2006) 703-708",
    "title": "Relativistic aberration of light as a corollary of relativity of   simultaneity",
    "url": "https://arxiv.org/abs/physics/0409013"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "60d60eb7-caa6-40ee-bfde-4cc859429fba",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}