{
  "annotation_id": "2597fa95-4859-4496-9705-245241d2eefd",
  "date_created": "2026-03-02T18:01:06.555000Z",
  "date_modified": "2026-03-02T18:01:06.555000Z",
  "file_hash": "315062a5e8236248d4f7f39c9f1b2bb92e47c6c6e04641fc8e8127f2a793f829",
  "private": false,
  "record": {
    "abstract": "Assuming a suitable rotation of the Universe as a whole, we can attribute the\nrotation of galaxies to it. Using Lagrangian Mechanics we then can find the\nequations governing the rotation of a galaxy. We find in this way the azimuthal\nequation, and we find its first integral. Then we derive from it the law of\ndifferrential rotation of galaxies, and we plot it. We also present the\nresulting flat rotation curve, which is found to resemble remarkably the\nobserved rotation curves.",
    "arxiv_id": "physics/0602035",
    "authors": [
      "Evangelos Chaliasos"
    ],
    "categories": [
      "physics.gen-ph"
    ],
    "license": "http://arxiv.org/licenses/nonexclusive-distrib/1.0/",
    "title": "The rotation of galaxies as a consequence of a rotation of the Universe",
    "url": "https://arxiv.org/abs/physics/0602035"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "789742d5-0b66-4955-8b04-a82d19c8cfef",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}