{
  "annotation_id": "0ab4489a-006b-48c5-a284-47b56a450ab1",
  "date_created": "2026-03-02T18:00:43.432000Z",
  "date_modified": "2026-03-02T18:00:43.432000Z",
  "file_hash": "2f5eabd732ee11d2264a640df011a6e8a873f9256ef5b35d03de4a6322fd1723",
  "private": false,
  "record": {
    "abstract": "In this note we consider a variable $G$ cosmology which is consistent with\nobservation and which had successfully predicted an ever expanding accelerating\nuniverse. It is shown that the observed shortening of the orbital periods of\nbinary pulsars is also in good agreement with this model.",
    "arxiv_id": "physics/0212054",
    "authors": [
      "B. G. Sidharth"
    ],
    "categories": [
      "physics.gen-ph"
    ],
    "journal_ref": "Nuovo Cim. B115 (2000) 115",
    "title": "A Test For Varying G",
    "url": "https://arxiv.org/abs/physics/0212054"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "3a8ced2b-7080-4204-840d-464adbd9cb9a",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}