{
  "annotation_id": "19cba4dc-6079-499e-9606-2165e52a389b",
  "date_created": "2026-03-02T18:00:57.099000Z",
  "date_modified": "2026-03-02T18:00:57.099000Z",
  "file_hash": "625f8716054c156340ec8e292b7f3ff1b24c3ea937ed4e8db31840ccbe6cccc0",
  "private": false,
  "record": {
    "abstract": "In the exact (non-linear) formulation of general relativity (GR) no motion of\nbodies can give origin to gravitational waves (GW\u0027s) - as it has been proved.\nAccordingly, the measured rate of change of the orbital period of binary pulsar\nB PSR1913+16 must have other causes, different from the emission of GW\u0027s; maybe\nthe viscous losses of the unseen pulsar companion, if it were e.g. a helium\nstar.",
    "arxiv_id": "physics/0502089",
    "authors": [
      "A. Loinger"
    ],
    "categories": [
      "physics.gen-ph"
    ],
    "title": "No GW is emitted by B PSR1913+16",
    "url": "https://arxiv.org/abs/physics/0502089"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "e3b3200e-382e-4b42-a9c0-202ef5f442aa",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}