{
  "annotation_id": "85e105bc-7766-4e0d-9507-27839daa1e39",
  "date_created": "2026-03-02T18:01:56.340000Z",
  "date_modified": "2026-03-02T18:01:56.340000Z",
  "file_hash": "7858896be6f05226925c0d33fd2c1f06a7f5c1741904a67a5c9462b30145a11b",
  "private": false,
  "record": {
    "abstract": "If the statement by Einstein, Podolsky and Rosen on incompleteness of\nQuantum-Mechanical description of nature is correct, then we can regard Quantum\nMechanics as a Method of Indirect Computation. The problem is, whether the\ntheory is incomplete or the nature itself does not allow complete description?\nAnd if the first option is correct, how is it possible to complete the\nQuantum-Mechanical description? Here we try to complement de-Broglie\u0027s idea on\nwave-pilot the stochastic gravitation gives origin to. We assume that\nde-Broglie\u0027s wave-pilots are gravitational stochastic ones, and we shall regard\nmicro-objects as test classical particles being subject to the influence of\nde-Broglie\u0027s waves stochastic gravitation.",
    "arxiv_id": "quant-ph/0212139",
    "authors": [
      "Timur F. Kamalov"
    ],
    "categories": [
      "quant-ph"
    ],
    "title": "How to Complete the Quantum-Mechanical Description?",
    "url": "https://arxiv.org/abs/quant-ph/0212139"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "b45fc34d-1aa2-49f3-a65c-954cc8b6e116",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}