{
  "annotation_id": "ab91805b-068d-437c-849f-cee4390cb543",
  "date_created": "2026-03-02T18:00:42.744000Z",
  "date_modified": "2026-03-02T18:00:42.744000Z",
  "file_hash": "b3176aa2aa142ddd0065ebea354feca8ff8d3774d9442b8276c709d2b7c9407a",
  "private": false,
  "record": {
    "abstract": "Model of Expansive Nondecelerative Universe (ENU) due to involving Vaidya\nmetric makes it possible to localize the energy density of gravitational field.\nThis its capability allows for answering several open questions and supporting\n(or contradicting) results obtained using different theoretical approaches.\nThis paper is aimed to contributing to a solution of some cosmological\nproblems, in particular those linked to the Yukawa potential consequences,\nindependent way of dark matter estimation, ionospheric F2 layer behaviour, and\ncyclotron radiation.",
    "arxiv_id": "physics/0304004",
    "authors": [
      "Miroslav Sukenik",
      "Jozef Sima"
    ],
    "categories": [
      "physics.gen-ph"
    ],
    "title": "Cosmological Consequences of the Yukawa Potential Involvement in   Gravitational and Electromagnetic Fields Interaction Evaluated by ENU Model",
    "url": "https://arxiv.org/abs/physics/0304004"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "6e283d8b-1727-485f-99c8-60d2e1f5f09d",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}