{
  "annotation_id": "c608a582-7a13-495f-804c-706eb3002680",
  "date_created": "2026-03-02T18:01:04.295000Z",
  "date_modified": "2026-03-02T18:01:04.295000Z",
  "file_hash": "dbe38b72ec6008b787ebde7896be2b2176ab462bfca90cc4a632100f3f5469c8",
  "private": false,
  "record": {
    "abstract": "The interactions of gravitational waves with interstellar matter, dealing\nwith resonant wave-particle and wave-wave interactions, are considered on the\nbasis of magnetic-type Maxwell-Vlasov equations. It is found that the behavior\nof the fields, involving the \"gravitoelectromagnetic\" or \"GEM \" fields, the\nperturbed density field and self-generated gravitomagnetic field with low\nfrequency,can be described by the nonlinear coupling equations Eqs.\n(6.10)-(6.12). Numerical results show that they may collapse. In other words,\ndue to self-condensing, a stronger GME fields could be produced; and they could\nappear as the gravitational waves with high energy reaching on Earth. In this\ncase, Weber\u0027s results, perhaps, are acceptable.",
    "arxiv_id": "physics/0511111",
    "authors": [
      "X. Q. Li",
      "S. Q. Liu",
      "X. Y. Tao"
    ],
    "categories": [
      "physics.plasm-ph"
    ],
    "doi": "10.1002/andp.200810352",
    "journal_ref": "Ann.Phys.(Berlin)18,No.6, 436-453(2009)",
    "title": "Nonlinear Interactions of Gravitational Wave with Matter in   Magnetic-type Maxwell-Vlasov Description",
    "url": "https://arxiv.org/abs/physics/0511111"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "72b34ea1-7018-42d0-add6-4022fba8ffa4",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}