{
  "annotation_id": "8e925897-5353-43de-a6b3-e0a2c2e8d31d",
  "date_created": "2026-03-02T18:01:20.784000Z",
  "date_modified": "2026-03-02T18:01:20.784000Z",
  "file_hash": "ea80248921cbc4b88373dd079adfcc1d932ac3961fa9aec62a8604dc370ec56c",
  "private": false,
  "record": {
    "abstract": "The radiation force on a single electron in an ultraintense plane wave ($a =\neE/mc\\omega \\sim 1$) is calculated and shown to be proportional to $a^4$ in the\nhigh-$a$ limit for arbitrary waveform and polarization. The cyclotron motion of\nan electron in a constant magnetic field and an ultraintense plane wave is\nnumerically found to be quasiperiodic even in the high-$a$ limit if the\nmagnetic field is not too strong, as suggested by previous analytical work. A\nstrong magnetic field causes highly chaotic electron motion and the boundary of\nthe highly chaotic region of parameter space is determined numerically.\nApplications to experiments and astrophysics are briefly discussed.",
    "arxiv_id": "physics/9802025",
    "authors": [
      "Joel E. Moore"
    ],
    "categories": [
      "physics.plasm-ph",
      "cond-mat.stat-mech"
    ],
    "doi": "10.1103/PhysRevE.59.2281",
    "journal_ref": "Phys. Rev. E 59, 2281-2285 (1999)",
    "title": "Nonlinear Radiation Pressure and Stochasticity in Ultraintense Laser   Fields",
    "url": "https://arxiv.org/abs/physics/9802025"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "7e9cb129-dcb4-46b4-a2da-b60d965384fa",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}