{
  "annotation_id": "23abad3f-b5c5-4c14-b776-aa3d89104666",
  "date_created": "2026-03-02T18:01:20.792000Z",
  "date_modified": "2026-03-02T18:01:20.792000Z",
  "file_hash": "1ac9aed80386f6c4564d67f681b24fe99adfab06342f14924fad3d3941d8128c",
  "private": false,
  "record": {
    "abstract": "Transverse quasilinear relaxation of the cyclotron-Cherenkov instability in\nthe inhomogeneous magnetic field of pulsar magnetospheres is considered. We\nfind quasilinear states in which the kinetic cyclotron-Cherenkov instability of\na beam propagating through strongly magnetized pair plasma is saturated by the\nforce arising in the inhomogeneous field due to the conservation of the\nadiabatic invariant. The resulting wave intensities generally have nonpower law\nfrequency dependence, but in a broad frequency range can be well approximated\nby the power law with the spectral index -2. The emergent spectra and fluxes\nare consistent with the one observed from pulsars.",
    "arxiv_id": "physics/9802026",
    "authors": [
      "Maxim Lyutikov"
    ],
    "categories": [
      "physics.plasm-ph"
    ],
    "doi": "10.1103/PhysRevE.58.2474",
    "title": "Transverse quasilinear relaxation in inhomogeneous magnetic field",
    "url": "https://arxiv.org/abs/physics/9802026"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "d78b36e2-3ed8-402e-bb9c-4ef0a06d87f7",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}