{
  "id": "1810.02279",
  "version": "v1",
  "published": "2018-10-04T15:36:56.000Z",
  "updated": "2018-10-04T15:36:56.000Z",
  "title": "Waves in the radiative zones of rotating, magnetized stars",
  "authors": [
    "Valade Aurélien",
    "Vincent Prat",
    "Stéphane Mathis",
    "Kyle Augustson"
  ],
  "comment": "2 pages, 1 figure, to appear in Proceedings of SF2A 2018",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "Asteroseismology has reached a level of accuracy that may allow us to detect the effect of a deep magnetic field on oscillation modes. We thus aim to develop an asymptotic theory for short-wavelength waves in radiative zones of rotating stars with a general magnetic field topology (toroidal and poloidal). A dispersion relation is derived for a uniformly rotating star with a low-amplitude, axisymmetric magnetic field. The parameter space for waves in this model is then explored with a Hamiltonian ray-tracing method. The features of the gravito-inertial waves modified by the magnetic field are studied with different magnetic topologies.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2018-10-04T15:36:56.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "radiative zones",
      "magnetized stars",
      "general magnetic field topology",
      "axisymmetric magnetic field",
      "deep magnetic field"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 2,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}