{
  "id": "1609.04583",
  "version": "v1",
  "published": "2016-09-15T11:50:40.000Z",
  "updated": "2016-09-15T11:50:40.000Z",
  "title": "Time-dependent injection as a model for rapid blazar flares",
  "authors": [
    "Michael Zacharias"
  ],
  "comment": "6 pages, proceeding of the 'Blazars through sharp multi-wavelength eyes' conference, to appear in a special issue of 'Galaxies', edited by J. L. G\\'omez, A. P. Marscher, and S. G. Jorstad",
  "categories": [
    "astro-ph.HE"
  ],
  "abstract": "Time-dependent injection can cause non-linear cooling effects, which lead to a faster energy loss of the electrons in jets. The most obvious result is the appearance of unique breaks in the SED, which would normally be attributed to a complicated electron distribution. The knowledge of the observation time and duration is important to interpret the observed spectra, because of the non-trivial evolution of the SED. Intrinsic gamma-gamma absorption processes in the emission region are only of minor importance.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2016-09-15T11:50:40.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "rapid blazar flares",
      "time-dependent injection",
      "intrinsic gamma-gamma absorption processes",
      "faster energy loss",
      "minor importance"
    ],
    "tags": [
      "conference paper"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 6,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}