{
  "id": "2008.00099",
  "version": "v1",
  "published": "2020-07-31T22:07:17.000Z",
  "updated": "2020-07-31T22:07:17.000Z",
  "title": "Fractal Gravitation",
  "authors": [
    "T Canavesi"
  ],
  "journal": "Bolet\\'in de la Asociaci\\'on Argentina de Astronom\\'ia (2020) 136-138;",
  "categories": [
    "astro-ph.GA"
  ],
  "abstract": "Considering the GAIA data for {$\\approx 10^6$} stars around the {barycenter,} we estimate the fractal dimension for different regions in the Milky Way. Then we use those fractal dimensions to calculate the gravitational potential considering the medium as a continuous fractal. Finally, {we use the gravitational potential to infer} the circular velocity {and adjust} rotation curves in the Milky Way. {For this,} we use two numerical models, the first considering uniform density and a second more realistic of a bulge and a disk. In none of these models we consider dark matter. We study their validity comparing them with circular speed data from the Milky Way.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2020-07-31T22:07:17.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "fractal gravitation",
      "milky way",
      "fractal dimension",
      "gravitational potential",
      "first considering uniform density"
    ],
    "tags": [
      "journal article"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}