{
  "id": "1407.7496",
  "version": "v1",
  "published": "2014-07-28T18:44:27.000Z",
  "updated": "2014-07-28T18:44:27.000Z",
  "title": "A correlation between the amount of dark matter in elliptical galaxies and their shape",
  "authors": [
    "Alexandre Deur"
  ],
  "comment": "Proceeding for a presentation given at Duke University, Apr. 2014. Based on A. D. PLB B676, 21 (2009); A.D, MNRAS, 438, 1535 (2014)",
  "categories": [
    "astro-ph.GA",
    "hep-ph"
  ],
  "abstract": "We discuss the correlation between the dark matter content of elliptical galaxies and their ellipticities. We then explore a mechanism for which the correlation would emerge naturally. Such mechanism leads to identifying the dark matter particles to gravitons. A similar mechanism is known in Quantum Chromodynamics (QCD) and is essential to our understanding of the mass and structure of baryonic matter.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2014-07-28T18:44:27.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "elliptical galaxies",
      "correlation",
      "dark matter particles",
      "dark matter content",
      "baryonic matter"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 1308694,
      "adsabs": "2014arXiv1407.7496D"
    }
  }
}