{
  "id": "1307.7267",
  "version": "v1",
  "published": "2013-07-27T14:45:43.000Z",
  "updated": "2013-07-27T14:45:43.000Z",
  "title": "Holographic turbulence",
  "authors": [
    "Allan Adams",
    "Paul M. Chesler",
    "Hong Liu"
  ],
  "comment": "6 pages, 3 figures",
  "journal": "Phys. Rev. Lett. 112, 151602 (2014)",
  "doi": "10.1103/PhysRevLett.112.151602",
  "categories": [
    "hep-th",
    "gr-qc",
    "physics.flu-dyn"
  ],
  "abstract": "We construct turbulent black holes in asymptotically AdS_4 spacetime by numerically solving Einstein equations. Both the dual holographic fluid and bulk geometry display signatures of an inverse cascade with the bulk geometry being well approximated by the fluid/gravity gradient expansion. We argue that statistically steady-state black holes dual to d dimensional turbulent flows have horizons which are approximately fractal with fractal dimension D=d+4/3.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2013-07-27T14:45:43.000Z"
    }
  ],
  "analyses": {
    "subjects": [
      "11.25.Tq",
      "04.50.Gh"
    ],
    "keywords": [
      "holographic turbulence",
      "bulk geometry display signatures",
      "statistically steady-state black holes dual",
      "construct turbulent black holes",
      "fluid/gravity gradient expansion"
    ],
    "tags": [
      "journal article"
    ],
    "publication": {
      "publisher": "APS",
      "journal": "Physical Review Letters",
      "year": 2014,
      "month": "Apr",
      "volume": 112,
      "number": 15,
      "pages": 151602
    },
    "note": {
      "typesetting": "TeX",
      "pages": 6,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 1245005,
      "adsabs": "2014PhRvL.112o1602A"
    }
  }
}