{
  "id": "cond-mat/0306406",
  "version": "v2",
  "published": "2003-06-16T12:50:15.000Z",
  "updated": "2004-03-23T17:45:43.000Z",
  "title": "Post-collapse dynamics of self-gravitating Brownian particles in D dimensions",
  "authors": [
    "Clement Sire",
    "Pierre-Henri Chavanis"
  ],
  "journal": "Phys.Rev. E69 (2004) 066109",
  "doi": "10.1103/PhysRevE.69.066109",
  "categories": [
    "cond-mat.stat-mech",
    "astro-ph"
  ],
  "abstract": "We address the post-collapse dynamics of a self-gravitating gas of Brownian particles in D dimensions, in both canonical and microcanonical ensembles. In the canonical ensemble, the post-collapse evolution is marked by the formation of a Dirac peak with increasing mass. The density profile outside the peak evolves self-similarly with decreasing central density and increasing core radius. In the microcanonical ensemble, the post-collapse regime is marked by the formation of a ``binary''-like structure surrounded by an almost uniform halo with high temperature. These results are consistent with thermodynamical predictions.",
  "revisions": [
    {
      "version": "v2",
      "updated": "2004-03-23T17:45:43.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "self-gravitating brownian particles",
      "post-collapse dynamics",
      "dimensions",
      "high temperature",
      "uniform halo"
    ],
    "tags": [
      "journal article"
    ],
    "publication": {
      "publisher": "APS",
      "journal": "Phys. Rev. E"
    },
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 668979
    }
  }
}