{
  "id": "gr-qc/0303042",
  "version": "v2",
  "published": "2003-03-11T18:53:34.000Z",
  "updated": "2003-10-24T13:35:45.000Z",
  "title": "The black holes of topologically massive gravity",
  "authors": [
    "Karim Ait Moussa",
    "Gerard Clement",
    "Cedric Leygnac"
  ],
  "comment": "10 pages; Eq. (15) corrected, references added, version to appear in Classical and Quantum Gravity",
  "journal": "Class.Quant.Grav. 20 (2003) L277-L283",
  "doi": "10.1088/0264-9381/20/24/L01",
  "categories": [
    "gr-qc",
    "hep-th"
  ],
  "abstract": "We show that an analytical continuation of the Vuorio solution to three-dimensional topologically massive gravity leads to a two-parameter family of black hole solutions, which are geodesically complete and causally regular within a certain parameter range. No observers can remain static in these spacetimes. We discuss their global structure, and evaluate their mass, angular momentum, and entropy, which satisfy a slightly modified form of the first law of thermodynamics.",
  "revisions": [
    {
      "version": "v2",
      "updated": "2003-10-24T13:35:45.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "black hole solutions",
      "vuorio solution",
      "remain static",
      "three-dimensional topologically massive gravity",
      "parameter range"
    ],
    "tags": [
      "journal article"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 10,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 614877
    }
  }
}