The Black holes of topologically massive gravity

By K. Moussa, G. Clément, C. Leygnac. 2003

150 citations recorded by the source corpus.

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.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics, Statistical and Nonlinear Physics

View Paper: https://www.semanticscholar.org/paper/441a0ad9e70782c8b01c7f27e5c4fccdef5476ad

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In Astronomy and Astrophysics

  1. Marika Taylor
  2. Thomas Hartman
  3. Dionysios Anninos
  4. Kostas Skenderis
  5. B. C. Rees
  6. A. Maloney
  7. Andrew Strominger
  8. D. Hofman

In Nuclear and High Energy Physics

  1. Marika Taylor
  2. Kostas Skenderis
  3. Thomas Hartman
  4. Dionysios Anninos
  5. B. C. Rees
  6. A. Maloney
  7. Andrew Strominger
  8. D. Hofman

In Statistical and Nonlinear Physics

  1. Marika Taylor
  2. Kostas Skenderis
  3. Thomas Hartman
  4. Dionysios Anninos
  5. Andrew Strominger
  6. B. C. Rees
  7. A. Maloney
  8. Wei Song

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