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Article Dans Une Revue Classical and Quantum Gravity Année : 2003

The black holes of topologically massive gravity

Résumé

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.

Dates et versions

hal-00356804 , version 1 (28-01-2009)

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Karim Ait Moussa, Gérard Clément, Cedric Leygnac. The black holes of topologically massive gravity. Classical and Quantum Gravity, 2003, 20, pp.L277-L283. ⟨hal-00356804⟩
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