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The black holes of topologically massive gravity

Karim Ait Moussa·Gerard Clement·Cedric Leygnac
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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.

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Karim Ait Moussa, Gerard Clement, Cedric Leygnac. 2003-10-24. The black holes of topologically massive gravity. https://doi.org/10.1088/0264-9381%2F20%2F24%2Fl01

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