The black holes of topologically massive gravity

Details The black holes of topologically massive gravity The black holes of topologically massive gravity

2003-03-11

arxiv.org/abs/gr-qc/0303042v2

Class.Quant.Grav. 20 (2003) L277-L283

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

10 pages; Eq. (15) corrected, references added, version to appear in Classical and Quantum Gravity

Scientific paper

10.1088/0264-9381/20/24/L01

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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