Journal
CLASSICAL AND QUANTUM GRAVITY
Volume 20, Issue 24, Pages L277-L283Publisher
IOP PUBLISHING LTD
DOI: 10.1088/0264-9381/20/24/L01
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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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