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We consider asymptotically anti-de Sitter spacetimes in three-dimensional topologically massive gravity with a negative cosmological constant, for all values of the mass parameter $\mu$ ($\mu\neq0$).
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Here we are using the conventions of Carlip : 16 π G = 1 16\pi G=1 , a metric of signature ( − + + ) (-++) , and a cosmological constant Λ = − 1 / l 2 \Lambda=-1/l^{2} , and set ϵ 012 = 1 \epsilon_{012}=1 (so ϵ 012 = − 1 \epsilon^{012}=-1 )
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A. Strominger, “A Simple Proof of the Chiral Gravity Conjecture,” arXiv:0808.0506 [hep-th]
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M. Henneaux, C. Martínez and R. Troncoso, in preparation
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2009
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