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Conserved quantities and Virasoro algebra in New massive gravity

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arxiv 1303.3691 v2 pith:JUIHCFQV submitted 2013-03-15 hep-th

classification hep-th
keywords blackholesentropygravityhorizonmassiveextremalfield
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Using the {\it off-shell} Noether current and potential we compute the entropy for the AdS black holes in new massive gravity. For the non-extremal BTZ black holes by implementing the so-called stretched horizon approach we reproduce the correct expression for the horizon entropy. For the extremal case, we adopt standard formalism in the AdS/CFT correspondence and reproduce the corresponding entropy by computing the central extension term on the asymptotic boundary of the near horizon geometry. We explicitly show the invariance of the angular momentum along the radial direction for extremal as well as non-extremal BTZ black holes in our model. Furthermore, we extend this invariance for the black holes in new massive gravity coupled with a scalar field, which correspond to the holographic renormalization group flow trajectory of the dual field theory. This provides another realization for the holographic c-theorem.

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  1. Extended Near Horizon Symmetries of Extremal BTZ Black Holes in 3D Massive Gravity

    hep-th 2024-12 conditional novelty 6.0 of 10

    Near-horizon extremal BTZ black holes in NMG and TMG carry two Virasoro algebras whose central charges equal their spatial-infinity values.

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