Conserved quantities and Virasoro algebra in New massive gravity
arXiv:1303.3691 · doi:10.1007/JHEP05(2013)041
Abstract
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.
29 pages, Published version
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- Noncommutative Heisenberg algebra in the neighbourhood of a generic null surface
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- Existence of conserved quantities and their algebra in curved spacetime
- Extended Near Horizon Symmetries of Extremal BTZ Black Holes in 3D Massive Gravity
- Topological charge and black hole photon spheres in massive gravity