Abstract
We consider critical gravity in three dimensions; that is, the New Massive Gravity theory formulated about Anti-de Sitter (AdS) space with the specific value of the graviton mass for which it results dual to a two-dimensional conformal field theory with vanishing central charge. As it happens with Kerr black holes in four-dimensional critical gravity, in three-dimensional critical gravity the Bañados–Teitelboim–Zanelli black holes have vanishing mass and vanishing angular momentum. However, provided suitable asymptotic conditions are chosen, the theory may also admit solutions carrying non-vanishing charges. Here, we give simple examples of exact solutions that exhibit falling-off conditions that are even weaker than those of the so-called Log-gravity. For such solutions, we define the quasilocal stress-tensor and use it to compute conserved charges. Despite the drastic deformation of AdS\(_3\) asymptotic, these solutions have non-zero mass and angular momentum, which we compute.
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Acknowledgments
This work has been supported by UBA, CONICET, and ANPCyT. The authors are grateful to Stéphane Detournay and Guillem Pérez–Nadal for discussions. G.G. thanks Pontificia Universidad Católica de Valparaíso for the hospitality during his stays, where part of this work was done.
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Garbarz, A., Giribet, G., Goya, A. et al. Quasilocal energy for three-dimensional massive gravity solutions with chiral deformations of AdS\(_3\) boundary conditions. Gen Relativ Gravit 46, 1735 (2014). https://doi.org/10.1007/s10714-014-1735-x
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DOI: https://doi.org/10.1007/s10714-014-1735-x