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Gregory-Laflamme instability of BTZ black hole in new massive gravity

arXiv:1310.3024 · doi:10.1103/PhysRevD.88.124014

Abstract

We find the Gregory-Laflamme $s$-mode instability of the non-rotating BTZ black hole in new massive gravity. This instability shows that the BTZ black hole could not exist as a stable static solution to the new massive gravity. For non-rotating BTZ black string in four dimensions, however, it is demonstrated that the BTZ black string can be stable against the metric perturbation.

13 pages, 1 figure