Instability of a Kerr black hole in f(R) gravity
arXiv:1309.3346 · doi:10.1103/PhysRevD.88.104017
Abstract
We study the stability of a rotating (Kerr) black hole in the viable gravity. The linearized-Ricci scalar equation shows the superradiant instability, leading to the instability of the Kerr black hole in gravity.
13 pages, no figures, title changed slightly, version to appear in PRD
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