Instability of a Kerr black hole in f(R) gravity

preprint2013arXivOpen access

We study the stability of a rotating (Kerr) black hole in the viable $f(R)$ gravity. The linearized-Ricci scalar equation shows the superradiant instability, leading to the instability of the Kerr black hole in $f(R)$ gravity.

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Instability of a Kerr black hole in f(R) gravity

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