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2013

What happens at the horizon(s) of an extreme black hole?

Murata, Keiju, Reall, Harvey S., Tanahashi, Norihiro

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A massless scalar field exhibits an instability at the event horizon of an extreme black hole.

We study numerically the nonlinear evolution of this instability for spherically symmetric perturbations of an extreme Reissner-Nordstrom (RN) black hole.
We find that generically the endpoint of the instability is a non-extreme RN solution.
However, there exist fine-tuned initial perturbations for which the instability never decays.

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