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

Keiju Murata, Harvey S. Reall, Norihiro Tanahashi

研究成果: Article査読

57 被引用数 (Scopus)


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. In this case, the perturbed spacetime describes a time-dependent extreme black hole. Such solutions settle down to extreme RN outside, but not on, the event horizon. The event horizon remains smooth but certain observers who cross it at late time experience large gradients there. Our results indicate that these dynamical extreme black holes admit a C1 extension across an inner (Cauchy) horizon.

ジャーナルClassical and Quantum Gravity
出版ステータスPublished - 2013 12月 7

ASJC Scopus subject areas

  • 物理学および天文学(その他)


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