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

Keiju Murata, Harvey S. Reall, Norihiro Tanahashi

Research output: Contribution to journalArticle

40 Citations (Scopus)

Abstract

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.

Original languageEnglish
Article number235007
JournalClassical and Quantum Gravity
Volume30
Issue number23
DOIs
Publication statusPublished - 2013 Dec 7

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horizon
event horizon
Reissner-Nordstrom solution
perturbation
scalars
gradients
decay

ASJC Scopus subject areas

  • Physics and Astronomy (miscellaneous)

Cite this

What happens at the horizon(s) of an extreme black hole? / Murata, Keiju; Reall, Harvey S.; Tanahashi, Norihiro.

In: Classical and Quantum Gravity, Vol. 30, No. 23, 235007, 07.12.2013.

Research output: Contribution to journalArticle

Murata, Keiju ; Reall, Harvey S. ; Tanahashi, Norihiro. / What happens at the horizon(s) of an extreme black hole?. In: Classical and Quantum Gravity. 2013 ; Vol. 30, No. 23.
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