The Fate of Instability of de Sitter Black Holes at Large $D$

Abstract

We study non-linearly the gravitational instabilities of Reissner-Nordstrom-de Sitter and Gauss-Bonnet-de Sitter black holes by using the large $D$ expansion method. In both cases, the thresholds of the instability are found to be consistent with the linear analysis, and on the thresholds the evolutions of the black holes under perturbations settle down to stationary lumpy solutions. However, the solutions in unstable region are highly time-dependent, and resemble the fully localized black spots and black ring with $S^{D-2}$ and $S^1\times S^{D-3}$ topologies, respectively. Our study indicates the possible transition between the lumpy black holes and localized black holes in higher dimensions.

arXiv comment17 pages, 4 figures, accepted version

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• The Large D Limit of Einstein's Equations
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• Black Holes and Wormholes in Higher-Curvature Corrected Theories of Gravity