Instability of Rotating Anti-de Sitter Black Holes

Abstract

We study the instability of higher-dimensional rotating anti-de Sitter black holes through fragmentation. Fragmentation occurs when black holes rotate too fast to sustain their horizon, and then the black holes are broken into small pieces. Using this process, we test the stability of AdS black holes and discover the dynamical upper bounds of the angular momentum and the cosmological constant. We show that AdS black holes can exist stably within limited parameter ranges in the general dimensions. The parameter ranges are obtained numerically in terms of angular momentum and cosmological constant.

arXiv comment11 pages, 5 figures, published version in PRD

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Cited by in corpus (8)

• Thermodynamics of Three-dimensional Black Holes via Charged Particle Absorption
• Superradiance Instability of Small Rotating AdS Black Holes in Arbitrary Dimensions
• Instability of Black Holes with a Gauss-Bonnet Term
• Instability of Charged Anti-de Sitter Black Holes
• The fragmentation instability of a black hole with $f(R)$ global monopole under GUP
• Dilaton Field Released under Collision of Dilatonic Black Holes with Gauss-Bonnet Term
• Spin Interaction under the Collision of Two Kerr-(anti-)de Sitter Black Holes
• The instability of a black hole with $f(R)$ global monopole under extended uncertainty principle