Instability of three dimensional conformally dressed black hole

Abstract

The three dimensional black hole solution of Einstein equations with negative cosmological constant coupled to a conformal scalar field is proved to be unstable against linear circularly symmetric perturbations.

5 pages, REVTeX

References in corpus (3)

• Conformally dressed black hole in 2+1 dimensions
• Spinning Black Holes in (2+1)-dimensional String and Dilaton Gravity
• Modifications of the BTZ black hole by a dilaton/scalar

Cited by in corpus (8)

• Influence of the back reaction of the Hawking radiation upon black hole quasinormal modes
• Instability of a four-dimensional de Sitter black hole with a conformally coupled scalar field
• Three-Dimensional Gravity with Conformal Scalar and Asymptotic Virasoro Algebra
• Fate of Three-Dimensional Black Holes Coupled to a Scalar Field and the Bekenstein-Hawking Entropy
• Gravity/CFT correspondence for three dimensional Einstein gravity with a conformal scalar field
• Anti-de Sitter massless scalar field spacetimes in arbitrary dimensions
• Hairy Black Hole Stability in AdS, Quantum Mechanics on the Half-Line and Holography
• Exact black-hole formation with a conformally coupled scalar field in three dimensions