Bubbles in Anti-de Sitter Space

Abstract

We explore the bubble spacetimes which can be obtained from double analytic continuations of static and rotating black holes in anti-de Sitter space. In particular, we find that rotating black holes with elliptic horizon lead to bubble spacetimes only in dimension greater than five. For dimension greater than seven, the topology of the bubble can be non-spherical. However, a bubble spacetime is shown to arise from a rotating de Sitter black hole in four dimensions. In all cases, the evolution of the bubble is of de Sitter type. Double analytic continuations of hyperbolic black holes and branes are also discussed.

8 pages, Latex

References in corpus (3)

• Cardy-Verlinde Formula and Thermodynamics of Black Holes in de Sitter Spaces
• Quasilocal Thermodynamics of Kerr de Sitter Spacetimes and the dS/CFT Correspondence
• Semiclassical instability of the brane-world: Randall-Sundrum bubbles

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