Extreme charged black holes in braneworld with cosmological constant
arXiv:1007.1820 · doi:10.1103/PhysRevD.82.085029
Abstract
Application of the adS/CFT correspondence to the RS models may predict that there is no static solution for black holes with a radius larger than the bulk curvature scale. When the black hole has an extremal horizon, however, the correspondence suggests that the black hole can stay static. We focus on the effects of cosmological constant on the brane on such extremal brane-localized black holes. We observe that the positive cosmological constant restrict the black hole size on the brane as in ordinary four-dimensional general relativity. The maximum black hole size differs from that in four-dimensional general relativity case due to the non-linear term in the effective Einstein equation. In the negative cosmological constant case, we obtain an implication on the Newton constant in the Karch-Randall model.
arXiv comment12 pages, 8 figures
References in corpus (22)
- A Large Mass Hierarchy from a Small Extra Dimension
- An Alternative to Compactification
- Holographic Reconstruction of Spacetime and Renormalization in the AdS/CFT Correspondence
- The Einstein Equations on the 3-Brane World
- Brane-World Gravity
- Locally Localized Gravity
- Gravity in the Randall-Sundrum Brane World
- Near-horizon symmetries of extremal black holes
- Quantum Black Holes as Holograms in AdS Braneworlds
- Classical black hole evaporation in Randall-Sundrum infinite braneworld
- Small localized black holes in a braneworld: Formulation and numerical method
- Black Hole Astrophysics in AdS Braneworlds
- A Cosmological Constant Limits the Size of Black Holes
- Microscopic Theory of Black Hole Superradiance
- Upper bound for entropy in asymptotically de Sitter space-time
- On the existence of a static black hole on a brane
- Quantum Radion on de Sitter branes
- Charged Randall-Sundrum black holes and N=4 super Yang-Mills in AdS(2)xS(2)
- Locally Localized Gravity: The Inside Story
- Accelerating a Black Hole in Higher Dimensions
- Quantum Back Reaction to asymptotically AdS Black Holes
- Floating Black Hole in the Karch-Randall Model and its Holographic Dual