Asymptotic stability conjecture for anti-de Sitter spacetime with dissipative boundary conditions

The pure anti-de Sitter spacetime has metric

gAdS=(1+(Λ3)r2)dt2+(1+(Λ3)r2)1dr2+r2dσ2.g_{AdS}=-\left(1+\bigl(-\frac{\Lambda}{3}\bigr)r^2\right)dt^2+\left(1+\bigl(-\frac{\Lambda}{3}\bigr)r^2\right)^{-1}dr^2+r^2d\sigma^2.

The boundary conditions are optimally dissipative. Asymptotic stability conjecture. Anti-de Sitter spacetime is asymptotically stable for optimally dissipative boundary conditions. Holzegel, Luk, Smulevici, and Warnick proved standard energy boundedness and integrated decay for the Klein–Gordon equation with α=2\alpha=-2 under these boundary conditions, providing a first step toward this conjecture; the full nonlinear stability statement remains open.

Sources & referencesView supporting material

Primary source

Weihao Zheng, “Exponentially-growing Mode Instability on Reissner-Nordström–Anti-de-Sitter black holes”, arXiv:2410.04750 (2024).

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