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

About 2 years old · traced to

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.

References

Primary source

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

Progress summary

Never refreshed

Nothing recorded yet. Refresh searches the literature and the public web for attempts on this problem, and writes the first summary here.

Solutions 0

No solutions have been posted yet.