Unstable mode solutions to the Klein-Gordon equation in Kerr-anti-de Sitter spacetimes

TL;DR

This paper demonstrates the existence of exponentially growing mode solutions to the Klein-Gordon equation in certain Kerr-AdS spacetimes, providing the first rigorous proof of superradiant instability with negative cosmological constant.

Contribution

It constructs explicit unstable solutions in Kerr-AdS spacetimes, revealing superradiant instability for negative cosmological constant, a novel result in mathematical physics.

Findings

Existence of exponentially growing modes in Kerr-AdS spacetimes

Violations of the Hawking-Reall bound lead to instabilities

First rigorous proof of superradiant instability with negative cosmological constant

Abstract

For any cosmological constant $\Lambda=-3/\ell^2<0$ and any $\alpha<9/4$, we find a Kerr-AdS spacetime $(\mathcal M,g_{\mathrm{KAdS}})$, in which the Klein-Gordon equation $\Box_{g_{\mathrm{KAdS}}}\psi+\alpha/\ell^2\psi=0$ has an exponentially growing mode solution satisfying a Dirichlet boundary condition at infinity. The spacetime violates the Hawking-Reall bound $r_+^2>|a|\ell$. We obtain an analogous result for Neumann boundary conditions if $5/4<\alpha<9/4$. Moreover, in the Dirichlet case, one can prove that, for any Kerr-AdS spacetime violating the Hawking-Reall bound, there exists an open family of masses $\alpha$ such that the corresponding Klein-Gordon equation permits exponentially growing mode solutions. Our result adopts methods of Shlapentokh-Rothman (see arXiv:1302.3448) and provides the first rigorous construction of a superradiant instability for negative cosmological constant.