Resonant Dynamics and the Instability of the Box Minkowski Model
arXiv:2209.05608 · doi:10.1103/PhysRevD.106.124020
Abstract
We revisit the box Minkowski model [Phys. Rev. Lett. 109, 221101 (2012)] and provide a strong argument that, subject to the Dirichlet boundary condition, it is unstable toward black hole formation for arbitrarily small generic perturbations. Using weakly nonlinear perturbation theory, we derive the resonant system, which compared to systems with the anti-de Sitter asymptotics, has extra resonant terms, and study its properties, including conserved quantities. We find that the generic solution of the resonant system becomes singular in finite time. Surprisingly, the additional resonant interactions do not significantly affect the singular evolution. Furthermore, we find that the interaction coefficients take a relatively simple form, making this a particularly attractive toy model of turbulent gravitational instability.
30 pages, 14 figures, v2: matches published version
References in corpus (6)
- Renormalization group, secular term resummation and AdS (in)stability
- Renormalization, averaging, conservation laws and AdS (in)stability
- Instability of Flat Space Enclosed in a Cavity
- What drives AdS unstable?
- Resonant Hamiltonian systems and weakly nonlinear dynamics in AdS spacetimes
- Gravitational turbulent instability of AdS