Dynamical Instability of Self-Gravitating Membranes
arXiv:2207.13754 · doi:10.1103/PhysRevLett.130.011402
Abstract
We show that a generic relativistic membrane with in-plane pressure and surface density having the same sign is unstable with respect to a series of warping mode instabilities with high wave numbers. We also examine the criteria of instability for commonly studied exotic compact objects with membranes, such as gravastars, AdS bubbles and thin-shell wormholes. For example, a gravastar which satisfies the weak energy condition turns out to be dynamically unstable. A thin-layer black hole mimicker is stable only if it has positive pressure and negative surface density (such as a wormhole), or vice versa.
8 pages, 3 figures. Accepted by Phys. Rev. Lett
References in corpus (8)
- First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole
- First Sagittarius A* Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole in the Center of the Milky Way
- Traversable wormholes: Some simple examples
- Echoes of ECOs: gravitational-wave signatures of exotic compact objects and of quantum corrections at the horizon scale
- Traversable wormholes from surgically modified Schwarzschild spacetimes
- Compactness bounds in General Relativity
- Dynamics and Observational Signatures of Shell-like Black Hole Mimickers
- Mimicking Kerr's multipole moments
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