Onset of superradiant instabilities in the hydrodynamic vortex model
arXiv:1405.7702 · doi:10.1103/PhysRevD.90.027501
Abstract
The hydrodynamic vortex, an effective spacetime geometry for propagating sound waves, is studied analytically. In contrast with the familiar Kerr black-hole spacetime, the hydrodynamic vortex model is described by an effective acoustic geometry which has no horizons. However, this acoustic spacetime possesses an ergoregion, a property which it shares with the rotating Kerr spacetime. It has recently been shown numerically that this physical system is linearly unstable due to the superradiant scattering of sound waves in the ergoregion of the effective spacetime. In the present study we use analytical tools in order to explore the onset of these superradiant instabilities which characterize the effective spacetime geometry. In particular, we derive a simple analytical formula which describes the physical properties of the hydrodynamic vortex system in its critical (marginally-stable) state, the state which marks the boundary between stable and unstable fluid configurations. The analytically derived formula is shown to agree with the recently published numerical data for the hydrodynamic vortex system.
5 pages
References in corpus (5)
Cited by in corpus (8)
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- Dissipative Quantum Vortices and Superradiant Scattering
- Marginally stable resonant modes of the polytropic hydrodynamic vortex
- Ergoregion instability in a fluid with vorticity
- Analytical investigation of wave absorption by a rotating black hole analogue
- Nonlinear evolution of the ergoregion instability: Turbulence, bursts of radiation, and black hole formation