Exotic compact object behavior in black hole analogues
arXiv:1902.06748 · doi:10.1103/PhysRevD.99.084029
Abstract
Classical phenomenological aspects of acoustic perturbations on a draining bathtub geometry where a surface with reflectivity is set at a small distance from the would-be acoustic horizon, which is excised, are addressed. Like most exotic compact objects featuring an ergoregion but not a horizon, this model is prone to instabilities when . However, stability can be attained for sufficiently slow drains when . It is shown that the superradiant scattering of acoustic waves is more effective when their frequency approaches one of the system's quasi-normal mode frequencies.
12 pages, 6 figures. Accepted for publication as a Regular Article in Physical Review D
References in corpus (11)
- GW170814: A Three-Detector Observation of Gravitational Waves from a Binary Black Hole Coalescence
- GW170608: Observation of a 19-solar-mass Binary Black Hole Coalescence
- Light ring stability in ultra-compact objects
- Tests for the existence of horizons through gravitational wave echoes
- Fate of gravitational collapse in semiclassical gravity
- Ergoregion instability of ultra-compact astrophysical objects
- The Kerr Metric
- Instability of hyper-compact Kerr-like objects
- Detecting Rotational Superradiance in Fluid Laboratories
- Ultra-spinning exotic compact objects supporting static massless scalar field configurations
- Marginally stable resonant modes of the polytropic hydrodynamic vortex