Synchronized stationary clouds in a static fluid
Carolina L. Benone, Lu\'is C. B. Crispino, Carlos A. R. Herdeiro, and Maur\'icio Richartz

TL;DR
This paper demonstrates the theoretical existence of long-lived, synchronized stationary clouds of sound and surface waves in a static fluid with a rotating inner cylinder, offering potential for experimental observation.
Contribution
It introduces the concept of stationary clouds in hydrodynamics, showing they can exist in static fluids with rotating boundaries, extending analogies from black hole physics.
Findings
Stationary clouds can form in static fluids with rotating inner cylinders.
Synchronization between cylinder rotation and wave phase velocity is essential.
Potential for first experimental observation of hydrodynamic stationary clouds.
Abstract
The existence of stationary bound states for the hydrodynamic velocity field between two concentric cylinders is established. We argue that rotational motion, together with a trapping mechanism for the associated field, is sufficient to mitigate energy dissipation between the cylinders, thus allowing the existence of infinitely long lived modes, which we dub stationary clouds. We demonstrate the existence of such stationary clouds for sound and surface waves when the fluid is static and the internal cylinder rotates with constant angular velocity . These setups provide a unique opportunity for the first experimental observation of synchronized stationary clouds. As in the case of bosonic fields around rotating black holes and black hole analogues, the existence of these clouds relies on a synchronization condition between and the angular phase velocity of the cloud.
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