Evanescent and inertial-like waves in rigidly-rotating odd viscous liquids
E.Kirkinis, M. Olvera de la Cruz

TL;DR
This paper investigates the behavior of inertial-like waves in rigidly rotating odd viscous liquids, revealing new wave types, their classification, and potential experimental methods to measure odd viscosity coefficients.
Contribution
It introduces the existence of non-axisymmetric, evanescent, and mixed inertial-like waves in rotating odd viscous liquids, expanding understanding beyond non-rotating cases.
Findings
Identification of non-axisymmetric inertial-like waves in rotating odd viscous liquids.
Classification of waves based on pairs of complex or real wavenumbers.
Proposal of experimental methods to determine odd viscosity coefficients.
Abstract
Three-dimensional non-rotating odd viscous liquids give rise to Taylor columns and support {axisymmetric} inertial-like waves [\emph{J. Fluid Mech.}, vol. {973}, A30, (2023)]. When an odd viscous liquid is subjected to rigid-body rotation however, there arise in addition a plethora of other phenomena that need to be clarified. In this paper we show that three-dimensional incompressible or two-dimensional compressible odd viscous liquids, rotating rigidly with angular velocity , give rise to both oscillatory and evanescent inertial-like waves or a combination thereof (which we call of mixed type), that can be \emph{non-axisymmetric}. By evanescent we mean that along the radial direction, typically when moving away from a solid boundary, the velocity field decreases exponentially. These waves precess in a prograde or retrograde manner with respect to the rotating frame. The…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsGeomagnetism and Paleomagnetism Studies · Solar and Space Plasma Dynamics · Astro and Planetary Science
