Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

Evanescent and inertial-like waves in rigidly rotating odd viscous liquids

Journal Article · · Journal of Fluid Mechanics
DOI:https://doi.org/10.1017/jfm.2024.791· OSTI ID:2877636
Three-dimensional non-rotating odd viscous liquids give rise to Taylor columns and support axisymmetric inertial-like waves (J. Fluid Mech., vol. 973, 2023, A30). 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 𝛺, give rise to both oscillatory and evanescent inertial-like waves or a combination thereof (which we call of mixed type) that can be 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 oscillatory and evanescent waves resemble respectively the body and wall-modes observed in (non-odd) rotating Rayleigh–Bénard convection (J. Fluid Mech., vol. 248, 1993, pp. 583–604). We show that the three types of waves (wall, body or mixed) can be classified with respect to pairs of planar wavenumbers 𝜅 which are complex, real or a combination, respectively. Experimentally, by observing the precession rate of the patterns, it would be possible to determine the largely unknown values of the odd viscosity coefficients. This formulation recovers as special cases recent studies of equatorial or topological waves in two-dimensional odd viscous liquids which provided examples of the bulk–interface correspondence at frequencies 𝜔 < 2⁢𝛺. We finally point out that the two- and three-dimensional problems are formally equivalent. Their difference then lies in the way data propagate along characteristic rays in three dimensions, which we demonstrate by classifying the resulting Poincaré–Cartan equations.
Research Organization:
Northwestern Univ., Evanston, IL (United States)
Sponsoring Organization:
USDOE Office of Science (SC); USDOE Office of Science (SC), Basic Energy Sciences (BES). Materials Sciences & Engineering Division (MSE)
Grant/Contract Number:
FG02-08ER46539
OSTI ID:
2877636
Alternate ID(s):
OSTI ID: 2577219
Journal Information:
Journal of Fluid Mechanics, Journal Name: Journal of Fluid Mechanics Vol. 996; ISSN 1469-7645; ISSN 0022-1120
Publisher:
Cambridge University PressCopyright Statement
Country of Publication:
United States
Language:
English

References (26)

Transverse momentum transport in polyatomic gases under the influence of a magnetic field journal November 1970
Wave focusing and ensuing mean flow due to symmetry breaking in rotating fluids journal June 2001
The rise of a body through a rotating fluid in a container of finite length journal March 1968
The flow created by a sphere moving along the axis of a rotating, slightly-viscous fluid journal February 1970
Convection in a rotating cylinder. Part 1 Linear theory for moderate Prandtl numbers journal March 1993
The influence of fast waves and fluctuations on the evolution of the dynamics on the slow manifold journal September 2014
A bulk-interface correspondence for equatorial waves journal April 2019
Robust wall states in rapidly rotating Rayleigh–Bénard convection journal May 2020
Stokes flows in three-dimensional fluids with odd and parity-violating viscosities journal January 2022
Evanescent inertial waves journal May 2021
Taylor columns and inertial-like waves in a three-dimensional odd viscous liquid journal October 2023
Odd Viscosity journal August 1998
Odd viscosity in chiral active fluids journal November 2017
The odd free surface flows of a colloidal chiral fluid journal September 2019
Taylor halos and Taylor spears in odd viscous liquids journal October 2023
Low Froude number limiting dynamics for stably stratified flow with small or finite Rossby numbers journal March 1998
Anisotropic odd viscosity via a time-modulated drive journal May 2020
Swimming at low Reynolds number in fluids with odd, or Hall, viscosity journal April 2014
Odd viscosity in two-dimensional incompressible fluids journal September 2017
Topological Waves in Fluids with Odd Viscosity journal March 2019
Odd Viscosity in Active Matter: Microscopic Origin and 3D Effects journal July 2021
Velocity-Vorticity Patterns in Turbulent Flow journal June 1985
Viscosity of Quantum Hall Fluids journal July 1995
Odd Viscosity and Odd Elasticity journal March 2023
Magnetic and Electric Effects on Transport Properties journal October 1970
Hopf Bifurcation with Broken Reflection Symmetry in Rotating Rayleigh-Bénard Convection journal June 1992

Similar Records

TIME EVOLUTION OF THE THREE-DIMENSIONAL ACCRETION FLOWS: EFFECTS OF THE ADIABATIC INDEX AND OUTER BOUNDARY CONDITION
Journal Article · Mon Nov 09 23:00:00 EST 2009 · Astrophysical Journal · OSTI ID:21378267

Inertial modes of rigidly rotating neutron stars in Cowling approximation
Journal Article · Sun Jun 15 00:00:00 EDT 2008 · Physical Review. D, Particles Fields · OSTI ID:21212029