Instability driven by boundary inflow across shear: a way to circumvent Rayleigh’s stability criterion in accretion disks?
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Publication:2797058
DOI10.1017/jfm.2015.613zbMath1382.76111arXiv1504.08028OpenAlexW2964232104MaRDI QIDQ2797058
Publication date: 30 March 2016
Published in: Journal of Fluid Mechanics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1504.08028
Related Items (3)
Inviscid instability of an incompressible flow between rotating porous cylinders to three-dimensional perturbations ⋮ Linear and weakly nonlinear analyses of cylindrical Couette flow with axial and radial flows ⋮ On the stability of the Couette-Taylor flow between rotating porous cylinders with radial flow
Uses Software
Cites Work
- On the stability of plane Couette–Poiseuille flow with uniform crossflow
- Instability of a two-dimensional viscous flow in an annulus with permeable walls to two-dimensional perturbations
- Energy dissipation in a shear layer with suction
- On the hydrodynamic stability of channel flow with cross flow
- Destabilizing Taylor–Couette flow with suction
- Fluid Mechanics in Disks Around Young Stars
- NON-LINEAR INSTABILITY OF THE ASYMPTOTIC SUCTION VELOCITY PROFILE
- Flow through a diverging channel: instability and bifurcation
- Hydrodynamic stability of viscous flow between rotating porous cylinders with radial flow
- Instability of an inviscid flow between porous cylinders with radial flow
- Stability of Taylor–Couette flow in a finite-length cavity with radial throughflow
- Absolute and convective instability of cylindrical Couette flow with axial and radial flows
- Hydromagnetic stability of dissipative flow between rotating permeable cylinders
- Stability of Plane Couette-Poiseuille Flow with Uniform Crossflow
- Convective instability boundary of Couette flow between rotating porous cylinders with axial and radial flows
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