# Taylor–Couette flow – Wikipedia

In fluid dynamics, the **Taylor–Couette flow** consists of a viscous fluid confined in the gap between two rotating cylinders. For low angular velocities, measured by the Reynolds number *Re*, the flow is steady and purely azimuthal. This basic state is known as circular Couette flow, after Maurice Marie Alfred Couette, who used this experimental device as a means to measure viscosity. Sir Geoffrey Ingram Taylor investigated the stability of Couette flow in a ground-breaking paper.^{[1]} Taylor’s paper became a cornerstone in the development of hydrodynamic stability theory and demonstrated that the no-slip condition, which was in dispute by the scientific community at the time, was the correct boundary condition for viscous flows at a solid boundary.

Taylor showed that when the angular velocity of the inner cylinder is increased above a certain threshold, Couette flow becomes unstable and a secondary steady state characterized by axisymmetric toroidal vortices, known as **Taylor vortex** flow, emerges. Subsequently, upon increasing the angular speed of the cylinder the system undergoes a progression of instabilities which lead to states with greater spatio-temporal complexity, with the next state being called **wavy vortex flow**. If the two cylinders rotate in opposite sense then **spiral vortex flow ** arises. Beyond a certain Reynolds number there is the onset of turbulence.

Circular Couette flow has wide applications ranging from desalination to magnetohydrodynamics and also in viscosimetric analysis. Different flow regimes have been categorized over the years including twisted Taylor vortices and wavy outflow boundaries. It has been a well researched and documented flow in fluid dynamics.^{[2]}

## Flow description[edit]

A simple Taylor–Couette flow is a steady flow created between two rotating infinitely long coaxial cylinders.^{[3]} Since the cylinder lengths are infinitely long, the flow is essentially unidirectional in steady state. If the inner cylinder with radius

is rotating at constant angular velocity

${displaystyle Omega _{1}}$and the outer cylinder with radius

${displaystyle R_{2}}$is rotating at constant angular velocity

${displaystyle Omega _{2}}$ as shown in figure, then the azimuthal velocity component is given by^{[4]}

where

## Rayleigh’s criterion^{[5]}[edit]

Lord Rayleigh^{[6]}^{[7]} studied the stability of the problem with inviscid assumption i.e., perturbing Euler equations. The criterion states that *in the absence of viscosity the necessary and sufficient condition for distribution of azimuthal velocity *

*${displaystyle v_{theta }(r)}$*

* to be stable is*

*everywhere in the interval; and, further, that the distribution is unstable if *

*${displaystyle (rv_{theta })^{2}}$*

* should decrease anywhere in the interval.* Since

represents angular momentum per unit mass, of a fluid element about the axis of rotation, an alternative way of stating the criterion is: *a stratification of angular momentum about an axis is stable if and if only it increases monotonically outward.*

## Taylor vortex[edit]

Taylor vortices (also named after Sir Geoffrey Ingram Taylor) are vortices formed in rotating Taylor–Couette flow when the Taylor number (

${displaystyle mathrm {Ta} }$) of the flow exceeds a critical value

${displaystyle mathrm {Ta_{c}} }$.

For flow in which

instabilities in the flow are not present, i.e. perturbations to the flow are damped out by viscous forces, and the flow is steady. But, as the

${displaystyle mathrm {Ta} }$exceeds

${displaystyle mathrm {Ta_{c}} }$, axisymmetric instabilities appear. The nature of these instabilities is that of an exchange of stabilities (rather than an overstability), and the result is not turbulence but rather a stable secondary flow pattern that emerges in which large toroidal vortices form in flow, stacked one on top of the other. These are the Taylor vortices. While the fluid mechanics of the original flow are unsteady when

${displaystyle mathrm {Ta} >mathrm {Ta_{c}} }$${displaystyle mu }$

,

${displaystyle eta }$, and

${displaystyle mathrm {Ta} }$. As

${displaystyle eta rightarrow 1}$and

${displaystyle mu rightarrow 0}$from below, the critical Taylor number is

${displaystyle mathrm {Ta_{c}} simeq 1708}$^{[4]}^{[8]}^{[9]}^{[10]}^{[11]}

## Gollub–Swinney circular Couette experiment[edit]

In 1975, J. P. Gollub and H. L. Swinney published a paper on the onset of turbulence in rotating fluid. In a Taylor–Couette flow system, they observed that, as the rotation rate increases, the fluid stratifies into a pile of “fluid donuts”. With further increases in the rotation rate, the donuts oscillate and twist and finally become turbulent.^{[12]} Their study helped establish the Ruelle–Takens scenario in turbulence,^{[13]} which is an important contribution by Floris Takens and David Ruelle towards understanding how hydrodynamic systems transition from stable flow patterns into turbulent. While the principal, governing factor for this transition is the Reynolds number, there are other important influencing factors: if the flow is open (meaning there is a lateral up- and downstream) or closed (flow is laterally bound; e.g. rotating), and bounded (influenced by wall effects) or unbounded (not influenced by wall effects). According to this classification the Taylor–Couette flow is an example of a flow pattern forming in a closed, bounded flow system.

## References[edit]

**^**Taylor, Geoffrey I. (1923). “Stability of a viscous liquid contained between two rotating cylinders”.*Philosophical Transactions of the Royal Society of London*. Series A, Containing Papers of a Mathematical or Physical Character.**223**(605–615): 289–343. Bibcode:1923RSPTA.223..289T. doi:10.1098/rsta.1923.0008. JSTOR 91148.**^**Andereck, C.D.; Liu, S.S.; Swinney, H.L. (1986). “Flow regimes in a circular Couette system with independently rotating cylinders”.*Journal of Fluid Mechanics*.**164**: 155–183. Bibcode:1986JFM…164..155A. doi:10.1017/S0022112086002513.**^**Drazin, Philip G.; Reid, William Hill (2004).*Hydrodynamic Stability*. Cambridge University Press. ISBN 978-0-521-52541-1.- ^
^{a}^{b}Davey (1962). “The growth of Taylor vortices in flow between rotating cylinders”.*Journal of Fluid Mechanics*.**14**(3): 336–368. doi:10.1017/S0022112062001287. **^**Chandrasekhar, Subrahmanyan. Hydrodynamic and hydromagnetic stability. Courier Corporation, 2013.**^**Rayleigh, Lord. “On the stability or instability of certain fluid motions. Scientific Papers, 3.” (1880): 594-596.**^**Rayleigh, Lord. “On the dynamics of revolving fluids.” Proceedings of the Royal Society of London. Series A, Containing Papers of a Mathematical and Physical Character 93.648 (1917): 148-154.**^**Weisberg, A. Y.; Kevrekidis, I. G.; Smits, A. J. (1997). “Delaying Transition in Taylor–Couette Flow with Axial Motion of the Inner Cylinder”.*Journal of Fluid Mechanics*.**348**: 141–151. doi:10.1017/S0022112097006630.**^**Takeda, Y. (1999). “Quasi-Periodic State and Transition to Turbulence in a Rotating Couette System”.*Journal of Fluid Mechanics*.**389**(1): 81–99. Bibcode:1999JFM…389…81T. doi:10.1017/S0022112099005091.**^**Wereley, S. T.; Lueptow, R. M. (1999). “Velocity field for Taylor–Couette flow with an axial flow”.*Physics of Fluids*.**11**(12): 3637–3649. Bibcode:1999PhFl…11.3637W. doi:10.1063/1.870228.**^**Marques, F.; Lopez, J. M.; Shen, J. (2001). “A Periodically Forced Flow Displaying Symmetry Breaking Via a Three-Tori Gluing Bifurcation and Two-Tori Resonances”.*Physica D: Nonlinear Phenomena*.**156**(1–2): 81–97. Bibcode:2001PhyD..156…81M. CiteSeerX 10.1.1.23.8712. doi:10.1016/S0167-2789(01)00261-5.**^**Gollub, J. P.; Swinney, H. L. (1975). “Onset of turbulence in a rotating fluid”.*Physical Review Letters*.**35**(14): 927–930. Bibcode:1975PhRvL..35..927G. doi:10.1103/PhysRevLett.35.927.**^**Guckenheimer, John (1983). “Strange attractors in fluid dynamics”.*Dynamical System and Chaos*. Lecture Notes in Physics. Vol. 179. Springer Berlin. pp. 149–156. doi:10.1007/3-540-12276-1_10. ISBN 978-3-540-12276-0.

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