Physics:Couette flow

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Short description: Model of viscous fluid flow between two surfaces moving relative to each other

In fluid dynamics, Couette flow is the flow of a viscous fluid in the space between two surfaces, one of which is moving tangentially relative to the other. The relative motion of the surfaces imposes a shear stress on the fluid and induces flow. Depending on the definition of the term, there may also be an applied pressure gradient in the flow direction.

The Couette configuration models certain practical problems, like the Earth's mantle and atmosphere,[1] and flow in lightly loaded journal bearings. It is also employed in viscometry and to demonstrate approximations of reversibility.[2][3]

It is named after Maurice Couette, a Professor of Physics at the French University of Angers in the late 19th century.

Planar Couette flow

Simple Couette configuration using two infinite flat plates.

Couette flow is frequently used in undergraduate physics and engineering courses to illustrate shear-driven fluid motion. A simple configuration corresponds to two infinite, parallel plates separated by a distance h; one plate translates with a constant relative velocity U in its own plane. Neglecting pressure gradients, the Navier–Stokes equations simplify to

d2udy2=0,

where y is the spatial coordinate normal to the plates and u(y) is the velocity field. This equation reflects the assumption that the flow is unidirectional — that is, only one of the three velocity components (u,v,w) is non-trivial. If the lower plate corresponds to y=0, the boundary conditions are u(0)=0 and u(h)=U. The exact solution

u(y)=Uyh

can be found by integrating twice and solving for the constants using the boundary conditions. A notable aspect of the flow is that shear stress is constant throughout the domain. In particular, the first derivative of the velocity, U/h, is constant. According to Newton's Law of Viscosity (Newtonian fluid), the shear stress is the product of this expression and the (constant) fluid viscosity.

Startup

Startup Couette flow

In reality, the Couette solution is not reached instantaneously. The "startup problem" describing the approach to steady state is given by

ut=ν2uy2

subject to the initial condition

u(y,0)=0,0<y<h,

and with the same boundary conditions as the steady flow:

u(0,t)=0,u(h,t)=U,t>0.

The problem can be made homogeneous by subtracting the steady solution. Then, applying separation of variables leads to the solution:[4]

u(y,t)=Uyh2Uπn=11nen2π2νth2sin[nπ(1yh)].

The timescale describing relaxation to steady state is th2/ν, as illustrated in the figure. The time required to reach the steady state depends only on the spacing between the plates h and the kinematic viscosity of the fluid, but not on U.

Planar flow with pressure gradient

A more general Couette flow includes a constant pressure gradient G=dp/dx=constant in a direction parallel to the plates. The Navier–Stokes equations are

d2udy2=Gμ,

where μ is the dynamic viscosity. Integrating the above equation twice and applying the boundary conditions (same as in the case of Couette flow without pressure gradient) gives

u(y)=G2μy(hy)+Uyh.

The pressure gradient can be positive (adverse pressure gradient) or negative (favorable pressure gradient). In the limiting case of stationary plates (U=0), the flow is referred to as Plane Poiseuille flow, and has a symmetric (with reference to the horizontal mid-plane) parabolic velocity profile.[5]

Compressible flow

Compressible Couette flow for M=0
Compressible Couette flow for M2Pr=7.5

In incompressible flow, the velocity profile is linear because the fluid temperature is constant. When the upper and lower walls are maintained at different temperatures, the velocity profile is more complicated. However, it has an exact implicit solution as shown by C. R. Illingworth in 1950.[6]

Consider the plane Couette flow with lower wall at rest and the upper wall in motion with constant velocity U. Denote fluid properties at the lower wall with subscript w and properties at the upper wall with subscript . The properties and the pressure at the upper wall are prescribed and taken as reference quantities. Let l be the distance between the two walls. The boundary conditions are

u=0, v=0, h=hw=cpwTw at y=0,
u=U, v=0, h=h=cpT, p=p at y=l

where h is the specific enthalpy and cp is the specific heat. Conservation of mass and y-momentum requires v=0, p=p everywhere in the flow domain. Conservation of energy and x-momentum reduce to

ddy(μdudy)=0,dτdy=0,τ=τw
1Prddy(μdhdy)+μ(dudy)2=0.

where τ=τw=constant is the wall shear stress. The flow does not depend on the Reynolds number Re=Ul/ν, but rather on the Prandtl number Pr=μcp/κ and the Mach number M=U/c=U/(γ1)h, where κ is the thermal conductivity, c is the speed of sound and γ is the specific heat ratio. Introduce the non-dimensional variables

y~=yl,T~=TT,T~w=TwT,h~=hh,h~w=hwh,u~=uU,μ~=μμ,τ~w=τwμU/l

In terms of these quantities, the solutions are

h~=h~w+[γ12M2Pr+(1h~w)]u~γ12M2Pru~2,
y~=1τ~w0u~μ~du~,τ~w=01μ~du~,qw=1Prτw(dhdu)w,

where qw is the heat transferred per unit time per unit area from the lower wall. Thus h~,T~,u~,μ~ are implicit functions of y. One can also write the solution in terms of the recovery temperature Tr and recovery enthalpy hr evaluated at the temperature of an insulated wall i.e., the values of Tw and hw for which qw=0.[clarification needed] Then the solution is

qwτwU=T~wT~r(γ1)M2Pr,T~r=1+γ12M2Pr,
h~=h~w+(h~rh~w)u~γ12M2Pru~2.

If the specific heat is constant, then h~=T~. When M0 and Tw=T,qw=0, then T and μ are constant everywhere, thus recovering the incompressible Couette flow solution. Otherwise, one must know the full temperature dependence of μ~(T~). While there is no simple expression for μ~(T~) that is both accurate and general, there are several approximations for certain materials — see, e.g., temperature dependence of viscosity. When M0 and qw0, the recovery quantities become unity T~r=1. For air, the values γ=1.4, μ~(T~)=T~2/3 are commonly used, and the results for this case are shown in the figure.

The effects of dissociation and ionization (i.e., cp is not constant) have also been studied; in that case the recovery temperature is reduced by the dissociation of molecules.[7]

Rectangular channel

Couette flow for square channel
Couette flow with h/l=0.1

One-dimensional flow u(y) is valid when both plates are infinitely long in the streamwise (x) and spanwise (z) directions. When the spanwise length is finite, the flow becomes two-dimensional and u is a function of both y and z. However, the infinite length in the streamwise direction must be retained in order to ensure the unidirectional nature of the flow.

As an example, consider an infinitely long rectangular channel with transverse height h and spanwise width l, subject to the condition that the top wall moves with a constant velocity U. Without an imposed pressure gradient, the Navier–Stokes equations reduce to

2uy2+2uz2=0

with boundary conditions

u(0,z)=0,u(h,z)=U,
u(y,0)=0,u(y,l)=0.

Using separation of variables, the solution is given by

u(y,z)=4Uπn=112n1sinh(βny)sinh(βnh)sin(βnz),βn=(2n1)πl.

When h/l1, the planar Couette flow is recovered, as shown in the figure.

Coaxial cylinders

Taylor–Couette flow is a flow between two rotating, infinitely long, coaxial cylinders.[8] The original problem was solved by Stokes in 1845,[9] but Geoffrey Ingram Taylor's name was attached to the flow because he studied its stability in a famous 1923 paper.[10]

The problem can be solved in cylindrical coordinates (r,θ,z). Denote the radii of the inner and outer cylinders as R1 and R2. Assuming the cylinders rotate at constant angular velocities Ω1 and Ω2, then the velocity in the θ-direction is[11]

vθ(r)=ar+br,a=Ω2R22Ω1R12R22R12,b=(Ω1Ω2)R12R22R22R12.

This equation shows that the effects of curvature no longer allow for constant shear in the flow domain.

Coaxial cylinders of finite length

The classical Taylor–Couette flow problem assumes infinitely long cylinders; if the cylinders have non-negligible finite length l, then the analysis must be modified (though the flow is still unidirectional). For Ω2=0, the finite-length problem can be solved using separation of variables or integral transforms, giving:[12]

vθ(r,z)=4R1Ω1πn=112n1I1(βnR2)K1(βnr)K1(βnR2)I1(βnr)I1(βnR2)K1(βnR1)K1(βnR2)I1(βnR1)sin(βnz),βn=(2n1)πl,

where I(βnr), K(βnr) are the Modified Bessel functions of the first and second kind.

See also

References

  1. Zhilenko et al. (2018)
  2. Guyon et al. (2001), p. 136
  3. Heller (1960)
  4. Pozrikidis (2011), pp. 338–339
  5. Kundu et al. (2016), p. 415
  6. Lagerstrom (1996)
  7. Liepmann et al. (1956, 1957)
  8. Landau and Lifshitz (1987)
  9. Stokes (1845)
  10. Taylor (1923)
  11. Guyon et al. (2001), pp. 163–166
  12. Wendl (1999)

Sources