Taylor dispersion or Taylor diffusion is an apparent or effective diffusion of some scalar field arising on the large scale due to the presence of a strong, confined, zero-mean shear flow on the small scale. Essentially, the shear acts to smear out the concentration distribution in the direction of the flow, enhancing the rate at which it spreads in that direction.[1] [2] [3] The effect is named after the British fluid dynamicist G. I. Taylor, who described the shear-induced dispersion for large Peclet numbers. The analysis was later generalized by Rutherford Aris for arbitrary values of the Peclet number. The dispersion process is sometimes also referred to as the Taylor-Aris dispersion.
The canonical example is that of a simple diffusing species in uniformPoiseuille flow through a uniform circular pipe with no-fluxboundary conditions.
We use z as an axial coordinate and r as the radialcoordinate, and assume axisymmetry. The pipe has radius a, andthe fluid velocity is:
\boldsymbol{u}=w\hat{\boldsymbol{z}}=w0(1-r2/a2)\hat{\boldsymbol{z}}
The concentration of the diffusing species is denoted c and itsdiffusivity is D. The concentration is assumed to be governed bythe linear advection–diffusion equation:
\partialc | |
\partialt |
+\boldsymbol{w} ⋅ \boldsymbol{\nabla}c=D\nabla2c
The concentration and velocity are written as the sum of a cross-sectional average (indicated by an overbar) and a deviation (indicated by a prime), thus:
w(r)=\bar{w}+w'(r)
c(r,z)=\bar{c}(z)+c'(r,z)
Under some assumptions (see below), it is possible to derive an equation just involving the average quantities:
\partial\bar{c | |
Observe how the effective diffusivity multiplying the derivative on the right hand side is greater than the original value of diffusion coefficient, D. The effective diffusivity is often written as:
Deff=D\left(1+
Pe2 | |
48 |
\right),
Pe=a\bar{w}/D
a
In a frame moving with the mean velocity, i.e., by introducing
\xi=z-\barwt
\partial\bar{c | |
with diffusivity given by the effective diffusivity.
The assumption is that
c'\ll\bar{c}
z
z
r
L
z
L\gg
a2 | |
D |
\barw=aPe
Dispersion is also a function of channel geometry. An interesting phenomenon for example is that the dispersion of a flow between two infinite flat plates and a rectangular channel, which is infinitely thin, differs approximately 8.75 times. Here the very small side walls of the rectangular channel have an enormous influence on the dispersion.
While the exact formula will not hold in more general circumstances, the mechanism still applies, and the effect is stronger at higher Péclet numbers. Taylor dispersion is of particular relevance for flows in porous media modelled by Darcy's law.[4]
One may derive the Taylor equation using method of averages, first introduced by Aris. The result can also be derived from large-time asymptotics, which is more intuitively clear. In the dimensional coordinate system
(x',r',\theta)
u=2U[1-(r'/a)2]
a
U
c
t'=0
U
t= | t' |
a2/D |
, x=
x'-Ut' | |
a |
, r=
r' | |
a |
, Pe=
Ua | |
D |
where
a2/D
D
Pe
\partialc | |
\partialt |
+
| |||||
Pe(1-2r | = |
\partial2c | |
\partialx2 |
+
1 | |
r |
\partial | \left(r | |
\partialr |
\partialc | |
\partialr |
\right).
Thus in this moving frame, at times
t\sim1
t'\sima2/D
t\gg1
t'\gga2/D
x
t
Suppose
t\sim1/\epsilon\gg1
a2/D
\epsilon\ll1
x\sim\sqrtt\sim\sqrt{1/\epsilon}\gg1
\tau=\epsilont, \xi=\sqrt\epsilonx
can be introduced. The equation then becomes
\epsilon | \partialc |
\partial\tau |
+\sqrt\epsilon
| ||||
Pe(1-2r |
=\epsilon
\partial2c | |
\partial\xi2 |
+
1 | |
r |
\partial | \left(r | |
\partialr |
\partialc | |
\partialr |
\right).
If pipe walls do not absorb or react with the species, then the boundary condition
\partialc/\partialr=0
r=1
\partialc/\partialr=0
r=0
Since
\epsilon\ll1
c=c0+\sqrt\epsilonc1+\epsilonc2+ …
1 | |
r |
\partial | \left(r | |
\partialr |
\partialc0 | |
\partialr |
\right)=0.
Integrating this equation with boundary conditions defined before, one finds
c0=c0(\xi,\tau)
c0
c0
r
t'\gga2/D
Terms of order
\sqrt\epsilon
1 | |
r |
\partial | \left(r | |
\partialr |
\partialc1 | |
\partialr |
\right)=Pe
| ||||
(1-2r |
.
Integrating this equation with respect to
r
c1(\xi,r,\tau)=c1a(\xi,\tau)+
Pe | |
8 |
(2r2-r
| ||||
where
c1a
c1
r=0
Terms of order
\epsilon
1 | |
r |
\partial | \left(r | |
\partialr |
\partialc2 | |
\partialr |
\right)=Pe
| ||||
(1-2r |
+
\partialc0 | |
\partial\tau |
-
\partial2c0 | |
\partial\xi2 |
.
This equation can also be integrated with respect to
r
2rdr
r=0
r=1
\partialc0 | =\left(1+ | |
\partial\tau |
Pe2 | |
48 |
\right)
\partial2c0 | |
\partial\xi2 |
⇒
\partialc0 | =\left(1+ | |
\partialt |
Pe2 | |
48 |
\right)
\partial2c0 | |
\partialx2 |
.
This is the required diffusion equation. Going back to the laboratory frame and dimensional variables, the equation becomes
\partialc0 | |
\partialt' |
+U
\partialc0 | =D\left(1+ | |
\partialx' |
U2a2 | |
48D2 |
\right)
\partial2c0 | |
\partialx'2 |
.
By the way in which this equation is derived, it can be seen that this is valid for
t'\gga2/D
c0
x'\gga
x\sim\sqrt{Dt'})
t'\gga2/D
x'-Ut'=xs'-Ut'
x'-xs'\sima
r
c=c0+\sqrt{\epsilon}c1.
Integrating the equations obtained at the second order, we find
c2(\xi,\tau)=c2a(\xi,\tau)+
Pe | |
4 |
| ||||
\left(r |
\right)
\partialc1a | |
\partial\xi |
+
Pe2 | \left( | |
32 |
r2 | + | |
6 |
r4 | - | |
2 |
5r6 | + | |
8 |
r8 | |
8 |
\right)
| |||||||
\partial\xi2 |
where
c2a(\xi,\tau)
Now collecting terms of order
\epsilon\sqrt\epsilon
1 | |
r |
\partial | \left(r | |
\partialr |
\partialc3 | |
\partialr |
\right)=Pe
| ||||
(1-2r |
+
\partialc1 | |
\partial\tau |
-
\partial2c1 | |
\partial\xi2 |
.
The solvability condition of the above equation yields the governing equation for
c1a(\xi,\tau)
\partialc1a | -\left(1+ | |
\partial\tau |
Pe2 | |
48 |
\right)
\partial2c1a | |
\partial\xi2 |
=-
Pe3 | |
2880 |
| |||||||
\partial\xi3 |
.