My watch list

Stokes flow

Stokes flow (named after George Gabriel Stokes) is a type of fluid flow where inertial forces are small compared with viscous forces. The Reynolds number is low, i.e. $\textit{Re} \ll 1$ . This is a typical situation in flows where the fluid velocities are very slow, the viscosities are very large, or the length-scales of the flow are very small, such as in MEMS devices or in the flow of viscous polymers.

Additional recommended knowledge

Recognize and detect the effects of electrostatic charges on your balance

Correct Test Weight Handling Guide: 12 Practical Tips

How to ensure accurate weighing results every day?

1 Stokes equations
- 1.1 Properties
- 1.2 Methods of solution
2 See also
3 References

Stokes equations

For this type of flow, the inertial forces are assumed to be negligible and the Navier-Stokes equations simplify to give the Stokes equations:

$\boldsymbol{\nabla} \cdot \mathbb{P} + \boldsymbol{f} = 0$

where $\mathbb{P}$ is the comoving stress tensor, and $\boldsymbol{f}$ an applied body force. There is also an equation for conservation of mass. In the common case of an incompressible Newtonian fluid, the Stokes equations are:

$\boldsymbol{\nabla}p = \mu \nabla^2 \boldsymbol{u} + \boldsymbol{f}$

$\boldsymbol{\nabla}\cdot\boldsymbol{u}=0$

Properties

The Stokes Equations represent a considerable simplification of the full Navier-Stokes Equations, especially in the incompressible Newtonian case.

Instantaneity: A Stokes flow has no dependence on time other than through time-dependent boundary conditions. This means that, given the boundary conditions of a Stokes flow, the flow can be found without knowledge of the flow at any other time.

Time-reversibility: An immediate consequence of instantaneity, time-reversibility means then a time-reversed Stokes flow solves the same equations as the original Stokes flow. This property can sometimes be used (in conjunction with linearity and symmetry in the boundary conditions) to derive results about a flow without solving it fully.

While these properties are true for incompressible Newtonian Stokes flows, the non-linear and sometimes time-dependent nature of Non-Newtonian fluids means that they do not hold in the more general case.

Methods of solution

By streamfunction

It can be shown that in 2-D, the streamfunction for an incompressible Newtonian Stokes flow satisfies the Biharmonic Equation $\nabla^4 \psi = 0$ .

In the 3-D axisymmetric case, the streamfunction $Ψ$ solves the equation $E 2 Ψ = 0$ , where $E = {\partial^2 \over \partial r^2} + {\sin{\theta} \over r^2} {\partial \over \partial \theta} { 1 \over \sin{\theta}} {\partial \over \partial \theta}.$

By Papkovich-Neuber solution

The Papkovich-Neuber Solution represents the velocity and pressure fields of an incompressible Newtonian Stokes flow in terms of two harmonic potentials.

By Boundary element method

Certain problems, such as the evolution of the shape of a bubble in a Stokes flow, are conducive to numerical solution by the Boundary Element method. This technique can be applied in both 2- and 3-dimensional flows.

By Green's function

The linearity of the Stokes equations in the case of an incompressible Newtonian fluid means that a Green's function for the equations can be found. The solution for the pressure $p$ and velocity $\boldsymbol{u}$ due to a point force $\boldsymbol{F}\delta(\boldsymbol{x})$ acting at the origin with $|\boldsymbol{u}|,p\to 0$ as $|\boldsymbol{x}|\to\infty$ is given by

$\boldsymbol{u}(\boldsymbol{x}) = \boldsymbol{F} \cdot \mathbb{J}(\boldsymbol{x})$

$p(\boldsymbol{x}) = \frac{\boldsymbol{F}\cdot\boldsymbol{x}}{4 \pi |\boldsymbol{x}|^3}$

where

$\mathbb{J}(\boldsymbol{x}) = {1 \over 8 \pi \mu} \left( \frac{\mathbb{I}}{|\boldsymbol{x}|} + \frac{\boldsymbol{x}\boldsymbol{x}}{|\boldsymbol{x}|^3} \right).$

is a second-rank tensor known as the Oseen Tensor (after Carl Wilhelm Oseen).

The solution for a distributed force density $\boldsymbol{f}(\boldsymbol{x})$ (again with decay at infinity) can then be constructed by superposition:

$\boldsymbol{u}(\boldsymbol{x}) = \int \boldsymbol{f}(\boldsymbol{y}) \cdot \mathbb{J}(\boldsymbol{x} - \boldsymbol{y}) \, \mathrm{d}^3\!y$

$p(\boldsymbol{x}) = \int \frac{\boldsymbol{f}(\boldsymbol{y})\cdot(\boldsymbol{x}-\boldsymbol{y})}{4 \pi |\boldsymbol{x}-\boldsymbol{y}|^3} \, \mathrm{d}^3\!y$

References

Happel, J. & Brenner, H. (1981) Low Reynolds Number Hydrodynamics, Springer. ISBN 9001371159.
Kim, S. & Karrila, S. J. (2005) Microhydrodynamics: Principles and Selected Applications, Dover. ISBN 0486442195.
Ockendon, H. & Ockendon J. R. (1995) Viscous Flow, Cambridge University Press. ISBN 0521458811.

Category: Fluid dynamics

This article is licensed under the GNU Free Documentation License. It uses material from the Wikipedia article "Stokes_flow". A list of authors is available in Wikipedia.