Stokes flow

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Stokes flow (named for George Stokes) is a type of flow where inertial forces are small as compared to viscous forces. The Reynolds number is low, i.e. \text{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.

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[edit] Stokes Equations

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

0 = \nabla \cdot \mathbb{P} + \rho\mathbf{f}

where \mathbb{P} is the comoving stress tensor. In the case of incompressible Newtonian fluids, the Stokes equations simplify to:

0 = - \nabla p + \mu \nabla^2 \mathbf{u} + \mathbf{f}
\nabla\cdot\mathbf{u}=0

[edit] Properties

The Stokes Equations represent a considerable simplification of the full Navier-Stokes Equations, especially in the incompressible Newtonian case. In this case, the equations are:

- Instantaneous: 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.

- Linear: The Stokes Equations are linear, which means that the response of a Stokes flow will be proportional to the forces applied to it. Linearity also allows superposition of solutions.

- Time-Reversible: An immidiate 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.

[edit] Methods of solution

[edit] 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 E2Ψ = 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}


[edit] 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.

[edit] 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.

[edit] 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. It is a second-rank tensor known as the Oseen Tensor, and takes the form:

\mathbb{J}(\mathbf{x}) = {1 \over 8 \pi \mu} ({\mathbb{I} \over r} + {\mathbf{x x} \over r^3})

The velocity and pressure fields \mathbf{u} and p are given in terms of the force applied the fluid \mathbf{F}( \mathbf{x} ) by:

\mathbf{u}(\mathbf{x}) = \mathbf{F} \cdot \mathbb{J}(\mathbf{x})
p(\mathbf{x}) = {\mathbf{F}\cdot\mathbf{x} \over 4 \pi r^3}
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