In fluid dynamics, Rayleigh problem also known as Stokes first problem is a problem of determining the flow created by a sudden movement of an infinitely long plate from rest, named after Lord Rayleigh and Sir George Stokes. This is considered as one of the simplest unsteady problems that have an exact solution for the Navier-Stokes equations. The impulse movement of semi-infinite plate was studied by Keith Stewartson.[1]
Consider an infinitely long plate which is suddenly made to move with constant velocity
U
x
y=0
\partialu | |
\partialt |
=\nu
\partial2u | |
\partialy2 |
where
\nu
u(y,0)=0, u(0,t>0)=U, u(infty,t>0)=0,
the last condition is due to the fact that the motion at
y=0
The problem on the whole is similar to the one dimensional heat conduction problem. Hence a self-similar variable can be introduced[4]
η=
y | |
\sqrt{\nut |
Substituting this the partial differential equation, reduces it to ordinary differential equation
f''+
1 | |
2 |
ηf'=0
with boundary conditions
f(0)=1, f(infty)=0
The solution to the above problem can be written in terms of complementary error function
u=Uerfc\left(
y | |
\sqrt{4\nut |
The force per unit area exerted on the plate is
F=\mu\left(
\partialu | |
\partialy |
\right)y=0=-\rho\sqrt{
\nuU2 | |
\pit |
Instead of using a step boundary condition for the wall movement, the velocity of the wall can be prescribed as an arbitrary function of time, i.e.,
U=f(t)
u(y,t)=
t | |
\int | |
0 |
f(\tau) | |
2\sqrt{\pi\nu |
Consider an infinitely long cylinder of radius
a
t=0
\Omega
\theta
v\theta=
a\Omega | |
2\pii |
iinfty | |
\int | |
-iinfty |
K1(r\sqrt{s/\nu | |
)}{K |
st | |
1(a\sqrt{s/\nu})}e |
ds | |
s |
where
K1
t → infty
F=\mu\left(
\partialv\theta | - | |
\partialr |
v\theta | |
r |
\right)r=a=
\rhoa2\Omega | |
t |
| ||||
e |
I | ||||
|
\right)-2\mu\Omega
where
I0
Exact solution is also available when the cylinder starts to slide in the axial direction with constant velocity
U
x
u=
U | |
2\pii |
iinfty | |
\int | |
-iinfty |
K0(r\sqrt{s/\nu | |
)}{K |
st | |
0(a\sqrt{s/\nu})}e |
ds | |
s |
.