Rahul Sharma (Editor)

Similarity solution

Updated on
Edit
Like
Comment
Share on FacebookTweet on TwitterShare on LinkedInShare on Reddit

In study of partial differential equations, particularly fluid dynamics, a similarity solution is a form of solution in which at least one co-ordinate lacks a distinguished origin; more physically, it describes a flow which 'looks the same' either at all times, or at all length scales. These include, for example, the Blasius boundary layer or the Sedov-Taylor shell.

Contents

Concept

A powerful tool in physics is the concept of dimensional analysis and scaling laws; by looking at the physical effects present in a system we may estimate their size and hence which, for example, might be neglected. If we have catalogued these effects we will occasionally find that the system has not fixed a natural lengthscale (timescale), but that the solution depends on space (time). It is then necessary to construct a lengthscale (timescale) using space (time) and the other dimensional quantities present - such as the viscosity ν . These constructs are not 'guessed' but are derived immediately from the scaling of the governing equations.

Example - The impulsively started plate

Consider a semi-infinite domain bounded by a rigid wall and filled with viscous fluid. At time t = 0 the wall is made to move with constant speed U in a fixed direction (for definiteness, say the x direction and consider only the x y plane). We can see that there is no distinguished length scale given in the problem, and we have the boundary conditions of no slip

u = U on y = 0

and that the plate has no effect on the fluid at infinity

u 0 as y .

Now, if we examine the Navier-Stokes equations

ρ ( u t + u u ) = p + μ 2 u

we can observe that this flow will be rectilinear, with gradients in the y direction and flow in the x direction, and that the pressure term will have no tangential component so that p y = 0 . The x component of the Navier-Stokes equations then becomes

u t = ν y 2 u

and we may apply scaling arguments to show that

U t ν U y 2

which gives us the scaling of the y co-ordinate as

y ( ν t ) 1 / 2 .

This allows us to pose a self-similar ansatz such that, with f and η dimensionless,

u = U f ( η y ( ν t ) 1 / 2 )

We have now extracted all of the relevant physics and need only solve the equations; for many cases this will need to be done numerically. This equation is

η f / 2 = f

with solution satisfying the boundary conditions that

f = 1 erf ( η / 2 ) or u = U ( 1 erf ( y / ( 4 ν t ) 1 / 2 ) )

which is a self-similar solution of the first kind.

References

Similarity solution Wikipedia