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8.4 Boundary Conditions
The two types of boundaries considered in this topic are free surfaces
and solid walls, and each has particular conditions associated with
viscosity.
In the case of a free surface, things are fairly straightforward. On the
other side of the boundary there is a vacuum, or another fluid of much
smaller density whose effect we assume is negligible. Thus there is nothing
with which to transfer momentum: there can be no traction at the free
surface. In other words, the boundary condition for the stress at the free
surface is
σn =
pn + τ n =0 .
Note that if the viscous stress τ is zero, this reduces to p =0asbefore;
however, this becomes significantly more complex when τ isn't zero.
At solid walls, things are also a little more interesting. Physically speak-
ing once we model viscosity, it turns out the velocity field must be contin-
uous everywhere: if it weren't, viscous transfer of momentum would in the
next instant make it smooth again. This results in the so-called no-slip
boundary condition:
u = u solid ,
which of course simplifies to u = 0 at stationary solids. Recall that in the
inviscid case, only the normal component of velocities had to match: here
we are forcing the tangential components to match as well.
The no-slip condition has been experimentally verified to be more ac-
curate than the inviscid no-stick condition. However, the caveat is that in
many cases something called a boundary layer develops. Loosely speaking,
a boundary layer is a thin region next to a solid where the tangential ve-
locity rapidly changes from u solid at the solid wall to u at the other side of
the layer, where u is the velocity the inviscid no-stick boundary condition
( u
n ) would have given. That is, the effect of viscous drag
at the surface of the solid is restricted to a very small region next to the
solid, and can be ignored elsewhere. When we discretize the fluid flow on
a relatively coarse grid, that boundary layer may be much thinner than a
grid cell, and thus it's no longer a good idea to implement the no-slip con-
dition numerically—we would artificially be expanding the boundary layer
to at least a grid cell thick, which would be a much worse approximation
than going back to the inviscid no-stick boundary condition. In this case,
·
n = u solid
·
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