
958 XIII Steady Navier–Stokes Flow in Domains with Unbounded Boundaries
XIII.9 Asymptotic Structure of Gener alize d Solutions
for Flow in an Aperture Domain
Using the results on the Stokes problem in the half-space as given in Theorem
IV.3. 2 and Theorem IV.3.3, it is a straightforward exercise to show that every
generalized solution to problem (XIII.5.2) satisfies the following asymptotic
properties
lim
|x|→∞
D
α
v(x) = 0
lim
|x|→∞,x∈R
3
±
D
α
(p(x) − p
±
) = 0,
(XIII.9.1)
for all |α| ≥ 0; cf. Exercise XIII.9.1. However, nothing can be said ab out the
order of decay, unless we put some suitable restriction on the magnitude of
the flux Φ of the velocity field through the aperture S. Actually, under the
hyp othesis of Theorem XIII.7.4, it is a relatively simple task to determine
the precise asymptotic structure of a ny corresponding generalized sol ution
v and of the associated pressure field p. In showing this, we shall follow an
approach entirely analogous to that employed in similar circumstances for flow
in exterior domains; cf. Section X.8 and X. 6.
First of all, we need a representation for v. By Theorem XI II.7.4, any
generalized solution corresponding to “small” Φ satisfies the condition
v
l
v
i
∈ L
2
(Ω), l, i = 1, 2, 3,
and so, by Lemma VI.5.1 , it follows that for all x ∈ R
3
±
v(x) admits the
representation
v
j
(x) = −
1
ν
Z
R
3
±
D
l
G
±
ij
(x, y)v
l
(y)v
i
(y)dy
−
Z
S
[v
i
(y)T
il
(G
±
j
, g
±
j
)(x, y)n
l
(y)dσ
y
,
(XIII.9.2)
where G
±
is the Green’s tensor for the Stokes problem in R
3
±
and g
±
is the
associated “pressure” field. Relation (XI II.9.2) is the starting point of our
asymptotic analysis. Since what we shall say equally applies to R
3
+
and R
3
−
,
to fix the i deas we shall deal with R
3
+
. Setting, for simplicity, G
+
= G and
g
+
= g, we begin to notice that from (XIII.9.2) we derive, in particular, for
all x ∈ R
3
+
v
j
(x) = −
1
ν
Z
R
3
+
D
l
G
ij
(x, y)v
l
(y)v
i
(y)dy + T
i3
(G
j
, g
j
)(x, 0)
Z
S
v
i
(y)dσ
y
−
Z
S
[T
il
(G
j
, g
j
)(x, y) −T
il
(G
j
, g
j
)(x, 0)] v
i
(y)n
l
(y)dσ
y
.