44 13. Function Space and Operator Theory for Nonlinear Analysis
Via the estimates used to prove Proposition 8.3, it follows that, for any given
s 2 R, q
.D/ 2 L
C
s
.R
n
/
has an operator norm that is a rapidly decreasing
function of . It is easy to establish the estimate
(8.20) ke
ix
uk
C
s
C.s/ hi
s
kuk
C
s
.s > 0/;
first for s … Z
C
, by using the characterization (8.1)ofC
s
D C
s
, then for general
s>0by interpolation. The desired operator bound on (8.18) follows easily.
To do the general case, one can use a partition of unity in the x-variables, of
the form
1 D
X
j 2Z
n
'
j
.x/; '
j
.x/ D '
0
.x C j/; '
0
2 C
1
0
.R
n
/;
and exploit the estimates on p
j
.x; D/u D '
j
.x/p.x; D/u obtained by the ar-
gument above, in concert with the rapid decrease of the Schwartz kernel of the
operator p.x; D/ away from the diagonal. Details are left to the reader.
In 9 we will establish a result that is somewhat stronger than Proposition 8.5,
but this relatively simple result is already useful for H¨older estimates on solutions
to linear, elliptic PDE.
It is useful to note that we can define Zygmund spaces C
s
.T
n
/ on the torus
just as in (8.6), but using Fourier series. We again have (8.7) and Propositions
8.3–8.5.
The issue of how Zygmund spaces form a complex interpolation scale is more
subtle than the analogous situation for L
p
-Sobolev spaces, treated in 6.Adiffer-
ent type of complex interpolation functor, ŒX; Y
b
, defined in Appendix A at the
end of this chapter, does a better job than ŒX; Y
. We have the following result
established in Appendix A.
Proposition 8.6. Fo r r; s 2 R;2 .0; 1/,
(8.21) ŒC
r
.T
n
/; C
s
.T
n
/
b
D C
sC.1/r
.T
n
/:
It is straightforward to extend the notions of H¨older and Zygmund spaces to
spaces C
s
.M / and C
s
.M / when M is a compact manifold without boundary.
Furthermore, the analogue of (8.14) is readily established, and we have
(8.22) P W C
s
.M / ! C
sm
.M / if P 2 OPS
m
1;0
.M /:
If
is a compact manifold with boundary, there is an obviousnotion of C
s
./,
for s 0. We will define C
s
./ below, for s 0. For now we look further at
C
s
./. The following simple observation is useful. Give a Riemannian metric
and let ı.x/ D dist.x; @/.