15
An upper bound for A* can be constructed by means of the Green's function G(x,y)
for A +
A,
with Dirichlet boundary conditions
([17],
[10], [8]). Indeed this Green's function
can be decomposed in a regular and a singular part as follows:
G{x
'
y)
=
4^hv\
+h
*
{x
'
y)
-
In D C R
3
, the regular part h\(x, y) is continuous in D. By the maximum principle,
h\(x,y) satisfies the inequality : hy(x,y) < h\{x,y), for A' <
A
< A^ Hence the function
A
—>
max
x
h\(x,x) is increasing. Since max
D
h
0
(x,x) < 0 and max
D
hx(x,x) —> oo as
A
—>
Ai, there is a unique value v* such that max
x
h
v
*
(x, x) = 0. Schoen [17] has shown
that v* > A*. Based on numerical computations, Budd and Humphries [10] conjectured
that
v* =
A*.
(5)
If this conjecture were true, it would yield a remarkable connection between a quantity
arising in a linear problem and a nonlinear phenomenon.
Remark 2.3 As stated
before
in the Proposition 2.2 (Hi), the range of \-values for which
a minimizer exists is an interval
(X*,\x).
This doesn't exclude solutions of (3) for A ^
(A*,A!).
They correspond to higher energy levels. Examples will be given in the next
section.
The tool to establish nonexistence is Pohozaev's identity and its variants. It is obtained
by testing (3) with suitable functions. A different approach which leads to a better
understanding of the role of this identity in the calculus of variations is proposed by
Reichel [16].
3 Problems with critical exponents in spaces of con-
stant curvature
As an application of the previous section, we shall study the Brezis-Nirenberg problem in
spaces of constant curvature. This topic has been studied in several papers [7, 5, 6, 4].
The iV-dimensional spherical space S
w
is described by {x e R
N+1
: \x\ = 1}. The TV-
dimensional hyperbolic space M
N
is given by {x £ K
w+1
:
x
2
N+l
=
l +
Eili^
2
}-
We shall
restrict ourselves to the spherical case and refer to [18] for the discussion of the hyperbolic
space. The stereographic projection maps S
N
into R
N
, with the Riemannian metric given
by the line element ds = j^ =:
p\dx\,
x e K
w
.
The corresponding variational problem follows immediately from (4), if we replace V
by V/p and the volume element dx by
p
N
dx.
The Laplace-Beltrami operator assumes the
form A
p
= p
_N
div(p
JV_2
V). Hence the Brezis-Nirenberg problem for S^ reads as
p~
N
div(p
JV
"
2
Vu) + \u + u
2
'-
1
= 0, in D ; u = 0, on dD. (6)