330 15. Nonlinear Parabolic Equations
M D 2,thenanyv 2 C
1
.M; N / is homotopic to a smooth harmonic map. If
dim M 3, there are nonsmooth harmonic maps, and there has been considerable
work on the nature of possible singularities. Details on matters mentioned in this
paragraph, and further references, can be found in [Hild, J1, Str, Str2]. We also
refer to [Ham] for extensions of Theorem 2.1 to cases where M and N have
boundary.
In case M and N are compact Riemann surfaces of genus 2 (endowed with
metrics of negative curvature, as done in 2 of Chap. 14), harmonic maps of de-
gree 1 are unique and are diffeomorphisms, as shown by R. Schoen and S.-T. Yau.
They measure well the degree to which M and N may fail to be conformally
equivalent, and they provide an excellent analytical tool for the study of Teich-
muller theory, replacing the more classical use of “quasi-conformal maps.” This
material is treated in [Tro].
We mention some other important geometrical results attacked via parabolic
equations. R. Hamilton [Ham2] obtained topological information on 3-manifolds
with positive Ricci curvature and in [Ham3] provided another approach to the
uniformization theorem for surfaces, an approach that works for the sphere as well
as for surfaces of higher genus; see also [Chow]. S. Donaldson [Don] constructed
Hermitian–Einstein metrics on stable bundles over compact algebraic surfaces;
see [Siu] for an exposition. Some facets of the Yamabe problem were treated via
the “Yamabe flow” in [Ye].
Hamilton’s Ricci flow equation
@g
@t
D2 Ric.g/
is a degenerate parabolic equation, but D. DeTurk [DeT] produced a strongly
parabolic modification, which fits into the framework of 7 of this chapter, giv-
ing short time solutions. Solutions typically develop singularities, and there has
been a lot of work on their behavior. Work of G. Perelman, [Per1]–[Per3], was
a tremendous breakthrough, greatly refining understanding of the Ricci flow and
using this to prove the Poincar´e Conjecture and Thurston’s Geometrization Con-
jecture, for compact 3-dimensional manifolds. This work has generated a large
additional body of work, quite a bit of it devoted to giving more digestible pre-
sentations of Perelman’s work. We refer to [CZ]and[MT] for such presentations,
and other references.
Exercises
For Exercises 1–3, choose local coordinates x near a point p 2 M and local coordi-
nates y near q D u.p/ 2 N . Then the energy density is given by
(2.26) e.t; x/ D
1
2
@u
@x
k
@u
@x
`
g
k`
.x/h
.u.t; x//;
where u.x/ D
u
1
.x/; ; u
n
.x/
in the y-coordinate system, n D dim N . Here,
g
k`
and h
define the metrics on M and N , respectively, and we use the summation