118 5. THE RICCI FLOW ON SURFACES
Since R (x, t) :::; p (t) :::; 0, this is possible only if
IRc-~gl2 = 0
at ( x, t). Tracing then implies that
Rmin ( t) = R ( X, t) = p ( t) ,
hence that R = r is constant in space. Substituting back into (5.16), we
conclude that
Rc(·,t) = p(t)g(·,t)
n
holds identically, hence that g (t) is Einstein. D
4.2. Surface solitons and the Kazdan-Warner identity. Now we
prove the main assertion of this section. Since the argument uses a partic-
ular formulation of the Kazdan- Warner identity [82], we follow it with a
discussion of that result.
PROPOSITION 5.21. If (M^2 ,g (t)) is a self-similar solution of the nor-
malized Ricci flow on a Riemannian surface, then g(t) = g(O) is a metric of
constant curvature.
PROOF. By Proposition 5.20, we may assume that r > 0. By passing to
a cover space if necessary, we may thus assume that M^2 is diffeomorphic to
52. Contracting the Ricci soliton equation (5.6) by Rg-^1 yields
2R (r - R) = 2Rdiv X,
and hence
- f (R-r)^2 dA= f R(r- R)dA= f RdivXdA.
Js2 Js2 ls2
Since X is a conformal Killing vector field, integrating by parts and applying
the Kazdan-Warner identity (5.18) implies that
f (R - r)^2 dA = f (\7 R, X) dA = 0.
Js2 Js2
Hence R = r, and the proposition is proved. D
We begin our discussion of the Kazdan- Warner identity by stating its
usual formulation. (See for example page 195 of [113].) Let g be an arbitrary
metric on a topological 52. We shall denote the standard round metric on
52 by g and will use bars to indicate geometric quantities associated to g.
Let t.p be a first eigenfunction of the rough Laplacian ~ on 52. (In other
words, cp is a spherical harmonic.) By the Uniformization Theorem, one may
write g = e^2 ug. Then one can write the standard Kazdan- Warner identity
in the form
(5.17)