1547671870-The_Ricci_Flow__Chow

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  1. NECKLIKE POINTS IN ANCIENT SOLUTIONS 271


On the other hand, if .A (T - t) 2: c, then μ^2 + v^2 > 8.\^2 and we have


d c 1 - c 8.\^2


  • log < c;,A - - -- < 0
    dt 2 (T - t) 2 .A+μ + v + p -


for c; > 0 small enough. D



  1. Necklike points in ancient solutions


The objective of this section is to show that an ancient solution of posi-
tive sectional curvature is either isometric to a spherical space form or else
contains points at arbitrarily ancient times where its geometry is arbitrarily
close to the product of a surface and a line. We begin with some general
observations about ancient solutions - including the fact that every ancient
solution (of any dimension) has nonnegative scalar curvature.


LEMMA 9.15. Let (Mn, g (t)) be a complete ancient solution of the Ricci
flow. Assume that Rmin (t) ~ infxEMn R (x, t) is finite for all t :S: 0 and that
there is a continuous function K (t) such that !sect [g (t)]I :S: K (t). Then
g (t) has nonnegative scalar curvature for as long as it exists.


PROOF. Recall that the parabolic maximum principle works on noncom-
pact as well as on compact rpanifolds. Recall also that

~~ = b.R + 2 IRcl


2
2: b.R + ~R

2
.

So if R ever becomes nonnegative, it remains so for as long as the solution

exists. On the other hand, if Rmin (t1) < 0, then Rmin (to) < 0 for all to :S: ti,


and one has
n n
Rmin (t) > 1 > ----


  • n (Rmin (to))- - 2 (t - to) - 2 (t - to)
    for all t > t 0. Since the solution is ancient, we may let to ""' - oo, obtaining


Rmin (t) 2: - lim ( n ) = 0.


to->- oo 2 t - to
D

REMARK 9.16. In dimension n = 3, we can strengthen this result, as we
proved in Corollary 9.8.

In Lemma 8.19, we derived a lower bound for the blow-up rate of so-
lutions that develop singularities in finite time. The analogous result for
ancient solutions is the following:

LEMMA 9.17. Let (Mn, g (t)) be an ancient solution with nonnegative
Ricci curvature. Then there exists a constant co > 0 depending only on n
such that
liminf ltl sup IRm (x, t)I 2: CO·
t->- oo xEMn
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