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Uniqueness of compact ancient solutions to the higher-dimensional Ricci flow

  • Simon Brendle , Panagiota Daskalopoulos , Keaton Naff ORCID logo EMAIL logo and Natasa Sesum
Published/Copyright: November 23, 2022

Abstract

In dimensions n 4 , an ancient κ-solution is a nonflat, complete, ancient solution of the Ricci flow that is uniformly PIC and weakly PIC2; has bounded curvature; and is κ-noncollapsed. In this paper, we study the classification of ancient κ-solutions to n-dimensional Ricci flow on S n , extending the result in [S. Brendle, P. Daskalopoulos and N. Sesum, Uniqueness of compact ancient solutions to three-dimensional Ricci flow, Invent. Math. 226 2021, 2, 579–651] to higher dimensions. We prove that such a solution is either isometric to a family of shrinking round spheres, or the Type II ancient solution constructed by Perelman.

Award Identifier / Grant number: DMS-1806190

Award Identifier / Grant number: DMS-1266172

Award Identifier / Grant number: DMS-1056387

Award Identifier / Grant number: DMS-1811833

Funding statement: The first author was supported by the National Science Foundation under grant DMS-1806190 and by the Simons Foundation. The second author was supported by the National Science Foundation under grant DMS-1266172. The fourth author was supported by the National Science Foundation under grants DMS-1056387 and DMS-1811833.

A The Bryant soliton

In [16] Bryant showed that up to constant multiples, there is only one complete, steady, rotationally symmetric soliton in dimension three that is not flat. It has positive sectional curvature. The maximum scalar curvature is equal to 1, and is attained at the center of rotation. The complete soliton can be written in the form g = d z d z + B ( z ) 2 g S n - 1 , where z is the distance from the center of rotation. For large z, the metric has the following asymptotics: the aperature B ( z ) has leading order term 2 ( n - 2 ) z , the orbital sectional curvature K orb has leading order term 1 2 ( n - 2 ) z , and the radial sectional curvature K rad has leading order term 1 4 z 2 .

Sometimes it is more convenient to write the metric in the form Φ ( r ) - 1 d r 2 + r 2 g S n - 1 , where the function Φ ( r ) is defined by

Φ ( B ( z ) ) = ( d d z B ( z ) ) 2 .

The function Φ ( r ) is known to satisfy the equation

Φ ( r ) Φ ′′ ( r ) - 1 2 Φ ( r ) 2 + n - 2 - Φ ( r ) r Φ ( r ) + 2 ( n - 2 ) r 2 Φ ( r ) ( 1 - Φ ( r ) ) = 0 .

The orbital and radial sectional curvatures are given by

K orb = 1 r 2 ( 1 - Φ ( r ) ) and K rad = - 1 2 r Φ ( r ) .

It is known that Φ ( r ) has the following asymptotics. Near r = 0 , Φ is smooth and has the asymptotic expansion

Φ ( r ) = 1 + b 0 r 2 + o ( r 2 ) ,

where b 0 is a negative constant (since the curvature is positive). As r , Φ is smooth and has the asymptotic expansion

Φ ( r ) = c 0 r - 2 + 5 - n n - 2 c 0 2 r - 4 + o ( r - 4 ) ,

where c 0 is a positive constant.

We will next find (for the convenience of the reader) the exact values of the constants b 0 and c 0 in the above asymptotics for the Bryant soliton of maximal scalar curvature one.

Recall that the scalar curvature is given by R = ( n - 1 ) ( n - 2 ) K orb + 2 ( n - 1 ) K rad . The maximal scalar curvature is attained at z = 0 , at which point K orb = K rad . The maximal scalar curvature being equal to 1 is equivalent to K orb = K rad = 1 n ( n - 1 ) at z = 0 . On the other hand, the asymptotic expansion of Φ ( r ) gives

K orb = 1 r 2 ( 1 - Φ ( r ) ) = - b 0 + o ( 1 ) as  r 0 .

Consequently, b 0 = - 1 n ( n - 1 ) .

Bryant’s asymptotics imply that for z sufficiently large, the aperture satisfies

r = ( 1 + o ( 1 ) ) 2 ( n - 2 ) z ,

implying that 2 ( n - 2 ) z = ( 1 + o ( 1 ) ) r 2 . The radial sectional curvature satisfies

K rad = ( 1 + o ( 1 ) ) 1 4 z 2 = ( 1 + o ( 1 ) ) ( n - 2 ) 2 r 4

for r large. On the other hand, the asymptotic expansion of Φ ( r ) implies

K rad = - 1 2 r Φ ( r ) = ( 1 + o ( 1 ) ) c 0 r - 4

for r large. Comparing the two formulae, we conclude that c 0 = ( n - 2 ) 2 .

Summarizing the above discussion we conclude the following asymptotics for the Bryant soliton with maximal scalar curvature equal to one:

Φ ( r ) = { 1 - r 2 n ( n - 1 ) + o ( r 2 ) as  r 0 , ( n - 2 ) 2 r - 2 + ( n - 2 ) 3 ( 5 - n ) r - 4 + o ( r - 4 ) as  r .

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Received: 2021-06-13
Revised: 2022-09-20
Published Online: 2022-11-23
Published in Print: 2023-02-01

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