Book 11A

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Course 11Book 11A: The Ricci Flow: Existence and Maximum PrinciplesChapter 6

Hamilton’s 1982 Theorem

Positive Ricci curvature in dimension 3 flows to a round metric.

13 min read · Updated Oct 3, 2026

Read Hamilton's "Three-manifolds with positive Ricci curvature" (Journal of Differential Geometry 17, 1982) alongside this chapter: it is long but readable, and the guide follows its structure. Chow and Knopf's The Ricci Flow: An Introduction, chapter 6, gives a streamlined account.

In this chapter · 5 sections
  1. 6.1A computed example: Berger spheres become round
  2. 6.2The four steps
  3. 6.3What the theorem does and does not say about Poincaré
  4. 6.4History
  5. 6.5Exercises

In 1982 Hamilton proved the first theorem about topology by the Ricci flow:

Theorem 6.1 Hamilton (1982)

Let (M3,g0)(M^3, g_0) be a closed 3-manifold with positive Ricci curvature. Then the normalised Ricci flow from g0g_0 exists for all time and converges smoothly to a metric of constant positive sectional curvature. Consequently MM is diffeomorphic to a spherical space form S3/ΓS^3/\Gamma.

The theorem says positive Ricci curvature is an open door to the round sphere: the flow walks through it. This chapter gives the proof in four steps, following Hamilton: positivity is preserved, the curvature pinches toward constant, its gradient is controlled, and the rescaled metrics converge. Each step uses tools already built: the maximum principles of 11A.4 Maximum Principles under Ricci Flow, the evolution equations of 11A.2 How Curvature Evolves, the extension criterion of 11A.3 Short-Time Existence and Uniqueness, and Myers' theorem (9A.7 Jacobi Fields and Curvature versus Topology). The chapter ends with what came after: the same strategy in higher dimensions, up to the differentiable sphere theorem.

By the end of this chapter you will be able to:

  • outline the four steps of Hamilton's proof and say which tool each uses;
  • explain the pinching estimate ∣Ric⁡˚∣2≤CR2−δ|\mathring{\operatorname{Ric}}|^2 \leq CR^{2 - \delta} and why it forces constant curvature;
  • describe how the gradient estimate and Myers' theorem control the shape at the singular time;
  • compute the flow of Berger spheres and watch them round out;
  • say what the theorem implies for the Poincaré conjecture, and what it does not.

A computed example: Berger spheres become round

In the world Model A squashed sphere rounds out

The Berger spheres of 9A.5 Computing Curvature are S3=SU(2)S^3 = SU(2) with the left-invariant metric A ω12+B(ω22+ω32)A\,\omega_1^2 + B(\omega_2^2 + \omega_3^2), where ωi\omega_i are the dual forms of a frame with [Xi,Xj]=2Xk[X_i, X_j] = 2X_k cyclically; the round unit sphere is A=B=1A = B = 1. Milnor's formulas give Ric⁡(e1,e1)=2AB2\operatorname{Ric}(e_1, e_1) = \frac{2A}{B^2} and Ric⁡(e2,e2)=Ric⁡(e3,e3)=2(2B−A)B2\operatorname{Ric}(e_2, e_2) = \operatorname{Ric}(e_3, e_3) = \frac{2(2B - A)}{B^2} in the orthonormal frame, so Ric⁡>0\operatorname{Ric} > 0 exactly when A<2BA < 2B. Because the flow preserves the symmetry, it reduces to an ODE (11A.8 Homogeneous Flows):

A′=−4A2B2,B′=−4(2−AB),A' = -\frac{4A^2}{B^2}, \qquad B' = -4\Big(2 - \frac AB\Big),

and the squashing ratio x=ABx = \frac AB satisfies x′=8x(1−x)Bx' = \frac{8x(1 - x)}{B}. So x→1x \to 1: a squashed (x<1x < 1) or stretched (x>1x > 1) Berger sphere rounds out as it shrinks (Figure 6.1). This is Hamilton's theorem in a case you can solve with a computer.

Figure 6.1. The squashing ratio AB\frac AB of Berger spheres under the Ricci flow, from AB=0.3\frac AB = 0.3 and 1.81.8 with B=1B = 1 (computed with a fourth-order Runge–Kutta integration). Both reach 11, the round metric, exactly as the sphere shrinks to a point (dots: extinction times 0.1790.179 and 0.3080.308).

The four steps

Step 1: positive Ricci curvature is preserved. In dimension three, Ric⁡≥0\operatorname{Ric} \geq 0 is a convex, ODE-invariant set of curvature operators (11A.4 Maximum Principles under Ricci Flow). Hamilton proved more: Ric⁡≥εRg\operatorname{Ric} \geq \varepsilon Rg is preserved for some ε>0\varepsilon > 0 depending on g0g_0. On a compact manifold with Ric⁡>0\operatorname{Ric} > 0, such an ε\varepsilon exists at t=0t = 0. By 11A.4 Maximum Principles under Ricci Flow, the flow becomes singular at a finite time TT, and Rmin⁡→∞R_{\min} \to \infty as t→Tt \to T.

Step 2: pinching toward constant curvature. Let Ric⁡˚=Ric⁡−R3g\mathring{\operatorname{Ric}} = \operatorname{Ric} - \frac R3g, the trace-free part. Hamilton's key estimate:

∣Ric⁡˚∣2≤CR2−δ|\mathring{\operatorname{Ric}}|^2 \leq CR^{2 - \delta}

for constants C,δ>0C, \delta > 0 depending on g0g_0. It follows from the maximum principle applied to f=∣Ric⁡˚∣2R2−δf = \frac{|\mathring{\operatorname{Ric}}|^2}{R^{2 - \delta}}, whose evolution equation has a reaction term that is nonpositive when δ\delta is small, thanks to Ric⁡≥εRg\operatorname{Ric} \geq \varepsilon Rg. Dividing by R2R^2: ∣Ric⁡˚∣2R2≤CR−δ→0\frac{|\mathring{\operatorname{Ric}}|^2}{R^2} \leq CR^{-\delta} \to 0 where R→∞R \to \infty. In dimension three the Weyl tensor vanishes (9A.5 Computing Curvature), so the curvature tensor is determined by Ric⁡\operatorname{Ric}, and Ric⁡\operatorname{Ric} close to R3g\frac R3g means all sectional curvatures are close to one another, relative to their size (Figure 6.2).

Step 3: the gradient estimate. Hamilton proved that for every η>0\eta > 0, ∣∇R∣2R3≤η\frac{|\nabla R|^2}{R^3} \leq \eta wherever RR is large enough, up to an error that decays like a negative power of RR: as curvature becomes large, its gradient becomes small relative to it. Integrating along geodesics, RR is nearly constant on balls of radius cRmax⁡\frac{c}{\sqrt{R_{\max}}}.

Step 4: convergence. As t→Tt \to T, Step 3 gives Rmin⁡Rmax⁡→1\frac{R_{\min}}{R_{\max}} \to 1. By Step 2, Ric⁡≥R3(1−o(1))g\operatorname{Ric} \geq \frac{R}{3}(1 - o(1))g, and Myers' theorem (9A.7 Jacobi Fields and Curvature versus Topology) bounds the diameter by CRmin⁡→0\frac{C}{\sqrt{R_{\min}}} \to 0: the manifold shrinks to a point while becoming round. Rescale to fixed volume: the normalised flow (11A.1 The Equation and Its First Solutions) exists for all time, and Hamilton showed it converges exponentially fast, in every CkC^k norm, to a metric with Ric⁡˚=0\mathring{\operatorname{Ric}} = 0. In dimension three, an Einstein metric has constant sectional curvature, here positive. Its universal cover is the round S3S^3 (9A.7 Jacobi Fields and Curvature versus Topology and 10A.5 Thurston’s Eight Geometries), so M=S3/ΓM = S^3/\Gamma.

Figure 6.2. The pinching quantity ∣Ric⁡˚∣R\frac{|\mathring{\operatorname{Ric}}|}{R} along the Berger flow with AB=0.3\frac AB = 0.3 initially, against RR (computed from Milnor's formulas). As the curvature grows, the trace-free part becomes negligible: the curvature becomes constant relative to its size.
Figure 6.3. The architecture of Hamilton's proof, with the tool behind each step.

What the theorem does and does not say about Poincaré

If MM is simply connected and carries some metric with Ric⁡>0\operatorname{Ric} > 0, the theorem gives M=S3/ΓM = S^3/\Gamma with Γ=π1(M)=1\Gamma = \pi_1(M) = 1: M=S3M = S^3. So the Poincaré conjecture holds for such manifolds. But a simply connected 3-manifold comes with no metric of positive Ricci curvature, and finding one is as hard as the conjecture itself. For an arbitrary initial metric, the flow develops regions of negative curvature, necks that pinch, and other singularities. Hamilton spent the next two decades building tools for that case (11B.5 Hamilton’s Program in 2002), and Perelman finished the job.

Where this goes After 1982

Hamilton extended the method to four-manifolds with positive curvature operator (1986): they are diffeomorphic to S4S^4 or RP4\mathbb{RP}^4. Christoph Böhm and Burkhard Wilking (2008) did the same in every dimension, using new ODE-invariant pinching sets. Simon Brendle and Richard Schoen (2009) proved the differentiable sphere theorem: a closed manifold whose sectional curvatures, at each point, lie in an interval (14K,K](\frac14K, K] is diffeomorphic to a spherical space form, again by showing the Ricci flow converges to constant curvature.

History

Hamilton's paper was submitted in 1982 and introduced the Ricci flow, its short-time existence, the evolution equations and the tensor maximum principle, all to prove this theorem. Hamilton's 1986 paper treated positive curvature operator in dimension four; Böhm–Wilking's paper appeared in the Annals of Mathematics in 2008, and Brendle–Schoen's in the Journal of the AMS in 2009.

Recall Where we stand

Hamilton's theorem: a closed 3-manifold with Ric⁡>0\operatorname{Ric} > 0 flows, after normalisation, to constant positive curvature, so it is a spherical space form. The proof: Ric⁡≥εRg\operatorname{Ric} \geq \varepsilon Rg is preserved; ∣Ric⁡˚∣2≤CR2−δ|\mathring{\operatorname{Ric}}|^2 \leq CR^{2-\delta} pinches curvature toward constant where it is large; ∣∇R∣2R3\frac{|\nabla R|^2}{R^3} becomes small, so curvature is nearly constant across the manifold; Myers shrinks the diameter, and the normalised flow converges exponentially. Berger spheres show it in a computable case. The theorem proves Poincaré only for manifolds already known to carry Ric⁡>0\operatorname{Ric} > 0. 11A.7 Ricci Flow on Surfaces turns to surfaces, where the flow proves uniformization.

Exercises

Exercise 6.2 Einstein implies constant curvature in dimension three

Using the formula for RijklR_{ijkl} in terms of Ric⁡\operatorname{Ric} in dimension three (9A.5 Computing Curvature), show that if Ric⁡=R3g\operatorname{Ric} = \frac R3g then Rijkl=R6(gilgjk−gikgjl)R_{ijkl} = \frac R6(g_{il}g_{jk} - g_{ik}g_{jl}), so the sectional curvature is R6\frac R6 everywhere, and constant by Schur's lemma (9A.4 Curvature and What It Means).

Solution

With Rij=R3gijR_{ij} = \frac R3g_{ij}: Rilgjk+Rjkgil−Rikgjl−Rjlgik=2R3(gilgjk−gikgjl)R_{il}g_{jk} + R_{jk}g_{il} - R_{ik}g_{jl} - R_{jl}g_{ik} = \frac{2R}{3}(g_{il}g_{jk} - g_{ik}g_{jl}), and subtracting R2(gilgjk−gikgjl)\frac R2(g_{il}g_{jk} - g_{ik}g_{jl}) leaves R6(… )\frac R6(\dots). Schur's lemma makes RR constant in dimension 33.

Exercise 6.3 The Berger ODE

(a) From Ric⁡(e1,e1)=2AB2\operatorname{Ric}(e_1, e_1) = \frac{2A}{B^2} and Ric⁡(e2,e2)=2(2B−A)B2\operatorname{Ric}(e_2, e_2) = \frac{2(2B - A)}{B^2}, derive A′=−4A2B2A' = -\frac{4A^2}{B^2} and B′=−4(2−AB)B' = -4(2 - \frac AB), remembering that A=g(X1,X1)A = g(X_1, X_1) and Ric⁡(X1,X1)=ARic⁡(e1,e1)\operatorname{Ric}(X_1, X_1) = A\operatorname{Ric}(e_1, e_1). (b) Derive x′=8x(1−x)Bx' = \frac{8x(1 - x)}{B} for x=ABx = \frac AB. (c) Check the round case A=B=1−4tA = B = 1 - 4t.

Solution

(a) A′=−2Ric⁡(X1,X1)=−2A⋅2AB2A' = -2\operatorname{Ric}(X_1, X_1) = -2A\cdot\frac{2A}{B^2}; B′=−2B⋅2(2B−A)B2=−4(2B−A)BB' = -2B\cdot\frac{2(2B - A)}{B^2} = -\frac{4(2B - A)}{B}. (b) x′=A′B−AB′B2=−4A2B+4A(2B−A)BB2=4A(2B−2A)B3=8x(1−x)Bx' = \frac{A'B - AB'}{B^2} = \frac{-\frac{4A^2}{B} + \frac{4A(2B - A)}{B}}{B^2} = \frac{4A(2B - 2A)}{B^3} = \frac{8x(1 - x)}{B}. (c) A′=−4=−4⋅(1−4t)2(1−4t)2A' = -4 = -4\cdot\frac{(1 - 4t)^2}{(1 - 4t)^2} and B′=−4(2−1)=−4B' = -4(2 - 1) = -4.

Exercise 6.4 Positive Ricci on a compact manifold

Show that if MM is compact and Ric⁡>0\operatorname{Ric} > 0, then Ric⁡≥εRg\operatorname{Ric} \geq \varepsilon Rg for some ε>0\varepsilon > 0. For the Berger sphere with AB=0.3\frac AB = 0.3, find the best ε\varepsilon.

Solution

The function min⁡∣v∣=1Ric⁡(v,v)R\min_{|v| = 1}\frac{\operatorname{Ric}(v, v)}{R} is continuous and positive on the compact unit sphere bundle, so it has a positive minimum. For the Berger sphere, the Ricci eigenvalues are 2AB2\frac{2A}{B^2} and 2(2B−A)B2\frac{2(2B - A)}{B^2} (twice), and R=8B−2AB2R = \frac{8B - 2A}{B^2}; with A=0.3A = 0.3, B=1B = 1: eigenvalues 0.60.6 and 3.43.4, R=7.4R = 7.4, so ε=0.67.4≈0.081\varepsilon = \frac{0.6}{7.4} \approx 0.081.

Exercise 6.5 The diameter goes to zero

Assume Ric⁡≥Rmin⁡3(1−η)g\operatorname{Ric} \geq \frac{R_{\min}}{3}(1 - \eta)g with η<1\eta < 1. Use Myers' theorem (9A.7 Jacobi Fields and Curvature versus Topology) to show diam⁡≤π6(1−η)Rmin⁡\operatorname{diam} \leq \pi\sqrt{\frac{6}{(1 - \eta)R_{\min}}}. Why does this tend to zero as t→Tt \to T?

Solution

Myers with (n−1)k=2k=Rmin⁡(1−η)3(n - 1)k = 2k = \frac{R_{\min}(1 - \eta)}{3} gives diam⁡≤πk=π6(1−η)Rmin⁡\operatorname{diam} \leq \frac{\pi}{\sqrt k} = \pi\sqrt{\frac{6}{(1 - \eta)R_{\min}}}. As t→Tt \to T, Rmin⁡→∞R_{\min} \to \infty (Step 1 with the gradient estimate), so the diameter tends to zero.

Exercise 6.6 Rehearsal: Poincaré for manifolds with positive Ricci curvature

Suppose a closed simply connected 3-manifold MM admits a metric with Ric⁡>0\operatorname{Ric} > 0. Deduce from Hamilton's theorem that M≅S3M \cong S^3. Then explain in two sentences why this does not prove the Poincaré conjecture, and what kind of statement would.

Solution

By the theorem M=S3/ΓM = S^3/\Gamma with Γ≅π1(M)=1\Gamma \cong \pi_1(M) = 1, so M=S3M = S^3. The conjecture concerns every closed simply connected 3-manifold, and nothing guarantees that such a manifold admits a metric with Ric⁡>0\operatorname{Ric} > 0; proving that it does would itself prove the conjecture. What is needed is a flow that works from an arbitrary metric, handling the singularities that then form: Ricci flow with surgery (12B.5 Ricci Flow with Surgery for All Time, 12C.3 The Poincaré Conjecture, Assembled).

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