Book 12C

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Course 12Book 12C: Extinction and the ProofChapter 2

Finite Extinction

Width, minimal spheres and a shrinking quantity that forces the flow to end.

21 min read · Updated Oct 3, 2026

Read Perelman III (seven pages), §1, and Colding and Minicozzi, "Estimates for the extinction time for the Ricci flow on certain 3-manifolds and a question of Perelman" (Journal of the AMS 18, 2005), §§1–2. Their expository "Width and finite extinction time of Ricci flow" (Geometry & Topology 12, 2008) gives complete proofs. 10A.8 Min–Max and Width prepared the width, and 6A.8 Curve Shortening and the First Geometric Flows the one-dimensional model.

In this chapter · 7 sections
  1. 2.1Shrinking at a rate set by topology
  2. 2.2The one-dimensional model
  3. 2.3Perelman's theorem
  4. 2.3.1The quantity: least-area discs spanning a family of loops
  5. 2.3.2From the inequality to extinction
  6. 2.3.3Surgery
  7. 2.4Colding and Minicozzi's width
  8. 2.5Two versions, one argument
  9. 2.6History
  10. 2.7Exercises

By 12C.1 Reading Off the Topology, the Poincaré conjecture now rests on one statement: on a closed simply connected 3-manifold, the Ricci flow with surgery becomes extinct in finite time. The idea of the proof fits in a line. Find a geometric quantity that is positive as long as anything is left, and show that it decreases at a definite rate. Then it would become negative, which is impossible, so the flow must end first. The quantity is an area: of discs spanning loops in Perelman's version, of 2-spheres sweeping out the manifold in Colding and Minicozzi's. Its rate of decrease comes from the Gauss–Bonnet theorem, so it is set by topology, not by the metric.

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

  • explain the one-dimensional model: under curve shortening, enclosed area drops at rate 2π2\pi;
  • state Perelman's finite extinction theorem and the topological input that makes the relevant quantity nontrivial;
  • derive the area inequalities, dAdt≤−2π−12Rmin⁡A\frac{dA}{dt} \leq -2\pi - \frac12R_{\min}A for Perelman's discs and dWdt≤−4π+34(t+C)W\frac{dW}{dt} \leq -4\pi + \frac{3}{4(t + C)}W for the width;
  • deduce finite extinction from either inequality, with an explicit bound on the extinction time;
  • explain how surgery is handled and what the two versions of the argument have in common.

Shrinking at a rate set by topology

In the world Model Grain growth and soap froth

A polycrystalline metal film, or a two-dimensional soap froth, coarsens over time: boundaries move to reduce their total length, small grains or bubbles shrink and vanish, and large ones grow. In the idealised model in which each boundary moves with normal velocity proportional to its curvature and boundaries meet at 120°120°, the area of a grain with nn sides changes at the rate dAdt=π3mγ(n−6)\frac{dA}{dt} = \frac{\pi}{3}m\gamma(n - 6), with mm the boundary mobility and γ\gamma its tension. This is the von Neumann–Mullins law, proposed by John von Neumann for soap froth and derived by W. W. Mullins for metal grains in 1956. The rate depends on the number of sides and on nothing else about the shape. A grain with fewer than six sides vanishes in finite time. An isolated round island grain, with no corners, is the curve shortening flow itself, and its area drops at the rate 2πmγ2\pi m\gamma. The law has been tested in experiments, and real materials depart from the idealised model in ways that are still studied. Finite extinction for the Ricci flow is the same principle in a higher dimension: a rate fixed by the Gauss–Bonnet theorem, and so by topology alone.

The one-dimensional model

Under curve shortening flow, a closed embedded plane curve moves with normal velocity equal to its curvature κ\kappa, and the area it encloses changes at the rate

dAdt=−∮κ ds=−2π,\frac{dA}{dt} = -\oint\kappa\,ds = -2\pi,

because the total curvature of a simple closed curve is 2π2\pi (6A.8 Curve Shortening and the First Geometric Flows). So the curve cannot survive past time A(0)2π\frac{A(0)}{2\pi}, whatever its shape. The Ricci flow arguments below follow this pattern, with two complications. The relevant area is not the area of a fixed surface but a min–max quantity, which must be shown to be nontrivial using topology. And the metric's own curvature enters, through the scalar curvature, with a sign that can work against the argument; the bound Rmin⁡≥−32(t+C)R_{\min} \geq -\frac{3}{2(t + C)} (11A.4 Maximum Principles under Ricci Flow) keeps it under control.

Perelman's theorem

Theorem 2.1 Finite extinction (Perelman III, Theorem 1.1)

Let MM be a closed oriented 3-manifold whose prime decomposition contains no aspherical factors. Then for every initial metric on MM, the Ricci flow with surgery becomes extinct in finite time.

A closed simply connected MM satisfies the hypothesis: its prime factors are simply connected, and an aspherical closed 3-manifold has infinite fundamental group. So, with 12C.1 Reading Off the Topology, this theorem proves the Poincaré conjecture. Perelman's own summary is that the proof needs no substantially new ideas: a least-area disc argument from Hamilton's work on nonsingular solutions, and a regularisation of the curve shortening flow due to Steven Altschuler and Matthew Grayson.

The quantity: least-area discs spanning a family of loops

Let ΛM\Lambda M be the space of contractible loops in MM. For a metric gg and a loop cc, let A(c,g)A(c, g) be the least area of a disc spanning cc. For a family Γ\Gamma of loops, let A(Γ,g)A(\Gamma, g) be the largest of these areas; for a nontrivial homotopy class α\alpha of families, relative to the constant loops, let

A(α,g)=inf⁡Γ∈αA(Γ,g).A(\alpha, g) = \inf_{\Gamma\in\alpha}A(\Gamma, g).

This is a min–max area, of the same kind as the width of 10A.8 Min–Max and Width. That a nontrivial class α\alpha exists when MM is not aspherical follows, Perelman notes, from a classical and elementary result of Serre. Some higher homotopy group of MM is nonzero, and the loop space detects it.

Lemma 2.2 The area estimate (Perelman III, Lemma 1.2)

For a smooth Ricci flow and any α\alpha, the function A(t)=A(α,g(t))A(t) = A(\alpha, g(t)) satisfies

dAdt≤−2π−12Rmin⁡(t)A(t)\frac{dA}{dt} \leq -2\pi - \frac12R_{\min}(t)A(t)

in the sense of the lim sup of forward difference quotients.

The idea

Suppose the family realising A(t)A(t) consists of smooth embedded loops, and for each loop cc take its least-area disc DcD_c. Let the metric evolve by the Ricci flow and the loops by curve shortening. The area of DcD_c changes at the rate

∫Dc(−tr⁡DcRic⁡)+∮c(−kg),\int_{D_c}\big(-\operatorname{tr}_{D_c}\operatorname{Ric}\big) + \oint_c(-k_g),

where kgk_g is the geodesic curvature of cc in DcD_c. In three dimensions, the Gauss equation gives tr⁡DRic⁡=12R+(K−det⁡II)\operatorname{tr}_{D}\operatorname{Ric} = \frac12R + (K - \det\mathrm{II}), where KK is the intrinsic curvature of the disc, and det⁡II≤0\det\mathrm{II} \leq 0 because the disc is minimal. So the rate is at most

∫Dc(−12R−K)−∮ckg=−12∫DcR−2π\int_{D_c}\Big(-\frac12R - K\Big) - \oint_ck_g = -\frac12\int_{D_c}R - 2\pi

by Gauss–Bonnet for a disc, ∫DK+∮kg=2π\int_DK + \oint k_g = 2\pi. Bounding R≥Rmin⁡R \geq R_{\min} gives the lemma.

The difficulty is that a family may contain loops that are not immersed, such as a loop that runs along an arc and back, and curve shortening is then not continuous in the family. Perelman's §3 avoids this by adding one dimension to the ambient manifold, following Altschuler and Grayson, who had regularised the singular curve shortening flow in the plane.

From the inequality to extinction

In dimension three, ∂tR=ΔR+23R2+2∣Ric⁡∘∣2\partial_tR = \Delta R + \frac23R^2 + 2|\operatorname{Ric}^\circ|^2, which gives Rmin⁡(t)≥−32(t+C)R_{\min}(t) \geq -\frac{3}{2(t + C)}. With Lemma 2.2,

dAdt≤−2π+34(t+C)A,soddtAt+C≤−2πt+C\frac{dA}{dt} \leq -2\pi + \frac{3}{4(t + C)}A, \qquad \text{so} \qquad \frac{d}{dt}\frac{A}{t + C} \leq -\frac{2\pi}{t + C}

(Exercise 2.4). The right-hand side is not integrable at infinity, while At+C\frac{A}{t + C} cannot become negative, so the flow must become extinct by a time that depends only on A(0)A(0) and CC.

Surgery

For irreducible MM, surgeries are topologically trivial: one component after the surgery is diffeomorphic to the manifold before, and the others are spheres. Perelman notes that the identification can be chosen (1+ξ)(1 + \xi)-Lipschitz with ξ\xi as small as one likes, so the min–max area does not increase at a surgery, and the lemma holds for the flow with surgery. For general MM, the Kneser finiteness theorem (10A.3 The Prime Decomposition) shows that only finitely many surgeries are topologically nontrivial, so from some time on all surgeries are trivial, and by Milnor's uniqueness of prime decomposition each component then satisfies the hypothesis and the irreducible argument applies. For a homotopy sphere, Perelman adds, even Kneser can be avoided, by following homotopy equivalences through each surgery.

Colding and Minicozzi's width

On 25 April 2003, at a dinner in New York, Perelman asked Tobias Colding what happens to the Ricci flow on S3S^3 from an arbitrary metric, and whether it becomes extinct in finite time; he added that he knew no good way of constructing minimal surfaces for a general metric. Colding and William Minicozzi answered with min–max: the smallest of the largest slices of sweepouts is a minimal surface. Perelman posted his own proof soon after, and their paper, which avoids the curve shortening flow, appeared in 2005.

Let MM be prime and not aspherical. If M=S2×S1M = S^2\times S^1, then π3(M)=Z\pi_3(M) = \mathbb{Z}; otherwise MM is irreducible, π2(M)=0\pi_2(M) = 0 by the sphere theorem, and the Hurewicz theorem gives π3(M)≠0\pi_3(M) \neq 0 (10A.8 Min–Max and Width). Either way, the space of maps S2→MS^2 \to M is not simply connected, and a nontrivial class [β][\beta] of sweepouts by 2-spheres exists: one-parameter families β(s)\beta(s), s∈[0,1]s \in [0, 1], of maps S2→MS^2 \to M, constant at both ends (Figure 2.1). The width is

W(g)=min⁡γ∈[β] max⁡s∈[0,1]E(γ(s)),W(g) = \min_{\gamma\in[\beta]}\ \max_{s\in[0, 1]}E(\gamma(s)),

with EE the energy of a map; using area instead gives the same value.

Figure 2.1. A sweepout of a 3-manifold by 2-spheres, drawn in cross-section (schematic). Each curve stands for a 2-sphere; the family starts and ends at points. The width is the least possible size of the largest slice, over all sweepouts in a nontrivial class.
Theorem 2.3 The width inequality (Colding–Minicozzi, JAMS 2005, Theorem 1.1)

Let MM be a closed orientable prime non-aspherical 3-manifold. Under the Ricci flow,

ddtW(g(t))≤−4π+34(t+C)W(g(t))\frac{d}{dt}W(g(t)) \leq -4\pi + \frac{3}{4(t + C)}W(g(t))

in the sense of the lim sup of forward difference quotients. Hence g(t)g(t) becomes extinct in finite time.

The 4π4\pi comes from Gauss–Bonnet for a sphere, and the 34\frac34 from the lower bound on Rmin⁡R_{\min}; both matter, while CC depends on the initial metric. For a single minimal sphere Σ\Sigma the computation is the one of 10A.8 Min–Max and Width: ddtArea⁡(Σ)=−12∫Σ(R+RΣ+∣A∣2)≤−4π+34(t+C)Area⁡(Σ)\frac{d}{dt}\operatorname{Area}(\Sigma) = -\frac12\int_\Sigma(R + R_\Sigma + |A|^2) \leq -4\pi + \frac{3}{4(t + C)}\operatorname{Area}(\Sigma), using ∫ΣRΣ=8π\int_\Sigma R_\Sigma = 8\pi. The work in their paper is to pass from minimal spheres to the width: they show that a nearly optimal sweepout can be chosen so that every slice whose energy is close to the maximum is close to a collection of harmonic spheres, to which the computation applies. Multiplying by (t+C)−3/4(t + C)^{-3/4} and integrating gives

(T+C)−3/4W(g(T))≤C−3/4W(g(0))−16π((T+C)1/4−C1/4),(T + C)^{-3/4}W(g(T)) \leq C^{-3/4}W(g(0)) - 16\pi\big((T + C)^{1/4} - C^{1/4}\big),

whose right-hand side becomes negative for large TT (Figure 2.2). For the flow with surgery and general MM without aspherical summands, they argue as in Perelman's §1.5.

Figure 2.2. The comparison bound for the width with C=1C = 1: the solution of w′=−4π+34(t+1)ww' = -4\pi + \frac{3}{4(t + 1)}w for w(0)=10,20,40w(0) = 10, 20, 40 (computed, and checked against the closed form w(t)=(t+1)3/4(w(0)−16π((t+1)1/4−1))w(t) = (t + 1)^{3/4}\big(w(0) - 16\pi((t + 1)^{1/4} - 1)\big)). For a large initial width the bound first rises, because the curvature term 3w4(t+1)\frac{3w}{4(t + 1)} outweighs 4π4\pi at early times; but that term decays, and each bound reaches 00 at a finite time, after which the flow cannot exist. A wider manifold may last longer, but every one becomes extinct.

Two versions, one argument

curve shortening (6A.8 Curve Shortening and the First Geometric Flows) Perelman III Colding–Minicozzi
quantity enclosed area min–max area of spanning discs width: min–max area of 2-spheres
topological input the curve is closed and embedded a nontrivial class of loop families (Serre) a nontrivial class in π3\pi_3 (Hurewicz, sphere theorem)
Gauss–Bonnet turning number: 2π2\pi disc: 2π2\pi sphere: 4π4\pi
curvature term none −12Rmin⁡A-\frac12R_{\min}A −12Rmin⁡W-\frac12R_{\min}W
technical core — regularised curve shortening (Altschuler–Grayson) min–max with energy and bubbling
conclusion extinct by A(0)2π\frac{A(0)}{2\pi} extinct in finite time extinct in finite time
Where this goes The proof assembled

12C.3 The Poincaré Conjecture, Assembled puts the pieces together: the flow and its short-time existence, the analysis of singularities, noncollapsing, canonical neighbourhoods, surgery for all time, finite extinction, and the topology. Every step has now been proved somewhere in the guide.

History

Hamilton had used least-area discs in his 1999 paper on nonsingular solutions to show that the boundary tori of hyperbolic pieces are incompressible, and Perelman adapted that argument. Perelman's third preprint was posted on 17 July 2003. Colding and Minicozzi's paper was submitted in August 2003 and published in 2005; their expository paper with full proofs appeared in 2008. Perelman also observed that finite extinction gives the elliptization conjecture without the long-time analysis of his second preprint (12C.1 Reading Off the Topology).

Recall Where we stand

A quantity that stays positive while the manifold exists, and decreases at a rate fixed by Gauss–Bonnet, forces finite extinction. Perelman used the min–max area of least-area discs spanning a nontrivial family of loops: A′≤−2π−12Rmin⁡AA' \leq -2\pi - \frac12R_{\min}A, with curve shortening (regularised) moving the loops. Colding and Minicozzi used the width of sweepouts by 2-spheres in a nontrivial class of π3\pi_3: W′≤−4π+34(t+C)WW' \leq -4\pi + \frac{3}{4(t + C)}W. With Rmin⁡≥−32(t+C)R_{\min} \geq -\frac{3}{2(t + C)}, either quantity would become negative in finite time. Surgery does not increase it. So the flow with surgery on any closed 3-manifold without aspherical prime factors, in particular any simply connected one, becomes extinct, and with 12C.1 Reading Off the Topology the manifold is S3S^3. 12C.3 The Poincaré Conjecture, Assembled assembles the whole proof.

Exercises

Exercise 2.4 Perelman's normalisation

Suppose A≥0A \geq 0 satisfies A′≤−2π+34(t+C)AA' \leq -2\pi + \frac{3}{4(t + C)}A. (a) Show that A^=At+C\hat A = \frac{A}{t + C} satisfies A^′≤−2πt+C\hat A' \leq -\frac{2\pi}{t + C}. (b) Integrate to show A^(t)≤A^(0)−2πlog⁡t+CC\hat A(t) \leq \hat A(0) - 2\pi\log\frac{t + C}{C}, and deduce that the flow becomes extinct by time C(eA(0)/(2πC)−1)C\big(e^{A(0)/(2\pi C)} - 1\big).

Solution

(a) A^′=A′t+C−A(t+C)2≤−2πt+C+3A4(t+C)2−A(t+C)2≤−2πt+C\hat A' = \frac{A'}{t + C} - \frac{A}{(t + C)^2} \leq -\frac{2\pi}{t + C} + \frac{3A}{4(t + C)^2} - \frac{A}{(t + C)^2} \leq -\frac{2\pi}{t + C}, since A≥0A \geq 0. (b) Integrating, A^(t)≤A(0)C−2πlog⁡t+CC\hat A(t) \leq \frac{A(0)}{C} - 2\pi\log\frac{t + C}{C}. The left side is nonnegative while the flow exists, so log⁡t+CC≤A(0)2πC\log\frac{t + C}{C} \leq \frac{A(0)}{2\pi C}, that is t≤C(eA(0)/(2πC)−1)t \leq C\big(e^{A(0)/(2\pi C)} - 1\big).

Exercise 2.5 The disc computation

Assume the identities in the proof idea of Lemma 2.2. Show that if R≥Rmin⁡R \geq R_{\min}, the rate of change of the area of DcD_c is at most −2π−12Rmin⁡Area⁡(Dc)-2\pi - \frac12R_{\min}\operatorname{Area}(D_c). Where exactly are minimality and Gauss–Bonnet used, and why does the sign of det⁡II\det\mathrm{II} matter?

Solution

Rate =∫D(−12R−K+det⁡II)−∮kg≤∫D(−12R−K)−∮kg= \int_D(-\frac12R - K + \det\mathrm{II}) - \oint k_g \leq \int_D(-\frac12R - K) - \oint k_g, using det⁡II≤0\det\mathrm{II} \leq 0. Minimality: the principal curvatures are ±λ\pm\lambda, so det⁡II=−λ2≤0\det\mathrm{II} = -\lambda^2 \leq 0. Gauss–Bonnet: ∫DK+∮kg=2π\int_DK + \oint k_g = 2\pi. So the rate is at most −12∫DR−2π≤−12Rmin⁡Area⁡(D)−2π-\frac12\int_DR - 2\pi \leq -\frac12R_{\min}\operatorname{Area}(D) - 2\pi. If det⁡II\det\mathrm{II} could be positive, the estimate would fail.

Exercise 2.6 The sweepouts of S2×S1S^2\times S^1

Show that π3(S2×S1)≅Z\pi_3(S^2\times S^1) \cong \mathbb{Z}, using the universal cover S2×RS^2\times\mathbb{R} and π3(S2)≅Z\pi_3(S^2) \cong \mathbb{Z} (the Hopf fibration, 10A.1 A Zoo of Three-Manifolds). Why does the width argument therefore apply to S2×S1S^2\times S^1, although it is not simply connected?

Solution

Covering maps induce isomorphisms on πk\pi_k for k≥2k \geq 2, and S2×R≃S2S^2\times\mathbb{R} \simeq S^2, so π3(S2×S1)≅π3(S2)≅Z\pi_3(S^2\times S^1) \cong \pi_3(S^2) \cong \mathbb{Z}. The argument needs only a nontrivial class of sweepouts by 2-spheres, which π3≠0\pi_3 \neq 0 provides; simple connectivity is not used.

Exercise 2.7 Why aspherical manifolds escape

For the flat 3-torus: (a) explain why πk(T3)=0\pi_k(T^3) = 0 for k≥2k \geq 2, so every sweepout by 2-spheres is trivial and the width is 00; (b) check that the flat metric is a static Ricci flow that never becomes extinct; (c) explain why this does not contradict Theorem 2.3.

Solution

(a) The universal cover R3\mathbb{R}^3 is contractible. A trivial class contains sweepouts by arbitrarily small spheres, so W=0W = 0. (b) Ric⁡=0\operatorname{Ric} = 0, so g(t)=g(0)g(t) = g(0). (c) The theorem assumes MM is not aspherical; T3T^3 is aspherical, there is no nontrivial class, and the inequality says nothing.

Exercise 2.8 Rehearsal: the round sphere

Let g(t)g(t) be the round S3S^3 of radius r(t)r(t), r2=r02−4tr^2 = r_0^2 - 4t. (a) The width is realised by great 2-spheres: W(t)=4πr(t)2W(t) = 4\pi r(t)^2. Compute W′W'. (b) Compute −4π−12Rmin⁡W-4\pi - \frac12R_{\min}W and check that Lemma 2.2's analogue for spheres, W′≤−4π−12Rmin⁡WW' \leq -4\pi - \frac12R_{\min}W, holds with equality. (c) Compare the true extinction time with the bound from the weaker inequality W′≤−4πW' \leq -4\pi, valid when R≥0R \geq 0.

Solution

(a) W=4π(r02−4t)W = 4\pi(r_0^2 - 4t), so W′=−16πW' = -16\pi. (b) Rmin⁡=6r2R_{\min} = \frac{6}{r^2}, so −4π−12⋅6r2⋅4πr2=−4π−12π=−16π-4\pi - \frac12\cdot\frac{6}{r^2}\cdot4\pi r^2 = -4\pi - 12\pi = -16\pi: equality, because a great sphere is totally geodesic (∣A∣2=0|A|^2 = 0) and RR is constant. (c) True extinction: t=r024t = \frac{r_0^2}{4}. From W′≤−4πW' \leq -4\pi: W(0)/4π=r02W(0)/4\pi = r_0^2, four times too late. The curvature term does real work when R>0R > 0; when RR may be negative, it is the term that must be controlled.

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