Book 11A

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Course 11Book 11A: The Ricci Flow: Existence and Maximum PrinciplesChapter 3

Short-Time Existence and Uniqueness

Why the flow is only weakly parabolic, DeTurck’s trick, and Shi’s estimates.

20 min read · Updated Oct 3, 2026

Read with Topping's Lectures on the Ricci Flow, chapters 4 and 5 (short-time existence via DeTurck's trick, uniqueness, Shi's estimates), and Chow and Knopf's The Ricci Flow: An Introduction, chapter 3. DeTurck's paper "Deforming metrics in the direction of their Ricci tensors" (Journal of Differential Geometry, 1983) is two pages of essential reading.

In this chapter · 7 sections
  1. 3.1Gauge fixing
  2. 3.2Why the flow is only weakly parabolic
  3. 3.3DeTurck's trick
  4. 3.4Shi's derivative estimates
  5. 3.5How long the flow lasts
  6. 3.6History
  7. 3.7Exercises

Does the Ricci flow have a solution? For a heat equation the answer is standard: linearise, check that the linearisation is uniformly parabolic, and solve by a contraction or an implicit function argument (6A.7 Nonlinear Parabolic Equations). The Ricci flow fails the second step. Its diffeomorphism invariance (11A.1 The Equation and Its First Solutions) makes the linearised operator degenerate: in the directions of infinitesimal diffeomorphisms it does no smoothing at all. Hamilton's 1982 existence proof had to use the Nash–Moser inverse function theorem. A year later Dennis DeTurck found a short way around the degeneracy: add a carefully chosen diffeomorphism term to make the equation strictly parabolic, solve it, and then undo the diffeomorphisms.

This chapter proves short-time existence and uniqueness on closed manifolds. It then proves the derivative estimates of Wan-Xiong Shi, which show that a curvature bound controls all derivatives of curvature. From them follows the basic fact about singularities: the flow continues as long as the curvature stays bounded.

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

  • compute the principal symbol of −2Ric⁡-2\operatorname{Ric} and identify its kernel;
  • carry out DeTurck's trick and prove short-time existence on a closed manifold;
  • explain uniqueness through the harmonic map heat flow;
  • state and prove the first of Shi's derivative estimates;
  • prove that at a finite maximal existence time the curvature is unbounded.

Gauge fixing

In the world In use Numerical relativity

Einstein's equations of general relativity share the problem of this chapter. They are invariant under diffeomorphisms (changes of coordinates), so written naively they are not a well-posed evolution system. Yvonne Choquet-Bruhat proved local existence in 1952 by imposing harmonic coordinates, in which the equations become a system of nonlinear wave equations. Numerical relativity faced the same problem in practice: for decades, simulations of colliding black holes broke down. Frans Pretorius achieved the first successful simulation of a binary black hole merger through to the final black hole (Physical Review Letters, 2005). He used a generalised harmonic gauge: the coordinate conditions are added to the equations as source terms, together with terms that damp violations of the constraints. That is the same idea as DeTurck's trick: add a gauge term that makes the system strictly hyperbolic (for Einstein) or strictly parabolic (for Ricci flow), solve, and recover the geometric solution. The gravitational-wave signals detected by LIGO since 2015 are interpreted with waveforms computed by numerical relativity.

Why the flow is only weakly parabolic

The linearisation of g↦−2Ric⁡(g)g \mapsto -2\operatorname{Ric}(g) at gg, from the variation formula of 11A.2 How Curvature Evolves, is

h↦Δhjk+∇j∇ktr⁡h−∇m∇jhkm−∇m∇khjm+(lower order).h \mapsto \Delta h_{jk} + \nabla_j\nabla_k\operatorname{tr}h - \nabla^m\nabla_jh_{km} - \nabla^m\nabla_kh_{jm} + (\text{lower order}).

Its principal symbol, obtained by replacing each ∇\nabla by iξi\xi for a covector ξ\xi and keeping the second-order part, is

σ(ξ)h=−∣ξ∣2h+ξ⊗h(ξ)+h(ξ)⊗ξ−(tr⁡h) ξ⊗ξ,\sigma(\xi)h = -|\xi|^2h + \xi\otimes h(\xi) + h(\xi)\otimes\xi - (\operatorname{tr}h)\,\xi\otimes\xi,

where h(ξ)j=hjmξmh(\xi)_j = h_{jm}\xi^m. For a strictly parabolic equation the symbol would be negative definite, like −∣ξ∣2h-|\xi|^2h for the heat equation. Here it is not. It vanishes on every h=ξ⊗X+X⊗ξh = \xi\otimes X + X\otimes\xi (Exercise 3.4), the symbols of Lie derivatives LXg\mathcal L_Xg. Those are exactly the directions in which a metric moves when you pull it back by a diffeomorphism, and the Ricci flow cannot smooth them, because it does not see them.

DeTurck's trick

Fix a background metric g~\tilde g, for example the initial metric, and define the vector field

Wk=gij(Γijk−Γ~ijk),W^k = g^{ij}\big(\Gamma_{ij}^k - \tilde\Gamma_{ij}^k\big),

which is a vector field because a difference of connections is a tensor (9A.2 Connections). It vanishes when g=g~g = \tilde g. The Ricci–DeTurck flow is

∂tg^=−2Ric⁡(g^)+LWg^,(LWg^)ij=∇iWj+∇jWi.\partial_t\hat g = -2\operatorname{Ric}(\hat g) + \mathcal L_W\hat g, \qquad (\mathcal L_W\hat g)_{ij} = \nabla_iW_j + \nabla_jW_i.

The added term contributes exactly −ξ⊗h(ξ)−h(ξ)⊗ξ+(tr⁡h)ξ⊗ξ-\xi\otimes h(\xi) - h(\xi)\otimes\xi + (\operatorname{tr}h)\xi\otimes\xi to the symbol (Exercise 3.5). It cancels the bad part, leaving −∣ξ∣2h-|\xi|^2h, and in coordinates the equation becomes

∂tg^ij=g^ab∂a∂bg^ij+(lower order):\partial_t\hat g_{ij} = \hat g^{ab}\partial_a\partial_b\hat g_{ij} + (\text{lower order}):

a strictly parabolic quasilinear system, which has a unique smooth solution for a short time on a closed manifold (6A.7 Nonlinear Parabolic Equations).

Theorem 3.1 Short-time existence (Hamilton 1982, DeTurck 1983)

For every smooth metric g0g_0 on a closed manifold MM there is T>0T > 0 and a smooth Ricci flow g(t)g(t), t∈[0,T)t \in [0, T), with g(0)=g0g(0) = g_0.

Proof. Solve the Ricci–DeTurck flow g^(t)\hat g(t) with g^(0)=g0\hat g(0) = g_0 and background g~=g0\tilde g = g_0. Let ϕt\phi_t be the diffeomorphisms solving the ODE ∂tϕt=−W(ϕt,t)\partial_t\phi_t = -W(\phi_t, t), ϕ0=id⁡\phi_0 = \operatorname{id} (they exist for the same time, by ODE theory on a compact manifold, 8A.6 Flows and the Lie Derivative). Set g(t)=ϕt∗g^(t)g(t) = \phi_t^*\hat g(t). For a family of diffeomorphisms generated by the vector fields VtV_t, ∂t(ϕt∗g^)=ϕt∗(∂tg^+LVtg^)\partial_t(\phi_t^*\hat g) = \phi_t^*(\partial_t\hat g + \mathcal L_{V_t}\hat g). With Vt=−WV_t = -W,

∂tg=ϕt∗(−2Ric⁡(g^)+LWg^−LWg^)=−2Ric⁡(ϕt∗g^)=−2Ric⁡(g),\partial_tg = \phi_t^*\big(-2\operatorname{Ric}(\hat g) + \mathcal L_W\hat g - \mathcal L_W\hat g\big) = -2\operatorname{Ric}(\phi_t^*\hat g) = -2\operatorname{Ric}(g),

by naturality of the Ricci tensor. And g(0)=g0g(0) = g_0.

Figure 3.1. DeTurck's trick. Solve the strictly parabolic Ricci–DeTurck flow from g0g_0, then pull back by the diffeomorphisms ϕt\phi_t generated by −W-W. The result is a Ricci flow from the same initial metric. The two flows differ only by a change of coordinates, so they have the same geometry.

Uniqueness. Given two Ricci flows g1(t)g_1(t), g2(t)g_2(t) with the same initial metric, one wants to reverse the construction: find diffeomorphisms turning each into a Ricci–DeTurck flow, and then use uniqueness for that strictly parabolic system. The needed diffeomorphisms solve the harmonic map heat flow from (M,gi(t))(M, g_i(t)) to (M,g~)(M, \tilde g), ∂tϕ=Δgi(t),g~ϕ\partial_t\phi = \Delta_{g_i(t), \tilde g}\phi, which is itself strictly parabolic (Eells and Sampson, 1964; 6A.9 Calculus of Variations and Gradient Flows). Its solutions starting at the identity push gi(t)g_i(t) forward to Ricci–DeTurck flows with the same initial data, which must coincide, and the gig_i are then recovered from them. Hamilton gave this argument for closed manifolds. Bing-Long Chen and Xi-Ping Zhu (2006) proved uniqueness among complete flows with bounded curvature, which matters for the noncompact limits of 11B.3 Compactness of Ricci Flows.

Shi's derivative estimates

A bound on curvature controls all its derivatives after any positive time: the flow is smoothing, like a heat equation.

Theorem 3.2 Shi's estimates (global version)

For each nn and k≥1k \geq 1 there is CkC_k such that, if g(t)g(t) is a Ricci flow on a closed nn-manifold with ∣Rm⁡∣≤K|\operatorname{Rm}| \leq K on M×[0,1K]M\times[0, \frac1K], then

∣∇kRm⁡∣≤CkKtk/2on M×(0,1K].|\nabla^k\operatorname{Rm}| \leq \frac{C_kK}{t^{k/2}} \qquad\text{on } M\times(0, \tfrac1K].

The proof is Bernstein's method (6A.6 Parabolic Regularity): build a quantity from ∣∇kRm⁡∣2|\nabla^k\operatorname{Rm}|^2 and lower derivatives whose heat-operator image has a good sign, and apply the maximum principle. For k=1k = 1 (Exercise 3.7), the evolution equations give

(∂t−Δ)∣Rm⁡∣2≤−2∣∇Rm⁡∣2+C∣Rm⁡∣3,(∂t−Δ)∣∇Rm⁡∣2≤−2∣∇2Rm⁡∣2+C∣Rm⁡∣∣∇Rm⁡∣2.(\partial_t - \Delta)|\operatorname{Rm}|^2 \leq -2|\nabla\operatorname{Rm}|^2 + C|\operatorname{Rm}|^3, \qquad (\partial_t - \Delta)|\nabla\operatorname{Rm}|^2 \leq -2|\nabla^2\operatorname{Rm}|^2 + C|\operatorname{Rm}||\nabla\operatorname{Rm}|^2.

The function F=t∣∇Rm⁡∣2+β∣Rm⁡∣2F = t|\nabla\operatorname{Rm}|^2 + \beta|\operatorname{Rm}|^2, with β\beta large, satisfies (∂t−Δ)F≤CβK3(\partial_t - \Delta)F \leq C\beta K^3, so F≤βK2+CβK2F \leq \beta K^2 + C\beta K^2, which gives ∣∇Rm⁡∣2≤CK2t|\nabla\operatorname{Rm}|^2 \leq \frac{CK^2}{t}. Higher kk follow by induction, each step using the bounds already proved (2A.1 The Natural Numbers). Shi (1989) also proved local versions, on balls, which are what blow-up arguments use (11B.3 Compactness of Ricci Flows). Figure 3.2 shows the same t−1/2t^{-1/2} smoothing for the ordinary heat equation.

Figure 3.2. The model for Shi's estimates: the heat equation on a circle of length 2π2\pi, started from a step function (computed from its Fourier series). The maximum of ∣ux∣|u_x| (accent) decays like 12πt\frac{1}{2\sqrt{\pi t}} (dashed) for small tt: a bounded solution has derivatives bounded by Ct−1/2Ct^{-1/2}, whatever its initial roughness.

How long the flow lasts

Theorem 3.3 Curvature blows up at a finite singular time

Let g(t)g(t), t∈[0,T)t \in [0, T), be a Ricci flow on a closed manifold, with T<∞T < \infty maximal. Then sup⁡M∣Rm⁡(⋅,t)∣→∞\sup_M|\operatorname{Rm}(\cdot, t)| \to \infty as t→Tt \to T. In fact sup⁡M∣Rm⁡(⋅,t)∣≥cnT−t\sup_M|\operatorname{Rm}(\cdot, t)| \geq \frac{c_n}{T - t}.

Proof. Suppose ∣Rm⁡∣≤K|\operatorname{Rm}| \leq K on [0,T)[0, T). By Shi's estimates (applied on intervals of length 1K\frac1K ending at each time), all derivatives of Rm⁡\operatorname{Rm} are bounded on [T2,T)[\frac T2, T). Then ∂tg=−2Ric⁡\partial_tg = -2\operatorname{Ric} is bounded, so the metrics are uniformly equivalent and converge as t→Tt \to T, smoothly, because all derivatives are bounded. Restarting the flow from the limit g(T)g(T) extends it beyond TT, contradicting maximality. For the rate: ∣Rm⁡∣2|\operatorname{Rm}|^2 satisfies (∂t−Δ)∣Rm⁡∣2≤C∣Rm⁡∣3(\partial_t - \Delta)|\operatorname{Rm}|^2 \leq C|\operatorname{Rm}|^3, so by the maximum principle (11A.4 Maximum Principles under Ricci Flow) κ(t)=sup⁡∣Rm⁡∣\kappa(t) = \sup|\operatorname{Rm}| satisfies κ′≤C2κ2\kappa' \leq \frac C2\kappa^2 in the sense of 9B.7 The Heat Equation on a Manifold. If κ(t0)\kappa(t_0) were less than 2C(T−t0)\frac{2}{C(T - t_0)}, the comparison ODE would keep κ\kappa finite past TT, contradicting the first part.

Nataša Šešum (2005) proved more: the Ricci curvature must blow up at a finite singular time. The sphere's curvature 12(n−1)(T−t)\frac{1}{2(n - 1)(T - t)} shows the rate 1T−t\frac{1}{T - t} is attained; singularities at this rate are called Type I (11B.4 Singularities).

Where this goes From existence to control

Short-time existence gives a flow; Shi's estimates and the blow-up criterion say that understanding the flow means controlling curvature. 11A.4 Maximum Principles under Ricci Flow provides the maximum principles that do this, and 11B.3 Compactness of Ricci Flows uses Shi's estimates to extract limits of rescaled flows near singularities.

History

Hamilton proved short-time existence in 1982 with the Nash–Moser implicit function theorem. DeTurck's trick appeared in 1983, with an improved version in 2003. Eells and Sampson introduced the harmonic map heat flow in 1964. Wan-Xiong Shi proved his derivative estimates, global and local, in 1989, and existence on complete noncompact manifolds with bounded curvature the same year. Chen and Zhu's uniqueness theorem dates from 2006, and Šešum's Ricci blow-up theorem from 2005. Choquet-Bruhat's harmonic-gauge existence theorem for Einstein's equations is from 1952, and Pretorius's binary black hole simulation from 2005.

Recall Where we stand

The symbol of −2Ric⁡-2\operatorname{Ric} is −∣ξ∣2h+ξ⊗h(ξ)+h(ξ)⊗ξ−(tr⁡h)ξ⊗ξ-|\xi|^2h + \xi\otimes h(\xi) + h(\xi)\otimes\xi - (\operatorname{tr}h)\xi\otimes\xi, which vanishes on the gauge directions ξ⊗X+X⊗ξ\xi\otimes X + X\otimes\xi: the flow is only weakly parabolic. DeTurck adds LWg^\mathcal L_W\hat g, with W=gij(Γ−Γ~)ijW = g^{ij}(\Gamma - \tilde\Gamma)_{ij}, to get a strictly parabolic flow, solves it, and pulls back by the flow of −W-W to get a Ricci flow: short-time existence on closed manifolds. Uniqueness follows through the harmonic map heat flow. Shi's estimates bound ∣∇kRm⁡∣|\nabla^k\operatorname{Rm}| by CkKt−k/2C_kKt^{-k/2} from ∣Rm⁡∣≤K|\operatorname{Rm}| \leq K, by Bernstein's method. So the flow continues while curvature is bounded, and at a finite singular time sup⁡∣Rm⁡∣≥cT−t\sup|\operatorname{Rm}| \geq \frac{c}{T - t}. 11A.4 Maximum Principles under Ricci Flow develops the maximum principles.

Exercises

Exercise 3.4 The kernel of the symbol

Show that σ(ξ)h=0\sigma(\xi)h = 0 for h=ξ⊗X+X⊗ξh = \xi\otimes X + X\otimes\xi, for any vector XX (identify vectors and covectors with gg). Show that σ(ξ)\sigma(\xi) is negative definite on the trace-free tensors orthogonal to these, for instance on hh with h(ξ)=0h(\xi) = 0 and tr⁡h=0\operatorname{tr}h = 0.

Solution

h(ξ)=ξ⟨X,ξ⟩+X∣ξ∣2h(\xi) = \xi\langle X, \xi\rangle + X|\xi|^2 and tr⁡h=2⟨X,ξ⟩\operatorname{tr}h = 2\langle X, \xi\rangle. Then σ(ξ)h=−∣ξ∣2(ξ⊗X+X⊗ξ)+ξ⊗(ξ⟨X,ξ⟩+X∣ξ∣2)+(ξ⟨X,ξ⟩+X∣ξ∣2)⊗ξ−2⟨X,ξ⟩ξ⊗ξ=0\sigma(\xi)h = -|\xi|^2(\xi\otimes X + X\otimes\xi) + \xi\otimes(\xi\langle X, \xi\rangle + X|\xi|^2) + (\xi\langle X, \xi\rangle + X|\xi|^2)\otimes\xi - 2\langle X, \xi\rangle\xi\otimes\xi = 0. If h(ξ)=0h(\xi) = 0 and tr⁡h=0\operatorname{tr}h = 0, then σ(ξ)h=−∣ξ∣2h\sigma(\xi)h = -|\xi|^2h, negative definite on such hh.

Exercise 3.5 The DeTurck term repairs the symbol

Show that, to leading order, Wk=gij(Γijk−Γ~ijk)W^k = g^{ij}(\Gamma_{ij}^k - \tilde\Gamma_{ij}^k) depends on the first derivatives of gg through Wk=gij∂igjk−12∂ktr⁡g+(zero order)W_k = g^{ij}\partial_ig_{jk} - \frac12\partial_k\operatorname{tr}g + (\text{zero order}), and deduce that the symbol of h↦LWgh \mapsto \mathcal L_Wg at gg is −ξ⊗h(ξ)−h(ξ)⊗ξ+(tr⁡h)ξ⊗ξ-\xi\otimes h(\xi) - h(\xi)\otimes\xi + (\operatorname{tr}h)\xi\otimes\xi. Hence the Ricci–DeTurck operator has symbol −∣ξ∣2h-|\xi|^2h.

Solution

glkgijΓijl=12gij(∂igjk+∂jgik−∂kgij)=gij∂igjk−12∂k(gijgij)g_{lk}g^{ij}\Gamma_{ij}^l = \frac12g^{ij}(\partial_ig_{jk} + \partial_jg_{ik} - \partial_kg_{ij}) = g^{ij}\partial_ig_{jk} - \frac12\partial_k(g^{ij}g_{ij})-type terms, giving the stated form. Linearising in hh: Wk≈∇ihik−12∇ktr⁡hW_k \approx \nabla^ih_{ik} - \frac12\nabla_k\operatorname{tr}h, and LWg=∇jWk+∇kWj≈∇j∇ihik+∇k∇ihij−∇j∇ktr⁡h\mathcal L_Wg = \nabla_jW_k + \nabla_kW_j \approx \nabla_j\nabla^ih_{ik} + \nabla_k\nabla^ih_{ij} - \nabla_j\nabla_k\operatorname{tr}h. Replacing ∇\nabla by iξi\xi: −ξjξihik−ξkξihij+ξjξktr⁡h-\xi_j\xi^ih_{ik} - \xi_k\xi^ih_{ij} + \xi_j\xi_k\operatorname{tr}h, the stated symbol. Adding it to σ(ξ)\sigma(\xi) leaves −∣ξ∣2h-|\xi|^2h.

Exercise 3.6 Differentiating a pullback

Let ϕt\phi_t be diffeomorphisms with ∂tϕt=Vt∘ϕt\partial_t\phi_t = V_t\circ\phi_t and g^(t)\hat g(t) a family of metrics. Show ∂t(ϕt∗g^(t))=ϕt∗(∂tg^+LVtg^)\partial_t(\phi_t^*\hat g(t)) = \phi_t^*\big(\partial_t\hat g + \mathcal L_{V_t}\hat g\big), using the definition of the Lie derivative (8A.6 Flows and the Lie Derivative) and the product rule.

Solution

Write ϕt+s=ψt,s∘ϕt\phi_{t + s} = \psi_{t, s}\circ\phi_t with ψt,s\psi_{t, s} the flow from time tt to t+st + s of VV, so dds∣0ψt,s∗=LVt\frac{d}{ds}\big|_0\psi_{t, s}^* = \mathcal L_{V_t}. Then ϕt+s∗g^(t+s)=ϕt∗ψt,s∗g^(t+s)\phi_{t + s}^*\hat g(t + s) = \phi_t^*\psi_{t, s}^*\hat g(t + s), and differentiating at s=0s = 0 gives ϕt∗(LVtg^(t)+∂tg^(t))\phi_t^*(\mathcal L_{V_t}\hat g(t) + \partial_t\hat g(t)).

Exercise 3.7 Shi's estimate for k=1k = 1

Assume the two differential inequalities in the text, ∣Rm⁡∣≤K|\operatorname{Rm}| \leq K and 0<t≤1K0 < t \leq \frac1K. Let F=t∣∇Rm⁡∣2+β∣Rm⁡∣2F = t|\nabla\operatorname{Rm}|^2 + \beta|\operatorname{Rm}|^2. Show (∂t−Δ)F≤∣∇Rm⁡∣2(1+Ct∣Rm⁡∣−2β)+Cβ∣Rm⁡∣3(\partial_t - \Delta)F \leq |\nabla\operatorname{Rm}|^2(1 + Ct|\operatorname{Rm}| - 2\beta) + C\beta|\operatorname{Rm}|^3, choose β\beta so the first term is ≤0\leq 0, and deduce ∣∇Rm⁡∣2≤β(1+C)K2t|\nabla\operatorname{Rm}|^2 \leq \frac{\beta(1 + C)K^2}{t}.

Solution

(∂t−Δ)(t∣∇Rm⁡∣2)=∣∇Rm⁡∣2+t(∂t−Δ)∣∇Rm⁡∣2≤∣∇Rm⁡∣2+Ct∣Rm⁡∣∣∇Rm⁡∣2(\partial_t - \Delta)(t|\nabla\operatorname{Rm}|^2) = |\nabla\operatorname{Rm}|^2 + t(\partial_t - \Delta)|\nabla\operatorname{Rm}|^2 \leq |\nabla\operatorname{Rm}|^2 + Ct|\operatorname{Rm}||\nabla\operatorname{Rm}|^2, dropping −2t∣∇2Rm⁡∣2-2t|\nabla^2\operatorname{Rm}|^2; and β(∂t−Δ)∣Rm⁡∣2≤−2β∣∇Rm⁡∣2+Cβ∣Rm⁡∣3\beta(\partial_t - \Delta)|\operatorname{Rm}|^2 \leq -2\beta|\nabla\operatorname{Rm}|^2 + C\beta|\operatorname{Rm}|^3. With t∣Rm⁡∣≤tK≤1t|\operatorname{Rm}| \leq tK \leq 1, choosing 2β≥1+C2\beta \geq 1 + C makes the gradient terms nonpositive, so (∂t−Δ)F≤CβK3(\partial_t - \Delta)F \leq C\beta K^3. By the maximum principle, F(t)≤F(0)+CβK3t≤βK2+CβK2F(t) \leq F(0) + C\beta K^3t \leq \beta K^2 + C\beta K^2. So t∣∇Rm⁡∣2≤β(1+C)K2t|\nabla\operatorname{Rm}|^2 \leq \beta(1 + C)K^2.

Exercise 3.8 Rehearsal: the blow-up rate on the sphere

For the shrinking round SnS^n of initial radius 11, compute ∣Rm⁡∣|\operatorname{Rm}| (with ∣Rm⁡∣2=RijklRijkl|\operatorname{Rm}|^2 = R_{ijkl}R^{ijkl}) and show ∣Rm⁡∣(T−t)|\operatorname{Rm}|(T - t) is constant. Compare with the lower bound of Theorem 3.3. Does the theorem rule out curvature blowing up faster than 1T−t\frac{1}{T - t}?

Solution

For constant curvature κ=1r2\kappa = \frac{1}{r^2}, Rijkl=κ(gilgjk−gikgjl)R_{ijkl} = \kappa(g_{il}g_{jk} - g_{ik}g_{jl}) and ∣Rm⁡∣2=2n(n−1)κ2|\operatorname{Rm}|^2 = 2n(n - 1)\kappa^2, so ∣Rm⁡∣=2n(n−1) κ=2n(n−1)2(n−1)(T−t)|\operatorname{Rm}| = \sqrt{2n(n - 1)}\,\kappa = \frac{\sqrt{2n(n - 1)}}{2(n - 1)(T - t)}, using r2=2(n−1)(T−t)r^2 = 2(n - 1)(T - t). The product with T−tT - t is constant, matching the lower bound's rate. The theorem does not rule out faster blow-up: it gives only a lower bound, and singularities that blow up faster than CT−t\frac{C}{T - t} are called Type II (11B.4 Singularities).

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