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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.
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.
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 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
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 at , from the variation formula of 11A.2 How Curvature Evolves, is
Its principal symbol, obtained by replacing each by for a covector and keeping the second-order part, is
where . For a strictly parabolic equation the symbol would be negative definite, like for the heat equation. Here it is not. It vanishes on every (Exercise 3.4), the symbols of Lie derivatives . 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 , for example the initial metric, and define the vector field
which is a vector field because a difference of connections is a tensor (9A.2 Connections). It vanishes when . The Ricci–DeTurck flow is
The added term contributes exactly to the symbol (Exercise 3.5). It cancels the bad part, leaving , and in coordinates the equation becomes
a strictly parabolic quasilinear system, which has a unique smooth solution for a short time on a closed manifold (6A.7 Nonlinear Parabolic Equations).
For every smooth metric on a closed manifold there is and a smooth Ricci flow , , with .
Proof. Solve the Ricci–DeTurck flow with and background . Let be the diffeomorphisms solving the ODE , (they exist for the same time, by ODE theory on a compact manifold, 8A.6 Flows and the Lie Derivative). Set . For a family of diffeomorphisms generated by the vector fields , . With ,
by naturality of the Ricci tensor. And .
Uniqueness. Given two Ricci flows , 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 to , , which is itself strictly parabolic (Eells and Sampson, 1964; 6A.9 Calculus of Variations and Gradient Flows). Its solutions starting at the identity push forward to Ricci–DeTurck flows with the same initial data, which must coincide, and the 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.
For each and there is such that, if is a Ricci flow on a closed -manifold with on , then
The proof is Bernstein's method (6A.6 Parabolic Regularity): build a quantity from and lower derivatives whose heat-operator image has a good sign, and apply the maximum principle. For (Exercise 3.7), the evolution equations give
The function , with large, satisfies , so , which gives . Higher 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 smoothing for the ordinary heat equation.
How long the flow lasts
Let , , be a Ricci flow on a closed manifold, with maximal. Then as . In fact .
Proof. Suppose on . By Shi's estimates (applied on intervals of length ending at each time), all derivatives of are bounded on . Then is bounded, so the metrics are uniformly equivalent and converge as , smoothly, because all derivatives are bounded. Restarting the flow from the limit extends it beyond , contradicting maximality. For the rate: satisfies , so by the maximum principle (11A.4 Maximum Principles under Ricci Flow) satisfies in the sense of 9B.7 The Heat Equation on a Manifold. If were less than , the comparison ODE would keep finite past , contradicting the first part.
Nataša Šešum (2005) proved more: the Ricci curvature must blow up at a finite singular time. The sphere's curvature shows the rate is attained; singularities at this rate are called Type I (11B.4 Singularities).
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.
The symbol of is , which vanishes on the gauge directions : the flow is only weakly parabolic. DeTurck adds , with , to get a strictly parabolic flow, solves it, and pulls back by the flow of to get a Ricci flow: short-time existence on closed manifolds. Uniqueness follows through the harmonic map heat flow. Shi's estimates bound by from , by Bernstein's method. So the flow continues while curvature is bounded, and at a finite singular time . 11A.4 Maximum Principles under Ricci Flow develops the maximum principles.
Exercises
Show that for , for any vector (identify vectors and covectors with ). Show that is negative definite on the trace-free tensors orthogonal to these, for instance on with and .
Solution
and . Then . If and , then , negative definite on such .
Show that, to leading order, depends on the first derivatives of through , and deduce that the symbol of at is . Hence the Ricci–DeTurck operator has symbol .
Solution
-type terms, giving the stated form. Linearising in : , and . Replacing by : , the stated symbol. Adding it to leaves .
Let be diffeomorphisms with and a family of metrics. Show , using the definition of the Lie derivative (8A.6 Flows and the Lie Derivative) and the product rule.
Solution
Write with the flow from time to of , so . Then , and differentiating at gives .
Assume the two differential inequalities in the text, and . Let . Show , choose so the first term is , and deduce .
Solution
, dropping ; and . With , choosing makes the gradient terms nonpositive, so . By the maximum principle, . So .
For the shrinking round of initial radius , compute (with ) and show is constant. Compare with the lower bound of Theorem 3.3. Does the theorem rule out curvature blowing up faster than ?
Solution
For constant curvature , and , so , using . The product with 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 are called Type II (11B.4 Singularities).
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