Book 12A

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Course 12Book 12A: Entropy and NoncollapsingChapter 7

Monotonicity of the Reduced Volume

The 𝓛-exponential map and its Jacobian, the injectivity domain, the limit at Ο„ = 0, barrier inequalities on complete flows, and min β„“ ≀ n/2, following Morgan and Tian's chapters 6 and 7.

38 min read Β· Updated Oct 23, 2026

Read Perelman I, Β§7.1, from (7.11) to the end of the subsection, with Morgan and Tian, chapter 6, Β§Β§2–3 and Β§7 (the L\mathcal L-exponential map, the injectivity domain, Proposition 6.78 on the limit at Ο„=0\tau = 0, Theorem 6.80 and Proposition 6.81 on monotonicity), and chapter 7, Β§Β§1–2 (complete flows of bounded curvature, the barrier inequality of Proposition 7.8 and Theorem 7.10, min⁑ℓ≀n2\min\ell \leq \frac n2). The Riemannian model is the proof of Bishop–Gromov by integrating the Jacobian of the exponential map over the interior of the cut locus (9B.2 Volume Comparison).

In this chapter Β· 6 sections
  1. 7.1The L\mathcal LL-exponential map and its injectivity domain
  2. 7.2Flat space and rescaling
  3. 7.3The Jacobian inequality
  4. 7.4The barrier sense and min⁑ℓ≀n2\min\ell \leq \frac n2minℓ≀2n​
  5. 7.5History
  6. 7.6Exercises
  7. β†—Free resources

12A.6 𝓛-Geodesics and the Variational Formulas proved Perelman's differential inequalities for the reduced distance at points where it is smooth: where the minimising L\mathcal L-geodesic is unique and nondegenerate. This chapter removes that assumption and proves, with full care, the two consequences used in the rest of the proof of the PoincarΓ© conjecture: the reduced volume is nonincreasing in Ο„\tau, with limit 11 as Ο„β†’0\tau \to 0, and min⁑ℓ(β‹…,Ο„)≀n2\min\ell(\cdot, \tau) \leq \frac n2 for every Ο„\tau.

The strategy is the one used for Bishop–Gromov (9B.2 Volume Comparison). There, one never differentiates the volume of a ball directly; one pulls the volume back to the tangent space by the exponential map, writes it as an integral of the Jacobian over the region inside the cut locus, and shows that the Jacobian, suitably normalised, is monotone along each geodesic and that the region shrinks. Perelman's proof of the monotonicity of V~\tilde V does exactly this, with the L\mathcal L-exponential map in place of the exponential map, the "injectivity domain" in place of the interior of the cut locus, and the quantity Ο„βˆ’n/2eβˆ’β„“J\tau^{-n/2}e^{-\ell}J in place of r1βˆ’nJr^{1-n}J. Nothing needs to be differentiated across the set where β„“\ell is not smooth, because that set is never seen: it is the image of the boundary of a region in the tangent space, and has measure zero. The bound min⁑ℓ≀n2\min\ell \leq \frac n2 needs a different technique, the maximum principle in the barrier sense, which is the space-time version of Calabi's trick for the Laplacian of the distance function.

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

  • define the L\mathcal L-exponential map, the injectivity set in the tangent space and the injectivity domain, and prove that the injectivity sets shrink as Ο„\tau increases;
  • compute the Jacobian of Lexp⁑\mathcal L\exp on flat space and show that Ο„βˆ’n/2eβˆ’β„“~J\tau^{-n/2}e^{-\tilde\ell}J is invariant under parabolic rescaling;
  • prove that Ο„βˆ’n/2eβˆ’β„“~Jβ†’2neβˆ’βˆ£v∣2\tau^{-n/2}e^{-\tilde\ell}J \to 2^ne^{-|v|^2} as Ο„β†’0\tau \to 0, and hence V~(Ο„)β†’1\tilde V(\tau) \to 1;
  • prove Perelman's Jacobian inequality (7.12) and the identity ddΟ„β„“~=βˆ’12Ο„βˆ’3/2K\frac{d}{d\tau}\tilde\ell = -\frac12\tau^{-3/2}K along L\mathcal L-geodesics, and conclude the monotonicity of V~\tilde V and V~≀1\tilde V \leq 1;
  • explain the localised reduced volume of a subset, the version used for flows with surgery;
  • define upper barriers and prove βˆ‚Ο„β„“+Δℓ≀n/2βˆ’β„“Ο„\partial_\tau\ell + \Delta\ell \leq \frac{n/2 - \ell}{\tau} in the barrier sense, and deduce min⁑ℓ≀n2\min\ell \leq \frac n2;
  • describe what is known about the regularity of β„“\ell on complete flows (local Lipschitz, smooth off a closed null set, the inequalities in the distributional sense).

The L\mathcal L-exponential map and its injectivity domain

Fix a base point x=(p,T)x = (p, T) in space-time and work in backward time Ο„=Tβˆ’t\tau = T - t. For v∈TpMv \in T_pM, let Ξ³v\gamma_v be the L\mathcal L-geodesic with Ξ³v(0)=p\gamma_v(0) = p and lim⁑τ→0Ο„X(Ο„)=v\lim_{\tau\to0}\sqrt\tau X(\tau) = v (12A.6 𝓛-Geodesics and the Variational Formulas), and define

Lexp⁑τ(v)=Ξ³v(Ο„),L~(v,Ο„)=L(Ξ³v∣[0,Ο„]),β„“~(v,Ο„)=L~(v,Ο„)2Ο„.\mathcal L\exp_\tau(v) = \gamma_v(\tau), \qquad \tilde L(v, \tau) = \mathcal L\big(\gamma_v|_{[0, \tau]}\big), \qquad \tilde\ell(v, \tau) = \frac{\tilde L(v, \tau)}{2\sqrt\tau}.

These are smooth where defined, by smooth dependence of solutions of the (regular, in s=Ο„s = \sqrt\tau) geodesic ODE on initial data. The tildes mark functions on the tangent space, as opposed to L(q,Ο„)L(q, \tau) and β„“(q,Ο„)\ell(q, \tau), which are functions on space-time defined by minimisation.

The differential. The derivative of Lexp⁑τ\mathcal L\exp_\tau at vv in the direction ww is Yw(Ο„)Y_w(\tau), where YwY_w is the L\mathcal L-Jacobi field along Ξ³v\gamma_v with Yw(0)=0Y_w(0) = 0 and limβ‘Ο„βˆ‡XYw=w\lim\sqrt\tau\nabla_XY_w = w (Morgan–Tian, Lemma 6.19). So Lexp⁑τ\mathcal L\exp_\tau is a local diffeomorphism at vv exactly when no nonzero L\mathcal L-Jacobi field along Ξ³v\gamma_v vanishes at 00 and at Ο„\tau. Near Ο„=0\tau = 0 this always holds (their Lemma 6.23): in the variable ss the Jacobi equation is regular, and a Jacobi field with Y(0)=0Y(0) = 0 and nonzero initial derivative is nonzero for small ss.

The injectivity set. Following Morgan and Tian (Definition 6.25), let U~(Ο„)βŠ†TpM\tilde U(\tau) \subseteq T_pM be the set of vv such that Lexp⁑τ\mathcal L\exp_\tau is a local diffeomorphism at vv and, for all vβ€²v' near vv, the geodesic Ξ³vβ€²βˆ£[0,Ο„]\gamma_{v'}|_{[0,\tau]} is the unique minimiser of L\mathcal L between its endpoints. Its image U(Ο„)=Lexp⁑τ(U~(Ο„))βŠ†MU(\tau) = \mathcal L\exp_\tau(\tilde U(\tau)) \subseteq M is the injectivity domain at time Ο„\tau. On it:

  • Lexp⁑τ:U~(Ο„)β†’U(Ο„)\mathcal L\exp_\tau : \tilde U(\tau) \to U(\tau) is a diffeomorphism onto an open set, and L(β‹…,Ο„)L(\cdot, \tau) and β„“(β‹…,Ο„)\ell(\cdot, \tau) are smooth on U(Ο„)U(\tau) with L∘Lexp⁑τ=L~L\circ\mathcal L\exp_\tau = \tilde L (their Proposition 6.28);
  • all the computations of 12A.6 𝓛-Geodesics and the Variational Formulas are valid, in particular (7.13)–(7.15).
Proposition 7.1 The injectivity sets shrink

If Ο„β€²>Ο„\tau' > \tau, then U~(Ο„β€²)βŠ†U~(Ο„)\tilde U(\tau') \subseteq \tilde U(\tau).

Proof. (Morgan–Tian, Proposition 6.30.) Let v∈U~(Ο„β€²)v \in \tilde U(\tau'). Uniqueness. Suppose another path Οƒ\sigma from pp to Ξ³v(Ο„)\gamma_v(\tau) had L(Οƒ)≀L(Ξ³v∣[0,Ο„])\mathcal L(\sigma) \leq \mathcal L(\gamma_v|_{[0,\tau]}). Then the broken path, Οƒ\sigma followed by Ξ³v∣[Ο„,Ο„β€²]\gamma_v|_{[\tau, \tau']}, has L\mathcal L-length at most that of Ξ³v∣[0,Ο„β€²]\gamma_v|_{[0,\tau']}, which is minimising; so the broken path is minimising too, hence an L\mathcal L-geodesic, hence smooth, hence (by uniqueness for the ODE) equal to Ξ³v\gamma_v. Nondegeneracy. Suppose dLexp⁑τd\mathcal L\exp_\tau were singular at vv, and let Ο„2≀τ\tau_2 \leq \tau be the first such time. Then there is a nonzero L\mathcal L-Jacobi field YY along Ξ³v∣[0,Ο„2]\gamma_v|_{[0,\tau_2]} vanishing at both ends, along which the second variation of L\mathcal L is zero. Extend YY by zero on [Ο„2,Ο„β€²][\tau_2, \tau']; the extended field is a variation of the minimiser Ξ³v∣[0,Ο„β€²]\gamma_v|_{[0,\tau']} with zero second variation, so (by the characterisation of null directions of the second variation of a minimiser, 12A.6 𝓛-Geodesics and the Variational Formulas) it would be an L\mathcal L-Jacobi field on all of [0,Ο„β€²][0, \tau']. But it is not smooth at Ο„2\tau_2, where YY vanishes with nonzero derivative. The same arguments apply to nearby vβ€²v', so v∈U~(Ο„)v \in \tilde U(\tau).

The proposition is the analogue of the fact that the interior of the cut locus is star-shaped: a geodesic that is minimising and nondegenerate up to time Ο„β€²\tau' is so at every earlier time. For a Ricci flow on a closed manifold, or a complete one of bounded curvature, the complement of U(Ο„)U(\tau) in MM is closed and of measure zero (Morgan–Tian, Proposition 7.5), as the cut locus is in Riemannian geometry; minimising L\mathcal L-geodesics exist from xx to every point (their Lemma 7.2); and LL and β„“\ell are locally Lipschitz on space-time (their Proposition 6.56). So the reduced volume can be computed by integrating over U(Ο„)U(\tau), and pulled back to U~(Ο„)\tilde U(\tau) by the change of variables formula:

V~(Ο„)=∫M(4πτ)βˆ’n/2eβˆ’β„“(q,Ο„) dVg(Ο„)(q)=∫U~(Ο„)(4πτ)βˆ’n/2eβˆ’β„“~(v,Ο„)J(v,Ο„) dv,\tilde V(\tau) = \int_M(4\pi\tau)^{-n/2}e^{-\ell(q,\tau)}\,dV_{g(\tau)}(q) = \int_{\tilde U(\tau)}(4\pi\tau)^{-n/2}e^{-\tilde\ell(v,\tau)}J(v, \tau)\,dv,

where J(v,Ο„)J(v, \tau) is the Jacobian determinant of Lexp⁑τ\mathcal L\exp_\tau at vv, computed with the metric g(T)g(T) on TpMT_pM and g(Ο„)g(\tau) on MM.

Flat space and rescaling

On static flat Rn\mathbb{R}^n, Lexp⁑τ(v)=p+2Ο„v\mathcal L\exp_\tau(v) = p + 2\sqrt\tau v, so J=2nΟ„n/2J = 2^n\tau^{n/2}, and β„“~(v,Ο„)=∣2Ο„v∣24Ο„=∣v∣2\tilde\ell(v, \tau) = \frac{|2\sqrt\tau v|^2}{4\tau} = |v|^2. Hence

Ο„βˆ’n/2eβˆ’β„“~(v,Ο„)J(v,Ο„)=2neβˆ’βˆ£v∣2,\tau^{-n/2}e^{-\tilde\ell(v, \tau)}J(v, \tau) = 2^ne^{-|v|^2},

independent of Ο„\tau (Morgan–Tian, Claim 6.77). Since ∫Rn2neβˆ’βˆ£v∣2dv=2nΟ€n/2=(4Ο€)n/2\int_{\mathbb{R}^n}2^ne^{-|v|^2}dv = 2^n\pi^{n/2} = (4\pi)^{n/2}, the normalised reduced volume of flat space is exactly 11. This explains the normalisation: the guide's V~\tilde V includes (4Ο€)βˆ’n/2(4\pi)^{-n/2} so that the model value is 11; Perelman and Morgan–Tian omit it, and their model value is (4Ο€)n/2(4\pi)^{n/2} (12A.1 How to Read Perelman).

Parabolic rescaling. Let gQ(t)=Qg(T+(tβˆ’T)/Q)g_Q(t) = Qg(T + (t - T)/Q) be the flow rescaled by QQ about the time TT, so Ο„Q=QΟ„\tau_Q = Q\tau. Then L\mathcal L-lengths scale as LQ=Q L\mathcal L_Q = \sqrt Q\,\mathcal L, the initial vectors as vQ=Qβˆ’1/2vv_Q = Q^{-1/2}v measured in gQ(T)=Qg(T)g_Q(T) = Qg(T) (so ∣vQ∣gQ=∣v∣g|v_Q|_{g_Q} = |v|_g), the reduced distance is invariant, and the Jacobian satisfies JQ=Qn/2JJ_Q = Q^{n/2}J (Morgan–Tian, Lemma 6.75). Consequently

Ο„Qβˆ’n/2eβˆ’β„“~QJQ=Ο„βˆ’n/2eβˆ’β„“~J:\tau_Q^{-n/2}e^{-\tilde\ell_Q}J_Q = \tau^{-n/2}e^{-\tilde\ell}J:

the integrand of the reduced volume, and the reduced volume itself, are scale invariant. This is what makes V~\tilde V useful for blow-up arguments: it is unchanged by the rescalings that produce blow-up limits, as W\mathcal W is (12A.3 The 𝓦-Entropy).

Proposition 7.2 The limit at Ο„=0\tau = 0

For every A<∞A < \infty, as Ο„β†’0\tau \to 0, Ο„βˆ’n/2eβˆ’β„“~(v,Ο„)J(v,Ο„)β†’2neβˆ’βˆ£v∣2\tau^{-n/2}e^{-\tilde\ell(v,\tau)}J(v, \tau) \to 2^ne^{-|v|^2} uniformly for ∣vβˆ£β‰€A|v| \leq A; and for Ο„\tau small, the ball {∣vβˆ£β‰€A}\{|v| \leq A\} lies in U~(Ο„)\tilde U(\tau). Consequently lim⁑τ→0V~(Ο„)=1\lim_{\tau\to0}\tilde V(\tau) = 1.

Proof. (Morgan–Tian, Proposition 6.78 and Corollary 6.79, in outline.) Take Ο„kβ†’0\tau_k \to 0 and rescale by Qk=Ο„kβˆ’1Q_k = \tau_k^{-1}, so that the time Ο„k\tau_k becomes time 11. On a fixed parabolic neighbourhood of (p,T)(p, T) the original flow is smooth with bounded derivatives of all orders, so the rescaled flows converge smoothly, on parabolic regions of any fixed size, to the static flat metric on Rn\mathbb{R}^n. The L\mathcal L-geodesic ODE in the variable ss is regular, so the rescaled L\mathcal L-exponential maps converge smoothly on bounded sets to the flat one. By scale invariance, Ο„kβˆ’n/2eβˆ’β„“~J\tau_k^{-n/2}e^{-\tilde\ell}J at (v,Ο„k)(v, \tau_k) equals the rescaled quantity at (v,1)(v, 1), which converges to the flat value 2neβˆ’βˆ£v∣22^ne^{-|v|^2}, uniformly for ∣vβˆ£β‰€A|v| \leq A. For the injectivity statement: for Ο„\tau small, Ο„βˆ£X∣\sqrt\tau|X| is almost constant along L\mathcal L-geodesics (a Gronwall argument using bounds on Ric⁑\operatorname{Ric} and βˆ‡R\nabla R: their Lemma 6.60), so L(Ξ³v∣[0,Ο„])β‰ˆ2Ο„βˆ£v∣2\mathcal L(\gamma_v|_{[0,\tau]}) \approx 2\sqrt\tau|v|^2, and geodesics with ∣vβˆ£β‰€A|v| \leq A are shorter than any geodesic with ∣v∣β‰₯3A|v| \geq 3A reaching the same point, while Lexp⁑τ\mathcal L\exp_\tau is a diffeomorphism on the ball of radius 3A3A; so they are unique minimisers. The limit of V~\tilde V follows from the uniform convergence on balls, the monotonicity below (which gives a dominating function, 2neβˆ’βˆ£v∣22^ne^{-|v|^2} itself), and dominated convergence.

The Jacobian inequality

Fix v∈U~(Ο„Λ‰)v \in \tilde U(\bar\tau) and the geodesic Ξ³=Ξ³v\gamma = \gamma_v. Choose a basis {wΞ±}\{w_\alpha\} of TpMT_pM whose images under dLexp⁑τˉd\mathcal L\exp_{\bar\tau} form an orthonormal basis {YΞ±(Ο„Λ‰)}\{Y_\alpha(\bar\tau)\} of TΞ³(Ο„Λ‰)MT_{\gamma(\bar\tau)}M, and let YΞ±(Ο„)Y_\alpha(\tau) be the corresponding L\mathcal L-Jacobi fields. Then J(Ο„)J(\tau) is a constant multiple of det⁑⟨YΞ±(Ο„),YΞ²(Ο„)⟩\sqrt{\det\langle Y_\alpha(\tau), Y_\beta(\tau)\rangle}, and at Ο„=Ο„Λ‰\tau = \bar\tau, where the Gram matrix is the identity,

ddΟ„log⁑Jβˆ£Ο„Λ‰=12βˆ‘Ξ±ddΟ„βˆ£Yα∣2βˆ£Ο„Λ‰.\frac{d}{d\tau}\log J\Big|_{\bar\tau} = \frac12\sum_\alpha\frac{d}{d\tau}|Y_\alpha|^2\Big|_{\bar\tau}.

By the identity for derivatives of inner products (12A.6 𝓛-Geodesics and the Variational Formulas), 12ddΟ„βˆ£Yα∣2=βŸ¨βˆ‡XYΞ±,Yα⟩+Ric⁑(YΞ±,YΞ±)\frac12\frac{d}{d\tau}|Y_\alpha|^2 = \langle\nabla_XY_\alpha, Y_\alpha\rangle + \operatorname{Ric}(Y_\alpha, Y_\alpha), and since YΞ±Y_\alpha is an L\mathcal L-Jacobi field along a minimiser, βŸ¨βˆ‡XYΞ±,Yα⟩=12Ο„Λ‰Hess⁑L(YΞ±,YΞ±)\langle\nabla_XY_\alpha, Y_\alpha\rangle = \frac{1}{2\sqrt{\bar\tau}}\operatorname{Hess}L(Y_\alpha, Y_\alpha) at Ο„Λ‰\bar\tau. The Hessian comparison (7.9) then gives

12ddΟ„βˆ£Yα∣2=Ric⁑(YΞ±,YΞ±)+12Ο„Λ‰Hess⁑L(YΞ±,YΞ±)≀12Ο„Λ‰βˆ’12Ο„Λ‰βˆ«0Ο„Λ‰Ο„H(X,Y~Ξ±) dΟ„,\frac12\frac{d}{d\tau}|Y_\alpha|^2 = \operatorname{Ric}(Y_\alpha, Y_\alpha) + \frac{1}{2\sqrt{\bar\tau}}\operatorname{Hess}L(Y_\alpha, Y_\alpha) \leq \frac{1}{2\bar\tau} - \frac{1}{2\sqrt{\bar\tau}}\int_0^{\bar\tau}\sqrt\tau H(X, \tilde Y_\alpha)\,d\tau,

which is Perelman's (7.11), with Y~Ξ±\tilde Y_\alpha the adapted field with Y~Ξ±(Ο„Λ‰)=YΞ±(Ο„Λ‰)\tilde Y_\alpha(\bar\tau) = Y_\alpha(\bar\tau). Summing over Ξ±\alpha with the trace identity of 12A.6 𝓛-Geodesics and the Variational Formulas:

ddΟ„log⁑J(Ο„Λ‰)≀n2Ο„Λ‰βˆ’12Ο„Λ‰βˆ’3/2K.(7.12)\frac{d}{d\tau}\log J(\bar\tau) \leq \frac{n}{2\bar\tau} - \frac12\bar\tau^{-3/2}K. \tag{7.12}

Equality holds exactly when every adapted field is L\mathcal L-Jacobi, which forces 2Ric⁑+1Ο„Λ‰Hess⁑L=1Ο„Λ‰g2\operatorname{Ric} + \frac{1}{\sqrt{\bar\tau}}\operatorname{Hess}L = \frac1{\bar\tau}g at Ξ³(Ο„Λ‰)\gamma(\bar\tau).

The reduced distance along a geodesic. Along Ξ³v\gamma_v, β„“~(v,Ο„)=L~(v,Ο„)2Ο„\tilde\ell(v, \tau) = \frac{\tilde L(v, \tau)}{2\sqrt\tau} with ddΟ„L~=Ο„(R+∣X∣2)\frac{d}{d\tau}\tilde L = \sqrt\tau(R + |X|^2), so

ddΟ„β„“~=12(R+∣X∣2)βˆ’β„“~2Ο„=βˆ’12Ο„βˆ’3/2K,\frac{d}{d\tau}\tilde\ell = \frac12(R + |X|^2) - \frac{\tilde\ell}{2\tau} = -\frac12\tau^{-3/2}K,

using (7.4) in the form R+∣X∣2=β„“~Ο„βˆ’Ο„βˆ’3/2KR + |X|^2 = \frac{\tilde\ell}{\tau} - \tau^{-3/2}K (Morgan–Tian, Corollary 6.54; Exercise 7.8). Note the contrast with βˆ‚Ο„β„“\partial_\tau\ell computed on space-time in 12A.6 𝓛-Geodesics and the Variational Formulas: the derivative along a geodesic and the partial derivative at a fixed point of MM differ by βŸ¨βˆ‡β„“,X⟩\langle\nabla\ell, X\rangle.

Theorem 7.3 The integrand is monotone along each geodesic (Perelman I, Β§7.1)

For vv with v∈U~(Ο„)v \in \tilde U(\tau) for Ο„βˆˆ(0,Ο„Λ‰]\tau \in (0, \bar\tau], the function

f(v,Ο„)=Ο„βˆ’n/2eβˆ’β„“~(v,Ο„)J(v,Ο„)f(v, \tau) = \tau^{-n/2}e^{-\tilde\ell(v, \tau)}J(v, \tau)

is nonincreasing in Ο„\tau, with lim⁑τ→0f(v,Ο„)=2neβˆ’βˆ£v∣2\lim_{\tau\to0}f(v, \tau) = 2^ne^{-|v|^2}. It is constant on an interval only if, along Ξ³v\gamma_v, Ric⁑+βˆ‡2β„“=12Ο„g\operatorname{Ric} + \nabla^2\ell = \frac{1}{2\tau}g.

Proof. ddΟ„log⁑f=βˆ’n2Ο„βˆ’dβ„“~dΟ„+ddΟ„log⁑Jβ‰€βˆ’n2Ο„+12Ο„βˆ’3/2K+n2Ο„βˆ’12Ο„βˆ’3/2K=0\frac{d}{d\tau}\log f = -\frac{n}{2\tau} - \frac{d\tilde\ell}{d\tau} + \frac{d}{d\tau}\log J \leq -\frac{n}{2\tau} + \frac12\tau^{-3/2}K + \frac{n}{2\tau} - \frac12\tau^{-3/2}K = 0. The limit is Proposition 7.2, and the equality case is that of (7.12), with βˆ‡2β„“=12Ο„Hess⁑L\nabla^2\ell = \frac{1}{2\sqrt\tau}\operatorname{Hess}L.

Theorem 7.4 Monotonicity of the reduced volume

For a Ricci flow on a closed manifold, or complete with bounded curvature, V~(Ο„)\tilde V(\tau) is nonincreasing in Ο„\tau, V~(Ο„)≀1\tilde V(\tau) \leq 1, and V~(Ο„)β†’1\tilde V(\tau) \to 1 as Ο„β†’0\tau \to 0. If V~(Ο„1)=V~(Ο„2)\tilde V(\tau_1) = \tilde V(\tau_2) for some Ο„1<Ο„2\tau_1 < \tau_2, the flow is a gradient shrinking soliton on [Ο„1,Ο„2][\tau_1, \tau_2].

Proof. For Ο„<Ο„β€²\tau < \tau',

(4Ο€)n/2V~(Ο„β€²)=∫U~(Ο„β€²)f(v,Ο„β€²) dvβ‰€βˆ«U~(Ο„β€²)f(v,Ο„) dvβ‰€βˆ«U~(Ο„)f(v,Ο„) dv=(4Ο€)n/2V~(Ο„),(4\pi)^{n/2}\tilde V(\tau') = \int_{\tilde U(\tau')}f(v, \tau')\,dv \leq \int_{\tilde U(\tau')}f(v, \tau)\,dv \leq \int_{\tilde U(\tau)}f(v, \tau)\,dv = (4\pi)^{n/2}\tilde V(\tau),

using Theorem 7.3 (every v∈U~(Ο„β€²)v \in \tilde U(\tau') lies in U~(Οƒ)\tilde U(\sigma) for all σ≀τ′\sigma \leq \tau', by Proposition 7.1) and U~(Ο„β€²)βŠ†U~(Ο„)\tilde U(\tau') \subseteq \tilde U(\tau). Letting Ο„β†’0\tau \to 0, f(v,Ο„)β†’2neβˆ’βˆ£v∣2f(v, \tau) \to 2^ne^{-|v|^2}, which dominates f(v,Ο„β€²)f(v, \tau'), so (4Ο€)n/2V~(Ο„β€²)β‰€βˆ«2neβˆ’βˆ£v∣2=(4Ο€)n/2(4\pi)^{n/2}\tilde V(\tau') \leq \int2^ne^{-|v|^2} = (4\pi)^{n/2}. Equality between two times forces equality in the first inequality on a set of full measure, hence the soliton equation Ric⁑+βˆ‡2β„“=12Ο„g\operatorname{Ric} + \nabla^2\ell = \frac{1}{2\tau}g on the injectivity domain, which is dense, hence everywhere by continuity of the curvature; the soliton is gradient, with potential β„“\ell, which is therefore smooth.

The localised version. The proof is local in the following sense, which is how the reduced volume is used in flows with surgery. For an open set AA of space-time, define V~(AΟ„)=∫AΟ„(4πτ)βˆ’n/2eβˆ’β„“β€‰dV\tilde V(A_\tau) = \int_{A_\tau}(4\pi\tau)^{-n/2}e^{-\ell}\,dV over its time-Ο„\tau slice. If every minimising L\mathcal L-geodesic from xx to a point of AA stays in AA, then V~(AΟ„)\tilde V(A_\tau) is nonincreasing (Morgan–Tian, Theorem 6.80): the same pull-back argument, restricted to the preimage of AA. In a flow with surgery, AA will be the set of points reachable by L\mathcal L-geodesics that avoid the surgery regions, and the theorem lets the reduced volume be used without ever crossing a surgery (12B.9 Surgery, 12B.13 Ricci Flow with Surgery for All Time).

The barrier sense and min⁑ℓ≀n2\min\ell \leq \frac n2

Perelman's argument for min⁑ℓ≀n2\min\ell \leq \frac n2 is one line: from (7.15), LΛ‰=2Ο„L\bar L = 2\sqrt\tau L satisfies βˆ‚Ο„LΛ‰+Ξ”Lˉ≀2n\partial_\tau\bar L + \Delta\bar L \leq 2n, so at a minimum point, where Ξ”LΛ‰β‰₯0\Delta\bar L \geq 0, βˆ‚Ο„Lˉ≀2n\partial_\tau\bar L \leq 2n, and min⁑LΛ‰βˆ’2nΟ„\min\bar L - 2n\tau is nonincreasing; since LΛ‰β†’0\bar L \to 0 at pp as Ο„β†’0\tau \to 0, min⁑Lˉ≀2nΟ„\min\bar L \leq 2n\tau, which is min⁑ℓ≀n2\min\ell \leq \frac n2. The difficulty is that the minimum point may be where β„“\ell is not smooth. The remedy is the device used by Calabi (1958) for the Laplacian of the distance function.

Upper barriers. A smooth function Ο†\varphi defined near a point yy is an upper barrier for a continuous function hh at yy if Ο†(y)=h(y)\varphi(y) = h(y) and Ο†β‰₯h\varphi \geq h nearby. A differential inequality such as βˆ‚Ο„h+Ξ”h≀F\partial_\tau h + \Delta h \leq F holds in the barrier sense at yy if for every Ξ΅>0\varepsilon > 0 there is an upper barrier Ο†\varphi at yy with βˆ‚Ο„Ο†+Δφ≀F+Ξ΅\partial_\tau\varphi + \Delta\varphi \leq F + \varepsilon there. The point is that at a minimum of hh in space, an upper barrier is also minimised there in space (it lies above hh and touches it), so Δφβ‰₯0\Delta\varphi \geq 0, and the inequality gives information about βˆ‚Ο„Ο†\partial_\tau\varphi, hence about the one-sided time derivative of hh.

Proposition 7.5 The barrier inequality (Morgan–Tian, Proposition 7.8)

On a Ricci flow on a closed manifold, or complete of bounded curvature, the reduced distance satisfies, at every (q,Ο„)(q, \tau) with 0<Ο„0 < \tau in the interval of definition,

βˆ‚Ο„β„“+Δℓ≀n2βˆ’β„“Ο„\partial_\tau\ell + \Delta\ell \leq \frac{\frac n2 - \ell}{\tau}

in the barrier sense.

Proof. At points of the injectivity domain this follows by adding the identity βˆ‚Ο„β„“=Rβˆ’β„“Ο„+K2Ο„3/2\partial_\tau\ell = R - \frac\ell\tau + \frac{K}{2\tau^{3/2}} to the Laplacian comparison Ξ”β„“β‰€βˆ’R+n2Ο„βˆ’K2Ο„3/2\Delta\ell \leq -R + \frac{n}{2\tau} - \frac{K}{2\tau^{3/2}} of 12A.6 𝓛-Geodesics and the Variational Formulas (Exercise 7.9). At a general point (q,Ο„)(q, \tau), take a minimising L\mathcal L-geodesic Ξ³\gamma from xx to (q,Ο„)(q, \tau), a small Ο„1>0\tau_1 > 0, and the point q1=Ξ³(Ο„1)q_1 = \gamma(\tau_1). The geodesic γ∣[Ο„1,Ο„]\gamma|_{[\tau_1, \tau]} from (q1,Ο„1)(q_1, \tau_1) is not conjugate along its length (Morgan–Tian, Proposition 6.31: a minimiser has no conjugate points in its interior, by the argument of Proposition 7.1), so the L\mathcal L-length from (q1,Ο„1)(q_1, \tau_1), computed along nearby geodesics, is a smooth function Lq1L_{q_1} near (q,Ο„)(q, \tau). Then

Ο†(qβ€²,Ο„β€²)=12Ο„β€²(L(γ∣[0,Ο„1])+Lq1(qβ€²,Ο„β€²))\varphi(q', \tau') = \frac{1}{2\sqrt{\tau'}}\Big(\mathcal L(\gamma|_{[0,\tau_1]}) + L_{q_1}(q', \tau')\Big)

is the reduced length of a particular broken path, so Ο†β‰₯β„“\varphi \geq \ell near (q,Ο„)(q, \tau) with equality at (q,Ο„)(q, \tau): an upper barrier. The computations of 12A.6 𝓛-Geodesics and the Variational Formulas, done with base point (q1,Ο„1)(q_1, \tau_1) instead of (p,0)(p, 0), give βˆ‚Ο„Ο†+Δφ\partial_\tau\varphi + \Delta\varphi bounded by n/2βˆ’β„“Ο„\frac{n/2 - \ell}{\tau} plus error terms that are continuous in Ο„1\tau_1 and vanish as Ο„1β†’0\tau_1 \to 0 (their Lemma 6.49 and Lemma 6.47). Choosing Ο„1\tau_1 small gives the barrier inequality with any Ξ΅>0\varepsilon > 0.

Theorem 7.6 min⁑ℓ≀n2\min\ell \leq \frac n2 (Perelman I, Β§7.1; Morgan–Tian, Theorem 7.10)

On a Ricci flow on a closed manifold, or complete of bounded curvature, for every Ο„\tau in the interval of definition there is a point qΟ„q_\tau with β„“(qΟ„,Ο„)≀n2\ell(q_\tau, \tau) \leq \frac n2.

Proof. Let β„“min⁑(Ο„)=min⁑qβ„“(q,Ο„)\ell_{\min}(\tau) = \min_q\ell(q, \tau); the minimum is attained (on a closed manifold by compactness; on a complete flow of bounded curvature because minimisers of bounded β„“\ell stay in a bounded region, by bounds on Ο„βˆ£X∣\sqrt\tau|X|: Morgan–Tian, Claim 7.11), and β„“min⁑\ell_{\min} is continuous. At a minimum point qq of β„“(β‹…,Ο„)\ell(\cdot, \tau), an upper barrier Ο†\varphi with βˆ‚Ο„Ο†+Δφ≀n/2βˆ’β„“Ο„+Ξ΅\partial_\tau\varphi + \Delta\varphi \leq \frac{n/2 - \ell}{\tau} + \varepsilon has a spatial minimum at qq too, so Δφ(q)β‰₯0\Delta\varphi(q) \geq 0 and βˆ‚Ο„Ο†(q)≀n/2βˆ’β„“min⁑(Ο„)Ο„+Ξ΅\partial_\tau\varphi(q) \leq \frac{n/2 - \ell_{\min}(\tau)}{\tau} + \varepsilon. Since β„“(q,Ο„β€²)≀φ(q,Ο„β€²)\ell(q, \tau') \leq \varphi(q, \tau') for Ο„β€²\tau' near Ο„\tau, the upper right Dini derivative of β„“min⁑\ell_{\min} satisfies

lim sup⁑τ′↓τℓmin⁑(Ο„β€²)βˆ’β„“min⁑(Ο„)Ο„β€²βˆ’Ο„β‰€n2βˆ’β„“min⁑(Ο„)Ο„.\limsup_{\tau'\downarrow\tau}\frac{\ell_{\min}(\tau') - \ell_{\min}(\tau)}{\tau' - \tau} \leq \frac{\frac n2 - \ell_{\min}(\tau)}{\tau}.

So wherever β„“min⁑>n2\ell_{\min} > \frac n2 it is strictly decreasing, and wherever β„“min⁑≀n2\ell_{\min} \leq \frac n2 it cannot cross above n2\frac n2 (Exercise 7.10). As Ο„β†’0\tau \to 0, β„“min⁑(Ο„)≀ℓ(p,Ο„)≀12Ο„βˆ«0τσR(p,Οƒ) dΟƒ=O(Ο„)\ell_{\min}(\tau) \leq \ell(p, \tau) \leq \frac{1}{2\sqrt\tau}\int_0^\tau\sqrt\sigma R(p, \sigma)\,d\sigma = O(\tau), using the constant path at pp; so β„“min⁑<n2\ell_{\min} < \frac n2 for small Ο„\tau, and hence for all Ο„\tau.

There is also a lower bound, much easier. In backward time, RΟ„=βˆ’Ξ”Rβˆ’2∣Ric⁑∣2β‰€βˆ’Ξ”Rβˆ’2nR2R_\tau = -\Delta R - 2|\operatorname{Ric}|^2 \leq -\Delta R - \frac2nR^2, and if the flow exists on [0,Ο„0][0, \tau_0] the maximum principle (11A.7 Maximum Principles under Ricci Flow) gives R(β‹…,Ο„)β‰₯βˆ’n2(Ο„0βˆ’Ο„)R(\cdot, \tau) \geq -\frac{n}{2(\tau_0 - \tau)}, the forward statement Rβ‰₯βˆ’n2tR \geq -\frac{n}{2t} for a flow that started at time 00. Then Lβ‰₯∫0τσRβ‰₯βˆ’n2(Ο„0βˆ’Ο„)β‹…23Ο„3/2L \geq \int_0^\tau\sqrt\sigma R \geq -\frac{n}{2(\tau_0 - \tau)}\cdot\frac23\tau^{3/2} is bounded below for Ο„\tau away from Ο„0\tau_0, and so is β„“\ell.

The other inequalities. Morgan and Tian also prove (their Theorem 7.13, adapting an argument of Ye) that (7.13) and (7.14) hold in the sense of distributions on all of MM, and that if equality holds in either, then β„“\ell is smooth and the flow is a gradient shrinking soliton. This gives a second proof of the monotonicity of V~\tilde V, by integrating (7.13) against the volume form, which is the one Perelman mentions in parentheses after (7.12).

In the world Analogy Calabi's trick and viscosity solutions

The barrier sense is a precursor of the viscosity solutions of 6C.9 Hamilton–Jacobi Equations and Viscosity Solutions. Calabi introduced it in 1958 to prove the Laplacian comparison Ξ”r≀nβˆ’1r\Delta r \leq \frac{n - 1}{r} for the distance function at points of the cut locus, where rr is not differentiable: at such a point one takes a point slightly along the minimising geodesic and uses the (smooth) distance from it as a barrier. Perelman's barrier for β„“\ell is the same construction in space-time, moving the base point a short way along the minimising L\mathcal L-geodesic. Crandall and Lions's theory of viscosity solutions (1983) made the idea systematic: a continuous function is a solution of a second-order equation if smooth functions touching it from above or below satisfy the corresponding inequalities. The reduced distance is, in that language, a viscosity supersolution of a parabolic Hamilton–Jacobi equation, and its minimum is controlled by the comparison principle.

Where this goes Where this goes

12A.8 Local Noncollapsing from the Reduced Volume uses Theorem 7.4 and Theorem 7.6 to prove noncollapsing under local curvature bounds: a collapsed ball makes V~\tilde V small at small Ο„\tau, while the point where ℓ≀n2\ell \leq \frac n2 makes it large at large Ο„\tau. 12B.1 ΞΊ-Solutions uses the equality case to produce the asymptotic soliton of a ΞΊ\kappa-solution. In flows with surgery, the localised version is used in 12B.13 Ricci Flow with Surgery for All Time.

History

Perelman stated the monotonicity of the reduced volume and min⁑ℓ≀n2\min\ell \leq \frac n2 in Β§7.1 of his first preprint (2002), with the remark that inequalities at non-smooth points hold "in the barrier sense, or in the sense of distributions". Rugang Ye's notes (2004) gave a careful treatment of the regularity of β„“\ell and the distributional inequalities, which Morgan and Tian follow in their chapter 7. Calabi's barrier argument dates from 1958, and Crandall and Lions's viscosity solutions from 1983. The analogy with Bishop–Gromov, whose classical proof integrates the Jacobian of the exponential map over the interior of the cut locus, goes back to Bishop (1963) and Gromov (1980).

Recall Where we stand

The L\mathcal L-exponential map v↦γv(Ο„)v \mapsto \gamma_v(\tau) has differential given by L\mathcal L-Jacobi fields; on the injectivity set U~(Ο„)\tilde U(\tau) (unique, nondegenerate minimisers) it is a diffeomorphism onto the injectivity domain, the sets U~(Ο„)\tilde U(\tau) shrink as Ο„\tau grows, and on complete flows of bounded curvature the injectivity domain has full measure. On flat space Ο„βˆ’n/2eβˆ’β„“~J=2neβˆ’βˆ£v∣2\tau^{-n/2}e^{-\tilde\ell}J = 2^ne^{-|v|^2}; the integrand is scale invariant, and by blowing up it tends to this flat value as Ο„β†’0\tau \to 0. Perelman's Jacobian inequality ddΟ„log⁑J≀n2Ο„βˆ’12Ο„βˆ’3/2K\frac{d}{d\tau}\log J \leq \frac{n}{2\tau} - \frac12\tau^{-3/2}K and ddΟ„β„“~=βˆ’12Ο„βˆ’3/2K\frac{d}{d\tau}\tilde\ell = -\frac12\tau^{-3/2}K make Ο„βˆ’n/2eβˆ’β„“~J\tau^{-n/2}e^{-\tilde\ell}J nonincreasing along every geodesic, so V~\tilde V is nonincreasing, at most 11, tends to 11 as Ο„β†’0\tau \to 0, and is constant only on gradient shrinking solitons; a localised version holds on regions closed under minimising geodesics. In the barrier sense βˆ‚Ο„β„“+Δℓ≀n/2βˆ’β„“Ο„\partial_\tau\ell + \Delta\ell \leq \frac{n/2 - \ell}{\tau}, and a Dini-derivative argument gives min⁑ℓ≀n2\min\ell \leq \frac n2; also Rβ‰₯βˆ’n2(Ο„0βˆ’Ο„)R \geq -\frac{n}{2(\tau_0 - \tau)} bounds β„“\ell below. 12A.8 Local Noncollapsing from the Reduced Volume turns these into local noncollapsing.

Exercises

Exercise 7.7 The flat integrand

On static flat Rn\mathbb{R}^n: (a) show that Lexp⁑τ(v)=p+2Ο„v\mathcal L\exp_\tau(v) = p + 2\sqrt\tau v has Jacobian 2nΟ„n/22^n\tau^{n/2} and that β„“~(v,Ο„)=∣v∣2\tilde\ell(v, \tau) = |v|^2; (b) show that ∫Rn(4πτ)βˆ’n/2eβˆ’β„“~J dv=1\int_{\mathbb{R}^n}(4\pi\tau)^{-n/2}e^{-\tilde\ell}J\,dv = 1; (c) check that the change of variables q=p+2Ο„vq = p + 2\sqrt\tau v turns this into ∫(4πτ)βˆ’n/2eβˆ’βˆ£qβˆ’p∣2/4Ο„dq\int(4\pi\tau)^{-n/2}e^{-|q-p|^2/4\tau}dq.

Solution

(a) The map is linear with matrix 2Ο„I2\sqrt\tau I, determinant 2nΟ„n/22^n\tau^{n/2}. The L\mathcal L-length of Ξ³v∣[0,Ο„]\gamma_v|_{[0,\tau]} is ∫0Ο„Οƒβˆ£vΟƒβˆ’1/2∣2dΟƒ=2Ο„βˆ£v∣2\int_0^\tau\sqrt\sigma|v\sigma^{-1/2}|^2d\sigma = 2\sqrt\tau|v|^2, so β„“~=∣v∣2\tilde\ell = |v|^2. (b) The integrand is (4πτ)βˆ’n/2eβˆ’βˆ£v∣22nΟ„n/2=Ο€βˆ’n/2eβˆ’βˆ£v∣2(4\pi\tau)^{-n/2}e^{-|v|^2}2^n\tau^{n/2} = \pi^{-n/2}e^{-|v|^2}, whose integral is 11. (c) dq=2nΟ„n/2dvdq = 2^n\tau^{n/2}dv and ∣v∣2=∣qβˆ’p∣24Ο„|v|^2 = \frac{|q - p|^2}{4\tau}.

Exercise 7.8 β„“~\tilde\ell along an L\mathcal L-geodesic

Using ddΟ„L~=Ο„(R+∣X∣2)\frac{d}{d\tau}\tilde L = \sqrt\tau(R + |X|^2) and (7.4), show that ddΟ„β„“~(v,Ο„)=βˆ’12Ο„βˆ’3/2K(Ξ³v,Ο„)\frac{d}{d\tau}\tilde\ell(v, \tau) = -\frac12\tau^{-3/2}K(\gamma_v, \tau). On flat space, check that β„“~\tilde\ell is constant along each geodesic.

Solution

ddΟ„β„“~=Ο„(R+∣X∣2)2Ο„βˆ’L~4Ο„3/2=12(R+∣X∣2)βˆ’β„“~2Ο„\frac{d}{d\tau}\tilde\ell = \frac{\sqrt\tau(R + |X|^2)}{2\sqrt\tau} - \frac{\tilde L}{4\tau^{3/2}} = \frac12(R + |X|^2) - \frac{\tilde\ell}{2\tau}. By (7.4), Ο„3/2(R+∣X∣2)=12L~βˆ’K=Ο„β„“~βˆ’K\tau^{3/2}(R + |X|^2) = \frac12\tilde L - K = \sqrt\tau\tilde\ell - K, so R+∣X∣2=β„“~Ο„βˆ’Ο„βˆ’3/2KR + |X|^2 = \frac{\tilde\ell}{\tau} - \tau^{-3/2}K, and ddΟ„β„“~=βˆ’12Ο„βˆ’3/2K\frac{d}{d\tau}\tilde\ell = -\frac12\tau^{-3/2}K. On flat space K=0K = 0 and β„“~=∣v∣2\tilde\ell = |v|^2 is constant.

Exercise 7.9 The inequality behind min⁑ℓ≀n2\min\ell \leq \frac n2

At a point where β„“\ell is smooth: (a) add the identity βˆ‚Ο„β„“=Rβˆ’β„“Ο„+K2Ο„3/2\partial_\tau\ell = R - \frac\ell\tau + \frac{K}{2\tau^{3/2}} and the inequality Ξ”β„“β‰€βˆ’R+n2Ο„βˆ’K2Ο„3/2\Delta\ell \leq -R + \frac{n}{2\tau} - \frac{K}{2\tau^{3/2}} to get βˆ‚Ο„β„“+Δℓ≀n/2βˆ’β„“Ο„\partial_\tau\ell + \Delta\ell \leq \frac{n/2 - \ell}{\tau}; (b) check that it also follows by adding the equalities βˆ‚Ο„β„“βˆ’Ξ”β„“+βˆ£βˆ‡β„“βˆ£2βˆ’R+n2Ο„=Ξ΄\partial_\tau\ell - \Delta\ell + |\nabla\ell|^2 - R + \frac{n}{2\tau} = \delta and 2Ξ”β„“βˆ’βˆ£βˆ‡β„“βˆ£2+R+β„“βˆ’nΟ„=βˆ’2Ξ΄2\Delta\ell - |\nabla\ell|^2 + R + \frac{\ell - n}{\tau} = -2\delta of 12A.6 𝓛-Geodesics and the Variational Formulas; (c) show that it is equivalent to (7.15) for LΛ‰=4Ο„β„“\bar L = 4\tau\ell.

Solution

(a) The RR and KK terms cancel: βˆ‚Ο„β„“+Ξ”β„“β‰€βˆ’β„“Ο„+n2Ο„\partial_\tau\ell + \Delta\ell \leq -\frac\ell\tau + \frac{n}{2\tau}. (b) Adding gives βˆ‚Ο„β„“+Ξ”β„“+n2Ο„+β„“βˆ’nΟ„=βˆ’Ξ΄\partial_\tau\ell + \Delta\ell + \frac{n}{2\tau} + \frac{\ell - n}{\tau} = -\delta, so βˆ‚Ο„β„“+Ξ”β„“=n/2βˆ’β„“Ο„βˆ’Ξ΄β‰€n/2βˆ’β„“Ο„\partial_\tau\ell + \Delta\ell = \frac{n/2 - \ell}{\tau} - \delta \leq \frac{n/2 - \ell}{\tau}. (Adding the inequalities (7.13) and (7.14) themselves would not work, since they point in opposite directions; the defect Ξ΄\delta is what links them.) (c) βˆ‚Ο„LΛ‰+Ξ”LΛ‰=4β„“+4Ο„(βˆ‚Ο„β„“+Ξ”β„“)≀4β„“+4(n2βˆ’β„“)=2n\partial_\tau\bar L + \Delta\bar L = 4\ell + 4\tau(\partial_\tau\ell + \Delta\ell) \leq 4\ell + 4(\frac n2 - \ell) = 2n, and conversely.

Exercise 7.10 A Dini-derivative comparison

Let m:(0,T)β†’Rm : (0, T) \to \mathbb{R} be continuous with m(Ο„)β†’0m(\tau) \to 0 as Ο„β†’0\tau \to 0, and suppose its upper right Dini derivative satisfies D+m(Ο„)≀cβˆ’m(Ο„)Ο„D^+m(\tau) \leq \frac{c - m(\tau)}{\tau} for every Ο„\tau, with c>0c > 0. Show that m(Ο„)≀cm(\tau) \leq c for all Ο„\tau. (Hint: compare with ddΟ„(Ο„(mβˆ’c))\frac{d}{d\tau}(\tau(m - c)), or argue at a first time where m>c+Ξ΅m > c + \varepsilon.)

Solution

Suppose m(Ο„1)>cm(\tau_1) > c for some Ο„1\tau_1. Since mβ†’0<cm \to 0 < c as Ο„β†’0\tau \to 0, by continuity there is Ο„0<Ο„1\tau_0 < \tau_1 with m(Ο„0)=cm(\tau_0) = c and m>cm > c on (Ο„0,Ο„1](\tau_0, \tau_1]. On that interval D+m<0D^+m < 0, and a continuous function with negative upper right Dini derivative everywhere on an interval is nonincreasing there (a standard lemma of real analysis); so m(Ο„1)≀m(Ο„0)=cm(\tau_1) \leq m(\tau_0) = c, a contradiction.

Exercise 7.11 Why the localised version needs closure under geodesics

Let AA be an open set of space-time and suppose a minimising L\mathcal L-geodesic from xx to some point of AΟ„β€²A_{\tau'} leaves AA at some earlier time. Explain why the inequality V~(AΟ„β€²)≀V~(AΟ„)\tilde V(A_{\tau'}) \leq \tilde V(A_\tau) may fail, by tracing the pull-back proof: which inclusion breaks?

Solution

The proof pulls AΟ„β€²A_{\tau'} back to a set A~βŠ†U~(Ο„β€²)\tilde A \subseteq \tilde U(\tau') and uses ∫A~f(v,Ο„β€²)β‰€βˆ«A~f(v,Ο„)=V~(Lexp⁑τ(A~))\int_{\tilde A}f(v, \tau') \leq \int_{\tilde A}f(v, \tau) = \tilde V(\mathcal L\exp_\tau(\tilde A)), then needs Lexp⁑τ(A~)βŠ†AΟ„\mathcal L\exp_\tau(\tilde A) \subseteq A_\tau to conclude ≀V~(AΟ„)\leq \tilde V(A_\tau). If some geodesic Ξ³v\gamma_v, v∈A~v \in \tilde A, is outside AA at time Ο„\tau, its contribution at time Ο„\tau is not counted in V~(AΟ„)\tilde V(A_\tau), and the last inclusion fails. In a flow with surgery, geodesics that pass through a surgery region are exactly such paths, which is why Morgan and Tian must show that the relevant minimisers avoid surgery caps (12B.13 Ricci Flow with Surgery for All Time).

Exercise 7.12 Scale invariance of V~\tilde V

Let gQ(t)=Qg(T+(tβˆ’T)/Q)g_Q(t) = Qg(T + (t - T)/Q). Show that LQ(Ξ³Q)=Q L(Ξ³)\mathcal L_Q(\gamma_Q) = \sqrt Q\,\mathcal L(\gamma) for corresponding paths (Ξ³Q(Ο„Q)=Ξ³(Ο„Q/Q)\gamma_Q(\tau_Q) = \gamma(\tau_Q/Q)), that β„“Q(q,QΟ„)=β„“(q,Ο„)\ell_Q(q, Q\tau) = \ell(q, \tau), and that V~Q(QΟ„)=V~(Ο„)\tilde V_Q(Q\tau) = \tilde V(\tau).

Solution

With Ο„Q=QΟ„\tau_Q = Q\tau: RQ=Qβˆ’1RR_Q = Q^{-1}R, βˆ£Ξ³Λ™Q∣gQ2=Qβ‹…Qβˆ’2βˆ£Ξ³Λ™βˆ£g2=Qβˆ’1βˆ£Ξ³Λ™βˆ£2|\dot\gamma_Q|^2_{g_Q} = Q\cdot Q^{-2}|\dot\gamma|^2_g = Q^{-1}|\dot\gamma|^2 (the metric gains QQ, the velocity loses QQ), Ο„Q=QΟ„\sqrt{\tau_Q} = \sqrt Q\sqrt\tau and dΟ„Q=Q dΟ„d\tau_Q = Q\,d\tau. So LQ=∫Qτ Qβˆ’1(R+βˆ£Ξ³Λ™βˆ£2)Q dΟ„=Q L\mathcal L_Q = \int\sqrt Q\sqrt\tau\,Q^{-1}(R + |\dot\gamma|^2)Q\,d\tau = \sqrt Q\,\mathcal L. Then β„“Q=QL2QΟ„=β„“\ell_Q = \frac{\sqrt QL}{2\sqrt{Q\tau}} = \ell. And (4πτQ)βˆ’n/2dVgQ=Qβˆ’n/2(4πτ)βˆ’n/2Qn/2dVg(4\pi\tau_Q)^{-n/2}dV_{g_Q} = Q^{-n/2}(4\pi\tau)^{-n/2}Q^{n/2}dV_g, so V~Q(QΟ„)=V~(Ο„)\tilde V_Q(Q\tau) = \tilde V(\tau).

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