Book 9B

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Course 9Book 9B: Comparison, Convergence and Heat on ManifoldsChapter 2

Volume Comparison

Bishop–Gromov, packing arguments, and why hyperbolic space fits trees.

20 min read · Updated Oct 3, 2026

Read with Petersen's Riemannian Geometry, the chapter on Ricci curvature comparison (Bishop–Gromov relative volume comparison and its first applications), and Lee's Introduction to Riemannian Manifolds (2nd edition), chapter 11. Cheeger and Ebin, chapter 1, is the classical reference.

In this chapter · 7 sections
  1. 2.1Why hyperbolic space fits trees
  2. 2.2Polar coordinates and the volume element
  3. 2.3Bishop–Gromov
  4. 2.4Doubling, packing and growth
  5. 2.5A pattern that returns: monotone volume ratios
  6. 2.6History
  7. 2.7Exercises

Laplacian comparison (9B.1 Laplacian Comparison) says that, under a lower Ricci bound, geodesic spheres bend at least as much as in the model space. Integrating that statement over the spheres gives the theorem used more than any other in this part of the Path. Bishop–Gromov volume comparison: if Ric⁡≥(n−1)k\operatorname{Ric} \geq (n - 1)k, the volume of a ball, divided by the volume of the ball of the same radius in the model space, can only decrease as the radius grows. Lower Ricci bounds cap the growth of volume, and they also guarantee that a ball keeps a definite fraction of the volume of any larger concentric ball. The second fact is what makes packing arguments, Gromov's compactness theorem and Perelman's noncollapsing work.

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

  • write the volume form in geodesic polar coordinates and relate its growth to the Laplacian of distance;
  • prove the Bishop–Gromov inequality and its absolute form, Bishop's inequality;
  • use relative volume comparison for doubling and packing estimates;
  • define the asymptotic volume ratio and compute it for cones, cylinders and paraboloids;
  • recognise the same monotone-ratio structure in Perelman's reduced volume.

Why hyperbolic space fits trees

In the world Model Trees, networks and hyperbolic space

In a tree where every node has bb children, the number of nodes at depth rr is brb^r: exponential in rr. In the plane, the number of points you can fit at distance about rr from a centre, keeping them a unit apart, grows only linearly in rr, so a large tree cannot be drawn in the plane without crushing its leaves together. In the hyperbolic plane the circumference of a circle is 2πsinh⁡r2\pi\sinh r, exponential in rr (9A.1 Riemannian Metrics and Model Spaces), and there is room. Rik Sarkar showed (2011) that every finite tree embeds in the hyperbolic plane with distortion arbitrarily close to 11.

This volume growth makes hyperbolic geometry useful for hierarchical data. Dmitri Krioukov and colleagues ("Hyperbolic geometry of complex networks", Physical Review E, 2010) showed that networks whose nodes are placed at random in a hyperbolic disc reproduce features of real networks such as the internet: heavy-tailed degree distributions and strong clustering. Maximilian Nickel and Douwe Kiela ("Poincaré embeddings for learning hierarchical representations", NeurIPS 2017) embedded the WordNet hierarchy of nouns in the Poincaré ball and represented it far more compactly than in Euclidean space. Both are active research areas, not settled practice. The underlying fact is the one this chapter quantifies: curvature controls how fast volume grows.

Polar coordinates and the volume element

Fix pp and use geodesic polar coordinates (r,θ)(r, \theta), θ∈Sn−1⊂TpM\theta \in S^{n-1} \subset T_pM, on the domain {r<c(θ)}\{r < c(\theta)\}, where c(θ)c(\theta) is the distance to the cut point in direction θ\theta. The volume form is

dV=A(r,θ) dr dθ,dV = \mathcal A(r, \theta)\,dr\,d\theta,

with dθd\theta the round measure on Sn−1S^{n-1} and A(r,θ)=rn−1+O(rn+1)\mathcal A(r, \theta) = r^{n-1} + O(r^{n+1}). Since A\mathcal A is the Jacobian of the exponential map along the radial geodesic, its logarithmic derivative is the mean curvature of the geodesic sphere (Exercise 2.2):

∂rlog⁡A(r,θ)=Δr(exp⁡p(rθ)).\partial_r\log\mathcal A(r, \theta) = \Delta r\big(\exp_p(r\theta)\big).

Set A=0\mathcal A = 0 for r≥c(θ)r \geq c(\theta); the cut locus has measure zero, so Vol⁡B(p,R)=∫Sn−1∫0RA dr dθ\operatorname{Vol}B(p, R) = \int_{S^{n-1}}\int_0^R\mathcal A\,dr\,d\theta (the polar formula of 3A.5 Product Measures and Change of Variables on a manifold). In the model space of curvature kk, Ak(r)=sn⁡k(r)n−1\mathcal A_k(r) = \operatorname{sn}_k(r)^{n-1} and Vk(R)=∣Sn−1∣∫0Rsn⁡kn−1V_k(R) = |S^{n-1}|\int_0^R\operatorname{sn}_k^{n-1} (Figure 2.1).

Figure 2.1. Areas of geodesic discs in the unit sphere (2π(1−cos⁡r)2\pi(1 - \cos r)), the plane (πr2\pi r^2) and the hyperbolic plane (2π(cosh⁡r−1)2\pi(\cosh r - 1)). Curvature 11 caps area at 4π4\pi, the whole sphere; curvature −1-1 makes it grow exponentially.

Bishop–Gromov

Theorem 2.1 Bishop–Gromov

Let MM be complete with Ric⁡≥(n−1)k g\operatorname{Ric} \geq (n - 1)k\,g. Then for every pp:

  1. r↦A(r,θ)sn⁡k(r)n−1r \mapsto \frac{\mathcal A(r, \theta)}{\operatorname{sn}_k(r)^{n-1}} is nonincreasing for each θ\theta;
  2. R↦Vol⁡B(p,R)Vk(R)R \mapsto \frac{\operatorname{Vol}B(p, R)}{V_k(R)} is nonincreasing (for k>0k > 0, on 0<R≤πk0 < R \leq \frac{\pi}{\sqrt k}), and tends to 11 as R→0R \to 0. In particular Vol⁡B(p,R)≤Vk(R)\operatorname{Vol}B(p, R) \leq V_k(R) (Bishop's inequality), and for r≤Rr \leq R,
Vol⁡B(p,r)Vol⁡B(p,R)≥Vk(r)Vk(R).\frac{\operatorname{Vol}B(p, r)}{\operatorname{Vol}B(p, R)} \geq \frac{V_k(r)}{V_k(R)}.

Proof. (1) For r<c(θ)r < c(\theta), ∂rlog⁡A=Δr≤(n−1)sn⁡k′sn⁡k=∂rlog⁡sn⁡kn−1\partial_r\log\mathcal A = \Delta r \leq (n - 1)\frac{\operatorname{sn}_k'}{\operatorname{sn}_k} = \partial_r\log\operatorname{sn}_k^{n-1} by Laplacian comparison (9B.1 Laplacian Comparison), so the ratio is nonincreasing; past c(θ)c(\theta) it is 00. (2) Write f(r)=∫Sn−1A(r,θ) dθf(r) = \int_{S^{n-1}}\mathcal A(r, \theta)\,d\theta and g(r)=∣Sn−1∣sn⁡kn−1g(r) = |S^{n-1}|\operatorname{sn}_k^{n-1}; by (1), fg\frac fg is nonincreasing. The lemma in Exercise 2.3 gives that ∫0Rf∫0Rg\frac{\int_0^Rf}{\int_0^Rg} is nonincreasing. As R→0R \to 0 the ratio tends to 11 because A∼rn−1\mathcal A \sim r^{n-1}. The last two claims follow by comparing the ratio at rr, at RR and at 00.

Equality characterises the model: if Vol⁡B(p,R)=Vk(R)\operatorname{Vol}B(p, R) = V_k(R) for some RR, then B(p,R)B(p, R) is isometric to a ball in the model space. For k>0k > 0 this gives Cheng's maximal diameter theorem (1975): if Ric⁡≥(n−1)g\operatorname{Ric} \geq (n - 1)g and diam⁡=π\operatorname{diam} = \pi, then MM is isometric to the unit sphere (Exercise 2.7).

Figure 2.2. The Bishop–Gromov ratio Area⁡B(o,s)πs2\frac{\operatorname{Area}B(o, s)}{\pi s^2} for geodesic discs about the vertex oo of the paraboloid z=x2+y2z = x^2 + y^2, which has K>0K > 0 (computed by quadrature, and checked to be decreasing). It starts at 11 and tends to 00: the paraboloid's asymptotic volume ratio is zero.

Doubling, packing and growth

Relative comparison is the useful form. With Ric⁡≥0\operatorname{Ric} \geq 0 it says Vol⁡B(p,2r)≤2nVol⁡B(p,r)\operatorname{Vol}B(p, 2r) \leq 2^n\operatorname{Vol}B(p, r): the volume measure is doubling, with a constant depending only on the dimension. With Ric⁡≥−(n−1)\operatorname{Ric} \geq -(n - 1), the same holds for r≤1r \leq 1 with a slightly larger constant. Two consequences are used again and again.

  • Packing. If Ric⁡≥0\operatorname{Ric} \geq 0 and the balls B(x1,r),…,B(xN,r)B(x_1, r), \dots, B(x_N, r) are disjoint and lie in B(p,R)B(p, R), then N≤(2Rr)nN \leq (\frac{2R}{r})^n (Exercise 2.4). Combined with the Vitali covering lemma (3A.6 Modes of Convergence and Differentiation), this bounds how many small balls are needed to cover a large one. Gromov's precompactness theorem (9B.4 Convergence of Manifolds) rests on exactly this count.
  • Growth. If Ric⁡≥0\operatorname{Ric} \geq 0, then Vol⁡B(p,R)≤ωnRn\operatorname{Vol}B(p, R) \leq \omega_nR^n: no more than Euclidean. A theorem of Calabi and Yau gives the lower bound for complete noncompact manifolds: Vol⁡B(p,R)≥cR\operatorname{Vol}B(p, R) \geq cR for R≥1R \geq 1 (Exercise 2.5).

The asymptotic volume ratio. If Ric⁡≥0\operatorname{Ric} \geq 0 and MM is complete and noncompact, the ratio Vol⁡B(p,R)ωnRn\frac{\operatorname{Vol}B(p, R)}{\omega_nR^n} is nonincreasing, so it has a limit

AVR⁡(M)=lim⁡R→∞Vol⁡B(p,R)ωnRn∈[0,1],\operatorname{AVR}(M) = \lim_{R\to\infty}\frac{\operatorname{Vol}B(p, R)}{\omega_nR^n} \in [0, 1],

which does not depend on pp (Exercise 2.6). It is 11 only for Rn\mathbb{R}^n. A cone of opening angle less than Euclidean has a positive value below 11; a cylinder Sn−1×RS^{n-1}\times\mathbb{R} and the paraboloid have AVR⁡=0\operatorname{AVR} = 0 (Exercise 2.8). Perelman proved that every κ\kappa-solution, the ancient solutions that model Ricci flow singularities, has asymptotic volume ratio zero (12B.2 The Structure of κ-Solutions). That is one of the facts that make the canonical neighbourhood theorem work.

In the world Model Counting galaxies to measure curvature

If space has constant curvature kk, the volume within distance rr grows like Vk(r)V_k(r): faster than r3r^3 if space is negatively curved, slower if positively. So counting galaxies out to a given distance, assuming they are spread uniformly, would measure the curvature of the universe. Edwin Hubble attempted this in the 1930s. The test failed in practice: distant galaxies are seen as they were long ago, and galaxies evolve, merge and change brightness, effects that swamp the curvature signal. Today the curvature of space is measured instead from the angular sizes of features in the cosmic microwave background (9A.6 The Laplacian and the Bochner Formula), which find it close to flat.

A pattern that returns: monotone volume ratios

Bishop–Gromov compares a manifold with a model, through a ratio that is monotone in the scale and equal to 11 exactly for the model. Perelman's reduced volume (12A.5 Reduced Distance and Reduced Volume) has the same structure, in space-time:

Bishop–Gromov Perelman's reduced volume
quantity Vol⁡B(p,r)ωnrn\dfrac{\operatorname{Vol}B(p, r)}{\omega_nr^n} V~(τ)=∫(4πτ)−n/2e−ℓ dV\tilde V(\tau) = \displaystyle\int(4\pi\tau)^{-n/2}e^{-\ell}\,dV
hypothesis Ric⁡≥0\operatorname{Ric} \geq 0 a Ricci flow, backwards in time τ\tau
monotonicity nonincreasing in rr nonincreasing in τ\tau
equality Rn\mathbb{R}^n (flat) the Gaussian soliton on Rn\mathbb{R}^n
proved from Laplacian comparison for rr Laplacian comparison for the reduced distance ℓ\ell

The second column is explained in 12A.5 Reduced Distance and Reduced Volume; it is listed here so that, when you meet it, it is a familiar theorem in new clothes.

Where this goes Where volume comparison is used

9B.3 Collapsing and Noncollapsing combines a volume lower bound with a curvature bound to bound the injectivity radius from below, the bridge from Perelman's noncollapsing to Hamilton's compactness. 9B.4 Convergence of Manifolds uses packing for Gromov's precompactness theorem. Perelman's definition of κ\kappa-noncollapsing (12A.4 κ-Noncollapsing) is a lower bound on the very ratio Vol⁡Brn\frac{\operatorname{Vol}B}{r^n} that this chapter controls from above.

History

Richard Bishop proved the absolute volume inequality in 1963 (it appears in Bishop and Crittenden's Geometry of Manifolds, 1964); Mikhail Gromov introduced the relative version and its use for compactness around 1980. Shiu-Yuen Cheng proved the maximal diameter theorem in 1975. The linear growth bound is due to Calabi (1975) and Yau (1976).

Recall Where we stand

In polar coordinates dV=A dr dθdV = \mathcal A\,dr\,d\theta with ∂rlog⁡A=Δr\partial_r\log\mathcal A = \Delta r. Laplacian comparison therefore makes Asn⁡kn−1\frac{\mathcal A}{\operatorname{sn}_k^{n-1}} nonincreasing, and integrating gives Bishop–Gromov: Vol⁡B(p,R)Vk(R)\frac{\operatorname{Vol}B(p, R)}{V_k(R)} is nonincreasing, at most 11, with equality only for the model. Relative comparison gives doubling and packing (N≤(2Rr)nN \leq (\frac{2R}{r})^n when Ric⁡≥0\operatorname{Ric} \geq 0), and for Ric⁡≥0\operatorname{Ric} \geq 0 it defines the asymptotic volume ratio, 11 only for Rn\mathbb{R}^n and 00 for cylinders, paraboloids and κ\kappa-solutions. Perelman's reduced volume is a space-time Bishop–Gromov. 9B.3 Collapsing and Noncollapsing asks what happens when volume is small: collapsing.

Exercises

Exercise 2.2 The volume element grows by the mean curvature

Let Φs\Phi_s be the flow of ∂r=∇r\partial_r = \nabla r, defined away from pp and the cut locus. Using ddsΦs∗dV=Φs∗(div⁡∂r dV)\frac{d}{ds}\Phi_s^*dV = \Phi_s^*(\operatorname{div}\partial_r\,dV) (8A.6 Flows and the Lie Derivative), show that ∂rlog⁡A=Δr\partial_r\log\mathcal A = \Delta r. Check it in Rn\mathbb{R}^n, where A=rn−1\mathcal A = r^{n-1}.

Solution

Φs\Phi_s maps exp⁡p(rθ)\exp_p(r\theta) to exp⁡p((r+s)θ)\exp_p((r + s)\theta), so in polar coordinates Φs∗(A dr dθ)=A(r+s,θ) dr dθ\Phi_s^*(\mathcal A\,dr\,d\theta) = \mathcal A(r + s, \theta)\,dr\,d\theta. Differentiating at s=0s = 0: ∂rA dr dθ=div⁡(∂r)A dr dθ\partial_r\mathcal A\,dr\,d\theta = \operatorname{div}(\partial_r)\mathcal A\,dr\,d\theta, and div⁡∇r=Δr\operatorname{div}\nabla r = \Delta r. In Rn\mathbb{R}^n: ∂rlog⁡rn−1=n−1r=Δr\partial_r\log r^{n-1} = \frac{n - 1}{r} = \Delta r.

Exercise 2.3 The ratio lemma

Let f,g>0f, g > 0 be integrable on (0,R0)(0, R_0) with fg\frac fg nonincreasing. Show that F(R)=∫0RfF(R) = \int_0^Rf and G(R)=∫0RgG(R) = \int_0^Rg have FG\frac FG nonincreasing. (Show (FG)′=fG−gFG2(\frac FG)' = \frac{fG - gF}{G^2} and fG−gF=∫0R(f(R)g(t)−g(R)f(t)) dt≤0fG - gF = \int_0^R(f(R)g(t) - g(R)f(t))\,dt \leq 0.)

Solution

For t≤Rt \leq R, f(t)g(t)≥f(R)g(R)\frac{f(t)}{g(t)} \geq \frac{f(R)}{g(R)}, so f(R)g(t)≤g(R)f(t)f(R)g(t) \leq g(R)f(t). Integrating in tt over [0,R][0, R] gives f(R)G(R)≤g(R)F(R)f(R)G(R) \leq g(R)F(R), so (FG)′≤0(\frac FG)' \leq 0.

Exercise 2.4 Packing

Suppose Ric⁡≥0\operatorname{Ric} \geq 0 and the balls B(xi,r)B(x_i, r), i=1,…,Ni = 1, \dots, N, are disjoint and contained in B(p,R)B(p, R). Show B(p,R)⊂B(xi,2R)B(p, R) \subset B(x_i, 2R), deduce Vol⁡B(xi,r)≥(r2R)nVol⁡B(p,R)\operatorname{Vol}B(x_i, r) \geq (\frac{r}{2R})^n\operatorname{Vol}B(p, R), and conclude N≤(2Rr)nN \leq (\frac{2R}{r})^n.

Solution

xi∈B(p,R)x_i \in B(p, R), so for y∈B(p,R)y \in B(p, R), d(xi,y)<2Rd(x_i, y) < 2R. Relative comparison with k=0k = 0: Vol⁡B(xi,r)≥(r2R)nVol⁡B(xi,2R)≥(r2R)nVol⁡B(p,R)\operatorname{Vol}B(x_i, r) \geq (\frac{r}{2R})^n\operatorname{Vol}B(x_i, 2R) \geq (\frac{r}{2R})^n\operatorname{Vol}B(p, R). Summing over the disjoint balls inside B(p,R)B(p, R): N(r2R)nVol⁡B(p,R)≤Vol⁡B(p,R)N(\frac{r}{2R})^n\operatorname{Vol}B(p, R) \leq \operatorname{Vol}B(p, R).

Exercise 2.5 Linear volume growth (guided)

Let MM be complete and noncompact with Ric⁡≥0\operatorname{Ric} \geq 0. For R≥2R \geq 2 pick xx with d(p,x)=Rd(p, x) = R (possible because MM is unbounded). Apply relative comparison at xx to the balls B(x,R−1)⊂B(x,R+1)B(x, R - 1) \subset B(x, R + 1), and observe that B(p,1)B(p, 1) lies in the annulus between them while B(x,R+1)⊂B(p,2R+1)B(x, R + 1) \subset B(p, 2R + 1). Deduce Vol⁡B(p,1)≤2nR+1Vol⁡B(p,2R+1)\operatorname{Vol}B(p, 1) \leq \frac{2n}{R + 1}\operatorname{Vol}B(p, 2R + 1), and hence that Vol⁡B(p,ρ)≥cρ\operatorname{Vol}B(p, \rho) \geq c\rho for ρ≥1\rho \geq 1, with c>0c > 0 depending on pp.

Solution

By relative comparison at xx, Vol⁡B(x,R−1)Vol⁡B(x,R+1)≥(R−1R+1)n\frac{\operatorname{Vol}B(x, R - 1)}{\operatorname{Vol}B(x, R + 1)} \geq (\frac{R - 1}{R + 1})^n, so the annulus A=B(x,R+1)∖B(x,R−1)A = B(x, R + 1)\setminus B(x, R - 1) has Vol⁡A≤(1−(R−1R+1)n)Vol⁡B(x,R+1)≤2nR+1Vol⁡B(x,R+1)\operatorname{Vol}A \leq \big(1 - (\frac{R - 1}{R + 1})^n\big)\operatorname{Vol}B(x, R + 1) \leq \frac{2n}{R + 1}\operatorname{Vol}B(x, R + 1). Since d(p,x)=Rd(p, x) = R, B(p,1)⊂AB(p, 1) \subset A, and B(x,R+1)⊂B(p,2R+1)B(x, R + 1) \subset B(p, 2R + 1). So Vol⁡B(p,1)≤2nR+1Vol⁡B(p,2R+1)\operatorname{Vol}B(p, 1) \leq \frac{2n}{R + 1}\operatorname{Vol}B(p, 2R + 1), that is Vol⁡B(p,2R+1)≥R+12nVol⁡B(p,1)\operatorname{Vol}B(p, 2R + 1) \geq \frac{R + 1}{2n}\operatorname{Vol}B(p, 1): linear growth with c=Vol⁡B(p,1)4nc = \frac{\operatorname{Vol}B(p, 1)}{4n}, say.

Exercise 2.6 The asymptotic volume ratio does not depend on the point

Show B(p,R−d)⊂B(q,R)⊂B(p,R+d)B(p, R - d) \subset B(q, R) \subset B(p, R + d) where d=d(p,q)d = d(p, q), and deduce that the limit defining AVR⁡\operatorname{AVR} is the same at pp and qq.

Solution

The inclusions follow from the triangle inequality. Dividing by ωnRn\omega_nR^n and using (R±d)nRn→1\frac{(R \pm d)^n}{R^n} \to 1: Vol⁡B(q,R)ωnRn\frac{\operatorname{Vol}B(q, R)}{\omega_nR^n} is squeezed between quantities converging to AVR⁡\operatorname{AVR} computed at pp.

Exercise 2.7 Maximal diameter (idea)

Suppose Ric⁡≥(n−1)g\operatorname{Ric} \geq (n - 1)g and d(p,q)=πd(p, q) = \pi. Using Bishop–Gromov at pp and at qq with radius π2\frac{\pi}{2}, and B(p,π2)∩B(q,π2)=∅B(p, \frac{\pi}{2})\cap B(q, \frac{\pi}{2}) = \emptyset, show Vol⁡M=∣Sn∣\operatorname{Vol}M = |S^n| and that both balls have the maximal volume allowed. (The equality case then gives Cheng's theorem.)

Solution

The balls are disjoint by the triangle inequality. Relative comparison at pp: Vol⁡B(p,π2)≥V1(π/2)V1(π)Vol⁡B(p,π)=12Vol⁡M\operatorname{Vol}B(p, \frac{\pi}{2}) \geq \frac{V_1(\pi/2)}{V_1(\pi)}\operatorname{Vol}B(p, \pi) = \frac12\operatorname{Vol}M, since B(p,π)B(p, \pi) is all of MM (diameter ≤π\leq \pi by Myers). Similarly at qq. Disjointness forces equality, Vol⁡B(p,π2)=12Vol⁡M\operatorname{Vol}B(p, \frac{\pi}{2}) = \frac12\operatorname{Vol}M, so the ratio Vol⁡B(p,R)V1(R)\frac{\operatorname{Vol}B(p, R)}{V_1(R)} is constant on [π2,π][\frac{\pi}{2}, \pi]. Then Asin⁡n−1r\frac{\mathcal A}{\sin^{n-1}r} is constant there in every direction, and since it is nonincreasing and tends to 11 at 00, in the equality case it is 11 throughout, which forces the model metric; in particular Vol⁡M=∣Sn∣\operatorname{Vol}M = |S^n|.

Exercise 2.8 Rehearsal: asymptotic volume ratios

(a) The cone dr2+a2r2gSn−1dr^2 + a^2r^2g_{S^{n-1}}, 0<a≤10 < a \leq 1, has Ric⁡≥0\operatorname{Ric} \geq 0 away from the tip (9A.5 Computing Curvature); show its AVR⁡\operatorname{AVR} is an−1a^{n-1}. (b) Show the cylinder Sn−1×RS^{n-1}\times\mathbb{R} has AVR⁡=0\operatorname{AVR} = 0. (c) For the paraboloid z=x2+y2z = x^2 + y^2, with ρ\rho the distance from the axis, the intrinsic radius is s(ρ)=∫0ρ1+4t2 dt∼ρ2s(\rho) = \int_0^\rho\sqrt{1 + 4t^2}\,dt \sim \rho^2 and the area is A(ρ)=∫0ρ2πt1+4t2 dt∼4π3ρ3A(\rho) = \int_0^\rho2\pi t\sqrt{1 + 4t^2}\,dt \sim \frac{4\pi}{3}\rho^3; show AVR⁡=0\operatorname{AVR} = 0. In 12B.2 The Structure of κ-Solutions the same conclusion for every κ\kappa-solution is what forces blow-down limits to be lower-dimensional.

Solution

(a) Vol⁡B(o,R)=∣Sn−1∣∫0R(ar)n−1dr=an−1ωnRn\operatorname{Vol}B(o, R) = |S^{n-1}|\int_0^R(ar)^{n-1}dr = a^{n-1}\omega_nR^n. (b) Vol⁡B(p,R)≤∣Sn−1(ρ)∣⋅2R\operatorname{Vol}B(p, R) \leq |S^{n-1}(\rho)|\cdot2R, linear in RR, so the ratio with RnR^n tends to 00 for n≥2n \geq 2. (c) Aπs2∼(4π/3)ρ3πρ4→0\frac{A}{\pi s^2} \sim \frac{(4\pi/3)\rho^3}{\pi\rho^4} \to 0.

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