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5. Codimension 4 Regularity of Singular Limits [01YG]

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5. Codimension 44 Regularity of Singular Limits

In this section we prove Theorem 1.1. Thus, we consider a Gromov-Hausdorff limit space,

(Mjn,dj,pj)⟶dG​H(X,d,p),\displaystyle(M^{n}_{j},d_{j},p_{j})\stackrel{{\scriptstyle d_{GH}}}{{\longrightarrow}}(X,d,p)\,, (5.1)

of a sequence of Riemannian manifolds (Mjn,gj,pj)(M^{n}_{j},g_{j},p_{j}), satisfying |RicMjn|≤n−1|{\rm Ric}_{M^{n}_{j}}|\leq n-1 and Vol⁡(B1​(pj))>v>0{\rm Vol}(B_{1}(p_{j}))>{\rm v}>0. We will show that there exists a subset 𝒮⊆X\mathcal{S}\subseteq X of codimension 44 such that X∖𝒮X\setminus\mathcal{S} is a C1,αC^{1,\alpha}-Riemannian manifold. In this section, we will show that 𝒮\mathcal{S} has Hausdorff codimension 4. We will postpone the improvement to Minkowski codimension 44 until Section 7.

As mentioned in Section 1, it has been understood since [ChCo2] that the main technical challenge lies in showing that spaces of the form ℝn−2×C⁡(Sβ1)\mathds{R}^{n-2}\times C(S^{1}_{\beta}), where Sβ1S^{1}_{\beta} is the circle of circumference β≤2​π\beta\leq 2\pi, cannot arise as limit spaces unless β=2​π\beta=2\pi and hence ℝn−2×C⁡(Sβ1)=ℝn\mathds{R}^{n-2}\times C(S^{1}_{\beta})=\mathds{R}^{n}. The Slicing Theorem (Theorem 1.8) was expressly designed to enable us to handle this point via a blow up argument. We will do this in Section 5.1.

In subsection 5.2 we then prove that more general spaces of the form ℝn−3×C⁡(Y)\mathds{R}^{n-3}\times C(Y) cannot arise as limit spaces. The proof of this statement, has a very different feel than the proof ruling out the codimension two limits, and essentially comes down to a bordism and curvature pinching argument for 33-manifolds.

Finally, in Section 5.3 we combine the tools developed in the previous subsections to prove the Hausdorff estimates of Theorem 1.1.

5.1. Nonexistence of Codimension 22 Singularities

In this subsection, we use the tools of Section 4 in order to prove that spaces that are (n−2)(n-2)-symmetric cannot arise as noncollapsed limits of manifolds with bounded Ricci curvature.

Theorem 5.1 ((n−2)(n-2)-Symmetric Limits).

Let (Mjn,gj,pj)(M^{n}_{j},g_{j},p_{j}) be a sequence of Riemannian manifolds satisfying |RicMjn|→0|{\rm Ric}_{M^{n}_{j}}|\to 0, Vol⁡(B1​(pj))>v>0{\rm Vol}(B_{1}(p_{j}))>{\rm v}>0 and such that

(Mjn,dj,pj)⟶dG​Hℝn−2×C⁡(Sβ1).\displaystyle(M_{j}^{n},d_{j},p_{j})\stackrel{{\scriptstyle d_{GH}}}{{\longrightarrow}}\mathds{R}^{n-2}\times C(S^{1}_{\beta})\,. (5.2)

Then β=2​π\beta=2\pi and ℝn−2×C⁡(Sβ1)=ℝn\mathds{R}^{n-2}\times C(S^{1}_{\beta})=\mathds{R}^{n}.

Proof of Theorem 5.1.

We will prove the result by contradiction. So let us assume it is false. Then there exists a sequence (Mjn,gj,pj)(M^{n}_{j},g_{j},p_{j}) of Riemannian manifolds satisfying |RicMjn|→0|{\rm Ric}_{M^{n}_{j}}|\to 0, Vol⁡(B1​(pj))>v>0{\rm Vol}(B_{1}(p_{j}))>{\rm v}>0 and such that

(Mjn,dj,pj)→(ℝn−2×C⁡(Sβ1),d,p),\displaystyle(M_{j}^{n},d_{j},p_{j})\to\big(\mathds{R}^{n-2}\times C(S^{1}_{\beta}),d,p\big)\,, (5.3)

with β<2​π\beta<2\pi and pp a vertex.

Note first that by the noncollapsing assumption we have β≥β0​(n,v)\beta\geq\beta_{0}(n,v).

Now by Lemma 1.7, there exists δj\delta_{j}-splitting maps uj:B2​(pj)→ℝn−2u_{j}:B_{2}(p_{j})\to\mathds{R}^{n-2} with δj→0\delta_{j}\to 0. Fix some sequence ϵj→0\epsilon_{j}\to 0 which is tending to zero so slowly compared to δj\delta_{j}, that Theorem 1.8 holds for uj:B2​(0)→ℝn−2u_{j}:B_{2}(0)\to\mathds{R}^{n-2} with ϵj\epsilon_{j}. Let Gϵj⊆B1​(0n−2)G_{\epsilon_{j}}\subseteq B_{1}(0^{n-2}) be the corresponding good values of uju_{j}, and let sj∈Gϵj∩B10−1​(0n−2)s_{j}\in G_{\epsilon_{j}}\cap B_{10^{-1}}(0^{n-2}) be fixed regular values.

Note that ℝn−2×C⁡(Sβ1)\mathds{R}^{n-2}\times C(S^{1}_{\beta}) is smooth outside of the singular set 𝒮=ℝn−2×{0}⊆ℝn−2×C⁡(Sβ1)\mathcal{S}=\mathds{R}^{n-2}\times\{0\}\subseteq\mathds{R}^{n-2}\times C(S^{1}_{\beta}). In particular on ℝn−2×C⁡(Sβ1)\mathds{R}^{n-2}\times C(S^{1}_{\beta}) we have rh​(x)≈1/d⁡(x,𝒮)r_{h}(x)\approx 1/d(x,\mathcal{S}), where rhr_{h} is the harmonic radius as in Section 1 and dd denotes distance. By the standard ϵ\epsilon-regularity theorem, it follows that the convergence of MjnM^{n}_{j} is in C1,α∩W2,qC^{1,\alpha}\cap W^{2,q} away from 𝒮\mathcal{S}, for every α<1\alpha<1 and q<∞q<\infty. Let fj:Bϵj−1​(p)→Bϵj−1​(pj)f_{j}:B_{\epsilon^{-1}_{j}}(p)\to B_{\epsilon^{-1}_{j}}(p_{j}) be the ϵj\epsilon_{j}-Gromov Hausdorff maps, and let us denote 𝒮j≡fj​(𝒮)⊆Mjn\mathcal{S}_{j}\equiv f_{j}(\mathcal{S})\subseteq M^{n}_{j}. Then by the previous statements, for every τ>0\tau>0, all jj sufficiently large, and x∈B1​(pj)∖Tτ​(𝒮j)x\in B_{1}(p_{j})\setminus T_{\tau}(\mathcal{S}_{j}), we have rh​(x)≥τ2r_{h}(x)\geq\frac{\tau}{2}.

Consider again the submanifold uj−1​(sj)∩B1​(pj)u^{-1}_{j}(s_{j})\cap B_{1}(p_{j}). Define the scale

rj=min⁡{rh​(x):x∈uj−1​(sj)∩B1​(pj)}.\displaystyle r_{j}=\min\{r_{h}(x):x\in u^{-1}_{j}(s_{j})\cap B_{1}(p_{j})\}\,. (5.4)

By the considerations of the previous paragraph, this minimum is actually obtained at some xj∈uj−1​(sj)∩B1​(pj)x_{j}\in u^{-1}_{j}(s_{j})\cap B_{1}(p_{j}), with xj→𝒮j∩B10−1​(pj)x_{j}\to\mathcal{S}_{j}\cap B_{10^{-1}}(p_{j}). Moreover, since Sβ1S^{1}_{\beta}, the cross-section of the cone factor, satisfies 0<β<2​π0<\beta<2\pi, it follows that rj→0r_{j}\to 0. According to Theorem 1.8, there exists a lower triangular matrix Aj∈G​L​(n−2)A_{j}\in GL(n-2) such that vj≡Aj∘(uj−sj):Brj​(xj)→ℝn−2v_{j}\equiv A_{j}\circ\big(u_{j}-s_{j}\big):B_{r_{j}}(x_{j})\to\mathds{R}^{n-2} is an ϵj\epsilon_{j}-splitting map. Note that we have renormalized so that each of our regular values is the zero level set.

Now let us consider the sequence (Mjn,rj−1​dj,xj)(M^{n}_{j},r_{j}^{-1}d_{j},x_{j}). After passing to a subsequence if necessary, which we will continue to denote by (Mjn,rj−1​dj,xj)(M^{n}_{j},r_{j}^{-1}d_{j},x_{j}), have

(Mjn,rj−1​dj,xj)⟶dG​H(X,dX,x),\displaystyle(M^{n}_{j},r_{j}^{-1}d_{j},x_{j})\stackrel{{\scriptstyle d_{GH}}}{{\longrightarrow}}(X,d_{X},x)\,, (5.5)

in the pointed Gromov-Hausdorff sense, where XX splits off ℝn−2\mathds{R}^{n-2} isometrically.

We begin by observing that by our noncollapsing assumption we have Vol⁡(B1​(xj))>c⁡(n)​v>0{\rm Vol}(B_{1}(x_{j}))>c(n){\rm v}>0, and hence, in the rescaled spaces, we have Vol⁡(Br​(xj))>c​v​rn{\rm Vol}(B_{r}(x_{j}))>c{\rm v}r^{n} for all r≤Rj→∞r\leq R_{j}\to\infty. In particular, XX has Euclidean volume growth at ∞\infty i.e. Vol⁡(Br​(x′))>c​v​rn{\rm Vol}(B_{r}(x^{\prime}))>c{\rm v}\,r^{n} for all r>0r>0.

After possibly passing to another subsequence, we can limit the functions vjv_{j} to a function v:X→ℝn−2v:X\to\mathds{R}^{n-2}. Note that by our normalization, we have vj:B2​(xj)→ℝn−2v_{j}:B_{2}(x_{j})\to\mathds{R}^{n-2} are ϵj\epsilon_{j}-splittings, and that by Theorem 1.11, we have for each R>2R>2 that vj:BR​(xj)→ℝn−2v_{j}:B_{R}(x_{j})\to\mathds{R}^{n-2} are C⁡(n,R)​ϵjC(n,R)\epsilon_{j}-splittings. In particular, we can conclude that

X=ℝn−2×S,\displaystyle X=\mathds{R}^{n-2}\times S\,, (5.6)

where v:X→ℝn−2v:X\to\mathds{R}^{n-2} is the projection map and S=u−1​(0)S=u^{-1}(0).

Now by construction, in the rescaled spaces we have for any y∈uj−1​(0)y\in u^{-1}_{j}(0) that rh​(y)≥1r_{h}(y)\geq 1. Therefore, the limit XX is C1,α∩W2,qC^{1,\alpha}\cap W^{2,q} in a neighborhood of u−1​(0)u^{-1}(0), and hence S=u−1​(0)S=u^{-1}(0) is a nonsingular surface. Thus, since X=ℝn−2×SX=\mathds{R}^{n-2}\times S it follows that XX is at least a C1,α∩W2,qC^{1,\alpha}\cap W^{2,q} manifold with rh≥1r_{h}\geq 1. Since the Ricci curvature is uniformly bounded, in fact tending to zero, we have by the standard ϵ\epsilon-regularity theorem that the convergence (Mjn,rj−1​dj,xj)→(X,dX,x)(M^{n}_{j},r_{j}^{-1}d_{j},x_{j})\to(X,d_{X},x) is in C1,α∩W2,qC^{1,\alpha}\cap W^{2,q}. Because the convergence is in C1,α∩W2,qC^{1,\alpha}\cap W^{2,q} we have that rhr_{h} converges continuously; [A90]. In particular, we have that rh​(xj′)→rh​(x′)r_{h}(x^{\prime}_{j})\to r_{h}(x^{\prime}) and so rh​(x′)=1r_{h}(x^{\prime})=1.

On the other hand, since |RicMjn|→0|{\rm Ric}_{M^{n}_{j}}|\to 0 and XX is C1,α∩W2,qC^{1,\alpha}\cap W^{2,q} it follows that XX is a smooth Ricci flat manifold. This is easiest to see by writing directly in harmonic coordinates on XX, see [A90] for the argument. Now since X=ℝn−2×SX=\mathds{R}^{n-2}\times S, we can conclude that SS is smooth and Ricci flat, hence flat. In particular, we have that XX is flat. Since we have already shown that XX has Euclidean volume growth, this implies that X=ℝnX=\mathds{R}^{n}. However, we have also already concluded that rh​(x′)=1r_{h}(x^{\prime})=1, which gives us our desired contradiction. ∎

We end this subsection with the following corollary, which states that a noncollapsed limit space is smooth away from a set of codimension 33. We will use this in the next subsection to show (n−3)(n-3)-symmetric splittings cannot arise as limits.

Corollary 5.2.

Let (Mjn,gj,pj)(M^{n}_{j},g_{j},p_{j}) be a sequence of Riemannian manifolds satisfying |RicMjn|≤n−1|{\rm Ric}_{M^{n}_{j}}|\leq n-1, Vol⁡(B1​(pj))>v>0{\rm Vol}(B_{1}(p_{j}))>{\rm v}>0 and such that

(Mjn,dj,pj)→(X,d,p).\displaystyle(M_{j}^{n},d_{j},p_{j})\to(X,d,p)\,. (5.7)

Then there exists a subset, 𝒮⊆X\mathcal{S}\subseteq X, with dim𝒮≤n−3\dim\mathcal{S}\leq n-3, such that for each x∈X∖𝒮x\in X\setminus\mathcal{S}, we have rh​(x)>0r_{h}(x)>0. In particular, x∈X∖𝒮x\in X\setminus\mathcal{S} is a C1,αC^{1,\alpha} Riemannian manifold.

Proof.

Recall the standard stratification of XX. In particular, if we consider the subset 𝒮n−3⊂X\mathcal{S}^{n-3}\subset X we have that dim𝒮n−3≤n−3\dim\mathcal{S}^{n-3}\leq n-3, and that for every point x∉𝒮n−3x\not\in\mathcal{S}^{n-3} there exists some tangent cone at xx which is isometric to ℝn−2×C⁡(Sβ1)\mathds{R}^{n-2}\times C(S^{1}_{\beta}). That is, there exists ra→0r_{a}\to 0 such that

(X,ra−1​d,x)→ℝn−2×C⁡(Sβ1).\displaystyle(X,r_{a}^{-1}d,x)\to\mathds{R}^{n-2}\times C(S^{1}_{\beta})\,. (5.8)

However by Theorem 5.1 we then have β=2​π\beta=2\pi, which is to say that

(X,ra−1​d,x)→ℝn.\displaystyle(X,r_{a}^{-1}d,x)\to\mathds{R}^{n}\,. (5.9)

Thus, for a∈ℕa\in\mathds{N} sufficiently large, we can apply the standard ϵ\epsilon-regularity theorem, Theorem 2.3, to see that a neighborhood of xx is a C1,αC^{1,\alpha} Riemannian manifold, which proves the corollary. ∎

5.2. Nonexistence of Codimension 33 singularities

In this subsection we use the tools of Section 4 and Section 5.1 in order to prove that (n−3)(n-3)-symmetric metric spaces cannot arise as limits of manifolds with bounded Ricci curvature. Specifically, we prove the following:

Theorem 5.3 ((n−3)(n-3)-Symmetric Limits).

Let (Mjn,gj,pj)(M^{n}_{j},g_{j},p_{j}) be a sequence of Riemannian manifolds satisfying |RicMjn|→0|{\rm Ric}_{M^{n}_{j}}|\to 0, Vol⁡(B1​(pj))>v>0{\rm Vol}(B_{1}(p_{j}))>{\rm v}>0 and such that

(Mjn,dj,pj)→ℝn−3×C⁡(Y),\displaystyle(M_{j}^{n},d_{j},p_{j})\to\mathds{R}^{n-3}\times C(Y)\,, (5.10)

in the pointed Gromov-Hausdorff sense, where YY is some compact metric space. Then Y=S2​(1)Y=S^{2}(1) is isometric to the unit 22-sphere and hence ℝn−3×C⁡(Y)=ℝn\mathds{R}^{n-3}\times C(Y)=\mathds{R}^{n}.

Proof.

Let us assume that this is not the case and study such a limit space ℝn−3×C⁡(Y)\mathds{R}^{n-3}\times C(Y). The first observation is that by Corollary 5.2, it follows that YY is a smooth surface. Indeed, if there were a point y∈Yy\in Y such that rh​(y)=0r_{h}(y)=0. Then since X=ℝn−3×C⁡(Y)X=\mathds{R}^{n-3}\times C(Y) it would follow that there is a set of codimension at least 22 such that rh≡0r_{h}\equiv 0, which cannot happen by Corollary 5.2.

Since YY a C1,α∩W2,qC^{1,\alpha}\cap W^{2,q} manifold and |RicMjn|→0|{\rm Ric}_{M^{n}_{j}}|\to 0, it follows that YY is a smooth Einstein manifold satisfying RicY=g{\rm Ric}_{Y}=g. Because YY is a surface, this means in particular that YY has constant sectional curvature ≡1\equiv 1. Thus, either Y=ℝ​ℙ2Y=\mathds{R}\mathds{P}^{2} or Y=S2Y=S^{2}, the unit 22-sphere, and in the latter case we are done.

So let us study the case Y=ℝ​ℙ2Y=\mathds{R}\mathds{P}^{2}. For ϵ>0\epsilon>0 small, choose uj:B2​(pj)→ℝn−3u_{j}:B_{2}(p_{j})\to\mathds{R}^{n-3} to be an ϵ\epsilon-splitting as in Lemma 1.7. Note that away from the singular set 𝒮≡ℝn−3×{0}\mathcal{S}\equiv\mathds{R}^{n-3}\times\{0\} we have that the MjnM_{j}^{n} converge to ℝn−3×C⁡(Y)\mathds{R}^{n-3}\times C(Y) in C1,αC^{1,\alpha}. If fj:B2​(p)→B2​(pj)f_{j}:B_{2}(p)\to B_{2}(p_{j}) denote the Gromov-Hausdorff maps, we put 𝒮j=fj​(𝒮)\mathcal{S}_{j}=f_{j}(\mathcal{S}). Then for τ>0\tau>0 small but fixed, we have for jj sufficiently large, that on B1​(p)∖Tτ​(𝒮j)B_{1}(p)\setminus T_{\tau}(\mathcal{S}_{j}), the estimates |∇uj|>12|\nabla u_{j}|>\frac{1}{2} and |∇2uj|≤1|\nabla^{2}u_{j}|\leq 1 hold.

Consider Poisson approximation hjh_{j} to the square of distance function d2​(x,pj)d^{2}(x,p_{j}) on B2​(pj)B_{2}(p_{j}). That is, Δ​hj=2​n\Delta h_{j}=2n and hj=1h_{j}=1 on ∂B2​(pj)\partial B_{2}(p_{j}). We have (see for instance [ChCo1]) that |hj−d⁡(⋅,pj)|→0|h_{j}-d(\cdot,p_{j})|\to 0 uniformly in B2​(pj)B_{2}(p_{j}), and again because the convergence is in C1,αC^{1,\alpha} we have for jj sufficiently large that |∇h|>δ|\nabla h|>\delta and |∇2h|≤4​n|\nabla^{2}h|\leq 4n on B1​(p)∖Bτ​(𝒮j)B_{1}(p)\setminus B_{\tau}(\mathcal{S}_{j}). Once again, appealing to the C1,αC^{1,\alpha} convergence, for all jj sufficiently large and all s∈B1​(0n−3)s\in B_{1}(0^{n-3}) we have that u−1​(s)∩h−1​(1)u^{-1}(s)\cap h^{-1}(1) is diffeomorphic to ℝ​ℙ2\mathds{R}\mathds{P}^{2}. By Sard’s theorem, there exists a regular value sj∈B1​(0n−3)s_{j}\in B_{1}(0^{n-3}). Then for jj sufficiently large, uj−1(sj)∩{h≤1}u^{-1}_{j}(s_{j})\cap\{h\leq 1\} is a smooth 33-manifold, whose boundary is diffeomorphic to ℝ​ℙ2\mathds{R}\mathds{P}^{2}. However, the second Stiefel-Whitney number of ℝ​ℙ2\mathds{R}\mathds{P}^{2} is nonzero, and in particular, ℝ​ℙ2\mathds{R}\mathds{P}^{2} does not bound a smooth 33-manifold. This contradicts Y=ℝ​ℙ2Y=\mathds{R}\mathds{P}^{2}.

∎

5.3. Proof of Hausdorff Estimates of Theorem 1.1

With Theorem 5.3 in hand, the proof of Theorem 1.1 becomes standard, and follows the same lines as the proof of Corollary 5.2. Thus, consider a sequence

(Mjn,dj,pj)→(X,d,p)\displaystyle(M^{n}_{j},d_{j},p_{j})\to(X,d,p) (5.11)

of Riemannian manifolds satisfying |RicMjn|≤n−1|{\rm Ric}_{M^{n}_{j}}|\leq n-1 and Vol⁡(B1​(pj))>v>0{\rm Vol}(B_{1}(p_{j}))>{\rm v}>0, which Gromov-Hausdorff converge to some XX. Recall again the standard stratification of XX, which is reviewed in Section 2.1. More specifically let us consider the closed stratum 𝒮n−4​(X)⊆X\mathcal{S}^{n-4}(X)\subseteq X. On the one hand, we have from [ChCo1]

dim𝒮n−4≤n−4.\displaystyle\dim\mathcal{S}^{n-4}\leq n-4\,. (5.12)

On the other hand, we have that for every point x∉𝒮n−4x\not\in\mathcal{S}^{n-4}, there exists some tangent cone at xx which is isometric to ℝn−3×C⁡(Y)\mathds{R}^{n-3}\times C(Y). That is, for some sequence ra→0r_{a}\to 0 we have

(X,ra−1​d,x)→ℝn−3×C⁡(Y).\displaystyle(X,r_{a}^{-1}d,x)\to\mathds{R}^{n-3}\times C(Y)\,. (5.13)

However, by Theorem 5.3, we have that YY is isometric to the unit 22-sphere, and hence,

(X,ra−1​d,x)→ℝn.\displaystyle(X,r_{a}^{-1}d,x)\to\mathds{R}^{n}\,. (5.14)

Then for a∈ℕa\in\mathds{N} sufficiently large, we can apply the standard ϵ\epsilon-regularity theorem, Theorem 2.3, to see that rh​(x)>0r_{h}(x)>0, and hence that a neighborhood of xx is a C1,αC^{1,\alpha} Riemannian manifold, which proves the theorem.

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