ScalingStacks

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5.3 Gromov-Hausdorff convergence

On the regular locus ℛ⊂∂Δλ∨\mathcal{R}\subset\partial\Delta_{\lambda}^{\vee} we have a well defined real MA metric,

g∞={12​∑i,j∂2u∞∂xi​∂xj​d​xi​d​xj, on the face regions,12​∑i,j∂2u∞,m∂xi​∂xj​d​xi​d​xj, on the star regions.g_{\infty}=\begin{cases}\frac{1}{2}\sum_{i,j}\frac{\partial^{2}u_{\infty}}{\partial x_{i}\partial x_{j}}dx_{i}dx_{j},\quad\text{ on the face regions},\\ \frac{1}{2}\sum_{i,j}\frac{\partial^{2}u_{\infty,m}}{\partial x_{i}\partial x_{j}}dx_{i}dx_{j},\quad\text{ on the star regions}.\end{cases} (34)

Notice the definitions are compatible on overlapping regions. Let (ℛ¯,g∞)(\bar{\mathcal{R}},g_{\infty}) be the metric completion. The metric asymptotes (32)(33) say that in some Cl​o​c∞C^{\infty}_{loc} sense the collapsing CY metrics gC​Y,sg_{CY,s} converge to the metric g∞g_{\infty} on ℛ\mathcal{R}, and we know ℛ\mathcal{R} is path connected because its complement has zero ℋn−1\mathcal{H}^{n-1}-measure.

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Remark 5.9. We do not know if ℛ¯\bar{\mathcal{R}} is homeomorphic to ∂Δλ∨≃Sn\partial\Delta_{\lambda}^{\vee}\simeq S^{n}, as the regularity theory of the real MA equation on a singular affine manifold is not yet developed, and we know little about what can happen near singularities.

The goal of this section is to show

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Theorem 5.10. The subsequence of collapsing CY metrics (Xs,gC​Y,s)(X_{s},g_{CY,s}) converges in the Gromov-Hausdorff sense to (ℛ¯,g∞)(\bar{\mathcal{R}},g_{\infty}).

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Proposition 5.11. There is a uniform diameter bound

diam​(Xs,gC​Y,s)≤C.\text{diam}(X_{s},g_{CY,s})\leq C.
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Proof. This argument is essentially the same as [36, Thm 3.1]. We quote [36, Lem 3.2]:

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Lemma 5.12. Let (M2​n,g)(M^{2n},g) be a closed Riemannian manifold with R​i​c​(g)≥0Ric(g)\geq 0, let p∈Mp\in Mand 1<R≤d​i​a​m​(X,g)1<R\leq diam(X,g). Then R−14​n≤Vol​(B​(p,2​(R+1)))Vol​(B​(p,1))\frac{R-1}{4n}\leq\frac{\text{Vol}(B(p,2(R+1)))}{\text{Vol}(B(p,1))}.

Using Thm. 5.6, we can find inside the regular region of XsX_{s} some geodesic ball BgC​Y,s​(p,r)B_{g_{CY,s}}(p,r) of radius r<1r<1, occupying a nontrivial portion of the total volume:

OPENVol​(BgC​Y,s​(p,r)))Vol​(Xs)≥ϵ>0,\frac{\text{Vol}(B_{g_{CY,s}}(p,r)))}{\text{Vol}(X_{s})}\geq\epsilon>0,

with ϵ\epsilon independent of ss. Now applying the Lemma to the rescaled CY metric r−2​gC​Y,sr^{-2}g_{CY,s},

diam​(Xs)−r4​n​r≤Vol​(BgC​Y,s​(p,2​(diam​(Xs)+r)))Vol​(BgC​Y,s​(p,r))≤Vol​(Xs)Vol​(BgC​Y,s​(p,r))≤ϵ−1,\frac{\text{diam}(X_{s})-r}{4nr}\leq\frac{\text{Vol}(B_{g_{CY,s}}(p,2(\text{diam}(X_{s})+r)))}{\text{Vol}(B_{g_{CY,s}}(p,r))}\leq\frac{\text{Vol}(X_{s})}{\text{Vol}(B_{g_{CY,s}}(p,r))}\leq\epsilon^{-1},

so diam​(Xs)≤C​r≤C\text{diam}(X_{s})\leq Cr\leq C as required. ∎

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Proof. (Thm. 5.10) By Thm 5.6 we already know the metric convergence over any properly contained open subset of ℛ\mathcal{R}, which corresponds to a region Us⊂XsU_{s}\subset X_{s}, with nearly the full measure:

Vol​(Us)>(1−ϵ)​Vol​(Xs),\text{Vol}(U_{s})>(1-\epsilon)\text{Vol}(X_{s}),

where ϵ\epsilon can be chosen arbitrarily small. It now suffices to show any point p∈Xs∖Usp\in X_{s}\setminus U_{s} is close to UsU_{s}. For any r>0r>0 such that the geodesic ball BgC​Y,s​(p,r)⊂Xs∖UsB_{g_{CY,s}}(p,r)\subset X_{s}\setminus U_{s}, the Bishop-Gromov inequality implies

(rdiam​(Xs))2​n≤Vol​(BgC​Y,s​(p,r))Vol​(Xs)≤Vol​(Xs∖Us)Vol​(Xs)<ϵ.\left(\frac{r}{\text{diam}(X_{s})}\right)^{2n}\leq\frac{\text{Vol}(B_{g_{CY,s}}(p,r))}{\text{Vol}(X_{s})}\leq\frac{\text{Vol}(X_{s}\setminus U_{s})}{\text{Vol}(X_{s})}<\epsilon.

Taking the sup of all such rr,

distgC​Y,s​(p,Us)≤ϵ1/2​n​diam​(Xs)≤C​ϵ1/2​n,\text{dist}_{g_{CY,s}}(p,U_{s})\leq\epsilon^{1/2n}\text{diam}(X_{s})\leq C\epsilon^{1/2n},

which can be made arbitrarily small. ∎

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