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Complete Calabi-Yau metrics in the complement of two divisors

Collins, Tristan C. · Li, Yang

Original paper

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Complete Calabi-Yau metrics in the complement of two divisors

Tristan C. Collins    Yang Li
Abstract

We construct new complete Calabi-Yau metrics on the complement of an anticanonical divisors DD in a Fano manifold of dimension at least three, when DD consists of two transversely intersecting smooth divisors. The asymptotic geometry is modeled on a generalization of the Calabi ansatz, related to the non-archimedean Monge-Ampère equation.

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1 Introduction

Following Yau’s solution of the Calabi conjecture [22], the analytic approach to the construction of complete Calabi-Yau metrics on noncompact manifolds was initiated by the seminal works of Tian-Yau [16, 17] who proved the following fundamental theorem

[021Y]
Theorem 1.1 (Tian-Yau, [16]).

Given a smooth irreducible anticanonical divisor DD on a smooth Fano manifold X¯\bar{X}, then the complement X=X¯∖DX=\bar{X}\setminus D admits a complete Calabi-Yau metric.

The asymptotic geometry, from the holomorphic viewpoint, is modelled on the normal bundle 𝒪⁡(D)|D=−KX|D→D\mathcal{O}(D)|_{D}=-K_{X}|_{D}\to D. This total space carries a model metric known as the Calabi ansatz, which specifies the asymptotic behaviour of the desired Calabi-Yau metric. The main gist of Tian and Yau’s work, which is improved later by Hein [8] among others, is that once we have a good asymptotic ansatz, then running a non-compact version of Yau’s proof of the Calabi conjecture would produce an actual Calabi-Yau metric on XX.

In the current paper we are motivated by the following well-known question, which dates back to the work of Tian-Yau;

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Question.

(‘Tian-Yau problem’) Let X¯\bar{X} be a smooth nn-dimensional Fano manifold, and D=∑DiD=\sum D_{i} be an anticanonical divisor, which we assume to be simple normal crossing, with only multiplicity one components. Let X=X¯∖DX=\bar{X}\setminus D, then XX has a nowhere vanishing holomorphic volume form Ω\Omega. When does XX admit a complete Calabi-Yau metric?

This setup has plenty of examples, for instance X¯\bar{X} can be ℂ​ℙn\mathbb{CP}^{n}, and DD is a multiplicity one simple normal crossing divisor in 𝒪⁡(n+1).\mathcal{O}(n+1). Morally speaking, we are asking ‘what would happen to the Tian-Yau construction once DD breaks up into several components’. Our main result is a solution of the Tian-Yau problem in the case of two proportional divisors.

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Theorem 1.2.

Let X¯\bar{X} be a smooth nn-dimensional Fano manifold with n≥3n\geq 3, whose anticanonical bundle is (d1+d2)​L0(d_{1}+d_{2})L_{0} for some positive line bundle L0L_{0}, and d1,d2d_{1},d_{2} are positive integers. Let D1,D2D_{1},D_{2} be two transversally intersecting smooth divisors in the linear system associated to d1​L0d_{1}L_{0} and d2​L0d_{2}L_{0} respectively. Then X=X¯∖D1∪D2X=\bar{X}\setminus D_{1}\cup D_{2} admits a complete Calabi-Yau metric.

More precisely, the holomorphic geometry in the generic region near infinity is modeled on the total space of the bundle d1​L0⊕d2​L0→D1∩D2d_{1}L_{0}\oplus d_{2}L_{0}\to D_{1}\cap D_{2}. We will explain that there is a generalized Calabi ansatz on (an open subset of) this total space, which is associated with a PDE we call the non-archimedean Monge-Ampère equation. This story has its origin in the context of polarized degenerations, non-archimedean geometry and the SYZ conjecture [14]. In our specialized setting, this equation can be dimensionally reduced to an ODE, whose solutions can be rather explicitly given in terms of hypergeometric functions.

The infinity of XX also contains non-generic regions, which complex geometrically correspond to the neighbourhood of D1∖D2D_{1}\setminus D_{2} (resp. D2∖D1D_{2}\setminus D_{1}) inside X¯\bar{X}. Notice that D1∩D2D_{1}\cap D_{2} is an anticanonical divisor inside the Fano manifold D1D_{1} (resp. D2D_{2}), and the metric geometry in the non-generic region involves a fibration by the Tian-Yau metrics on D1∖D2D_{1}\setminus D_{2} (resp. D2∖D1D_{2}\setminus D_{1}) with some power law scalings. Matching the generalized Calabi ansatz with the metric behaviour in the non-generic region involves a nontrivial ODE matching problem.

The main strategy to construct the Calabi-Yau metric, is to first produce an approximate metric ansatz, and after suitably improving the decay rate of the volume form error, we appeal to Tian-Yau-Hein’s existence package. This strategy has been used in a number of recent works, notably [10][12][13][6][20].

Our construction suggests that the Tian-Yau problem has an inductive structure in terms of the depth of intersections of the divisors DiD_{i} on X¯\bar{X}. For instance, in the case of three divisors D1,D2,D3D_{1},D_{2},D_{3} with nonempty intersections, we expect the Tian-Yau problem on D1∖(D2∪D3)∩D1D_{1}\setminus(D_{2}\cup D_{3})\cap D_{1} (and the cyclic permutations) to appear in the non-generic region at infinity. The generic region would involve a generalized Calabi ansatz metric, associated with a more complicated non-archimedean Monge-Ampère equation, whose boundary conditions are prescribed by the need to match with the nongeneric regions. We think the principal remaining difficulty is then to solve the non-archimedean Monge-Ampère equation, which can in general no longer be reduced to an ODE as we increase the number of divisors. Another interesting direction is to further develop the link with non-archimedean geometry (cf. section 2.8.3).

The organization of this paper is as follows. Section 2 contains most of the geometric aspects. It introduces the generalized Calabi ansatz, the ODE reduction of the non-archimedean Monge-Ampère equation, and the boundary conditions. We also discuss further relations to the literature and future directions. Section 3 explicitly solves the ODE and implements the matching problem. Section 4 is concerned with producing an approximate metric ansatz, and the rather technical issue of error estimates. Section 5 reviews the Tian-Yau-Hein existence package, and hammers a few final nails.

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Acknowledgement.

Y.L is a current Clay Research Fellow and a CLE Moore Instructor at MIT. He thanks S. Sun for related discussions in the past. T.C.C is supported in part by NSF CAREER grant DMS-1944952 and an Alfred P. Sloan Fellowship.

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2 Generalized Calabi ansatz and ODE reduction

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2.1 The generalized Calabi ansatz

We shall describe an approximate ansatz for producing Calabi-Yau metrics, which simultaneously generalizes the Calabi ansatz on the total space of a positive line bundle over a compact Calabi-Yau manifold, and the semiflat metrics coming from torus invariant dimensional reductions of Calabi-Yau metrics. A very closely related ansatz in the context of polarized algebraic degenerations, was discovered in [14] in an attempt to give a conjectural differential geometric interpretation to the non-archimedean Monge-Ampère equation. Some of our terminologies will therefore reflect the non-archimedean origin of this ansatz.

Let L1,…​LmL_{1},\ldots L_{m} be positive line bundles over an (n−m)(n-m)-dimensional compact Calabi-Yau manifold YY with positively curved smooth Hermitian metrics hL1,…​hLmh_{L_{1}},\ldots h_{L_{m}}, and let ZZ be the total space of L1⊕…⊕Lm→YL_{1}\oplus\ldots\oplus L_{m}\to Y. Let rir_{i} be the radius distance function on LiL_{i}. In local holomorphic trivializations of LiL_{i}, the Hermitian metric on LiL_{i} can be written in terms of local potentials as hLi=e−2​ϕih_{L_{i}}=e^{-2\phi_{i}}, and the radius distance ri=|ξi|​e−ϕir_{i}=|\xi_{i}|e^{-\phi_{i}}, where ξi\xi_{i} are the local fibre coordinates on LiL_{i}. Our task is to construct approximate Calabi-Yau metrics on the region {0<ri≪1,∀i}\{0<r_{i}\ll 1,\forall i\} inside ZZ, on the line bundle L→ZL\to Z obtained by pulling back a (semi-positive) line bundle L→XL\to X. For our main intended applications, LL is in fact trivial, and m=2m=2. An important conceptual point is that these ansatz metrics will be incomplete in the ri∼1r_{i}\sim 1 region. Their aim is to provide local metric models on the generic regions of complete Calabi-Yau manifolds, and the global problem would also involve the nontrivial step of finding partial completions of these ansatz metrics. Concretely, this incompleteness means in the ri∼1r_{i}\sim 1 region this particular ansatz breaks down, and one must find some alternative ansatz.

It would be helpful to keep in mind that the metric will look like an iterated fibration. On the smallest scale, we have the TmT^{m} tori, coming from the circle directions of the line bundles L1,…​LmL_{1},\ldots L_{m}. These are fibred over compact manifolds diffeomorphic to YY, which are close to being Calabi-Yau with length scale much bigger than the tori, and this torus fibration structure is in turn fibred over mm noncompact real directions, corresponding roughly to the log⁡ri\log r_{i} variables. The length scale of the base is much larger than the intermediate length scale of the YY-fibres.

[0224]
Notation.

Our convention is d=∂+∂¯d=\partial+\bar{\partial}, dc=−12​π(−∂+∂¯)d^{c}=\frac{\sqrt{-1}}{2\pi}(-\partial+\bar{\partial}), so d​dc=−1π​∂∂¯dd^{c}=\frac{\sqrt{-1}}{\pi}\partial\bar{\partial}. Given a Hermitian metric hh on a line bundle LL, its curvature form is −d​dc​log⁡h1/2-dd^{c}\log h^{1/2} in the class c1​(L)c_{1}(L).

Let hLh_{L} be a smooth Hermitian metric on L→YL\to Y, which we pull back to L→ZL\to Z. For our main applications, LL is trivial and hL=1h_{L}=1. To zeroth approximation, we try the ansatz (which shall be improved later)

h1=hL​exp⁡(−2​u​(−log⁡r1,…,−log⁡rm))h_{1}=h_{L}\exp\left(-2u(-\log r_{1},\ldots,-\log r_{m})\right)

where uu is some smooth convex function, which should be thought of as the leading order Kähler potential in a particular normalisation convention. Write xi=−log⁡rix_{i}=-\log r_{i}, where the sign is chosen so that xi>0x_{i}>0 in the region of interest. We calculate the Kähler metric (the positivity is not automatic, and amounts to an extra assumption)

−d​dc​log⁡h11/2=−d​dc​log⁡hL1/2+d​dc​u=−d​dc​log​hL1/2+∑∂2u∂xi​∂xj​d​log​ri∧dc​log​rj−∑∂u∂xi​d​dc​log​ri.\begin{split}&-dd^{c}\log h_{1}^{1/2}=-dd^{c}\log h_{L}^{1/2}+dd^{c}u\\ =&-dd^{c}\log h_{L}^{1/2}+\sum\frac{\partial^{2}u}{\partial x_{i}\partial x_{j}}d\log r_{i}\wedge d^{c}\log r_{j}-\sum\frac{\partial u}{\partial x_{i}}dd^{c}\log r_{i}.\end{split}

Recall in local coordinates ri=|ξi|​e−ϕir_{i}=|\xi_{i}|e^{-\phi_{i}}. The Hessian term contains a term

−14​π​∑∂2u∂xi​∂xj​d​log⁡ξi∧d​log⁡ξj¯,\frac{\sqrt{-1}}{4\pi}\sum\frac{\partial^{2}u}{\partial x_{i}\partial x_{j}}d\log\xi_{i}\wedge d\overline{\log\xi_{j}},

which for |ξi|≪1|\xi_{i}|\ll 1 exponentially dominates the TmT^{m}-tori and the mm base directions, since ∑d​log⁡ξi∧d​log⁡ξi¯\sum d\log\xi_{i}\wedge d\overline{\log\xi_{i}} is exponentially larger than ∑d​ξi∧d​ξi¯\sum d\xi_{i}\wedge d\overline{\xi_{i}} in the logarithmic coordinates. The term

−∑∂u∂xiddclogri=∑∂u∂xiddcϕi,-\sum\frac{\partial u}{\partial x_{i}}dd^{c}\log r_{i}=\sum\frac{\partial u}{\partial x_{i}}dd^{c}\phi_{i},

since d​dc​log⁡|ξi|=0dd^{c}\log|\xi_{i}|=0 holds for ξi≠0\xi_{i}\neq 0, which is valid on the region 0<ri≪10<r_{i}\ll 1 under consideration. The ansatz will only be used in the region with

|D2​u|≪1≪|D​u|.|D^{2}u|\ll 1\ll|Du|.

As such, we can essentially ignore the other contributions produced by the Hessian term.

There are compact directions diffeomorphic to YY. For this, notice for each fixed value of x=(x1,…​xm)x=(x_{1},\ldots x_{m}), we get a TmT^{m}-invariant subset Zx⊂ZZ_{x}\subset Z, which projects down to YY via the natural map Z→YZ\to Y. This projection map is topologically the quotient map by the TmT^{m}-action, so Zx/TmZ_{x}/T^{m} is naturally diffeomorphic to YY. Since Zx/TmZ_{x}/T^{m} has no a priori complex structure, one cannot say that this is a biholomorphism. Nevertheless, the natural Riemannian metric on ZxZ_{x} induces a metric on Zx/TmZ_{x}/T^{m} by looking at the transverse directions to the TmT^{m}-action, and via the diffeomorphism this is close to the Kähler metric on YY

−d​dc​log⁡hL1/2+∑∂u∂xi​d​dc​ϕi.-dd^{c}\log h_{L}^{1/2}+\sum\frac{\partial u}{\partial x_{i}}dd^{c}\phi_{i}. (1)

This expression requires some explanation: by definition −d​dc​log⁡hL1/2-dd^{c}\log h_{L}^{1/2} and d​dc​ϕidd^{c}\phi_{i} make sense on YY. The term ∂u∂xi\frac{\partial u}{\partial x_{i}} is a function of xx, and for fixed xx it is merely a constant coefficient on YY. Notice the metric (1) on YY lies in the Kähler class 𝒟​u=c1​(L)+∑∂u∂xi​c1​(Li)\mathcal{D}u=c_{1}(L)+\sum\frac{\partial u}{\partial x_{i}}c_{1}(L_{i}). The reason we are able to acquire a cohomology class which is not obvious in the topological setup, comes from the distributional terms of d​dc​log⁡|ξi|dd^{c}\log|\xi_{i}| being discarded in the above calculations. We will refer to this 𝒟​u\mathcal{D}u as an ‘effective Kähler class’, since it is only present in the effective approximate description of the metric. Its size affects the length scale of the metric on the YY-fibres.

The next goal is to improve the metric so that the YY-fibres approximately have the Calabi-Yau metrics in the same class c1​(L)+∑∂u∂xi​c1​(Li)c_{1}(L)+\sum\frac{\partial u}{\partial x_{i}}c_{1}(L_{i}). This is conceptually similar to the semi-Ricci-flat metrics in the context of holomorphic fibred Calabi-Yau manifolds [18]. We take

h=h1​exp⁡(−2​ϕx),h=h_{1}\exp(-2\phi_{x}),

where for each xx, we associate some potential ϕx\phi_{x} on YY, which pulls back to ZxZ_{x}, so varying over all xx we get a function on an open subset of ZZ. We shall assume that the dependence on xx is sufficiently weak. Then the dominant effect is to change the metric on Zx/Tm≃YZ_{x}/T^{m}\simeq Y to

−d​dc​log⁡hL1/2+∑∂u∂xi​d​dc​ϕi+d​dc​ϕx,-dd^{c}\log h_{L}^{1/2}+\sum\frac{\partial u}{\partial x_{i}}dd^{c}\phi_{i}+dd^{c}\phi_{x}, (2)

and the other effects in the log⁡ξi\log\xi_{i} directions are suppressed. We choose ϕx\phi_{x} so that the effective fibre metrics (2) are the unique Calabi-Yau metrics in the cohomology class 𝒟​u​(x)\mathcal{D}u(x). This determines ϕx\phi_{x} up to fibrewise constants depending on xx. For the purpose of constructing approximate Calabi-Yau metrics, the choice is inessential as long as the xx-derivatives are small enough, just like what happens for semi-Ricci-flat metrics.

To leading order,

(−d​dc​log⁡h1/2)n≈n!(n−m)!​det(D2​u)​∏1m−14​π​d​log⁡ξi∧d​log⁡ξi¯∧(−d​dc​log⁡hL1/2+∑∂u∂xi​d​dc​ϕi+d​dc​ϕx)n−m=n!​∫Y(𝒟​u)n−m(n−m)!​det(D2​u)​(∏1m−14​π​d​log⁡ξi∧d​log⁡ξi¯)∧−1(n−m)2​ΩY∧Ω¯Y,\begin{split}&(-dd^{c}\log h^{1/2})^{n}\approx\frac{n!}{(n-m)!}\det(D^{2}u)\prod_{1}^{m}\frac{\sqrt{-1}}{4\pi}d\log\xi_{i}\wedge d\overline{\log\xi_{i}}\\ &\wedge(-dd^{c}\log h_{L}^{1/2}+\sum\frac{\partial u}{\partial x_{i}}dd^{c}\phi_{i}+dd^{c}\phi_{x})^{n-m}\\ =&\frac{n!\int_{Y}(\mathcal{D}u)^{n-m}}{(n-m)!}\det(D^{2}u)(\prod_{1}^{m}\frac{\sqrt{-1}}{4\pi}d\log\xi_{i}\wedge d\overline{\log\xi_{i}})\wedge\sqrt{-1}^{(n-m)^{2}}\Omega_{Y}\wedge\overline{\Omega}_{Y},\end{split}

where ΩY\Omega_{Y} is the holomorphic volume form on YY, normalized to

−1(n−m)2​∫YΩY∧Ω¯Y=1.\sqrt{-1}^{(n-m)^{2}}\int_{Y}\Omega_{Y}\wedge\overline{\Omega}_{Y}=1.

The term ∫Y(𝒟​u)n−m\int_{Y}(\mathcal{D}u)^{n-m} is intersection theoretic, and is polynomial in the derivative of uu. The natural holomorphic form on ZZ is up to a global constant

Ω=∏1md​log⁡ξi∧ΩY,\Omega=\prod_{1}^{m}d\log\xi_{i}\wedge\Omega_{Y}, (3)

which is well defined independent of trivializations. We see that

(−d​dc​log⁡h1/2)n≈const ​Ω∧Ω¯​det(D2​u)​∫Y(𝒟​u)n−m.(-dd^{c}\log h^{1/2})^{n}\approx\text{const }\Omega\wedge\overline{\Omega}\det(D^{2}u)\int_{Y}(\mathcal{D}u)^{n-m}.

Thus provided the various assumptions involved in the approximation are satisfied, then the condition for the metric −d​dc​log⁡h1/2-dd^{c}\log h^{1/2} to define an approximate Calabi-Yau metric is

det(D2​u)​∫Y(𝒟​u)n−m=const.\det(D^{2}u)\int_{Y}(\mathcal{D}u)^{n-m}=\text{const}. (4)

This is a Monge-Ampère type PDE on the real mm-dimensional base, which we call the non-archimedean Monge-Ampère equation (NA MA for short) on account of a very similar construction in [14]. The associated almost Calabi-Yau metric is called the generalized Calabi ansatz.

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2.2 Semiflat metrics and the Calabi ansatz

The generalized Calabi ansatz has two familiar special cases:

For m=nm=n, then YY is just a point, and 0<ri≪10<r_{i}\ll 1 amounts to the subset |ξi|≪1|\xi_{i}|\ll 1 inside (ℂ∗)n(\mathbb{C}^{*})^{n}. The NA MA equation is just the real MA equation

det(D2​u)=const.\det(D^{2}u)=\text{const}.

The ansatz then produces a Calabi-Yau metric, known as the semiflat metric, familiar in the SYZ conjecture [15].

For m=1m=1, and LL trivial, then ZZ is the total space of a positive line bundle L1L_{1} over an (n−1)(n-1)-dimensional Calabi-Yau manifold YY. We then take hL1h_{L_{1}} to be the Hermitian metric corresponding to the Calabi-Yau metric in c1​(L1)c_{1}(L_{1}). We can also view hL1h_{L_{1}} as a function on ZZ, equal to rL12r_{L_{1}}^{2}. Up to a normalising constant, the Calabi ansatz is

ωC​a​l=nn+1​d​dc​(−log⁡hL11/2)(n+1)/n.\omega_{Cal}=\frac{n}{n+1}dd^{c}(-\log h_{L_{1}}^{1/2})^{(n+1)/n}.

We compare this to the NA MA equation (4) in this case: uu is a function of a single real variable xx, satisfying

u′′​u′n−1=const.u^{\prime\prime}u^{\prime n-1}=\text{const}.

Up to constant u=x(n+1)/nu=x^{(n+1)/n}. Thus the NA MA equation reproduces the Calabi ansatz.

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2.3 Simplifications for proportional line bundles

A special case of the generalized Calabi ansatz is when LL is trivial, and Li=di​L0L_{i}=d_{i}L_{0} for some positive line bundle L0L_{0} and positive integers di>0d_{i}>0. In this case, we can take hL=1h_{L}=1, and hLih_{L_{i}} is the suitable tensor power of hL0h_{L_{0}}, where hL0h_{L_{0}} can be chosen to correspond to the Calabi-Yau metric in the class c1​(L0)c_{1}(L_{0}). The ansatz metric is simply

d​dc​u=∑∂2u∂xi​∂xj​d​log⁡ri∧dc​log⁡rj+∑∂u∂xi​d​dc​ϕi=∑∂2u∂xi​∂xj​d​log⁡ri∧dc​log⁡rj+(∑∂u∂xi​di)​d​dc​ϕ0.\begin{split}dd^{c}u=\sum\frac{\partial^{2}u}{\partial x_{i}\partial x_{j}}d\log r_{i}\wedge d^{c}\log r_{j}+\sum\frac{\partial u}{\partial x_{i}}dd^{c}\phi_{i}\\ =\sum\frac{\partial^{2}u}{\partial x_{i}\partial x_{j}}d\log r_{i}\wedge d^{c}\log r_{j}+(\sum\frac{\partial u}{\partial x_{i}}d_{i})dd^{c}\phi_{0}.\end{split}

Observe that for rank reasons

(∑∂2u∂xi​∂xj​d​log⁡ri∧dc​log⁡rj)m+1=0,(d​dc​ϕ0)n−m+1=0.(\sum\frac{\partial^{2}u}{\partial x_{i}\partial x_{j}}d\log r_{i}\wedge d^{c}\log r_{j})^{m+1}=0,\quad(dd^{c}\phi_{0})^{n-m+1}=0.

We compute the volume form using binomial expansion

(d​dc​u)n=n!(n−m)!​(∑∂u∂xi​di)n−m​det(D2​u)​(∏1md​log⁡ri∧dc​log⁡ri)∧(d​dc​ϕ0)n−m.(dd^{c}u)^{n}=\frac{n!}{(n-m)!}(\sum\frac{\partial u}{\partial x_{i}}d_{i})^{n-m}\det(D^{2}u)(\prod_{1}^{m}d\log r_{i}\wedge d^{c}\log r_{i})\wedge(dd^{c}\phi_{0})^{n-m}.

Since (d​dc​ϕ0)n−m(dd^{c}\phi_{0})^{n-m} already exhaust all base terms, we can replace log⁡ri\log r_{i} by log⁡|ξi|\log|\xi_{i}|, and obtain

(d​dc​u)n=n!(n−m)!​(∑∂u∂xi​di)n−m​det(D2​u)​(∏1m−14​π​d​log⁡ξi∧d​log⁡ξi¯)∧(d​dc​ϕ0)n−m.(dd^{c}u)^{n}=\frac{n!}{(n-m)!}(\sum\frac{\partial u}{\partial x_{i}}d_{i})^{n-m}\det(D^{2}u)(\prod_{1}^{m}\frac{\sqrt{-1}}{4\pi}d\log\xi_{i}\wedge d\overline{\log\xi_{i}})\wedge(dd^{c}\phi_{0})^{n-m}.

The Calabi-Yau condition on d​dc​ϕ0dd^{c}\phi_{0} and the normalization on ΩY\Omega_{Y} imply

(d​dc​ϕ0)n−m=(∫Yc1​(L0)n−m)​−1(n−m)2​ΩY∧Ω¯Y.(dd^{c}\phi_{0})^{n-m}=(\int_{Y}c_{1}(L_{0})^{n-m})\sqrt{-1}^{(n-m)^{2}}\Omega_{Y}\wedge\overline{\Omega}_{Y}.

The conclusion is that

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Lemma 2.1.

As long as the NA MA equation holds

det(D2​u)​(∑∂u∂xi​di)n−m=const,\det(D^{2}u)(\sum\frac{\partial u}{\partial x_{i}}d_{i})^{n-m}=\text{const},

then the generalized Calabi ansatz d​dc​udd^{c}u is a Calabi-Yau metric, in this case of proportional line bundles.

[0228]
Remark 2.2.

It is understood that uu is strictly convex, and ∑∂u∂xi​di\sum\frac{\partial u}{\partial x_{i}}d_{i} is positive. These two conditions guarantee the metric is positive definite.

[0229]

2.4 Relevance to the Tian-Yau problem

The relevance of the generalized Calabi ansatz to the Tian-Yau problem (cf. Question 2.4) is as follows. Let X¯\bar{X} be a smooth Fano manifold, and D=∑DiD=\sum D_{i} be an anticanonical divisor, which we assume to be simple normal crossing, with only multiplicity one components. Let X=X¯∖DX=\bar{X}\setminus D, then XX has a nowhere vanishing holomorphic volume form Ω\Omega, and one can ask when this admits a complete Calabi-Yau metric.

An important intuition to keep in mind, is that most of the volume growth near the infinity of XX in fact concentrates near the deeper intersection strata DJ=∩i∈JDiD_{J}=\cap_{i\in J}D_{i} of the component divisors DiD_{i}. Let mm denote the maximal |J||J| for which DJD_{J} is non-empty, then from the volume growth perspective, the neighbourhood of the mm-fold intersection loci are the generic regions in the Calabi-Yau XX. For any such subset JJ with |J|=m|J|=m, the neighbourhood of DJD_{J} is essentially the total space of ⊕j∈J𝒪(Dj)|DJ\oplus_{j\in J}\mathcal{O}(D_{j})|_{D_{J}}, which corresponds to ZZ, and an application of the adjunction formula shows DJD_{J} is a compact Calabi-Yau, which corresponds to YY. Up to inessential normalization constants, the holomorphic volume form is (3) up to negligible errors. In many examples all the 𝒪⁡(Di)\mathcal{O}(D_{i}) are ample. The possible relevance of LL comes from the prescribed global Kähler class on XX. The picture we would like to advocate, for which our present paper is a very special case, is that one can find new Tian-Yau type metrics on XX, whose behaviour in the generic region is modelled on the generalized Calabi ansatz. Morever, further details from this paper suggests the whole problem is inductive on mm, in the sense that what happens in non-generic regions is related to the generalized Calabi ansatz with smaller mm.

[022A]

2.5 ODE reduction

While we believe the generalized Calabi ansatz has wide applicability, both in the Tian-Yau problem, and in the collapsing polarized degeneration problem as described in [14], solving the NA MA equation (4) is practically quite nontrivial for m≥2m\geq 2. We shall now specialize to the proportional line bundle case of section 2.3, and further assume m=2m=2. The NA MA equation becomes a PDE with two independent variables

det(D2​u)​(d1​∂u∂x1+d2​∂u∂x2)n−2=const.\det(D^{2}u)(d_{1}\frac{\partial u}{\partial x_{1}}+d_{2}\frac{\partial u}{\partial x_{2}})^{n-2}=\text{const}. (5)

Motivated by the Calabi ansatz, we wish to look for homogeneous solutions. A preliminary dimensional analysis is useful:

u∼O⁡(|x|α),D​u∼O⁡(|x|α−1),D2​u∼O⁡(|x|α−2).u\sim O(|x|^{\alpha}),\quad Du\sim O(|x|^{\alpha-1}),\quad D^{2}u\sim O(|x|^{\alpha-2}).

Thus we want

2​(α−2)+(n−2)​(α−1)=0,α=n+2n.2(\alpha-2)+(n-2)(\alpha-1)=0,\quad\alpha=\frac{n+2}{n}.

We try the ansatz

x2=d2d1​t​x1,u⁡(x1,x2)=x1n+2n​v​(t).x_{2}=\frac{d_{2}}{d_{1}}tx_{1},\quad u(x_{1},x_{2})=x_{1}^{\frac{n+2}{n}}v(t). (6)

Routine computation then reduces the NA MA equation to an ODE:

[022B]
Lemma 2.3.

Under the homogeneous ansatz, the NA MA equation is equivalent to

(v​v′′−2n+2​v′2)​(n+2n​v+(1−t)​v′)n−2=const.(vv^{\prime\prime}-\frac{2}{n+2}v^{\prime 2})(\frac{n+2}{n}v+(1-t)v^{\prime})^{n-2}=\text{const}. (7)
[022C]
Proof.

We compute

∂u∂x1=(n+2n​v−t​v′)​x12/n,∂u∂x2=d1d2​v′​x12/n,\frac{\partial u}{\partial x_{1}}=(\frac{n+2}{n}v-tv^{\prime})x_{1}^{2/n},\quad\frac{\partial u}{\partial x_{2}}=\frac{d_{1}}{d_{2}}v^{\prime}x_{1}^{2/n},

and the second derivatives

{∂2u∂x12=x12/n−1​{2​(n+2)n2​v−4​tn​v′+t2​v′′},∂2u∂x1​∂x2=d1d2​(2n​v′−t​v′′)​x12n−1,∂2u∂x22=(d1d2)2​x12n−1​v′′.\begin{cases}&\frac{\partial^{2}u}{\partial x_{1}^{2}}=x_{1}^{2/n-1}\{\frac{2(n+2)}{n^{2}}v-\frac{4t}{n}v^{\prime}+t^{2}v^{\prime\prime}\},\\ &\frac{\partial^{2}u}{\partial x_{1}\partial x_{2}}=\frac{d_{1}}{d_{2}}(\frac{2}{n}v^{\prime}-tv^{\prime\prime})x_{1}^{\frac{2}{n}-1},\\ &\frac{\partial^{2}u}{\partial x_{2}^{2}}=(\frac{d_{1}}{d_{2}})^{2}x_{1}^{\frac{2}{n}-1}v^{\prime\prime}.\end{cases} (8)

Whence

det(D2​u)=(d1d2)2​x14n−2​(2​(n+2)n2​v​v′′−4n2​v′2),\det(D^{2}u)=(\frac{d_{1}}{d_{2}})^{2}x_{1}^{\frac{4}{n}-2}(\frac{2(n+2)}{n^{2}}vv^{\prime\prime}-\frac{4}{n^{2}}v^{\prime 2}),
d1​∂u∂x1+d2​∂u∂x2=d1​x12/n​(n+2n​v+(1−t)​v′),d_{1}\frac{\partial u}{\partial x_{1}}+d_{2}\frac{\partial u}{\partial x_{2}}=d_{1}x_{1}^{2/n}(\frac{n+2}{n}v+(1-t)v^{\prime}),

so the NA MA equation becomes

(2​(n+2)n2​v​v′′−4n2​v′2)​(n+2n​v+(1−t)​v′)n−2=const.(\frac{2(n+2)}{n^{2}}vv^{\prime\prime}-\frac{4}{n^{2}}v^{\prime 2})(\frac{n+2}{n}v+(1-t)v^{\prime})^{n-2}=\text{const}.

∎

[022D]
Remark 2.4.

The constant is not essential: it just amounts to rescaling the metric.

[022E]
Remark 2.5.

The Kähler condition requires D2​uD^{2}u to be positive definite, and d1​∂u∂x1+d2​∂u∂x2>0d_{1}\frac{\partial u}{\partial x_{1}}+d_{2}\frac{\partial u}{\partial x_{2}}>0. These are equivalent to

v′′>0,(n+2)​v​v′′−2​v′2>0,n+2n​v+(1−t)​v′>0.v^{\prime\prime}>0,\quad(n+2)vv^{\prime\prime}-2v^{\prime 2}>0,\quad\frac{n+2}{n}v+(1-t)v^{\prime}>0.

The first two inequalities imply v>0v>0. These constraints are all quite natural in view of the ODE.

[022F]
Remark 2.6.

The ODE enjoys a symmetry: under the substitution

v⁡(t)=tn+2n​v~​(1/t),v(t)=t^{\frac{n+2}{n}}\tilde{v}(1/t),

we have

(n+2)​v​v′′−2​v′2=t4n−2​((n+2)​v~′′​v~−2​v~′2),(n+2)vv^{\prime\prime}-2v^{\prime 2}=t^{\frac{4}{n}-2}((n+2)\tilde{v}^{\prime\prime}\tilde{v}-2\tilde{v}^{\prime 2}),
n+2n​v+(1−t)​v′=t2/n​{n+2n​v~+(1−t−1)​v~′},\frac{n+2}{n}v+(1-t)v^{\prime}=t^{2/n}\{\frac{n+2}{n}\tilde{v}+(1-t^{-1})\tilde{v}^{\prime}\},

so the function v~\tilde{v} is another solution of the same ODE. The geometric origin of this symmetry is that the NA MA equation is symmetric in x1,x2x_{1},x_{2}, up to the minor issue of d1,d2d_{1},d_{2} which disappears after trivial changes of variables.

[022G]

2.6 Basic length scales of the generic region

We mentioned in the beginning that the generalized Calabi ansatz geometrically describes an iterated fibration, which is supposedly the model for the generic region near infinity on the noncompact Calabi-Yau X=X¯∖DX=\bar{X}\setminus D. Figuring out the order of magnitude of various length scales is essentially a matter of dimensional analysis. In the generic region tt is of order ∼1\sim 1, vv is smooth and of order ∼1\sim 1. Our homogeneous ansatz prescribes

u∼O⁡(|x|(n+2)/n),|d​u|∼O⁡(|x|2/n),|D2​u|∼O⁡(|x|(2−n)/n).u\sim O(|x|^{(n+2)/n}),\quad|du|\sim O(|x|^{2/n}),\quad|D^{2}u|\sim O(|x|^{(2-n)/n}).

We have |D2​u|≪1≪|d​u||D^{2}u|\ll 1\ll|du|. From the descriptions in section 2.1, the Hessian term is responsible for the base and torus direction of the metric, while d​udu is responsible for the effective Kähler class, and therefore the size of the fibres diffeomorphic to Y≃D1∩D2Y\simeq D_{1}\cap D_{2}. Thus

diam​(T2)=O⁡(|D2​u|1/2)=O⁡(|x|(2−n)/2​n),diam​(Y)=O⁡(|d​u|1/2)=O⁡(|x|1/n),\text{diam}(T^{2})=O(|D^{2}u|^{1/2})=O(|x|^{(2-n)/2n}),\quad\text{diam}(Y)=O(|du|^{1/2})=O(|x|^{1/n}),

the distance to the origin is of order

O⁡(∫|D2​u|1/2)=O⁡(|x|(2+n)/2​n),O(\int|D^{2}u|^{1/2})=O(|x|^{(2+n)/2n}),

and the volume within |x|≤r|x|\leq r is O⁡(r2)O(r^{2}) from the two log directions of the base. In terms of geodesic distance to the origin, the volume grows with power 4​n/(n+2)4n/(n+2).

For |x|≫1|x|\gg 1, this reaffirms the intuition that the T2T^{2} length scale is far smaller than Y≃D1∩D2Y\simeq D_{1}\cap D_{2}, which is far smaller than the real 2-dimensional base.

[022H]

2.7 Boundary condition of the ODE

The ODE (7) is posed on 0<t<∞0<t<\infty, and we now discuss the boundary conditions to put at t=0t=0 and t=∞t=\infty. The infinity boundary can be reduced to the t=0t=0 case by the symmetry of the ODE, which geometrically comes from the symmetry between x1,x2x_{1},x_{2} (up to elementary scaling). Geometrically one would like to find a partial completion of the generalized Calabi ansatz, near the infinity of X¯∖D1∪D2\bar{X}\setminus D_{1}\cup D_{2}. The generalized Calabi ansatz works in the neighbourhood of D1∩D2D_{1}\cap D_{2}, and one would like to understand what happens near D1∖D2D_{1}\setminus D_{2} and D2∖D1D_{2}\setminus D_{1}.

The simplest boundary conditions to imagine is for the ODE to remain analytic at t=0t=0. In this case, one would specify v⁡(0)=v0>0v(0)=v_{0}>0 and v′​(0)>−n+2n​v0v^{\prime}(0)>-\frac{n+2}{n}v_{0}, and the ODE is non-singular in a neighbourhood of t=0t=0, so that vv has a Taylor expansion at t=0t=0. Geometrically, the size of T2T^{2} remains of order O⁡(x12−n2​n)O(x_{1}^{\frac{2-n}{2n}}) and the effective Kähler class of YY remains of order O⁡(x12/n)O(x_{1}^{2/n}) as t→0t\to 0. There seems to be no known metric near D1∖D2D_{1}\setminus D_{2} that one may attempt to glue to the generalized Calabi ansatz. Intuitively, one cannot suddenly ‘switch off’ the effective Kähler class at t=0t=0.

We are thus led to look for boundary conditions such that n+2n​v+(1−t)​v′→0\frac{n+2}{n}v+(1-t)v^{\prime}\to 0 as t→0t\to 0, which intuitively means the effective Kähler class ‘switches off gradually’. The following type of boundary conditions is perhaps best motivated by fixing v0>0v_{0}>0, and trying to decrease v′​(0)v^{\prime}(0) until v′​(0)+n+2n​v0v^{\prime}(0)+\frac{n+2}{n}v_{0} tends to zero. As t→0t\to 0, we require v′v^{\prime} has some subleading power law behaviour

{v=v0+O⁡(t),v′=−n+2n​v0+a​tβ+O⁡(t),v′′=a​β​tβ−1+O⁡(1).\begin{cases}&v=v_{0}+O(t),\\ &v^{\prime}=-\frac{n+2}{n}v_{0}+at^{\beta}+O(t),\\ &v^{\prime\prime}=a\beta t^{\beta-1}+O(1).\end{cases} (9)

Here 0<β<10<\beta<1 and a>0a>0 are some constants to be determined. Thus

v​v′′−2n+2​v′2=a​v0​β​tβ−1+O⁡(1),vv^{\prime\prime}-\frac{2}{n+2}v^{\prime 2}=av_{0}\beta t^{\beta-1}+O(1),
n+2n​v+(1−t)​v′=a​tβ+O⁡(t),\frac{n+2}{n}v+(1-t)v^{\prime}=at^{\beta}+O(t),

and the ODE predicts

β−1+(n−2)​β=0,β=1n−1,\beta-1+(n-2)\beta=0,\quad\beta=\frac{1}{n-1},

and

a​v0n−1an−2=const,a∝v0−1/(n−1).\frac{av_{0}}{n-1}a^{n-2}=\text{const},\quad a\propto v_{0}^{-1/(n-1)}.
[022I]

Geometric meaning of the boundary condition

We can translate the boundary condition near t=0t=0 into the asymptotic behaviour of the Calabi-Yau metric for 1≪x2≪x11\ll x_{2}\ll x_{1}. Using the second derivative computation (8), we get

{∂2u∂x12∼2​(n+2)n2​v0​x12n−1,∂2u∂x1​∂x2∼−d1d2​2​(n+2)n2​v0​x12n−1∂2u∂x22∼(d1d2)2​an−1​t−n−2n−1​x12n−1.\begin{cases}\frac{\partial^{2}u}{\partial x_{1}^{2}}\sim\frac{2(n+2)}{n^{2}}v_{0}x_{1}^{\frac{2}{n}-1},\\ \frac{\partial^{2}u}{\partial x_{1}\partial x_{2}}\sim-\frac{d_{1}}{d_{2}}\frac{2(n+2)}{n^{2}}v_{0}x_{1}^{\frac{2}{n}-1}\\ \frac{\partial^{2}u}{\partial x_{2}^{2}}\sim(\frac{d_{1}}{d_{2}})^{2}\frac{a}{n-1}t^{-\frac{n-2}{n-1}}x_{1}^{\frac{2}{n}-1}.\end{cases}

Recall that in the generalized Calabi-Yau ansatz, this Hessian matrix controls the base metric and the torus fibres. In the x1x_{1}-direction of the base (i.e. the direction transverse to D1D_{1} at infinity), and the log⁡ξ1\log\xi_{1} circle direction, the behaviour is similar to what happens in the generic region where tt is of order one. However, in the x2x_{2} direction, the base metric has a different scaling law:

∂2u∂x22∼(d1d2)2​an−1​t−n−2n−1​x12n−1=O⁡(x12n−1n−1​x2−n−2n−1).\frac{\partial^{2}u}{\partial x_{2}^{2}}\sim(\frac{d_{1}}{d_{2}})^{2}\frac{a}{n-1}t^{-\frac{n-2}{n-1}}x_{1}^{\frac{2}{n}-1}=O(x_{1}^{\frac{2}{n}-\frac{1}{n-1}}x_{2}^{-\frac{n-2}{n-1}}).

The distance to x2∼O⁡(1)x_{2}\sim O(1) is O⁡(x11n−12​(n−1)​x2n2​(n−1))O(x_{1}^{\frac{1}{n}-\frac{1}{2(n-1)}}x_{2}^{\frac{n}{2(n-1)}}). The log⁡ξ2\log\xi_{2} circle direction now has diameter of order

O⁡(x2−n−22​(n−1)​x11n−12​(n−1)),O(x_{2}^{-\frac{n-2}{2(n-1)}}x_{1}^{\frac{1}{n}-\frac{1}{2(n-1)}}),

which is much larger compared to the log⁡ξ1\log\xi_{1} circle. In other words, the metric exhibits inhomogeneous collapsing phenomenon.

The potential is roughly

u=x1n+2n​v​(t)≈x1n+2n​(v0−n+2n​v0​t+n−1n​a​tnn−1)≈v0​(x1−d1d2​x2)n+2n+n−1n​a​x1n+2n​(d1d2​x2x1)nn−1.\begin{split}&u=x_{1}^{\frac{n+2}{n}}v(t)\approx x_{1}^{\frac{n+2}{n}}(v_{0}-\frac{n+2}{n}v_{0}t+\frac{n-1}{n}at^{\frac{n}{n-1}})\\ &\approx v_{0}(x_{1}-\frac{d_{1}}{d_{2}}x_{2})^{\frac{n+2}{n}}+\frac{n-1}{n}ax_{1}^{\frac{n+2}{n}}(\frac{d_{1}}{d_{2}}\frac{x_{2}}{x_{1}})^{\frac{n}{n-1}}.\end{split}

Here x2≪x1x_{2}\ll x_{1}. For fixed values of x1−d1d2​x2x_{1}-\frac{d_{1}}{d_{2}}x_{2}, the second term dominates the metric contribution on the slices. Up to scaling factors by powers of x1x_{1}, the key dependence on x2x_{2} is d​dc​x2n/(n−1)dd^{c}x_{2}^{n/(n-1)}, which is the Calabi ansatz on an open subset of the (n−1)(n-1)-dimensional total space of the line bundle 𝒪⁡(D2)→D1∩D2\mathcal{O}(D_{2})\to D_{1}\cap D_{2} (cf. section 2.2). When ξ1\xi_{1} is allowed to vary, the scales of the S1S^{1}, the Calabi ansatz, and the base metric, all depend on x1x_{1} in some power law fashion.

The significance to the compactification question, is that 𝒪⁡(D2)→D1∩D2\mathcal{O}(D_{2})\to D_{1}\cap D_{2} describes the infinity of the non-compact Calabi-Yau manifold D1∖D2D_{1}\setminus D_{2}, and the Calabi ansatz is the asymptote of the Tian-Yau metric on D1∖D2D_{1}\setminus D_{2}. We can thus glue the Calabi ansatz to the Tian-Yau metric, in a parametrized fashion over the x1x_{1} variable, in order to achieve the partial completion of the generalized Calabi ansatz. After this, we would have an approximate Calabi-Yau metric outside a compact set in X=X¯∖D1∪D2X=\bar{X}\setminus D_{1}\cup D_{2}, from which one can hope to use a non-compact version of Yau’s proof to the Calabi conjecture to obtain an actual Calabi-Yau metric on XX.

[022J]
Remark 2.7.

An appealing feature is that the boundary behaviour of the m=2m=2 generalized Calabi ansatz is essentially the ordinary Calabi ansatz. We think this feature may generalize to larger mm, so that the boundaries have an inductive stratification structure.

[022K]

2.8 Remarks on other related literature

The main previously known source of complete Calabi-Yau metrics on the complement of a singular anticanonical divisor are due to Hein [10] on certain complex surfaces. These examples are constructed on rational elliptic surfaces, which in particular admit elliptic fibrations onto ℙ1\mathbb{P}^{1} with fibers lying in the anticanonical linear system. Hein constructs complete Calabi-Yau metrics asymptotic to the semi-flat Calabi-Yau metrics discovered by Greene-Shapere-Vafa-Yau [7]. Interestingly, for Kodaira type IbI_{b} singular fibers, these metrics turn out to be the same as the metrics constructed by Tian-Yau [16] on the complement of an ample anticanonical divisors in a del Pezzo surface [4, 5, 11]. In what follows we collect some sporadic comparisons to other works in the literature which are not directly connected to the Tian-Yau problem.

[022L]

2.8.1 Degenerating hypersurfaces

Sun and Zhang [19] studied the degenerating Calabi-Yau metric on the family of hypersurfaces

Xt={F1F2+tF=0}⊂ℂℙn,0<|t|≪1,X_{t}=\{F_{1}F_{2}+tF=0\}\subset\mathbb{CP}^{n},\quad 0<|t|\ll 1,

where F1,F2F_{1},F_{2} define two transverse degree d1,d2d_{1},d_{2} smooth irreducible hypersurfaces D1,D2D_{1},D_{2}, with d1+d2=n+1d_{1}+d_{2}=n+1, and FF defines a generic hypersurface of degree n+1n+1, so that the F=0F=0 locus in D1∩D2D_{1}\cap D_{2} is smooth and irreducible. A concrete special case, studied previously by [11], is when XtX_{t} is a family of quartic K3 surfaces degenerating into the union of two quadrics.

The Calabi-Yau metric on XtX_{t} is fibred over an interval. The ends of the interval correspond to the two regions D1∖D2D_{1}\setminus D_{2} and D2∖D1D_{2}\setminus D_{1}, and the metrics therein are modelled on the Tian-Yau metrics, whose asymptotes match up with the Calabi ansatz. The transition between the two Calabi ansatzs on the two ends is modelled on an Ooguri-Vafa type metric, obtained by a generalized Gibbons-Hawking type ansatz.

Now algebro-geometrically, our Tian-Yau type space ℂ​ℙn∖D1∪D2\mathbb{CP}^{n}\setminus D_{1}\cup D_{2} can be imagined as the limit of ℂ​ℙn∖Xt\mathbb{CP}^{n}\setminus X_{t} as t→0t\to 0. It is then natural (but somewhat naïve) to imagine taking the usual Tian-Yau metric construction on ℂ​ℙn∖Xt\mathbb{CP}^{n}\setminus X_{t}, and try to extract limits. It is then not surprising that the Tian-Yau metric on D1∖D2D_{1}\setminus D_{2} and D1∖D2D_{1}\setminus D_{2} should appear in the asymptotic description of the metric on ℂ​ℙn∖D1∪D2\mathbb{CP}^{n}\setminus D_{1}\cup D_{2}, even though the precise scaling factors of these Tian-Yau regions do not seem to be predicted by this naïve limit. However, the Ooguri-Vafa type region in [19] has no direct relation to the generalized Calabi ansatz in our construction.

There is a further way our construction is related to a natural generalization of [19]:

Xt={F1F2F3+tF=0}⊂ℂℙn,0<|t|≪1.X_{t}=\{F_{1}F_{2}F_{3}+tF=0\}\subset\mathbb{CP}^{n},\quad 0<|t|\ll 1.

The algebro-geometric limit as t→0t\to 0 is the union of transversely intersecting hypersurfaces D1,D2,D3D_{1},D_{2},D_{3}. One can similarly ask for the description of the Calabi-Yau metric on XtX_{t} for small tt. It is quite conceivable that the metric model in the region D1∖D2∪D3D_{1}\setminus D_{2}\cup D_{3} (and the cyclic permutations) is provided by our construction, although how the transition happens between these three ends is an interesting open problem, which likely involves a further generalization of the Ooguri-Vafa type metric in [19].

As a more general remark, we think the higher mm version of the NA MA equation in this paper is the noncompact analogue of the NA MA equation appearing in the collapsing case of polarized degeneration of Calabi-Yau metrics explained in [14], and we expect the generalized Calabi ansatz to be relevant for local metric models in the polarized degenerations.

[022M]

2.8.2 Exotic metrics on ℂn\mathbb{C}^{n}

There are a number of recent constructions of complete Calabi-Yau metrics on ℂn\mathbb{C}^{n} with n≥3n\geq 3, that share the unifying theme of holomorphic fibrations. The works [12][20][6] start with a holomorphic fibration given by a weighted homogeneous polynomial F:ℂn→ℂF:\mathbb{C}^{n}\to\mathbb{C}, such that F−1​(0)F^{-1}(0) carries a Sasakian-Einstein cone metric. The other fibres carry asymptotically conical Calabi-Yau metrics modelled at infinity on F−1​(0)F^{-1}(0). From this, one builds a Calabi-Yau metric on ℂn\mathbb{C}^{n}, whose fibrewise restrictions are approximated by these Calabi-Yau metrics on the fibres outside of a compact region, and in the horizontal direction is approximated by the pullback of the Euclidean metric on ℂ\mathbb{C}. Such metrics on ℂn\mathbb{C}^{n} have maximal volume growth, and the tangent cone at infinity is F−1​(0)×ℂF^{-1}(0)\times\mathbb{C} with the product metric. From an algebro-geometric perspective, the singularities on F−1​(0)F^{-1}(0) are klt, which should be viewed as mild singularities. The coordinate functions on ℂn\mathbb{C}^{n} all have polynomial growth with respect to the geodesic distance to the origin, even though the growth rates are typically not linear.

[022N]
Remark 2.8.

One moral is that the holomorphic structure alone is very far from specifying the metric. The recent uniqueness result [21] suggests that an additional filtration structure associated with the growth of holomorphic functions is key to the uniqueness and classification of the metrics.

More recently a family of new Taub-NUT type Calabi-Yau metrics were constructed on ℂ3\mathbb{C}^{3} [13], using a generalized Gibbons-Hawking framework. The asymptotic geometry near infinity is generically a T2T^{2}-fibration over ℝ4\mathbb{R}^{4}, but along three rays inside ℝ4\mathbb{R}^{4} the metric looks like a Taub-NUT fibration over a cylinder. These metrics are fundamentally different in that it has volume growth order V​o​l​(B⁡(r))∼O⁡(r4)Vol(B(r))\sim O(r^{4}) coming from the ℝ4\mathbb{R}^{4} direction, which is not maximal volume growth. Algebro-geometrically, these metrics are associated with the holomorphic fibration

F⁡(z1,z2,z3)=z1​z2​z3:ℂ3→ℂ,F(z_{1},z_{2},z_{3})=z_{1}z_{2}z_{3}:\mathbb{C}^{3}\to\mathbb{C},

whose fibres are generically cylinders, contributing two dimensions to T2T^{2} and two other dimensions to ℝ4\mathbb{R}^{4}. The ℂ\mathbb{C} factor contributes the other two dimensions to ℝ4\mathbb{R}^{4}. Notice the singular fibres are reducible, and the nature of the singularity is much worse than klt. In terms of the growth of holomorphic functions, only z1​z2​z3z_{1}z_{2}z_{3} has polynomial growth, while z1,z2,z3z_{1},z_{2},z_{3} individually all have exponential type growth, meaning that log⁡|zk|\log|z_{k}| has polynomial growth.

[022P]
Remark 2.9.

The Taub-NUT metric is a much more classical prototype. Its asymptotic geometry is an S1S^{1}-bundle over ℝ3\mathbb{R}^{3}, with non-maximal volume growth V​o​l​(B⁡(r))=O⁡(r3)Vol(B(r))=O(r^{3}). Algebro-geometrically the Taub-NUT is associated with the fibration ℂ2→z1​z2ℂ\mathbb{C}^{2}\xrightarrow{z_{1}z_{2}}\mathbb{C}, whose fibres are cylinders. The holomorphic function z1​z2z_{1}z_{2} has polynomial growth, while z1,z2z_{1},z_{2} individually have exponential growth.

In view of these constructions, the new feature of this paper is that in the generalized Calabi ansatz, the approximately Calabi-Yau fibres do not appear as fibres of holomorphic fibrations, but rather come from the effective description of an iterated non-holomorphic fibration. The algebraic functions on XX have exponential type growth. The prototype of these phenomena is of course already known in the case of the Calabi ansatz, but we believe the NA MA equation points towards a much larger generality of examples, not limited to ODE reduction methods.

[022Q]
Remark 2.10.

A recent paper of Biquard and Delcroix [2] constructs Calabi-Yau metrics on certain rank 2 complex symmetric spaces using small cohomogeneity methods. A real Monge-Ampère type ODE [2, Prop 2.3] also plays a prominent role, and the relation with our construction seems to deserve some further investigation.

[022R]

2.8.3 Non-archimedean meaning?

As we mentioned before, the generalized Calabi ansatz was discovered in an attempt to interpret the non-archimedean version of the Monge-Ampère equation in the context of polarized degenerations [14]. This relation to non-archimedean geometry remains conjectural, because at least some regularity is needed in order for the NA MA equation to admit a metric interpretation, which is unfortunately still not proven even in some cases where the Calabi-Yau metric is completely understood, such as the case studied in [19]. The reader is thus warned that the following discussions will be rather speculative; they are meant to provide a more general and higher brow perspective to section 2.4, and to motivate directions of future research.

In the polarized degeneration setting, one associates dual complexes to SNC models (or more generally dlt models) of the degeneration family. When the SNC models are related by blow ups with centres supported on the central fibre, then there exist comparison maps between the dual complexes, and the Berkovich space is the inductive limit of these dual complexes. One should think of the Berkovich space as encoding the pure birational geometry of the degeneration family. The polarization provides an extra positive line bundle structure on the Berkovich space, which one should imagine as metric information. One can make sense of the non-archimedean version of plurisubharmonic functions and semipositive metrics, and associate the non-archimedean Monge-Ampère measure. The foundational result of this non-archimedean pluripotential theory is that one can solve the non-archimedean Calabi conjecture on the Berkovich space by a variational method, as is expertly surveyed in [3].

Now in the noncompact setting, the natural analogue of SNC models is SNC pairs (X¯,D)(\bar{X},D) with X=X¯∖DX=\bar{X}\setminus D,11 1 In general X¯\bar{X} needs not be Fano. to which one can associate dual complexes and build up a version of the Berkovich space. To the author’s knowledge, non-archimedean pluripotential theory has not been developed in this noncompact setting, but the key point we would like to suggest is that the non-archimedean Monge-Ampère equation in this conjectural theory, should be equivalent to the differential geometric version (4), and its purpose is to prescribe the asymptotic of the Kähler potential.

The Berkovich space by itself only has the complex geometric information, and by Remark 2.8 we know that this is far from sufficient to specify the metric. Another problem with the non-compact setting, is that the Calabi-Yau volume is infinite. In the concrete setting of this paper, the problem of infinity is essentially solved by imposing the homogeneity ansatz, which reduced the NA MA equation to a boundary value problem with two ends, which is morally a compact problem. Now the geometric meaning of the homogeneity ansatz has to do with the growth order of the algebraic functions with respect to the geodesic distance. This growth information goes beyond pure complex geometry, and knows something about the metric. We would like to suggest it plays a similar role to the positive line bundle in the context of polarized degenerations. Once this is taken into account, one can at least hope for a non-archimedean Calabi conjecture type result in this noncompact setting.

The above picture fits quite well with a heuristic principle of Yau, that complete non-compact Calabi-Yau manifolds should (under mild conditions) admit a natural (quasi-)projective compactifications. When this compactification is projective, one may hope that under an additional specification of the homogeneity ansatz, the non-archimedean geometry produces a version of the NA MA solution, which one can then use to prescribe the asymptotic Kähler potential in the generic region. One then tries to find a completion of the ansatz metric, and hopes that a (highly elaborate) application of the Tian-Yau existence proof would eventually construct a Calabi-Yau metric.

[022S]
Remark 2.11.

Currently it is an art to guess an appropriate homogeneity ansatz (i.e. the growth order of the algebraic functions). Compatibility with the positivity requirements of Kähler geometry makes this a highly delicate issue. Could there be some connections to stability conditions?

This very large pool of potential examples still do not exhaust the full richness of the complete Calabi-Yau metrics. The reason is that in general Yau’s compactification is only a partial compactification into a quasi-projective variety. A typical phenomenon is that there is a holomorphic fibration to a lower dimensional variety, and the partial compactification amounts to the compactification of the fibres. For instance, the Taub-NUT metric on ℂ2\mathbb{C}^{2} can be compactified into the rational surface

{([X0:X1:X2],y)|X1X2=yX02}⊂ℂℙ2×ℂy,\{([X_{0}:X_{1}:X_{2}],y)|X_{1}X_{2}=yX_{0}^{2}\}\subset\mathbb{CP}^{2}\times\mathbb{C}_{y},

where we added in two compactification divisors D1={X0=X1=0}D_{1}=\{X_{0}=X_{1}=0\} and D2={X0=X2=0}D_{2}=\{X_{0}=X_{2}=0\}. These divisors encode the exponential growth of the coordinate functions in the fibre direction, and are responsible for the fact that the fibrewise metric restrictions are approximately cylindrical. A very similar phenomenon happens with the Taub-NUT type metric on ℂ3\mathbb{C}^{3} mentioned above. The upshot is that by mixing the holomorphic fibration with the NA MA ansatz, one can hope to generate an even larger supply of Calabi-Yau metrics.

[022T]

3 More on the ODE reduction

The aim of this section is to study further the ODE reduction (7) from the special case of the NA MA equation. It turns out the ODE can be solved exactly, and the solution is related to the hypergeometric function.

[022U]

3.1 Reformulations of the ODE

[022V]

First reformulation of the ODE

The ODE (7) can be somewhat further simplified:

[022W]
Lemma 3.1.

Under the substitution w=n+2n​vn/(n+2)w=\frac{n+2}{n}v^{n/(n+2)}, the ODE (7) is equivalent to

w′′​(w+(1−t)​w′)n−2=const⋅w−3.w^{\prime\prime}(w+(1-t)w^{\prime})^{n-2}=\text{const}\cdot w^{-3}. (10)
[022X]
Proof.

Observe

(v′v2/(n+2))′=v​v′′−2n+2​v′2v(n+4)/(n+2).\left(\frac{v^{\prime}}{v^{2/(n+2)}}\right)^{\prime}=\frac{vv^{\prime\prime}-\frac{2}{n+2}v^{\prime 2}}{v^{(n+4)/(n+2)}}.

We can rewrite the ODE (7) as

v​v′′−2n+2​v′2v(n+4)/(n+2)(n+2nvn/(n+2)+(1−t)v′v2/(n+2))n−2=const⋅v−3n/(n+2).\frac{vv^{\prime\prime}-\frac{2}{n+2}v^{\prime 2}}{v^{(n+4)/(n+2)}}\left(\frac{n+2}{n}v^{n/(n+2)}+(1-t)\frac{v^{\prime}}{v^{2/(n+2)}}\right)^{n-2}=\text{const}\cdot v^{-3n/(n+2)}.

Now

w=n+2n​vn/(n+2),w′=v′v2/(n+2),w′′=v​v′′−2n+2​v′2v(n+4)/(n+2),w=\frac{n+2}{n}v^{n/(n+2)},\quad w^{\prime}=\frac{v^{\prime}}{v^{2/(n+2)}},\quad w^{\prime\prime}=\frac{vv^{\prime\prime}-\frac{2}{n+2}v^{\prime 2}}{v^{(n+4)/(n+2)}},

so the ODE simplifies to (10) after slightly modifying the constant. ∎

[022Y]
Remark 3.2.

The Kähler condition (cf. Remark 2.5) translates into

w>0,w′′>0,w+(1−t)​w′>0.w>0,\quad w^{\prime\prime}>0,\quad w+(1-t)w^{\prime}>0.
[022Z]
Remark 3.3.

The symmetry of the ODE (cf. Remark 2.6) translates into the following. Let

w⁡(t)=t​w~​(1/t),w(t)=t\tilde{w}(1/t),

then

w′=w~−t−1​w~′,w′′=t−3​w~′′,w^{\prime}=\tilde{w}-t^{-1}\tilde{w}^{\prime},\quad w^{\prime\prime}=t^{-3}\tilde{w}^{\prime\prime},
w+(1−t)​w′=w~+(1−t−1)​w~′,w′′​w3=w~′′​w~3.w+(1-t)w^{\prime}=\tilde{w}+(1-t^{-1})\tilde{w}^{\prime},\quad w^{\prime\prime}w^{3}=\tilde{w}^{\prime\prime}\tilde{w}^{3}.

Thus if ww solves (10), then so does w~\tilde{w}.

In terms of the substitution w=n+2n​vn/(n+2)w=\frac{n+2}{n}v^{n/(n+2)}, the boundary condition at t→0t\to 0 becomes

{w=w0+O(t),w0=n+2nv0n/(n+2),w′=−w0+b1t1/(n−1)+O(t),b1=av0−2/(n+2),w′′=b1n−1t−(n−2)/(n−1)+O(1).\begin{cases}&w=w_{0}+O(t),\quad w_{0}=\frac{n+2}{n}v_{0}^{n/(n+2)},\\ &w^{\prime}=-w_{0}+b_{1}t^{1/(n-1)}+O(t),\quad b_{1}=av_{0}^{-2/(n+2)},\\ &w^{\prime\prime}=\frac{b_{1}}{n-1}t^{-(n-2)/(n-1)}+O(1).\end{cases} (11)

In the normalization of the ODE

w′′​w3​(w+(1−t)​w′)n−2=1n−1,w^{\prime\prime}w^{3}(w+(1-t)w^{\prime})^{n-2}=\frac{1}{n-1}, (12)

we would have

b1n−1​w03=1.b_{1}^{n-1}w_{0}^{3}=1.

Notice w0w_{0} determines b1b_{1}, which means this boundary condition at t=0t=0 comes in a 1-parameter family, instead of the generic 2-parameter family for second order ODEs. The t=+∞t=+\infty end has a closely related boundary condition via the ODE symmetry (cf. Remark 3.3), which also arises in a 1-parameter family, so one expects the global solutions to the ODE to be isolated.

[0230]

Second reformulation of the ODE

We write for 0<t<10<t<1,

s=11−t∈(1,∞),𝔴⁡(s)=w⁡(t)1−t.s=\frac{1}{1-t}\in(1,\infty),\quad\mathfrak{w}(s)=\frac{w(t)}{1-t}. (13)

Then

d​𝔴d​s=(1−t)2​d​𝔴d​t=(1−t)2​dd​t​(w1−t)=(1−t)​w′+w.\frac{d\mathfrak{w}}{ds}=(1-t)^{2}\frac{d\mathfrak{w}}{dt}=(1-t)^{2}\frac{d}{dt}(\frac{w}{1-t})=(1-t)w^{\prime}+w.
d2​𝔴d​s2=(1−t)2​dd​t​((1−t)​w′+w)=(1−t)3​w′′.\frac{d^{2}\mathfrak{w}}{ds^{2}}=(1-t)^{2}\frac{d}{dt}((1-t)w^{\prime}+w)=(1-t)^{3}w^{\prime\prime}.

Thus the ODE (12) can be reformulated as

dd​s​(d​𝔴d​s)n−1=(n−1)​d2​𝔴d​s2​(d​𝔴d​s)n−2=𝔴−3.\frac{d}{ds}(\frac{d\mathfrak{w}}{ds})^{n-1}=(n-1)\frac{d^{2}\mathfrak{w}}{ds^{2}}(\frac{d\mathfrak{w}}{ds})^{n-2}=\mathfrak{w}^{-3}. (14)

The Kähler condition (cf. Remark 3.2) translates into

𝔴>0,d​𝔴d​s>0,d2​𝔴d​s2>0.\mathfrak{w}>0,\quad\frac{d\mathfrak{w}}{ds}>0,\quad\frac{d^{2}\mathfrak{w}}{ds^{2}}>0. (15)

The initial condition at s=1s=1 is

𝔴=w0+O⁡(t),d​𝔴d​s=b1​t1/(n−1)+O⁡(t),t=1−s−1.\mathfrak{w}=w_{0}+O(t),\quad\frac{d\mathfrak{w}}{ds}=b_{1}t^{1/(n-1)}+O(t),\quad t=1-s^{-1}. (16)
[0231]

3.2 First integral of the ODE

[0232]
Lemma 3.4.

If 𝔴\mathfrak{w} solves the ODE (14) with the initial condition (16), then

n−1n​(d​𝔴d​s)n+12​𝔴2=12​w02.\frac{n-1}{n}(\frac{d\mathfrak{w}}{ds})^{n}+\frac{1}{2\mathfrak{w}^{2}}=\frac{1}{2w_{0}^{2}}. (17)
[0233]
Proof.

We differentiate

dd​s​((n−1)n​(d​𝔴d​s)n+12​𝔴2)\displaystyle\frac{d}{ds}\left(\frac{(n-1)}{n}\left(\frac{d\mathfrak{w}}{ds}\right)^{n}+\frac{1}{2\mathfrak{w}^{2}}\right) =(n−1)​(d​𝔴d​s)n−1​(d2​𝔴d​s2)−𝔴−3​d​𝔴d​s\displaystyle=(n-1)\left(\frac{d\mathfrak{w}}{ds}\right)^{n-1}\left(\frac{d^{2}\mathfrak{w}}{ds^{2}}\right)-\mathfrak{w}^{-3}\frac{d\mathfrak{w}}{ds}
=(d​𝔴d​s)​(dd​s​(d​𝔴d​s)n−1−𝔴−3)\displaystyle=\left(\frac{d\mathfrak{w}}{ds}\right)\left(\frac{d}{ds}\left(\frac{d\mathfrak{w}}{ds}\right)^{n-1}-\mathfrak{w}^{-3}\right)
=0\displaystyle=0

Now the result follows by observing that, from the initial conditions we have

((n−1)n​(d​𝔴d​s)n+12​𝔴2)|s=1=12​w02.\left(\frac{(n-1)}{n}\left(\frac{d\mathfrak{w}}{ds}\right)^{n}+\frac{1}{2\mathfrak{w}^{2}}\right)\bigg|_{s=1}=\frac{1}{2w_{0}^{2}}.

∎

This first integral can be solved explicitly. Rewriting the first integral in terms of the rescaled variables 𝔴w0\frac{\mathfrak{w}}{w_{0}} and (2​(n−1)nw0n+2)−1/ns\left(\frac{2(n-1)}{n}w_{0}^{n+2}\right)^{-1/n}s, the ODE simplifies to the form

f′n=1−f−2.f^{\prime n}=1-f^{-2}.

We introduce the function

F(x)=∫1x(1−y−2)−1/ndy,F(x)=\int_{1}^{x}(1-y^{-2})^{-1/n}dy,

then

F(𝔴w0)=(2​(n−1)nw0n+2)−1/n(s−1).F(\frac{\mathfrak{w}}{w_{0}})=\left(\frac{2(n-1)}{n}w_{0}^{n+2}\right)^{-1/n}(s-1). (18)

Inverting FF solves 𝔴\mathfrak{w} as a function of ss. It is clear that

𝔴>0,d​𝔴d​s>0.\mathfrak{w}>0,\quad\frac{d\mathfrak{w}}{ds}>0.

The ODE (14) then implies d2​𝔴d​s2>0\frac{d^{2}\mathfrak{w}}{ds^{2}}>0, namely the Kähler condition is satisfied. We remark that FF can be expressed in terms of the hypergeometric functions, cf. the Appendix.

We then check the initial conditions and the analyticity of the solution near s=1s=1.

[0234]
Corollary 3.5.

The function 𝔴⁡(s)\mathfrak{w}(s) is a power series in (s−1)n/(n−1)(s-1)^{n/(n-1)} near s=1s=1. To leading orders

𝔴=w0+n−1n​w0−3n−1​(s−1)nn−1+O⁡((s−1)2​nn−1).\mathfrak{w}=w_{0}+\frac{n-1}{n}w_{0}^{-\frac{3}{n-1}}(s-1)^{\frac{n}{n-1}}+O((s-1)^{\frac{2n}{n-1}}). (19)
[0235]
Proof.

Notice near y=1y=1, the function

(1−y−2)−1/n=(y−1)−1/n×Taylor series in y−1 with constant term 2−1/n.(1-y^{-2})^{-1/n}=(y-1)^{-1/n}\times\text{Taylor series in $y-1$ with constant term $2^{-1/n}$}.

Upon integration,

F⁡(x)=(x−1)(n−1)/n×Taylor series in x−1 with constant term 2−1/nnn−1.F(x)=(x-1)^{(n-1)/n}\times\text{Taylor series in $x-1$ with constant term $2^{-1/n}\frac{n}{n-1}$}.

Raising (18) to the power n/(n−1)n/(n-1), we see

w0−n+2n−1​(s−1)n/(n−1)=Taylor series in 𝔴w0−1 with first coefficient nn−1.w_{0}^{-\frac{n+2}{n-1}}(s-1)^{n/(n-1)}=\text{Taylor series in $\frac{\mathfrak{w}}{w_{0}}-1$ with first coefficient $\frac{n}{n-1}$}.

Inverting the function, 𝔴w0−1\frac{\mathfrak{w}}{w_{0}}-1 is a power series of (s−1)n/(n−1)(s-1)^{n/(n-1)} near s=1s=1. To leading order,

𝔴w0−1=n−1n​w0−n+2n−1​(s−1)nn−1​(1+O⁡((s−1)n2​n−1)),\frac{\mathfrak{w}}{w_{0}}-1=\frac{n-1}{n}w_{0}^{-\frac{n+2}{n-1}}(s-1)^{\frac{n}{n-1}}\left(1+O((s-1)^{\frac{n}{2n-1}})\right),
d​𝔴d​s≈w0−3n−1​(s−1)1/(n−1)=b1​(s−1)1/(n−1),\frac{d\mathfrak{w}}{ds}\approx w_{0}^{-\frac{3}{n-1}}(s-1)^{1/(n-1)}=b_{1}(s-1)^{1/(n-1)},

which agrees with the initial condition (16). ∎

[0236]

3.3 Global matching problem

We have solved the ODE with the prescribed initial condition, on the interval 0<t<10<t<1. For the application to the generalized Calabi ansatz, we need solutions over 0<t<∞0<t<\infty, and for this purpose the ODE (14) is inadequate. From the ODE (12), it is however a priori clear that t=1t=1 is not a singularity.

[0237]
Lemma 3.6.

For any given w0>0w_{0}>0, the solution to the ODE (12) exists smoothly on 0<t<1+ϵ⁡(w0)0<t<1+\epsilon(w_{0}) for some ϵ⁡(w0)>0\epsilon(w_{0})>0.

[0238]
Proof.

The ODE (12) can be smoothly extended as long as ww remains bounded positively below and (1−t)​w′+w(1-t)w^{\prime}+w remains bounded (which imply boundedness of w′′w^{\prime\prime}, and in particular the boundedness of w,w′w,w^{\prime}). Notice

dd​t​((1−t)​w′+w)=(1−t)​w′′>0,\frac{d}{dt}((1-t)w^{\prime}+w)=(1-t)w^{\prime\prime}>0,

so (1−t)​w′+w(1-t)w^{\prime}+w is monotone increasing, and in particular positive. By

dd​t​((1−t)​w′+w)n−1=1−tw3,\frac{d}{dt}((1-t)w^{\prime}+w)^{n-1}=\frac{1-t}{w^{3}},

we see (1−t)​w′+w(1-t)w^{\prime}+w will be bounded as long as ww is bounded positively below.

The convexity of ww is ensured whenever the solution is smooth. Thus for some small ϵ>0\epsilon>0,

w⁡(t)≥w⁡(ϵ)−w′​(ϵ)​(t−ϵ),t≥ϵ.w(t)\geq w(\epsilon)-w^{\prime}(\epsilon)(t-\epsilon),\quad t\geq\epsilon.

For small ϵ\epsilon, we have w0−w0​ϵ<w⁡(ϵ)<w0w_{0}-w_{0}\epsilon<w(\epsilon)<w_{0} and −w0<w′​(ϵ)<0-w_{0}<w^{\prime}(\epsilon)<0, so w⁡(ϵ)/w′​(ϵ)>1−ϵw(\epsilon)/w^{\prime}(\epsilon)>1-\epsilon, whence w⁡(t)w(t) has an a priori lower bound slightly beyond t=1t=1. ∎

Recall the ODE has a symmetry under t→t−1t\to t^{-1} (cf. Remark 3.3). Our strategy to achieve both the t=0t=0 and the t=∞t=\infty boundary conditions, is to look for symmetric solutions:

w⁡(t)=t​w~​(1/t),w⁡(t)=w~​(t).w(t)=t\tilde{w}(1/t),\quad w(t)=\tilde{w}(t).

This is a functional equation on w⁡(t)w(t), and it amounts to a matching condition at t=1t=1:

w⁡(1)=w~​(1),w′​(1)=w~′​(1).w(1)=\tilde{w}(1),\quad w^{\prime}(1)=\tilde{w}^{\prime}(1).

This is equivalent to

w′​(1)=12​w​(1).w^{\prime}(1)=\frac{1}{2}w(1). (20)

The problem is then to look for w0>0w_{0}>0 to solve (20). The key is to extract w′​(1)w^{\prime}(1) from the asymptote of 𝔴\mathfrak{w} as s→+∞s\to+\infty, namely t→1t\to 1. The starting point is the identity

w′​(t)=s​d​𝔴d​s−𝔴.w^{\prime}(t)=s\frac{d\mathfrak{w}}{ds}-\mathfrak{w}. (21)

which means the value of w′w^{\prime} is related to the Legendre transform of 𝔴\mathfrak{w}.

[0239]

3.4 Legendre transform

The Legendre transform of the convex function 𝔴\mathfrak{w} is given by

𝔴∗​(p)=sups∈[1,∞)s​p−𝔴⁡(s).\mathfrak{w}^{*}(p)=\sup_{s\in[1,\infty)}sp-\mathfrak{w}(s).

In particular, we have

𝔴∗​(p)=s​d​𝔴d​s−𝔴⁡(s) at ​p=d​𝔴d​s\mathfrak{w}^{*}(p)=s\frac{d\mathfrak{w}}{ds}-\mathfrak{w}(s)\qquad\text{ at }p=\frac{d\mathfrak{w}}{ds}

We are now going to rewrite the first integral (17) in terms of 𝔴∗​(p)\mathfrak{w}^{*}(p). First, since lims→∞𝔴⁡(s)=∞\lim_{s\rightarrow\infty}\mathfrak{w}(s)=\infty we see from (17) that

d​𝔴d​s([1,∞))=[0,p∗=(n2​(n−1)​w02)1n)\frac{d\mathfrak{w}}{ds}([1,\infty))=[0,p_{*}=\left(\frac{n}{2(n-1)w_{0}^{2}}\right)^{\frac{1}{n}})

and so the Legendre transform is defined on this interval. Furthermore, since d​𝔴d​s​(s=1)=0\frac{d\mathfrak{w}}{ds}(s=1)=0 we have d​𝔴∗d​p​(p=0)=1\frac{d\mathfrak{w}^{*}}{dp}(p=0)=1, and 𝔴∗​(p=0)=−𝔴⁡(s=1)=−w0\mathfrak{w}^{*}(p=0)=-\mathfrak{w}(s=1)=-w_{0} by the properties of the Legendre transform. Now from the involution property of the Legendre transform,

𝔴⁡(s⁡(p))=s⁡(p)​p−𝔴∗​(p)=d​𝔴∗d​p​p−𝔴∗​(p).\mathfrak{w}(s(p))=s(p)p-\mathfrak{w}^{*}(p)=\frac{d\mathfrak{w}^{*}}{dp}p-\mathfrak{w}^{*}(p).

The first integral (17) is rewritten as

n−1n​pn+12​(d​𝔴∗d​p​p−𝔴∗​(p))−2=12​w02,\frac{n-1}{n}p^{n}+\frac{1}{2}\left(\frac{d\mathfrak{w}^{*}}{dp}p-\mathfrak{w}^{*}(p)\right)^{-2}=\frac{1}{2w_{0}^{2}},

namely

(p​dd​p​𝔴∗−𝔴∗)2​(1w02−2​(n−1)​pnn)=1.(p\frac{d}{dp}\mathfrak{w}^{*}-\mathfrak{w}^{*})^{2}\left(\frac{1}{w_{0}^{2}}-\frac{2(n-1)p^{n}}{n}\right)=1.

To simplify matters we can rescale. Define

y=1p∗​p,g⁡(y)=1w0​𝔴∗.y=\frac{1}{p_{*}}p,\quad g(y)=\frac{1}{w_{0}}\mathfrak{w}^{*}.

Then the ODE is recast on the interval y∈[0,1)y\in[0,1) as

(y​d​gd​y−g⁡(y))2​(1−yn)=1,(y\frac{dg}{dy}-g(y))^{2}(1-y^{n})=1, (22)

subject to the initial conditions

g⁡(0)=−1,g′​(0)=p∗w0=(n2​(n−1)​w02+n)1n.g(0)=-1,\quad g^{\prime}(0)=\frac{p_{*}}{w_{0}}=\left(\frac{n}{2(n-1)w_{0}^{2+n}}\right)^{\frac{1}{n}}.

This can be integrated explicitly:

[023A]
Lemma 3.7.

The function

g(y)=−2F1[12,−1n,n−1n;yn]+p∗w0y,g(y)=-\,_{2}F_{1}[\frac{1}{2},-\frac{1}{n},\frac{n-1}{n};y^{n}]+\frac{p_{*}}{w_{0}}y,

where F12​[a,b,c;z]\,{}_{2}F_{1}[a,b,c;z] is the hypergeometric function (38). In particular,

g⁡(1)=p∗w0−Γ⁡(1−1n)​πΓ⁡(12−1n).g(1)=\frac{p_{*}}{w_{0}}-\frac{\Gamma(1-\frac{1}{n})\sqrt{\pi}}{\Gamma(\frac{1}{2}-\frac{1}{n})}.
[023B]
Proof.

First note that if gg solves the equation, then so does g+c​yg+cy for any constant cc. Thus, we may reduce to the initial condition g⁡(0)=−1,g′​(0)=0g(0)=-1,g^{\prime}(0)=0 below. The initial condition specifies a sign choice of the square root, whence

dd​y​(gy)=1y2​(1−yn)12,\frac{d}{dy}\left(\frac{g}{y}\right)=\frac{1}{y^{2}(1-y^{n})^{\frac{1}{2}}},

and the Lemma is reduced to Prop. 5.3. ∎

We can implement the matching condition w′​(1)=12​w​(1)w^{\prime}(1)=\frac{1}{2}w(1) as follows. From (21) and the definition of the Legendre transform,

w′​(t=1)=𝔴∗​(p∗)=w0​g​(1)=w0​(p∗w0−Γ⁡(1−1n)​πΓ⁡(12−1n)).w^{\prime}(t=1)=\mathfrak{w}^{*}(p_{*})=w_{0}g(1)=w_{0}\left(\frac{p_{*}}{w_{0}}-\frac{\Gamma(1-\frac{1}{n})\sqrt{\pi}}{\Gamma(\frac{1}{2}-\frac{1}{n})}\right).

On the other hand, we have

w⁡(t=1)\displaystyle w(t=1) =lims→∞𝔴⁡(s)s\displaystyle=\lim_{s\rightarrow\infty}\frac{\mathfrak{w}(s)}{s}
=limp→p∗p⁡(d​𝔴∗/d​p)−𝔴∗(d​𝔴∗/d​p)\displaystyle=\lim_{p\rightarrow p_{*}}\frac{p(d\mathfrak{w}^{*}/dp)-\mathfrak{w}^{*}}{(d\mathfrak{w}^{*}/dp)}
=limp→p∗p−𝔴∗(d​𝔴∗/d​p)\displaystyle=\lim_{p\rightarrow p_{*}}p-\frac{\mathfrak{w}^{*}}{(d\mathfrak{w}^{*}/dp)}

but from the first integral we have (d​𝔴∗/d​p)→∞(d\mathfrak{w}^{*}/dp)\rightarrow\infty as p→p∗p\rightarrow p_{*}, while 𝔴∗→𝔴∗​(1)<+∞\mathfrak{w}^{*}\rightarrow\mathfrak{w}^{*}(1)<+\infty. Thus we get

w⁡(1)=p∗=(n2​(n−1)​w02)1/n.w(1)=p_{*}=\left(\frac{n}{2(n-1)w_{0}^{2}}\right)^{1/n}.

All together, the matching amounts to solving the equation

w0​(p∗w0−Γ⁡(1−1n)​πΓ⁡(12−1n))=12​p∗,w_{0}\left(\frac{p_{*}}{w_{0}}-\frac{\Gamma(1-\frac{1}{n})\sqrt{\pi}}{\Gamma(\frac{1}{2}-\frac{1}{n})}\right)=\frac{1}{2}p_{*},

Or equivalently

12​(n2​(n−1)​w02)1/n=w0​Γ⁡(1−1n)​πΓ⁡(12−1n)\frac{1}{2}\left(\frac{n}{2(n-1)w_{0}^{2}}\right)^{1/n}=w_{0}\frac{\Gamma(1-\frac{1}{n})\sqrt{\pi}}{\Gamma(\frac{1}{2}-\frac{1}{n})}

which yields

w0=(12)n+1n+2​(n(n−1))1n+2​(1π​Γ⁡(12−1n)Γ⁡(1−1n))nn+2\displaystyle w_{0}=\left(\frac{1}{2}\right)^{\frac{n+1}{n+2}}\left(\frac{n}{(n-1)}\right)^{\frac{1}{n+2}}\left(\frac{1}{\sqrt{\pi}}\frac{\Gamma(\frac{1}{2}-\frac{1}{n})}{\Gamma(1-\frac{1}{n})}\right)^{\frac{n}{n+2}} (23)

which tends to 12\frac{1}{2} as n→+∞n\rightarrow+\infty. For our purpose the important fact is that w0>0w_{0}>0 for n≥3n\geq 3, which means we have found the initial condition that ensures matching.

[023C]
Remark 3.8.

If n=2n=2, then g⁡(1)=p∗w0g(1)=\frac{p_{*}}{w_{0}}, so w′​(t=1)=p∗w^{\prime}(t=1)=p_{*}, and w⁡(t=1)=p∗w(t=1)=p_{*}. The matching condition has no positive solution. Correspondingly, our generalization of the Calabi ansatz only yield nontrivial examples in dimension at least three.

[023D]

4 Asymptotic ansatz and initial error

The goal of this section is to produce a metric ansatz, and the main technical part is to estimate its deviation from being Calabi-Yau in weighted Hölder spaces. Our setting is a special case of section 2.4. Let n≥3n\geq 3, and X¯\bar{X} be a Fano manifold of dimension nn. The anticanonical bundle is (d1+d2)​L0(d_{1}+d_{2})L_{0} for some positive line bundle L0L_{0} over X¯\bar{X}, and let D1,D2D_{1},D_{2} be smooth divisors in the linear system d1​L0d_{1}L_{0} and d2​L0d_{2}L_{0} respectively, such that the intersection Y=D1∩D2Y=D_{1}\cap D_{2} is transverse. Lefschetz hyperplane theorem then implies that D1∩D2D_{1}\cap D_{2} is smooth and irreducible (notice irreducibility would fail in dimension two, which is excluded in our construction). By adjunction, YY is a compact Calabi-Yau manifold, and the noncompact manifold X=X¯∖D1∪D2X=\bar{X}\setminus D_{1}\cup D_{2} carries a natural nowhere vanishing holomorphic volume form.

[023E]

4.1 Generic region near infinity

We start from the solution w⁡(t)w(t) of the ODE (12) with the matching condition w′​(1)=12​w​(1)w^{\prime}(1)=\frac{1}{2}w(1), which guarantees the existence of the solution for 0<t<+∞0<t<+\infty. As discussed in section 3, this specifies the parameter choices in (11)

w0=(12)n+1n+2​(n(n−1))1n+2​(1π​Γ⁡(12−1n)Γ⁡(1−1n))nn+2,b1=w0−3n−1.w_{0}=\left(\frac{1}{2}\right)^{\frac{n+1}{n+2}}\left(\frac{n}{(n-1)}\right)^{\frac{1}{n+2}}\left(\frac{1}{\sqrt{\pi}}\frac{\Gamma(\frac{1}{2}-\frac{1}{n})}{\Gamma(1-\frac{1}{n})}\right)^{\frac{n}{n+2}},\quad b_{1}=w_{0}^{-\frac{3}{n-1}}.

The boundary behaviour near t→0t\to 0 is prescribed by (11). The t→+∞t\to+\infty boundary is determined from w⁡(t)=t​w​(1/t)w(t)=tw(1/t). Since the geometry of the t→+∞t\to+\infty limit is essentially identical to t→0t\to 0, we will later only focus on t→0t\to 0.

Reversing the previous ODE reductions, let

v⁡(t)=(n​wn+2)n+2n,u⁡(x1,x2)=x1n+2n​v​(t),t=d1​x2d2​x1.v(t)=(\frac{nw}{n+2})^{\frac{n+2}{n}},\quad u(x_{1},x_{2})=x_{1}^{\frac{n+2}{n}}v(t),\quad t=\frac{d_{1}x_{2}}{d_{2}x_{1}}.

Then after restoring a few unpleasant constants

(v​v′′−2n+2​v′2)​(n+2n​v+(1−t)​v′)n−2=1n−1​(nn+2)3,(vv^{\prime\prime}-\frac{2}{n+2}v^{\prime 2})(\frac{n+2}{n}v+(1-t)v^{\prime})^{n-2}=\frac{1}{n-1}(\frac{n}{n+2})^{3},
det(D2​u)​(d1​∂u∂x1+d2​∂u∂x2)n−2=2​n(n+2)2​(n−1)​(d1d2)2​d1n−2.\det(D^{2}u)(d_{1}\frac{\partial u}{\partial x_{1}}+d_{2}\frac{\partial u}{\partial x_{2}})^{n-2}=\frac{2n}{(n+2)^{2}(n-1)}(\frac{d_{1}}{d_{2}})^{2}d_{1}^{n-2}.

In the asymptotic formula (9) for vv at t→0t\to 0, we can recover the constants

v0=(n​w0n+2)n+2n,a=b1​v02n+2=(nn+2)2/n​w0−n+2n⁡(n−1).v_{0}=(\frac{nw_{0}}{n+2})^{\frac{n+2}{n}},\quad a=b_{1}v_{0}^{\frac{2}{n+2}}=(\frac{n}{n+2})^{2/n}w_{0}^{-\frac{n+2}{n(n-1)}}. (24)

Let S1∈H0​(X¯,d1​L0)S_{1}\in H^{0}(\bar{X},d_{1}L_{0}) (resp. S2∈H0​(X¯,d2​L0)S_{2}\in H^{0}(\bar{X},d_{2}L_{0})) be the defining section of D1⊂X¯D_{1}\subset\bar{X} (resp. D2D_{2}). Recall hL0h_{L_{0}} is the Hermitian metric on the line bundle L0L_{0} over YY, whose curvature form is the Calabi-Yau metric on YY in the class c1​(L0)c_{1}(L_{0}). We extend hL0h_{L_{0}} smoothly over X¯\bar{X}. This induces Hermitian metrics on d1​L0d_{1}L_{0} and d2​L0d_{2}L_{0}, and in particular we can make sense of xi=−log⁡|Si|.x_{i}=-\log|S_{i}|. A technical subtlety is that S1,S2S_{1},S_{2} have the ambiguity of a multiplicative constant, which corresponds to the ambiguity of additive constants on x1,x2x_{1},x_{2} of order O⁡(1)O(1), to be fixed in section 4.3. Very large x1,x2x_{1},x_{2} corresponds to the generic region near infinity on the noncompact manifold XX. The function u⁡(x1,x2)u(x_{1},x_{2}) can be regarded as a Kähler potential on the tubular neighbourhood of YY (with YY deleted). Up to exponentially small error in the x1,x2x_{1},x_{2} variables, the Kähler metric is modelled on the generalized Calabi ansatz.

The normal bundle of Y=D1∩D2⊂X¯Y=D_{1}\cap D_{2}\subset\bar{X} is 𝒪⁡(D1)⊕𝒪⁡(D2)|Y=d1​L0⊕d2​L0|Y\mathcal{O}(D_{1})\oplus\mathcal{O}(D_{2})|_{Y}=d_{1}L_{0}\oplus d_{2}L_{0}|_{Y}. Using an auxiliary smooth Hermitian metric on X¯\bar{X}, we can identify this normal bundle with a tubular neighbourhood of Y⊂X¯Y\subset\bar{X} (eg. via normal geodesic flow). The choices of the identifications only produce errors which are exponentially small in the logarithmic variables, which will be negligible since the distance scales of the ansatz metric have power law dependence on the log variables (cf. section 2.6).

Setting up the Hölder norms require a little care, since the injectivity radius of the T2T^{2}-fibres tends to zero in the generic region near infinity. However, for 1≪x2≤x11\ll x_{2}\leq x_{1} (the case of 1≪x1≤x21\ll x_{1}\leq x_{2} being entirely similar), the harmonic radius grows like O⁡(x11/n​t12​(n−1))=O⁡(x11n−12​(n−1)​x212​(n−1))O(x_{1}^{1/n}t^{\frac{1}{2(n-1)}})=O(x_{1}^{\frac{1}{n}-\frac{1}{2(n-1)}}x_{2}^{\frac{1}{2(n-1)}}). This motivates the weighting function

ρ={(|x1|+1)n−22​n​(n−1)​(|x2|+1)12​(n−1),x2≤x1,(|x2|+1)n−22​n​(n−1)​(|x1|+1)12​(n−1),x1≤x2.\rho=\begin{cases}(|x_{1}|+1)^{\frac{n-2}{2n(n-1)}}(|x_{2}|+1)^{\frac{1}{2(n-1)}},\quad x_{2}\leq x_{1},\\ (|x_{2}|+1)^{\frac{n-2}{2n(n-1)}}(|x_{1}|+1)^{\frac{1}{2(n-1)}},\quad x_{1}\leq x_{2}.\end{cases} (25)

We shall only use ρ\rho up to a uniform equivalence constant; no derivative control on ρ\rho is required. Each YY-fibre is covered by O⁡(1)O(1) number of charts each of length scale O⁡(ρ)O(\rho), such that the T2T^{2}-bundle is trivialized over the charts. Given a tensor field TT on an O⁡(ρ)O(\rho) neighbourhood inside XX, we can pass to the local universal cover of the charts by unwrapping the T2T^{2} factors. The local Hölder seminorm is

[T]α:=supd​i​s​t​(P,Q)≲ρρα​|T⁡(P)−T⁡(Q)||P−Q|α,[T]_{\alpha}:=\sup_{dist(P,Q)\lesssim\rho}\rho^{\alpha}\frac{|T(P)-T(Q)|}{|P-Q|^{\alpha}}, (26)

using geodesic parallel transport with respect to the generalized Calabi ansatz metric on the local universal cover of the charts. The local Ck,αC^{k,\alpha} norm is

‖T‖k,α,l​o​c:=∑j=0ksupd​i​s​t​(P,Q)≲ρρj​|∇jT|+ρk​[∇kT]α.\left\lVert T\right\rVert_{k,\alpha,loc}:=\sum_{j=0}^{k}\sup_{dist(P,Q)\lesssim\rho}\rho^{j}|\nabla^{j}T|+\rho^{k}[\nabla^{k}T]_{\alpha}. (27)

There is up to constant multiple a natural holomorphic volume form Ω\Omega on X=X¯∖D1∪D2X=\bar{X}\setminus D_{1}\cup D_{2}. We take the normalization such that near Y⊂X¯Y\subset\bar{X} (cf. (3) for the model case)

Ω=(1+fΩ)​∏12d​log⁡ξi∧ΩY,\Omega=(1+f_{\Omega})\prod_{1}^{2}d\log\xi_{i}\wedge\Omega_{Y},

where ξ1,ξ2\xi_{1},\xi_{2} are local defining functions of the smooth divisors D1,D2D_{1},D_{2}, and fΩf_{\Omega} is a local holomorphic function near YY, of order O⁡(|ξ1|+|ξ2|)O(|\xi_{1}|+|\xi_{2}|), which is exponentially small in the x1,x2x_{1},x_{2} variables. Higher order derivatives of fΩf_{\Omega} are also exponentially small by holomorphicity.

We write

(d​dc​u)n=K0​(1+E​r​r1)​−1n2​Ω∧Ω¯,(dd^{c}u)^{n}=K_{0}(1+Err_{1})\sqrt{-1}^{n^{2}}\Omega\wedge\overline{\Omega}, (28)

where E​r​r1Err_{1} is some error function, and K0K_{0} is the (unfortunately complicated) proportionality constant in the model case of generalized Calabi ansatz

K0=∫Yc1​(L0)n−2(4​π)2​2​n2(n+2)2​(d1d2)2​d1n−2.K_{0}=\frac{\int_{Y}c_{1}(L_{0})^{n-2}}{(4\pi)^{2}}\frac{2n^{2}}{(n+2)^{2}}(\frac{d_{1}}{d_{2}})^{2}d_{1}^{n-2}.

Recall that Lemma 2.1 says the model case is exactly Calabi-Yau.

[023F]
Lemma 4.1.

(Volume form error) In the generic region min⁡(x1,x2)≫1\min(x_{1},x_{2})\gg 1, we have exponential decay on the local Ck,αC^{k,\alpha} norm of the error function: ‖E​r​r1‖k,α,l​o​c=O⁡(e−c​min⁡(x1,x2))\left\lVert Err_{1}\right\rVert_{k,\alpha,loc}=O(e^{-c\min(x_{1},x_{2})}) for some c>0c>0.

[023G]

4.2 Asymptotic expansion near D1D_{1}

We now translate the ODE asymptote at t→0t\to 0 to the geometry of the region 1≪x2≪x11\ll x_{2}\ll x_{1}. The analyticity of the ODE solution (cf. Cor. 3.5) gives a fractional power series expansion (19), which converts via (13) to

w⁡(t)=(1−t)​{w0+n−1n​w0−3n−1​(t1−t)nn−1+O⁡((t1−t)2​nn−1)}.w(t)=(1-t)\{w_{0}+\frac{n-1}{n}w_{0}^{-\frac{3}{n-1}}(\frac{t}{1-t})^{\frac{n}{n-1}}+O((\frac{t}{1-t})^{\frac{2n}{n-1}})\}.

Now

w=n+2n​vn/(n+2),v0=(n​w0n+2)n+2n,a=(nn+2)2/n​w0−n+2n⁡(n−1),w=\frac{n+2}{n}v^{n/(n+2)},\quad v_{0}=(\frac{nw_{0}}{n+2})^{\frac{n+2}{n}},\quad a=(\frac{n}{n+2})^{2/n}w_{0}^{-\frac{n+2}{n(n-1)}},

hence we have a fractional power series

v⁡(t)=(1−t)n+2n​{v0+n−1n​a​(t1−t)nn−1+∑k=2∞ak​(t1−t)k​nn−1}.\begin{split}v(t)=(1-t)^{\frac{n+2}{n}}\{v_{0}+\frac{n-1}{n}a(\frac{t}{1-t})^{\frac{n}{n-1}}+\sum_{k=2}^{\infty}a_{k}(\frac{t}{1-t})^{\frac{kn}{n-1}}\}.\end{split}

Recall

x2=t​d2d1​x1,u=x1n+2n​v​(t).x_{2}=\frac{td_{2}}{d_{1}}x_{1},\quad u=x_{1}^{\frac{n+2}{n}}v(t).

We introduce the new variable

x~1:=x1−d1d2​x2=(1−t)​x1=d1d2​1−tt​x2.\tilde{x}_{1}:=x_{1}-\frac{d_{1}}{d_{2}}x_{2}=(1-t)x_{1}=\frac{d_{1}}{d_{2}}\frac{1-t}{t}x_{2}.

In terms of the defining sections Si∈H0​(X¯,di​L0)S_{i}\in H^{0}(\bar{X},d_{i}L_{0}) for D1,D2D_{1},D_{2}, we have

x~1=−log⁡|S1|+d1d2​log⁡|S2|=1d2​log⁡|S1⊗d1/S1⊗d2|,\tilde{x}_{1}=-\log|S_{1}|+\frac{d_{1}}{d_{2}}\log|S_{2}|=\frac{1}{d_{2}}\log|S_{1}^{\otimes d_{1}}/S_{1}^{\otimes d_{2}}|,

where

ξ′:=S2⊗d1/S1⊗d2\xi^{\prime}:=S_{2}^{\otimes d_{1}}/S_{1}^{\otimes d_{2}}

is actually a holomorphic function, which means its magnitude does not involve the choice of a Hermitian metric. The geometric significance of this function is that although the normal bundle 𝒪⁡(D1)=d1​L0\mathcal{O}(D_{1})=d_{1}L_{0} of D1⊂X¯D_{1}\subset\bar{X} is nontrivial, it restricts to a line bundle on D1∖D2D_{1}\setminus D_{2} which becomes trivial after taking finite power.

We then have an expansion for 1≪x2≪x11\ll x_{2}\ll x_{1},

u=v0​x~1n+2n+n−1n​a​x~1n+2n−nn−1​(d1​x2d2)nn−1+∑k≥2ak​x~1n+2n−k​nn−1​(d1​x2d2)k​nn−1.u=v_{0}\tilde{x}_{1}^{\frac{n+2}{n}}+\frac{n-1}{n}a\tilde{x}_{1}^{\frac{n+2}{n}-\frac{n}{n-1}}(\frac{d_{1}x_{2}}{d_{2}})^{\frac{n}{n-1}}+\sum_{k\geq 2}a_{k}\tilde{x}_{1}^{\frac{n+2}{n}-\frac{kn}{n-1}}(\frac{d_{1}x_{2}}{d_{2}})^{\frac{kn}{n-1}}. (29)
[023H]

4.3 More background on the Tian-Yau metric

We recall some details of the Tian-Yau metric (cf. [11, section 3] for more expositions).

In our setup, D1D_{1} is a Fano manifold in its own right with anticanonical bundle d2​L0|D1d_{2}L_{0}|_{D_{1}}, and Y=D2∩D1Y=D_{2}\cap D_{1} is an anticanonical divisor defined by some section S∈H0​(D1,d2​L0)S\in H^{0}(D_{1},d_{2}L_{0}), which in our context is the restriction of S2∈H0​(X¯,d2​L0)S_{2}\in H^{0}(\bar{X},d_{2}L_{0}) to D1D_{1}. Up to a multiplicative constant S−1S^{-1} can be viewed as a holomorphic volume form ΩD1\Omega_{D_{1}} on D1∖D2D_{1}\setminus D_{2} with a simple pole along YY, which we normalize to have residue ΩY\Omega_{Y} along YY. In local coordinates,

ΩD1≈d​log⁡ξ2∧ΩY,\Omega_{D_{1}}\approx d\log\xi_{2}\wedge\Omega_{Y},

where ξ2\xi_{2} is a local defining function of D2∩D1⊂D1D_{2}\cap D_{1}\subset D_{1}. Recall hL0⊗d2h_{L_{0}}^{\otimes d_{2}} is the Hermitian metric on L0|YL_{0}|_{Y} whose curvature form is the Calabi-Yau metric on YY in the class d2​c1​(L0)d_{2}c_{1}(L_{0}). We extend hL0h_{L_{0}} to a smooth, positively curved metric on D1D_{1}, so that

ωC​a​l′=n−1n​d​dc​(−log⁡|S|)nn−1\omega_{Cal^{\prime}}=\frac{n-1}{n}dd^{c}(-\log|S|)^{\frac{n}{n-1}}

defines a Kähler form on a neighbourhood of infinity in D1∖D2D_{1}\setminus D_{2}. Up to an approximately holomorphic diffeomorphism, the metric ωC​a​l′\omega_{Cal^{\prime}} on (D1∖D2)(D_{1}\setminus D_{2}) outside a compact set, agrees with the Calabi ansatz on the total space of the line bundle L0→YL_{0}\to Y, up to exponentially small errors. The slightly unusual exponent nn−1\frac{n}{n-1} is because dimY=n−2\dim Y=n-2. Asymptotically, the distance to a fixed basepoint in D1∖D2D_{1}\setminus D_{2} is uniformly equivalent to rD1∼(−log⁡|S|)n2​(n−1).r_{D_{1}}\sim(-\log|S|)^{\frac{n}{2(n-1)}}. We can arrange ωC​a​l′\omega_{Cal^{\prime}} to extend to an exact global Kähler metric on D1∖D2D_{1}\setminus D_{2}, agreeing with the previous formula outside a compact set, still denoted ωC​a​l′\omega_{Cal^{\prime}}.

A technical subtlety is that SS is only defined up to a multiplicative constant, and correspondingly log⁡|S|\log|S| has an additive constant ambiguity, which is fixed by the integral normalization condition

∫D1∖D2(ωC​a​l′n−1−d2n−2​∫Yc1​(L0)n−24​π​−1(n−1)2​ΩD1∧Ω¯D1)=0.\int_{D_{1}\setminus D_{2}}\left(\omega_{Cal^{\prime}}^{n-1}-\frac{d_{2}^{n-2}\int_{Y}c_{1}(L_{0})^{n-2}}{4\pi}\sqrt{-1}^{(n-1)^{2}}\Omega_{D_{1}}\wedge\overline{\Omega}_{D_{1}}\right)=0. (30)

This makes sense because the integrand has exponential decay near infinity, and morever Stokes theorem on large compact sets shows that the integral only depends on the asymptotic information of ωc​a​l′\omega_{cal^{\prime}} near infinity. The preferred normalization of log⁡|S|\log|S| resolves the additive ambiguity of x2=−log⁡|S2|x_{2}=-\log|S_{2}|; a completely analogous normalization on the Tian-Yau space D2∖D1D_{2}\setminus D_{1} fixes the additive ambiguity of x1=−log⁡|S1|x_{1}=-\log|S_{1}|.

The main existence theorem and asymptotic information of the Tian-Yau metric is summarized as follows:

[023I]
Theorem 4.2.

[16][10, Prop. 2.9] There is a complete Ricci-flat Kähler metric

ωT​Y=d​dc​ϕT​Y=ωC​a​l′+d​dc​ϕT​Y,r​e​l\omega_{TY}=dd^{c}\phi_{TY}=\omega_{Cal^{\prime}}+dd^{c}\phi_{TY,rel}

solving the complex Monge-Ampère equation

ωT​Yn−1=d2n−2​∫Yc1​(L0)n−24​π​−1(n−1)2​ΩD1∧Ω¯D1,\omega_{TY}^{n-1}=\frac{d_{2}^{n-2}\int_{Y}c_{1}(L_{0})^{n-2}}{4\pi}\sqrt{-1}^{(n-1)^{2}}\Omega_{D_{1}}\wedge\overline{\Omega}_{D_{1}},

with exponential decay estimate for some constant c>0c>0 depending on D1,D2D_{1},D_{2}:

|∇ωC​a​l′kϕT​Y,r​e​l|ωC​a​l′=O⁡(e−c​rD1n−1n),rD1→+∞,k≥0.|\nabla_{\omega_{Cal^{\prime}}}^{k}\phi_{TY,rel}|_{\omega_{Cal^{\prime}}}=O(e^{-cr_{D_{1}}^{\frac{n-1}{n}}}),\quad r_{D_{1}}\to+\infty,\quad k\geq 0.

The volume growth rate of geodesic balls on the Tian-Yau space is Vol​(B⁡(rD1))∼rD12​(n−1)n\text{Vol}(B(r_{D_{1}}))\sim r_{D_{1}}^{\frac{2(n-1)}{n}}, which is less than quadratic. As such, solving the Poisson equation with potential decaying at infinity would require an integral normalization on the forcing term, which is related to (30) as the Poisson equation is the linearization of the complex Monge-Ampère equation.

[023J]
Proposition 4.3.

Let ff be a smooth function on the Tian-Yau space satisfying the integral normalization ∫f​ωT​Yn−1=0\int f\omega_{TY}^{n-1}=0 and the fast decay

|∇T​Ykf|=O⁡(e−c​rD1n−1n),∀k≥0,|\nabla_{TY}^{k}f|=O(e^{-cr_{D_{1}}^{\frac{n-1}{n}}}),\quad\forall k\geq 0,

then there is a smooth function uu with ΔT​Y​U=f\Delta_{TY}U=f with fast decay

|∇T​YkU|=O⁡(e−c​rD1n−1n),∀k≥0,|\nabla_{TY}^{k}U|=O(e^{-cr_{D_{1}}^{\frac{n-1}{n}}}),\quad\forall k\geq 0,

where the decay rate c>0c>0 may be shrinked.

[023K]
Remark 4.4.

The existence of solution with L∞L^{\infty} bound and L2L^{2}-gradient bound follows from [9, Thm 1.5]. The exponential type decay estimate is because the Tian-Yau space is CYL​(1n)\text{CYL}(\frac{1}{n}) in the sense of Hein [10, Def. 2.5], and the proof of [10, Prop. 2.9] works almost verbatim for the Poisson equation.

To solve the Poisson equation without the integral normalization condition on the forcing term, we need to allow solutions growing at infinity. Consider the special function (−log⁡|S|)1n−1(-\log|S|)^{\frac{1}{n-1}} defined near infinity, which we extend smoothly to a global function u0u_{0} on the Tian-Yau space D1∖D2D_{1}\setminus D_{2}.

[023L]
Lemma 4.5.

The function f0=Δ​u0f_{0}=\Delta u_{0} satisfies the fast decay near infinity

|∇T​Ykf0|=O⁡(e−c​rD1n−1n)|\nabla_{TY}^{k}f_{0}|=O(e^{-cr_{D_{1}}^{\frac{n-1}{n}}})

and the total integral

12​π​(n−1)​∫D1∖D2f0​ωT​Yn−1=∫D1∖D2d​dc​u0∧ωT​Yn−2=d2n−2n−1​∫Yc1​(L0)n−2≠0.\frac{1}{2\pi(n-1)}\int_{D_{1}\setminus D_{2}}f_{0}\omega_{TY}^{n-1}=\int_{D_{1}\setminus D_{2}}dd^{c}u_{0}\wedge\omega_{TY}^{n-2}=\frac{d_{2}^{n-2}}{n-1}\int_{Y}c_{1}(L_{0})^{n-2}\neq 0.
[023M]
Proof.

The exponential type decay is because the deviation between the Tian-Yau metric and the Calabi ansatz is exponentially small, and on the Calabi ansatz model (−log⁡|S|)1n−1(-\log|S|)^{\frac{1}{n-1}} is precisely harmonic. This is the intimately connected to the freedom to add a constant to −log⁡|S|-\log|S| in the Calabi ansatz, without affecting the complex Monge-Ampère measure.

To evaluate ∫f0​ωT​Yn−1\int f_{0}\omega_{TY}^{n-1}, we take a very large compact set K={log|S|≤R}K=\{\log|S|\leq R\}, and consider the R→∞R\to\infty limit. We have up to exponentially suppressed errors

∫Kd​dc​u0∧ωT​Yn−2=∫∂Kdc​u0∧ωT​Yn−2≈∫∂Kdc​u0∧ωC​a​l′n−2.\int_{K}dd^{c}u_{0}\wedge\omega_{TY}^{n-2}=\int_{\partial K}d^{c}u_{0}\wedge\omega_{TY}^{n-2}\approx\int_{\partial K}d^{c}u_{0}\wedge\omega_{Cal^{\prime}}^{n-2}.

Computing in the Calabi ansatz model, this is

−1n−1∫∂Kdclog|S|∧(ddc(−log|S|))n−2-\frac{1}{n-1}\int_{\partial K}d^{c}\log|S|\wedge(dd^{c}(-\log|S|))^{n-2}

which is

1n−1​∫Y(d​dc​(−log⁡|S|))n−2=1n−1​∫Y(d2​c1​(L0))n−2=d2n−2n−1​∫Yc1​(L0)n−2.\frac{1}{n-1}\int_{Y}(dd^{c}(-\log|S|))^{n-2}=\frac{1}{n-1}\int_{Y}(d_{2}c_{1}(L_{0}))^{n-2}=\frac{d_{2}^{n-2}}{n-1}\int_{Y}c_{1}(L_{0})^{n-2}.

Taking the R→+∞R\to+\infty gives the total integral. ∎

[023N]
Corollary 4.6.

Let ff be a smooth function on the Tian-Yau space satisfying the fast decay

|∇T​Ykf|=O⁡(e−c​rD1n−1n),∀k≥0,|\nabla_{TY}^{k}f|=O(e^{-cr_{D_{1}}^{\frac{n-1}{n}}}),\quad\forall k\geq 0,

then there is a smooth function UU with ΔT​Y​U=f\Delta_{TY}U=f in the form

U=const⋅u0+U~,|∇T​YkU|=O⁡(e−c​rD1n−1n),∀k≥0,U=\text{const}\cdot u_{0}+\tilde{U},\quad|\nabla_{TY}^{k}U|=O(e^{-cr_{D_{1}}^{\frac{n-1}{n}}}),\quad\forall k\geq 0,

for some possibly shrinked c>0c>0.

[023P]

4.4 Non-generic region near infinity

Next, we need to move up one dimension, and produce some ansatz metric on X=X¯∖D1∪D2X=\bar{X}\setminus D_{1}\cup D_{2} in the region near infinity close to D1∖D2D_{1}\setminus D_{2}, corresponding in the logarithmic coordinate to x1≫|x2|+1x_{1}\gg|x_{2}|+1, including in particular the region with x2=O⁡(1),x1≫1x_{2}=O(1),x_{1}\gg 1. Pick an auxiliary smooth Hermitian metric on X¯\bar{X}, such that the normal vector field to D1⊂X¯D_{1}\subset\bar{X} is tangent to D2D_{2} along Y=D1∩D2Y=D_{1}\cap D_{2}. Then normal geodesic flow identifies a tubular neighbourhood of D1D_{1} with the normal bundle of D1D_{1}, and the error caused by the failure of holomorphicity is exponentially suppressed in the log coordinates. We can thus regard the potential ϕT​Y\phi_{TY} of the Tian-Yau metric on D1∖D2D_{1}\setminus D_{2} as a function on its tubular neighbourhood, via pullback.

To match with the asymptote (29) in the region 1≪x2≪x11\ll x_{2}\ll x_{1}, we are motivated to consider the local ansatz potential near D1∖D2D_{1}\setminus D_{2}

ϕD1=v0​x~1n+2n+a​(d1d2)nn−1​x~1n−2n⁡(n−1)​ϕT​Y+∑k≥2ak​x~1n+2n−k​nn−1​(d1​x2d2)k​nn−1.\phi_{D_{1}}=v_{0}\tilde{x}_{1}^{\frac{n+2}{n}}+a(\frac{d_{1}}{d_{2}})^{\frac{n}{n-1}}\tilde{x}_{1}^{\frac{n-2}{n(n-1)}}\phi_{TY}+\sum_{k\geq 2}a_{k}\tilde{x}_{1}^{\frac{n+2}{n}-\frac{kn}{n-1}}(\frac{d_{1}x_{2}}{d_{2}})^{\frac{kn}{n-1}}. (31)

Here we make a fixed choice of a positive valued smooth function on the Tian-Yau space matching with x2x_{2} outside a compact set, still denoted as x2x_{2}, so that when x2=O⁡(1)x_{2}=O(1) the expression ϕD1\phi_{D_{1}} remains smooth. The convergence of the series is valid for x2≪x1x_{2}\ll x_{1}. Of course, the ad hoc choice means that the ansatz needs to be corrected later by more refined terms.

The local geometry should be imagined as a fibration of Tian-Yau metrics with slowly changing size depending on the logarithmic variable x1x_{1}. Consider x~1\tilde{x}_{1} around a given large value x1′≫1x_{1}^{\prime}\gg 1. The dominant terms in d​dc​ϕD1dd^{c}\phi_{D_{1}} are

ωx1′=a​(d1d2)n/(n−1)​x1′n−2n⁡(n−1)​d​dc​ϕT​Y+2​(n+2)​v0n2​d22​x1′−n−2n​−14​π​d​log⁡ξ′∧d​log⁡ξ′¯.\omega_{x_{1}^{\prime}}=a(\frac{d_{1}}{d_{2}})^{n/(n-1)}x_{1}^{\prime\frac{n-2}{n(n-1)}}dd^{c}\phi_{TY}+\frac{2(n+2)v_{0}}{n^{2}d_{2}^{2}}x_{1}^{\prime-\frac{n-2}{n}}\frac{\sqrt{-1}}{4\pi}d\log\xi^{\prime}\wedge d\overline{\log\xi^{\prime}}. (32)

Up to taking a finite cover (to do with taking fractional powers of ξ′\xi^{\prime}), this model metric describes the product of the Tian-Yau metric with length scale O⁡(ρ)O(\rho) corresponding to the harmonic radius scale, and a cylinder of circle length scale O⁡(x1′2−n2​n)O(x_{1}^{\prime\frac{2-n}{2n}}) corresponding to the injectivity scale.

We can now set up the local Hölder norms in the nongeneric region x2≪x1x_{2}\ll x_{1} (The case of x1≪x2x_{1}\ll x_{2} is completely similar). When x2=O⁡(1),x1≫1x_{2}=O(1),x_{1}\gg 1, we unwind the S1S^{1} factor of the cylinder to pass to the local universal cover. On O⁡(ρ)O(\rho) neighbourhoods, we can use the local product metric (32) to define the local Hölder seminorm and the Ck,αC^{k,\alpha}-norms, as in (26)(27).

The case of 1≪x2≪x11\ll x_{2}\ll x_{1} is already covered by section 4.1. If we had used the local product metric (32) as reference metric, it would lead to an equivalent definition of local Hölder norms up to uniform equivalence. Notice that within O⁡(ρ)O(\rho) neighbourhoods the values of x1,x2x_{1},x_{2} do not vary drastically, so expressions like O⁡(x1α​x2β)O(x_{1}^{\alpha}x_{2}^{\beta}) are not sensitive to the choice of points in the O⁡(ρ)O(\rho) neighbourhood, except when x2=O⁡(1)x_{2}=O(1), in which case we use a slightly abusive convention that O⁡(x2β)O(x_{2}^{\beta}) stands for O⁡(1)O(1) in this region.

We start by observing the derivative bounds of basic functions, which can be read off using the leading order metric ansatz, remembering that the Tian-Yau metric is well approximated by the Calabi ansatz except when x2=O⁡(1)x_{2}=O(1), and that the x1′x_{1}^{\prime}-dependence in ωx1′\omega_{x_{1}^{\prime}} introduces scaling factors.

[023Q]
Lemma 4.7.

In the region {x2≤x1,and ​x1≫1}\{x_{2}\leq x_{1},\text{and }x_{1}\gg 1\},

‖d​x1‖k,α,l​o​c=O⁡(x1n−22​n),‖d​x2‖k,α,l​o​c=O⁡(x1−n−22​n​(n−1)​x2n−22​(n−1)),\left\lVert dx_{1}\right\rVert_{k,\alpha,loc}=O(x_{1}^{\frac{n-2}{2n}}),\quad\left\lVert dx_{2}\right\rVert_{k,\alpha,loc}=O(x_{1}^{-\frac{n-2}{2n(n-1)}}x_{2}^{\frac{n-2}{2(n-1)}}),
d​dc​(x1−d1d2​x2)=0,‖d​dc​x2‖k,α,l​o​c=O⁡(x2−1n−1​x1−n−2n⁡(n−1)).dd^{c}(x_{1}-\frac{d_{1}}{d_{2}}x_{2})=0,\quad\left\lVert dd^{c}x_{2}\right\rVert_{k,\alpha,loc}=O(x_{2}^{-\frac{1}{n-1}}x_{1}^{-\frac{n-2}{n(n-1)}}).
[023R]
Lemma 4.8.

For x2≪x1x_{2}\ll x_{1}, the Tian-Yau potential satisfies the bound

|ϕT​Y|=O⁡(x2n(n−1)),|d​ϕT​Y|=O⁡(x1−n−22​n​(n−1)​x2n2​(n−1)),|\phi_{TY}|=O(x_{2}^{\frac{n}{(n-1)}}),\quad|d\phi_{TY}|=O(x_{1}^{-\frac{n-2}{2n(n-1)}}x_{2}^{\frac{n}{2(n-1)}}),
‖d​dc​ϕT​Y‖k,α,l​o​c=O⁡(x1−n−2n⁡(n−1)).\left\lVert dd^{c}\phi_{TY}\right\rVert_{k,\alpha,loc}=O(x_{1}^{-\frac{n-2}{n(n-1)}}).

The following lemma quantifies the approximation of the local ansatz potential ϕD1\phi_{D_{1}} by the model product metric:

[023S]
Lemma 4.9.

(Metric deviation) For x1′≫1x_{1}^{\prime}\gg 1, then in the region with |x1−x1′|≤x1′n−22​(n−1)|x_{1}-x_{1}^{\prime}|\leq x_{1}^{\prime\frac{n-2}{2(n-1)}} and |x2|≪x1′|x_{2}|\ll x_{1}^{\prime}, the metric deviation between d​dc​ϕD1dd^{c}\phi_{D_{1}} and the local product metric (32) satisfies the local Ck,αC^{k,\alpha} estimate on O⁡(ρ)O(\rho) neighbourhoods around a given point:

‖d​dc​ϕD1−ωx1′‖k,α,l​o​c=O⁡((x2x1)n2​(n−1))\left\lVert dd^{c}\phi_{D_{1}}-\omega_{x_{1}^{\prime}}\right\rVert_{k,\alpha,loc}=O((\frac{x_{2}}{x_{1}})^{\frac{n}{2(n-1)}})
[023T]
Proof.

We will ignore all exponentially small errors coming from identifying tubular neighbourhoods with normal bundles. We compute d​dc​ϕD1dd^{c}\phi_{D_{1}} by the Leibniz rule:

d​dc​x~1n+2n=2​(n+2)n2​x~1n+2n−2​−14​π​d22​d​log⁡ξ′∧d​log⁡ξ′¯,dd^{c}\tilde{x}_{1}^{\frac{n+2}{n}}=\frac{2(n+2)}{n^{2}}\tilde{x}_{1}^{\frac{n+2}{n}-2}\frac{\sqrt{-1}}{4\pi d_{2}^{2}}d\log\xi^{\prime}\wedge d\overline{\log\xi^{\prime}},
d​dc​(x~1n−2n⁡(n−1)​ϕT​Y)=n−2n⁡(n−1)​(n−2n⁡(n−1)−1)​x~1n−2n⁡(n−1)−2​ϕT​Y​−14​π​d22​d​log⁡ξ′∧d​log⁡ξ′¯+n−2n⁡(n−1)​x~1n−2n⁡(n−1)−1​(d​x~1∧dc​ϕT​Y+d​ϕT​Y∧dc​x~1)+x~1n−2n⁡(n−1)​d​dc​ϕT​Y.\begin{split}&dd^{c}(\tilde{x}_{1}^{\frac{n-2}{n(n-1)}}\phi_{TY})=\frac{n-2}{n(n-1)}(\frac{n-2}{n(n-1)}-1)\tilde{x}_{1}^{\frac{n-2}{n(n-1)}-2}\phi_{TY}\frac{\sqrt{-1}}{4\pi d_{2}^{2}}d\log\xi^{\prime}\wedge d\overline{\log\xi^{\prime}}\\ &+\frac{n-2}{n(n-1)}\tilde{x}_{1}^{\frac{n-2}{n(n-1)}-1}(d\tilde{x}_{1}\wedge d^{c}\phi_{TY}+d\phi_{TY}\wedge d^{c}\tilde{x}_{1})+\tilde{x}_{1}^{\frac{n-2}{n(n-1)}}dd^{c}\phi_{TY}.\end{split}

and similarly with d​dc​(x~1n+2n−k​nn−1​x2k​nn−1)dd^{c}(\tilde{x}_{1}^{\frac{n+2}{n}-\frac{kn}{n-1}}x_{2}^{\frac{kn}{n-1}}).

Comparing v0​d​dc​x~1n+2nv_{0}dd^{c}\tilde{x}_{1}^{\frac{n+2}{n}} and the term 2​(n+2)​v0n2​d22​x1′−n−2n​−14​π​d​log⁡ξ′∧d​log⁡ξ′¯\frac{2(n+2)v_{0}}{n^{2}d_{2}^{2}}x_{1}^{\prime-\frac{n-2}{n}}\frac{\sqrt{-1}}{4\pi}d\log\xi^{\prime}\wedge d\overline{\log\xi^{\prime}}, the deviation is of order O⁡(|x2|+|x1−x1′|x1′)O(\frac{|x_{2}|+|x_{1}-x_{1}^{\prime}|}{x_{1}^{\prime}}). Notice for n≥3n\geq 3, we have n2​(n−1)<1\frac{n}{2(n-1)}<1 and so |x2|x1′≤(x2x1)n2​(n−1)\frac{|x_{2}|}{x_{1}^{\prime}}\leq\left(\frac{x_{2}}{x_{1}}\right)^{\frac{n}{2(n-1)}}. For |x1−x1′|≤x1′n−22​(n−1)|x_{1}-x_{1}^{\prime}|\leq x_{1}^{\prime\frac{n-2}{2(n-1)}}, the error O⁡(|x1−x1′|x1′)=O⁡(x1−n2​(n−1))O(\frac{|x_{1}-x_{1}^{\prime}|}{x_{1}^{\prime}})=O(x_{1}^{-\frac{n}{2(n-1)}}), which is absorbed into O⁡((x2x1)n2​(n−1))O((\frac{x_{2}}{x_{1}})^{\frac{n}{2(n-1)}}).

Using the lemmas, we can estimate the terms appearing in d​dc​(x~1n−2n⁡(n−1)​ϕT​Y)dd^{c}(\tilde{x}_{1}^{\frac{n-2}{n(n-1)}}\phi_{TY}) in the local Ck,αC^{k,\alpha}-norms:

‖ϕT​Y​x1n−2n⁡(n−1)−2​d​log⁡ξ′∧d​log⁡ξ′¯‖k,α,l​o​c=O⁡(x2n(n−1)​x1n−2n⁡(n−1)−2​x1n−2n)=O⁡((x2x1)nn−1).\left\lVert\phi_{TY}x_{1}^{\frac{n-2}{n(n-1)}-2}d\log\xi^{\prime}\wedge d\overline{\log\xi^{\prime}}\right\rVert_{k,\alpha,loc}=O(x_{2}^{\frac{n}{(n-1)}}x_{1}^{\frac{n-2}{n(n-1)}-2}x_{1}^{\frac{n-2}{n}})=O((\frac{x_{2}}{x_{1}})^{\frac{n}{n-1}}).

The cross terms have order

‖x1n−2n⁡(n−1)−1​d​log⁡ξ′∧dc​ϕT​Y‖k,α,l​o​c=O⁡(x1n−2n⁡(n−1)−1​x1n−22​n​x1−n−22​n​(n−1)​x2n2​(n−1))=O⁡((x2x1)n2​(n−1)).\left\lVert x_{1}^{\frac{n-2}{n(n-1)}-1}d\log\xi^{\prime}\wedge d^{c}\phi_{TY}\right\rVert_{k,\alpha,loc}=O(x_{1}^{\frac{n-2}{n(n-1)}-1}x_{1}^{\frac{n-2}{2n}}x_{1}^{-\frac{n-2}{2n(n-1)}}x_{2}^{\frac{n}{2(n-1)}})=O((\frac{x_{2}}{x_{1}})^{\frac{n}{2(n-1)}}).

So does its complex conjugate. The last error comes from the deviation between x~1n−2n⁡(n−1)​d​dc​ϕT​Y\tilde{x}_{1}^{\frac{n-2}{n(n-1)}}dd^{c}\phi_{TY} from x1′n−2n⁡(n−1)​d​dc​ϕT​Yx_{1}^{\prime\frac{n-2}{n(n-1)}}dd^{c}\phi_{TY}. This error is again of order O⁡(|x2|+|x1−x1′|x1′)O(\frac{|x_{2}|+|x_{1}-x_{1}^{\prime}|}{x_{1}^{\prime}}).

The remainder terms have leading order contribution d​dc​(x~1n+2n−2​nn−1​x22​nn−1).dd^{c}(\tilde{x}_{1}^{\frac{n+2}{n}-\frac{2n}{n-1}}x_{2}^{\frac{2n}{n-1}}). Its main contribution is x~1n+2n−2​nn−1​d​dc​x22​nn−1\tilde{x}_{1}^{\frac{n+2}{n}-\frac{2n}{n-1}}dd^{c}x_{2}^{\frac{2n}{n-1}}, which has magnitude O⁡((x2x1)nn−1)O((\frac{x_{2}}{x_{1}})^{\frac{n}{n-1}}). Combining all the errors, the deviation between d​dc​ϕD1dd^{c}\phi_{D_{1}} and the local product metric (32) has magnitude bounded by O⁡((x2x1)n2​(n−1)).O((\frac{x_{2}}{x_{1}})^{\frac{n}{2(n-1)}}). ∎

[023U]
Lemma 4.10.

(Volume form error) In the region with x1≫1x_{1}\gg 1 and x2≪x1x_{2}\ll x_{1},

‖(d​dc​ϕD1)n−K0​−1n2​Ω∧Ω¯‖k,α,l​o​c=O⁡(x1−n(n−1)​e−c​x21/2).\left\lVert(dd^{c}\phi_{D_{1}})^{n}-K_{0}\sqrt{-1}^{n^{2}}\Omega\wedge\overline{\Omega}\right\rVert_{k,\alpha,loc}=O(x_{1}^{-\frac{n}{(n-1)}}e^{-cx_{2}^{1/2}}).
[023V]
Proof.

The volume form error will be smaller than the metric deviation due to extra cancellation effects. Recall the computation of d​dc​ϕD1dd^{c}\phi_{D_{1}} from Lemma 4.9 above. Notice (d​dc​ϕD1)n(dd^{c}\phi_{D_{1}})^{n} is a volume form, so must take one d​log⁡ξ′d\log\xi^{\prime} and d​log⁡ξ′¯d\overline{\log\xi^{\prime}} from either a pair of cross derivative terms, or from a factor d​dc​x~1n+2n−k​nn−1dd^{c}\tilde{x}_{1}^{\frac{n+2}{n}-\frac{kn}{n-1}} for k≥0k\geq 0. The differentiation of ϕT​Y\phi_{TY} and the powers of x2x_{2} would only produce factors on D1∖D2D_{1}\setminus D_{2} without x~1\tilde{x}_{1} dependence. By thinking about all the possible ways to take wedge products contributing to (d​dc​ϕD1)n(dd^{c}\phi_{D_{1}})^{n}, we get an absolutely convergent series within x2≪x1x_{2}\ll x_{1}:

(d​dc​ϕD1)n≈∑k≥0x~1−k​nn−1​−1​d​log⁡ξ′∧d​log⁡ξ′¯∧ℐk,(dd^{c}\phi_{D_{1}})^{n}\approx\sum_{k\geq 0}\tilde{x}_{1}^{-\frac{kn}{n-1}}\sqrt{-1}d\log\xi^{\prime}\wedge d\overline{\log\xi^{\prime}}\wedge\mathcal{I}_{k}, (33)

where the coefficients ℐk\mathcal{I}_{k} are top degree forms on the D1∖D2D_{1}\setminus D_{2} factor, without x~1\tilde{x}_{1} dependence. Here we write ≈\approx as a reminder that we have ignored the exponentially small errors from identifying the tubular neighbourhood with the normal bundles of D1∖D2D_{1}\setminus D_{2}, which is holomorphically trivial up to finite cover.

We now identify the leading term d​log⁡ξ′∧d​log⁡ξ′¯∧ℐ0d\log\xi^{\prime}\wedge d\overline{\log\xi^{\prime}}\wedge\mathcal{I}_{0}. By thinking about form types, this comes from the binomial expansion term

n​v0​d​dc​x~1n+2n∧(a​(d1d2)nn−1​x~1n−2n⁡(n−1)​d​dc​ϕT​Y)n−1,nv_{0}dd^{c}\tilde{x}_{1}^{\frac{n+2}{n}}\wedge\left(a(\frac{d_{1}}{d_{2}})^{\frac{n}{n-1}}\tilde{x}_{1}^{\frac{n-2}{n(n-1)}}dd^{c}\phi_{TY}\right)^{n-1},

which is

2​(n+2)​v0n​d22​−14​π​d​log⁡ξ′∧d​log⁡ξ′¯∧an−1​(d1d2)n​(d​dc​ϕT​Y)n−1.\frac{2(n+2)v_{0}}{nd_{2}^{2}}\frac{\sqrt{-1}}{4\pi}d\log\xi^{\prime}\wedge d\overline{\log\xi^{\prime}}\wedge a^{n-1}(\frac{d_{1}}{d_{2}})^{n}(dd^{c}\phi_{TY})^{n-1}.

From the explicit formula (24) for v0,av_{0},a,

v0​an−1=(nn+2)3,v_{0}a^{n-1}=(\frac{n}{n+2})^{3},

and recalling the complex Monge-Ampère equation for the Tian-Yau metric in Theorem 4.2, the above simplifies to

2​n2​∫Yc1​(L0)n−2(n+2)2​d22​(d1d2)n​d2n−2​−14​π​d​log⁡ξ′∧d​log⁡ξ′¯∧−1(n−1)2​ΩD1∧Ω¯D1.\frac{2n^{2}\int_{Y}c_{1}(L_{0})^{n-2}}{(n+2)^{2}d_{2}^{2}}(\frac{d_{1}}{d_{2}})^{n}d_{2}^{n-2}\frac{\sqrt{-1}}{4\pi}d\log\xi^{\prime}\wedge d\overline{\log\xi^{\prime}}\wedge\sqrt{-1}^{(n-1)^{2}}\Omega_{D_{1}}\wedge\overline{\Omega}_{D_{1}}.

Up to exponentially small errors from complex structure identifications, in terms of the local defining functions ξ1,ξ2\xi_{1},\xi_{2} for D1,D2D_{1},D_{2},

ΩD1≈d​log​ξ2∧ΩY,log⁡ξ′≈d2​log​ξ1−d1​log​ξ2,Ω≈d​log​ξ1∧d​log​ξ2∧ΩY,\Omega_{D_{1}}\approx d\log\xi_{2}\wedge\Omega_{Y},\quad\log\xi^{\prime}\approx d_{2}\log\xi_{1}-d_{1}\log\xi_{2},\quad\Omega\approx d\log\xi_{1}\wedge d\log\xi_{2}\wedge\Omega_{Y},

and the above reduce to K0​−1n2​Ω∧Ω¯,K_{0}\sqrt{-1}^{n^{2}}\Omega\wedge\overline{\Omega}, for the constant K0K_{0} in (28). In short, the leading term cancels with K0​−1n2​Ω∧Ω¯K_{0}\sqrt{-1}^{n^{2}}\Omega\wedge\overline{\Omega}.

The subleading terms are suppressed by the factor x~1−nn−1\tilde{x}_{1}^{-\frac{n}{n-1}}, and the fast convergence of the power series means we only need to consider ℐ1\mathcal{I}_{1}. In the Tian-Yau core region x2=O⁡(1)x_{2}=O(1), the crude information is that d​log⁡ξ′∧d​log⁡ξ′¯∧ℐ1d\log\xi^{\prime}\wedge d\overline{\log\xi^{\prime}}\wedge\mathcal{I}_{1} has local Ck,αC^{k,\alpha} norm O⁡(1)O(1). This explains the O⁡(x1−nn−1)O(x_{1}^{-\frac{n}{n-1}}) decay in the x2=O⁡(1)x_{2}=O(1) subregion.

For 1≪x2≪x11\ll x_{2}\ll x_{1}, the deviation between the Tian-Yau potential ϕT​Y\phi_{TY} and the Calabi ansatz potential is O⁡(e−c​x21/2)O(e^{-cx_{2}^{1/2}}), namely O⁡(e−c​rD1n−1n)O(e^{-cr_{D_{1}}^{\frac{n-1}{n}}}) (for some changing constant c>0c>0). After replacing ϕT​Y\phi_{TY} by n−1n​x2nn−1\frac{n-1}{n}x_{2}^{\frac{n}{n-1}}, we recover the potential uu in the generic region. Ignoring exponentially small complex structure errors as usual, then uu is by construction a solution to the complex Monge-Ampère equation. This explains the exponential decay ℐk=O⁡(e−c​x21/2)\mathcal{I}_{k}=O(e^{-cx_{2}^{1/2}}) for k≥1k\geq 1. ∎

[023W]

4.5 Refined local ansatz in the non-generic region

Recall the distance to the origin is O⁡(|x|n+22​n)O(|x|^{\frac{n+2}{2n}}). Thus the O⁡(x1−nn−1)O(x_{1}^{-\frac{n}{n-1}}) decay is slower than quadratic, and we need further correction terms to improve the ansatz. The linearization of the complex Monge-Ampère equation will naturally lead to a Poisson equation.

Using section 4.3, we can solve (a rescaled version of) the Poisson equation on the Tian-Yau space D1∖D2D_{1}\setminus D_{2}:

(n+2)​(n−1)2​π​n​d22​v0​an−2​(d1d2)n⁡(n−2)n−1​(d​dc​U)∧ωT​Yn−2=−ℐ1,\frac{(n+2)(n-1)}{2\pi nd_{2}^{2}}v_{0}a^{n-2}(\frac{d_{1}}{d_{2}})^{\frac{n(n-2)}{n-1}}(dd^{c}U)\wedge\omega_{TY}^{n-2}=-\mathcal{I}_{1}, (34)

where we recall from (33) that ℐ1\mathcal{I}_{1} is a top degree form on D1∖D2D_{1}\setminus D_{2}, with exponential decay O⁡(e−c​x21/2)O(e^{-cx_{2}^{1/2}}) for some c>0c>0 to all orders of derivatives. The caveat is that ∫D1∖D2ℐ1\int_{D_{1}\setminus D_{2}}\mathcal{I}_{1} is not guaranteed to be zero, so UU may not decay at infinity. Instead,

U=a′​u0+U~,U=a^{\prime}u_{0}+\tilde{U},

where |∇T​YkU~|=O⁡(e−c​x21/2)|\nabla^{k}_{TY}\tilde{U}|=O(e^{-cx_{2}^{1/2}}) for some possibly shrinked c>0c>0, and a′a^{\prime} is a constant.

We regard UU as a function in the region x2≪x1x_{2}\ll x_{1}, namely the tubular neighbourhood around D1∖D2D_{1}\setminus D_{2}, and let ϕD1(2)=ϕD1+x~1n+2n−2​nn−1​U\phi_{D_{1}}^{(2)}=\phi_{D_{1}}+\tilde{x}_{1}^{\frac{n+2}{n}-\frac{2n}{n-1}}U. From the leading term u0∼x21n−1u_{0}\sim x_{2}^{\frac{1}{n-1}} in UU, we can compute using Lemma 4.7 that the correction term x~1n+2n−2​nn−1​U\tilde{x}_{1}^{\frac{n+2}{n}-\frac{2n}{n-1}}U has local Ck,αC^{k,\alpha}-norm O⁡(x1−nn−1​x2−1)O(x_{1}^{-\frac{n}{n-1}}x_{2}^{-1}). This small correction term leads to better volume form decay:

[023X]
Lemma 4.11.

In the region |x2|+1≪x1|x_{2}|+1\ll x_{1}, we have the improved decay

‖(d​dc​ϕD1(2))n−K0​−1n2​Ω∧Ω¯‖k,α,l​o​c=O⁡(x1−2​nn−1​x21n−1).\left\lVert(dd^{c}\phi_{D_{1}}^{(2)})^{n}-K_{0}\sqrt{-1}^{n^{2}}\Omega\wedge\overline{\Omega}\right\rVert_{k,\alpha,loc}=O(x_{1}^{-\frac{2n}{n-1}}x_{2}^{\frac{1}{n-1}}).
[023Y]
Proof.

We revisit the calculations in Lemma 4.10. The volume form (d​dc​ϕD1(2))n(dd^{c}\phi_{D_{1}}^{(2)})^{n} should be viewed as a perturbation of (d​dc​ϕD1)n(dd^{c}\phi_{D_{1}})^{n}. Again (d​dc​ϕD1(2))n(dd^{c}\phi_{D_{1}}^{(2)})^{n} is a convergent power series of x~1−nn−1\tilde{x}_{1}^{-\frac{n}{n-1}}, with coefficient in top degree forms on D1∖D2D_{1}\setminus D_{2}. The leading order contribution to (d​dc​ϕD1(2))n−(d​dc​ϕD1)n(dd^{c}\phi_{D_{1}}^{(2)})^{n}-(dd^{c}\phi_{D_{1}})^{n} is

n⁡(n−1)​v0​d​dc​x~1n+2n∧(a​(d1d2)nn−1​x~1n−2n⁡(n−1)​d​dc​ϕT​Y)n−2∧x~1n+2n−2​nn−1​d​dc​U,n(n-1)v_{0}dd^{c}\tilde{x}_{1}^{\frac{n+2}{n}}\wedge(a(\frac{d_{1}}{d_{2}})^{\frac{n}{n-1}}\tilde{x}_{1}^{\frac{n-2}{n(n-1)}}dd^{c}\phi_{TY})^{n-2}\wedge\tilde{x}_{1}^{\frac{n+2}{n}-\frac{2n}{n-1}}dd^{c}U,

which after some calculation gives

2​(n+2)​(n−1)n​d22​v0​an−2​(d1d2)n⁡(n−2)n−1​(d​dc​U)∧ωT​Yn−2∧x~1−nn−1​−14​π​d​log⁡ξ′∧d​log⁡ξ′¯.\frac{2(n+2)(n-1)}{nd_{2}^{2}}v_{0}a^{n-2}(\frac{d_{1}}{d_{2}})^{\frac{n(n-2)}{n-1}}(dd^{c}U)\wedge\omega_{TY}^{n-2}\wedge\tilde{x}_{1}^{-\frac{n}{n-1}}\frac{\sqrt{-1}}{4\pi}d\log\xi^{\prime}\wedge d\overline{\log\xi^{\prime}}.

This is by construction −−1​d​log⁡ξ′∧d​log⁡ξ′¯∧ℐ1,-\sqrt{-1}d\log\xi^{\prime}\wedge d\overline{\log\xi^{\prime}}\wedge\mathcal{I}_{1}, which is precisely designed to cancel the leading order error −1​d​log⁡ξ′∧d​log⁡ξ′¯∧ℐ1\sqrt{-1}d\log\xi^{\prime}\wedge d\overline{\log\xi^{\prime}}\wedge\mathcal{I}_{1} in (33).

The next order of error has x~1−2​nn−1\tilde{x}_{1}^{-\frac{2n}{n-1}} in front. Within the x2=O⁡(1)x_{2}=O(1) region, the volume error is now O⁡(x~1−2​nn−1)O(\tilde{x}_{1}^{-\frac{2n}{n-1}}). For x2≫1x_{2}\gg 1 one needs to be careful about the effect of UU having a growing term a′​u0a^{\prime}u_{0}, which will damage the exponential decay. Recall from section 4.3 that u0=x21n−1u_{0}=x_{2}^{\frac{1}{n-1}} outside some compact region in the Tian-Yau space. The largest new contributions to the volume forms error come from terms such as

(x~1n−2n⁡(n−1)​d​dc​ϕT​Y)n−2∧dc​x~1n−2n⁡(n−1)∧d​ϕT​Y∧d​x~1n+2n−2​nn−1∧dc​u0,(\tilde{x}_{1}^{\frac{n-2}{n(n-1)}}dd^{c}\phi_{TY})^{n-2}\wedge d^{c}\tilde{x}_{1}^{\frac{n-2}{n(n-1)}}\wedge d\phi_{TY}\wedge d\tilde{x}_{1}^{\frac{n+2}{n}-\frac{2n}{n-1}}\wedge d^{c}u_{0},

whose local Ck,αC^{k,\alpha}-norm is O⁡(x~1−2​nn−1​x21n−1)O(\tilde{x}_{1}^{-\frac{2n}{n-1}}x_{2}^{\frac{1}{n-1}}). ∎

[023Z]

4.6 Gluing the regions

We now glue the potential uu in the generic region 1≪min⁡{x1,x2}1\ll\min\{x_{1},x_{2}\}, and the potential ϕD1(2)\phi_{D_{1}}^{(2)} in the region x1≫|x2|+1x_{1}\gg|x_{2}|+1 (and a completely similar potential ϕD2(2)\phi_{D_{2}}^{(2)} in the region x2≫|x1|+1x_{2}\gg|x_{1}|+1). We now take a smooth cutoff function η:ℝ→[0,1]\eta:\mathbb{R}\to[0,1], with

η⁡(x)={1,x≤1,0,x≥2.\eta(x)=\begin{cases}1,\quad x\leq 1,\\ 0,\quad x\geq 2.\end{cases}

The glued potential is defined for |x1|+|x2|≫1|x_{1}|+|x_{2}|\gg 1,

ϕg​l​u​e=η⁡(C~​x2x1)​(ϕD1(2)−u)+η⁡(C~​x1x2)​(ϕD2(2)−u)+u,\phi_{glue}=\eta(\tilde{C}\frac{x_{2}}{x_{1}})(\phi_{D_{1}}^{(2)}-u)+\eta(\tilde{C}\frac{x_{1}}{x_{2}})(\phi_{D_{2}}^{(2)}-u)+u, (35)

where C~≫1\tilde{C}\gg 1 is some large fixed constant, specifying the gluing region x1∼C~​x2x_{1}\sim\tilde{C}x_{2} (resp. x2∼C~​x1x_{2}\sim\tilde{C}x_{1}). For large x1≥C~​x~2x_{1}\geq\tilde{C}\tilde{x}_{2}, then ϕg​l​u​e\phi_{glue} agrees with ϕD1(2)\phi_{D_{1}}^{(2)}, while for 2​C~​x~2≤x1≤(2​C~)−1​x22\tilde{C}\tilde{x}_{2}\leq x_{1}\leq(2\tilde{C})^{-1}x_{2}, then ϕg​l​u​e\phi_{glue} agrees with uu.

[0240]
Lemma 4.12.

For |x1|+|x2|≫1|x_{1}|+|x_{2}|\gg 1, the local Ck,αC^{k,\alpha}-norm of the metric gluing error

‖η⁡(C~​x2x1)​(ϕD1(2)−u)‖k,α,l​o​c=O⁡(x1−2​n−1n−1).\left\lVert\eta(\tilde{C}\frac{x_{2}}{x_{1}})(\phi_{D_{1}}^{(2)}-u)\right\rVert_{k,\alpha,loc}=O(x_{1}^{-\frac{2n-1}{n-1}}).

In particular the glued metric remains Kähler.

[0241]
Proof.

In the gluing region x1∼C~​x2x_{1}\sim\tilde{C}x_{2}, namely x1,x2x_{1},x_{2} and x~1\tilde{x}_{1} are comparably large, the deviation between ϕD1(2)\phi_{D_{1}}^{(2)} and uu comes from the O⁡(e−c​x21/2)O(e^{-cx_{2}^{1/2}}) small deviation between the Tian-Yau potential and the Calabi ansatz, and the correction term x~1n+2n−2​nn−1​U\tilde{x}_{1}^{\frac{n+2}{n}-\frac{2n}{n-1}}U. Ignoring the exponentially small effects, the only important term is x~1n+2n−2​nn−1​x21n−1\tilde{x}_{1}^{\frac{n+2}{n}-\frac{2n}{n-1}}x_{2}^{\frac{1}{n-1}}. We compute from Lemma 4.7

‖d​dc​(η​x~1n+2n−2​nn−1​x21n−1)‖k,α,l​o​c=O⁡(x1n+2n−2​nn−1+1n−1−2+n−2n)=O⁡(x1−2​n−1n−1).\left\lVert dd^{c}(\eta\tilde{x}_{1}^{\frac{n+2}{n}-\frac{2n}{n-1}}x_{2}^{\frac{1}{n-1}})\right\rVert_{k,\alpha,loc}=O(x_{1}^{\frac{n+2}{n}-\frac{2n}{n-1}+\frac{1}{n-1}-2+\frac{n-2}{n}})=O(x_{1}^{-\frac{2n-1}{n-1}}).

∎

We also need to extend the gluing ansatz to a Kähler metric over the compact region with x1,x2=O⁡(1)x_{1},x_{2}=O(1). We can first extend ϕg​l​u​e\phi_{glue} to a smooth potential over XX, which may not be Kähler inside a fixed compact set. Taking a very ample linear system H0​(X¯,m⁡(d1+d2)​L0)H^{0}(\bar{X},m(d_{1}+d_{2})L_{0}) for m≫1m\gg 1, we can construct a Fubini-Study metric on X¯\bar{X}. Using the defining section S1​S2∈H0​(X¯,(d1+d2)​L0)S_{1}S_{2}\in H^{0}(\bar{X},(d_{1}+d_{2})L_{0}) of the divisor D1+D2D_{1}+D_{2}, we can regard the Fubini-Study metric as a function on X=X¯∖D1∪D2X=\bar{X}\setminus D_{1}\cup D_{2}, of the form

ϕF​S=log∑i|si(S1​S2)m|2.\phi_{FS}=\log\sum_{i}|\frac{s_{i}}{(S_{1}S_{2})^{m}}|^{2}.

Clearly ϕF​S\phi_{FS} tends to infinity near D1∪D2D_{1}\cup D_{2} at a speed comparable to x1+x2x_{1}+x_{2}. We take some large constant A≫1A\gg 1, and R≫1R\gg 1 depending on AA, and add to ϕg​l​u​e\phi_{glue} the term A​ϕF​S​η​(ϕF​SR).A\phi_{FS}\eta(\frac{\phi_{FS}}{R}). Intuitively, the cutoff function η\eta turns off the Fubini-Study potential outside a large compact subset. By making AA large enough, we can improve ϕg​l​u​e\phi_{glue} to be Kähler in a fixed compact set. For R≫1R\gg 1, the cutoff error in the region ϕF​S∼R\phi_{FS}\sim R is suppressed by d​dc​ϕg​l​u​edd^{c}\phi_{glue}, and the metric remains positive. By a slight abuse, we shall continue to use ϕg​l​u​e\phi_{glue} to refer to the global Kähler metric on XX.

Define the volume error function E​r​r2Err_{2} by

(d​dc​ϕg​l​u​e)n=K0​(1+E​r​r2)​−1n2​Ω∧Ω¯.(dd^{c}\phi_{glue})^{n}=K_{0}(1+Err_{2})\sqrt{-1}^{n^{2}}\Omega\wedge\overline{\Omega}. (36)
[0242]
Corollary 4.13.

The volume form error of the glued ansatz is

‖E​r​r2‖k,α,l​o​c=O⁡((1+|x1|+|x2|)−2​n−1n−1).\left\lVert Err_{2}\right\rVert_{k,\alpha,loc}=O((1+|x_{1}|+|x_{2}|)^{-\frac{2n-1}{n-1}}).
[0243]
Proof.

For |x2|+1≪x1|x_{2}|+1\ll x_{1}, Lemma 4.11 says that the volume form error of ϕD1(2)\phi_{D_{1}}^{(2)} is O⁡(x1−2​nn−1​x21n−1)=O⁡(x1−2​n−1n−1)O(x_{1}^{-\frac{2n}{n-1}}x_{2}^{\frac{1}{n-1}})=O(x_{1}^{-\frac{2n-1}{n-1}}). In the gluing region x1∼C~​x2x_{1}\sim\tilde{C}x_{2}, the volume form error is controlled by the metric gluing error, which is again O⁡(x1−2​n−1n−1)O(x_{1}^{-\frac{2n-1}{n-1}}) by Lemma 4.12. What happens near D2D_{2} is completely analogous. Finally, in the compact region x1,x2=O⁡(1)x_{1},x_{2}=O(1), the smoothness of ϕg​l​u​e\phi_{glue} means that the local Ck,αC^{k,\alpha}-norm is O⁡(1)O(1). ∎

[0244]

4.7 Distance-like function

For our later invocation of Hein’s package (cf. section 5.1), we need to know the existence of distance-like functions with gradient and complex Hessian control.

Define a smooth function

ρ~=(x12+x22+1)n+24​n.\tilde{\rho}=(x_{1}^{2}+x_{2}^{2}+1)^{\frac{n+2}{4n}}.

As discussed in section 2.6, the distance function to the origin is uniformly equivalent outside a compact set to |x|n+22​n,|x|^{\frac{n+2}{2n}}, and ρ~\tilde{\rho} can be viewed as a regularized version. An easy consequence of Lemma 4.7 is

[0245]
Lemma 4.14.

The function ρ~\tilde{\rho} satisfies |d​ρ~|≤C|d\tilde{\rho}|\leq C and ρ~​|d​dc​ρ~|≤C.\tilde{\rho}|dd^{c}\tilde{\rho}|\leq C.

In terms of the distance-like function ρ~\tilde{\rho}, we can rewrite Cor. 4.13 as

‖E​r​r2‖k,α,l​o​c=O⁡(ρ~−2​n​(2​n−1)(n−1)​(n+2)).\left\lVert Err_{2}\right\rVert_{k,\alpha,loc}=O(\tilde{\rho}^{-\frac{2n(2n-1)}{(n-1)(n+2)}}). (37)

Crucially for our later purpose, this decay is faster than quadratic O⁡(ρ~−2)O(\tilde{\rho}^{-2}) to all orders of derivatives. Morever, the formula for the Ricci form

Ric=−−1∂∂¯log((d​dc​ϕg​l​u​e)nK0​−1n2​Ω∧Ω¯)Ric=-\sqrt{-1}\partial\bar{\partial}\log\left(\frac{(dd^{c}\phi_{glue})^{n}}{K_{0}\sqrt{-1}^{n^{2}}\Omega\wedge\overline{\Omega}}\right)

implies |R​i​c|=O⁡(ρ~−2)|Ric|=O(\tilde{\rho}^{-2}) for the glued ansatz.

[0246]

5 Weighted Sobolev and Calabi-Yau metric

[0247]

5.1 Hein’s package

Hein [8, Chapter 3, 4] sets out a framework for solving the complex Monge-Ampère equation on complete noncompact manifolds, building on the seminal paper by Tian and Yau [16]. We explain Hein’s results in a variant form which follows from his arguments. The ambient complete manifold MM needs to satisfy the following analytic properties:

  • •

    There is a Ck,αC^{k,\alpha} quasi-atlas with k≥3k\geq 3, meaning a collection of charts on which the metric is uniformly equivalent to the Euclidean metric, and the complex structure and the metric has Ck,αC^{k,\alpha} bounds. Beware that in our applications the injectivity radius can degenerate, and the charts involve local universal covers.

  • •

    There is a function ρ~\tilde{\rho} uniformly equivalent to dist​(0,x)+1\text{dist}(0,x)+1, and satisfies |∇ρ~|+ρ~​|d​dc​ρ~|≤C|\nabla\tilde{\rho}|+\tilde{\rho}|dd^{c}\tilde{\rho}|\leq C. This assumption is useful in integration by part arguments.

  • •

    We need the weighted Sobolev inequality on functions: assume the power law volume growth Vol​(B​(r))∼rp′\text{Vol}(B(r))\sim r^{p^{\prime}} with rate p′>2p^{\prime}>2. For 1≤p≤dimℝMdimℝM−21\leq p\leq\frac{\dim_{\mathbb{R}}M}{\dim_{\mathbb{R}}M-2} and functions uu with L2L^{2}-gradient,

    (∫|u|2​p​ρ~p⁡(p′−2)−p′​𝑑v​o​l)1/p≤C​∫|∇u|2.(\int|u|^{2p}\tilde{\rho}^{p(p^{\prime}-2)-p^{\prime}}dvol)^{1/p}\leq C\int|\nabla u|^{2}.

    These inequalities differ from the standard Sobolev inequalities in the sense that they do not require the manifold to have Euclidean volume growth, which makes them remarkably flexible.

The output of this package is:

  • •

    Denote ω0\omega_{0} as the ambient Kähler form. Let f∈C2,αf\in C^{2,\alpha} satisfy |f|≤C​ρ~−q|f|\leq C\tilde{\rho}^{-q} for p′>q>2p^{\prime}>q>2. Then there is some 0<α′≤α0<\alpha^{\prime}\leq\alpha and u∈C4,α′u\in C^{4,\alpha^{\prime}} which solves (ω0+d​dc​u)dimℂM=ef​ω0dimℂM(\omega_{0}+dd^{c}u)^{\dim_{\mathbb{C}}M}=e^{f}\omega_{0}^{\dim_{\mathbb{C}}M}, with decay estimate |u|≤C​ρ~2−q+ϵ|u|\leq C\tilde{\rho}^{2-q+\epsilon}, where ϵ≪1\epsilon\ll 1 is any fixed small number.

Here we have separated the assumptions on the ambient manifolds from the decay assumptions to emphasize that these are difficulties of distinct nature. The key idea in Hein’s package is to obtain a priori L∞L^{\infty} estimates and power law decay estimates on potentials via the method of weighted Moser iteration, which hinges on the weighted Sobolev inequalities. The estimates from Hein’s package are constructive. It is essential to assume faster than quadratic decay on the source function ff, because the method needs the potential u=O⁡(ρ2−q)u=O(\rho^{2-q}) to be bounded.

[0248]

5.2 Sufficient condition for weighted Sobolev

Now recall [9, Def. 1.1] a complete manifold (M,g)(M,g) is called SOB​(p′)\text{SOB}(p^{\prime}), if there exist x0∈Mx_{0}\in M and C≥1C\geq 1 such that

  • •

    B⁡(x0,s)∖B⁡(x0,t)B(x_{0},s)\setminus B(x_{0},t) is connected for all s≥t≥Cs\geq t\geq C,

  • •

    Vol​(B⁡(x0,s))≤C​sp′\text{Vol}(B(x_{0},s))\leq Cs^{p^{\prime}} for all s≥Cs\geq C,

  • •

    Vol​(B⁡(x,(1−C−1)​r​(x)))≥C−1​r​(x)p′\text{Vol}(B(x,(1-C^{-1})r(x)))\geq C^{-1}r(x)^{p^{\prime}} and R​i​c​(x)≥−C​r​(x)−2Ric(x)\geq-Cr(x)^{-2} if r⁡(x)=d​i​s​t​(x0,x)≥Cr(x)=dist(x_{0},x)\geq C.

Hein [9] shows that when p′>2p^{\prime}>2, then S​O​B​(p′)SOB(p^{\prime}) is a sufficient conditions for the weighted Sobolev inequality. As observed in [20, section 7], the connectivity of the annulus can be relaxed to the weaker requirement of relative connected annulus:

  • •

    For sufficiently large DD, any two points x1,x2∈Mx_{1},x_{2}\in M with d⁡(x0,xi)=Dd(x_{0},x_{i})=D can be joined by a curve of length at most C​DCD, lying in the annulus B⁡(x0,C​D)∖B⁡(x0,C−1​D)B(x_{0},CD)\setminus B(x_{0},C^{-1}D), for a uniform constant C>1C>1.

For our particular metric ansatz d​dc​ϕg​l​u​edd^{c}\phi_{glue}, the assumptions on the volume growth rate of balls are immediate consequences of the our much more refined description of the generalized Calabi ansatz, and the metric behaviour near the Tian-Yau region. The quadratic decay on the Ricci tensor is a consequence of the faster than quadratic decay on the volume form error to all derivatives (cf. section 4.7).

To verify the relative connnected annulus property, notice any point close to the Tian-Yau region can be first connected via a path of length O⁡(ρ~)O(\tilde{\rho}) contained inside the annulus, to a point in the generic region where x1,x2x_{1},x_{2} are comparable, and the statement is obvious for two points in the generic region.

[0249]

5.3 Assembling the pieces

[024A]
Theorem 5.1.

(Existence of complete Calabi-Yau metric) There is a potential ϕr​e​l\phi_{rel} such that ϕ=ϕg​l​u​e+ϕr​e​l\phi=\phi_{glue}+\phi_{rel} solves the complex Monge-Ampère equation with decay bound

(d​dc​ϕ)n=K0​−1n2​Ω∧Ω¯,‖ϕr​e​l‖k,α,l​o​c=O⁡(ρ~−q),(dd^{c}\phi)^{n}=K_{0}\sqrt{-1}^{n^{2}}\Omega\wedge\overline{\Omega},\quad\left\lVert\phi_{rel}\right\rVert_{k,\alpha,loc}=O(\tilde{\rho}^{-q}),

where qq can be chosen as any positive number smaller than 2​n−4n+2\frac{2n-4}{n+2}.

[024B]
Proof.

We have verified the weighted Sobolev inequality (cf. section 5.2), the existence of the distance-like function (cf. section 4.7), and the existence of Ck,αC^{k,\alpha} quasi-atlas (cf. section 4.1, 4.2).

The volume form error for d​dc​ϕg​l​u​edd^{c}\phi_{glue} decays like O⁡(ρ~−2​n​(2​n−1)(n−1)​(n+2))O(\tilde{\rho}^{-\frac{2n(2n-1)}{(n-1)(n+2)}}) (cf. (36)). On the other hand, the volume growth rate is O⁡(ρ~p′)O(\tilde{\rho}^{p^{\prime}}) with 2<p′=4​nn+2<2​n​(2​n−1)(n−1)​(n+2)2<p^{\prime}=\frac{4n}{n+2}<\frac{2n(2n-1)}{(n-1)(n+2)}. In particular the volume error is bounded by O⁡(ρ~−p′)O(\tilde{\rho}^{-p^{\prime}}). Applying Hein’s package, we can find a Ck,αC^{k,\alpha} bounded solution ϕr​e​l\phi_{rel}, such that

(d​dc​ϕg​l​u​e+d​dc​ϕr​e​l)n=(1+E​r​r2)−1​(d​dc​ϕg​l​u​e)n=K0​−1n2​Ω∧Ω¯,(dd^{c}\phi_{glue}+dd^{c}\phi_{rel})^{n}=(1+Err_{2})^{-1}(dd^{c}\phi_{glue})^{n}=K_{0}\sqrt{-1}^{n^{2}}\Omega\wedge\overline{\Omega},

with decay estimate |ϕr​e​l|=O⁡(ρ~2−p0+ϵ)=O⁡(ρ~−q)|\phi_{rel}|=O(\tilde{\rho}^{2-p_{0}+\epsilon})=O(\tilde{\rho}^{-q}). Since the charts on the local universal covers have harmonic radius scale O⁡(ρ)O(\rho), elliptic regularity improves the decay estimate to local Ck,αC^{k,\alpha}-norms. ∎

The smallness of d​dc​ϕr​e​ldd^{c}\phi_{rel} near infinity means that the main features of the asymptotic geometry are preserved. In particular, the volume growth of the Calabi-Yau metric d​dc​ϕdd^{c}\phi is Vol​(B⁡(ρ~))∼ρ~4​nn+2\text{Vol}(B(\tilde{\rho}))\sim\tilde{\rho}^{\frac{4n}{n+2}}. The tangent cone at infinity refers to the pointed Gromov-Hausdorff limit of rescaled geodesic balls centred at a fixed reference point. In our case, the rescaling procedure obliviates the T2T^{2} and YY-fibres . The tangent cone is topologically ℝ≥02\mathbb{R}_{\geq 0}^{2} with the variables x1,x2x_{1},x_{2}, and metrically it is up to a constant the Hessian metric

g∞=∂2u∂xi​∂xj​d​xi​d​xj,g_{\infty}=\frac{\partial^{2}u}{\partial x_{i}\partial x_{j}}dx_{i}dx_{j},

where u⁡(x1,x2)u(x_{1},x_{2}) is the solution to the non-archimedean Monge-Ampère equation. The renormalized measure on the tangent cone, which comes from pushing forward the complex Monge-Ampère measure, is up to constant factor d​x1​d​x2dx_{1}dx_{2}.

[024C]

Appendix: Hypergeometric functions

Recall that the hypergeometric function F12​[a,b;c;z]\,{}_{2}F_{1}[a,b;c;z] is defined by

2F1[a,b;c;z]=∑n=0∞(a)n​(b)nn!​(c)nzn\,_{2}F_{1}[a,b;c;z]=\sum_{n=0}^{\infty}\frac{(a)_{n}(b)_{n}}{n!(c)_{n}}z^{n} (38)

where

(α)n:=α(α+1)(α+2)⋯(α+n−1),(α)0=1(\alpha)_{n}:=\alpha(\alpha+1)(\alpha+2)\cdots(\alpha+n-1),\quad(\alpha)_{0}=1

and we assume that c∉ℤ≤0c\notin\mathbb{Z}_{\leq 0}. It is a standard fact that the hypergeometric series converges when |z|<1|z|<1 and when Re⁡(c−a−b)>0{\rm Re}(c-a-b)>0 is also converges when z=1z=1; see for instance [1, Chapter 1].

We start from the elementary Taylor expansion

(1−y)−β=∑k=0∞(β)kk!​yk,|y|<1.(1-y)^{-\beta}=\sum_{k=0}^{\infty}\frac{(\beta)_{k}}{k!}y^{k},\quad|y|<1.
[024D]
Lemma 5.2.

For x≥1x\geq 1 we have

∫1x(1−y−2)−1/ndy=x2F1[−12,1n;12;x−2]−2F1[−12,1n;12;1].\int_{1}^{x}(1-y^{-2})^{-1/n}dy=x\,_{2}F_{1}[-\frac{1}{2},\frac{1}{n};\frac{1}{2};x^{-2}]-\,_{2}F_{1}[-\frac{1}{2},\frac{1}{n};\frac{1}{2};1].
[024E]
Proof.

We compute

∫1x(1−y−2)−1/ndy=∫1x∑k=0∞(1n)kk!y−2​kdy=y∑k=0∞(1n)kk!y−2​k(−2​k+1)|y=1y=x.\displaystyle\int_{1}^{x}(1-y^{-2})^{-1/n}dy=\int_{1}^{x}\sum_{k=0}^{\infty}\frac{(\frac{1}{n})_{k}}{k!}y^{-2k}dy=y\sum_{k=0}^{\infty}\frac{(\frac{1}{n})_{k}}{k!}\frac{y^{-2k}}{(-2k+1)}\bigg|_{y=1}^{y=x}.

The Lemma follows from the observation (−12)k(12)k=−12​k−1.\frac{(-\frac{1}{2})_{k}}{(\frac{1}{2})_{k}}=-\frac{1}{2k-1}. ∎

[024F]
Proposition 5.3.

Let n≥3n\geq 3. Suppose gg satisfies the ODE

dd​y​(gy)=1y2​(1−yn)12,0<y<1,\frac{d}{dy}\left(\frac{g}{y}\right)=\frac{1}{y^{2}(1-y^{n})^{\frac{1}{2}}},\qquad 0<y<1,

together with the initial conditions g⁡(0)=−1,g′​(0)=0g(0)=-1,g^{\prime}(0)=0. Then we have

g(y)=−2F1[12,−1n;n−1n;yn].g(y)=-\,_{2}F_{1}[\frac{1}{2},-\frac{1}{n};\frac{n-1}{n};y^{n}].

In particular

g(1)=limy→1g(y)=−2F1[12,−1n;n−1n;1]=−Γ⁡(n−1n)​πΓ⁡(n−22​n).g(1)=\lim_{y\to 1}g(y)=-\,_{2}F_{1}[\frac{1}{2},-\frac{1}{n};\frac{n-1}{n};1]=-\frac{\Gamma(\frac{n-1}{n})\sqrt{\pi}}{\Gamma(\frac{n-2}{2n})}.
[024G]
Proof.

Integrating

y−2(1−yn)−1/2=∑k=0∞(12)kk!yn​k−2,y^{-2}(1-y^{n})^{-1/2}=\sum_{k=0}^{\infty}\frac{(\frac{1}{2})_{k}}{k!}y^{nk-2},

and utilizing the initial conditions to fix the leading coefficients,

g⁡(y)=∑k=0∞(12)kk!​yn​kn​k−1.g(y)=\sum_{k=0}^{\infty}\frac{(\frac{1}{2})_{k}}{k!}\frac{y^{nk}}{nk-1}.

The formula for g⁡(y)g(y) follows from the observation −1n​k−1=(−1n)k(n−1n)k.\frac{-1}{nk-1}=\frac{(-\frac{1}{n})_{k}}{(\frac{n-1}{n})_{k}}. The evaluation of g⁡(1)g(1) appeals to Gauss’ hypergeometric theorem [1, Section 1.3]:

[024H]
Lemma 5.4.

For a,b,ca,b,c with Re⁡(c−a−b)>0{\rm Re}(c-a-b)>0 we have

F12​[a,b;c;1]=Γ⁡(c)​Γ​(c−a−b)Γ⁡(c−a)​Γ​(c−b).\,{}_{2}F_{1}[a,b;c;1]=\frac{\Gamma(c)\Gamma(c-a-b)}{\Gamma(c-a)\Gamma(c-b)}.

∎

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Department of Mathematics, Massachusetts Institute of Technology, 77 Massachusetts Avenue, Cambridge, MA 02139

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