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Chapter 1 Introduction and Background Review [03Y2]

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Chapter 1 Introduction and Background Review

The principal motivation of this paper lies in the metric aspect of the Strominger-Yau-Zaslow (SYZ) conjecture for 3-folds, a strong form of which states

Conjecture 1.1.

[26][16] Let (Xt,gt)(X_{t},g_{t}) be a degenerating family of (polarized) Calabi-Yau 3-folds near the large complex structure limit, equipped with Calabi-Yau metrics gtg_{t}. Then for |t|≪1|t|\ll 1, the 3-fold XtX_{t} admits a special Lagrangian T3T^{3}-fibration over a base BB homeomorphic to a 3-sphere, known as the SYZ fibration. The base BB is equipped with an affine structure and a compatible metric gBg_{B} solving the real Monge-Ampère equation with singularities along a trivalent graph 𝔇⊂B\mathfrak{D}\subset B, such that the rescaled Calabi-Yau metrics (Xt,diam​(gt)−2​gt)(X_{t},\text{diam}(g_{t})^{-2}g_{t}) converge to (B,gB)(B,g_{B}) in Gromov-Hausdorff sense as t→0t\to 0. Morever, suitably away from 𝔇\mathfrak{D} the metrics gtg_{t} are approximated by a semiflat metric up to exponentially small errors.

The SYZ conjecture stands at the crossroad of algebraic, symplectic, Riemannian and calibrated geometry. In the past two decades following the SYZ proposal there has emerged a sophisticated topological, algebro-geometric and symplectic picture [16][9]. The topological and complex geometric description for SYZ fibrations developed by Gross, Ruan, Joyce and Zharkov will be recalled in Section 1.1.

The prototype result in the metric direction is Gross and Wilson’s description of the degenerating K3 metrics [11]. Crucial in [11] is an explicit metric model for the neighbourhood of the singular SYZ fibres, known as the Ooguri-Vafa metric, constructed via the Gibbons-Hawking ansatz (cf. review Section 1.3). After hyperkähler rotation, the SYZ fibration turns into a holomorphic fibration by elliptic curves over ℙ1≃S2\mathbb{P}^{1}\simeq S^{2}, where the fibres have much smaller diameters compared to the base, a phenomenon known as collapsing. Gross and Wilson construct the collapsing K3 metrics by gluing the Ooguri-Vafa metric to a semiflat metric with exponentially small gluing error. Some features of their construction persist on higher dimensional hyperkähler manifolds with holomorphic Lagrangian Abelian variety fibrations [10]. Variants of the Ooguri-Vafa metric feature prominently in other types of metric degenerations on K3 surfaces [13].

Beyond the hyperkähler case, Zharkov et al [31][32] established a formal differential geometric framework called the generalised Gibbons-Hawking ansatz designed to construct Calabi-Yau metrics with torus symmetry, and pointed out its relevance to the metric aspects of the SYZ conjecture (cf. review Section 1.2 and 1.1.6). Despite all the progress, essentially no analytic result was known concerning the Calabi-Yau metric on a quintic 3-fold near the large complex structure limit, beyond its abstract existence due to Yau’s solution of the Calabi conjecture.

The main accomplishment of this paper is to use the generalised Gibbons-Hawking ansatz to construct two types of analogues for the Ooguri-Vafa metrics on Calabi-Yau 3-folds, corresponding to the positive vertex and the negative vertex, referring to the neighbourhoods of the two types of most singular SYZ fibres in a generic 3-fold SYZ fibration according to the Gross-Ruan-Joyce classification. As a byproduct of our project, we construct a family of new exotic Calabi-Yau metrics on ℂ3\mathbb{C}^{3} with properties akin to the Taub-NUT metric on ℂ2\mathbb{C}^{2}.

Here is a crude statement for the main results. A fuller summary can be found in the introductions to individual Chapters.

Theorem 1.2.

(Taub-NUT type metric on ℂ3\mathbb{C}^{3}, cf. Chapter 2) There is a family of Calabi-Yau metrics on (ℂz0,z1,z23,−d​z0∧d​z1∧d​z2)(\mathbb{C}^{3}_{z_{0},z_{1},z_{2}},-dz_{0}\wedge dz_{1}\wedge dz_{2}) invariant under the diagonal T2T^{2}-action, which are parametrised by positive definite rank 2 real symmetric matrices (ai​j)(a_{ij}). The base of the T2T^{2}-fibration is ℝμ1,μ22×ℂη\mathbb{R}^{2}_{\mu_{1},\mu_{2}}\times\mathbb{C}_{\eta} and the discriminant locus is the trivalent graph

𝔇={μ2≥0,μ1=0,η=0}∪{μ1≥0,μ2=0,η=0}∪{μ1=μ2≤0,η=0}.\mathfrak{D}=\{\mu_{2}\geq 0,\mu_{1}=0,\eta=0\}\cup\{\mu_{1}\geq 0,\mu_{2}=0,\eta=0\}\cup\{\mu_{1}=\mu_{2}\leq 0,\eta=0\}.

The tangent cone at infinity is the Euclidean ℝ4\mathbb{R}^{4}. Near spatial infinity suitably away from 𝔇\mathfrak{D}, the metric is approximately a flat T2T^{2} fibration over an open subset of Euclidean ℝ4\mathbb{R}^{4}, such that the metric on the T2T^{2}-fibres is asymptotically given by the inverse matrix (ai​j)(a^{ij}) in distinguished coordinates. The metric transverse to 𝔇\mathfrak{D} is modelled on a fibration by Taub-NUT metrics.

Remark 1.1.

Readers primarily interested in this Taub-NUT type metric on ℂ3\mathbb{C}^{3} can treat Chapter 2 as an indepenent paper, and refer to Section 1.2 for backgrounds.

Theorem 1.3.

(Ooguri-Vafa type metric on the positive vertex, cf. Chapter 3) There is a family of incomplete Calabi-Yau metrics with T2T^{2}-symmetry, which are parametrised by positive definite rank 2 real symmetric matrices (ai​j)(a_{ij}), such that

  • •

    The ambient space has the same topology as the positive vertex predicted by Gross-Ruan-Joyce, namely it is a singular T2T^{2}-bundle over a 4-dimensional base contained in ℝμ1,μ22×(S1×ℝ)η\mathbb{R}^{2}_{\mu_{1},\mu_{2}}\times(S^{1}\times\mathbb{R})_{\eta} with discriminant locus along

    𝔇={μ2≥0,μ1=0,η=0}∪{μ1≥0,μ2=0,η=0}∪{μ1=μ2≤0,η=0}.\mathfrak{D}=\{\mu_{2}\geq 0,\mu_{1}=0,\eta=0\}\cup\{\mu_{1}\geq 0,\mu_{2}=0,\eta=0\}\cup\{\mu_{1}=\mu_{2}\leq 0,\eta=0\}.
  • •

    The holomorphic structure together with the holomorphic volume form agrees with the Zharkov prediction (cf. Section 1.1.6).

  • •

    Suitably away from 𝔇\mathfrak{D} there is a T3T^{3}-fibration structure such that the Calabi-Yau metrics decay exponentially to semiflat metrics.

  • •

    These metrics extend over an exponentially large region, under the unit homological volume normalisation on T3T^{3}.

  • •

    Metric behaviour near the origin is modelled on the Taub-NUT type metrics on ℂ3\mathbb{C}^{3} mentioned above. Metric behaviour transverse to 𝔇\mathfrak{D} but suitably away from the origin is modelled on a fibration by Taub-NUT metrics. Metric behaviour suitably away from 𝔇\mathfrak{D} is approximately a flat T2T^{2}-bundle over an open subset of ℝμ1,μ22×(S1×ℝ)η\mathbb{R}^{2}_{\mu_{1},\mu_{2}}\times(S^{1}\times\mathbb{R})_{\eta} with a Euclidean metric.

  • •

    These Calabi-Yau metrics admit special Lagrangian T3T^{3}-fibrations.

Theorem 1.4.

(Ooguri-Vafa type metric on the negative vertex, cf. Chapter 4) There is a family of incomplete Calabi-Yau metrics with S1S^{1}-symmetry, which are parametrised by rank 2 Hermitian matrices (ap​q¯)(a_{p\bar{q}}), such that

  • •

    The ambient space is topologically a singular S1S^{1}-bundle over a 5-dimensional base contained in (ℂ∗)z1,z22×ℝμ(\mathbb{C}^{*})^{2}_{z_{1},z_{2}}\times\mathbb{R}_{\mu}, with discriminant locus along

    S={z1+z2=1,μ=0}⊂(ℂ∗)z1,z22×ℝμ.S=\{z_{1}+z_{2}=1,\mu=0\}\subset(\mathbb{C}^{*})^{2}_{z_{1},z_{2}}\times\mathbb{R}_{\mu}.
  • •

    The holomorphic structure together with the holomorphic volume form agrees with the Zharkov prediction (cf. Section 1.1.6).

  • •

    Suitably away from SS there is a T3T^{3}-fibration structure such that these Calabi-Yau metrics decay exponentially to semiflat metrics.

  • •

    These metrics extend over an exponentially large region, under the unit homological volume normalisation on T3T^{3}.

  • •

    Metric behaviour transverse to SS is modelled on a fibration by Taub-NUT metrics. Metric behaviour suitably away from SS is approximately a flat S1S^{1}-bundle over an open subset of (ℂ∗)z1,z22×ℝμ(\mathbb{C}^{*})^{2}_{z_{1},z_{2}}\times\mathbb{R}_{\mu} with a Euclidean metric.

Remark 1.2.

Loftin, Yau and Zaslow [21] attempted to find semiflat metrics on the vertices by a reduction from the 3-dimensional real Monge-Ampère equation to the elliptic affine sphere. However it is unclear whether their construction has the requisite topology, or how it compares with our construction.

Remark 1.3.

After the completion of this paper, S. Sun and R. Zhang inform the author that they have independently expected the same construction.

Notation.

Summation convention will be used throughout the paper.

We now proceed with an extended review of the necessary backgrounds. Some of the main techniques in this paper will be demonstrated below on the Taub-NUT metric and the Ooguri-Vafa metric.

1.1. Gross-Ruan-Joyce picture of SYZ fibrations

Here we review the expected picture of special Lagrangian T3T^{3}-fibrations (=SYZ fibrations) f:M→Bf:M\to B on a Calabi-Yau 3-fold near the large complex structure limit. The primary sources are the work of M. Gross [6][8] and W. D. Ruan [24], with important modifications proposed by D. Joyce (cf. [14] Section 8). The survey of Morrison [22] provides good background reading.

Gross [8] observes that if f:M→Bf:M\to B is a smooth SYZ fibration then the discriminant locus 𝔇⊂B\mathfrak{D}\subset B is of Hausdorff codimension 2. Combined with monodromy considerations, this leads to the speculation that for generic such fibrations 𝔇\mathfrak{D} is a trivalent graph, consisting of smooth edges and two kinds of vertices, which we refer to as positive and negative vertices following [14].

1.1.1. Generic region

In the generic region f:M→Bf:M\to B is a smooth proper submersion with T3T^{3} fibres. A torus fibration is called semiflat if the metric restricts to flat metrics on the tori. The Calabi-Yau structure (g,ω,Ω)(g,\omega,\Omega) on a semiflat SYZ T3T^{3}-fibration can be locally described in action-angle coordinates as

{ω=∑13d​μi∧d​θi,Ω=(det(gi​j))−1/2⋀i=13(dθi−−1gi​jdμj),g=gi​j​d​θi​d​θj+gi​j​d​μi​d​μj.\begin{cases}\omega=\sum_{1}^{3}d\mu_{i}\wedge d\theta_{i},\\ \Omega=(\det(g_{ij}))^{-1/2}\bigwedge_{i=1}^{3}(d\theta_{i}-\sqrt{-1}g_{ij}d\mu_{j}),\\ g=g^{ij}d\theta_{i}d\theta_{j}+g_{ij}d\mu_{i}d\mu_{j}.\end{cases}

Here gi​jg_{ij} is the Hessian of a real valued function φ\varphi on BB solving the real Monge-Ampère equation:

gi​j=∂2φ∂μi​∂μj,det(∂2φ∂μi​∂μj)=const.g_{ij}=\frac{\partial^{2}\varphi}{\partial\mu_{i}\partial\mu_{j}},\quad\det(\frac{\partial^{2}\varphi}{\partial\mu_{i}\partial\mu_{j}})=\text{const}.

and gi​jg_{ij} defines a metric on the base gB=gi​j​d​μi​d​μjg_{B}=g_{ij}d\mu_{i}d\mu_{j} such that f:M→Bf:M\to B is a Riemannian submersion.

The Calabi-Yau structure induce two sets of affine structures on the base BB: the symplectic moment coordinates μi\mu_{i} satisfying d​μi=−ω⁡(∂∂θi,⋅)d\mu_{i}=-\omega(\frac{\partial}{\partial\theta_{i}},\cdot), and the complex affine coordinates yiy_{i} satisfying dyi=ImΩ(∂∂θj,∂∂θk,⋅)dy_{i}=\text{Im}\Omega(\frac{\partial}{\partial\theta_{j}},\frac{\partial}{\partial\theta_{k}},\cdot) for cyclic indices i,j,ki,j,k. These coordinates are related by the Legendre transform yi=−∂φ∂μi.y_{i}=-\frac{\partial\varphi}{\partial\mu_{i}}.

Semiflat mirror symmetry is the observation that if over the same base BB we fibrewise replace T3T^{3} by the dual tori, then there is a canonical Calabi-Yau structure exhibiting this dual torus fibration as a semiflat SYZ fibration. Furthermore, the base metric gBg_{B} is unchanged while the roles of the two affine structures are interchanged.

A major part of the SYZ Conjecture 1.1 is that Calabi-Yau metrics on (polarised) manifolds near the large complex structure limit are asymptotically described by such semiflat SYZ fibrations in the generic region up to exponentially small errors.

1.1.2. Edges

Along an edge Δ⊂𝔇\mathfrak{\Delta}\subset\mathfrak{D}, the singular fibres have the topology of T3T^{3} with T2T^{2} collapsed to S1S^{1}, alternatively written as I1×S1I_{1}\times S^{1}, where I1I_{1} refers to the nodal elliptic curve or equivalently S2S^{2} with two points identified. Notice the singularity on the fibre is not isolated. These singular fibres have Betti numbers (b1,b2)=(2,2)(b_{1},b_{2})=(2,2) and Euler characteristic 0. The T3T^{3}-fibration is locally described as the Kodaira type I1I_{1} degenerating family of elliptic curves over a disc D2⊂ℂD^{2}\subset\mathbb{C}, Cartesian product with the trivial S1S^{1}-bundle S1×ℝ→ℝS^{1}\times\mathbb{R}\to\mathbb{R}. The monodromy around the edge Δ⊂𝔇\mathfrak{\Delta}\subset\mathfrak{D} acting on H1​(T3)≃ℤ3H_{1}(T^{3})\simeq\mathbb{Z}^{3} can be written in a suitable basis as

[110010001].\begin{bmatrix}1&1&0\\ 0&1&0\\ 0&0&1\end{bmatrix}.

For an alternative viewpoint which ties in better with the Gibbons-Hawking construction (see later Sections 1.2), the base is B⊂ℝ3B\subset\mathbb{R}^{3}, and the total space MM is a singular S1S^{1}-bundle over S1×B×S1S^{1}\times B\times S^{1}, where the S1S^{1}-fibres collapse to points along the codimension 3 locus {0}×Δ×S1⊂S1×B×S1\{0\}\times\mathfrak{\Delta}\times S^{1}\subset S^{1}\times B\times S^{1}. In the 3 transverse directions, the singular S1S^{1}-bundle structure is topologically modelled on the Hopf map

(1.1) πℂ2:ℂ2→ℝ×ℂ,(z0,z1)↦(12​(|z1|2−|z0|2),z0​z1).\pi_{\mathbb{C}^{2}}:\mathbb{C}^{2}\to\mathbb{R}\times\mathbb{C},\quad(z_{0},z_{1})\mapsto\left(\frac{1}{2}(|z_{1}|^{2}-|z_{0}|^{2}),z_{0}z_{1}\right).

The Chern class c1∈H2​(S1×B×S1∖({0}×Δ×S1),ℤ)c_{1}\in H^{2}(S^{1}\times B\times S^{1}\setminus(\{0\}\times\mathfrak{\Delta}\times S^{1}),\mathbb{Z}) evaluates to 1 on a suitably oriented S2S^{2}-cycle linking {0}×Δ×S1\{0\}\times\mathfrak{\Delta}\times S^{1} inside S1×B×S1S^{1}\times B\times S^{1}.

Remark 1.4.

In this review Section topology refers to the continuous topology. There are subtleties with extending the smooth structure on the singular S1S^{1}-bundle across the discriminant locus (cf. Section 2.3).

1.1.3. Positive vertices

Let 𝔇⊂B\mathfrak{D}\subset B be a graph with one vertex emitting 3 edges. Topologically, we can present 𝔇\mathfrak{D} as

(1.2) 𝔇=𝔇1∪𝔇2∪𝔇3∪{0}={μ1=0,μ2>0}∪{μ2=0,μ1>0}∪{μ1=μ2<0}∪{0}⊂ℝμ1,μ22×{0}⊂ℝ2×ℝ=B.\begin{split}\mathfrak{D}&=\mathfrak{D}_{1}\cup\mathfrak{D}_{2}\cup\mathfrak{D}_{3}\cup\{0\}\\ &=\{\mu_{1}=0,\mu_{2}>0\}\cup\{\mu_{2}=0,\mu_{1}>0\}\cup\{\mu_{1}=\mu_{2}<0\}\cup\{0\}\\ &\subset\mathbb{R}^{2}_{\mu_{1},\mu_{2}}\times\{0\}\subset\mathbb{R}^{2}\times\mathbb{R}=B.\end{split}

The total space M+M^{+} is built as a singular T2T^{2}-bundle over B×S1=ℝμ1,μ22×ℝ×S1B\times S^{1}=\mathbb{R}^{2}_{\mu_{1},\mu_{2}}\times\mathbb{R}\times S^{1} with discriminant locus 𝔇×{0}⊂B×S1\mathfrak{D}\times\{0\}\subset B\times S^{1}. Let e1,e2e_{1},e_{2} denote a basis of H1​(T2,ℤ)H_{1}(T^{2},\mathbb{Z}), and denote T⁡(a​e1+b​e2)T(ae_{1}+be_{2}) as the subtorus with homology class a​e1+b​e2ae_{1}+be_{2}. Over (B×S1)∖(𝔇×{0})(B\times S^{1})\setminus(\mathfrak{D}\times\{0\}) the space M+M^{+} is a principal T2T^{2}-bundle, whose Chern class c1∈H2​(B×S1∖(𝔇×{0}),ℤ​e1⊕ℤ​e2)c_{1}\in H^{2}(B\times S^{1}\setminus(\mathfrak{D}\times\{0\}),\mathbb{Z}e_{1}\oplus\mathbb{Z}e_{2}) evaluates to e1,−e2,−e1+e2e_{1},-e_{2},-e_{1}+e_{2} respectively on the S2S^{2}-cycles linking 𝔇1×{0},𝔇2×{0},𝔇3×{0}\mathfrak{D}_{1}\times\{0\},\mathfrak{D}_{2}\times\{0\},\mathfrak{D}_{3}\times\{0\} inside B×S1B\times S^{1}. Over the codimension 3 loci 𝔇1×{0}\mathfrak{D}_{1}\times\{0\}, 𝔇2×{0}\mathfrak{D}_{2}\times\{0\}, 𝔇3×{0}\mathfrak{D}_{3}\times\{0\} inside B×S1B\times S^{1}, the T2T^{2}-fibres collapse to circle fibres T2/T⁡(e1)T^{2}/T(e_{1}), T2/T⁡(−e2)T^{2}/T(-e_{2}), T2/T⁡(−e1+e2)T^{2}/T(-e_{1}+e_{2}) respectively. Finally, over the origin {0}⊂B×S1\{0\}\subset B\times S^{1}, the T2T^{2}-fibre collapses to a point. The singular T2T^{2}-bundle over a small neighbourhood of the origin D4⊂B×S1D^{4}\subset B\times S^{1} is topologically modelled on

(1.3) πℂ3:ℂ3→ℝμ1,μ22×ℝ×ℝ,(z0,z1,z2)↦(12​(|z1|2−|z0|2),12​(|z2|2−|z0|2),Im​(z0​z1​z2),Re​(z0​z1​z2))\begin{split}&\pi_{\mathbb{C}^{3}}:\mathbb{C}^{3}\to\mathbb{R}^{2}_{\mu_{1},\mu_{2}}\times\mathbb{R}\times\mathbb{R},\\ &(z_{0},z_{1},z_{2})\mapsto\left(\frac{1}{2}(|z_{1}|^{2}-|z_{0}|^{2}),\frac{1}{2}(|z_{2}|^{2}-|z_{0}|^{2}),\text{Im}(z_{0}z_{1}z_{2}),\text{Re}(z_{0}z_{1}z_{2})\right)\end{split}

whose discriminant locus is compatible with 𝔇\mathfrak{D}.

By construction M+M^{+} fibres over BB with generic fibre T3T^{3}. The singular fibre over 0∈B0\in B has the topology of T3T^{3} with T2T^{2} collapsed to a point, so has Betti numbers (b1,b2)=(1,2)(b_{1},b_{2})=(1,2) and Euler characteristic +1+1 (hence the name ‘positive vertex’). A basis of H1​(T3)H_{1}(T^{3}) is given by e1,e2∈H1​(T2)⊂H1​(T3)e_{1},e_{2}\in H_{1}(T^{2})\subset H_{1}(T^{3}) and an S1S^{1}-cycle e0e_{0} on the total space lifting the cycle S1⊂B×S1S^{1}\subset B\times S^{1}. The monodromies around the 3 edges 𝔇1\mathfrak{D}_{1}, 𝔇2\mathfrak{D}_{2}, 𝔇3\mathfrak{D}_{3} acting on H1​(T3)H_{1}(T^{3}) are given in the basis e0,e1,e2e_{0},e_{1},e_{2} as

[100110001],[100010−101], and ​[100−110101].\begin{bmatrix}1&0&0\\ 1&1&0\\ 0&0&1\end{bmatrix},\quad\begin{bmatrix}1&0&0\\ 0&1&0\\ -1&0&1\end{bmatrix},\text{ and }\begin{bmatrix}1&0&0\\ -1&1&0\\ 1&0&1\end{bmatrix}.

1.1.4. Negative vertices

We recount here the historical perspective of Gross and Ruan on negative vertices, to be modified in Section 1.1.5. Let 𝔇⊂B\mathfrak{D}\subset B be a graph with one vertex emitting 3 edges. Topologically, we present 𝔇\mathfrak{D} as

𝔇=𝔇1∪𝔇2∪𝔇3∪{0}={y1=0,y2>0}∪{y2=0,y1>0}∪{y1=y2<0}∪{0}⊂ℝy1,y22×{0}⊂ℝ2×ℝ=B.\begin{split}\mathfrak{D}&=\mathfrak{D}_{1}\cup\mathfrak{D}_{2}\cup\mathfrak{D}_{3}\cup\{0\}=\{y_{1}=0,y_{2}>0\}\cup\{y_{2}=0,y_{1}>0\}\cup\{y_{1}=y_{2}<0\}\cup\{0\}\\ &\subset\mathbb{R}^{2}_{y_{1},y_{2}}\times\{0\}\subset\mathbb{R}^{2}\times\mathbb{R}=B.\end{split}

Let e1,e2e_{1},e_{2} be a basis of H1​(T2,ℤ)H_{1}(T^{2},\mathbb{Z}). Let S⊂B×T2S\subset B\times T^{2} be a ‘pair of pants’ (namely a surface homeomorphic to the complement of 3 points in S2S^{2}) sitting over 𝔇⊂B\mathfrak{D}\subset B, such that S∩(𝔇i×T2)S\cap(\mathfrak{D}_{i}\times T^{2}) is a cylinder 𝔇i×S1\mathfrak{D}_{i}\times S^{1}, where the S1S^{1} factor inside T2T^{2} has homology class e2,e1,−e1−e2e_{2},e_{1},-e_{1}-e_{2} for i=1,2,3i=1,2,3 respectively. The fact that these 3 classes add up to zero means the 3 cylinders 𝔇i×S1\mathfrak{D}_{i}\times S^{1} can be joined together over {0}×T2\{0\}\times T^{2}. The fibre of S→𝔇S\to\mathfrak{D} over 0∈𝔇0\in\mathfrak{D} is a ‘figure 8 diagram’.

Then the total space M−M^{-} is built as a singular S1S^{1}-bundle over B×T2B\times T^{2}, which restricts to a principal S1S^{1}-bundle over the complement of the codimension 3 locus S⊂B×T2S\subset B\times T^{2}, and along SS the S1S^{1}-fibres collapse to points. The first Chern class of the S1S^{1}-bundle evaluates trivially on T2⊂B×T2T^{2}\subset B\times T^{2} but nontrivially on the S2S^{2}-cycle wrapping SS. In the 3 transverse directions, the S1S^{1} fibration is modelled topologically on (1.1).

By construction M−M^{-} fibres over BB with generic fibre T3T^{3}, where T3T^{3} itself is an S1S^{1}-bundle over T2T^{2}. The class of this S1⊂T3S^{1}\subset T^{3} is denoted e3e_{3}. The singular fibre of M−→BM^{-}\to B over 0∈B0\in B is obtained by taking the bundle T3→T2T^{3}\to T^{2}, and collapse down its S1S^{1}-fibres over a ‘figure 8 diagram’ inside T2T^{2}. This singular fibre has Betti numbers (b1,b2)=(2,1)(b_{1},b_{2})=(2,1) and Euler characteristic −1-1 (hence the name ‘negative vertex’). The homology classes e1,e2e_{1},e_{2} lift to H1​(T3)H_{1}(T^{3}). The monodromies around the edges 𝔇1,𝔇2,𝔇3\mathfrak{D}_{1},\mathfrak{D}_{2},\mathfrak{D}_{3} acting on H1​(T3,ℤ)H_{1}(T^{3},\mathbb{Z}) are given in the basis e1,e2,e3e_{1},e_{2},e_{3} of H1​(T3,ℤ)H_{1}(T^{3},\mathbb{Z}) as

[100010101],[1000100−11], and ​[100010−111].\begin{bmatrix}1&0&0\\ 0&1&0\\ 1&0&1\end{bmatrix},\quad\begin{bmatrix}1&0&0\\ 0&1&0\\ 0&-1&1\end{bmatrix},\text{ and }\begin{bmatrix}1&0&0\\ 0&1&0\\ -1&1&1\end{bmatrix}.

1.1.5. Joyce’s critique

Joyce [14] gave reasons that the above topological picture of Gross-Ruan cannot literally describe a special Lagrangian fibration in a generic Calabi-Yau 3-fold, based on his study of local U⁡(1)U(1)-invariant special Lagrangian submanifolds inside ℂ3\mathbb{C}^{3}. Joyce’s critique hinges on two geometric observations:

  • •

    Special Lagrangian fibrations need not be defined by a smooth map, and the discriminant locus needs not have codimension 2.

  • •

    The I1×S1I_{1}\times S^{1} singular fibres have non-isolated special Lagrangian singularities, which is an infinite codimensional phenomenon in the parameter space, namely the singularity structure cannot persist under almost any perturbation of the Kähler structure or the boundary data of the special Lagrangian.

Furthermore, in the U⁡(1)U(1)-invariant setting, Joyce constructed examples illustrating the possibility that fibres with I1×S1I_{1}\times S^{1} singularities can break up into fibres with a pair of special Lagrangian T2T^{2} cones. Such fibres lie over a thickened version of the original edges in 𝔇\mathfrak{D}, and in particular the discriminant locus of the SYZ fibration now has codimension 1.

As suggested by Morrison [22] this thickening picture is linked to the description of the negative vertex (Section 1.1.4) as follows. We can view B×T2B\times T^{2} as (ℂ∗)z1,z22×ℝ≃ℝ2×ℝ×T2(\mathbb{C}^{*})_{z_{1},z_{2}}^{2}\times\mathbb{R}\simeq\mathbb{R}^{2}\times\mathbb{R}\times T^{2}. The ‘pair of pants’ SS is realised topologically by

{z1+z2=1}⊂(ℂ∗)z1,z22=(ℂ∗)2×{0}⊂(ℂ∗)2×ℝ.\{z_{1}+z_{2}=1\}\subset(\mathbb{C}^{*})_{z_{1},z_{2}}^{2}=(\mathbb{C}^{*})^{2}\times\{0\}\subset(\mathbb{C}^{*})^{2}\times\mathbb{R}.

The algebraic 2-torus (ℂ∗)2(\mathbb{C}^{*})^{2} maps to ℝy1,y22\mathbb{R}^{2}_{y_{1},y_{2}} via

y1=−12​π​log⁡|z1|,y2=−12​π​log⁡|z2|.y_{1}=-\frac{1}{2\pi}\log|z_{1}|,\quad y_{2}=-\frac{1}{2\pi}\log|z_{2}|.

The image of SS in ℝy1,y22\mathbb{R}^{2}_{y_{1},y_{2}} under this map is an amoeba which can be thought as a thickend version of 𝔇⊂ℝy1,y22\mathfrak{D}\subset\mathbb{R}^{2}_{y_{1},y_{2}}. Along the 3 directions defined by 𝔇\mathfrak{D}, the asymptotic geometry of SS near infinity approaches 3 cylinders. In the modified construction M−M^{-} is a singular S1S^{1}-bundle over (ℂ∗)2×ℝ(\mathbb{C}^{*})^{2}\times\mathbb{R} whose fibres collapse to points along the codimension 3 locus S⊂(ℂ∗)2×ℝS\subset(\mathbb{C}^{*})^{2}\times\mathbb{R}. The natural smooth map M−→(ℂ∗)2×ℝ→B=ℝy1,y22×ℝM^{-}\to(\mathbb{C}^{*})^{2}\times\mathbb{R}\to B=\mathbb{R}^{2}_{y_{1},y_{2}}\times\mathbb{R} cannot be exactly a special Lagrangian fibration since its discriminant locus is of codimension 1, but it is still possible to be an approximate special Lagrangian fibration.

We also wish to resolve a paradox here in advance. Part of our plan is to construct a family of T2T^{2}-symmetric Ooguri-Vafa type Calabi-Yau metrics on the positive vertex, which admit a special Lagrangian fibration with all the topological features predicted by Gross and Ruan, and in particular the singular fibres will have non-isolated singularities. We emphasize there is no contradiction with Joyce’s critique: it is possible for the Ooguri-Vafa type metrics to be a good metric model for a generic Calabi-Yau 3-fold near the large complex structure limit, while the singularity structure of the SYZ fibration changes drastically. Joyce’s critique does not rule out the Gross-Ruan picture as a limiting description of SYZ fibrations.

1.1.6. Degenerating toric Calabi-Yau hypersurfaces

A familiar picture from Riemann surface theory is that higher genus algebraic curves can be obtained topologically by patching together ‘pairs of pants’ along cylindrical necks. There is a similar picture for Calabi-Yau toric hypersurfaces approaching a large complex structure limit, well studied in tropical geometry. The discussions below are loosely based on Zharkov [32][31], and are included to predict the holomorphic structure of the positive and the negative vertices.

Let ℙ△\mathbb{P}_{\triangle} be a toric manifold whose moment polytope is the reflexive integral polytope △\triangle in ℝ4\mathbb{R}^{4}, so the integral points v∈△v\in\triangle correspond to a basis {sv}\{s_{v}\} for anticanonical sections. Let λ\lambda be a (suitably generic) function on △∩ℤ4\triangle\cap\mathbb{Z}^{4} whose piecewise linear extension is a convex function on ℝ4\mathbb{R}^{4} minimized at 0∈△0\in\triangle with minimum value 0. We consider a polarised family of hypersurfaces XtX_{t} defined by

(1.4) s0+∑v∈△∖{0}tλ⁡(v)​av​sv=0,s_{0}+\sum_{v\in\triangle\setminus\{0\}}t^{\lambda(v)}a_{v}s_{v}=0,

where ava_{v} are fixed nonzero complex numbers and tt is a small positive parameter. The holomorphic volume form is determined from the adjunction formula.

The key point is that when tt is very small, the hypersurface XtX_{t} decompose into a finite number of regions, on each of which only a small number of monomial functions svs0\frac{s_{v}}{s_{0}} dominate the rest. Thus up to scaling coordinates by powers of tt, there are only a small number of complex geometric local models, typically with some torus symmetry. Furthermore there is some combinatorial structure which controls how these local models patch together to give XtX_{t} as a complex manifold.

Example 1.1.

(Generic region) Suppose in some region only s0s_{0} and tλ⁡(v)​av​svt^{\lambda(v)}a_{v}s_{v} dominate, so the hypersurface locally looks like svs0=const\frac{s_{v}}{s_{0}}=\text{const}. After normalising by powers of tt we may write this as {z0=1}\{z_{0}=1\} in the coordinates z0,z1,z2,z3z_{0},z_{1},z_{2},z_{3} on the algebraic torus (ℂ∗)4(\mathbb{C}^{*})^{4}. This model has T3T^{3}-symmetry under the diagonal action on z1,z2,z3z_{1},z_{2},z_{3}. The T3T^{3}-orbits are the natural candidate for approximate SYZ fibres. Thus we naturally look for a Kähler metric with potential ϕ=ϕ⁡(u1,u2,u3)\phi=\phi(u_{1},u_{2},u_{3}) depending only on the logarithms u1=log⁡|z1|,u2=log⁡|z2|,u3=log⁡|z3|u_{1}=\log|z_{1}|,u_{2}=\log|z_{2}|,u_{3}=\log|z_{3}|. The holomorphic volume form Ω\Omega on the hypersurface is up to a scale factor given by

d​z0z0∧d​z1z1∧d​z2z2∧d​z3z3=d⁡(z0−1)∧Ω,\frac{dz_{0}}{z_{0}}\wedge\frac{dz_{1}}{z_{1}}\wedge\frac{dz_{2}}{z_{2}}\wedge\frac{dz_{3}}{z_{3}}=d(z_{0}-1)\wedge\Omega,

namely Ω=d​z1z1∧d​z2z2∧d​z3z3=d​log⁡z1∧d​log⁡z2∧d​log⁡z3\Omega=\frac{dz_{1}}{z_{1}}\wedge\frac{dz_{2}}{z_{2}}\wedge\frac{dz_{3}}{z_{3}}=d\log z_{1}\wedge d\log z_{2}\wedge d\log z_{3}. The complex Monge-Ampère equation (−1​∂∂¯​ϕ)3=const​−1​Ω∧Ω¯(\sqrt{-1}\partial\bar{\partial}\phi)^{3}=\text{const}\sqrt{-1}\Omega\wedge\overline{\Omega} naturally reduces to the real Monge-Ampère equation det(∂2ϕ∂ui​∂uj)=const\det(\frac{\partial^{2}\phi}{\partial u_{i}\partial u_{j}})=\text{const}. One can further calculate that such regions take up most of the volume measure on XtX_{t}, thus lending some evidence for the SYZ conjecture. We remark that the description only applies to local regions so the metrics are not complete.

Example 1.2.

The real Monge-Ampère equation governs also the region near the intersection of XtX_{t} with a smooth component of the toric boundary. Suppose after normalising by powers of tt, the dominant monomials are z0−1,z0−1​z1,z0−1​z2,z0−1​z3,1z_{0}^{-1},z_{0}^{-1}z_{1},z_{0}^{-1}z_{2},z_{0}^{-1}z_{3},1 in the coordinates z0,z1,z2,z3z_{0},z_{1},z_{2},z_{3} on the algebraic torus (ℂ∗)4(\mathbb{C}^{*})^{4}, so the hypersurface has the local complex geometric model {z0−1(1+z1+z2+z3)+1=0}⊂(ℂ∗)4\{z_{0}^{-1}(1+z_{1}+z_{2}+z_{3})+1=0\}\subset(\mathbb{C}^{*})^{4}, or equivalently −z0=1+z1+z2+z3-z_{0}=1+z_{1}+z_{2}+z_{3}. The adjunction formula

d​z0z0∧d​z1z1∧d​z2z2∧d​z3z3=d⁡(z0−1​(1+z1+z2+z3)+1)∧Ω\frac{dz_{0}}{z_{0}}\wedge\frac{dz_{1}}{z_{1}}\wedge\frac{dz_{2}}{z_{2}}\wedge\frac{dz_{3}}{z_{3}}=d(z_{0}^{-1}(1+z_{1}+z_{2}+z_{3})+1)\wedge\Omega

leads to Ω=d​z1z1∧d​z2z2∧d​z3z3\Omega=\frac{dz_{1}}{z_{1}}\wedge\frac{dz_{2}}{z_{2}}\wedge\frac{dz_{3}}{z_{3}} as before. The diagonal T3T^{3}-action on z1,z2,z3z_{1},z_{2},z_{3} provides the candidate for an approximate SYZ fibration, and a solution to the real Monge-Ampère equation in the log⁡|z1|,log⁡|z2|,log⁡|z3|\log|z_{1}|,\log|z_{2}|,\log|z_{3}| coordinates induces a local Calabi-Yau metric.

Example 1.3.

Suppose after normalising by powers of tt, the dominant monomials are (z1​z2)−1,−(z1​z2)−1​z3,−1(z_{1}z_{2})^{-1},-(z_{1}z_{2})^{-1}z_{3},-1, so the hypersurface admits the local complex geometric model {(z1z2)−1(1−z3)=1}⊂(ℂ∗)z0,z1,z2,z34\{(z_{1}z_{2})^{-1}(1-z_{3})=1\}\subset(\mathbb{C}^{*})^{4}_{z_{0},z_{1},z_{2},z_{3}}, or equivalently z1​z2=1−z3z_{1}z_{2}=1-z_{3}. This happens near the intersection of two smooth components of the toric boundary. Up to numerical factors, the holomorphic volume form is given by

d​z0z0∧d​z1z1∧d​z2z2∧d​z3z3=d⁡((z1​z2)−1​(1−z3)−1)∧Ω,\frac{dz_{0}}{z_{0}}\wedge\frac{dz_{1}}{z_{1}}\wedge\frac{dz_{2}}{z_{2}}\wedge\frac{dz_{3}}{z_{3}}=d((z_{1}z_{2})^{-1}(1-z_{3})-1)\wedge\Omega,

namely Ω=d​log⁡z0∧d​z1∧d​z2z3\Omega=d\log z_{0}\wedge\frac{dz_{1}\wedge dz_{2}}{z_{3}}. This model has a natural T2T^{2}-symmetry: one S1S^{1} acts trivially on z1,z2,z3z_{1},z_{2},z_{3} and rotates z0z_{0}, while the other S1S^{1} acts trivially on z0,z3z_{0},z_{3} and diagonally on z1,z2z_{1},z_{2}. The model is intimately related to the Ooguri-Vafa metric (cf. Section 1.3.2), and we expect this region to coincide with the neighbourhood of edges in the Gross-Ruan-Joyce picture.

In this paper we are primarily interested in the positive and negative vertices. These are relevant for certain regions near the intersection of XtX_{t} with some higher depth strata of the toric boundary of ℙ△\mathbb{P}_{\triangle}.

Example 1.4.

The positive vertex M+M^{+} describes a neighbourhood of the point (0,0,0,1)(0,0,0,1) inside {z0z1z2=1−z3}⊂ℂ3×ℂz3∗\{z_{0}z_{1}z_{2}=1-z_{3}\}\subset\mathbb{C}^{3}\times\mathbb{C}^{*}_{z_{3}}. In the toric hypersurface picture, we are looking at a region where the dominating monomials are up to scale factors (z0​z1​z2)−1,−z3​(z0​z1​z2)−1,1(z_{0}z_{1}z_{2})^{-1},-z_{3}(z_{0}z_{1}z_{2})^{-1},1, so the defining equation of XtX_{t} is approximately (z0​z1​z2)−1​(1−z3)=1(z_{0}z_{1}z_{2})^{-1}(1-z_{3})=1 once we absorb the scale factors into ziz_{i}. The holomorphic volume form Ω\Omega is up to constant given by

−−12​π​d​log​z0∧d​log​z1∧d​log​z2∧d​log​z3=d⁡((z0​z1​z2)−1​(1−z3)−1)∧Ω,-\frac{\sqrt{-1}}{2\pi}d\log z_{0}\wedge d\log z_{1}\wedge d\log z_{2}\wedge d\log z_{3}=d((z_{0}z_{1}z_{2})^{-1}(1-z_{3})-1)\wedge\Omega,

or equivalently Ω=−−12​π​1z3​d​z0∧d​z1∧d​z2\Omega=-\frac{\sqrt{-1}}{2\pi}\frac{1}{z_{3}}dz_{0}\wedge dz_{1}\wedge dz_{2}. An important feature of this model is the diagonal T2T^{2}-symmetry:

ei​θ1⋅(z0,z1,z2)=(e−i​θ1​z0,ei​θ1​z1,z2),ei​θ2⋅(z0,z1,z2)=(e−i​θ2​z0,z1,ei​θ2​z2).e^{i\theta_{1}}\cdot(z_{0},z_{1},z_{2})=(e^{-i\theta_{1}}z_{0},e^{i\theta_{1}}z_{1},z_{2}),\quad e^{i\theta_{2}}\cdot(z_{0},z_{1},z_{2})=(e^{-i\theta_{2}}z_{0},z_{1},e^{i\theta_{2}}z_{2}).

We have Ω(∂∂θ1,∂∂θ2,⋅)=−−12​πdlogz3=dη\Omega(\frac{\partial}{\partial\theta_{1}},\frac{\partial}{\partial\theta_{2}},\cdot)=-\frac{\sqrt{-1}}{2\pi}d\log z_{3}=d\eta, where η=−−12​π​log⁡(z3)\eta=-\frac{\sqrt{-1}}{2\pi}\log(z_{3}) is a holomorphic coordinate with period 1, and takes the value zero at z0=z1=z2=0z_{0}=z_{1}=z_{2}=0. The relation between this complex geometric perspective and the topological picture in Section 1.1.3 is perhaps clearest with the generalised Gibbons-Hawking construction in mind (cf. Section 1.2 below). Essentially M+M^{+} is a singular T2T^{2}-bundle over a 4-dimensional base contained in ℝμ1,μ22×(S1×ℝ)η\mathbb{R}^{2}_{\mu_{1},\mu_{2}}\times(S^{1}\times\mathbb{R})_{\eta}, where μ1,μ2\mu_{1},\mu_{2} are the T2T^{2}-moment maps normalised to have value 0 at z0=z1=z2=0z_{0}=z_{1}=z_{2}=0. We shall notice that the discriminant locus 𝔇×{0}\mathfrak{D}\times\{0\} of this singular T2T^{2}-bundle is not sensitive to the choice of the Kähler form (cf. Lemma 1.6 and its ensuing Remark). The normalising constant on Ω\Omega imply that the SYZ T3T^{3}-fibres have ∫T3Ω=4​π2\int_{T^{3}}\Omega=4\pi^{2}.

Example 1.5.

The negative vertex M−M^{-} describes an open subset inside {z3z4=1−z1−z2}⊂ℂz1∗×ℂz2∗×ℂz3,z42\{z_{3}z_{4}=1-z_{1}-z_{2}\}\subset\mathbb{C}^{*}_{z_{1}}\times\mathbb{C}^{*}_{z_{2}}\times\mathbb{C}^{2}_{z_{3},z_{4}}. In the toric hypersurface picture, we are looking at a region where the dominating monomials are up to scale factors just (z3​z4)−1(z_{3}z_{4})^{-1}, z1​(z3​z4)−1z_{1}(z_{3}z_{4})^{-1}, z2​(z3​z4)−1z_{2}(z_{3}z_{4})^{-1} and 1, so the defining equation of XtX_{t} is approximately (1−z1−z2)​(z3​z4)−1−1=0(1-z_{1}-z_{2})(z_{3}z_{4})^{-1}-1=0 once we absorb the scale factors into ziz_{i}. The holomorphic volume form Ω\Omega is given up to constant by

−14​π2​d​log​z1∧d​log​z2∧d​log​z3∧d​log​z4=d⁡((1−z1−z2)​(z3​z4)−1−1)∧Ω,\frac{\sqrt{-1}}{4\pi^{2}}d\log z_{1}\wedge d\log z_{2}\wedge d\log z_{3}\wedge d\log z_{4}=d\left((1-z_{1}-z_{2})(z_{3}z_{4})^{-1}-1\right)\wedge\Omega,

or equivalently Ω=−−14​π2​1z1​z2​d​z2∧d​z3∧d​z4.\Omega=\frac{-\sqrt{-1}}{4\pi^{2}}\frac{1}{z_{1}z_{2}}dz_{2}\wedge dz_{3}\wedge dz_{4}. This model has S1S^{1}-symmetry:

ei​θ⋅(z1,z2,z3,z4)=(z1,z2,ei​θ​z3,e−i​θ​z4).e^{i\theta}\cdot(z_{1},z_{2},z_{3},z_{4})=(z_{1},z_{2},e^{i\theta}z_{3},e^{-i\theta}z_{4}).

Hence M−M^{-} is a singular S1S^{1}-bundle over ℝμ×ℂz1∗×ℂz2∗\mathbb{R}_{\mu}\times\mathbb{C}^{*}_{z_{1}}\times\mathbb{C}^{*}_{z_{2}}, where μ\mu is the S1S^{1}-moment coordinate which takes the value zero on the singular locus {z3=z4=0}\{z_{3}=z_{4}=0\} (notice that the degeneracy of the S1S^{1} factor implies that the moment map is constant on this singular locus for any choice of Kähler form). This agrees with the modified topological description in Section 1.1.5. We calculate

ι∂∂θ​Ω=−14​π2​d​log⁡z1∧d​log⁡z2=d​η1∧d​η2,\iota_{\frac{\partial}{\partial\theta}}\Omega=-\frac{1}{4\pi^{2}}d\log z_{1}\wedge d\log z_{2}=d\eta_{1}\wedge d\eta_{2},

where the logarithmic coordinates ηp=12​π​−1​log⁡zp\eta_{p}=\frac{1}{2\pi\sqrt{-1}}\log z_{p} for p=1,2p=1,2 have period 1. The arg⁡z1,arg⁡z2\arg z_{1},\arg z_{2} coordinates provide a family of 2-tori in ℝ×ℂz1∗×ℂz2∗\mathbb{R}\times\mathbb{C}^{*}_{z_{1}}\times\mathbb{C}^{*}_{z_{2}}, and the restriction of the S1S^{1}-bundle over these 2-tori defines a family of 3-tori. The normalising constant on Ω\Omega imply that ∫T3Ω=2​π\int_{T^{3}}\Omega=2\pi.

1.2. Generalised Gibbons-Hawking ansatz

The materials in this Section draws heavily from the presentation of Zharkov [31]. Suppose MM is a complex NN-dimensional Kähler manifold with a nonvanishing holomorphic volume form admitting a holomorphic isometric free T𝔫T^{\mathfrak{n}} action. The generalised Gibbons-Hawking ansatz expresses the Kähler and Calabi-Yau conditions in terms of the 𝔫\mathfrak{n} moment map coordinates and the N−𝔫N-\mathfrak{n} holomorphic coordinates on the Kähler quotient.

Let 𝔱\mathfrak{t} denote the Lie algebra of T𝔫T^{\mathfrak{n}}, and let 𝔱ℤ\mathfrak{t}_{\mathbb{Z}} be the natural integral lattice in 𝔱\mathfrak{t}. A choice of basis in 𝔱ℤ\mathfrak{t}_{\mathbb{Z}} defines linear coordinates μi\mu_{i} on the dual space 𝔱∗≃ℝ𝔫\mathfrak{t}^{*}\simeq\mathbb{R}^{\mathfrak{n}}. Let YY be either ℂN−𝔫\mathbb{C}^{N-\mathfrak{n}} or (ℂ∗)N−𝔫(\mathbb{C}^{*})^{N-\mathfrak{n}}, and let ηp\eta_{p} denote the standard complex coordinates on ℂN−𝔫\mathbb{C}^{N-\mathfrak{n}} or the logarithmic coordinates on (ℂ∗)N−𝔫(\mathbb{C}^{*})^{N-\mathfrak{n}} with period 1 (in which case e2​π​i​ηpe^{2\pi i\eta_{p}} are the standard coordinates on (ℂ∗)N−𝔫(\mathbb{C}^{*})^{N-\mathfrak{n}}). Consider a principal T𝔫T^{\mathfrak{n}}-bundle π:M→ℬ0\pi:M\to\mathcal{B}^{0} over an open set ℬ0\mathcal{B}^{0} in 𝔱∗×Y\mathfrak{t}^{*}\times Y, whose first Chern class is an element c1∈H2​(ℬ0,𝔱ℤ)c_{1}\in H^{2}(\mathcal{B}^{0},\mathfrak{t}_{\mathbb{Z}}). Later we will partially compactify MM into a singular T𝔫T^{\mathfrak{n}}-bundle. Summation convention will be used throughout.

Theorem 1.5.

(cf. Theorem 2.1 in [31]) Let Vi​jV^{ij}, respectively Wp​q¯W^{p\bar{q}}, be real symmetric positive definite/Hermitian matrices of smooth functions on ℬ0\mathcal{B}^{0}, locally given by some potential function Φ\Phi:

(1.5) Vi​j=∂2Φ∂μi​∂μj,Wp​q¯=−4​∂2Φ∂ηp​∂η¯q,1≤i,j≤𝔫,1≤p,q≤N−𝔫.V^{ij}=\frac{\partial^{2}\Phi}{\partial\mu_{i}\partial\mu_{j}},\quad W^{p\bar{q}}=-4\frac{\partial^{2}\Phi}{\partial\eta_{p}\partial\bar{\eta}_{q}},\quad 1\leq i,j\leq\mathfrak{n},\quad 1\leq p,q\leq N-\mathfrak{n}.

Then the following 𝔱\mathfrak{t}-valued real 2-form is closed:

(1.6) Fj=−1​(12​∂Wp​q¯∂μj​d​ηp∧d​η¯q+∂Vi​j∂ηp​d​μi∧d​ηp−∂Vi​j∂η¯q​d​μi∧d​η¯q).F_{j}=\sqrt{-1}\left(\frac{1}{2}\frac{\partial W^{p\bar{q}}}{\partial\mu_{j}}d\eta_{p}\wedge d\bar{\eta}_{q}+\frac{\partial V^{ij}}{\partial\eta_{p}}d\mu_{i}\wedge d\eta_{p}-\frac{\partial V^{ij}}{\partial\bar{\eta}_{q}}d\mu_{i}\wedge d\bar{\eta}_{q}\right).

Suppose further that 12​π​(F1,…,F𝔫)\frac{1}{2\pi}(F_{1},\ldots,F_{\mathfrak{n}}) is in the cohomology class c1∈H2​(ℬ0,𝔱ℤ)c_{1}\in H^{2}(\mathcal{B}^{0},\mathfrak{t}_{\mathbb{Z}}). Then there exists a connection ϑ\vartheta on the principal bundle M→ℬ0M\to\mathcal{B}^{0} with curvature d​ϑi=Fid\vartheta_{i}=F_{i} for i=1,…,𝔫i=1,\ldots,\mathfrak{n}, such that MM is a Kähler manifold with metric tensor

(1.7) h=(V−1)i​j​ζi⊗ζ¯j+Wp​q¯​d​ηp⊗d​η¯q,ω=d​μj∧ϑj+−12​Wp​q¯​d​ηp∧d​η¯q,h=(V^{-1})^{ij}\zeta_{i}\otimes\bar{\zeta}_{j}+W^{p\bar{q}}d\eta_{p}\otimes d\bar{\eta}_{q},\quad\omega=d\mu_{j}\wedge\vartheta_{j}+\frac{\sqrt{-1}}{2}W^{p\bar{q}}d\eta_{p}\wedge d\bar{\eta}_{q},

where ζj=Vi​j​d​μi+−1​ϑj\zeta_{j}=V^{ij}d\mu_{i}+\sqrt{-1}\vartheta_{j} and ηp\eta_{p} form a basis of type (1,0) forms which defines an integrable complex structure. There is a nowhere vanishing holomorphic form on MM:

(1.8) Ω=∧j=1𝔫(−−1ζj)⋀∧p=1N−𝔫dηp.\Omega=\wedge_{j=1}^{\mathfrak{n}}(-\sqrt{-1}\zeta_{j})\bigwedge\wedge_{p=1}^{N-\mathfrak{n}}d\eta_{p}.

The Calabi-Yau condition ωN=N!2N​−1N2​Ω∧Ω¯\omega^{N}=\frac{N!}{2^{N}}\sqrt{-1}^{N^{2}}\Omega\wedge\overline{\Omega} is equivalent to the equation

(1.9) det(Vi​j)=det(Wp​q¯).\det(V^{ij})=\det(W^{p\bar{q}}).
Remark 1.5.

The inverse matrix (V−1)i​j(V^{-1})^{ij} describes the metric restricted to the torus fibres, and the matrix Wp​q¯W^{p\bar{q}} describes the metric induced on the Kähler quotients. This viewpoint is taken by Pedersen and Poon [23], whose argument shows that Calabi-Yau manifolds with Hamiltonian torus symmetries necessarily arise from this construction locally. The local existence of the potential Φ\Phi is equivalent to the linear integrability condition

(1.10) ∂Vi​j∂μk=∂Vi​k∂μj,∂Wp​q¯∂ηr=∂Wr​q∂ηp,∂Wp​r∂η¯q=∂Wp​q¯∂η¯r,\frac{\partial V^{ij}}{\partial\mu_{k}}=\frac{\partial V^{ik}}{\partial\mu_{j}},\quad\frac{\partial W^{p\bar{q}}}{\partial\eta_{r}}=\frac{\partial W^{rq}}{\partial\eta_{p}},\quad\frac{\partial W^{pr}}{\partial\bar{\eta}_{q}}=\frac{\partial W^{p\bar{q}}}{\partial\bar{\eta}_{r}},

and

(1.11) ∂2Wp​q¯∂μi​∂μj+4​∂2Vi​j∂ηp​∂η¯q=0.\frac{\partial^{2}W^{p\bar{q}}}{\partial\mu_{i}\partial\mu_{j}}+4\frac{\partial^{2}V^{ij}}{\partial\eta_{p}\partial\bar{\eta}_{q}}=0.

In particular when N=2,𝔫=1N=2,\mathfrak{n}=1, the Calabi-Yau condition is V=WV=W and we recover the usual Gibbons-Hawking equation from (1.11).

Proof.

(Theorem 1.5, sketch) By formula (1.6) and the integrability condition (1.10),

(1.12) d​Fj=−12​(∂2Wp​q¯∂μi​∂μj+4​∂2Vi​j∂ηp​∂η¯q)​d​μi∧d​ηp∧d​η¯q,dF_{j}=\frac{\sqrt{-1}}{2}\left(\frac{\partial^{2}W^{p\bar{q}}}{\partial\mu_{i}\partial\mu_{j}}+4\frac{\partial^{2}V^{ij}}{\partial\eta_{p}\partial\bar{\eta}_{q}}\right)d\mu_{i}\wedge d\eta_{p}\wedge d\bar{\eta}_{q},

so the closedness of FjF_{j} is equivalent to (1.11). Since 12​π​F\frac{1}{2\pi}F represents the appropriate first Chern class, FF must be the curvature of a T𝔫T^{\mathfrak{n}}-connection ϑ\vartheta. Modulo gauge ϑ\vartheta admits the local formula

(1.13) ϑj=−1​{∂2Φ∂ηp​∂μ​d​ηp−∂2Φ∂η¯p​∂μ​d​η¯p}.\vartheta_{j}=\sqrt{-1}\{\frac{\partial^{2}\Phi}{\partial\eta_{p}\partial\mu}d\eta_{p}-\frac{\partial^{2}\Phi}{\partial\bar{\eta}_{p}\partial\mu}d\bar{\eta}_{p}\}.

Gauge equivalent choices of the connection define the structures on MM up to holomorphic isometry.

The integrability of the complex structure follows from the fact that the differential ideal generated by (1,0)(1,0) forms is closed:

(1.14) d​ζj=(12​∂Wp​q¯∂μj​d​η¯q−2​∂Vi​j∂ηp​d​μi)∧d​ηp,d\zeta_{j}=\left(\frac{1}{2}\frac{\partial W^{p\bar{q}}}{\partial\mu_{j}}d\bar{\eta}_{q}-2\frac{\partial V^{ij}}{\partial\eta_{p}}d\mu_{i}\right)\wedge d\eta_{p},

using (1.10)(1.6) and the definition of ζj\zeta_{j}. The Kähler condition d​ω=0d\omega=0 follows from (1.10)(1.6). The Calabi-Yau condition follows from the more general formula

ωN=det(Wp​q¯)​det(Vi​j)−1​N!2N​−1N2​Ω∧Ω¯.\omega^{N}=\det(W^{p\bar{q}})\det(V^{ij})^{-1}\frac{N!}{2^{N}}\sqrt{-1}^{N^{2}}\Omega\wedge\overline{\Omega}.

∎

Remark 1.6.

If ∂∂θj\frac{\partial}{\partial\theta_{j}} are the Hamiltonian vector fields dual to ϑi\vartheta_{i}, namely ϑi​(∂∂θj)=δi​j\vartheta_{i}(\frac{\partial}{\partial\theta_{j}})=\delta_{ij}, then d​μi=−ι∂∂θi​ωd\mu_{i}=-\iota_{\frac{\partial}{\partial\theta_{i}}}\omega, namely μi\mu_{i} are the symplectic moment coordinates up to sign. When N−𝔫=1N-\mathfrak{n}=1, namely there is only one η\eta coordinate, then dη=Ω(∂∂θ1,…,∂∂θ𝔫,⋅)d\eta=\Omega(\frac{\partial}{\partial\theta_{1}},\ldots,\frac{\partial}{\partial\theta_{\mathfrak{n}}},\cdot), and accordingly we refer to η\eta as the holomorphic moment coordinate. In this situation MM admits a fibration

M→(μ1,…,μ𝔫,Im​(η))𝔱∗×ℝ,M\xrightarrow{(\mu_{1},\ldots,\mu_{\mathfrak{n}},\text{Im}(\eta))}\mathfrak{t}^{*}\times\mathbb{R},

where fibres are special Lagrangians with phase zero: the Lagrangian condition follows from d​μi=−ι∂∂θi​ω=0d\mu_{i}=-\iota_{\frac{\partial}{\partial\theta_{i}}}\omega=0 on fibres, while the special condition is equivalent to ImΩ(∂∂θ1,…∂∂θ𝔫,⋅)=dImη=0\text{Im}\Omega(\frac{\partial}{\partial\theta_{1}},\ldots\frac{\partial}{\partial\theta_{\mathfrak{n}}},\cdot)=d\text{Im}\eta=0.

Remark 1.7.

The information contained in the generalised Gibbons-Hawking ansatz can be encoded by a Riemannian metric on the base, written in distinguished coordinates as

(1.15) gℬ0=Vi​j​d​μi⊗d​μj+Re​(Wp​q¯​d​ηp⊗d​η¯q),g_{\mathcal{B}^{0}}=V^{ij}d\mu_{i}\otimes d\mu_{j}+\text{Re}(W^{p\bar{q}}d\eta_{p}\otimes d\bar{\eta}_{q}),

such that the map M→ℬ0M\to\mathcal{B}^{0} is a Riemannian submersion.

Remark 1.8.

There is an additional freedom to twist the connection ϑ\vartheta by a flat connection. Up to gauge equivalence, the choice of ϑ\vartheta is parametrised by H1​(ℬ0,Tn)H^{1}(\mathcal{B}^{0},T^{n}).

1.2.1. Elementary examples

Example 1.6.

(Constant solution) The simplest solution is where Vi​jV^{ij} and Wp​q¯W^{p\bar{q}} are independent of the base variables and satisfy (1.9). We shall see that many interesting solutions can be thought heuristically as perturbation of the constant solution after introducing some topology. Some important special cases for us are:

  • •

    N=2,𝔫=1N=2,\mathfrak{n}=1, V=W=A>0V=W=A>0. The subcase where η\eta takes value in ℂ\mathbb{C} is relevant for the Taub-NUT metric (cf. Example 1.8), and the subcase where η\eta is a periodic variable is relevant for the Ooguri-Vafa metric (cf. Section 1.3). In the periodic case the choice of the connection ϑ\vartheta is parametrised by H1​(S1×ℝ2,S1)≃S1H^{1}(S^{1}\times\mathbb{R}^{2},S^{1})\simeq S^{1}.

  • •

    N=3,𝔫=2N=3,\mathfrak{n}=2, Vi​j=ai​jV^{ij}=a_{ij} is symmetric positive definite, and W=A=det(ai​j)W=A=\det(a_{ij}). We write ga=ai​j​d​μi​d​μj+A​|d​η|2g_{a}=a_{ij}d\mu_{i}d\mu_{j}+A|d\eta|^{2}. The subcase where η\eta takes value in ℂ\mathbb{C} will be relevant for constructing new Taub-NUT type Calabi-Yau metrics on ℂ3\mathbb{C}^{3}, and the subcase where η\eta is a periodic variable will be relevant for the positive vertex. In the periodic case the choice of the connection ϑ\vartheta is parametrised by H1​(S1×ℝ3,T2)≃T2H^{1}(S^{1}\times\mathbb{R}^{3},T^{2})\simeq T^{2}.

  • •

    N=3,𝔫=1N=3,\mathfrak{n}=1, Wp​q¯=ap​q¯W^{p\bar{q}}=a_{p\bar{q}} is Hermitian, and V=A=det(ap​q¯)V=A=\det(a_{p\bar{q}}). We write ga=Re​(ap​q¯​d​ηp​d​η¯q)+A​d​μ⊗d​μg_{a}=\text{Re}(a_{p\bar{q}}d\eta_{p}d\bar{\eta}_{q})+Ad\mu\otimes d\mu. Here η1,η2\eta_{1},\eta_{2} are periodic coordinates with period 1. The choice of the connection ϑ\vartheta is parametrised by H1​(T2×ℝ3,S1)≃T2H^{1}(T^{2}\times\mathbb{R}^{3},S^{1})\simeq T^{2}. This case will be relevant for the negative vertex. Notice that if we demand that the fibration on MM induced by μ,Im​(η1),Im​(η2)\mu,\text{Im}(\eta_{1}),\text{Im}(\eta_{2}) is a special Lagrangian fibration with phase zero, then we would need a1​2¯=a2​1¯a_{1\bar{2}}=a_{2\bar{1}}, namely ap​q=ap​q¯a_{pq}=a_{p\bar{q}} is symmetric.

Example 1.7.

(ℂN\mathbb{C}^{N} Harvey-Lawson example) The affine space ℂN\mathbb{C}^{N} with the standard Euclidean metric ω=−12​∑i=0N−1d​zi∧d​z¯i\omega=\frac{\sqrt{-1}}{2}\sum_{i=0}^{N-1}dz_{i}\wedge d\bar{z}_{i} and holomorphic volume form Ω=−1N−1​d​z0∧…​d​zN−1\Omega=\sqrt{-1}^{N-1}dz_{0}\wedge\ldots dz_{N-1} admits a diagonal TN−1T^{N-1}-action, where the kk-th circle factor acts by

ei​θk⋅(z0,z1,…,zN−1)=(e−i​θk​z0,z1,…,ei​θk​zk,zk+1,…,zN−1).e^{i\theta_{k}}\cdot(z_{0},z_{1},\ldots,z_{N-1})=(e^{-i\theta_{k}}z_{0},z_{1},\ldots,e^{i\theta_{k}}z_{k},z_{k+1},\ldots,z_{N-1}).

The corresponding moment coordinates are

μi=12(|zi|2−|z0|2),i=1,2,…N−1, and η=z0z1…zN−1.\mu_{i}=\frac{1}{2}(|z_{i}|^{2}-|z_{0}|^{2}),\quad i=1,2,\ldots N-1,\text{ and }\eta=z_{0}z_{1}\ldots z_{N-1}.

This defines a TN−1T^{N-1}-bundle away from the singular locus ⋃{zi=zj=0}\bigcup\{z_{i}=z_{j}=0\}. Special cases include (1.1)(1.3). The inverse matrices are

(V−1)i​j=|z0|2+δi​j​|zi|2,W−1=|z0​z1​…​zN−1|2​(1|z0|2+…+1|zN−1|2),(V^{-1})^{ij}=|z_{0}|^{2}+\delta_{ij}|z_{i}|^{2},\quad W^{-1}=|z_{0}z_{1}\ldots z_{N-1}|^{2}\left(\frac{1}{|z_{0}|^{2}}+\ldots+\frac{1}{|z_{N-1}|^{2}}\right),

viewed as functions of μi\mu_{i} and η\eta. The special Lagrangian fibration described by Remark 1.6 is the well known Harvey-Lawson example.

We notice in particular when N=3N=3 that the discriminant locus of the singular T2T^{2}-bundle is given by 𝔇⊂ℝμ1,μ22×{0}⊂ℝμ1,μ22×ℂη\mathfrak{D}\subset\mathbb{R}^{2}_{\mu_{1},\mu_{2}}\times\{0\}\subset\mathbb{R}^{2}_{\mu_{1},\mu_{2}}\times\mathbb{C}_{\eta} as in (1.2). This is not an accidental feature of the Euclidean metric:

Lemma 1.6.

Let ℂ3\mathbb{C}^{3} be equipped with the holomorphic volume form Ω\Omega above, and let ω\omega be any T2T^{2}-invariant Kähler form with infinite volume on the singular loci {zi=zj=0}\{z_{i}=z_{j}=0\} for any i,ji,j. Then the discriminant locus of the singular T2T^{2}-bundle is 𝔇⊂ℝμ1,μ22×ℂη\mathfrak{D}\subset\mathbb{R}^{2}_{\mu_{1},\mu_{2}}\times\mathbb{C}_{\eta} in moment coordinates μ1,μ2\mu_{1},\mu_{2} and η\eta.

Proof.

The discriminant locus is the image of the singular locus 𝒞i​j={zi=zj=0}\mathcal{C}_{ij}=\{z_{i}=z_{j}=0\} under the moment map. We shall focus on 𝒞01\mathcal{C}_{01}. The holomorphic moment coordinate η\eta depends only on Ω\Omega and the T2T^{2} action, so η=z0​z1​z2\eta=z_{0}z_{1}z_{2} as before and vanishes on 𝒞01\mathcal{C}_{01}. The symplectic moment coordinates are defined by d​μi=−ι∂∂θi​ωd\mu_{i}=-\iota_{\frac{\partial}{\partial\theta_{i}}}\omega, and are normalised to be zero at (z1,z2,z3)=0(z_{1},z_{2},z_{3})=0. In particular since the Hamiltonian vector field ∂∂θ1\frac{\partial}{\partial\theta_{1}} vanishes on 𝒞01\mathcal{C}_{01}, the moment μ1\mu_{1} must be the constant zero on 𝒞01\mathcal{C}_{01}. Furthermore μ2>0\mu_{2}>0 on 𝒞01\mathcal{C}_{01} by considering the weight of the remaining S1S^{1} action at the fixed point, so the image of 𝒞01\mathcal{C}_{01} is contained in 𝔇1∪{0}\mathfrak{D}_{1}\cup\{0\}. The infinite volume condition and the formula

0≤∫𝒞01∩{μ2<m}ω=−2π∫μ2=m0dμ2=2πm,∀m≥0,0\leq\int_{\mathcal{C}_{01}\cap\{\mu_{2}<m\}}\omega=-2\pi\int_{\mu_{2}=m}^{0}d\mu_{2}=2\pi m,\quad\forall m\geq 0,

ensure that μ2\mu_{2} stretches to infinity, so 𝔇1∪{0}\mathfrak{D}_{1}\cup\{0\} is the image of 𝒞01\mathcal{C}_{01}. Likewise the image of 𝒞02\mathcal{C}_{02} is 𝔇2∪{0}\mathfrak{D}_{2}\cup\{0\} and the image of 𝒞12\mathcal{C}_{12} is 𝔇3∪{0}\mathfrak{D}_{3}\cup\{0\}. ∎

Remark 1.9.

The same method shows the complex geometry of the positive vertex in Section 1.1.6 is compatible with the discriminant locus described in Section 1.1.3.

Example 1.8.

(Taub-NUT) We take N=2,𝔫=1N=2,\mathfrak{n}=1, and V=W=12​μ2+|η|2+AV=W=\frac{1}{2\sqrt{\mu^{2}+|\eta|^{2}}}+A, where AA is a positive constant. This defines a Calabi-Yau metric whose asymptotic geometry at infinity approaches the constant solution (cf. Example 1.6), with asymptotic circles of length 2​πA\frac{2\pi}{\sqrt{A}} fibred over a flat 3-dimensional base. Different choices of AA define the same metric up to scaling. The first Chern class c1c_{1} of the S1S^{1}-bundle over (ℝμ×ℂη)∖{0}(\mathbb{R}_{\mu}\times\mathbb{C}_{\eta})\setminus\{0\} evaluates to −1-1 on any sphere around the origin in ℝμ×ℂη\mathbb{R}_{\mu}\times\mathbb{C}_{\eta}; equivalently, the 3-current −12​π​d​F-\frac{1}{2\pi}dF is represented by the origin 0∈ℝμ×ℂη0\in\mathbb{R}_{\mu}\times\mathbb{C}_{\eta} viewed as a codimension 3 cycle. Written in terms of the delta function,

12​π​d​F=12​π​(∂2∂μ2+4​∂2∂η​∂η¯)​V​d​μ∧d​Re​η∧d​Im​η=−δ⁡(μ,η,η¯)​d​μ∧d​Re​η∧d​Im​η.\frac{1}{2\pi}dF=\frac{1}{2\pi}(\frac{\partial^{2}}{\partial\mu^{2}}+4\frac{\partial^{2}}{\partial\eta\partial\bar{\eta}})Vd\mu\wedge d\text{Re}\eta\wedge d\text{Im}{\eta}=-\delta(\mu,\eta,\bar{\eta})d\mu\wedge d\text{Re}\eta\wedge d\text{Im}{\eta}.

From the holomorphic perspective, LeBrun [17] observes that the Taub-NUT space is biholomorphic to ℂ2\mathbb{C}^{2}. To see this, recall ζ=V​d​μ+−1​ϑ\zeta=Vd\mu+\sqrt{-1}\vartheta and notice the (1,0) form ζ−μ2​η​μ2+|η|2​d​η\zeta-\frac{\mu}{2\eta\sqrt{\mu^{2}+|\eta|^{2}}}d\eta is closed, so locally is the differential of a holomorphic function. The line integrals

logz1=∫ζ+(12​η−μ2​η​μ2+|η|2)dη,logz0=∫−ζ+(12​η+μ2​η​μ2+|η|2)dη\log z_{1}=\int\zeta+(\frac{1}{2\eta}-\frac{\mu}{2\eta\sqrt{\mu^{2}+|\eta|^{2}}})d\eta,\quad\log z_{0}=\int-\zeta+(\frac{1}{2\eta}+\frac{\mu}{2\eta\sqrt{\mu^{2}+|\eta|^{2}}})d\eta

define holomorphic functions up to 2​π​−1​ℤ2\pi\sqrt{-1}\mathbb{Z} over the regions ℝ×ℂ∖{η=0,μ≤0}\mathbb{R}\times\mathbb{C}\setminus\{\eta=0,\mu\leq 0\} and ℝ×ℂ∖{η=0,μ≥0}\mathbb{R}\times\mathbb{C}\setminus\{\eta=0,\mu\geq 0\} respectively, so z1z_{1} and z0z_{0} are well defined over the respective regions. Since d​log⁡z1+d​log⁡z0=d​log⁡ηd\log z_{1}+d\log z_{0}=d\log\eta we can normalise z0,z1z_{0},z_{1} to satisfy the functional equation z1​z0=ηz_{1}z_{0}=\eta, whence z1z_{1} and z0z_{0} extend as global holomorphic functions. These coordinates exhibit the biholomorphism to ℂ2\mathbb{C}^{2}. By considering the Hamiltonian vector field acting on log⁡z1,log⁡z0\log z_{1},\log z_{0}, we idenitfy the S1S^{1} action as

ei​θ⋅(z1,z0)=(ei​θ​z1,e−i​θ​z0).e^{i\theta}\cdot(z_{1},z_{0})=(e^{i\theta}z_{1},e^{-i\theta}z_{0}).

The holomorphic volume form is

Ω=−−1​ζ∧d​η=−−1​d​log⁡z1∧d⁡(z1​z0)=−1​d​z0∧d​z1.\Omega=-\sqrt{-1}\zeta\wedge d\eta=-\sqrt{-1}d\log z_{1}\wedge d(z_{1}z_{0})=\sqrt{-1}dz_{0}\wedge dz_{1}.

Thus η=z0​z1\eta=z_{0}z_{1} defines holomorphic fibration of ℂ2\mathbb{C}^{2} by affine quadrics. The generic quadric fibre is topologically a cylinder, and metrically is also approaching the flat cylindrical metric near spatial infinity. When η=0\eta=0, the quadric fibre degenerates into a union of two complex lines with simple normal crossing, where each line looks metrically like a cylinder with one capped end.

1.2.2. Compactification and distributional equation

When we partially compactify the principal TnT^{n}-bundle over ℬ0\mathcal{B}^{0} to a singular T𝔫T^{\mathfrak{n}}-bundle over ℬ⊃ℬ0\mathcal{B}\supset\mathcal{B}^{0} by allowing torus fibres to degenerate, we need to encode the topology into the generalised Gibbons-Hawking ansatz, by changing the RHS of (1.11) into a distributional term reflecting the nontriviality of the first Chern class (cf. the Taub-NUT example 1.8). This has been worked out by Zharkov [31] in general dimensions; here we will focus on the vertices in N=3N=3.

Example 1.9.

(Positive vertex and Taub-NUT type ℂ3\mathbb{C}^{3}) Recall from Section 1.1.3 that e1,e2e_{1},e_{2} are the homology classes of the two circle factors in the T2T^{2}-fibre, or equivalently an integral basis in 𝔱\mathfrak{t}. The 𝔱\mathfrak{t}-valued curvature 2-form F=F1​e1+F2​e2F=F_{1}e_{1}+F_{2}e_{2} satisfies (cf. (1.12))

12​π​d​Fj⊗ej=−14​π​(∂2W∂μi​∂μj+4​∂2Vi​j∂η​∂η¯)​d​μi∧d​η∧d​η¯⊗ej,\frac{1}{2\pi}dF_{j}\otimes e_{j}=\frac{\sqrt{-1}}{4\pi}\left(\frac{\partial^{2}W}{\partial\mu_{i}\partial\mu_{j}}+4\frac{\partial^{2}V^{ij}}{\partial\eta\partial\bar{\eta}}\right)d\mu_{i}\wedge d\eta\wedge d\bar{\eta}\otimes e_{j},

which is a 𝔱\mathfrak{t}-valued 3-current supported on the codimension 3 discriminant locus 𝔇⊂ℝμ1,μ22×(S1×ℝ)η\mathfrak{D}\subset\mathbb{R}^{2}_{\mu_{1},\mu_{2}}\times(S^{1}\times\mathbb{R})_{\eta}. Now take small 3-balls transverse to 𝔇1,𝔇2,𝔇3\mathfrak{D}_{1},\mathfrak{D}_{2},\mathfrak{D}_{3} respectively. The integrals of 12​π​d​Fj⊗ej\frac{1}{2\pi}dF_{j}\otimes e_{j} over the balls are equal to the integrals of the Chern class representative 12​π​F\frac{1}{2\pi}F over the S2S^{2} linking 𝔇1,𝔇2,𝔇3\mathfrak{D}_{1},\mathfrak{D}_{2},\mathfrak{D}_{3}, which by Section 1.1.3 are e1,−e2,−e1+e2e_{1},-e_{2},-e_{1}+e_{2} up to orientation issues. Thus

(1.16) −14​π​(∂2W∂μi​∂μj+4​∂2Vi​j∂η​∂η¯)​d​μi∧d​η∧d​η¯⊗ej=𝔇1⊗e1−𝔇2⊗e2+𝔇3⊗(e2−e1),\frac{\sqrt{-1}}{4\pi}\left(\frac{\partial^{2}W}{\partial\mu_{i}\partial\mu_{j}}+4\frac{\partial^{2}V^{ij}}{\partial\eta\partial\bar{\eta}}\right)d\mu_{i}\wedge d\eta\wedge d\bar{\eta}\otimes e_{j}=\mathfrak{D}_{1}\otimes e_{1}-\mathfrak{D}_{2}\otimes e_{2}+\mathfrak{D}_{3}\otimes(e_{2}-e_{1}),

where the RHS is a 𝔱\mathfrak{t}-valued codimension 3 cycle. The orientation here is decided by comparing with the Taub-NUT example. If d​μ1∧d​μ2∧d​Re​η∧d​Im​ηd\mu_{1}\wedge d\mu_{2}\wedge d\text{Re}\eta\wedge d\text{Im}\eta is an orientation form on ℝμ1,μ22×(S1×ℝ)η\mathbb{R}^{2}_{\mu_{1},\mu_{2}}\times(S^{1}\times\mathbb{R})_{\eta}, then the orientation forms on 𝔇1,𝔇2,𝔇3\mathfrak{D}_{1},\mathfrak{D}_{2},\mathfrak{D}_{3} are d​μ2,d​μ1,−d​μ1d\mu_{2},d\mu_{1},-d\mu_{1}, compatible with the directions pointing to infinity.

In the variant situation where η∈ℂ\eta\in\mathbb{C} instead of being periodic, to which previous discussions still apply, the generalised Gibbons-Hawking ansatz has a scaling symmetry compatible with the distributional equation (1.16): a new solution ΦΛ\Phi_{\Lambda} may be constructed from an old solution Φ\Phi by

(1.17) {ΦΛ​(μ1,μ2,η)=Λ−1​Φ​(Λ​μ1,Λ​μ2,Λ1.5​η),VΛi​j​(μ1,μ2,η)=Λ​Vi​j​(Λ​μ1,Λ​μ2,Λ1.5​η),WΛ​(μ1,μ2,η)=Λ2​W​(Λ​μ1,Λ​μ2,Λ1.5​η)\begin{cases}\Phi_{\Lambda}(\mu_{1},\mu_{2},\eta)=\Lambda^{-1}\Phi(\Lambda\mu_{1},\Lambda\mu_{2},\Lambda^{1.5}\eta),\\ V^{ij}_{\Lambda}(\mu_{1},\mu_{2},\eta)=\Lambda V^{ij}(\Lambda\mu_{1},\Lambda\mu_{2},\Lambda^{1.5}\eta),\\ W_{\Lambda}(\mu_{1},\mu_{2},\eta)=\Lambda^{2}W(\Lambda\mu_{1},\Lambda\mu_{2},\Lambda^{1.5}\eta)\end{cases}

These solutions are isometric up to a scaling factor, analogous to Taub-NUT metrics with different asymptotic circle lengths. The presence of the periodicty condition (or more abstractly an integral lattice structure) breaks down scaling symmetry by singling out a special scale.

Example 1.10.

(Negative vertex) By a similar argument, in the negative vertex setting (cf. Section 1.1.5) the curvature 2-form FF satisfies

(1.18) −12​π​d​F=−−14​π​(∂2Wp​q¯∂μ​∂μ+4​∂2V∂ηp​∂η¯q)​d​μ∧d​ηp∧d​η¯q=S,-\frac{1}{2\pi}dF=-\frac{\sqrt{-1}}{4\pi}\left(\frac{\partial^{2}W^{p\bar{q}}}{\partial\mu\partial\mu}+4\frac{\partial^{2}V}{\partial\eta_{p}\partial\bar{\eta}_{q}}\right)d\mu\wedge d\eta_{p}\wedge d\bar{\eta}_{q}=S,

where S={z1+z2=1}={e2​π​i​η1+e2​π​i​η2=1}⊂ℂz1∗×ℂz2∗×{0}⊂ℂz1∗×ℂz2∗×ℝμS=\{z_{1}+z_{2}=1\}=\{e^{2\pi i\eta_{1}}+e^{2\pi i\eta_{2}}=1\}\subset\mathbb{C}^{*}_{z_{1}}\times\mathbb{C}^{*}_{z_{2}}\times\{0\}\subset\mathbb{C}^{*}_{z_{1}}\times\mathbb{C}^{*}_{z_{2}}\times\mathbb{R}_{\mu} defines a codimension 3 cycle. Here SS is endowed with the complex orientation, and the orientation on ℂz2∗×ℝμ\mathbb{C}^{*}_{z_{2}}\times\mathbb{R}_{\mu} is defined by the form d​μ∧d​Re​η1∧d​Im​η1∧d​Re​η2∧d​Im​η2d\mu\wedge d\text{Re}\eta_{1}\wedge d\text{Im}\eta_{1}\wedge d\text{Re}\eta_{2}\wedge d\text{Im}\eta_{2}.

1.3. Ooguri-Vafa metric

In this Section we will review the Ooguri-Vafa metric, based on Gross and Wilson [11]. The recent paper [13] is an influence to our viewpoint, and the author thanks Song Sun for useful discussions.

1.3.1. Gibbons-Hawking viewpoint

The Ooguri-Vafa metric is an incomplete S1S^{1}-invariant hyperKähler metric constructed via the Gibbons-Hawking ansatz (cf. Section 1.2 with N=2,𝔫=1N=2,\mathfrak{n}=1). In our normalisation conventions, the metric lives on the singular S1S^{1}-bundle M→ℬ⊂ℝμ×(S1×ℝ)ηM\to\mathcal{B}\subset\mathbb{R}_{\mu}\times(S^{1}\times\mathbb{R})_{\eta} where the complex variable η\eta has period 1, and the S1S^{1}-fibre collapses to a point over the origin (μ,η)=0(\mu,\eta)=0. The first Chern class c1c_{1} of the S1S^{1}-bundle evaluates to −1-1 on a sphere around the origin in ℝμ×(S1×ℝ)η\mathbb{R}_{\mu}\times(S^{1}\times\mathbb{R})_{\eta}. The composition M→ℬ→(μ,Im​η)ℝ2M\to\mathcal{B}\xrightarrow{(\mu,\text{Im}\eta)}\mathbb{R}^{2} gives a singular T2T^{2}-fibration, and the periodicity condition on η\eta amounts to imposing ∫T2Ω=2​π\int_{T^{2}}\Omega=2\pi.

Let A≫1A\gg 1 be a large parameter. The Ooguri-Vafa metric can be thought as a perturbation of the constant solution (cf. Example 1.6) which is encoded by

gA=A⁡(d​μ2+|d​η|2).g_{A}=A(d\mu^{2}+|d\eta|^{2}).

after incorporating some topology. We denote |(μ,η)|=μ2+|η|2|(\mu,\eta)|=\sqrt{\mu^{2}+|\eta|^{2}}, and set

(1.19) V⁡(μ,η)=W=A+12​|(μ,η)|+∑n∈ℤ∖{0}{12​|(μ,η+n)|−12​|n|}V(\mu,\eta)=W=A+\frac{1}{2|(\mu,\eta)|}+\sum_{n\in\mathbb{Z}\setminus\{0\}}\{\frac{1}{2|(\mu,\eta+n)|}-\frac{1}{2|n|}\}

This series is convergent, 1-periodic in the η\eta variable, and satisfies the Laplace equation on ℬ\mathcal{B} with distributional term which encodes simultaneously the Calabi-Yau condition and the topology:

12​π​(∂2∂μ​∂μ+4​∂2∂η​∂η¯)​V​d​μ∧d​Re​η∧d​Im​η=−δ0,\frac{1}{2\pi}\left(\frac{\partial^{2}}{\partial\mu\partial\mu}+4\frac{\partial^{2}}{\partial\eta\partial\bar{\eta}}\right)Vd\mu\wedge d\text{Re}\eta\wedge d\text{Im}{\eta}=-\delta_{0},

where δ0\delta_{0} is the delta measure at the origin in ℝμ×S1×ℝ\mathbb{R}_{\mu}\times S^{1}\times\mathbb{R}. The metric on MM

g=V⁡(d​μ2+|d​η|2)+V−1​ϑ2g=V(d\mu^{2}+|d\eta|^{2})+V^{-1}\vartheta^{2}

is called the Ooguri-Vafa metric. Strictly speaking, the connection ϑ\vartheta can be twisted by a flat connection, and this choice is parametrised by H1​(ℬ∖{0},S1)=H1​(ℬ,S1)=H1​(S1×ℝ2,S1)≃S1H^{1}(\mathcal{B}\setminus\{0\},S^{1})=H^{1}(\mathcal{B},S^{1})=H^{1}(S^{1}\times\mathbb{R}^{2},S^{1})\simeq S^{1} using that a codimension 3 subset in the base does not affect the fundamental group. We sometimes suppress mentioning this choice as it does not affect the geometry significantly. By Remark 1.6 the μ,Im​η\mu,\text{Im}\eta coordinates define a special Lagrangian fibration with phase zero on MM.

The Ooguri-Vafa metric has the important exponential decay property for μ2+(Im​η)2≥1\mu^{2}+(\text{Im}\eta)^{2}\geq 1,

(1.20) |V⁡(μ,η)−A+γE−log⁡2+12​log⁡(μ2+|Im​η|2)|≤C​exp⁡(−2​π​μ2+(Im​η)2).|V(\mu,\eta)-A+\gamma_{E}-\log 2+\frac{1}{2}\log(\mu^{2}+|\text{Im}\eta|^{2})|\leq C\exp(-2\pi\sqrt{\mu^{2}+(\text{Im}\eta)^{2}}).

where γE=limn→∞∑k=1n1k−log⁡n\gamma_{E}=\lim_{n\to\infty}\sum_{k=1}^{n}\frac{1}{k}-\log n is the Euler constant. For μ2+(Im​η)2≫1\sqrt{\mu^{2}+(\text{Im}\eta)^{2}}\gg 1, the dependence of VV on the periodic Re​(η)\text{Re}(\eta)-variable decays exponentially, so up to exponentially small error the Ooguri-Vafa metric is asymptotic to a semiflat metric. This property is the main reason why the Ooguri-Vafa metric is useful for the gluing construction of Gross and Wilson [11]. On the other hand VV becomes negative roughly when log⁡(μ2+|Im​η|2)>2​A\log(\mu^{2}+|\text{Im}\eta|^{2})>2A, so the metric is only defined on a bounded set and is incomplete.

1.3.2. Holomorphic viewpoint

As a hyperKähler metric, the Ooguri-Vafa metric admits a 2-sphere of compatible integrable complex structures. There is one distinguished complex structure giving rise to a holomorphic elliptic fibration, which is described in detail in [11]. Here we wish to focus on another distinguished complex structure where η\eta is holomorphic and μ\mu is the symplectic moment map, which is more natural for special Lagrangian fibrations. The author is not aware of explicit references for the content of this Section.

Our main goal is to identify the complex structure on MM explicitly, which requires us to construct holomorphic functions on MM. We start with the type (1,0)(1,0) form ζ=V​d​μ+−1​ϑ\zeta=Vd\mu+\sqrt{-1}\vartheta and recall formula (1.14). To turn ζ\zeta into a holomorphic differential, we need to subtract a function times d​ηd\eta, whose differential cancels out d​ζd\zeta. Inspired by the Taub-NUT example 1.8, and taking care of periodicity requirement, we introduce the functions

{β+=π​−12−−1​θ∞+limk→∞∑n=−kn=k{12​(η+n)−μ2​(η+n)​μ2+|η+n|2}β−=π​−12+−1​θ∞+limk→∞∑n=−kn=k{12​(η+n)+μ2​(η+n)​μ2+|η+n|2}\begin{cases}\beta_{+}=\frac{\pi\sqrt{-1}}{2}-\sqrt{-1}\theta_{\infty}+\lim_{k\to\infty}\sum_{n=-k}^{n=k}\{\frac{1}{2(\eta+n)}-\frac{\mu}{2(\eta+n)\sqrt{\mu^{2}+|\eta+n|^{2}}}\}\\ \beta_{-}=\frac{\pi\sqrt{-1}}{2}+\sqrt{-1}\theta_{\infty}+\lim_{k\to\infty}\sum_{n=-k}^{n=k}\{\frac{1}{2(\eta+n)}+\frac{\mu}{2(\eta+n)\sqrt{\mu^{2}+|\eta+n|^{2}}}\}\end{cases}

These series are convergent and 1-periodic in η\eta, such that the forms ζ′=ζ+β+​d​η\zeta^{\prime}=\zeta+\beta_{+}d\eta, ζ′′=−ζ+β−​d​η\zeta^{\prime\prime}=-\zeta+\beta_{-}d\eta are closed. The real number θ∞\theta_{\infty} is chosen to cancel the asymptotic holonomy of the S1S^{1}-connection ϑ\vartheta along the Re​(η)\text{Re}(\eta)-circle as Im​η→∞\text{Im}\eta\to\infty. We have

ζ′+ζ′′=π​−1​d​η+limk→∞∑n=−kk1η+n​d​η=π​−1​d​η+d​log⁡(η​∏n=1∞(1−η2n2))=π​−1​d​η+d​log⁡(sin⁡(π​η)π)=d​log⁡(1−e2​π​i​η),\begin{split}\zeta^{\prime}+\zeta^{\prime\prime}&=\pi\sqrt{-1}d\eta+\lim_{k\to\infty}\sum_{n=-k}^{k}\frac{1}{\eta+n}d\eta\\ &=\pi\sqrt{-1}d\eta+d\log(\eta\prod_{n=1}^{\infty}(1-\frac{\eta^{2}}{n^{2}}))\\ &=\pi\sqrt{-1}d\eta+d\log(\frac{\sin(\pi\eta)}{\pi})=d\log(1-e^{2\pi i\eta}),\end{split}

where we made use of Euler’s factorisation identity of sin⁡(π​η)π​η\frac{\sin(\pi\eta)}{\pi\eta}. The line integrals ∫ζ′\int\zeta^{\prime} and ∫ζ′′\int\zeta^{\prime\prime} are locally holomorphic functions on MM, defined over the complement of {μ≤0,η=0}\{\mu\leq 0,\eta=0\} and {μ≥0,η=0}\{\mu\geq 0,\eta=0\} inside ℬ\mathcal{B}. Their T2T^{2}-periods lie in 2​π​−1​ℤ2\pi\sqrt{-1}\mathbb{Z}: the periods along the S1S^{1}-fibre over ℬ\mathcal{B} is ∫S1−1​ϑ=2​π​−1\int_{S^{1}}\sqrt{-1}\vartheta=2\pi\sqrt{-1}, while the periods along the S1S^{1}-cycle in MM lifting S1⊂ℝ×S1×ℝS^{1}\subset\mathbb{R}\times S^{1}\times\mathbb{R} can be evaluated by their asymptotic value as Im​(η)→+∞\text{Im}(\eta)\to+\infty; in particular if we twist the connection ϑ\vartheta by a flat connection, then we can always use the choice of θ∞\theta_{\infty} to cancel that twist. Thus we can define the holomorphic functions without multivalue issues

z1=exp⁡(∫ζ′),z2=exp⁡(∫ζ′′).z_{1}=\exp(\int\zeta^{\prime}),\quad z_{2}=\exp(\int\zeta^{\prime\prime}).

We are free to choose the multiplicative constants on z1,z2z_{1},z_{2} to satisfy the functional equation z1​z2=1−e2​π​i​ηz_{1}z_{2}=1-e^{2\pi i\eta}, from which we see that z1,z2z_{1},z_{2} extend to global holomorphic functions on MM, with zero locus {μ≤0,η=0}\{\mu\leq 0,\eta=0\} and {μ≥0,η=0}\{\mu\geq 0,\eta=0\} inside ℬ\mathcal{B} respectively. Setting z3=exp⁡(2​π​−1​η)z_{3}=\exp(2\pi\sqrt{-1}\eta), we obtain a holomorphic map

M→{z1z2=1−z3}⊂ℂz1,z22×ℂz3∗,M\to\{z_{1}z_{2}=1-z_{3}\}\subset\mathbb{C}^{2}_{z_{1},z_{2}}\times\mathbb{C}^{*}_{z_{3}},

which is easily seen to be an open embedding.

By looking at the action of the Hamiltonian vector field ∂∂θ\frac{\partial}{\partial\theta}, we can identify the circle action as

ei​θ⋅(z1,z2,z3)=(ei​θ​z1,e−i​θ​z2,z3).e^{i\theta}\cdot(z_{1},z_{2},z_{3})=(e^{i\theta}z_{1},e^{-i\theta}z_{2},z_{3}).

By construction the holomorphic volume form Ω\Omega satisfies ι∂∂θ​Ω=d​η\iota_{\frac{\partial}{\partial\theta}}\Omega=d\eta, which implies Ω=−12​π​1z3​d​z1∧d​z2,\Omega=-\frac{1}{2\pi}\frac{1}{z_{3}}dz_{1}\wedge dz_{2}, or equivalently

Ω∧d⁡((z1​z2)−1​(1−z3)−1)=12​π​d​log​z1∧d​log​z2∧d​log​z3.\Omega\wedge d((z_{1}z_{2})^{-1}(1-z_{3})-1)=\frac{1}{2\pi}d\log z_{1}\wedge d\log z_{2}\wedge d\log z_{3}.

The reader is advised to compare this discussion to Section 1.1.6.

Remark 1.10.

The viewpoint taken here starts with geometry, and the algebraic structure on the holomorphic functions only emerges a posteriori as a consequence of functional equations on transcendental integrals. This is conceptually rather similar to elliptic curves where algebraic relations arise from theta functions.

1.3.3. Some conceptual aspects of the Ooguri-Vafa metrics

The Ooguri-Vafa metric comes with an intrinsic parameter AA, and admits different geometric behaviours at different scales, which can be formalised in terms of blow up limits. Recall by periodicity we may assume Re​(η)\text{Re}(\eta) lies in some interval [0,1][0,1]. The periodicity condition we chose amounts to the normalisation that ∫T2Ω=2​π\int_{T^{2}}\Omega=2\pi.

  • •

    When μ2+|η|2≲1A\sqrt{\mu^{2}+|\eta|^{2}}\lesssim\frac{1}{A}, the leading order behaviour is V∼A+12​μ2+|η|2V\sim A+\frac{1}{2\sqrt{\mu^{2}+|\eta|^{2}}}, and the metric is modelled on the Taub-NUT metric with parameter AA. The length of the circle fibres ∼2​πA\sim\frac{2\pi}{\sqrt{A}}. After scaling up the metric by a factor AA and taking the limit A→∞A\to\infty, the pointed Gromov-Hausdorff limit based at the origin is the standard Taub-NUT metric with parameter 1. Most Riemannian curvature is concentrated in this region.

  • •

    When 1A≪μ2+|η|2≪1\frac{1}{A}\ll\sqrt{\mu^{2}+|\eta|^{2}}\ll 1, the leading order behaviour is the constant solution V∼AV\sim A, and the metric is locally modelled on a flat circle bundle over a flat base ℝ3\mathbb{R}^{3}. A suitable blow up limit space is flat ℝ3\mathbb{R}^{3}.

  • •

    When μ2+|η|2∼1\sqrt{\mu^{2}+|\eta|^{2}}\sim 1, the leading order behaviour is still V∼AV\sim A, but the periodicity condition is now visible. The metric is locally modelled on a flat circle bundle over a flat base ℝμ×S1×ℝ\mathbb{R}_{\mu}\times S^{1}\times\mathbb{R}. The length of the circle factor of the base is approximately A\sqrt{A}. If we scale down the metric by a factor 1A\frac{1}{A} and take the limit A→∞A\to\infty, the pointed Gromov-Hausdorff limit based at the origin is the flat ℝμ×S1×ℝ\mathbb{R}_{\mu}\times S^{1}\times\mathbb{R}.

  • •

    When 1≪μ2+|η|2≪exp⁡(A)1\ll\sqrt{\mu^{2}+|\eta|^{2}}\ll\exp(A), the metric becomes almost semiflat up to exponentially small errors, and the leading order behaviour is

    V∼A+log⁡2−γE−12​log⁡(μ2+|Im​(η)|2).V\sim A+\log 2-\gamma_{E}-\frac{1}{2}\log(\mu^{2}+|\text{Im}(\eta)|^{2}).

    We remark that the log function grows very slowly. Thus within an exponentially long neck region, the constant solution V∼AV\sim A is a good approximation. If we view AA as related to the average length of circles, then we can think of VV as approximated by a family of constant solutions whose parameter slowly drifts down as we move up the logarithmic scale. The author finds it attractive to call this phenomenon running coupling.

  • •

    When μ2+|η|2∼exp⁡(A)\sqrt{\mu^{2}+|\eta|^{2}}\sim\exp(A) the incompleteness of the metric is manifested. This is best understood by viewing the Ooguri-Vafa metric as an effective local description of the hyperKähler metric on a family of collapsing K3 surfaces, and incompleteness is an indication that there is a scale beyond which this description must break down. On the other hand, if we are looking at smaller distance scales, then the Ooguri-Vafa metric becomes better approximations of the K3 metric. In particular, the K3 hyperKähler structure involves 60 parameters while the Ooguri-Vafa metric only involves one scaling parameter AA and a gauge parameter in S1S^{1}, but the metric at smaller distance scales are not sensitive to many extra parameters as long as the K3 surfaces are sufficiently collapsed. This phenomenon may be called effective uniqueness or local universality, which is an essential aspect of Gross and Wilson’s gluing construction [11]. The analogy with K. Wilson’s philosophy of effective quantum field theory will be further explained in Section 3.10.

The analysis of the blow up limits reveals the cause d’etre of the Ooguri-Vafa metric. Recall the Taub-NUT metrics arise in a 1-parameter family, which are related by the scaling symmetry. The Ooguri-Vafa metric is obtained conceptually by gluing the Taub-NUT metric to the constant solution. The periodicity condition, which is a kind of integral lattice structure, breaks down the scaling symmetry, and results in an intrinsic gluing parameter AA. Another major effect of the periodicity condition is the exponential decay of higher Fourier modes, which works via spectral theory, and results in the semiflat asymptotic picture.

A notable feature in the Ooguri-Vafa metric is the appearance of the Green’s function VV. This is because we are perturbing from the constant solution, and the first order correction to the flat ambient solution natually invovles harmonic functions at least away from the singular locus. The precise nature of the singularity of VV is dictated by the topology, or more precisely the Chern class, via the distributional equation.

These principles are sufficient to lead to the discovery of the Ooguri-Vafa metric. While the exact linearity of the equation governing the Gibbons-Hawking ansatz in complex dimension 2 is a fortunate simplifying feature, it does not appear essential in our discussions above. A core idea in this paper is that essentially the same principles dictate how to generalise the Ooguri-Vafa metric to dimension 3.

1.4. Synopsis of the new metrics

A central theme running through this paper is the strong analogy between the Taub-NUT type metric on ℂ3\mathbb{C}^{3} and the Ooguri-Vafa type metrics on the positive/negative vertices (cf. Theorem 1.2, 1.3 and 1.4). The purpose of this Section is to give a unified view on our strategy to produce these three types of new metrics, which involves a geometric part concerning the construction of an ansatz, and an analytic part concerning perturbing the ansatz into a Calabi-Yau metric. Many aspects of these new metrics naturally generalise features of the Taub-NUT metric (cf. Example 1.8) and the Ooguri-Vafa metric (cf. Section 1.3).

1.4.1. Geometric aspects

All three types of metric ansatzs are constructed in the generalised Gibbons-Hawking framework, by perturbing from the constant solution after incorporating topology. The constant solutions in Example 1.6 serve as zeroth order approximations to the metric ansatz, and can be thought as scaling limits (cf. Section 1.3.3). Geometrically they describe a flat torus fibration fibred over a Euclidean base with distinguished coordinates related to moment maps. The choice of this Euclidean metric is parametrised by a positive definite rank 2 real symmetric or Hermitian matrix, depending on the 3 cases. The principal difference between the Taub-NUT type metric on ℂ3\mathbb{C}^{3} and the Ooguri-Vafa type metrics is that the bases in the latter cases have periodic directions.

In order to build in the Gross-Ruan-Joyce topology (cf. Section 1.1) we need to make first order corrections to the constant solutions. Recall the generalised Gibbons-Hawking construction involves three sets of equations:

  • •

    The integrability condition is responsible for the integrability of the complex structure and the Kähler condition.

  • •

    The distributional equation captures the topology and the discriminant locus.

  • •

    The Calabi-Yau condition is the only nonlinear equation.

It is natural to impose that the first order corrections satisfy the linearised version of these equations; in particular the linearisation of the Calabi-Yau condition gives rise to harmonic functions. These linearised equations combine into a coupled overdetermined system. Our method to solve this system is to first determine by educated guess the singularities of the harmonic functions along the discriminant locus, explicitly construct such harmonic functions using Green’s representation, and then verify the other equations in the overdetermined system by means of Liouville theorem type arguments. The first order corrections we obtain are canonical (up to constants) under mild growth constraints. For the Taub-NUT type ℂ3\mathbb{C}^{3} case the first order corrections admit elementary formulae. For the Ooguri-Vafa type metrics on the vertices the first order corrections involve infinite series and Green representation integrals, which are a priori divergent but become convergent after subtracting logarithmically divergent terms, much like what happens already for the Ooguri-Vafa metric.

We then extract various asymptotes of the first order ansatz. Transverse to the discriminant locus, the leading asymptotes can be interpreted geometrically as giving rise to Taub-NUT metrics; ultimately this is forced on us by the distributional equation coming from the topology. In the Ooguri-Vafa type situations, we can also perform Fourier analysis in the periodic variables. Suitably away from the discriminant locus, the zeroth Fourier mode is the dominant contribution, giving rise to a semiflat metric. The harmonicity condition implies that the higher Fourier modes satisfy Helmholtz equations, thereby decay exponentially. An additional problem in the Ooguri-Vafa type situations is that the metric ansatzs are only positive definite on a bounded region, whereby metrically incomplete.

The strategy to identify the holomorphic structure is to produce holomorphic differentials with integral periods, in a manner similar to the Taub-NUT metric and the Ooguri-Vafa metric (cf. Section 1.3.2). The functional equation satisfied by the holomorphic functions allows us to identify the holomorphic volume form. It should be emphasized that while topology is built a priori into the generalised Gibbons-Hawking construction, the holomorphic structure is a nontrivial a posteriori consequence.

The first order corrections are small perturbations suitably away from the discriminant locus, but near the discriminant locus they are large compared to the constant solution. This explains why the first order metric ansatz is approximately Calabi-Yau suitably away from the discriminant locus. In the suitable weighted Hölder norms this approximation continues to hold good near the discriminant locus, except on small balls near the origin in the Taub-NUT type ℂ3\mathbb{C}^{3} case and the positive vertex case. Geometrically this problem is caused by the 3 edges of 𝔇\mathfrak{D} interacting strongly at their intersection point. The same problem does not appear on the negative vertex because the discriminant locus SS has no singular point.

Our strategy trifurcates at this point. The small ball is a fully nonlinear region in which linear approximation methods fail completely. In the case of the Taub-NUT type metric on ℂ3\mathbb{C}^{3}, we instead shift to the complex geometric perspective, and solve the complex Monge-Ampère equation with prescribed asymptotes at infinity. This is viable because the exterior of the small ball does admit an approximately Calabi-Yau ansatz. The output is a Calabi-Yau metric on ℂ3\mathbb{C}^{3} whose deviation from the first order ansatz satisfies an asymptotically good estimate.

The Ooguri-Vafa type metric on the positive vertex is best thought as the periodic version of the Taub-NUT type metric on ℂ3\mathbb{C}^{3}, and is obtained by gluing the Taub-NUT type ℂ3\mathbb{C}^{3} to the first order ansatz on the positive vertex. The periodicity condition breaks down the scaling symmetry of the Taub-NUT type metrics, and instead results in the gluing picture, exactly analogous to the relation between the Taub-NUT metric and the usual Ooguri-Vafa metric. The nonlinear effect on the positive vertex is already fully present on the Taub-NUT type ℂ3\mathbb{C}^{3}. It is worth comparing with the topological prediction of Gross-Ruan (cf. Section 1.1.3) where the neighbourhood of the origin is modelled on ℂ3\mathbb{C}^{3} with a T2T^{2} fibration related to the Harvey-Lawson example 1.7. But for metric purposes we need to use an exotic Calabi-Yau metric on ℂ3\mathbb{C}^{3}, rather than the Euclidean ℂ3\mathbb{C}^{3}.

The Ooguri-Vafa type metric on the negative vertex, on the other hand, is constructed entirely perturbatively from the first order ansatz.

1.4.2. Analytic aspects

The analytic step is aimed at perturbing the first order ansatz into a genuine Calabi-Yau metric, and the techniques involved overlap substantially in all three cases.

A central issue, roughly put, is to produce a parametrix for the right inverse to the Laplacian with accurate control on weighted Hölder norm estimates. Some of the main difficulties are:

  • •

    The first order corrected metric is multiscaled, namely it has very different characteristic behaviours in different regions and at different length scales.

  • •

    The initial error decays slowly.

The core idea in our methodology is divide and conquer. We decompose the source function according to its support. The contribution supported sufficiently away from the discriminant locus is inverted approximately using the Euclidean Green operator, reflecting the fact that the constant solution is the zeroth order approximation to the metric ansatz. Afterwards the source function is effectively supported near the discriminant locus. We then use a Green operator adapted to the Taub-NUT fibration near the discriminant locus to cure the remaining source.

We now turn to specifics. The 3 cases are arranged in pedagogical order, and each case contains most difficulties of previous cases. As a general policy, detailed proofs will be omitted if the main techniques appeared previously.

In the Taub-NUT type ℂ3\mathbb{C}^{3} case, the parametrix is used to improve the approximation to the Calabi-Yau condition asymptotically outside a compact region. Once the decay of the approximation error is sufficiently fast, we can appeal to a non-compact version of Yau’s solution to the Calabi conjecture, developed in H-J. Hein’s thesis [12], to turn the ansatz into a genuine Calabi-Yau metric with effective estimates.

Here a difficulty caused by the slow decay of error is that the inverse of the Laplacian is not well behaved in the weighted Hölder spaces. Instead it is preferable to work with the zeroth order operator ∇2Δ−1\nabla^{2}\Delta^{-1}, which controls how to correct a Kähler metric for a given amount of volume form error. The advantage is that this operator maps between function spaces with the same Hölder weights, the operator norm is not affected by rescaling the metric, and crucially the Schwartz kernel has two extra order of decay compared to Δ−1\Delta^{-1}.

In the positive vertex case, the main new difficulty is to prove exponential decay of higher Fourier modes. This comes down to mapping properties of the periodic Euclidean Green operator, ultimately thanks to the exponential decay of the higher Fourier modes of the periodic Newtonian potential.

The second new difficulty is that that the volume form error does not decay, and in fact grows logarithmically at large distance, causing problem for perturbation theory over an exponentially long region. The strategy is to first correct the error inside the generic region in the generalised Gibbons-Hawking framework, using the periodic Green operator. We then switch to the complex geometric viewpoint and solve the complex Monge-Ampère equation perturbatively, which avoids the difficulty of the generalised Gibbons-Hawking equation near the discriminant locus.

The third new difficulty comes from metric incompleteness: the Laplacian has no good mapping property in the naïve weighted Hölder spaces. In our approach, this means the parametrix is only defined on compactly supported sources, but the outputs are generally not compactly supported. A formal trick called extension norms [27] effectively allows us to assume the source is compactly supported. This circumvents the need to impose a non-canonical boundary condition.

In the negative vertex case, the main new difficulty comes from the curved nature of the discriminant locus SS, making it harder to produce a parametrix near SS. A closely related issue is that there is no obvious a priori choice of smooth topology such that the first order metric ansatz is smooth along SS. These problems force us to work in weighted Hölder spaces with low regularity, in which it makes no sense to speak of an arbitrarily high order of differentiability. Crucially there is enough regularity to make the Laplacian well defined. The smooth topology emerges a posteriori only after solving the complex Monge-Ampère equation. The solution itself defines a complex structure, hence induces a smooth topology, and the compatibility of the metric with this smooth topology is a consequence of the well known regularity theory for complex Monge-Ampère equation.

1.4.3. Outlook: towards the SYZ conjecture

We now explain how this paper fits into a program to prove the metric version of the SYZ conjecture for Calabi-Yau 3-folds (cf. Conjecture 1.1). This program runs as follows:

  1. (1)

    Produce the metric models on the positive and negative vertices.

  2. (2)

    The metric structure near the edges in the Gross-Ruan picture are expected to be modelled on a fibration by Ooguri-Vafa metrics. The problem is that Ooguri-Vafa metrics transverse to the edge depend on a moduli parameter which can vary along the edge, possibly governed by an adiabatic equation.

  3. (3)

    The SYZ base BB as an affine manifold with singularity along a trivalent graph, can be produced from algebraic geometry in some degree of generality [32][16]. The central problem is then to solve the real Monge-Ampère equation with some prescribed singularities along the trivalent graph. This would allow us to produce a semiflat metric which models the generic region of the SYZ fibration.

  4. (4)

    One then glues together the metric models in various regions to obtain the global Calabi-Yau metric on the Calabi-Yau 3-fold, similar to Gross and Wilson’s work on K3 surfaces [11]. Some Fourier analysis is needed to prove exponential decay estimates for deviation from the semiflat metric.

  5. (5)

    The existence of the SYZ fibration in the generic region is expected to be a straightforward consequence of the gluing construction. To produce the SYZ fibration near the trivalent graph, one needs to produce models for singular SYZ fibrations on the metric models, and set up a Fredholm deformation theory to ensure the SYZ fibration persists when the metric deforms.

The principal contribution of this paper is to carry out Step (1), and our linear analysis is likely to be useful in Step (4). Some informal digressions in this paper go some way towards addressing difficulties in the other Steps:

In Step (3), the singularity of the real Monge-Ampère equation near the trivalent graph in BB should match up with the asymptotic behaviour of the metric models around the trivalent graph, in order to enable the gluing construction in Step (4). This requires understanding how the Ooguri-Vafa type metrics on the vertices transition into the generic region of the SYZ fibration. We propose a mechanism called running coupling for this transition to take place over an exponentially long neck region (cf. Section 3.10 and 4.13). Starting from the observation that Ooguri-Vafa type metrics naturally arise in a family parametrised by some positive definite rank 2 matrices referred to as coupling constants, we argue semi-heuristically that these coupling constants drift slowly as the logarithmic scale increases, governed by an ODE called the renormalistion flow equation which can be solved exactly.

The behaviour of the special Lagrangian fibrations is discussed in Corollary 2.29, Corollary 3.35 and Section 4.12. In both the Taub-NUT type ℂ3\mathbb{C}^{3} case and the positive vertex case, the T2T^{2}-symmetry provides two symplectic moment coordinates and another real coordinate Im​(η)\text{Im}(\eta), which define a map to ℝ3\mathbb{R}^{3} whose fibres are T2T^{2}-invariant special Lagrangians with phase zero. However, Joyce’s critique suggests the singularity structure of this SYZ fibration is not stable under metric perturbation.

In the negative vertex case (cf. Section 4.12), there is a homological constraint for the SYZ fibration to exist, namely the Hermitian matrix ap​q¯a_{p\bar{q}} needs to be symmetric. When this constraint holds, we outline a speculative description of a U⁡(1)U(1)-invariant SYZ fibration on the model metric, and explain how it fits with Joyce’s work on U⁡(1)U(1)-invariant special Lagrangians. The case where this constraint does not hold is possibly relevant for metric degenerations outside the scope of the SYZ conjecture.

Original mathematics by the credited authors. Source-backed reader collection; mathematical self-containment is not assessed.