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Singularities of special Lagrangian fibrations and the SYZ Conjecture

Joyce, Dominic

Original paper

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Singularities of special Lagrangian fibrations
and the SYZ Conjecture

Dominic Joyce Affiliation: Lincoln College, Oxford
November 2000
[03KB]

1 Introduction

The Strominger–Yau–Zaslow Conjecture [22], or SYZ Conjecture, explains Mirror Symmetry between Calabi–Yau 3-folds X,X^X,\hat{X} in terms of the existence of special Lagrangian fibrations f:X→Bf:X\rightarrow B and f^:X^→B\hat{f}:\hat{X}\rightarrow B over the same base BB, such that for generic b∈Bb\in B the fibres f−1​(b)f^{-1}(b) and f^−1​(b)\hat{f}^{-1}(b) are dual 3-tori in XX and X^\hat{X} respectively.

The original SYZ Conjecture was motivated by physical reasoning, and was somewhat vague on mathematical details, so that it is not yet clear exactly what the final form of the conjecture ought to be. But it has been obvious from the beginning that many of the problems in formulating and proving the conjecture will have to do with the singular fibres of the fibrations.

Much work has already been done on the SYZ Conjecture by Zharkov [23], Gross [5, 6, 7], Ruan [18, 19, 20, 21] and others. By and large these papers have focussed on difficult questions of global symplectic topology, and have dealt mostly with Lagrangian fibrations, without making great use of the special Lagrangian condition.

The goal of this paper is to build up a (partly conjectural) picture of the singularities of special Lagrangian fibrations f:X→Bf:X\rightarrow B of a Calabi–Yau 3-fold XX, particularly in the case when XX is generic in a suitable sense. We take a different point of view from the authors above, in that we adopt a local geometric approach rather than a global topological one, and we make essential use of the special Lagrangian condition throughout.

One of our main contentions is that generically the singularities of a special Lagrangian 3-fold NN in XX will be finitely many isolated points p1,…,pkp_{1},\ldots,p_{k}, and that the best way to understand them is in terms of local models for the singularities in ℂ3\mathbin{\mathbb{C}}^{3}. That is, in a small neighbourhood of each pjp_{j} in XX, NN will look like a special Lagrangian 3-fold in ℂ3≅TpjX\mathbin{\mathbb{C}}^{3}\cong T_{\smash{p_{j}}}X with a singularity at 0.

So to study singularities of special Lagrangian 3-folds in Calabi–Yau 3-folds, we should begin by finding and classifying examples of special Lagrangian 3-folds in ℂ3\mathbin{\mathbb{C}}^{3}. The author has made a start on this process in three papers [11, 12, 13] constructing explicit examples of special Lagrangian mm-folds in ℂm\mathbin{\mathbb{C}}^{m}, and expects to write others. While these papers are not directly relevant to the present work, the general understanding of special Lagrangian singularities acquired in these papers was very helpful to the author in thinking about special Lagrangian fibrations.

Most other authors writing about the SYZ Conjecture have considered special Lagrangian fibrations f:X→Bf:X\rightarrow B of a Calabi–Yau 3-fold in which the base space BB is a smooth 3-manifold, and ff is a smooth map. This implies that the discriminant Δf\Delta_{f} (the set of singular fibres) of ff is of codimension two in BB, and that generic singular fibres are singular along a real curve.

My picture is rather different from this. I believe that in the generic case special Lagrangian fibrations f:X→Bf:X\rightarrow B are only piecewise smooth, being continuous but not differentiable on real hypersurfaces in XX. Furthermore, the discriminant Δf\Delta_{f} is of codimension one in BB, and all singular fibres have only finitely many singular points.

Whilst I do not prove this conclusively — this would require some rather difficult analytic results which I hope to prove one day — I do present a lot of evidence in favour of my ideas. As the view that special Lagrangian fibrations are smooth has appeared in so many papers, I also felt it necessary to explain why I think this is wrong. I hope the authors I have disagreed with in person will take this as a mark of respect, as I have learnt a lot from their papers.

We begin in §2 with an introduction to special Lagrangian geometry. We include a discussion of almost Calabi–Yau manifolds and genericity which will probably be unfamiliar to most readers. Section 3 discusses the SYZ Conjecture, explains why generic special Lagrangian fibrations cannot be smooth, and reviews a construction of piecewise smooth Lagrangian fibrations by Wei-Dong Ruan which has many features in common with the picture of special Lagrangian fibrations we will propose.

Section 4 describes two symmetric special Lagrangian fibrations of ℂ3\mathbin{\mathbb{C}}^{3} due to Harvey and Lawson, and studies their singular fibres. Then §5 defines our local model for codimension one singularities in generic special Lagrangian fibrations. It is an entirely explicit, piecewise smooth special Lagrangian fibration f:ℂ3→ℝ3f:\mathbin{\mathbb{C}}^{3}\rightarrow\mathbin{\mathbb{R}}^{3}, given by a simple formula. The fibres of ff are translations of parts of fibres from the Harvey–Lawson fibration in §4.

We move on in §6–§8 to consider codimension two singularities in special Lagrangian fibrations. We do this by studying a class of U(1)\mathbin{\rm U}(1)-invariant 3-folds NN in ℂ3\mathbin{\mathbb{C}}^{3} defined in terms of functions u,v:ℝ2→ℝu,v:\mathbin{\mathbb{R}}^{2}\rightarrow\mathbin{\mathbb{R}}. The condition for NN to be special Lagrangian is a p.d.e. on uu and vv, a nonlinear version of the Cauchy–Riemann equations.

Making some conjectures about solutions of these equations, in §7 we describe the expected structure of codimension two singularities. We apply this in §8 to a situation with some nontrivial global topology, and do a monodromy calculation.

Finally, in §9 we review the global properties of smooth special Lagrangian fibrations f:X→Bf:X\rightarrow B uncovered by Mark Gross and Wei-Dong Ruan, and propose how their picture should be modified under a generic perturbation of XX. Based on this we draw some conclusions, which contradict the stronger current forms of the SYZ Conjecture.

Acknowledgements. I would like to thank Mark Gross, Richard Thomas, Nigel Hitchin and David Morrison for helpful conversations.

[03KC]

2 Special Lagrangian geometry

We now introduce the idea of special Lagrangian submanifolds, in three different geometric contexts. First, in §2.1, we discuss special Lagrangian submanifolds in ℂm\mathbin{\mathbb{C}}^{m}. Then §2.2 considers special Lagrangian submanifolds in Calabi–Yau manifolds, a class of compact Ricci-flat Kähler manifolds equipped with a holomorphic volume form.

Finally, §2.3 generalizes this to almost Calabi–Yau manifolds, which are compact Kähler manifolds with a holomorphic volume form, but need not be Ricci-flat. We argue that almost Calabi–Yau manifolds are a good setting in which to study generic special Lagrangian submanifolds and fibrations.

[03KD]

2.1 Special Lagrangian submanifolds in ℂm\mathbin{\mathbb{C}}^{m}

We begin by defining calibrations and calibrated submanifolds, following Harvey and Lawson [9].

[03KE]

Definition 2.1 Let (M,g)(M,g) be a Riemannian manifold. An oriented tangent kk-plane VV on MM is a vector subspace VV of some tangent space Tx​MT_{x}M to MM with dimV=k\mathop{\rm dim}V=k, equipped with an orientation. If VV is an oriented tangent kk-plane on MM then g|Vg|_{V} is a Euclidean metric on VV, so combining g|Vg|_{V} with the orientation on VV gives a natural volume form volV\mathop{\rm vol}_{V} on VV, which is a kk-form on VV.

Now let φ\varphi be a closed kk-form on MM. We say that φ\varphi is a calibration on MM if for every oriented kk-plane VV on MM we have φ|V⩽volV\varphi|_{V}\leqslant\mathop{\rm vol}_{V}. Here φ|V=α⋅volV\varphi|_{V}=\alpha\cdot\mathop{\rm vol}_{V} for some α∈ℝ\alpha\in\mathbin{\mathbb{R}}, and φ|V⩽volV\varphi|_{V}\leqslant\mathop{\rm vol}_{V} if α⩽1\alpha\leqslant 1. Let NN be an oriented submanifold of MM with dimension kk. Then each tangent space Tx​NT_{x}N for x∈Nx\in N is an oriented tangent kk-plane. We say that NN is a calibrated submanifold if φ|Tx​N=volTx​N\varphi|_{T_{x}N}=\mathop{\rm vol}_{T_{x}N} for all x∈Nx\in N.

It is easy to show that calibrated submanifolds are automatically minimal submanifolds [9, Th. II.4.2]. Here is the definition of special Lagrangian submanifolds in ℂm\mathbin{\mathbb{C}}^{m}, taken from [9, §III].

[03KF]

Definition 2.2 Let ℂm\mathbin{\mathbb{C}}^{m} have complex coordinates (z1,…,zm)(z_{1},\dots,z_{m}), and define a metric gg, a real 2-form ω\omega and a complex mm-form Ω\Omega on ℂm\mathbin{\mathbb{C}}^{m} by

g=|d​z1|2+⋯+|d​zm|2,ω=i2​(d​z1∧d​z¯1+⋯+d​zm∧d​z¯m),andΩ=d​z1∧⋯∧d​zm.\begin{split}g=|{\rm d}z_{1}|^{2}+\cdots+|{\rm d}z_{m}|^{2},\quad\omega&=\frac{i}{2}({\rm d}z_{1}\wedge{\rm d}\bar{z}_{1}+\cdots+{\rm d}z_{m}\wedge{\rm d}\bar{z}_{m}),\\ \text{and}\quad\Omega&={\rm d}z_{1}\wedge\cdots\wedge{\rm d}z_{m}.\end{split} (1)

Then ReΩ\mathop{\rm Re}\Omega and ImΩ\mathop{\rm Im}\Omega are real mm-forms on ℂm\mathbin{\mathbb{C}}^{m}. Let LL be an oriented real submanifold of ℂm\mathbin{\mathbb{C}}^{m} of real dimension mm. We say that LL is a special Lagrangian submanifold of ℂm,\mathbin{\mathbb{C}}^{m}, or SL mm-fold for short, if LL is calibrated with respect to ReΩ\mathop{\rm Re}\Omega, in the sense of Definition 2.1.

As in [10, 11] there is a more general definition of special Lagrangian mm-fold involving a phase ei​θ{\rm e}^{i\theta}, but we will not use it here. Harvey and Lawson [9, Cor. III.1.11] give the following alternative characterization of special Lagrangian submanifolds.

[03KG]
Proposition 2.3

Let LL be a real mm-dimensional submanifold of ℂm\mathbin{\mathbb{C}}^{m}. Then LL admits an orientation making it into an SL submanifold of ℂm\mathbin{\mathbb{C}}^{m} if and only if ω|L≡0\omega|_{L}\equiv 0 and ImΩ|L≡0\mathop{\rm Im}\Omega|_{L}\equiv 0.

An mm-dimensional submanifold LL in ℂm\mathbin{\mathbb{C}}^{m} is called Lagrangian if ω|L≡0\omega|_{L}\equiv 0. Thus special Lagrangian submanifolds are Lagrangian submanifolds satisfying the extra condition that ImΩ|L≡0\mathop{\rm Im}\Omega|_{L}\equiv 0, which is how they get their name.

Next we give a result characterizing SL 3-planes ℝ3\mathbin{\mathbb{R}}^{3} in ℂ3\mathbin{\mathbb{C}}^{3}, which will be useful in §7. Define an anti-bilinear cross product ×:ℂ3×ℂ3→ℂ3\times:\mathbin{\mathbb{C}}^{3}\times\mathbin{\mathbb{C}}^{3}\rightarrow\mathbin{\mathbb{C}}^{3} by

(r1,r2,r3)×(s1,s2,s3)=(r¯2​s¯3−r¯3​s¯2,r¯3​s¯1−r¯1​s¯3,r¯1​s¯2−r¯2​s¯1).(r_{1},r_{2},r_{3})\times(s_{1},s_{2},s_{3})=(\bar{r}_{2}\bar{s}_{3}-\bar{r}_{3}\bar{s}_{2},\bar{r}_{3}\bar{s}_{1}-\bar{r}_{1}\bar{s}_{3},\bar{r}_{1}\bar{s}_{2}-\bar{r}_{2}\bar{s}_{1}). (2)

It is equivariant under the SU(3)\mathop{\rm SU}(3)-action on ℂ3\mathbin{\mathbb{C}}^{3}. Using this notation, we prove

[03KH]
Proposition 2.4

Let 𝐫,𝐬∈ℂ3{\bf r},{\bf s}\in\mathbin{\mathbb{C}}^{3} be linearly independent over ℝ\mathbin{\mathbb{R}}, with ω⁡(𝐫,𝐬)=0\omega({\bf r},{\bf s})=0. Then 𝐫,𝐬{\bf r},{\bf s} and 𝐫×𝐬{\bf r}\times{\bf s} are linearly independent over ℝ\mathbin{\mathbb{R}}, and ⟨𝐫,𝐬,𝐫×𝐬⟩ℝ\langle{\bf r},{\bf s},{\bf r}\times{\bf s}\rangle_{\scriptscriptstyle\mathbb{R}} is the unique special Lagrangian 33-plane in ℂ3\mathbin{\mathbb{C}}^{3} containing ⟨𝐫,𝐬⟩ℝ\langle{\bf r},{\bf s}\rangle_{\scriptscriptstyle\mathbb{R}}.

[03KI]

Proof. Explicit calculation using (2) shows that

g⁡(𝐫,𝐫×𝐬)=g⁡(𝐬,𝐫×𝐬)=0,\displaystyle g({\bf r},{\bf r}\times{\bf s})=g({\bf s},{\bf r}\times{\bf s})=0, (3)
ω⁡(𝐫,𝐫×𝐬)=ω⁡(𝐬,𝐫×𝐬)=0,\displaystyle\omega({\bf r},{\bf r}\times{\bf s})=\omega({\bf s},{\bf r}\times{\bf s})=0, (4)
|𝐫×𝐬|2=|𝐫|𝟐​|𝐬|𝟐−𝐠​(𝐫,𝐬)𝟐−ω​(𝐫,𝐬)𝟐,\displaystyle|{\bf r}\times{\bf s}|^{2}=|\bf r|^{2}|\bf s|^{2}-g({\bf r},{\bf s})^{2}-\omega({\bf r},{\bf s})^{2}, (5)
and(ImΩ)​(𝐫,𝐬,𝐫×𝐬)=0,\displaystyle\text{and}\quad(\mathop{\rm Im}\Omega)({\bf r},{\bf s},{\bf r}\times{\bf s})=0, (6)

for all 𝐫,𝐬∈ℂ3{\bf r},{\bf s}\in\mathbin{\mathbb{C}}^{3}. When 𝐫,𝐬{\bf r},{\bf s} are linearly independent and ω⁡(𝐫,𝐬)=0\omega({\bf r},{\bf s})=0, equation (3) shows that 𝐫×𝐬{\bf r}\times{\bf s} is orthogonal to 𝐫,𝐬{\bf r},{\bf s}, and (5) that |𝐫×𝐬|≠0|{\bf r}\times{\bf s}|\neq 0. Therefore 𝐫,𝐬{\bf r},{\bf s} and 𝐫×𝐬{\bf r}\times{\bf s} are linearly independent.

Also we have ω⁡(𝐫,𝐬)=ω⁡(𝐫,𝐫×𝐬)=ω⁡(𝐬,𝐫×𝐬)=0\omega({\bf r},{\bf s})=\omega({\bf r},{\bf r}\times{\bf s})=\omega({\bf s},{\bf r}\times{\bf s})=0 by (4), so that ⟨𝐫,𝐬,𝐫×𝐬⟩ℝ\langle{\bf r},{\bf s},{\bf r}\times{\bf s}\rangle_{\scriptscriptstyle\mathbb{R}} is a Lagrangian 3-plane. Then (6) shows that ⟨𝐫,𝐬,𝐫×𝐬⟩ℝ\langle{\bf r},{\bf s},{\bf r}\times{\bf s}\rangle_{\scriptscriptstyle\mathbb{R}} is a special Lagrangian 3-plane, by Proposition 2.7. It is easy to see that this is the only SL 3-plane in ℂ3\mathbin{\mathbb{C}}^{3} containing ⟨𝐫,𝐬⟩ℝ\langle{\bf r},{\bf s}\rangle_{\scriptscriptstyle\mathbb{R}}. □\square

[03KJ]

2.2 Special Lagrangian mm-folds in Calabi–Yau mm-folds

Now special Lagrangian submanifolds in ℂm\mathbin{\mathbb{C}}^{m} are the local model for special Lagrangian submanifolds in Calabi–Yau manifolds. We adopt the following definition of Calabi–Yau manifolds, which is not the usual one, but will be useful for our purposes.

[03KK]

Definition 2.5 Let m⩾2m\geqslant 2. A Calabi–Yau mm-fold, or CY mm-fold for short, is a quadruple (X,J,ω,Ω)(X,J,\omega,\Omega) such that (X,J)(X,J) is a compact mm-dimensional complex manifold, ω\omega the Kähler form of a Kähler metric gg on XX, and Ω\Omega a non-vanishing holomorphic (m,0)(m,0)-form on XX which satisfies

ωm/m!=(−1)m⁡(m−1)/2​(i/2)m​Ω∧Ω¯.\omega^{m}/m!=(-1)^{m(m-1)/2}(i/2)^{m}\Omega\wedge\bar{\Omega}. (7)

Then for each x∈Xx\in X there exists an isomorphism TxX≅ℂmT_{x}X\cong\mathbin{\mathbb{C}}^{m} that identifies gx,ωxg_{x},\omega_{x} and Ωx\Omega_{x} with the flat versions g,ω,Ωg,\omega,\Omega on ℂm\mathbin{\mathbb{C}}^{m} in (1).

Generally we will refer to a Calabi–Yau mm-fold as XX, taking J,ω,ΩJ,\omega,\Omega as given. Note that if (X,J,ω,Ω)(X,J,\omega,\Omega) is a CY mm-fold and θ∈[0,2​π)\theta\in[0,2\pi) then (X,J,ω,ei​θ​Ω)(X,J,\omega,{\rm e}^{i\theta}\Omega) is also a CY mm-fold. It can be shown that gg is Ricci-flat with holonomy group Hol(g){\textstyle\mathop{\rm Hol}}(g) contained in SU(m)\mathop{\rm SU}(m), and that ∇ω=∇Ω=0\nabla\omega=\nabla\Omega=0, where ∇\nabla is the Levi-Civita connection of gg. Furthermore, as Ω\Omega is a nonvanishing section of the canonical bundle KX=Λm,0​XK_{X}=\Lambda^{m,0}X of XX, we see that KXK_{X} is trivial, so that the first Chern class c1​(X)c_{1}(X) is zero.

Here is how to construct examples of Calabi–Yau manifolds. Using algebraic geometry one can find many examples of compact complex manifolds (X,J)(X,J) with c1​(X)=0c_{1}(X)=0, for instance as hypersurfaces in toric varieties. If XX is simply-connected, KXK_{X} is trivial, and has a nonvanishing holomorphic section Ω\Omega.

If XX admits Kähler metrics, then as c1​(X)=0c_{1}(X)=0 Yau’s solution of the Calabi Conjecture shows that there exists a unique Ricci-flat Kähler metric gg in each Kähler class, with Kähler form ω\omega. It then follows that ∇ω=∇Ω=0\nabla\omega=\nabla\Omega=0, and therefore that ωm\omega^{m} is a constant multiple of Ω∧Ω¯\Omega\wedge\bar{\Omega}. We can rescale Ω\Omega by a constant factor to make (7) hold, and then (X,J,ω,Ω)(X,J,\omega,\Omega) is a CY mm-fold.

We move on to discuss special Lagrangian submanifolds of Calabi–Yau manifolds. Following Definition 2.1, we define:

[03KL]

Definition 2.6 Let (X,J,ω,Ω)(X,J,\omega,\Omega) be a Calabi–Yau mm-fold with metric gg, and NN an oriented real mm-dimensional submanifold of XX. We call NN a special Lagrangian submanifold, or SL mm-fold for short, if NN is calibrated with respect to ReΩ\mathop{\rm Re}\Omega.

Then Proposition 2.3 gives:

[03KM]
Proposition 2.7

Let (X,J,ω,Ω)(X,J,\omega,\Omega) be a Calabi–Yau mm-fold, and NN a real mm-dimensional submanifold of XX. Then there is a unique orientation on NN making it into an SL mm-fold if and only if ω|N≡0\omega|_{N}\equiv 0 and ImΩ|N≡0\mathop{\rm Im}\Omega|_{N}\equiv 0.

Now ω\omega and ImΩ\mathop{\rm Im}\Omega are closed forms on XX, and so if NN is an mm-dimensional submanifold of XX then we can consider the de Rham cohomology classes [ω|N][\omega|_{N}] in H2​(N,ℝ)H^{2}(N,\mathbin{\mathbb{R}}) and [ImΩ|N][\mathop{\rm Im}\Omega|_{N}] in Hm​(N,ℝ)H^{m}(N,\mathbin{\mathbb{R}}). Clearly, by the proposition, these have to be zero for NN to be an SL mm-fold. Furthermore, they are invariant under continuous deformations of NN as a submanifold in XX, and so they have to be zero for any deformation of NN to be special Lagrangian. So we prove:

[03KN]
Corollary 2.8

Let (X,J,ω,Ω)(X,J,\omega,\Omega) be a Calabi–Yau mm-fold, and NN a compact mm-dimensional submanifold of XX. Then there exists a special Lagrangian submanifold N′N^{\prime} of XX isotopic to NN in XX only if [ω|N]=0[\omega|_{N}]=0 in H2​(N,ℝ)H^{2}(N,\mathbin{\mathbb{R}}) and [ImΩ|N]=0[\mathop{\rm Im}\Omega|_{N}]=0 in Hm​(N,ℝ)H^{m}(N,\mathbin{\mathbb{R}}).

This gives us a cohomological obstruction to finding special Lagrangian submanifolds in XX. The deformation theory of special Lagrangian submanifolds was studied by McLean [14, §3], who proved the following result.

[03KP]
Theorem 2.9

Let (X,J,ω,Ω)(X,J,\omega,\Omega) be a Calabi–Yau mm-fold, and NN a compact special Lagrangian submanifold of XX. Then the moduli space ℳ\mathcal{M} of special Lagrangian submanifolds in XX is near NN a smooth manifold of dimension b1​(N)b^{1}(N), the first Betti number of NN.

The idea in the proof of this theorem is that an infinitesimal deformation of NN as a submanifold in XX corresponds to a section of the normal bundle ν\nu of NN in XX. But because NN is Lagrangian, contracting with ω\omega gives an isomorphism between the vector bundles ν\nu and T∗​NT^{*}N over NN. So there is a 1-1 correspondence between infinitesimal deformations of NN in XX and 1-forms α\alpha on NN.

McLean shows that α\alpha corresponds to an infinitesimal deformation of NN as an SL submanifold if and only if d​α=d∗​α=0{\rm d}\alpha={\rm d}^{*}\alpha=0. But as NN is compact, by Hodge theory the vector space of 1-forms α\alpha with d​α=d∗​α=0{\rm d}\alpha={\rm d}^{*}\alpha=0 is isomorphic to H1​(N,ℝ)H^{1}(N,\mathbin{\mathbb{R}}), and so has dimension b1​(N)b^{1}(N).

Our next result concerns the stability of compact special Lagrangian submanifolds NN under small deformations of the underlying Calabi–Yau mm-fold (X,J,ω,Ω)(X,J,\omega,\Omega). McLean does not discuss this question, but it can be answered by the same techniques used to prove Theorem 2.9.

[03KQ]
Theorem 2.10

Let (X,J,ω,Ω)(X,J,\omega,\Omega) be a Calabi–Yau mm-fold, and NN a compact special Lagrangian mm-fold in XX. Suppose (X,J~,ω~,Ω~)(X,\tilde{J},\tilde{\omega},\tilde{\Omega}) is a nearby Calabi–Yau structure on XX. Provided (X,J~,ω~,Ω~)(X,\tilde{J},\tilde{\omega},\tilde{\Omega}) is sufficiently close to (X,J,ω,Ω)(X,J,\omega,\Omega), there exists a special Lagrangian mm-fold N~\tilde{N} in (X,J~,ω~,Ω~)(X,\tilde{J},\tilde{\omega},\tilde{\Omega}) close to NN in XX if and only if [ω~|N]=0[\tilde{\omega}|_{N}]=0 in H2​(N,ℝ)H^{2}(N,\mathbin{\mathbb{R}}) and [ImΩ~|N]=0[\mathop{\rm Im}\tilde{\Omega}|_{N}]=0 in Hm​(N,ℝ)H^{m}(N,\mathbin{\mathbb{R}}).

Note that the condition [ω~|N]=0[\tilde{\omega}|_{N}]=0 in H2​(N,ℝ)H^{2}(N,\mathbin{\mathbb{R}}) is automatically satisfied if the image of H2​(N,ℝ)H_{2}(N,\mathbin{\mathbb{R}}) in H2​(X,ℝ)H_{2}(X,\mathbin{\mathbb{R}}) is zero, and the condition [ImΩ~|N]=0[\mathop{\rm Im}\tilde{\Omega}|_{N}]=0 can always be satisfied by choosing the phase of Ω~\tilde{\Omega} correctly. So the conditions [ω~|N]=[ImΩ~|N]=0[\tilde{\omega}|_{N}]=[\mathop{\rm Im}\tilde{\Omega}|_{N}]=0 are often not very stringent.

[03KR]

2.3 Almost Calabi–Yau manifolds and genericity

Later in the paper we will discuss fibrations of Calabi–Yau 3-folds by special Lagrangian 3-folds. We will be particularly interested in the question of what kind of fibrations one should expect in a generic Calabi–Yau 3-fold. Now when one speaks of a geometric object as generic, usually one thinks of it as chosen at random out of an infinite-dimensional family of similar geometric objects.

However, the family of Calabi–Yau structures (X,J,ω,Ω)(X,J,\omega,\Omega) on a compact 6-manifold XX, up to diffeomorphism, is only finite-dimensional, of dimension h1,1​(X)+2​h2,1​(X)+1h^{1,1}(X)+2h^{2,1}(X)+1. Thus the family of Calabi–Yau structures on a compact 6-manifold is too small for the device of picking a generic Calabi–Yau 3-fold XX to be really useful in a proof.

To get round this we introduce the following generalizations of Calabi–Yau and special Lagrangian geometry.

[03KS]

Definition 2.11 Let m⩾2m\geqslant 2. An almost Calabi–Yau mm-fold, or ACY mm-fold for short, is a quadruple (X,J,ω,Ω)(X,J,\omega,\Omega) such that (X,J)(X,J) is a compact mm-dimensional complex manifold, ω\omega is the Kähler form of a Kähler metric gg on XX, and Ω\Omega is a non-vanishing holomorphic (m,0)(m,0)-form on XX.

The difference between this and Definition 2.2 is that we do not require ω\omega and Ω\Omega to satisfy equation (7). For some purposes it may be useful to restrict to real analytic Kähler forms ω\omega, but we will not worry about this in this paper. Here is the appropriate definition of SL mm-folds in ACY mm-folds.

[03KT]

Definition 2.12 Let (X,J,ω,Ω)(X,J,\omega,\Omega) be an almost Calabi–Yau mm-fold with metric gg, and NN a real mm-dimensional submanifold of XX. We call NN a special Lagrangian submanifold, or SL mm-fold for short, if ω|N≡ImΩ|N≡0\omega|_{N}\equiv\mathop{\rm Im}\Omega|_{N}\equiv 0. It easily follows that ReΩ|N\mathop{\rm Re}\Omega|_{N} is a nonvanishing mm-form on NN. Thus NN is orientable, with a unique orientation in which ReΩ|N\mathop{\rm Re}\Omega|_{N} is positive.

By Proposition 2.7, if (X,J,ω,Ω)(X,J,\omega,\Omega) is Calabi–Yau rather than almost Calabi–Yau, then NN is special Lagrangian in the sense of Definition 2.2. Thus, this is a genuine extension of the idea of special Lagrangian submanifold.

The idea of extending special Lagrangian geometry to almost Calabi–Yau manifolds is not new. It appears in the work of Goldstein, who introduced the term ‘almost Calabi–Yau’, and Bryant [1, §1], who uses the term ‘special Kähler’ instead of ‘almost Calabi–Yau’.

Many of the good properties of special Lagrangian submanifolds in Calabi–Yau manifolds also apply in almost Calabi–Yau manifolds. For instance:

[03KU]
Theorem 2.13

Corollary 2.8 and Theorems 2.9 and 2.10 also hold in almost Calabi–Yau manifolds rather than Calabi–Yau manifolds.

This is because the proofs of these results only really depend on the conditions ω|N≡ImΩ|N≡0\omega|_{N}\equiv\mathop{\rm Im}\Omega|_{N}\equiv 0, and the pointwise connection (7) between ω\omega and Ω\Omega is not important. Let (X,J,ω,Ω)(X,J,\omega,\Omega) be an ACY mm-fold, with metric gg. In general, SL mm-folds in XX are neither calibrated nor minimal with respect to gg.

However, let f:X→(0,∞)f:X\rightarrow(0,\infty) be the unique smooth function such that f2​m​ωm/m!=(−1)m⁡(m−1)/2​(i/2)m​Ω∧Ω¯f^{2m}\omega^{m}/m!=(-1)^{m(m-1)/2}(i/2)^{m}\Omega\wedge\bar{\Omega}, and define g~\tilde{g} to be the conformally equivalent metric f2​gf^{2}g on XX. Then it is easy to show that ReΩ\mathop{\rm Re}\Omega is a calibration on the Riemannian manifold (X,g~)(X,\tilde{g}), and that SL mm-folds NN in (X,J,ω,Ω)(X,J,\omega,\Omega) are calibrated with respect to it, so that they are minimal with respect to g~\tilde{g}.

We can also give a volume bound for compact SL mm-folds in XX using these ideas. If NN is an SL mm-fold in XX then ReΩ|Tx​N=f(x)mvolTx​N\mathop{\rm Re}\Omega|_{T_{x}N}=f(x)^{m}\mathop{\rm vol}_{T_{x}N} for each x∈Nx\in N, where volTx​N\mathop{\rm vol}_{T_{x}N} is computed using gg. Integrating this over NN yields

vol(N)⩽C​∫NReΩ=C⁡[ReΩ]⋅[N],where C=(infx∈Xf⁡(x))−m.\mathop{\rm vol}(N)\leqslant C\int_{N}\mathop{\rm Re}\Omega=C[\mathop{\rm Re}\Omega]\cdot[N],\quad\text{where $C=\bigl({\textstyle\inf_{x\in X}}f(x)\bigr)^{-m}$.}

This is a bound on the volume of NN using gg, depending only on (X,J,ω,Ω)(X,J,\omega,\Omega) and the homology class of NN.

Another important point about SL mm-folds in ACY mm-folds is that locally, in a small neighbourhood of any point, they look like SL mm-folds in CY mm-folds. Therefore we expect the singularities of SL mm-folds in ACY mm-folds to behave in the same way as singularities of SL mm-folds in CY mm-folds.

Almost Calabi–Yau mm-folds are useful in problems involving special Lagrangian fibrations because it is very easy to write down explicit examples of ACY mm-folds, and so to study fibrations on them, whereas Calabi–Yau structures on the same mm-folds are usually given only by an existence theorem, with no explicit formula for the metric or Kähler form.

The reason why almost Calabi–Yau manifolds are useful in discussing problems involving generic Calabi–Yau manifolds is the following. Although the family of Calabi–Yau structures on a compact manifold XX is finite-dimensional, the family of almost Calabi–Yau structures on the same manifold is infinite-dimensional. So arguments involving choosing a generic almost Calabi–Yau structure on XX will be far more powerful.

Here is an example of the kind of thing the author has in mind, which we will return to in §3.1. Let (X,J,ω,Ω)(X,J,\omega,\Omega) be a CY 3-fold, and NN a compact, nonsingular, immersed SL 3-fold in XX. If NN is generically placed in XX as an immersed submanifold then it will intersect itself in only finitely many points, but if NN is very nongeneric it could intersect itself in a 1-dimensional set such as a circle.

Now if we choose a generic Calabi–Yau structure on XX, we cannot guarantee that NN will not intersect itself in a circle, because we cannot completely eliminate the possibility that by a miracle, all the Calabi–Yau structures on XX happen to have this property. (Indeed, this is to be expected when XX is a product K​3×T2K3\times T^{2}). However, one can show that in a generic almost Calabi–Yau 3-fold, any compact, nonsingular, immersed SL 3-fold NN intersects itself in only finitely many points.

[03KV]

3 The SYZ Conjecture

In 1996, Strominger, Yau and Zaslow [22] suggested a geometrical interpretation of Mirror Symmetry between Calabi–Yau 3-folds X,X^X,\hat{X} in terms of dual fibrations by special Lagrangian 3-tori. Their proposal was rewritten for mathematicians by Morrison [15], and is known as the SYZ Conjecture. Here is an attempt to state it.

The SYZ Conjecture. Suppose XX and X^\hat{X} are mirror Calabi–Yau 33-folds. Then (under some additional conditions) there should exist a compact topological 33-manifold BB and surjective, continuous maps f:X→Bf:X\rightarrow B and f^:X^→B\hat{f}:\hat{X}\rightarrow B, such that

  • (i)

    There exists a dense open set B0⊂BB_{0}\subset B, such that for each b∈B0b\in B_{0}, the fibres f−1​(b)f^{-1}(b) and f^−1​(b)\hat{f}^{-1}(b) are nonsingular special Lagrangian 33-tori T3T^{3} in XX and X^\hat{X}. Furthermore, f−1​(b)f^{-1}(b) and f^−1​(b)\hat{f}^{-1}(b) are in some sense dual to one another.

  • (ii)

    For each b∈Δ=B∖B0b\in\Delta=B\setminus B_{0}, the fibres f−1​(b)f^{-1}(b) and f^−1​(b)\hat{f}^{-1}(b) are expected to be singular special Lagrangian 33-folds in XX and X^\hat{X}.

We call ff and f^\hat{f} special Lagrangian fibrations, and f−1​(b)f^{-1}(b), f^−1​(b)\hat{f}^{-1}(b) for b∈Δb\in\Delta the singular fibres. The original discussion of [22] is written in physics language, and is mathematically rather vague. In particular, three areas need clarification to make the SYZ conjecture a precise mathematical statement:

  • (a)

    What are the conditions on XX and X^\hat{X} for these dual fibrations to exist? Strominger et al. only argue that the conjecture should hold in a neighbourhood of the ‘large complex structure limit’, and it is not expected that the conjecture holds for all mirror pairs. For a definition of the large complex structure limit, see Morrison [16, §6].

  • (b)

    What does it mean for two 3-tori L,L^L,\hat{L} in X,X^X,\hat{X} to be dual to one another? On the level of homology and cohomology this makes sense, for instance as an isomorphism H1​(L,ℤ)≅H1​(L^,ℤ)H^{1}(L,\mathbin{\mathbb{Z}})\cong H_{1}(\hat{L},\mathbin{\mathbb{Z}}). If the metrics g,g^g,\hat{g} on LL and L^\hat{L} are flat, as should happen in the (degenerate) large complex structure limit, then duality between gg and g^\hat{g} also makes sense. But we do not have a geometrical concept of duality between LL and L^\hat{L} when g,g^g,\hat{g} are curved.

  • (c)

    What is the nature of the ‘singular fibres’ of the fibration, and what do f,f^f,\hat{f} look like near the singularities?

In this paper we shall try to answer question (c). First we discuss the literature on the subject so far. The most popular assumption appears to be that BB is a smooth 3-manifold, and that f:X→Bf:X\rightarrow B and f^:X^→B\hat{f}:\hat{X}\rightarrow B are smooth maps. This idea and its consequences are developed by Mark Gross [5, 6, 7].

Other authors have also made use of smooth fibrations. Zharkov [23] proves that mm-dimensional Calabi–Yau hypersurfaces in toric varieties admit smooth, non-Lagrangian TmT^{m}-fibrations over 𝒮m{\mathcal{S}}^{m}. Gross and Wilson [8] construct smooth SL fibrations of a class of degenerate Calabi–Yau 3-folds. Goldstein [2, 3, 4] gives examples of smooth SL fibrations in noncompact Calabi–Yau manifolds with large symmetry groups, and in large subsets of almost Calabi–Yau hypersurfaces in toric varieties.

However, some authors have also considered fibrations which are not smooth. In a series of papers, Wei-Dong Ruan [18, 19, 20, 21] constructs piecewise smooth Lagrangian fibrations of almost Calabi–Yau hypersurfaces using a ‘gradient flow’ method. These will be discussed in §3.2. But first we explain why, in the author’s view, generic (almost) Calabi–Yau 3-folds cannot admit smooth special Lagrangian fibrations.

[03KW]

3.1 Why generic SL fibrations cannot be smooth

One of the key claims of this paper is that generic special Lagrangian fibrations are not smooth. So we should begin by defining what we mean by ‘generic’ here.

[03KX]

Definition 3.1 Let (X,J,ω,Ω)(X,J,\omega,\Omega) be a Calabi–Yau or almost Calabi–Yau 3-fold, and f:X→Bf:X\rightarrow B a special Lagrangian fibration of (X,J,ω,Ω)(X,J,\omega,\Omega). We shall say that some property of ff is generic if for all Kähler forms ω~\tilde{\omega} on XX in the same Kähler class as ω\omega and sufficiently close to ω\omega, there exists close to ff a special Lagrangian fibration f~:X→B\tilde{f}:X\rightarrow B of the almost Calabi–Yau 3-fold (X,J,ω~,Ω)(X,J,\tilde{\omega},\Omega) with the same property. Examples of properties of ff that might or might not be generic are: existence, smoothness, every singular fibre has only finitely many singular points, and so on.

Here is the reasoning behind this definition. We intend to call a property of a special Lagrangian fibration generic if it holds for fibrations of all nearby almost Calabi–Yau 3-folds (X,J~,ω~,Ω~)(X,\tilde{J},\tilde{\omega},\tilde{\Omega}). Now if NN is a smooth fibre of ff, then Corollary 2.8 and Theorem 2.10 show that the only obstructions to finding an SL 3-fold in (X,J~,ω~,Ω~)(X,\tilde{J},\tilde{\omega},\tilde{\Omega}) near NN are that [ω~|N]≡[ImΩ~|N]≡0[\tilde{\omega}|_{N}]\equiv[\mathop{\rm Im}\tilde{\Omega}|_{N}]\equiv 0.

To make sure this holds, we restrict our attention to ACY 3-folds (X,J~,ω~,Ω~)(X,\tilde{J},\tilde{\omega},\tilde{\Omega}) with [ω~]=[ω][\tilde{\omega}]=[\omega] in H2​(X,ℝ)H^{2}(X,\mathbin{\mathbb{R}}) and [ImΩ~]=[ImΩ][\mathop{\rm Im}\tilde{\Omega}]=[\mathop{\rm Im}\Omega] in H3​(X,ℝ)H^{3}(X,\mathbin{\mathbb{R}}). But one can show that if [ImΩ~]=[ImΩ][\mathop{\rm Im}\tilde{\Omega}]=[\mathop{\rm Im}\Omega] and (X,J,Ω)(X,J,\Omega), (X,J~,Ω~)(X,\tilde{J},\tilde{\Omega}) are close, then they are isomorphic. So we may as well fix J~=J\tilde{J}=J and Ω~=Ω\tilde{\Omega}=\Omega, and just vary the Kähler form ω~\tilde{\omega} within the Kähler class of ω\omega.

It could be asked why Definition 3.1 is a good definition, if we are only interested in Calabi–Yau and not in almost Calabi–Yau 3-folds. My answer is that anything that is true of special Lagrangian fibrations of generic Calabi–Yau 3-folds with holonomy SU(3)\mathop{\rm SU}(3) really ought to be true of nearby generic almost Calabi–Yau 3-folds as well, as we know of no relevant geometric properties of such CY 3-folds that do not also hold for ACY 3-folds.

We now give some reasons why generic special Lagrangian fibrations f:X→Bf:X\rightarrow B cannot be smooth. Gross [6, §1] gives the following rough argument why ff should be smooth. Let Xb=f−1​(b)X_{b}=f^{-1}(b) be a singular fibre for b∈Bb\in B. Then XbX_{b} is nonsingular at a general point x∈Xbx\in X_{b}. Using the exponential map at xx on the normal vector space νx\nu_{x} to XbX_{b} at xx gives a natural, smooth local section for f:X→Bf:X\rightarrow B. Projecting this down to BB using ff, we define the structure of a smooth manifold on BB near bb. Hopefully ff will be smooth with respect to this.

The problem with this argument is as follows. For two different nonsingular points x,yx,y in XbX_{b}, the maps f∘expx:νx→Bf\circ\exp_{x}:\nu_{x}\rightarrow B and f∘expy:νy→Bf\circ\exp_{y}:\nu_{y}\rightarrow B do define smooth structures on BB near bb. However, in general these will be different smooth structures. There will be no one smooth structure near bb such that ff is smooth at every point of XbX_{b}, even at every nonsingular point.

Next, we discuss the codimension of the set of singular fibres in the base BB, and the dimension of the singular set in a generic singular fibre XbX_{b}. The assumption that f:X→Bf:X\rightarrow B is smooth has strong consequences for these. In particular, Gross [6, p. 10] proves:

[03KY]
Proposition 3.2

Suppose XX is a Calabi–Yau mm-fold, BB a smooth mm-manifold, and f:X→Bf:X\rightarrow B a smooth special Lagrangian fibration. Then f−1​(b)f^{-1}(b) is nonsingular for all bb outside a subset Δ\Delta of Hausdorff codimension at least two in BB.

His proof uses the fact that the fibres are both Lagrangian and minimal. The Lagrangian assumption is used to prove [6, Prop. 2.2] that if x∈Xbx\in X_{b} and rankdx​f:Tx​X→Tb​B\mathop{\rm rank}{\rm d}_{x}f:T_{x}X\rightarrow T_{b}B is kk, then XbX_{b} contains a kk-dimensional submanifold through xx on which rankd​f\mathop{\rm rank}{\rm d}f is kk. But by a result of Almgren, the singularities of a minimal submanifold are of Hausdorff codimension at least two. Combining these two shows that rankdx​f\mathop{\rm rank}{\rm d}_{x}f cannot be m−1m-1, so that if xx is a singular point of XbX_{b} then rankdx​f⩽m−2\mathop{\rm rank}{\rm d}_{x}f\leqslant m-2.

Using these ideas, one can show that if f:X→Bf:X\rightarrow B is a smooth special Lagrangian fibration of an (almost) Calabi–Yau 3-fold, and Δ\Delta the set of b∈Bb\in B with Xb=f−1​(b)X_{b}=f^{-1}(b) singular, then under good circumstances we expect the following properties:

  • (i)

    Δ\Delta is a union Δ0∪Δ1\Delta_{0}\cup\Delta_{1}, where Δ0\Delta_{0} is a finite set of points, and Δ1\Delta_{1} a finite set of open intervals. Essentially, Δ\Delta is a graph in BB.

  • (ii)

    For each b∈Δ1b\in\Delta_{1}, the singular set of XbX_{b} is a finite number of circles 𝒮1{\mathcal{S}}^{1}, and the singularities are locally modelled on L×ℝL\times\mathbin{\mathbb{R}} in ℂ2×ℂ\mathbin{\mathbb{C}}^{2}\times\mathbin{\mathbb{C}}, where LL is a special Lagrangian 2-fold in ℂ2\mathbin{\mathbb{C}}^{2} with an isolated singularity at 0.

That is, singular fibres occur in codimension two in the base, and the generic singular fibre has a one-dimensional singular set.

Ruan [18, §4] argues that as in two dimensions special Lagrangian fibrations have singular fibres of codimension two in the base, it is reasonable to expect this in three dimensions as well. The problem with this argument is that two dimensions is a special case: SL 2-folds in a Calabi–Yau 2-fold XX are equivalent to complex curves with respect to an alternative complex structure on XX. So singularities occur in complex codimension one, which is real codimension two. But for m⩾3m\geqslant 3 there is no such complex interpretation of SL mm-folds.

Now in the fibrations we shall define later in the paper, singular fibres occur in codimension one in the base, and all the singular fibres have zero-dimensional singular sets. We claim that is what one should expect of generic special Lagrangian fibrations in three dimensions.

Here is a heuristic argument why fibrations satisfying (i) and (ii) above cannot be generic. Suppose XX is a generic almost Calabi–Yau 3-fold, f:X→Bf:X\rightarrow B a special Lagrangian fibration satisfying (i) and (ii), and let b∈Δ1b\in\Delta_{1}. Then the singular set of XbX_{b} is a finite number of circles 𝒮1{\mathcal{S}}^{1}, with singularities locally modelled on L×ℝL\times\mathbin{\mathbb{R}} in ℂ2×ℂ\mathbin{\mathbb{C}}^{2}\times\mathbin{\mathbb{C}}, where LL is an SL 2-fold in ℂ2\mathbin{\mathbb{C}}^{2} with an isolated singularity at 0.

As XX is generic, it is reasonable to expect that LL should be the most generic kind of singular SL 2-fold. But the most generic singularity of SL 2-folds is the normal crossing, where LL is the union of two distinct SL 2-planes ℝ2\mathbin{\mathbb{R}}^{2} in ℂ2\mathbin{\mathbb{C}}^{2} intersecting at 0. Assume the singularities of XbX_{b} are of this kind.

Then XbX_{b} is in fact nonsingular as an immersed 3-submanifold. So we can regard XbX_{b} as a compact, nonsingular, immersed SL 3-fold in XX. It intersects itself in a collection of circles, but a generic immersed 3-submanifold in XX should intersect itself in finitely many points. Thus, as an immersed 3-submanifold XbX_{b} is not generic, and indeed highly non-generic, as submanifolds of this kind are of infinite codimension in the family of all immersed 3-submanifolds.

Now the local deformation theory of compact immersed SL 3-folds is well understood (see for example Theorems 2.9 and 2.10). It is easy to show that in a generic almost Calabi–Yau 3-fold, compact immersed SL 3-folds should be of at most finite codimension in the family of all immersed 3-submanifolds. Therefore XbX_{b} is an SL 3-fold of a kind that should not occur in a generic almost Calabi–Yau 3-fold, which is a contradiction. The author believes that this argument could be upgraded to a rigorous proof without difficulty.

[03KZ]

3.2 Ruan’s Lagrangian fibrations by gradient flow

We now describe some aspects of the work of Wei-Dong Ruan in [18, 19, 20, 21]. This is based on the following idea. Suppose we are given a family of Calabi–Yau hypersurfaces XX in some projective toric variety. As in [18, 19, 21] we take this to be a pencil of quintics {Xc:c∈ℂ∪{∞}}\bigl\{X_{c}:c\in\mathbin{\mathbb{C}}\cup\{\infty\}\bigr\} in ℂ​ℙ4\mathbb{CP}^{4}, where

Xc={[z0,…,z4]∈ℂ​ℙ4:p⁡(z0,…,z4)+c​q​(z0,…,z4)=0},X_{c}=\bigl\{[z_{0},\ldots,z_{4}]\in\mathbb{CP}^{4}:p(z_{0},\ldots,z_{4})+c\,q(z_{0},\ldots,z_{4})=0\bigr\},

and p,qp,q are homogeneous, linearly independent quintic polynomials.

Choose a Kähler metric gg on ℂ​ℙ4\mathbb{CP}^{4}, with Kähler form ω\omega. Let ss be the meromorphic function p⁡(z0,…,z4)/q⁡(z0,…,z4)p(z_{0},\ldots,z_{4})/q(z_{0},\ldots,z_{4}) on ℂ​ℙ4∖X∞\mathbb{CP}^{4}\setminus X_{\infty}, and let f=Re(s)f=\mathop{\rm Re}(s). Define a vector field vv on ℂ​ℙ4\mathbb{CP}^{4} by va=|d​f|−2​ga​b​(d​f)bv^{a}=|{\rm d}f|^{-2}g^{ab}({\rm d}f)_{b}, using the index notation for tensors. Note that vv becomes infinite on X∞X_{\infty}, as ff is infinite there, and also on the set of points where d​f=0{\rm d}f=0. Ruan shows that flowing along the vector field vv for time tt takes XcX_{c} to Xc+tX_{c+t} for each c∈ℂc\in\mathbin{\mathbb{C}}, at least where vv is finite. Furthermore, the flow takes Lagrangian submanifolds of XcX_{c} to Lagrangian submanifolds of Xc+tX_{c+t}.

Ruan’s method is to set p⁡(z0,…,z4)=z0​z1​z2​z3​z4p(z_{0},\ldots,z_{4})=z_{0}z_{1}z_{2}z_{3}z_{4}, so that X0X_{0} is the union of five copies of ℂ​ℙ3\mathbb{CP}^{3} in ℂ​ℙ4\mathbb{CP}^{4}, a very degenerate, singular quintic. He defines an explicit Lagrangian fibration of X0X_{0}, with respect to the Fubini–Study metric on ℂ​ℙ4\mathbb{CP}^{4}. Then he uses the flow from X0X_{0} to XtX_{t} to translate this fibration to a Lagrangian fibration of the general, nonsingular quintic XtX_{t} for t∈ℝ∖{0}t\in\mathbin{\mathbb{R}}\setminus\{0\}. One has to consider carefully what happens when vv is infinite, and around the singularities of X0X_{0}. But it turns out that these do not spoil things, and we end up with a genuine Lagrangian fibration of XtX_{t}.

Part of the motivation for Ruan’s construction is that X0X_{0} is considered to be the ‘large complex structure limit’ of Calabi–Yau quintics. Thus, the construction starts with an explicit fibration of the singular ‘large complex structure limit’ 3-fold, and deforms it to a fibration of nonsingular 3-folds close to this limit. This is quite a natural thing to do from the String Theory point of view, and others such as Zharkov and Goldstein have tried similar ideas.

Now we are interested in the nature of the set of singular fibres in Ruan’s fibrations, and in their singularities. Ruan proves [19, Th. 2.2]:

[03L0]
Theorem 3.3

Let XtX_{t} be a generic, nonsingular quintic in ℂ​ℙ4\mathbb{CP}^{4} near the large complex structure limit. Then Ruan’s construction yields a Lagrangian fibration f:Xt→𝒮3f:X_{t}\rightarrow{\mathcal{S}}^{3} with the following properties:

  • (i)

    ff is a piecewise smooth map.

  • (ii)

    The set of singular points in XtX_{t} of singular fibres of ff is a holomorphic curve in XtX_{t}.

  • (iii)

    The set Δ={b∈B:f−1(b)\Delta=\{b\in B:f^{-1}(b) is singular}\} is a 22-manifold with boundary in 𝒮3{\mathcal{S}}^{3}. It splits naturally into a disjoint union Δ=Δ0∪Δ1∪Δ2\Delta=\Delta_{0}\cup\Delta_{1}\cup\Delta_{2}, where Δ2\Delta_{2} is the 22-dimensional interior of Δ\Delta, and Δ1\Delta_{1} is a finite set of open intervals on the boundary of Δ\Delta, and Δ0\Delta_{0} is a finite set.

  • (iv)

    If b∈𝒮3∖Δb\in{\mathcal{S}}^{3}\setminus\Delta then f−1​(b)f^{-1}(b) is diffeomorphic to T3T^{3}.

  • (v)

    If b∈Δ2b\in\Delta_{2} then f−1​(b)f^{-1}(b) is a T3T^{3} with two isotopic circles collapsed to two singular points.

  • (vi)

    If b∈Δ1b\in\Delta_{1} then f−1​(b)f^{-1}(b) is a T3T^{3} with one circle collapsed to one singular point.

  • (vii)

    If b∈Δ0b\in\Delta_{0} then f−1​(b)f^{-1}(b) is a T3T^{3} with one T2T^{2} collapsed to one singular point.

The properties of Ruan’s fibrations given above are very similar to the fibrations we shall propose later in the paper. In particular, versions of parts (i) and (iii)–(vi) will hold for our fibrations. For part (ii), the set of singular points in the fibrations we shall discuss need not be a holomorphic curve, but it will be a real 2-manifold in XX that is close to being holomorphic. Only in part (vii) do we seriously diverge from Ruan, as our fibrations will not contain fibres in which T2T^{2} collapses to a point.

Ruan himself, however, appears to regard these properties of his fibrations as a problem (see for instance [21, Conj. 1.1], where he conjectures that special Lagrangian fibrations are always smooth, the ‘Precise SYZ mirror conjecture’ in [20, §9], and many other places), and spends much effort in showing how to deform his fibrations to smooth Lagrangian fibrations. One moral of this paper may be that Ruan’s construction gives something quite close to the right answer, and it might even be possible to modify it to yield genuine special Lagrangian fibrations of (almost) Calabi–Yau manifolds.

[03L1]

4 Two simple SL fibrations of ℂ3\mathbin{\mathbb{C}}^{3}

We now describe two very elementary examples of (smooth) special Lagrangian fibrations of ℂ3\mathbin{\mathbb{C}}^{3}, which we will build on later. The results of this section are not new, and can mostly be found in Harvey and Lawson [9, §III.3] and the author [10, §3]. The proofs are easy and will generally be omitted. Here is our first family of SL 3-folds in ℂ3\mathbin{\mathbb{C}}^{3}.

[03L2]
Theorem 4.1

Let a,b,c∈ℝa,b,c\in\mathbin{\mathbb{R}}, and define a subset Ka,b,cK_{a,b,c} in ℂ3\mathbin{\mathbb{C}}^{3} by

Ka,b,c={(z1,z2,z3)∈ℂ3:|z1|2−|z2|2=a,Re(z1z2)=b,Im(z3)=c}.\begin{split}K_{a,b,c}=\bigl\{(z_{1},z_{2},z_{3})\in\mathbin{\mathbb{C}}^{3}:\,&|z_{1}|^{2}-|z_{2}|^{2}=a,\\ &\mathop{\rm Re}(z_{1}z_{2})=b,\quad\mathop{\rm Im}(z_{3})=c\bigr\}.\end{split} (8)

Then Ka,b,cK_{a,b,c} is a special Lagrangian 33-fold in ℂ3\mathbin{\mathbb{C}}^{3}. If a,ba,b are not both zero, then Ka,b,cK_{a,b,c} is a nonsingular embedded submanifold diffeomorphic to 𝒮1×ℝ2{\mathcal{S}}^{1}\times\mathbin{\mathbb{R}}^{2}. Also K0,0,cK_{0,0,c} is the union of the two special Lagrangian 33-planes

Πc+={(z,iz¯,t+ic):z∈ℂ,t∈ℝ}andΠc−={(z,−iz¯,t+ic):z∈ℂ,t∈ℝ},\begin{split}\Pi^{+}_{c}&=\bigl\{(z,i\bar{z},t+ic):z\in\mathbin{\mathbb{C}},\quad t\in\mathbin{\mathbb{R}}\bigr\}\\ \text{and}\qquad\Pi^{-}_{c}&=\bigl\{(z,-i\bar{z},t+ic):z\in\mathbin{\mathbb{C}},\quad t\in\mathbin{\mathbb{R}}\bigr\},\end{split} (9)

which intersect in the real line {(0,0,t+ic):t∈ℝ}\bigl\{(0,0,t+ic):t\in\mathbin{\mathbb{R}}\bigr\}. It is singular as an embedded submanifold, but nonsingular as an immersed submanifold.

Clearly Ka,b,cK_{a,b,c} is invariant under the group U(1)×ℝ\mathbin{\rm U}(1)\times\mathbin{\mathbb{R}} acting on ℂ3\mathbin{\mathbb{C}}^{3} by

(ei​θ,t):(z1,z2,z3)⟼(ei​θ​z1,e−i​θ​z2,z3+t),({\rm e}^{i\theta},t):(z_{1},z_{2},z_{3})\longmapsto({\rm e}^{i\theta}z_{1},{\rm e}^{-i\theta}z_{2},z_{3}+t), (10)

and using the methods of [11] one can show that any connected SL 3-fold in ℂ3\mathbin{\mathbb{C}}^{3} invariant under this group is a subset of some Ka,b,cK_{a,b,c}. From the theorem we immediately deduce:

[03L3]
Corollary 4.2

The map f:ℂ3→ℝ3f:\mathbin{\mathbb{C}}^{3}\rightarrow\mathbin{\mathbb{R}}^{3} defined by

f:(z1,z2,z3)⟼(|z1|2−|z2|2,Re(z1​z2),Im(z3))f:(z_{1},z_{2},z_{3})\longmapsto\bigl(\,|z_{1}|^{2}-|z_{2}|^{2},\mathop{\rm Re}(z_{1}z_{2}),\mathop{\rm Im}(z_{3})\bigr) (11)

is a smooth special Lagrangian fibration of ℂ3\mathbin{\mathbb{C}}^{3}.

This fibration is the local model for the most generic kind of singularity in smooth SL fibrations of Calabi–Yau 3-folds, as studied by Gross [5, 6], for instance. Note that the set of singular fibres in ℝ3\mathbin{\mathbb{R}}^{3} is {(0,0,c):c∈ℝ}\bigl\{(0,0,c):c\in\mathbin{\mathbb{R}}\bigr\}, of codimension two, and each singular fibre has a one-dimensional singular set {(0,0,t+ic):t∈ℝ}\bigl\{(0,0,t+ic):t\in\mathbin{\mathbb{R}}\bigr\}. Also, the set of all singular points of singular fibres is {(0,0,z3):z3∈ℂ}\bigl\{(0,0,z_{3}):z_{3}\in\mathbin{\mathbb{C}}\bigr\}, a complex line in ℂ3\mathbin{\mathbb{C}}^{3}.

Here is our second family of SL 3-folds in ℂ3\mathbin{\mathbb{C}}^{3}, due originally to Harvey and Lawson [9, §III.3.A].

[03L4]
Theorem 4.3

Let a,b,c∈ℝa,b,c\in\mathbin{\mathbb{R}}, and define a subset La,b,cL_{a,b,c} in ℂ3\mathbin{\mathbb{C}}^{3} by

La,b,c={(z1,z2,z3)∈ℂ3:|z1|2−|z2|2=a,|z1|2−|z3|2=b,Im(z1z2z3)=c}.\begin{split}L_{a,b,c}=\bigl\{(z_{1},z_{2},z_{3})\in\mathbin{\mathbb{C}}^{3}:\,&|z_{1}|^{2}-|z_{2}|^{2}=a,\\ &|z_{1}|^{2}-|z_{3}|^{2}=b,\quad\mathop{\rm Im}(z_{1}z_{2}z_{3})=c\bigr\}.\end{split} (12)

Then La,b,cL_{a,b,c} is a special Lagrangian 33-fold in ℂ3\mathbin{\mathbb{C}}^{3}. Moreover

  • (i)

    L0,0,0L_{0,0,0} has one singular point at 00.

  • (ii)

    If α>0\alpha>0 then Lα,α,0L_{\alpha,\alpha,0} has singular set {(α1/2​ei​θ,0,0):θ∈[0,2​π)}\bigl\{(\alpha^{1/2}{\rm e}^{i\theta},0,0):\theta\in[0,2\pi)\bigr\}.

  • (iii)

    If α>0\alpha>0 then L−α,0,0L_{-\alpha,0,0} has singular set {(0,α1/2​ei​θ,0):θ∈[0,2​π)}\bigl\{(0,\alpha^{1/2}{\rm e}^{i\theta},0):\theta\in[0,2\pi)\bigr\}.

  • (iv)

    If α>0\alpha>0 then L0,−α,0L_{0,-\alpha,0} has singular set {(0,0,α1/2​ei​θ):θ∈[0,2​π)}\bigl\{(0,0,\alpha^{1/2}{\rm e}^{i\theta}):\theta\in[0,2\pi)\bigr\}.

All other La,b,cL_{a,b,c} are nonsingular embedded submanifolds diffeomorphic to T2×ℝT^{2}\times\mathbin{\mathbb{R}}.

Again, these 3-folds La,b,cL_{a,b,c} have a two-dimensional symmetry group, this time

U(1)2={(ei​θ1,ei​θ2,ei​θ3):θ1,θ2,θ3∈ℝ,θ1+θ2+θ3=0},\mathbin{\rm U}(1)^{2}=\bigl\{({\rm e}^{i\theta_{1}},{\rm e}^{i\theta_{2}},{\rm e}^{i\theta_{3}}):\theta_{1},\theta_{2},\theta_{3}\in\mathbin{\mathbb{R}},\quad\theta_{1}+\theta_{2}+\theta_{3}=0\bigr\}, (13)

which acts on ℂ3\mathbin{\mathbb{C}}^{3} as a subgroup of SU(3)\mathop{\rm SU}(3) by

(ei​θ1,ei​θ2,ei​θ3):(z1,z2,z3)⟼(ei​θ1​z1,ei​θ2​z2,ei​θ3​z3).({\rm e}^{i\theta_{1}},{\rm e}^{i\theta_{2}},{\rm e}^{i\theta_{3}}):(z_{1},z_{2},z_{3})\longmapsto({\rm e}^{i\theta_{1}}z_{1},{\rm e}^{i\theta_{2}}z_{2},{\rm e}^{i\theta_{3}}z_{3}). (14)

Any connected SL 3-fold in ℂ3\mathbin{\mathbb{C}}^{3} invariant under this group is a subset of some La,b,cL_{a,b,c}. The theorem immediately yields

[03L5]
Corollary 4.4

The map f:ℂ3→ℝ3f:\mathbin{\mathbb{C}}^{3}\rightarrow\mathbin{\mathbb{R}}^{3} defined by

f:(z1,z2,z3)⟼(|z1|2−|z2|2,|z1|2−|z3|2,Im(z1​z2​z3))f:(z_{1},z_{2},z_{3})\longmapsto\bigl(\,|z_{1}|^{2}-|z_{2}|^{2},|z_{1}|^{2}-|z_{3}|^{2},\mathop{\rm Im}(z_{1}z_{2}z_{3})\bigr) (15)

is a smooth special Lagrangian fibration of ℂ3\mathbin{\mathbb{C}}^{3}.

This is the local model for another, nongeneric kind of singularity in smooth SL fibrations of Calabi–Yau 3-folds. The set of singular fibres in ℝ3\mathbin{\mathbb{R}}^{3} is

{(α,α,0),(−α,0,0),(0,−α,0):α⩾0}\bigl\{(\alpha,\alpha,0),(-\alpha,0,0),(0,-\alpha,0):\alpha\geqslant 0\bigr\}

which is three half-lines meeting at a point, and is again of codimension two in ℝ3\mathbin{\mathbb{R}}^{3}. Generic singular fibres have singular fibre a circle, which is one-dimensional. Note that in a small neighbourhood of a singular point of a generic singular fibre, the fibration is a smooth deformation of the fibration of Corollary 4.2. The set of all singular points of singular fibres is

{(z,0,0),(0,z,0),(0,0,z):z∈ℂ},\bigl\{(z,0,0),(0,z,0),(0,0,z):z\in\mathbin{\mathbb{C}}\bigr\},

a singular complex curve in ℂ3\mathbin{\mathbb{C}}^{3}.

In the rest of the section we explore the structure of the singular fibres in cases (i)–(iv) of Theorem 4.3, following [10, §3].

Case (i). Define subsets L0±L_{0}^{\pm} in ℂ3\mathbin{\mathbb{C}}^{3} by

L0+={(rei​θ1,rei​θ2,rei​θ3):r⩾0,θ1,θ2,θ3∈ℝ,θ1+θ2+θ3=0},L0−={(rei​θ1,rei​θ2,rei​θ3):r⩾0,θ1,θ2,θ3∈ℝ,θ1+θ2+θ3=π}.\begin{split}&L_{0}^{+}=\bigl\{(r{\rm e}^{i\theta_{1}},r{\rm e}^{i\theta_{2}},r{\rm e}^{i\theta_{3}}):r\geqslant 0,\quad\theta_{1},\theta_{2},\theta_{3}\in\mathbin{\mathbb{R}},\quad\theta_{1}+\theta_{2}+\theta_{3}=0\bigr\},\\ &L_{0}^{-}=\bigl\{(r{\rm e}^{i\theta_{1}},r{\rm e}^{i\theta_{2}},r{\rm e}^{i\theta_{3}}):r\geqslant 0,\quad\theta_{1},\theta_{2},\theta_{3}\in\mathbin{\mathbb{R}},\quad\theta_{1}+\theta_{2}+\theta_{3}=\pi\bigr\}.\end{split} (16)

Then L0±L_{0}^{\pm} are both special Lagrangian cones on T2T^{2}, which intersect only at 0, their common singular point. But L0,0,0=L0+∪L0−L_{0,0,0}=L_{0}^{+}\cup L_{0}^{-}. Thus in this case La,b,cL_{a,b,c} splits into two pieces L0±L_{0}^{\pm}. Harvey and Lawson remark [9, p. 97] that L0±L_{0}^{\pm} are not real analytic.

Case (ii). Let α>0\alpha>0, write 𝒮1={ei​θ:θ∈[0,2​π)}{\mathcal{S}}^{1}=\bigl\{{\rm e}^{i\theta}:\theta\in[0,2\pi)\bigr\}, and define maps ϕ±1,α:𝒮1×ℂ→ℂ3\phi^{\pm}_{1,\alpha}:{\mathcal{S}}^{1}\times\mathbin{\mathbb{C}}\rightarrow\mathbin{\mathbb{C}}^{3} by

ϕ1,α+:(ei​θ,z)↦((|z|2+α)1/2​ei​θ,z,e−i​θ​z¯),\displaystyle\phi^{+}_{1,\alpha}:(e^{i\theta},z)\mapsto\bigl((|z|^{2}+\alpha)^{1/2}{\rm e}^{i\theta},z,e^{-i\theta}\bar{z}\bigr),
ϕ1,α−:(ei​θ,z)↦((|z|2+α)1/2​ei​θ,z,−e−i​θ​z¯).\displaystyle\phi^{-}_{1,\alpha}:(e^{i\theta},z)\mapsto\bigl((|z|^{2}+\alpha)^{1/2}{\rm e}^{i\theta},z,-e^{-i\theta}\bar{z}\bigr).

Now ϕ1,α±\phi_{1,\alpha}^{\pm} are smooth, injective maps 𝒮1×ℂ→ℂ3{\mathcal{S}}^{1}\times\mathbin{\mathbb{C}}\rightarrow\mathbin{\mathbb{C}}^{3}, whose first derivatives have full rank at every point. Therefore the images of ϕ1,α±\phi_{1,\alpha}^{\pm} are nonsingular submanifolds of ℂ3\mathbin{\mathbb{C}}^{3}, which are embedded and closed.

So define L1,α±=ϕ1,α±(𝒮1×ℂ)L_{1,\alpha}^{\pm}=\phi_{1,\alpha}^{\pm}({\mathcal{S}}^{1}\times\mathbin{\mathbb{C}}). An equivalent definition is

L1,α+={(z1,z2,z3)∈ℂ3:|z1|2−|z2|2=α,|z1|2−|z3|2=α,Im(z1z2z3)=0,Re(z1z2z3)⩾0},L1,α−={(z1,z2,z3)∈ℂ3:|z1|2−|z2|2=α,|z1|2−|z3|2=α,Im(z1z2z3)=0,Re(z1z2z3)⩽0}.\begin{split}L_{1,\alpha}^{+}=\bigl\{(z_{1},z_{2},z_{3})\in\mathbin{\mathbb{C}}^{3}:\,&|z_{1}|^{2}-|z_{2}|^{2}=\alpha,\quad|z_{1}|^{2}-|z_{3}|^{2}=\alpha,\\ &\mathop{\rm Im}(z_{1}z_{2}z_{3})=0,\quad\mathop{\rm Re}(z_{1}z_{2}z_{3})\geqslant 0\bigr\},\\ L_{1,\alpha}^{-}=\bigl\{(z_{1},z_{2},z_{3})\in\mathbin{\mathbb{C}}^{3}:\,&|z_{1}|^{2}-|z_{2}|^{2}=\alpha,\quad|z_{1}|^{2}-|z_{3}|^{2}=\alpha,\\ &\mathop{\rm Im}(z_{1}z_{2}z_{3})=0,\quad\mathop{\rm Re}(z_{1}z_{2}z_{3})\leqslant 0\bigr\}.\end{split} (17)

Then L1,α+L_{1,\alpha}^{+} and L1,α−L_{1,\alpha}^{-} are both nonsingular, embedded 3-submanifolds of ℂ3\mathbin{\mathbb{C}}^{3} diffeomorphic to 𝒮1×ℂ{\mathcal{S}}^{1}\times\mathbin{\mathbb{C}}. Comparing (12) and (17) we see that Lα,α,0=L1,α+∪L1,α−L_{\alpha,\alpha,0}=L_{1,\alpha}^{+}\cup L_{1,\alpha}^{-}. Since Lα,α,0L_{\alpha,\alpha,0} is an SL 3-fold we deduce that L1,α±L_{1,\alpha}^{\pm} are also SL 3-folds in ℂ3\mathbin{\mathbb{C}}^{3}, which is easy to verify directly.

Observe that L1,α+∩L1,α−={(α1/2​ei​θ,0,0):θ∈[0,2​π)}L_{1,\alpha}^{+}\cap L_{1,\alpha}^{-}=\bigl\{(\alpha^{1/2}{\rm e}^{i\theta},0,0):\theta\in[0,2\pi)\bigr\}, which is the singular set of Lα,α,0L_{\alpha,\alpha,0} given in Theorem 4.3. Thus Lα,α,0L_{\alpha,\alpha,0} is the union of two nonsingular special Lagrangian 3-folds L1,α+L_{1,\alpha}^{+} and L1,α−L_{1,\alpha}^{-}, and the singularities of Lα,α,0L_{\alpha,\alpha,0} occur at their intersection. Note that we could consider Lα,α,0L_{\alpha,\alpha,0} to be a nonsingular, immersed submanifold.

Cases (iii) and (iv). We can treat these exactly like case (ii), but with a cyclic permutation of z1,z2z_{1},z_{2} and z3z_{3}. In particular, if for α>0\alpha>0 we define

L2,α+={(z1,z2,z3)∈ℂ3:|z1|2−|z2|2=−α,|z1|2−|z3|2=0,Im(z1z2z3)=0,Re(z1z2z3)⩾0},L2,α−={(z1,z2,z3)∈ℂ3:|z1|2−|z2|2=−α,|z1|2−|z3|2=0,Im(z1z2z3)=0,Re(z1z2z3)⩽0},\displaystyle\begin{split}L_{2,\alpha}^{+}=\bigl\{(z_{1},z_{2},z_{3})\in\mathbin{\mathbb{C}}^{3}:\,&|z_{1}|^{2}-|z_{2}|^{2}=-\alpha,\quad|z_{1}|^{2}-|z_{3}|^{2}=0,\\ &\mathop{\rm Im}(z_{1}z_{2}z_{3})=0,\quad\mathop{\rm Re}(z_{1}z_{2}z_{3})\geqslant 0\bigr\},\\ L_{2,\alpha}^{-}=\bigl\{(z_{1},z_{2},z_{3})\in\mathbin{\mathbb{C}}^{3}:\,&|z_{1}|^{2}-|z_{2}|^{2}=-\alpha,\quad|z_{1}|^{2}-|z_{3}|^{2}=0,\\ &\mathop{\rm Im}(z_{1}z_{2}z_{3})=0,\quad\mathop{\rm Re}(z_{1}z_{2}z_{3})\leqslant 0\bigr\},\end{split} (18)
L3,α+={(z1,z2,z3)∈ℂ3:|z1|2−|z2|2=0,|z1|2−|z3|2=−α,Im(z1z2z3)=0,Re(z1z2z3)⩾0},L3,α−={(z1,z2,z3)∈ℂ3:|z1|2−|z2|2=0,|z1|2−|z3|2=−α,Im(z1z2z3)=0,Re(z1z2z3)⩽0},\displaystyle\begin{split}L_{3,\alpha}^{+}=\bigl\{(z_{1},z_{2},z_{3})\in\mathbin{\mathbb{C}}^{3}:\,&|z_{1}|^{2}-|z_{2}|^{2}=0,\quad|z_{1}|^{2}-|z_{3}|^{2}=-\alpha,\\ &\mathop{\rm Im}(z_{1}z_{2}z_{3})=0,\quad\mathop{\rm Re}(z_{1}z_{2}z_{3})\geqslant 0\bigr\},\\ L_{3,\alpha}^{-}=\bigl\{(z_{1},z_{2},z_{3})\in\mathbin{\mathbb{C}}^{3}:\,&|z_{1}|^{2}-|z_{2}|^{2}=0,\quad|z_{1}|^{2}-|z_{3}|^{2}=-\alpha,\\ &\mathop{\rm Im}(z_{1}z_{2}z_{3})=0,\quad\mathop{\rm Re}(z_{1}z_{2}z_{3})\leqslant 0\bigr\},\end{split} (19)

then L2,α±L_{2,\alpha}^{\pm} and L3,α±L_{3,\alpha}^{\pm} are all nonsingular SL 3-folds diffeomorphic to 𝒮1×ℂ{\mathcal{S}}^{1}\times\mathbin{\mathbb{C}}, with L−α,0,0=L2,α+∪L2,α−L_{-\alpha,0,0}=L_{2,\alpha}^{+}\cup L_{2,\alpha}^{-} and L0,−α,0=L3,α+∪L3,α−L_{0,-\alpha,0}=L_{3,\alpha}^{+}\cup L_{3,\alpha}^{-}.

It is not difficult to show that Lj,α+L_{j,\alpha}^{+} is asymptotic to the T2T^{2}-cone L0+L_{0}^{+} at infinity for j=1,2,3j=1,2,3. Thus the Lj,α+L_{j,\alpha}^{+} for j=1,2,3j=1,2,3 are three different families of asymptotically conical SL 3-folds asymptotic to the same singular cone L0+L_{0}^{+}. We may interpret them as three different ways to ‘resolve’ the same SL 3-fold singularity L0+L_{0}^{+}. This point of view was taken in [10, §3–§5]. Similarly, Lj,α−L_{j,\alpha}^{-} is asymptotic to L0−L_{0}^{-} at infinity for j=1,2,3j=1,2,3.

For α>0\alpha>0, define a holomorphic disc D1,αD_{1,\alpha} in ℂ3\mathbin{\mathbb{C}}^{3} by

D1,α={(z1,0,0):z1∈ℂ,|z1|2⩽α}.D_{1,\alpha}=\bigl\{(z_{1},0,0):z_{1}\in\mathbin{\mathbb{C}},\quad|z_{1}|^{2}\leqslant\alpha\bigr\}. (20)

Then ∂D1,α\partial D_{1,\alpha} is the intersection of L1,α+L_{1,\alpha}^{+} and L1,α−L_{1,\alpha}^{-}. Therefore D1,αD_{1,\alpha} is a holomorphic disc with boundary in both of the nonsingular SL 3-folds L1,α±L_{1,\alpha}^{\pm}. In the same way, there are holomorphic discs D2,αD_{2,\alpha} and D3,αD_{3,\alpha} with boundaries in L2,α±L_{2,\alpha}^{\pm} and L3,α±L_{3,\alpha}^{\pm}. This will be significant later, when we discuss holomorphic discs in Calabi–Yau 3-folds with boundary in special Lagrangian 3-folds.

[03L6]

5 Two piecewise smooth SL fibrations of ℂ3\mathbin{\mathbb{C}}^{3}

We shall now define two piecewise smooth special Lagrangian fibrations f:ℂ3→ℝ3f:\mathbin{\mathbb{C}}^{3}\rightarrow\mathbin{\mathbb{R}}^{3} with singular fibres of codimension one in ℝ3\mathbin{\mathbb{R}}^{3}. These will be our local models for the most generic kind of singularity in special Lagrangian fibrations of generic Calabi–Yau 3-folds. We begin by defining a family of SL 3-folds Na,cN_{a,c} in ℂ3\mathbin{\mathbb{C}}^{3} depending on a∈ℝa\in\mathbin{\mathbb{R}} and c∈ℂc\in\mathbin{\mathbb{C}}.

[03L7]

Definition 5.1 Let a∈ℝa\in\mathbin{\mathbb{R}} and c∈ℂc\in\mathbin{\mathbb{C}}. Define a special Lagrangian 3-fold Na,cN_{a,c} in ℂ3\mathbin{\mathbb{C}}^{3} as follows:

  • (i)

    When a=0a=0, define

    N0,c={(z1,z2,z3)∈ℂ3:|z1|2=|z2|2=|z3−c|2,Im(z1z2(z3−c))=0,Re(z1z2(z3−c))⩾0}.\begin{split}N_{0,c}=\Bigl\{(z_{1}&,z_{2},z_{3})\in\mathbin{\mathbb{C}}^{3}:|z_{1}|^{2}=|z_{2}|^{2}=|z_{3}-c|^{2},\\ &\mathop{\rm Im}\bigl(z_{1}z_{2}(z_{3}-c)\bigr)=0,\quad\mathop{\rm Re}\bigl(z_{1}z_{2}(z_{3}-c)\bigr)\geqslant 0\Bigr\}.\end{split} (21)

    Then N0,cN_{0,c} is the translation of the special Lagrangian T2T^{2}-cone L0+L_{0}^{+} of (16) by the vector (0,0,c)(0,0,c). It has one singular point at (0,0,c)(0,0,c).

  • (ii)

    When a>0a>0, define

    Na,c={(z1,z2,z3)∈ℂ3:|z1|2−a=|z2|2=|z3−c|2,Im(z1z2(z3−c))=0,Re(z1z2(z3−c))⩾0}.\begin{split}N_{a,c}=\Bigl\{(z_{1}&,z_{2},z_{3})\in\mathbin{\mathbb{C}}^{3}:|z_{1}|^{2}-a=|z_{2}|^{2}=|z_{3}-c|^{2},\\ &\mathop{\rm Im}\bigl(z_{1}z_{2}(z_{3}-c)\bigr)=0,\quad\mathop{\rm Re}\bigl(z_{1}z_{2}(z_{3}-c)\bigr)\geqslant 0\Bigr\}.\end{split} (22)

    Then Na,cN_{a,c} is the translation of the nonsingular SL 3-fold L1,a+L_{1,a}^{+} of (17) by the vector (0,0,c)(0,0,c). It is diffeomorphic to 𝒮1×ℝ2{\mathcal{S}}^{1}\times\mathbin{\mathbb{R}}^{2}.

  • (iii)

    When a<0a<0, define

    Na,c={(z1,z2,z3)∈ℂ3:|z1|2=|z2|2+a=|z3−c|2,Im(z1z2(z3−c))=0,Re(z1z2(z3−c))⩾0}.\begin{split}N_{a,c}=\Bigl\{(z_{1}&,z_{2},z_{3})\in\mathbin{\mathbb{C}}^{3}:|z_{1}|^{2}=|z_{2}|^{2}+a=|z_{3}-c|^{2},\\ &\mathop{\rm Im}\bigl(z_{1}z_{2}(z_{3}-c)\bigr)=0,\quad\mathop{\rm Re}\bigl(z_{1}z_{2}(z_{3}-c)\bigr)\geqslant 0\Bigr\}.\end{split} (23)

    Then Na,cN_{a,c} is the translation of the nonsingular SL 3-fold L2,−a+L_{2,-a}^{+} of (18) by the vector (0,0,c)(0,0,c). It is diffeomorphic to 𝒮1×ℝ2{\mathcal{S}}^{1}\times\mathbin{\mathbb{R}}^{2}.

These 3-folds Na,cN_{a,c} are the fibres of a special Lagrangian fibration of ℂ3\mathbin{\mathbb{C}}^{3}.

[03L8]
Theorem 5.2

Define f:ℂ3→ℝ3f:\mathbin{\mathbb{C}}^{3}\rightarrow\mathbin{\mathbb{R}}^{3} by f⁡(z1,z2,z3)=(a,Rec,Imc)f(z_{1},z_{2},z_{3})=(a,\mathop{\rm Re}c,\mathop{\rm Im}c), where

a\displaystyle a =|z1|2−|z2|2\displaystyle=|z_{1}|^{2}-|z_{2}|^{2} (24)
andc\displaystyle\text{and}\quad c ={z3−z¯1​z¯2/|z1|,a=0 and z1,z2≠0,z3,a=z1=z2=0,z3−z¯1​z¯2/|z1|,a>0,z3−z¯1​z¯2/|z2|,a<0.\displaystyle=\begin{cases}z_{3}-\bar{z}_{1}\bar{z}_{2}/|z_{1}|,&\text{$a=0$ and\/ $z_{1},z_{2}\neq 0$,}\\ z_{3},&\text{$a=z_{1}=z_{2}=0$,}\\ z_{3}-\bar{z}_{1}\bar{z}_{2}/|z_{1}|,&\text{$a>0$,}\\ z_{3}-\bar{z}_{1}\bar{z}_{2}/|z_{2}|,&\text{$a<0$.}\end{cases} (25)

Then ff is continuous and piecewise smooth, and f−1​(a,Rec,Imc)=Na,cf^{-1}(a,\mathop{\rm Re}c,\mathop{\rm Im}c)=N_{a,c}, where Na,cN_{a,c} is given in Definition 5. Hence, ff is a piecewise smooth special Lagrangian fibration of ℂ3\mathbin{\mathbb{C}}^{3}.

[03L9]

Proof. Clearly ff is well-defined and piecewise smooth. It is also not difficult to show from (24) and (25) that ff is continuous. Observe from Definition 5 that if (z1,z2,z3)∈Na,c(z_{1},z_{2},z_{3})\in N_{a,c} then a=|z1|2−|z2|2a=|z_{1}|^{2}-|z_{2}|^{2} and

z1​z2​(z3−c)={|z1|​|z2|2,a⩾0,|z1|2​|z2|,a<0.z_{1}z_{2}(z_{3}-c)=\begin{cases}|z_{1}||z_{2}|^{2},&a\geqslant 0,\\ |z_{1}|^{2}|z_{2}|,&a<0.\end{cases}

Thus, if z1​z2≠0z_{1}z_{2}\neq 0 dividing by z1​z2z_{1}z_{2} and rearranging yields

c={z3−|z1|​|z2|2/(z1​z2),a⩾0,z3−|z1|2​|z2|/(z1​z2),a<0.c=\begin{cases}z_{3}-|z_{1}||z_{2}|^{2}/(z_{1}z_{2}),&a\geqslant 0,\\ z_{3}-|z_{1}|^{2}|z_{2}|/(z_{1}z_{2}),&a<0.\end{cases}

Using the equations |z1|2=z1​z¯1|z_{1}|^{2}=z_{1}\bar{z}_{1} and |z2|2=z2​z¯2|z_{2}|^{2}=z_{2}\bar{z}_{2} to rewrite these expressions gives the first case of (25), the third case when z2≠0z_{2}\neq 0, and the fourth case when z1≠0z_{1}\neq 0. If z1​z2=0z_{1}z_{2}=0 on the other hand, in each of parts (i)–(iii) of Definition 5 we have |z3−c|2=0|z_{3}-c|^{2}=0, so c=z3c=z_{3}, giving the second case of (25), the third case when z2=0z_{2}=0, and the fourth case when z1=0z_{1}=0.

So, if (z1,z2,z3)∈Na,c(z_{1},z_{2},z_{3})\in N_{a,c} then we can recover aa and cc from (z1,z2,z3)(z_{1},z_{2},z_{3}) as in the theorem. Conversely, for any (z1,z2,z3)(z_{1},z_{2},z_{3}) in ℂ3\mathbin{\mathbb{C}}^{3}, defining a,ca,c by (24)–(25) and reversing the proof above, we find that (z1,z2,z3)∈Na,c(z_{1},z_{2},z_{3})\in N_{a,c}. Hence f−1​(a,Rec,Imc)=Na,cf^{-1}(a,\mathop{\rm Re}c,\mathop{\rm Im}c)=N_{a,c}, and ff is a special Lagrangian fibration of ℂ3\mathbin{\mathbb{C}}^{3}. □\square

The singular fibres of the fibration are N0,cN_{0,c} for c∈ℂc\in\mathbin{\mathbb{C}}, which is singular only at (0,0,c)(0,0,c). Thus the set of singular points of singular fibres of the fibration is {(0,0,c):c∈ℂ}\bigl\{(0,0,c):c\in\mathbin{\mathbb{C}}\bigr\}. Note that this is the same as in Corollary 4.2, and is a complex curve in ℂ3\mathbin{\mathbb{C}}^{3}.

However, ff is not smooth on the whole real hypersurface |z1|=|z2||z_{1}|=|z_{2}|, which includes the set of singular points but many other points as well. Thus ff fails to be smooth not only at singular points of singular fibres, but also at nonsingular points of singular fibres. We should understand the non-smoothness of ff as being related not to a singularity at the point in question, but to a change in the global topology of the whole fibre.

Let us consider the symmetries of the fibration. The fibres Na,cN_{a,c} were defined as translations by (0,0,c)(0,0,c) of the SL 3-folds L0+L_{0}^{+}, L1,a+L_{1,a}^{+} and L2,−a+L_{2,-a}^{+} defined in §4, and we know that these have symmetry group U(1)2\mathbin{\rm U}(1)^{2} in SU(3)\mathop{\rm SU}(3). However, because this U(1)2\mathbin{\rm U}(1)^{2}-action doesn’t commute with the (0,0,c)(0,0,c) translations, the subgroup of SU(3)⋉ℂ3\mathop{\rm SU}(3)\ltimes\mathbin{\mathbb{C}}^{3} preserving every fibre is smaller: it is U(1)\mathbin{\rm U}(1), acting by

ei​θ:(z1,z2,z3)⟼(ei​θ​z1,e−i​θ​z2,z3).{\rm e}^{i\theta}:(z_{1},z_{2},z_{3})\longmapsto({\rm e}^{i\theta}z_{1},{\rm e}^{-i\theta}z_{2},z_{3}). (26)

Note that the moment map of this action is |z1|2−|z2|2|z_{1}|^{2}-|z_{2}|^{2}, which is aa in (24). This is as one would expect, because Lagrangian submanifolds must lie in level sets of the moment maps of their symmetry groups by [11, Prop. 4.2].

The subgroup of SU(3)⋉ℂ3\mathop{\rm SU}(3)\ltimes\mathbin{\mathbb{C}}^{3} preserving the fibration, but acting nontrivially on the set of fibres, is rather larger. It is generated by U(1)2\mathbin{\rm U}(1)^{2} acting on ℂ3\mathbin{\mathbb{C}}^{3} as in (13)–(14), and the translations (z1,z2,z3)↦(z1,z2,z3+c)(z_{1},z_{2},z_{3})\mapsto(z_{1},z_{2},z_{3}+c) for c∈ℂc\in\mathbin{\mathbb{C}}. The involution (z1,z2,z3)↦(z2,z1,z3)(z_{1},z_{2},z_{3})\mapsto(z_{2},z_{1},z_{3}) also preserves the fibration and takes (a,Rec,Imc)↦(−a,Rec,Imc)(a,\mathop{\rm Re}c,\mathop{\rm Im}c)\mapsto(-a,\mathop{\rm Re}c,\mathop{\rm Im}c), but it does not lie in SU(3)⋉ℂ3\mathop{\rm SU}(3)\ltimes\mathbin{\mathbb{C}}^{3} as it changes the sign of Ω\Omega.

Now we defined the fibration ff and fibres Na,cN_{a,c} above using the SL 3-folds L0+L_{0}^{+}, L1,a+L_{1,a}^{+} and L2,−a+L_{2,-a}^{+} of equations (21)–(23). The choice of ++ rather than −- was arbitrary, and we could equally well have used L0−L_{0}^{-}, L1,a−L_{1,a}^{-} and L2,−a−L_{2,-a}^{-} instead. When we do, we get the following analogues of Definition 5 and Theorem 5.2.

[03LA]

Definition 5.3 Let a∈ℝa\in\mathbin{\mathbb{R}} and c∈ℂc\in\mathbin{\mathbb{C}}. Define a special Lagrangian 3-fold Na,c′N^{\prime}_{a,c} in ℂ3\mathbin{\mathbb{C}}^{3} as in equations (21)–(23), but in each case replace the inequality Re(z1​z2​(z3−c))⩾0\mathop{\rm Re}\bigl(z_{1}z_{2}(z_{3}-c)\bigr)\geqslant 0 by Re(z1​z2​(z3−c))⩽0\mathop{\rm Re}\bigl(z_{1}z_{2}(z_{3}-c)\bigr)\leqslant 0. Then

  • (i)

    N0,c′N^{\prime}_{0,c} is the translation of the special Lagrangian T2T^{2}-cone L0−L_{0}^{-} of (16) by (0,0,c)(0,0,c), and has one singular point at (0,0,c)(0,0,c).

  • (ii)

    For a>0a>0, Na,c′N^{\prime}_{a,c} is the translation of the nonsingular SL 3-fold L1,a−L_{1,a}^{-} of (17) by (0,0,c)(0,0,c), and is diffeomorphic to 𝒮1×ℝ2{\mathcal{S}}^{1}\times\mathbin{\mathbb{R}}^{2}.

  • (iii)

    For a<0a<0, Na,c′N^{\prime}_{a,c} is the translation of the nonsingular SL 3-fold L2,−a−L_{2,-a}^{-} of (18) by (0,0,c)(0,0,c), and is diffeomorphic to 𝒮1×ℝ2{\mathcal{S}}^{1}\times\mathbin{\mathbb{R}}^{2}.

[03LB]
Theorem 5.4

Define f′:ℂ3→ℝ3f^{\prime}:\mathbin{\mathbb{C}}^{3}\rightarrow\mathbin{\mathbb{R}}^{3} by f′​(z1,z2,z3)=(a,Rec,Imc)f^{\prime}(z_{1},z_{2},z_{3})=(a,\mathop{\rm Re}c,\mathop{\rm Im}c), where

a\displaystyle a =|z1|2−|z2|2\displaystyle=|z_{1}|^{2}-|z_{2}|^{2} (27)
andc\displaystyle\text{and}\quad c ={z3+z¯1​z¯2/|z1|,a=0 and z1,z2≠0,z3,a=z1=z2=0,z3+z¯1​z¯2/|z1|,a>0,z3+z¯1​z¯2/|z2|,a<0.\displaystyle=\begin{cases}z_{3}+\bar{z}_{1}\bar{z}_{2}/|z_{1}|,&\text{$a=0$ and\/ $z_{1},z_{2}\neq 0$,}\\ z_{3},&\text{$a=z_{1}=z_{2}=0$,}\\ z_{3}+\bar{z}_{1}\bar{z}_{2}/|z_{1}|,&\text{$a>0$,}\\ z_{3}+\bar{z}_{1}\bar{z}_{2}/|z_{2}|,&\text{$a<0$.}\end{cases} (28)

Then f′f^{\prime} is continuous and piecewise smooth, and (f′)−1​(a,Rec,Imc)=Na,c′(f^{\prime})^{-1}(a,\mathop{\rm Re}c,\mathop{\rm Im}c)=N^{\prime}_{a,c}, where Na,c′N^{\prime}_{a,c} is given in Definition 5. Hence, f′f^{\prime} is a piecewise smooth special Lagrangian fibration of ℂ3\mathbin{\mathbb{C}}^{3}.

The fibres of the fibrations of Theorems 5.2 and 5.4 are singular if and only if a=0a=0, that is, on a hyperplane of real codimension one in the base ℝ3\mathbin{\mathbb{R}}^{3} of the fibrations. But by Proposition 3.2 (which also applies in the noncompact case), if ff were a smooth fibration then the set of singular fibres would have Hausdorff codimension at least two. Therefore the piecewise-smoothness of ff is essential, not merely cosmetic.

To see what we might mean by a special Lagrangian fibration whose non-smoothness is merely cosmetic, consider the following fairly trivial example.

[03LC]

Example 5.5 Define SS to be the set of linear special Lagrangian 3-planes ℝ3\mathbin{\mathbb{R}}^{3} in ℂ3\mathbin{\mathbb{C}}^{3} containing the real line {(0,0,t):t∈ℝ}\bigl\{(0,0,t):t\in\mathbin{\mathbb{R}}\bigr\}. Then S≅𝒮2S\cong{\mathcal{S}}^{2}. Let L={(x1,x2,x3)∈ℂ3:xj∈ℝ}L=\bigl\{(x_{1},x_{2},x_{3})\in\mathbin{\mathbb{C}}^{3}:x_{j}\in\mathbin{\mathbb{R}}\bigr\}. Then L∈SL\in S. Let γ:ℝ→S∖{L}\gamma:\mathbin{\mathbb{R}}\rightarrow S\setminus\{L\} be a function which is continuous, but not smooth.

For each (a,b,c)∈ℝ3(a,b,c)\in\mathbin{\mathbb{R}}^{3}, define Πa,b,c\Pi_{a,b,c} to be the affine special Lagrangian 3-plane γ⁡(c)+(a,b,i​c)\gamma(c)+(a,b,ic). It is not difficult to show that there is a unique, continuous special Lagrangian fibration f:ℂ3→ℝ3f:\mathbin{\mathbb{C}}^{3}\rightarrow\mathbin{\mathbb{R}}^{3} with f−1​(a,b,c)=Πa,b,cf^{-1}(a,b,c)=\Pi_{a,b,c}. However, because γ\gamma is not smooth, ff is not smooth.

What is going on here is that we divide ℂ3\mathbin{\mathbb{C}}^{3} into the family of parallel real hyperplanes Im(z3)=c\mathop{\rm Im}(z_{3})=c, and fibre each such hyperplane by a 2-dimensional family of parallel special Lagrangian 3-planes. There is an 𝒮2{\mathcal{S}}^{2} family SS of different ways of fibring Im(z3)=c\mathop{\rm Im}(z_{3})=c by such parallel 3-planes. We exclude LL because then any L′∈S∖{L}L^{\prime}\in S\setminus\{L\} is transverse to ℝ2={(a,b,0):a,b∈ℝ}\mathbin{\mathbb{R}}^{2}=\bigl\{(a,b,0):a,b\in\mathbin{\mathbb{R}}\bigr\}, so we can use a,ba,b to parametrize the family of parallel 3-planes in Im(z3)=c\mathop{\rm Im}(z_{3})=c.

The key idea is that we can treat different hyperplanes Im(z3)=c\mathop{\rm Im}(z_{3})=c essentially independently. The map γ\gamma is arbitrary; we could choose it to be smooth, or piecewise smooth, or merely continuous, and we then get a fibration f:ℂ3→ℝ3f:\mathbin{\mathbb{C}}^{3}\rightarrow\mathbin{\mathbb{R}}^{3} with the same property. So this example generates many examples of piecewise smooth SL fibrations of ℂ3\mathbin{\mathbb{C}}^{3}. However, though Example 5 does show that non-smooth SL fibrations are possible locally, it tells us almost nothing about the smoothness of fibrations of Calabi–Yau 3-folds XX by compact special Lagrangian 3-folds NN, in particular tori.

This is because we know from Theorem 2.9 that if NN is a nonsingular SL T3T^{3} in XX, then the family of deformations of NN is locally smooth and 3-dimensional. Hence, if these deformations are locally transverse to NN, then near NN they do form a smooth SL fibration. Where this argument breaks down is when the fibres of the fibration develop singularities. Thus, any argument as to whether SL fibrations are smooth must focus on the behaviour of the fibrations near their singularities.

As Example 5 involves no singular fibres, it is irrelevant to the discussion. However, Theorems 5.2 and 5.4 are relevant as they model fibrations with many singular fibres, whose singularities are of a kind that cannot appear in smooth fibrations. They are evidence in favour of our contention that special Lagrangian fibrations of Calabi–Yau 3-folds will not in general be smooth.

[03LD]

6 A class of U(1)\mathbin{\rm U}(1)-invariant SL 3-folds in ℂ3\mathbin{\mathbb{C}}^{3}

As a preparation for §7, in which we will describe a conjectural local model for a certain kind of singularity of special Lagrangian fibrations of Calabi–Yau 3-folds, we will now study singular special Lagrangian 3-folds NN in ℂ3\mathbin{\mathbb{C}}^{3} invariant under the U(1)\mathbin{\rm U}(1)-action

ei​θ:(z1,z2,z3)↦(ei​θ​z1,e−i​θ​z2,z3)for ei​θ∈U(1).{\rm e}^{i\theta}:(z_{1},z_{2},z_{3})\mapsto({\rm e}^{i\theta}z_{1},{\rm e}^{-i\theta}z_{2},z_{3})\quad\text{for ${\rm e}^{i\theta}\in\mathbin{\rm U}(1)$.} (29)

We shall assume that NN may be written

N={(z1,z2,z3)∈ℂ3:Re(z1z2)=u(Re(z3),Im(z1z2)),Im(z3)=v(Re(z3),Im(z1z2)),|z1|2−|z2|2=a},\begin{split}N=\Bigl\{(z_{1}&,z_{2},z_{3})\in\mathbin{\mathbb{C}}^{3}:\mathop{\rm Re}(z_{1}z_{2})=u\bigl(\mathop{\rm Re}(z_{3}),\mathop{\rm Im}(z_{1}z_{2})\bigr),\\ &\mathop{\rm Im}(z_{3})=v\bigl(\mathop{\rm Re}(z_{3}),\mathop{\rm Im}(z_{1}z_{2})\bigr),\quad|z_{1}|^{2}-|z_{2}|^{2}=a\Bigr\},\end{split} (30)

where a∈ℝa\in\mathbin{\mathbb{R}} and u,v:ℝ2→ℝu,v:\mathbin{\mathbb{R}}^{2}\rightarrow\mathbin{\mathbb{R}} are continuous functions, which are smooth except at certain singular points. Here is why we choose to write NN in this form. As the functions Re(z1​z2),Im(z1​z2),|z1|2−|z2|2,Re(z3)\mathop{\rm Re}(z_{1}z_{2}),\mathop{\rm Im}(z_{1}z_{2}),|z_{1}|^{2}-|z_{2}|^{2},\mathop{\rm Re}(z_{3}) and Im(z3)\mathop{\rm Im}(z_{3}) involved in (30) are U(1)\mathbin{\rm U}(1)-invariant, NN is automatically U(1)\mathbin{\rm U}(1)-invariant.

Also, as in [11, Prop. 4.2], if NN is a connected Lagrangian submanifold of ℂm\mathbin{\mathbb{C}}^{m} invariant under a Lie subgroup GG of the automorphism group U(m)⋉ℂm\mathbin{\rm U}(m)\ltimes\mathbin{\mathbb{C}}^{m} of ℂm\mathbin{\mathbb{C}}^{m}, then the moment map μ\mu of GG is constant on NN. Now the moment map of the U(1)\mathbin{\rm U}(1)-action (29) is |z1|2−|z2|2|z_{1}|^{2}-|z_{2}|^{2}. Thus |z1|2−|z2|2=a|z_{1}|^{2}-|z_{2}|^{2}=a for some a∈ℝa\in\mathbin{\mathbb{R}} on any U(1)\mathbin{\rm U}(1)-invariant SL mm-fold NN in ℂm\mathbin{\mathbb{C}}^{m}, which is why we have taken |z1|2−|z2|2=a|z_{1}|^{2}-|z_{2}|^{2}=a to be one of the equations defining NN.

In the other two equations Re(z1​z2)=u⁡(Re(z3),Im(z1​z2))\mathop{\rm Re}(z_{1}z_{2})=u\bigl(\mathop{\rm Re}(z_{3}),\mathop{\rm Im}(z_{1}z_{2})\bigr) and Im(z3)=v⁡(Re(z3),Im(z1​z2))\mathop{\rm Im}(z_{3})=v\bigl(\mathop{\rm Re}(z_{3}),\mathop{\rm Im}(z_{1}z_{2})\bigr), what we are doing is regarding the functions x=Re(z3)x=\mathop{\rm Re}(z_{3}) and y=Im(z1​z2)y=\mathop{\rm Im}(z_{1}z_{2}) as coordinates on N/U(1)N/\mathbin{\rm U}(1), and expressing the other two degrees of freedom Re(z1​z2)\mathop{\rm Re}(z_{1}z_{2}) and Im(z3)\mathop{\rm Im}(z_{3}) as functions of xx and yy. Thus we define NN as a kind of graph of the pair of functions (u,v)(u,v).

Note that not every U(1)\mathbin{\rm U}(1)-invariant SL 3-fold NN in ℂ3\mathbin{\mathbb{C}}^{3} may be written in the form (30). Locally this is generally possible, but globally the functions uu and vv would have to be multi-valued, branched covers of ℝ2\mathbin{\mathbb{R}}^{2} for instance. However, we will see that the class of SL 3-folds of this form do have many nice properties, and are interesting both in themselves and for our later applications. So equation (30) should be regarded as more than just an arbitrary choice of coordinate system.

[03LE]

6.1 Finding the equations on uu and vv

We now calculate the conditions on the functions u(x,y),v(x,y):ℝ2→ℝu(x,y),v(x,y):\mathbin{\mathbb{R}}^{2}\rightarrow\mathbin{\mathbb{R}} for the 3-fold NN of (30) to be special Lagrangian.

[03LF]
Proposition 6.1

Let u,v:ℝ2→ℝu,v:\mathbin{\mathbb{R}}^{2}\rightarrow\mathbin{\mathbb{R}} be continuous, and let a∈ℝa\in\mathbin{\mathbb{R}}. Define

N={(z1,z2,z3)∈ℂ3:Re(z1z2)=u(Re(z3),Im(z1z2)),Im(z3)=v(Re(z3),Im(z1z2)),|z1|2−|z2|2=a}.\begin{split}N=\Bigl\{(z_{1}&,z_{2},z_{3})\in\mathbin{\mathbb{C}}^{3}:\mathop{\rm Re}(z_{1}z_{2})=u\bigl(\mathop{\rm Re}(z_{3}),\mathop{\rm Im}(z_{1}z_{2})\bigr),\\ &\mathop{\rm Im}(z_{3})=v\bigl(\mathop{\rm Re}(z_{3}),\mathop{\rm Im}(z_{1}z_{2})\bigr),\quad|z_{1}|^{2}-|z_{2}|^{2}=a\Bigr\}.\end{split} (31)

Then

  • (a)

    If a=0a=0, then NN is a singular special Lagrangian 33-fold in ℂ3\mathbin{\mathbb{C}}^{3} if u,vu,v are differentiable and satisfy

    ∂u∂x=−2​(u2+y2)1/2​∂v∂yand∂u∂y=∂v∂x,\frac{\partial u}{\partial x}=-2\bigl(u^{2}+y^{2}\bigr)^{1/2}\frac{\partial v}{\partial y}\quad\text{and}\quad\frac{\partial u}{\partial y}=\frac{\partial v}{\partial x}, (32)

    except at points (x,0)(x,0) in ℝ2\mathbin{\mathbb{R}}^{2} with u⁡(x,0)=0u(x,0)=0, where u,vu,v need not be differentiable. The singular points of NN are those of the form (0,0,z3)(0,0,z_{3}), where z3=x+i​v​(x,0)z_{3}=x+iv(x,0) for x∈ℝx\in\mathbin{\mathbb{R}} with u⁡(x,0)=0u(x,0)=0.

  • (b)

    If a≠0a\neq 0, then NN is a nonsingular special Lagrangian 33-fold in ℂ3\mathbin{\mathbb{C}}^{3} if and only if u,vu,v are differentiable on all of ℝ2\mathbin{\mathbb{R}}^{2} and satisfy

    ∂u∂x=−(4​u2+4​y2+a2)1/2​∂v∂yand∂u∂y=∂v∂x.\frac{\partial u}{\partial x}=-\bigl(4u^{2}+4y^{2}+a^{2}\bigr)^{1/2}\frac{\partial v}{\partial y}\quad\text{and}\quad\frac{\partial u}{\partial y}=\frac{\partial v}{\partial x}. (33)
[03LG]

Proof. We shall give the proof for part (a). Part (b) is similar but more complicated, and will be left to the reader. Let a=0a=0, let NN be defined by (31), and let 𝐳=(z1,z2,z3)∈N{\bf z}=(z_{1},z_{2},z_{3})\in N. For 𝐳\bf z to be a nonsingular point of NN, we need uu and vv to be differentiable at (x,y)=(Re(z3),Im(z1​z2))(x,y)=\bigl(\mathop{\rm Re}(z_{3}),\mathop{\rm Im}(z_{1}z_{2})\bigr) in ℝ2\mathbin{\mathbb{R}}^{2}, and for the derivatives of the three functions

Re(z1​z2)−u⁡(Re(z3),Im(z1​z2)),Im(z3)−v⁡(Re(z3),Im(z1​z2)),|z1|2−|z2|2\mathop{\rm Re}(z_{1}z_{2})-u\bigl(\mathop{\rm Re}(z_{3}),\mathop{\rm Im}(z_{1}z_{2})\bigr),\quad\mathop{\rm Im}(z_{3})-v\bigl(\mathop{\rm Re}(z_{3}),\mathop{\rm Im}(z_{1}z_{2})\bigr),\quad|z_{1}|^{2}-|z_{2}|^{2}

on ℂ3\mathbin{\mathbb{C}}^{3} to be linearly independent at 𝐳\bf z.

Now if z1=z2=0z_{1}=z_{2}=0 then |z1|2−|z2|2|z_{1}|^{2}-|z_{2}|^{2} has zero derivative at 𝐳\bf z. Thus points of the form (0,0,z3)(0,0,z_{3}) in NN will be singular. Clearly, these occur exactly when z3=x+i​v​(x,0)z_{3}=x+iv(x,0) for x∈ℝx\in\mathbin{\mathbb{R}} with u⁡(x,0)=0u(x,0)=0. Also, as |z1|2−|z2|2=0|z_{1}|^{2}-|z_{2}|^{2}=0, such points occur in NN only when a=0a=0. We shall see that these are the only singular points in NN, provided uu and vv are differentiable.

To prove part (a) we need to show that each 𝐳∈N{\bf z}\in N not of the form (0,0,z3)(0,0,z_{3}) is a nonsingular point of NN, and the tangent space T𝐳​NT_{\bf z}N is a special Lagrangian 3-plane ℝ3\mathbin{\mathbb{R}}^{3} in ℂ3\mathbin{\mathbb{C}}^{3}. As NN is U(1)\mathbin{\rm U}(1)-invariant, it is enough to prove this for one point in each orbit of the U(1)\mathbin{\rm U}(1)-action (29). Since |z1|=|z2||z_{1}|=|z_{2}| on NN, each U(1)\mathbin{\rm U}(1)-orbit in NN contains one or two points (z1,z2,z3)(z_{1},z_{2},z_{3}) with z1=z2z_{1}=z_{2}.

Thus it is enough to show that T𝐳​NT_{\bf z}N exists and is special Lagrangian for points 𝐳=(z1,z1,z3){\bf z}=(z_{1},z_{1},z_{3}) in NN with z1≠0z_{1}\neq 0. In our next lemma we identify T𝐳​NT_{\bf z}N at such a point. The proof is elementary, and is left as an exercise.

[03LH]
Lemma 6.2

Let 𝐳=(z1,z1,z3)∈N{\bf z}=(z_{1},z_{1},z_{3})\in N, with z1≠0z_{1}\neq 0. Set x=Re(z3)x=\mathop{\rm Re}(z_{3}) and y=Im(z12)y=\mathop{\rm Im}(z_{1}^{2}). Then NN is nonsingular at 𝐳\bf z, and T𝐳​N=⟨𝐩1,𝐩2,𝐩3⟩ℝ,T_{\bf z}N=\langle{\bf p}_{1},{\bf p}_{2},{\bf p}_{3}\rangle_{\scriptscriptstyle\mathbb{R}}, where

𝐩1\displaystyle{\bf p}_{1} =(i​z1,−i​z1,0),\displaystyle=(iz_{1},-iz_{1},0), (34)
𝐩2\displaystyle{\bf p}_{2} =((2z1)−1∂u∂x(x,y),(2z1)−1∂u∂x(x,y),1+i∂v∂x(x,y))and\displaystyle=\bigl((2z_{1})^{-1}{\textstyle\frac{\partial u}{\partial x}}(x,y),(2z_{1})^{-1}{\textstyle\frac{\partial u}{\partial x}}(x,y),1+i{\textstyle\frac{\partial v}{\partial x}}(x,y)\bigr)\quad\text{and} (35)
𝐩3\displaystyle{\bf p}_{3} =((2​z1)−1​(∂u∂y​(x,y)+i),(2​z1)−1​(∂u∂y​(x,y)+i),i​∂v∂y​(x,y)).\displaystyle=\bigl((2z_{1})^{-1}({\textstyle\frac{\partial u}{\partial y}}(x,y)+i),(2z_{1})^{-1}({\textstyle\frac{\partial u}{\partial y}}(x,y)+i),i{\textstyle\frac{\partial v}{\partial y}}(x,y)\bigr). (36)

Now define ×:ℂ3×ℂ3→ℂ3\times:\mathbin{\mathbb{C}}^{3}\times\mathbin{\mathbb{C}}^{3}\rightarrow\mathbin{\mathbb{C}}^{3} as in (2), and apply Proposition 2.4 with 𝐫=𝐩1{\bf r}={\bf p}_{1} and 𝐬=𝐩2{\bf s}={\bf p}_{2}. Clearly 𝐩1{\bf p}_{1} and 𝐩2{\bf p}_{2} are linearly independent, and ω⁡(𝐩1,𝐩2)=0\omega({\bf p}_{1},{\bf p}_{2})=0. So Proposition 2.4 shows that ⟨𝐩1,𝐩2,𝐩1×𝐩2⟩ℝ\langle{\bf p}_{1},{\bf p}_{2},{\bf p}_{1}\times{\bf p}_{2}\rangle_{\scriptscriptstyle\mathbb{R}} is the unique SL 3-plane in ℂ3\mathbin{\mathbb{C}}^{3} containing ⟨𝐩1,𝐩2⟩ℝ\langle{\bf p}_{1},{\bf p}_{2}\rangle_{\scriptscriptstyle\mathbb{R}}.

Therefore ⟨𝐩1,𝐩2,𝐩3⟩ℝ\langle{\bf p}_{1},{\bf p}_{2},{\bf p}_{3}\rangle_{\scriptscriptstyle\mathbb{R}} is an SL 3-plane if and only if 𝐩3∈⟨𝐩1,𝐩2,𝐩1×𝐩2⟩ℝ{\bf p}_{3}\in\langle{\bf p}_{1},{\bf p}_{2},{\bf p}_{1}\times{\bf p}_{2}\rangle_{\scriptscriptstyle\mathbb{R}}. Combining equations (2), (34) and (35) gives

𝐩1×𝐩2=(z¯1​(∂v∂x+i),z¯1​(∂v∂x+i),−i​∂u∂x).{\bf p}_{1}\times{\bf p}_{2}=\bigl(\bar{z}_{1}({\textstyle\frac{\partial v}{\partial x}}+i),\bar{z}_{1}({\textstyle\frac{\partial v}{\partial x}}+i),-i{\textstyle\frac{\partial u}{\partial x}}\bigr). (37)

So suppose 𝐩3=α​𝐩1+β​𝐩2+γ​𝐩1×𝐩2{\bf p}_{3}=\alpha{\bf p}_{1}+\beta{\bf p}_{2}+\gamma{\bf p}_{1}\times{\bf p}_{2}. As the first two coordinates are equal in 𝐩2,𝐩3{\bf p}_{2},{\bf p}_{3} and 𝐩1×𝐩2{\bf p}_{1}\times{\bf p}_{2} but not in 𝐩1{\bf p}_{1}, we see that α=0\alpha=0. Taking real parts in the third coordinate gives β=0\beta=0. And comparing real multiples of i​z¯1i\bar{z}_{1} in the first coordinate shows that γ=12​|z1|−2\gamma={\textstyle\frac{1}{2}}|z_{1}|^{-2}.

Thus T𝐳​NT_{\bf z}N is special Lagrangian if and only if 𝐩1×𝐩2=2​|z1|2​𝐩3{\bf p}_{1}\times{\bf p}_{2}=2|z_{1}|^{2}{\bf p}_{3}. By (36) and (37), this reduces to

∂u∂x=−2​|z1|2​∂v∂yand∂u∂y=∂v∂xat (x,y).\frac{\partial u}{\partial x}=-2|z_{1}|^{2}\frac{\partial v}{\partial y}\quad\text{and}\quad\frac{\partial u}{\partial y}=\frac{\partial v}{\partial x}\quad\text{at $(x,y)$.} (38)

But u=Re(z12)u=\mathop{\rm Re}(z_{1}^{2}) and y=Im(z12)y=\mathop{\rm Im}(z_{1}^{2}) by (31), so that |z1|4=u2+y2|z_{1}|^{4}=u^{2}+y^{2}, and |z1|2=(u2+y2)1/2|z_{1}|^{2}=(u^{2}+y^{2})^{1/2}. Substituting this into (38) gives equation (32), which proves part (a) of Proposition 6.1. Part (b) is left to the reader. □\square

Equations (32) and (33) are nonlinear versions of the Cauchy–Riemann equations. For if we replace the factors 2​(u2+y2)1/22(u^{2}+y^{2})^{1/2} and (4​u2+4​y2+a2)1/2(4u^{2}+4y^{2}+a^{2})^{1/2} in (32) and (33) by 1, the equations become

∂u∂x=−∂v∂yand∂u∂y=∂v∂x,\frac{\partial u}{\partial x}=-\,\frac{\partial v}{\partial y}\quad\text{and}\quad\frac{\partial u}{\partial y}=\frac{\partial v}{\partial x},

which are the conditions for u−i​vu-iv to be a holomorphic function of x+i​yx+iy. We may therefore expect the solutions of (32) and (33) to have qualitative features in common with solutions of the Cauchy–Riemann equations.

Note that (32) is the case a=0a=0 of equation (33), so we will often use (33) to refer to both, without assuming a≠0a\neq 0. Following Harvey and Lawson [9, Th. III.2.7], who use results of Morrey, we may prove:

[03LI]
Proposition 6.3

Any solutions u,vu,v of (33) are real analytic, except in the case a=0a=0 at points (x,0)(x,0) with u⁡(x,0)=0u(x,0)=0.

Now holomorphic functions on ℂ\mathbin{\mathbb{C}} are determined uniquely by their values on ℝ\mathbin{\mathbb{R}}. In the same way, solutions of (33) on ℝ2\mathbin{\mathbb{R}}^{2} are determined by their values on the xx-axis. We state this in the following proposition, which may be proved using the Cauchy–Kowalevksy Theorem [17, p. 234].

[03LJ]
Proposition 6.4

Let UU be an open neighbourhood of ww in ℝ\mathbin{\mathbb{R}} and u′,v′:U→ℝu^{\prime},v^{\prime}:U\rightarrow\mathbin{\mathbb{R}} be real analytic functions. If either a≠0a\neq 0, or a=0a=0 and u′​(w)≠0u^{\prime}(w)\neq 0, then in an open neighbourhood VV of (w,0)(w,0) in ℝ2\mathbin{\mathbb{R}}^{2} there exist unique real analytic solutions u,v:V→ℝu,v:V\rightarrow\mathbin{\mathbb{R}} of (33) such that u⁡(x,0)=u′​(x)u(x,0)=u^{\prime}(x) and v⁡(x,0)=v′​(x)v(x,0)=v^{\prime}(x) for all x∈Ux\in U with (x,0)∈V(x,0)\in V.

Next we show that solutions u,v:ℝ2→ℝu,v:\mathbin{\mathbb{R}}^{2}\rightarrow\mathbin{\mathbb{R}} of (33) may be written in terms of a single potential f:ℝ2→ℝf:\mathbin{\mathbb{R}}^{2}\rightarrow\mathbin{\mathbb{R}}.

[03LK]
Proposition 6.5

Let u,v:ℝ2→ℝu,v:\mathbin{\mathbb{R}}^{2}\rightarrow\mathbin{\mathbb{R}} be solutions of (33). Then there exists a unique function f:ℝ2→ℝf:\mathbin{\mathbb{R}}^{2}\rightarrow\mathbin{\mathbb{R}} with

∂f∂x=u,∂f∂y=vandf(0,0)=0,satisfying∂2f∂x2+(4​(∂f∂x)2+4​y2+a2)1/2​∂2f∂y2=0.\begin{gathered}\frac{\partial f}{\partial x}=u,\quad\frac{\partial f}{\partial y}=v\quad\text{and}\quad f(0,0)=0,\\ \text{satisfying}\quad\frac{\partial^{2}f}{\partial x^{2}}+\Bigl(4\Bigl(\frac{\partial f}{\partial x}\Bigr)^{2}+4y^{2}+a^{2}\Bigr)^{1/2}\frac{\partial^{2}f}{\partial y^{2}}=0.\end{gathered} (39)

Conversely, all solutions of (39) yield solutions of (33).

[03LL]

Proof. Let u,v:ℝ2→ℝu,v:\mathbin{\mathbb{R}}^{2}\rightarrow\mathbin{\mathbb{R}} be solutions of (33), and define ff by

f⁡(x,y)=∫0xu⁡(s,0)​𝑑s+∫0yv⁡(x,t)​𝑑t.f(x,y)=\int_{0}^{x}u(s,0){\rm d}s+\int_{0}^{y}v(x,t){\rm d}t.

Then ∂f∂y​(x,y)=v​(x,y)\frac{\partial f}{\partial y}(x,y)=v(x,y) and f⁡(0,0)=0f(0,0)=0 are immediate, and

∂f∂x​(x,y)\displaystyle\frac{\partial f}{\partial x}(x,y) =u⁡(x,0)+∫0y∂v∂x​(x,t)​𝑑t\displaystyle=u(x,0)+\int_{0}^{y}\frac{\partial v}{\partial x}(x,t){\rm d}t
=u⁡(x,0)+∫0y∂u∂y​(x,t)​𝑑t\displaystyle=u(x,0)+\int_{0}^{y}\frac{\partial u}{\partial y}(x,t){\rm d}t
=u⁡(x,0)+[u⁡(x,t)]0y=u⁡(x,y),\displaystyle=u(x,0)+\bigl[u(x,t)\bigr]^{y}_{0}=u(x,y),

as ∂u∂y=∂v∂x\frac{\partial u}{\partial y}=\frac{\partial v}{\partial x}. This proves the first line of (39), and the second follows by substituting ∂f∂x=u\frac{\partial f}{\partial x}=u and ∂f∂y=v\frac{\partial f}{\partial y}=v into the first equation of (33). The converse is easy. □\square

[03LM]

6.2 Writing the fibrations of §4 and §5 in this form

In Corollary 4.2 and Theorems 5.2 and 5.4 we defined examples of special Lagrangian fibrations f:ℂ3→ℝ3f:\mathbin{\mathbb{C}}^{3}\rightarrow\mathbin{\mathbb{R}}^{3}. We shall now show that each fibre f−1​(a,b,c)f^{-1}(a,b,c) of these fibrations may be written in the form (30). For Corollary 4.2 this is trivial:

[03LN]
Lemma 6.6

Let f:ℂ3→ℝ3f:\mathbin{\mathbb{C}}^{3}\rightarrow\mathbin{\mathbb{R}}^{3} be the special Lagrangian fibration of Corollary 4.2. Then each fibre f−1​(a,b,c)f^{-1}(a,b,c) may be written in the form (30), with u≡bu\equiv b and v≡cv\equiv c.

Next we show that the fibres f−1​(a,b,c)=Na,b+i​cf^{-1}(a,b,c)=N_{a,b+ic} of the fibration ff of Theorem 5.2 may be written in the form (30).

[03LP]
Proposition 6.7

Let a,b,c∈ℝa,b,c\in\mathbin{\mathbb{R}}. Then there exist unique functions u,v:ℝ2→ℝu,v:\mathbin{\mathbb{R}}^{2}\rightarrow\mathbin{\mathbb{R}} such that

N={(z1,z2,z3)∈ℂ3:Re(z1z2)=u(Re(z3),Im(z1z2)),Im(z3)=v(Re(z3),Im(z1z2)),|z1|2−|z2|2=a}\begin{split}N=\Bigl\{(z_{1}&,z_{2},z_{3})\in\mathbin{\mathbb{C}}^{3}:\mathop{\rm Re}(z_{1}z_{2})=u\bigl(\mathop{\rm Re}(z_{3}),\mathop{\rm Im}(z_{1}z_{2})\bigr),\\ &\mathop{\rm Im}(z_{3})=v\bigl(\mathop{\rm Re}(z_{3}),\mathop{\rm Im}(z_{1}z_{2})\bigr),\quad|z_{1}|^{2}-|z_{2}|^{2}=a\Bigr\}\end{split} (40)

is the special Lagrangian 33-fold Na,b+i​cN_{a,b+ic} of Definition 5. Furthermore:

  • (a)

    u,vu,v are smooth on ℝ2\mathbin{\mathbb{R}}^{2} and satisfy (33), except at (b,0)(b,0) when a=0a=0, where they are only continuous.

  • (b)

    u⁡(x,y)>0u(x,y)>0 when x>bx>b for all yy, and u⁡(b,y)=0u(b,y)=0 for all yy, and u⁡(x,y)<0u(x,y)<0 when x<bx<b for all yy.

  • (c)

    v⁡(x,y)<cv(x,y)<c when y>0y>0 for all xx, and v⁡(x,0)=cv(x,0)=c for all xx, and v⁡(x,y)>cv(x,y)>c when y<0y<0 for all xx.

  • (d)

    u⁡(x,0)=(x−b)​((x−b)2+|a|)1/2u(x,0)=(x-b)\bigl((x-b)^{2}+|a|\bigr)^{1/2} for all xx.

  • (e)

    v(b,y)=c−y(12|a|+y2+14​a2)−1/2v(b,y)=c-y\Bigl(\frac{1}{2}|a|+\sqrt{y^{2}+\frac{1}{4}a^{2}}\,\,\Bigr)^{-1/2} for all yy.

[03LQ]

Proof. For simplicity, we first consider the case a=0a=0. Let N0,b+i​cN_{0,b+ic} be as in (21), let (z1,z2,z3)∈N0,b+i​c(z_{1},z_{2},z_{3})\in N_{0,b+ic}, and set

x=Re(z3),y=Im(z1z2),u=Re(z1z2)andv=Imz3.x=\mathop{\rm Re}(z_{3}),\quad y=\mathop{\rm Im}(z_{1}z_{2}),\quad u=\mathop{\rm Re}(z_{1}z_{2})\quad\text{and}\quad v=\mathop{\rm Im}z_{3}. (41)

Then z3−(b+i​c)=(x−b)+i⁡(v−c)z_{3}-(b+ic)=(x-b)+i(v-c), and z1​z2=u+i​yz_{1}z_{2}=u+iy. Thus the first condition |z1|2=|z2|2=|z3−b−i​c|2|z_{1}|^{2}=|z_{2}|^{2}=|z_{3}-b-ic|^{2} in (21) becomes

|z1|2=|z2|2=(x−b)2+(v−c)2.|z_{1}|^{2}=|z_{2}|^{2}=(x-b)^{2}+(v-c)^{2}.

Squaring gives |z1​z2|2=((x−b)2+(v−c)2)2|z_{1}z_{2}|^{2}=\bigl((x-b)^{2}+(v-c)^{2}\bigr)^{2}, so substituting for z1​z2z_{1}z_{2} yields

u2+y2=((x−b)2+(v−c)2)2.u^{2}+y^{2}=\bigl((x-b)^{2}+(v-c)^{2}\bigr)^{2}. (42)

Similarly, using the expressions for z1​z2z_{1}z_{2} and z−(b+i​c)z-(b+ic) above, the second and third conditions on (z1,z2,z3)(z_{1},z_{2},z_{3}) in (21) become

u⁡(v−c)+y⁡(x−b)=0\displaystyle u(v-c)+y(x-b)=0 (43)
andu⁡(x−b)−y⁡(v−c)⩾0\displaystyle\text{and}\qquad u(x-b)-y(v-c)\geqslant 0 . (44)

We will use equations (42)–(44) to prove parts (b) and (c) of the proposition. First suppose x=bx=b. Then (43) gives u⁡(v−c)=0u(v-c)=0, so u=0u=0 or v=cv=c. If v=cv=c then (42) gives u2+y2=0u^{2}+y^{2}=0, so u=y=0u=y=0. Thus x=bx=b implies u=0u=0. By a similar argument u=0u=0 implies x=bx=b, so u=0u=0 if and only if x=bx=b, as in part (b). In the same way, v=cv=c if and only if y=0y=0, as in part (c).

We claim that the two terms u⁡(x−b)u(x-b) and −y⁡(v−c)-y(v-c) in (44) are both nonnegative. If one is zero this is obvious. So suppose both are nonzero, so that x−b,y,ux-b,y,u and v−cv-c are all nonzero. From (43), the signs of three of these terms determine the sign of the fourth. It is easy to verify that for all eight sign possibilities, u⁡(x−b)u(x-b) and −y⁡(v−c)-y(v-c) have the same sign. So both are nonnegative by (44). Hence u⁡(x−b)⩾0u(x-b)\geqslant 0, and u=0u=0 if and only if x=bx=b. Clearly, this proves part (b). Part (c) follows in the same way.

Next we shall show that for each pair (x,y)(x,y), there is exactly one pair (u,v)(u,v) satisfying (42)–(44). Multiplying (42) by (v−c)2(v-c)^{2} and replacing u2​(v−c)2u^{2}(v-c)^{2} by y2​(x−b)2y^{2}(x-b)^{2} using (43), we get

(v−c)6+2​(x−b)2​(v−c)4+((x−b)2−y2)​(v−c)2−y2​(x−b)2=0.(v-c)^{6}+2(x-b)^{2}(v-c)^{4}+\bigl((x-b)^{2}-y^{2}\bigr)(v-c)^{2}-y^{2}(x-b)^{2}=0.

This is a sextic in vv, independent of uu. Putting α=(v−c)2\alpha=(v-c)^{2}, it becomes

P⁡(α)=α3+2​(x−b)2​α2+((x−b)2−y2)​α−y2​(x−b)2=0.P(\alpha)=\alpha^{3}+2(x-b)^{2}\alpha^{2}+\bigl((x-b)^{2}-y^{2}\bigr)\alpha-y^{2}(x-b)^{2}=0.

Thus (v−c)2(v-c)^{2} is a real, nonnegative root of the cubic PP. Divide into cases

  • (i)

    x≠bx\neq b, y≠0y\neq 0 and PP has three real roots γ1,γ2,γ3\gamma_{1},\gamma_{2},\gamma_{3}, not necessarily distinct;

  • (ii)

    x≠bx\neq b, y≠0y\neq 0 and PP has one real root γ\gamma and a complex conjugate pair of non-real roots δ,δ¯\delta,\bar{\delta};

  • (iii)

    y=0y=0; and (iv) x=bx=b and y≠0y\neq 0.

We shall show that in cases (i)–(iii), the cubic PP has exactly one real nonnegative root, giving a unique value of (v−c)2(v-c)^{2}. In case (iv) there are two nonnegative roots, but one can be excluded.

In case (i) we have γ1+γ2+γ3=−2​(x−b)2<0\gamma_{1}+\gamma_{2}+\gamma_{3}=-2(x-b)^{2}<0, so at least one γj\gamma_{j} is negative. But γ1​γ2​γ3=y2​(x−b)2>0\gamma_{1}\gamma_{2}\gamma_{3}=y^{2}(x-b)^{2}>0, so an even number of γj\gamma_{j} are negative and an odd number positive. The only possibility is that one γj\gamma_{j} is positive and two negative. So PP has exactly one nonnegative root. In case (ii) we have γ​|δ|2=y2​(x−b)2>0\gamma|\delta|^{2}=y^{2}(x-b)^{2}>0, proving that γ>0\gamma>0, so PP has exactly one nonnegative root. In case (iii) we have P⁡(α)=α​(α+(x−b)2)2P(\alpha)=\alpha\bigl(\alpha+(x-b)^{2}\bigr)^{2}, with roots 0 and −(x−b)2-(x-b)^{2} (twice), so the only nonnegative root is 0.

In case (iv) we have P⁡(α)=α3−y2​αP(\alpha)=\alpha^{3}-y^{2}\alpha, with roots y,0y,0 and −y-y. Thus there are two nonnegative roots, |y||y| and 0. However, if α=0\alpha=0 then (v−c)2=0(v-c)^{2}=0, and (x−b)2=0(x-b)^{2}=0 by assumption, so the right hand side of (42) is zero. But y≠0y\neq 0, so the left hand side is positive, a contradiction. So α≠0\alpha\neq 0, and there is one allowable value for α\alpha, which is |y||y|.

We have shown that (42) and (43) determine (v−c)2(v-c)^{2} uniquely, and that there is a solution (v−c)2(v-c)^{2} for all x,yx,y. This yields (v−c)(v-c) up to sign. But part (c) gives the sign of v−cv-c, so vv is determined uniquely. If v≠cv\neq c, equation (43) determines uu. If v=cv=c then y=0y=0 by (c), so (42) gives u2=(x−b)2u^{2}=(x-b)^{2}, and u=±(x−b)u=\pm(x-b). The sign of uu is given by (b). Therefore for all pairs x,yx,y, there are unique solutions u,vu,v to (42)–(44).

Let us review what we have proved so far. If (z1,z2,z3)∈N0,b+i​c(z_{1},z_{2},z_{3})\in N_{0,b+ic} and x,y,u,vx,y,u,v are defined by (41), then they satisfy (42)–(44). Also, given any x,yx,y there exist unique u,vu,v satisfying (42)–(44). This defines the functions u⁡(x,y),v⁡(x,y)u(x,y),v(x,y) in the proposition uniquely, and it shows that N0,b+i​cN_{0,b+ic} is a subset of the 3-fold NN of (40). The converse, that N⊆N0,b+i​cN\subseteq N_{0,b+ic}, follows easily by reversing the argument above, since if (z1,z2,z3)∈N(z_{1},z_{2},z_{3})\in N then (42)–(44) are equivalent to the equations defining N0,b+i​cN_{0,b+ic}. Hence N=N0,b+i​cN=N_{0,b+ic}.

It remains to prove parts (a), (d) and (e). The smoothness in (a) follows directly from (42)–(44), or indirectly from the fact that N0,b+i​cN_{0,b+ic} is smooth except at (0,0,b+i​c)(0,0,b+ic), and u,vu,v satisfy (33) where they are smooth by Proposition 6.1. For part (d), set y=0y=0. Then v=cv=c by (c), so (42) gives u2=(x−b)4u^{2}=(x-b)^{4}. So u⁡(x,0)=±(x−b)2u(x,0)=\pm(x-b)^{2}, and the sign is determined by (b). Part (e) follows in the same way. This completes the proof for a=0a=0.

When a≠0a\neq 0, equation (42) must be replaced by

u2+y2=((x−b)2+(v−c)2)​((x−b)2+(v−c)2+|a|),u^{2}+y^{2}=\bigl((x-b)^{2}+(v-c)^{2}\bigr)\bigl((x-b)^{2}+(v-c)^{2}+|a|\bigr),

but the rest of the proof is more-or-less unchanged. □\square

Here is the analogue of this for the fibration f′f^{\prime} of Theorem 5.4.

[03LR]
Proposition 6.8

Let a,b,c∈ℝa,b,c\in\mathbin{\mathbb{R}}. Then there exist unique functions u,v:ℝ2→ℝu,v:\mathbin{\mathbb{R}}^{2}\rightarrow\mathbin{\mathbb{R}} such that

N′={(z1,z2,z3)∈ℂ3:Re(z1z2)=u(Re(z3),Im(z1z2)),Im(z3)=v(Re(z3),Im(z1z2)),|z1|2−|z2|2=a}\begin{split}N^{\prime}=\Bigl\{(z_{1}&,z_{2},z_{3})\in\mathbin{\mathbb{C}}^{3}:\mathop{\rm Re}(z_{1}z_{2})=u\bigl(\mathop{\rm Re}(z_{3}),\mathop{\rm Im}(z_{1}z_{2})\bigr),\\ &\mathop{\rm Im}(z_{3})=v\bigl(\mathop{\rm Re}(z_{3}),\mathop{\rm Im}(z_{1}z_{2})\bigr),\quad|z_{1}|^{2}-|z_{2}|^{2}=a\Bigr\}\end{split} (45)

is the special Lagrangian 33-fold Na,b+i​c′N^{\prime}_{a,b+ic} of Definition 5. Furthermore:

  • (a)

    u,vu,v are smooth on ℝ2\mathbin{\mathbb{R}}^{2} and satisfy (33), except at (b,0)(b,0) when a=0a=0, where they are only continuous.

  • (b)

    u⁡(x,y)<0u(x,y)<0 when x>bx>b for all yy, and u⁡(b,y)=0u(b,y)=0 for all yy, and u⁡(x,y)>0u(x,y)>0 when x<bx<b for all yy.

  • (c)

    v⁡(x,y)>cv(x,y)>c when y>0y>0 for all xx, and v⁡(x,0)=cv(x,0)=c for all xx, and v⁡(x,y)<cv(x,y)<c when y<0y<0 for all xx.

  • (d)

    u⁡(x,0)=−(x−b)​((x−b)2+|a|)1/2u(x,0)=-(x-b)\bigl((x-b)^{2}+|a|\bigr)^{1/2} for all xx.

  • (e)

    v(b,y)=c+y(12|a|+y2+14​a2)−1/2v(b,y)=c+y\Bigl(\frac{1}{2}|a|+\sqrt{y^{2}+\frac{1}{4}a^{2}}\,\,\Bigr)^{-1/2} for all yy.

The last three results show that the fibres of the fibrations of Corollary 4.2 and Theorems 5.2 and 5.4 may all be written in the form (30). This will be important to us in §7, where we shall discuss fibrations which mix the properties of these three fibrations, and we will use the coordinate system (30) to define the fibres.

[03LS]

6.3 Other examples of solutions to (32) and (33)

The functions u,vu,v of Propositions 6.7 and 6.8 provide examples of explicit solutions of equations (32) and (33). Here are some more examples of solutions to (32) and (33). The author constructed them by choosing a particular form for u,vu,v involving arbitrary functions of only one variable, and solving the resulting o.d.e.s.

[03LT]

Example 6.9 Let α,b,c∈ℝ\alpha,b,c\in\mathbin{\mathbb{R}} and define u⁡(x,y)=α​y+bu(x,y)=\alpha y+b and v⁡(x,y)=α​x+cv(x,y)=\alpha x+c. Then u,vu,v satisfy (33) for any value of aa. The corresponding special Lagrangian 3-folds are the result of applying a diagonal SU(3)\mathop{\rm SU}(3) matrix to one of the fibres of the fibration of Corollary 4.2.

The next example uses the idea that if u⁡(x)=12​y2​g​(x)−(2​g​(x))−1u(x)={\textstyle\frac{1}{2}}y^{2}g(x)-(2g(x))^{-1} for some function g>0g>0, then (u2+y2)1/2=12​y2​g​(x)+(2​g​(x))−1(u^{2}+y^{2})^{1/2}={\textstyle\frac{1}{2}}y^{2}g(x)+(2g(x))^{-1}. This simplifies (32).

[03LU]

Example 6.10 Define u⁡(x,y)=12​y2​sech2x−12​cosh2⁡xu(x,y)={\textstyle\frac{1}{2}}y^{2}{\textstyle\mathop{\rm sech}}^{2}x-{\textstyle\frac{1}{2}}\cosh^{2}x and v⁡(x,y)=y​tanh⁡xv(x,y)=y\tanh x. Then uu and vv satisfy (32). Equation (31) with a=0a=0 defines an explicit nonsingular special Lagrangian 3-fold NN in ℂ3\mathbin{\mathbb{C}}^{3}. It can be shown that NN is ruled, and arises from Harvey and Lawson’s ‘austere submanifold’ construction [9, §III.3.C] of SL mm-folds in ℂm\mathbin{\mathbb{C}}^{m}, as the normal bundle of a catenoid in ℝ3\mathbin{\mathbb{R}}^{3}.

The following example assumes that u⁡(x,y)=y​g​(x)u(x,y)=y\,g(x) for some nonzero gg.

[03LV]

Example 6.11 Define u⁡(x,y)=−y​sinh⁡2​xu(x,y)=-y\sinh 2x and v=y−12​cosh⁡2​xv=y-{\textstyle\frac{1}{2}}\cosh 2x on the half-plane y⩾0y\geqslant 0 in ℝ2\mathbin{\mathbb{R}}^{2}. Then u,vu,v satisfy (32). So equation (31), with the additional condition that y=Im(z1​z2)⩾0y=\mathop{\rm Im}(z_{1}z_{2})\geqslant 0, defines an explicit special Lagrangian 3-fold NN in ℂ3\mathbin{\mathbb{C}}^{3}. It turns out (surprisingly) that NN is nonsingular, and is equivalent to one of the SL 3-folds constructed in [12, Ex. 7.4] by evolving paraboloids in ℂ3\mathbin{\mathbb{C}}^{3}.

[03LW]

6.4 Isolated singularities of solutions to (32)

We shall now focus on the behaviour of solutions of (32) near points (x,0)(x,0) with u⁡(x,0)=0u(x,0)=0.

[03LX]

Definition 6.12 Let UU be an open subset of ℝ2\mathbin{\mathbb{R}}^{2}, and suppose that u,v:ℝ2→ℝu,v:\mathbin{\mathbb{R}}^{2}\rightarrow\mathbin{\mathbb{R}} are continuous in UU and smooth except at points (x,0)(x,0) with u⁡(x,0)=0u(x,0)=0, and that they satisfy (32) except at such points. As a shorthand we shall often just say that u,v:U→ℝu,v:U\rightarrow\mathbin{\mathbb{R}} satisfy (32), without discussing the exceptional points (x,0)(x,0).

We call a point (x,0)(x,0) in UU with u⁡(x,0)=0u(x,0)=0 a singularity of the solution u,vu,v. We call a singularity (x,0)(x,0) isolated if there exists ϵ>0\epsilon>0 such that the open disc Bϵ​(x,0)B_{\epsilon}(x,0) of radius ϵ\epsilon about (x,0)(x,0) lies in UU, and the only point (x′,y′)(x^{\prime},y^{\prime}) in Bϵ​(x,0)B_{\epsilon}(x,0) with u⁡(x′,y′)=0u(x^{\prime},y^{\prime})=0 and v⁡(x′,y′)=v⁡(x,0)v(x^{\prime},y^{\prime})=v(x,0) is (x,0)(x,0).

Let (x,0)(x,0) be an isolated singularity of u,vu,v, and let ϵ\epsilon be as above. Consider the map γ:𝒮1→ℂ\gamma:{\mathcal{S}}^{1}\rightarrow\mathbin{\mathbb{C}} given by

γ:ei​θ↦u⁡(x+12​ϵ​cos⁡θ,12​ϵ​sin⁡θ)−i​v​(x+12​ϵ​cos⁡θ,12​ϵ​sin⁡θ)+i​v​(x,0).\gamma:{\rm e}^{i\theta}\mapsto u\bigl(x+{\textstyle\frac{1}{2}}\epsilon\cos\theta,{\textstyle\frac{1}{2}}\epsilon\sin\theta\bigr)-iv\bigl(x+{\textstyle\frac{1}{2}}\epsilon\cos\theta,{\textstyle\frac{1}{2}}\epsilon\sin\theta\bigr)+iv(x,0).

As (x,0)(x,0) is isolated we see that γ\gamma is smooth and maps 𝒮1→ℂ∖{0}{\mathcal{S}}^{1}\rightarrow\mathbin{\mathbb{C}}\setminus\{0\}. Define the order of the isolated singularity (x,0)(x,0) to be the winding number of γ\gamma about 0 in ℂ\mathbin{\mathbb{C}}. It is easy to show that the order is independent of ϵ\epsilon, provided ϵ>0\epsilon>0 is sufficiently small.

Not all singularities are isolated. For instance, if we put u⁡(x,y)=α​yu(x,y)=\alpha y and v⁡(x,y)=α​x+cv(x,y)=\alpha x+c for α,c∈ℝ\alpha,c\in\mathbin{\mathbb{R}}, as in Example 6.3, then (x,0)(x,0) is a nonisolated singularity for all xx. However, the author believes that nonisolated singularities are rather nongeneric, and so not of much interest in this paper. Also, by analogy with the Identity Theorem of complex analysis, the author conjectures that if (x,0)(x,0) is a singularity of u,vu,v and xx is an isolated zero of u⁡(x′,0)u(x^{\prime},0), then (x,0)(x,0) is isolated.

The motivation for this definition is as follows. In §6.1 we saw that equation (32) is a nonlinear version of the Cauchy–Riemann equations for u−i​vu-iv to be a holomorphic function of x+i​yx+iy. So it seems reasonable for singularities of u,vu,v to be a bit like zeros of holomorphic functions.

But zeros of holomorphic functions have an order, which is a positive integer. Definition 6.4 mimics the definition of this. In particular, if u−i​vu-iv were really holomorphic near (x,0)(x,0) then for (x′,y′)(x^{\prime},y^{\prime}) near (x,0)(x,0) we would expect

u⁡(x′,y′)−i​v​(x′,y′)≈α​(x′−x+i​y′)k+i​cu(x^{\prime},y^{\prime})-iv(x^{\prime},y^{\prime})\approx\alpha(x^{\prime}-x+iy^{\prime})^{k}+ic

for α∈ℂ∖{0}\alpha\in\mathbin{\mathbb{C}}\setminus\{0\}, c∈ℝc\in\mathbin{\mathbb{R}} and k>0k>0 in ℤ\mathbin{\mathbb{Z}}, and the order of (x,0)(x,0) would be kk.

Our next result follows from Propositions 6.7 and 6.8. In particular, parts (b) and (c) of each imply that the singularity is isolated and of order 1.

[03LY]
Lemma 6.13

Let a=0a=0 and b,c∈ℝb,c\in\mathbin{\mathbb{R}}. Then the solutions u,vu,v of (32) defined in Propositions 6.7 and 6.8 both have an isolated zero of order 11 at (b,0)(b,0).

Here is a conjecture on isolated singularities.

[03LZ]
Conjecture 6.14

Isolated singularities of solutions u,vu,v of (32) have the following properties:

  • (a)

    Let u,vu,v satisfy (32) on an open set UU in ℝ2\mathbin{\mathbb{R}}^{2}, and let (x,0)(x,0) be an isolated singularity of u,vu,v. Then the order of (x,0)(x,0) is a positive integer.

  • (b)

    For each k⩾1k\geqslant 1, there exist solutions u,vu,v of (32) defined on a small ball BB about (0,0)(0,0) in ℝ2\mathbin{\mathbb{R}}^{2}, with an isolated zero of order kk at (0,0)(0,0).

  • (c)

    For kk odd, the solutions u,vu,v in part (b) may be chosen to satisfy

    u⁡(x,y)=u⁡(x,−y)=−u⁡(−x,y)andv⁡(x,y)=−v⁡(x,−y)=v⁡(−x,y)u(x,y)=u(x,-y)=-u(-x,y)\quad\text{and}\quad v(x,y)=-v(x,-y)=v(-x,y)

    for all (x,y)∈B(x,y)\in B, and such that u⁡(x,0)u(x,0) is a strictly increasing function.

  • (d)

    For kk even, the solutions u,vu,v in part (b) may be chosen to satisfy

    u⁡(x,y)=u⁡(x,−y)=u⁡(−x,y)andv⁡(x,y)=−v⁡(x,−y)=−v⁡(−x,y)u(x,y)=u(x,-y)=u(-x,y)\quad\text{and}\quad v(x,y)=-v(x,-y)=-v(-x,y)

    for all (x,y)∈B(x,y)\in B, and such that u⁡(x,0)u(x,0) is strictly increasing for x>0x>0 and strictly decreasing for x<0x<0.

Note that if u,vu,v are solutions of (25), then so are u′,v′u^{\prime},v^{\prime}, where u′=−uu^{\prime}=-u and v′=−vv^{\prime}=-v. If u⁡(x,0)u(x,0) is strictly increasing, as in (c), then u′​(x,0)u^{\prime}(x,0) is strictly decreasing. Similarly, if u⁡(x,0)u(x,0) is strictly increasing for x>0x>0 and decreasing for x<0x<0, then u′​(x,0)u^{\prime}(x,0) is strictly decreasing for x>0x>0 and increasing for x<0x<0. The author speculates that there are essentially only two kinds of isolated singularity at (0,0) of order kk, those in which u⁡(x,0)u(x,0) increases or decreases near x=0x=0 as in the conjecture, and those in which it does the opposite.

The author does not yet know how to prove Conjecture 6.14. However, by Proposition 6.5 the conjecture can be reduced to a statement about singular solutions of the second-order nonlinear p.d.e.

∂2f∂x2+2​((∂f∂x)2+y2)1/2​∂2f∂y2=0\frac{\partial^{2}f}{\partial x^{2}}+2\Bigl(\Bigl(\frac{\partial f}{\partial x}\Bigr)^{2}+y^{2}\Bigr)^{1/2}\frac{\partial^{2}f}{\partial y^{2}}=0 (46)

on ℝ2\mathbin{\mathbb{R}}^{2}. This is a fairly simple equation, and it seems likely that the conjecture could be proved (or disproved) using existing results. If any reader knows how to do this, the author would be glad to be told.

As supporting evidence for Conjecture 6.14, consider the related linear problem of functions f:ℝ2→ℝf:\mathbin{\mathbb{R}}^{2}\rightarrow\mathbin{\mathbb{R}} satisfying

∂2f∂x2+2​(x4+y2)1/2​∂2f∂y2=0.\frac{\partial^{2}f}{\partial x^{2}}+2(x^{4}+y^{2})^{1/2}\frac{\partial^{2}f}{\partial y^{2}}=0. (47)

This equation has singular behaviour at (0,0)(0,0) that is somewhat similar to that of (46) at points (x,0)(x,0) with ∂f∂x​(x,0)=0\frac{\partial f}{\partial x}(x,0)=0. It also has a useful scaling property: if f⁡(x,y)f(x,y) is a solution to (47) then so is f⁡(t​x,t2​y)f(tx,t^{2}y) for any t>0t>0.

Therefore we may look for solutions ff of (47) which are homogeneous of order α\alpha under this scaling, so that f⁡(t​x,t2​y)=tα​f​(x,y)f(tx,t^{2}y)=t^{\alpha}f(x,y) for some α>2\alpha>2. Then ff is determined by α\alpha and its values on the circle x2+y2=1x^{2}+y^{2}=1, and (47) reduces to a linear o.d.e. on the circle.

For generic values of α\alpha this o.d.e. has no nonzero solutions, but for a discrete set of values of α\alpha there do exist nontrivial solutions, which give solutions of (47). By studying these homogeneous solutions, the author is able to prove an analogue of Conjecture 6.14 for the equations

∂u∂x=−2​(x4+y2)1/2​∂v∂yand∂u∂y=∂v∂x.\frac{\partial u}{\partial x}=-2\bigl(x^{4}+y^{2}\bigr)^{1/2}\frac{\partial v}{\partial y}\quad\text{and}\quad\frac{\partial u}{\partial y}=\frac{\partial v}{\partial x}.
[03M0]

6.5 Geometric interpretation

Suppose that u,vu,v are solutions of (32) near (0,0)(0,0) in ℝ2\mathbin{\mathbb{R}}^{2}, with an isolated singularity of order kk at (0,0)(0,0), and that u⁡(0,0)=v⁡(0,0)=0u(0,0)=v(0,0)=0. Let NN be the associated SL 3-fold in ℂ3\mathbin{\mathbb{C}}^{3}, defined by (31) with a=0a=0. Then NN has an isolated singular point at (0,0,0)(0,0,0). What can we say about it?

Well, the coordinates x,yx,y give a natural map from NN to ℝ2\mathbin{\mathbb{R}}^{2}. The fibre of this map over (0,0)(0,0) is a point, and the fibre of the map over other points (x,y)≠(0,0)(x,y)\neq(0,0) near (0,0)(0,0) in ℝ2\mathbin{\mathbb{R}}^{2} is a circle. Thus, NN near (0,0,0)(0,0,0) has the topology of 𝒮1×ℝ2{\mathcal{S}}^{1}\times\mathbin{\mathbb{R}}^{2} with 𝒮1×{(0,0)}{\mathcal{S}}^{1}\times\bigl\{(0,0)\bigr\} collapsed to a point. That is, topologically NN is a T2T^{2}-cone near (0,0,0)(0,0,0).

The author conjectures that when k=1k=1, to leading order uu and vv should agree with the functions u,vu,v of Proposition 6.7 or 6.8 with a=b=c=0a=b=c=0, at least in the generic case, and therefore that the tangent cone to NN at (0,0,0)(0,0,0) should be one of the T2T^{2}-cones L0±L_{0}^{\pm} from (16). This gives a good description of the local geometry of NN when k=1k=1.

When k>1k>1, the author conjectures that u,vu,v satisfy

u⁡(x,y)=o⁡(x2+|y|)andv⁡(x,y)=o⁡(|x|+|y|1/2)for small x,y.u(x,y)=o\bigl(x^{2}+|y|\bigr)\quad\text{and}\quad v(x,y)=o\bigl(|x|+|y|^{1/2}\bigr)\quad\text{for small $x,y$.} (48)

This is because u⁡(x,y)=O⁡(x2+|y|)u(x,y)=O(x^{2}+|y|) and v⁡(x,y)=O⁡(|x|+|y|1/2)v(x,y)=O(|x|+|y|^{1/2}) when k=1k=1, and by analogy with the zeros of holomorphic functions we expect zeros of higher order to decrease more quickly near (0,0)(0,0).

Let t>0t>0, and define t−1​N={t−1​𝐳:𝐳∈N}t^{-1}N=\{t^{-1}{\bf z}:{\bf z}\in N\}. Then t−1​Nt^{-1}N is also an SL 3-fold, and may be written in the form (30) with u,vu,v replaced by

ut​(x,y)=t−2​u​(t​x,t2​y)andvt​(x,y)=t−1​v​(t​x,t2​y).u^{t}(x,y)=t^{-2}u(tx,t^{2}y)\quad\text{and}\quad v^{t}(x,y)=t^{-1}v(tx,t^{2}y).

Now equation (48) implies that ut​(x,y)→0u^{t}(x,y)\rightarrow 0 and vt​(x,y)→0v^{t}(x,y)\rightarrow 0 as t→0t\rightarrow 0 for fixed x,yx,y. It follows that t−1​Nt^{-1}N converges to

N0={(z1,z2,z3)∈ℂ3:Re(z1z2)=0,Im(z3)=0,|z1|=|z2|}N_{0}=\bigl\{(z_{1},z_{2},z_{3})\in\mathbin{\mathbb{C}}^{3}:\mathop{\rm Re}(z_{1}z_{2})=0,\quad\mathop{\rm Im}(z_{3})=0,\quad|z_{1}|=|z_{2}|\bigr\}

as t→0t\rightarrow 0, and this is the tangent cone to NN at (0,0,0)(0,0,0).

But this is just the union of the two special Lagrangian 3-planes

Π+={(z,iz¯,x):z∈ℂ,x∈ℝ},Π−={(z,−iz¯,x):z∈ℂ,x∈ℝ},\Pi_{+}=\bigl\{(z,i\bar{z},x):z\in\mathbin{\mathbb{C}},\quad x\in\mathbin{\mathbb{R}}\bigr\},\quad\Pi_{-}=\bigl\{(z,-i\bar{z},x):z\in\mathbin{\mathbb{C}},\quad x\in\mathbin{\mathbb{R}}\bigr\},

which intersect in the real line {(0,0,x):x∈ℝ}\bigl\{(0,0,x):x\in\mathbin{\mathbb{R}}\bigr\}. Thus, when k>1k>1 we expect NN to resemble the union of two SL 3-planes Π±\Pi_{\pm} intersecting in a line, to leading order near (0,0,0)(0,0,0).

As this tangent cone is singular not just at (0,0,0)(0,0,0) but all along the line Π+∩Π−\Pi_{+}\cap\Pi_{-}, to have a good picture of NN near (0,0,0)(0,0,0) we need to include the next nonzero terms in uu and vv as well. Unfortunately, the author does not know what these terms are. But here is a rather crude approximation, which illustrates the kind of behaviour we expect.

For k>1k>1 even, suppose that u⁡(x,y)≈|x|αu(x,y)\approx|x|^{\alpha} for some α>2\alpha>2, and v⁡(x,y)≈0v(x,y)\approx 0 for small x,yx,y. Then we have

N≈{(z1,z2,z3)∈ℂ3:Re(z1​z2)=|Re(z3)|α,Im(z3)=0,|z1|=|z2|}.\begin{split}N\approx\bigl\{(z_{1},z_{2},z_{3})\in\mathbin{\mathbb{C}}^{3}:&\mathop{\rm Re}(z_{1}z_{2})=|\mathop{\rm Re}(z_{3})|^{\alpha},\\ &\mathop{\rm Im}(z_{3})=0,\quad|z_{1}|=|z_{2}|\bigr\}.\end{split} (49)

This may be written more nicely in different coordinates on ℂ3\mathbin{\mathbb{C}}^{3}. Define new coordinates (w1,w2,x1,x2)(w_{1},w_{2},x_{1},x_{2}) on ℂ3\mathbin{\mathbb{C}}^{3} by

w1=z1−i​z¯2,w2=z2+i​z¯1,x1=Re(z3),x2=Im(z3).w_{1}=z_{1}-i\bar{z}_{2},\quad w_{2}=z_{2}+i\bar{z}_{1},\quad x_{1}=\mathop{\rm Re}(z_{3}),\quad x_{2}=\mathop{\rm Im}(z_{3}).

Then w1​w2=2​Re(z1​z2)+i⁡(|z1|2−|z2|2)w_{1}w_{2}=2\mathop{\rm Re}(z_{1}z_{2})+i\bigl(|z_{1}|^{2}-|z_{2}|^{2}\bigr). Therefore, in these new coordinates, (49) becomes

N≈{(w1,w2,x1,x2)∈ℂ2×ℝ2:w1w2=2|x1|α,x2=0}.N\approx\bigl\{(w_{1},w_{2},x_{1},x_{2})\in\mathbin{\mathbb{C}}^{2}\times\mathbin{\mathbb{R}}^{2}:w_{1}w_{2}=2|x_{1}|^{\alpha},\quad x_{2}=0\bigr\}. (50)

So NN may be thought of as approximating a slowly varying 1-parameter family of complex quadratics w1​w2=cw_{1}w_{2}=c in ℂ2\mathbin{\mathbb{C}}^{2}, for c∈ℝc\in\mathbin{\mathbb{R}} varying with x1x_{1}. When x1=0x_{1}=0 the quadratic degenerates into w1​w2=0w_{1}w_{2}=0, the union of two complex lines in ℂ2\mathbin{\mathbb{C}}^{2}. For k>1k>1 odd, the appropriate approximation is u⁡(x,y)≈x​|x|α−1u(x,y)\approx x|x|^{\alpha-1} for some α>2\alpha>2 and v⁡(x,y)≈0v(x,y)\approx 0, and then

N≈{(w1,w2,x1,x2)∈ℂ2×ℝ2:w1w2=2x1|x1|α−1,x2=0}.N\approx\bigl\{(w_{1},w_{2},x_{1},x_{2})\in\mathbin{\mathbb{C}}^{2}\times\mathbin{\mathbb{R}}^{2}:w_{1}w_{2}=2x_{1}|x_{1}|^{\alpha-1},\quad x_{2}=0\bigr\}. (51)

We stress that (50) and (51) are just very approximate guesses, and the true behaviour of u,vu,v and NN will be different and more complicated than this.

[03M1]

7 Higher-order singularities of SL fibrations

Theorems 5.2 and 5.4 gave explicit SL fibrations f,f′:ℂ3→ℝ3f,f^{\prime}:\mathbin{\mathbb{C}}^{3}\rightarrow\mathbin{\mathbb{R}}^{3} with singular fibres of codimension one in ℝ3\mathbin{\mathbb{R}}^{3}. These are our local models for the most generic singularities of special Lagrangian fibrations of Calabi–Yau 3-folds. But there will also be other kinds of singularity in such fibrations.

In this section we describe a conjectural local model f:ℂ3→ℝ3f:\mathbin{\mathbb{C}}^{3}\rightarrow\mathbin{\mathbb{R}}^{3} for the next most generic kind of singularity in SL fibrations of CY 3-folds, which occurs in codimension two. That is, ff has singular fibres in codimension one in ℝ3\mathbin{\mathbb{R}}^{3}, most of which are locally modelled on Theorems 5.2 and 5.4. But in a subset ℝ\mathbin{\mathbb{R}} of codimension two in ℝ3\mathbin{\mathbb{R}}^{3} there will be a different kind of singular fibre.

The singular fibres in Theorems 5.2 and 5.4 have only one singularity, which is a T2T^{2}-cone. In the fibrations described below, generic singular fibres in codimension one have two T2T^{2}-cone singular points. In codimension two these two points come together and fuse to form a new kind of singularity. Topologically this is also a T2T^{2}-cone, but geometrically things are more complicated.

[03M2]

7.1 A conjectural local model for SL fibrations

We shall proceed by giving a series of assumptions that define the properties of the fibrations we seek to construct. Here is the first, largely concerned with the symmetries of the fibration.

[03M3]

Assumption 7.1 Let UU be a connected open neighbourhood of (0,0,0)(0,0,0) in ℂ3\mathbin{\mathbb{C}}^{3}, which is invariant under the symmetries in parts (ii) and (v)–(viii) below. We aim to construct a special Lagrangian fibration f:U→ℝ3f:U\rightarrow\mathbin{\mathbb{R}}^{3}, with fibres Na,b,c=f−1​(a,b,c)N_{a,b,c}=f^{-1}(a,b,c), with the following properties:

  • (i)

    ff is continuous, and smooth except on the real hypersurface |z1|=|z2||z_{1}|=|z_{2}|.

  • (ii)

    f⁡(ei​θ​z1,e−i​θ​z2,z3)=f⁡(z1,z2,z3)f({\rm e}^{i\theta}z_{1},{\rm e}^{-i\theta}z_{2},z_{3})=f(z_{1},z_{2},z_{3}) for all (z1,z2,z3)∈U(z_{1},z_{2},z_{3})\in U and θ∈ℝ\theta\in\mathbin{\mathbb{R}}. Equivalently, every fibre Na,b,cN_{a,b,c} is invariant under the U(1)\mathbin{\rm U}(1)-action given by

    ei​θ:(z1,z2,z3)↦(ei​θ​z1,e−i​θ​z2,z3).{\rm e}^{i\theta}:(z_{1},z_{2},z_{3})\mapsto({\rm e}^{i\theta}z_{1},{\rm e}^{-i\theta}z_{2},z_{3}). (52)
  • (iii)

    If f⁡(z1,z2,z3)=(a,b,c)f(z_{1},z_{2},z_{3})=(a,b,c) then a=|z1|2−|z2|2a=|z_{1}|^{2}-|z_{2}|^{2}.

  • (iv)

    The set of singular points of singular fibres of ff is {(0,0,z3)∈U}\bigl\{(0,0,z_{3})\in U\bigr\}. In particular, Na,b,cN_{a,b,c} is nonsingular if a≠0a\neq 0.

  • (v)

    If f⁡(z1,z2,z3)=(a,b,c)f(z_{1},z_{2},z_{3})=(a,b,c) then f⁡(z1,z2,z3+i​t)=(a,b,c+t)f(z_{1},z_{2},z_{3}+it)=(a,b,c+t) for all t∈ℝt\in\mathbin{\mathbb{R}}. This means that Na,b,c+tN_{a,b,c+t} is the translation of Na,b,cN_{a,b,c} by (0,0,i​t)(0,0,it), and that

    Na,b,c={(z1,z2,z3+i​c):(z1,z2,z3)∈Na,b,0}.N_{a,b,c}=\bigl\{(z_{1},z_{2},z_{3}+ic):(z_{1},z_{2},z_{3})\in N_{a,b,0}\bigr\}. (53)
  • (vi)

    If f⁡(z1,z2,z3)=(a,b,c)f(z_{1},z_{2},z_{3})=(a,b,c) then f⁡(z2,z1,z3)=(−a,b,c)f(z_{2},z_{1},z_{3})=(-a,b,c).

  • (vii)

    If f⁡(z1,z2,z3)=(a,b,c)f(z_{1},z_{2},z_{3})=(a,b,c) then f⁡(z¯1,z¯2,z¯3)=(a,b,−c)f(\bar{z}_{1},\bar{z}_{2},\bar{z}_{3})=(a,b,-c).

  • (viii)

    If f⁡(z1,z2,z3)=(a,b,c)f(z_{1},z_{2},z_{3})=(a,b,c) then f⁡(z1,z2,−z3)=(a,b,−c)f(z_{1},z_{2},-z_{3})=(a,b,-c).

Really we would like the domain UU of ff to be all of ℂ3\mathbin{\mathbb{C}}^{3}, and perhaps also to impose some asymptotic conditions on ff at infinity. But this would make our assumptions unnecessarily strong, and the author is not sure what asymptotic conditions would be appropriate. So instead we just suppose that ff is defined near (0,0,0)(0,0,0). We will not worry very much about the issues raised by ff not being defined on all of ℂ3\mathbin{\mathbb{C}}^{3}, as they are primarily notational.

To understand where this list of properties has come from, note that the fibrations of Corollary 4.2 and Theorems 5.2 and 5.4 satisfy all of Assumption 7.1, except part (viii). We are aiming for a fibration that at a generic singular point is modelled one of the fibrations of Theorems 5.2 and 5.4, but will also have features in common with that of Corollary 4.2.

Therefore we simplify things by assuming that nearly all the symmetries these three fibrations have in common are also symmetries of the fibration we are aiming to construct. Here is our second assumption, drawing on the ideas of §6.

[03M4]

Assumption 7.2 Suppose that each fibre Na,b,cN_{a,b,c} of ff may be written

Na,b,c={(OPENz1,z2,z3)∈U:Re(z1​z2)=ua,b​(Re(z3),Im(z1​z2)),Im(z3)=va,b(Re(z3),Im(z1z2))+c,|z1|2−|z2|2=a},\begin{split}N_{a,b,c}=\Bigl\{(&z_{1},z_{2},z_{3})\in U:\mathop{\rm Re}(z_{1}z_{2})=u_{a,b}\bigl(\mathop{\rm Re}(z_{3}),\mathop{\rm Im}(z_{1}z_{2})\bigr),\\ &\mathop{\rm Im}(z_{3})=v_{a,b}\bigl(\mathop{\rm Re}(z_{3}),\mathop{\rm Im}(z_{1}z_{2})\bigr)+c,\;\>|z_{1}|^{2}-|z_{2}|^{2}=a\Bigr\},\end{split} (54)

where ua,b,va,b:Va,b→ℝu_{a,b},v_{a,b}:V_{a,b}\rightarrow\mathbin{\mathbb{R}} are 2-parameter families of functions and

Va,b={(Re(z3),Im(z1​z2)):(z1,z2,z3)∈Na,b,0}V_{a,b}=\bigl\{\bigl(\mathop{\rm Re}(z_{3}),\mathop{\rm Im}(z_{1}z_{2})\bigr):(z_{1},z_{2},z_{3})\in N_{a,b,0}\bigr\} (55)

is an open set in ℝ2\mathbin{\mathbb{R}}^{2}. Suppose also that the ua,b,va,bu_{a,b},v_{a,b} satisfy:

  • (i)

    u0,b,v0,bu_{0,b},v_{0,b} are smooth except at points (x,0)(x,0) in V0,bV_{0,b} with u0,b​(x,0)=0u_{0,b}(x,0)=0, and

    ∂u0,b∂x=−2​(u0,b2+y2)1/2​∂v0,b∂yand∂u0,b∂y=∂v0,b∂x\frac{\partial u_{0,b}}{\partial x}=-2\bigl(u_{0,b}^{2}+y^{2}\bigr)^{1/2}\frac{\partial v_{0,b}}{\partial y}\quad\text{and}\quad\frac{\partial u_{0,b}}{\partial y}=\frac{\partial v_{0,b}}{\partial x} (56)

    hold except at these points.

  • (ii)

    When a≠0a\neq 0, ua,bu_{a,b} and va,bv_{a,b} are smooth on Va,bV_{a,b} and satisfy

    ∂ua,b∂x=−(4​ua,b2+4​y2+a2)1/2​∂va,b∂yand∂ua,b∂y=∂va,b∂x.\frac{\partial u_{a,b}}{\partial x}=-\bigl(4u_{a,b}^{2}+4y^{2}+a^{2}\bigr)^{1/2}\frac{\partial v_{a,b}}{\partial y}\quad\text{and}\quad\frac{\partial u_{a,b}}{\partial y}=\frac{\partial v_{a,b}}{\partial x}. (57)
  • (iii)

    ua,bu_{a,b} and va,bv_{a,b} depend continuously on a,ba,b, and smoothly wherever a≠0a\neq 0.

  • (iv)

    ua,b≡u−a,bu_{a,b}\equiv u_{-a,b} and va,b≡v−a,bv_{a,b}\equiv v_{-a,b} for all a,ba,b.

  • (v)

    ua,b​(x,−y)=ua,b​(x,y)u_{a,b}(x,-y)=u_{a,b}(x,y) and va,b​(x,−y)=−va,b​(x,y)v_{a,b}(x,-y)=-v_{a,b}(x,y) for all a,b,x,ya,b,x,y.

  • (vi)

    ua,b​(−x,y)=ua,b​(x,y)u_{a,b}(-x,y)=u_{a,b}(x,y) and va,b​(−x,y)=−va,b​(x,y)v_{a,b}(-x,y)=-v_{a,b}(x,y) for all a,b,x,ya,b,x,y.

Here equation (54) essentially says that the fibres of ff may be written in the form (30). The explicit dependence on cc follows from part (v) of Assumption 7.1. Parts (i) and (ii) come from Proposition 6.1, and parts (iii)–(vi) from parts (i) and (vi)–(viii) of Assumption 7.1 respectively. Thus, the only thing Assumption 7.1 adds to Assumption 7.1 is that the fibres of ff may be written in the form (30).

Next we impose some conditions of a general topological nature which specify the ‘shape’ of the fibration we want, in particular the location and nature of its singularities.

[03M5]

Assumption 7.3 In the situation above, the functions ua,bu_{a,b} and va,bv_{a,b} satisfy

  • (i)

    For all a,ba,b, the function ua,b​(x,0)u_{a,b}(x,0) is strictly increasing for x<0x<0 and strictly decreasing for x>0x>0, with a maximum at 0.

  • (ii)

    For all a,b,b′,x,ya,b,b^{\prime},x,y with b<b′b<b^{\prime} we have ua,b​(x,y)<ua,b′​(x,y)u_{a,b}(x,y)<u_{a,b^{\prime}}(x,y).

  • (iii)

    Let b>0b>0, and write b=β2b=\beta^{2} for β>0\beta>0. Then ua,b​(β,0)=ua,b​(−β,0)=0u_{a,b}(\beta,0)=u_{a,b}(-\beta,0)=0 for all aa. The solution u0,b,v0,bu_{0,b},v_{0,b} of (32) has isolated singularities of order 1 at (±β,0)(\pm\beta,0), in the sense of Definition 6.4.

    Near (−β,0)(-\beta,0) for small aa, the functions ua,b,va,bu_{a,b},v_{a,b} are approximately equal to the functions u,vu,v constructed from Na,−βN_{a,-\beta} in Proposition 6.7.

    Near (β,0)(\beta,0) for small aa, the functions ua,b,va,bu_{a,b},v_{a,b} are approximately equal to the functions u,vu,v constructed from Na,β′N^{\prime}_{a,\beta} in Proposition 6.8.

  • (iv)

    For all aa we have ua,0​(0,0)=0u_{a,0}(0,0)=0, and the solution u0,0,v0,0u_{0,0},v_{0,0} of (32) has an isolated singularity of order 2 at (0,0)(0,0), in the sense of Definition 6.4.

  • (v)

    For all a,x∈ℝa,x\in\mathbin{\mathbb{R}} and b<0b<0, we have ua,b​(x,0)<0u_{a,b}(x,0)<0.

We will see in §7.2 that ua,bu_{a,b} and va,bv_{a,b} actually depend only on the values of ua,bu_{a,b} on the xx-axis. In Figure 1 we sketch the functions u0,b​(x,0)u_{0,b}(x,0) for several values of bb, on the same graph, to display the general features we expect of these functions. The curves are smooth except where they intersect the xx-axis. The condition that u0,b​(x,0)<u0,b′​(x,0)u_{0,b}(x,0)<u_{0,b^{\prime}}(x,0) when b<b′b<b^{\prime} corresponds to the fact that the curves do not intersect, and move up the graph as bb increases.

u0,b​(x,0)\textstyle{u_{0,b}(x,0)}x\textstyle{x} 0\textstyle{\,\scriptstyle 0}+\textstyle{\scriptstyle+}1\textstyle{\scriptstyle 1}+\textstyle{\scriptstyle+}2\textstyle{\scriptstyle\sqrt{2}}+\textstyle{\scriptstyle+}3\textstyle{\scriptstyle\sqrt{3}}+\textstyle{\scriptstyle+}2\textstyle{\scriptstyle 2}+\textstyle{\scriptstyle+}−1\textstyle{\scriptstyle-1\,\,}+\textstyle{\scriptstyle+}−2\textstyle{\scriptstyle-\sqrt{2}\,\,}+\textstyle{\scriptstyle+}−3\textstyle{\scriptstyle-\sqrt{3}\,\,}+\textstyle{\scriptstyle+}−2\textstyle{\scriptstyle-2\,\,}b=−2\textstyle{b=-2}b=−1\textstyle{b=-1}b=0\textstyle{b=0}b=1\textstyle{b=1}b=2\textstyle{\,b=2}b=3\textstyle{\,b=3}b=4\textstyle{\,b=4}

Figure 1: approximate curves u0,b​(x,0)u_{0,b}(x,0) for different bb

For β>0\beta>0 and b=β2b=\beta^{2}, the curve u0,b​(x,0)u_{0,b}(x,0) intercepts the xx-axis at (±β,0)(\pm\beta,0). By part (d) of Propositions 6.7 and 6.8 and part (iii) of Assumption 7.1, near (−β,0)(-\beta,0) we have u0,b​(x,0)≈(x+β)​|x+β|u_{0,b}(x,0)\approx(x+\beta)|x+\beta|, and near (β,0)(\beta,0) we have u0,b​(x,0)≈−(x−β)​|x−β|u_{0,b}(x,0)\approx-(x-\beta)|x-\beta|. Thus u0,b​(x,0)u_{0,b}(x,0) is differentiable at (±β,0)(\pm\beta,0) with gradient zero.

For comparison, in Figure 2 we sketch the functions ua,b​(x,0)u_{a,b}(x,0) for some small fixed a≠0a\neq 0, and the same values of bb. The general shapes of the curves are the same, as are the intercepts with the xx-axis. But the curves are all smooth, and using part (d) of Propositions 6.7 and 6.8 and part (iii) of Assumption 7.1, we see that

ua,b​(x,0)\displaystyle u_{a,b}(x,0) ≈(x+β)​((x+β)2+|a|)1/2\displaystyle\approx(x+\beta)\bigl((x+\beta)^{2}+|a|\bigr)^{1/2} near x=−βx=-\beta, and
ua,b​(x,0)\displaystyle u_{a,b}(x,0) ≈−(x−β)​((x−β)2+|a|)1/2\displaystyle\approx-(x-\beta)\bigl((x-\beta)^{2}+|a|\bigr)^{1/2} near x=βx=\beta,

so that the gradient at (−β,0)(-\beta,0) is approximately |a|1/2|a|^{1/2}, and at (β,0)(\beta,0) approximately −|a|1/2-|a|^{1/2}. However, this approximation breaks down near β=0\beta=0.

ua,b​(x,0)\textstyle{u_{a,b}(x,0)}x\textstyle{x} 0\textstyle{\,\scriptstyle 0}+\textstyle{\scriptstyle+}1\textstyle{\scriptstyle 1}+\textstyle{\scriptstyle+}2\textstyle{\scriptstyle\sqrt{2}}+\textstyle{\scriptstyle+}3\textstyle{\scriptstyle\sqrt{3}}+\textstyle{\scriptstyle+}2\textstyle{\scriptstyle 2}+\textstyle{\scriptstyle+}−1\textstyle{\scriptstyle-1\,\,}+\textstyle{\scriptstyle+}−2\textstyle{\scriptstyle-\sqrt{2}\,\,}+\textstyle{\scriptstyle+}−3\textstyle{\scriptstyle-\sqrt{3}\,\,}+\textstyle{\scriptstyle+}−2\textstyle{\scriptstyle-2\,\,}b=−2\textstyle{b=-2}b=−1\textstyle{b=-1}b=0\textstyle{b=0}b=1\textstyle{b=1}b=2\textstyle{\,b=2}b=3\textstyle{\,b=3}b=4\textstyle{\,b=4}

Figure 2: curves ua,b​(x,0)u_{a,b}(x,0) for fixed small a≠0a\neq 0 and different bb

Recall that our goal is to model a fibration in which generic singular fibres in codimension one have two singularities, each locally a T2T^{2}-cone, but in codimension two these two cone points come together and fuse to form a new kind of singularity.

Assumption 7.1 implies that when b=β2b=\beta^{2} for β>0\beta>0, the fibre N0,b,cN_{0,b,c} will have two singular points at (0,0,±β+i​c)(0,0,\pm\beta+ic). Near (0,0,−β+i​c)(0,0,-\beta+ic) it is locally modelled on the special Lagrangian T2T^{2}-cone N0,−β+i​cN_{0,-\beta+ic} of Definition 5, and near (0,0,β+i​c)(0,0,\beta+ic) it is locally modelled on the SL T2T^{2}-cone N0,β+i​c′N^{\prime}_{0,\beta+ic} of Definition 5.

When b=0b=0, the fibre N0,0,cN_{0,0,c} has one singular point at (0,0,i​c)(0,0,ic). It results from an isolated singular point of order 2 in u0,0,v0,0u_{0,0},v_{0,0}, so as in §6.4 we expect the tangent cone at (0,0,i​c)(0,0,ic) to be the union of two special Lagrangian 3-planes Π±\Pi_{\pm} intersecting in a real line. We cannot describe the singularity of N0,0,cN_{0,0,c} much more explicitly without proving Conjecture 6.14.

When b<0b<0, the fibre N0,b,cN_{0,b,c} is nonsingular. Thus the picture is that as bb decreases from positive to negative, two T2T^{2}-cone singular points in N0,b,cN_{0,b,c} come together, fuse to form a new kind of singularity, and then vanish. We can think of the two singular points in N0,b,cN_{0,b,c} for b>0b>0 as having opposite sign, so that when they come together they cancel out.

We can now formulate our main conjecture.

[03M6]
Conjecture 7.4

There exists an open neighbourhood UU of (0,0,0)(0,0,0) in ℂ3\mathbin{\mathbb{C}}^{3} and a special Lagrangian fibration f:U→ℝ3f:U\rightarrow\mathbin{\mathbb{R}}^{3} satisfying Assumptions 7.1–7.1.

[03M7]

7.2 Justification for the conjecture

The author is unable to prove Conjecture 7.4 at present, but here are some reasons for believing it, amounting to a sketch of a partial proof. In §7.1 we started with the fibration f:U→ℝ3f:U\rightarrow\mathbin{\mathbb{R}}^{3}, and extracted the functions ua,b,va,bu_{a,b},v_{a,b} from it. However, any proof of Conjecture 7.4 will probably go the other way, and first construct functions ua,b,va,bu_{a,b},v_{a,b} satisfying (57), and then define the fibres Na,b,cN_{a,b,c} by (54), and put them together to form ff.

It is not obvious that if we did define families of functions ua,b,va,bu_{a,b},v_{a,b} satisfying (57), then the corresponding SL 3-folds Na,b,cN_{a,b,c} would actually be the fibres of a fibration. We will show that part (ii) of Assumption 7.1 comes close to ensuring that they do, because it implies that the Na,b,cN_{a,b,c} are disjoint.

[03M8]
Lemma 7.5

Suppose we are given functions ua,b,va,b:Va,b→ℝu_{a,b},v_{a,b}:V_{a,b}\rightarrow\mathbin{\mathbb{R}} for all a,b∈ℝa,b\in\mathbin{\mathbb{R}} satisfying part (ii) of Assumption 7.1. Define 33-folds Na,b,cN_{a,b,c} in UU for a,b,c∈ℝa,b,c\in\mathbin{\mathbb{R}} by (54). Then Na,b,c∩Na′,b′,c′=∅N_{a,b,c}\cap N_{a^{\prime},b^{\prime},c^{\prime}}=\emptyset unless (a,b,c)=(a′,b′,c′)(a,b,c)=(a^{\prime},b^{\prime},c^{\prime}).

[03M9]

Proof. Suppose (z1,z2,z3)(z_{1},z_{2},z_{3}) lies in Na,b,c∩Na′,b′,c′N_{a,b,c}\cap N_{a^{\prime},b^{\prime},c^{\prime}}. Then a=|z1|2−|z2|2=a′a=|z_{1}|^{2}-|z_{2}|^{2}=a^{\prime}, so a=a′a=a^{\prime}. Let x=Re(z3)x=\mathop{\rm Re}(z_{3}) and y=Im(z1​z2)y=\mathop{\rm Im}(z_{1}z_{2}). Then (54) gives

Re(z1​z2)=ua,b​(x,y)=ua′,b′​(x,y),Im(z3)=va,b​(x,y)+c=va′,b′​(x,y)+c′.\mathop{\rm Re}(z_{1}z_{2})=u_{a,b}(x,y)=u_{a^{\prime},b^{\prime}}(x,y),\quad\mathop{\rm Im}(z_{3})=v_{a,b}(x,y)+c=v_{a^{\prime},b^{\prime}}(x,y)+c^{\prime}.

As a=a′a=a^{\prime} the first equation gives ua,b​(x,y)=ua,b′​(x,y)u_{a,b}(x,y)=u_{a,b^{\prime}}(x,y), and part (ii) of Assumption 7.1 shows that b=b′b=b^{\prime}. The second equation then becomes va,b​(x,y)+c=va,b​(x,y)+c′v_{a,b}(x,y)+c=v_{a,b}(x,y)+c^{\prime}, so c=c′c=c^{\prime}. □\square

A 3-dimensional family of disjoint 3-folds in ℂ3\mathbin{\mathbb{C}}^{3} must locally define a fibration. So if we define UU to be the total space of all the Na,b,cN_{a,b,c} then we do have a fibration f:U→ℝ3f:U\rightarrow\mathbin{\mathbb{R}}^{3} with fibres Na,b,cN_{a,b,c}. Therefore, we have more-or-less reduced the problem to finding families of functions ua,b,va,bu_{a,b},v_{a,b}, which need only be defined near (0,0)(0,0) in ℝ2\mathbin{\mathbb{R}}^{2} for small a,ba,b, satisfying Assumption 7.1 and parts (i)–(vi) of Assumption 7.1.

Now by Proposition 6.4, given any real analytic values for ua,bu_{a,b} and va,bv_{a,b} on the xx-axis, there exist unique solutions of (57) near the xx-axis with these values, except when a=0a=0 near points (x,0)(x,0) with u0,b​(x,0)=0u_{0,b}(x,0)=0. But part (v) of Assumption 7.1 gives va,b​(x,0)≡0v_{a,b}(x,0)\equiv 0. Thus the function ua,b​(x,0)u_{a,b}(x,0) captures all the essential information about the behaviour of ua,bu_{a,b} and va,bv_{a,b} near the xx-axis.

Note also that part (ii) of Assumption 7.1 can be restricted to the xx-axis. For if ua,b​(x,0)<ua,b′​(x,0)u_{a,b}(x,0)<u_{a,b^{\prime}}(x,0) for all a,b,b′,xa,b,b^{\prime},x with b<b′b<b^{\prime}, then by continuity of the ua,bu_{a,b} we have ua,b​(x,y)<ua,b′​(x,y)u_{a,b}(x,y)<u_{a,b^{\prime}}(x,y) for sufficiently small yy. Thus part (ii) holds near the xx-axis, so by making UU smaller if necessary we ensure that part (ii) of Assumption 7.1 holds on all of Va,bV_{a,b}.

We may therefore try to proceed as follows. We choose real analytic functions ua,b​(x,0)u_{a,b}(x,0) satisfying the applicable parts of Assumptions 7.1 and 7.1, in a fairly arbitrary way. We then extend these uniquely to satisfy (57) in a small open neighbourhood of the xx-axis. Finally we construct the associated SL 3-folds, and argue that they locally form a fibration of ℂ3\mathbin{\mathbb{C}}^{3}.

The main problem with this approach is when a=0a=0 near the singular points (x,0)(x,0) with u0,b​(x,0)=0u_{0,b}(x,0)=0, as Proposition 6.4 does not apply. To overcome this problem we will need a good understanding of how solutions of (32) behave near isolated singular points of order 1 and 2. If we could prove Conjecture 6.14, then probably we could prove Conjecture 7.4 too.

[03MA]

7.3 Holomorphic discs with boundary in Na,b,cN_{a,b,c}

We now discuss the holomorphic discs with boundary in the nonsingular fibres Na,b,cN_{a,b,c}, and their relation with the singularities of the singular fibres. For generic a,b,ca,b,c we expect all holomorphic discs in ℂ3\mathbin{\mathbb{C}}^{3} with boundary in Na,b,cN_{a,b,c} to be U(1)\mathbin{\rm U}(1)-invariant, as the virtual dimension of the moduli space of such discs is zero. In the next proposition we identify all such holomorphic discs.

[03MB]
Proposition 7.6

In the notation above, suppose that a>0a>0 and b,c,x∈ℝb,c,x\in\mathbin{\mathbb{R}} with ua,b​(x,0)=0u_{a,b}(x,0)=0. Then

D={(z1,0,x+ic):z1∈ℂ,|z1|2⩽a}D=\bigl\{(z_{1},0,x+ic):z_{1}\in\mathbin{\mathbb{C}},\quad|z_{1}|^{2}\leqslant a\bigr\} (58)

is a holomorphic disc in ℂ3\mathbin{\mathbb{C}}^{3} with boundary in Na,b,cN_{a,b,c}, and

D′={(0,z2,x+ic):z2∈ℂ,|z2|2⩽a}D^{\prime}=\bigl\{(0,z_{2},x+ic):z_{2}\in\mathbin{\mathbb{C}},\quad|z_{2}|^{2}\leqslant a\bigr\} (59)

is a holomorphic disc in ℂ3\mathbin{\mathbb{C}}^{3} with boundary in N−a,b,cN_{-a,b,c}. Furthermore, all holomorphic discs in ℂ3\mathbin{\mathbb{C}}^{3} with boundary in N±a,b,cN_{\pm a,b,c} and invariant under the U(1)\mathbin{\rm U}(1)-action (52) are of this form.

[03MC]

Proof. Clearly DD is a holomorphic disc, and it is easy to show that its boundary lies in Na,b,cN_{a,b,c}. As ua,b=u−a,bu_{a,b}=u_{-a,b} by part (iv) of Assumption 7.1, it follows in a similar way that D′D^{\prime} is a holomorphic disc with boundary in N−a,b,cN_{-a,b,c}.

Now let D^\hat{D} be a U(1)\mathbin{\rm U}(1)-invariant holomorphic disc in ℂ3\mathbin{\mathbb{C}}^{3} with boundary in Na,b,cN_{a,b,c}, and let (z1,z2,z3)∈D^(z_{1},z_{2},z_{3})\in\hat{D}. We claim that z1=0z_{1}=0 or z2=0z_{2}=0. Suppose z1,z2≠0z_{1},z_{2}\neq 0. As DD contains the U(1)\mathbin{\rm U}(1)-orbit of (z1,z2,z3)(z_{1},z_{2},z_{3}) and is holomorphic, it must locally contain the orbit of (z1,z2,z3)(z_{1},z_{2},z_{3}) under the complexification of the U(1)\mathbin{\rm U}(1)-action (52). Therefore, DD must locally be a subset of

{(uz1,u−1z2,z3):u∈ℂ∖{0}}.\bigl\{(uz_{1},u^{-1}z_{2},z_{3}):u\in\mathbin{\mathbb{C}}\setminus\{0\}\bigr\}.

But there are no U(1)\mathbin{\rm U}(1)-invariant holomorphic discs in this set; the best one can do is an annulus. Thus one of z1,z2z_{1},z_{2} must be zero.

Let (z1,z2,z3)(z_{1},z_{2},z_{3}) be a point in the boundary of D^\hat{D}. Then (z1,z2,z3)∈Na,b,c(z_{1},z_{2},z_{3})\in N_{a,b,c}, so |z1|2−|z2|2=a>0|z_{1}|^{2}-|z_{2}|^{2}=a>0. This implies that z1≠0z_{1}\neq 0, so z2=0z_{2}=0. It is then easy to show that D^\hat{D} must be {(z,0,z3):|z|2⩽a}\bigl\{(z,0,z_{3}):|z|^{2}\leqslant a\bigr\}. This agrees with (58) with x=Re(z3)x=\mathop{\rm Re}(z_{3}) and c=Im(z3)c=\mathop{\rm Im}(z_{3}), and (z1,0,z3)∈Na,b,c(z_{1},0,z_{3})\in N_{a,b,c} implies that ua,b​(x,0)=0u_{a,b}(x,0)=0. So all U(1)\mathbin{\rm U}(1)-invariant holomorphic discs D^\hat{D} with boundary in Na,b,cN_{a,b,c} are as in the proposition. For N−a,b,cN_{-a,b,c} the argument works in the same way. □\square

Now Assumption 7.1 determines all the zeros of the functions ua,b​(x,0)u_{a,b}(x,0) exactly. When b>0b>0, there are two zeros at x=±bx=\pm\sqrt{b}, when b=0b=0 there is one zero at x=0x=0, and when b<0b<0 there are no zeros at all. Therefore the proposition shows that for a≠0a\neq 0, when b>0b>0 there are two holomorphic discs with boundary in Na,b,cN_{a,b,c}, when b=0b=0 there is one, and when b<0b<0 there are none.

For generic (a,b,c)(a,b,c), these should be all the holomorphic discs with boundary in Na,b,cN_{a,b,c}. We think of the two holomorphic discs with boundary in Na,b,cN_{a,b,c} for b>0b>0 as having opposite sign. As bb decreases though zero, they come together and cancel out.

Such holomorphic discs are relevant to the singularities of special Lagrangian fibrations, for the following reason. Let DD be a holomorphic disc in a Calabi–Yau 3-fold XX, with boundary in a special Lagrangian 3-fold NN. Then the area of DD is ∫Dω=[ω]⋅[D]\int_{D}\omega=[\omega]\cdot[D], where [ω][\omega] is the relative de Rham cohomology class of ω\omega in H2(X,N;ℝ)H^{2}(X,N;\mathbin{\mathbb{R}}), and [D][D] the relative homology class of DD in H2(X,N;ℤ)H_{2}(X,N;\mathbin{\mathbb{Z}}).

Thus the area of DD depends only on its relative homology class, and homologous holomorphic discs have the same area. Clearly, the area of a holomorphic disc DD must be positive. So what happens when we deform NN so that the area [ω]⋅[D][\omega]\cdot[D] becomes zero? It turns out that usually DD shrinks to a point, and NN becomes singular. The singularity is the result of collapsing the boundary 𝒮1{\mathcal{S}}^{1} of DD in NN to a point, and thus is a T2T^{2}-cone.

This has three important consequences:

  • •

    The singularities induced by holomorphic discs shrinking to zero appear in codimension one in the base BB of an SL fibration f:X→Bf:X\rightarrow B, on the hyperplane where the area of the disc shrinks to zero.

  • •

    There may be several homologous holomorphic discs D1,…,DkD_{1},\ldots,D_{k} with boundary in a generic fibre NN. As the area of the discs shrinks to zero, NN will simultaneously develop kk singular points.

  • •

    We can guess what the singularity looks like for generic singular fibres. The author is developing (and hopes one day to publish) a theory of singularities of SL 3-folds and their deformations. It predicts that when a holomorphic disc shrinks to zero, in the generic case the singularity that develops is locally modelled on the (isomorphic) T2T^{2}-cones L0±L_{0}^{\pm} of (16).

These three ideas were part of the author’s motivation in constructing the fibrations described above.

[03MD]

8 A model of a ‘ribbon’ in the discriminant

We will now modify the picture of §7 to give it a more interesting global topology, and use it to explain some features of how special Lagrangian fibrations of Calabi–Yau 3-folds might work. In §7, when ff is defined on all of ℂ3\mathbin{\mathbb{C}}^{3} the nonsingular fibres had topology 𝒮1×ℝ2{\mathcal{S}}^{1}\times\mathbin{\mathbb{R}}^{2}. We shall modify this so that ff is defined on a subset of ℂ3/ℤ\mathbin{\mathbb{C}}^{3}/\mathbin{\mathbb{Z}}, and the nonsingular fibres have topology T2×[−π,π]T^{2}\times[-\pi,\pi].

By identifying the two copies of T2T^{2} in the boundary of each fibre, we make a fibration over ℝ3\mathbin{\mathbb{R}}^{3} with nonsingular fibres diffeomorphic to T3T^{3}. The discriminant locus in ℝ3\mathbin{\mathbb{R}}^{3} is a ‘ribbon’, the set {(0,b,c):b∈[−1,1]\bigl\{(0,b,c):b\in[-1,1], c∈ℝ}c\in\mathbin{\mathbb{R}}\bigr\}. We calculate the monodromy of the fibration about this ribbon. In §9 we will relate this to the Gross–Ruan picture of smooth special Lagrangian fibrations.

[03ME]

8.1 A variation on the fibration of §7.1

Consider a fibration ff satisfying the following analogues of Assumptions 7.1–7.1.

[03MF]

Assumption 8.1 Let ℤ\mathbin{\mathbb{Z}} act on ℂ3\mathbin{\mathbb{C}}^{3} by (z1,z2,z3)↦n(z1,z2,z3+2​π​n)(z_{1},z_{2},z_{3})\,{\mathrel{\mathop{\kern 0.0pt\mapsto}\limits^{n}}}\,(z_{1},z_{2},z_{3}+2\pi n) for n∈ℤn\in\mathbin{\mathbb{Z}}. Define U={(z1,z2,z3+2πℤ)∈ℂ3/ℤ:Im(z1z2)∈[−π,π]}U=\bigl\{(z_{1},z_{2},z_{3}\!+\!2\pi\mathbin{\mathbb{Z}})\in\mathbin{\mathbb{C}}^{3}/\mathbin{\mathbb{Z}}:\mathop{\rm Im}(z_{1}z_{2})\in[-\pi,\pi]\bigr\}. Consider a special Lagrangian fibration f:U→ℝ3f:U\rightarrow\mathbin{\mathbb{R}}^{3}, with fibres Na,b,c=f−1​(a,b,c)N_{a,b,c}=f^{-1}(a,b,c). Suppose that ff satisfies parts (i)–(viii) of Assumption 7.1.

[03MG]

Assumption 8.2 Suppose that each fibre Na,b,cN_{a,b,c} of ff may be written

Na,b,c={(\displaystyle N_{a,b,c}=\Bigl\{( z1,z2,z3+2πℤ)∈U:Re(z1z2)=ua,b(Re(z3)+2πℤ,Im(z1z2)),\displaystyle z_{1},z_{2},z_{3}+2\pi\mathbin{\mathbb{Z}})\in U:\mathop{\rm Re}(z_{1}z_{2})=u_{a,b}\bigl(\mathop{\rm Re}(z_{3})+2\pi\mathbin{\mathbb{Z}},\mathop{\rm Im}(z_{1}z_{2})\bigr),
Im(z3)=va,b(Re(z3)+2πℤ,Im(z1z2))+c,|z1|2−|z2|2=a},\displaystyle\mathop{\rm Im}(z_{3})=v_{a,b}\bigl(\mathop{\rm Re}(z_{3})+2\pi\mathbin{\mathbb{Z}},\mathop{\rm Im}(z_{1}z_{2})\bigr)+c,\;\>|z_{1}|^{2}-|z_{2}|^{2}=a\Bigr\},

where ua,b,va,bu_{a,b},v_{a,b} are functions (ℝ/2πℤ)×[−π,π]→ℝ(\mathbin{\mathbb{R}}/2\pi\mathbin{\mathbb{Z}})\times[-\pi,\pi]\rightarrow\mathbin{\mathbb{R}}. Suppose also that ua,bu_{a,b} and va,bv_{a,b} satisfy parts (i)–(vi) of Assumption 7.1.

[03MH]

Assumption 8.3 In the situation above, the functions ua,bu_{a,b} and va,bv_{a,b} satisfy

  • (i)

    For all a,ba,b, the function ua,b(x+2πℤ,0)u_{a,b}(x+2\pi\mathbin{\mathbb{Z}},0) is strictly increasing for xx in (−π,0)(-\pi,0) and strictly decreasing for xx in (0,π)(0,\pi), with a maximum at 2πℤ2\pi\mathbin{\mathbb{Z}} and a minimum at π+2πℤ\pi+2\pi\mathbin{\mathbb{Z}}.

  • (ii)

    For all a,b,b′,x,ya,b,b^{\prime},x,y with b<b′b<b^{\prime} we have ua,b(x+2πℤ,y)<ua,b′(x+2πℤ,y)u_{a,b}(x+2\pi\mathbin{\mathbb{Z}},y)<u_{a,b^{\prime}}(x+2\pi\mathbin{\mathbb{Z}},y).

  • (iii)

    For all a,b,x∈ℝa,b,x\in\mathbin{\mathbb{R}} we have ua,b(x+2πℤ,0)=0u_{a,b}(x+2\pi\mathbin{\mathbb{Z}},0)=0 if and only if b+cos⁡x=0b+\cos x=0.

  • (iv)

    Let b∈(−1,1)b\in(-1,1), and write b=cos⁡βb=\cos\beta for β∈(0,π)\beta\in(0,\pi). Then the solution u0,b,v0,bu_{0,b},v_{0,b} of (32) has isolated singularities of order 1 at (±β+2πℤ,0)(\pm\beta+2\pi\mathbin{\mathbb{Z}},0), in the sense of Definition 6.4.

    Near (−β+2πℤ,0)(-\beta+2\pi\mathbin{\mathbb{Z}},0) for small aa, the functions ua,b,va,bu_{a,b},v_{a,b} are approximately equal to the functions u,vu,v constructed from Na,−βN_{a,-\beta} in Proposition 6.7.

    Near (β+2πℤ,0)(\beta+2\pi\mathbin{\mathbb{Z}},0) for small aa, the functions ua,b,va,bu_{a,b},v_{a,b} are approximately equal to the functions u,vu,v constructed from Na,β′N^{\prime}_{a,\beta} in Proposition 6.8.

  • (v)

    The solution u0,−1,v0,−1u_{0,-1},v_{0,-1} of (32) has an isolated singularity of order 2 at (2πℤ,0)(2\pi\mathbin{\mathbb{Z}},0), and the solution u0,1,v0,1u_{0,1},v_{0,1} has an isolated singularity of order 2 at (π+2πℤ,0)(\pi+2\pi\mathbin{\mathbb{Z}},0), in the sense of Definition 6.4.

  • (vi)

    For all a,b,x,y∈ℝa,b,x,y\in\mathbin{\mathbb{R}} we have ua,−b(x+2πℤ,y)=−ua,b(x+π+2πℤ,y)u_{a,-b}(x+2\pi\mathbin{\mathbb{Z}},y)=-u_{a,b}(x+\pi+2\pi\mathbin{\mathbb{Z}},y) and va,−b(x+2πℤ,y)=−va,b(x+π+2πℤ,y)v_{a,-b}(x+2\pi\mathbin{\mathbb{Z}},y)=-v_{a,b}(x+\pi+2\pi\mathbin{\mathbb{Z}},y).

These assumptions are a kind of toy model, designed to illustrate some aspects of how the fibrations of §5 and §7 might fit together in a Calabi–Yau 3-fold, and to perform a topological calculation. We are not making the conjecture that a fibration actually exists satisfying these assumptions.

u0,b​(x,0)\textstyle{u_{0,b}(x,0)}x\textstyle{x} 0\textstyle{\,\scriptstyle 0}+\textstyle{\scriptstyle+}π3\textstyle{\scriptstyle\frac{\pi}{3}}+\textstyle{\scriptstyle+}π2\textstyle{\scriptstyle\frac{\pi}{2}}+\textstyle{\scriptstyle+}2​π3\textstyle{\scriptstyle\frac{2\pi}{3}}+\textstyle{\scriptstyle+}π\textstyle{\scriptstyle\pi}+\textstyle{\scriptstyle+}−π3\textstyle{\scriptstyle-\frac{\pi}{3}}+\textstyle{\scriptstyle+}−π2\textstyle{\scriptstyle-\frac{\pi}{2}}+\textstyle{\scriptstyle+}−2​π3\textstyle{\scriptstyle-\frac{2\pi}{3}}+\textstyle{\scriptstyle+}−π\textstyle{\scriptstyle-\pi}b=−32\textstyle{\,\,b=-\frac{3}{2}}b=−1\textstyle{\,\,b=-1}b=−12\textstyle{\,\,b=-\frac{1}{2}}b=0\textstyle{\,\,b=0}b=12\textstyle{\,\,b=\frac{1}{2}}b=1\textstyle{\,\,b=1}b=32\textstyle{\,\,b=\frac{3}{2}}

Figure 3: approximate curves u0,b​(x,0)u_{0,b}(x,0) for different bb

In Figure 3 we sketch the functions u0,b​(x,0)u_{0,b}(x,0) for several values of bb, on the same graph, to display the general features we expect of these functions. The basic idea is that u0,b​(x,0)u_{0,b}(x,0) should look a bit like b+cos⁡xb+\cos x, in that it has the same periodic behaviour, is zero at the same points, and is increasing and decreasing in the same regions. But at its zeros u0,b​(x,0)u_{0,b}(x,0) has gradient zero, whereas b+cos⁡xb+\cos x generally does not.

Let us describe the fibres Na,b,cN_{a,b,c} of ff. From §6, Na,b,cN_{a,b,c} is singular if and only if a=0a=0 and u0,b​(x,0)=0u_{0,b}(x,0)=0 for some xx. But part (iii) of Assumption 8.1 shows that u0,b(x+2πℤ,0)=0u_{0,b}(x+2\pi\mathbin{\mathbb{Z}},0)=0 if and only if cos⁡x=−b\cos x=-b. This has solutions when b∈[−1,1]b\in[-1,1]. Therefore Na,b,cN_{a,b,c} is singular if and only if a=0a=0 and b∈[−1,1]b\in[-1,1].

It is easy to show that the nonsingular fibres of ff are all diffeomorphic to T2×[−π,π]T^{2}\times[-\pi,\pi]. The singular fibres N0,b,cN_{0,b,c} for b∈(−1,1)b\in(-1,1) are diffeomorphic to T2×[−π,π]T^{2}\times[-\pi,\pi] with two homologous circles collapsed to two points, and the singular fibres N0,±1,cN_{0,\pm 1,c} are diffeomorphic to T2×[−π,π]T^{2}\times[-\pi,\pi] with one circle collapsed to a point.

[03MI]

8.2 Monodromy around a ‘ribbon’

The discriminant Δf\Delta_{f} of ff is the set of (a,b,c)∈ℝ3(a,b,c)\in\mathbin{\mathbb{R}}^{3} such that f−1​(a,b,c)f^{-1}(a,b,c) is singular. From above we see that

Δf={(0,b,c):b∈[−1,1],c∈ℝ}.\Delta_{f}=\bigl\{(0,b,c):b\in[-1,1],\quad c\in\mathbin{\mathbb{R}}\bigr\}. (60)

We can think of Δf\Delta_{f} as a ‘ribbon’ in ℝ3\mathbin{\mathbb{R}}^{3}. To understand the topology of a fibration f:X→Bf:X\rightarrow B with singularities, it is often helpful to calculate the monodromy around nontrivial loops in B∖ΔfB\setminus\Delta_{f}, as in Ruan [18, §4] or Gross [7, §1], for instance.

In our case, π1(ℝ3∖Δf)\pi_{1}\bigl(\mathbin{\mathbb{R}}^{3}\setminus\Delta_{f}\bigr) is isomorphic to ℤ\mathbin{\mathbb{Z}}, and generated by the circle γ:𝒮1→ℝ3∖Δf\gamma:{\mathcal{S}}^{1}\rightarrow\mathbin{\mathbb{R}}^{3}\setminus\Delta_{f} given by γ⁡(ei​θ)=(2​cos⁡θ,2​sin⁡θ,0)\gamma({\rm e}^{i\theta})=(2\cos\theta,2\sin\theta,0). So we would like to understand the monodromy around γ\gamma. It turns out that the monodromy action on the homology H1(T2×[−π,π];ℤ)≅ℤ2H_{1}\bigl(T^{2}\times[-\pi,\pi];\mathbin{\mathbb{Z}}\bigr)\cong\mathbin{\mathbb{Z}}^{2} is trivial.

This is because the topologically interesting transformations happen in the [−π,π][-\pi,\pi] directions, which H1​(T2×[−π,π],ℤ)H_{1}\bigl(T^{2}\times[-\pi,\pi];\mathbin{\mathbb{Z}}\bigr) does not detect. To get round this we will identify the two boundary components T2×{π}T^{2}\times\{\pi\} and T2×{−π}T^{2}\times\{-\pi\} of each fibre Na,b,cN_{a,b,c}, so that the nonsingular fibres become 3-tori T3T^{3}, and then evaluate the monodromy around γ\gamma on H1​(T3,ℤ)H_{1}(T^{3};\mathbin{\mathbb{Z}}), which is nontrivial.

Let Na,b,cN_{a,b,c} be a fibre of ff. We need a way to identify the two components of ∂Na,b,c\partial N_{a,b,c}. Here is one way to do it. Let 𝐳=(z1,z2,z3+2πℤ){\bf z}=(z_{1},z_{2},z_{3}+2\pi\mathbin{\mathbb{Z}}) and 𝐳′=(z1′,z2′,z3′+2πℤ){\bf z}^{\prime}=(z_{1}^{\prime},z_{2}^{\prime},z_{3}^{\prime}+2\pi\mathbin{\mathbb{Z}}) lie in Na,b,cN_{a,b,c} with Im(z1​z2)=π\mathop{\rm Im}(z_{1}z_{2})=\pi and Im(z1′​z2′)=−π\mathop{\rm Im}(z_{1}^{\prime}z_{2}^{\prime})=-\pi, so that 𝐳{\bf z} and 𝐳′{\bf z}^{\prime} lie in different boundary components. We identify 𝐳\bf z and 𝐳′{\bf z}^{\prime} if

Re(z3)+2πℤ=Re(z3′)+2πℤandarg(z1)+2πℤ=arg(z1′)+2πℤ,\mathop{\rm Re}(z_{3})+2\pi\mathbin{\mathbb{Z}}=\mathop{\rm Re}(z_{3}^{\prime})+2\pi\mathbin{\mathbb{Z}}\quad\text{and}\quad\arg(z_{1})+2\pi\mathbin{\mathbb{Z}}=\arg(z_{1}^{\prime})+2\pi\mathbin{\mathbb{Z}}, (61)

where arg⁡(r​ei​θ)=θ\arg(r{\rm e}^{i\theta})=\theta for r>0r>0 and θ∈[0,2​π)\theta\in[0,2\pi) is the argument of a nonzero complex number. As Im(z1​z2)=π\mathop{\rm Im}(z_{1}z_{2})=\pi and Im(z1′​z2′)=−π\mathop{\rm Im}(z_{1}^{\prime}z_{2}^{\prime})=-\pi both z1z_{1} and z1′z_{1}^{\prime} are nonzero, and so arg⁡(z1)\arg(z_{1}) and arg⁡(z1′)\arg(z_{1}^{\prime}) are well-defined.

Let N~a,b,c\tilde{N}_{a,b,c} be Na,b,cN_{a,b,c} with its boundary components identified as above. It is easy to show that (61) defines a diffeomorphism between the two components of ∂Na,b,c\partial N_{a,b,c}, and that N~a,b,c\tilde{N}_{a,b,c} is a copy of T3T^{3} when Na,b,cN_{a,b,c} is nonsingular.

To calculate the monodromy we will cover ℝ3∖Δf\mathbin{\mathbb{R}}^{3}\setminus\Delta_{f} by two closed sets U±U^{\pm}, and define a trivialization of ff over each set. Let

U+={(a,b,c)∈ℝ3:a⩾0, and b∉[−1,1] if a=0}.U^{+}=\bigl\{(a,b,c)\in\mathbin{\mathbb{R}}^{3}:\text{$a\geqslant 0$, and $b\notin[-1,1]$ if $a=0$}\bigr\}. (62)

For each (a,b,c)∈U+(a,b,c)\in U^{+}, define Φa,b,c+:N~a,b,c→(ℝ/2πℤ)3\Phi^{+}_{a,b,c}:\tilde{N}_{a,b,c}\rightarrow(\mathbin{\mathbb{R}}/2\pi\mathbin{\mathbb{Z}})^{3} by

Φ+a,b,c:(z1,z2,z3+2πℤ)↦(arg(z1)+2πℤ,Re(z3)+2πℤ,Im(z1z2)+2πℤ).\begin{split}&\Phi^{+}_{a,b,c}:(z_{1},z_{2},z_{3}+2\pi\mathbin{\mathbb{Z}})\mapsto\\ &\bigl(\arg(z_{1})+2\pi\mathbin{\mathbb{Z}},\mathop{\rm Re}(z_{3})+2\pi\mathbin{\mathbb{Z}},\mathop{\rm Im}(z_{1}z_{2})+2\pi\mathbin{\mathbb{Z}}\bigr).\end{split} (63)

There are two issues involved in proving Φa,b,c+\Phi_{a,b,c}^{+} is well-defined. Firstly, we must show that z1≠0z_{1}\neq 0 in N~a,b,c\tilde{N}_{a,b,c}, so that arg⁡(z1)\arg(z_{1}) exists. This is true because z1z_{1} and z2z_{2} cannot both be zero, as then (z1,z2,z3+2πℤ)(z_{1},z_{2},z_{3}+2\pi\mathbin{\mathbb{Z}}) would be a singular point, contradicting (a,b,c)∉Δf(a,b,c)\notin\Delta_{f}. But |z1|2−|z2|2=a⩾0|z_{1}|^{2}-|z_{2}|^{2}=a\geqslant 0, so that if z1=0z_{1}=0 then z2=0z_{2}=0. Thus z1≠0z_{1}\neq 0 in N~a,b,c\tilde{N}_{a,b,c}. The second issue is that points identified in Na,b,cN_{a,b,c} must have the same image under Φa,b,c+\Phi_{a,b,c}^{+}. This follows from (61).

The other closed set in ℝ3∖Δf\mathbin{\mathbb{R}}^{3}\setminus\Delta_{f} is

U−={(a,b,c)∈ℝ3:a⩽0, and b∉[−1,1] if a=0}.U^{-}=\bigl\{(a,b,c)\in\mathbin{\mathbb{R}}^{3}:\text{$a\leqslant 0$, and $b\notin[-1,1]$ if $a=0$}\bigr\}. (64)

We cannot use (63) to trivialize ff over this set, because z1z_{1} will become zero in some Na,b,cN_{a,b,c}, and so arg⁡(z1)\arg(z_{1}) may not be well-defined. Instead we must do something more complicated.

Let η:[−π,π]→[0,1]\eta:[-\pi,\pi]\rightarrow[0,1] be smooth with η⁡(y)=0\eta(y)=0 for |y|⩽1|y|\leqslant 1 and η⁡(y)=1\eta(y)=1 for |y|⩾2|y|\geqslant 2. For each (a,b,c)∈U−(a,b,c)\in U^{-}, define Φa,b,c−:N~a,b,c→(ℝ/2πℤ)3\Phi^{-}_{a,b,c}:\tilde{N}_{a,b,c}\rightarrow(\mathbin{\mathbb{R}}/2\pi\mathbin{\mathbb{Z}})^{3} by

Φa,b,c−:(z1CLOSE,z2,z3+2πℤ)↦(η(Im(z1z2))arg(z1z2)−arg(z2)+2πℤ,Re(z3)+2πℤ,Im(z1z2)+2πℤ).\begin{split}\Phi^{-}_{a,b,c}:(z_{1}&,z_{2},z_{3}+2\pi\mathbin{\mathbb{Z}})\mapsto\bigl(\eta\bigl(\mathop{\rm Im}(z_{1}z_{2})\bigr)\arg(z_{1}z_{2})\\ &-\arg(z_{2})+2\pi\mathbin{\mathbb{Z}},\mathop{\rm Re}(z_{3})+2\pi\mathbin{\mathbb{Z}},\mathop{\rm Im}(z_{1}z_{2})+2\pi\mathbin{\mathbb{Z}}\bigr).\end{split} (65)

Here for a<0a<0 we may have z1​z2=0z_{1}z_{2}=0 at some points in N~a,b,c\tilde{N}_{a,b,c}, so that arg⁡(z1​z2)\arg(z_{1}z_{2}) is undefined. But then η⁡(Im(z1​z2))=0\eta\bigl(\mathop{\rm Im}(z_{1}z_{2})\bigr)=0, so we take this term to be zero.

Also, arg⁡(z1​z2)\arg(z_{1}z_{2}) changes discontinuously when z1​z2z_{1}z_{2} is real and positive, but the η\eta term is zero here, so that Φa,b,c−\Phi^{-}_{a,b,c} is continuous. The term arg⁡(z2)\arg(z_{2}) in (65) always exists by the argument above. When |Im(z1​z2)|⩾2|\mathop{\rm Im}(z_{1}z_{2})|\geqslant 2 we have

η(Im(z1z2))arg(z1z2)−arg(z2)+2πℤ=arg(z1)+2πℤ,\eta\bigl(\mathop{\rm Im}(z_{1}z_{2})\bigr)\arg(z_{1}z_{2})-\arg(z_{2})+2\pi\mathbin{\mathbb{Z}}=\arg(z_{1})+2\pi\mathbin{\mathbb{Z}},

so that (65) agrees with (63). Therefore points identified in Na,b,cN_{a,b,c} have the same image under Φa,b,c−\Phi_{a,b,c}^{-}, as above. So Φa,b,c−\Phi^{-}_{a,b,c} is well-defined.

Now we can calculate the monodromy around γ\gamma. Starting at ei​θ=1{\rm e}^{i\theta}=1, and going round γ\gamma once in the positive direction, we first cross over from U+U^{+} to U−U^{-} at ei​θ=i{\rm e}^{i\theta}=i. The transition map between trivializations is Φ0,2,0−∘(Φ0,2,0+)−1\Phi^{-}_{0,2,0}\circ(\Phi^{+}_{0,2,0})^{-1}. Then we cross from U−U^{-} back to U+U^{+} at ei​θ=−i{\rm e}^{i\theta}=-i, with transition map Φ0,−2,0+∘(Φ0,−2,0−)−1\Phi^{+}_{0,-2,0}\circ(\Phi^{-}_{0,-2,0})^{-1}. So the overall monodromy transformation round γ\gamma is

Φ0,−2,0+∘(Φ0,−2,0−)−1∘Φ0,2,0−∘(Φ0,2,0+)−1.\Phi^{+}_{0,-2,0}\circ(\Phi^{-}_{0,-2,0})^{-1}\circ\Phi^{-}_{0,2,0}\circ(\Phi^{+}_{0,2,0})^{-1}. (66)

Let (z1,z2,z3+2πℤ)∈N0,2,0(z_{1},z_{2},z_{3}+2\pi\mathbin{\mathbb{Z}})\in N_{0,2,0} and write

Φ0,2,0+(z1,z2,z3+2πℤ)\displaystyle\Phi^{+}_{0,2,0}(z_{1},z_{2},z_{3}+2\pi\mathbin{\mathbb{Z}}) =(θ++2πℤ,x+2πℤ,y+2πℤ)\displaystyle=(\theta^{+}+2\pi\mathbin{\mathbb{Z}},x+2\pi\mathbin{\mathbb{Z}},y+2\pi\mathbin{\mathbb{Z}})
andΦ0,2,0−(z1,z2,z3+2πℤ)\displaystyle\text{and}\quad\Phi^{-}_{0,2,0}(z_{1},z_{2},z_{3}+2\pi\mathbin{\mathbb{Z}}) =(θ−+2πℤ,x+2πℤ,y+2πℤ).\displaystyle=(\theta^{-}+2\pi\mathbin{\mathbb{Z}},x+2\pi\mathbin{\mathbb{Z}},y+2\pi\mathbin{\mathbb{Z}}).

Then θ+=arg⁡(z1)\theta^{+}=\arg(z_{1}) and θ−=η⁡(Im(z1​z2))​arg⁡(z1​z2)−arg⁡(z2)\theta^{-}=\eta\bigl(\mathop{\rm Im}(z_{1}z_{2})\bigr)\arg(z_{1}z_{2})-\arg(z_{2}) by (63) and (65), so that

θ+−θ−=(1−η⁡(Im(z1​z2)))​arg⁡(z1​z2)=(1−η⁡(y))​arg⁡(u0,2​(x,y)+i​y).\theta^{+}-\theta^{-}=\bigl(1-\eta\bigl(\mathop{\rm Im}(z_{1}z_{2})\bigr)\bigr)\arg(z_{1}z_{2})=\bigl(1-\eta(y)\bigr)\arg\bigl(u_{0,2}(x,y)+iy\bigr).

But u0,2​(x,0)>0u_{0,2}(x,0)>0 for all xx by Assumption 8.1. It follows that

arg⁡(u0,2​(x,y)+i​y)={0,y=0,cot−1⁡(y−1​u0,2​(x,y)),y>0,π+cot−1⁡(y−1​u0,2​(x,y)),y<0,\arg\bigl(u_{0,2}(x,y)+iy\bigr)=\begin{cases}0,&y=0,\\ \cot^{-1}\bigl(y^{-1}u_{0,2}(x,y)\bigr),&y>0,\\ \pi+\cot^{-1}\bigl(y^{-1}u_{0,2}(x,y)\bigr),&y<0,\\ \end{cases}

as arg\arg maps into [0,2​π)[0,2\pi), where cot−1\cot^{-1} maps ℝ→(0,π)\mathbin{\mathbb{R}}\rightarrow(0,\pi). Combining the last four equations gives

Φ0,2,0+∘(Φ0,2,0−)−1:(θ+2πℤ,x+2πℤ,y+2πℤ)↦\displaystyle\Phi^{+}_{0,2,0}\circ(\Phi^{-}_{0,2,0})^{-1}:(\theta+2\pi\mathbin{\mathbb{Z}},x+2\pi\mathbin{\mathbb{Z}},y+2\pi\mathbin{\mathbb{Z}})\mapsto
{(θ+2πℤ,x+2πℤ,2πℤ),y=0,(θ+(1−η(y))cot−1(y−1u0,2(x,y))+2πℤ,x+2πℤ,y+2πℤ),y>0,(θ+(1−η(y))(π+cot−1(y−1u0,2(x,y)))+2πℤ,x+2πℤ,y+2πℤ),y<0.\displaystyle\begin{cases}\bigl(\theta+2\pi\mathbin{\mathbb{Z}},x+2\pi\mathbin{\mathbb{Z}},2\pi\mathbin{\mathbb{Z}}\bigr),&y=0,\\ \bigl(\theta+(1-\eta(y))\cot^{-1}(y^{-1}u_{0,2}(x,y))+2\pi\mathbin{\mathbb{Z}},x+2\pi\mathbin{\mathbb{Z}},y+2\pi\mathbin{\mathbb{Z}}\bigr),&y>0,\\ \bigl(\theta+(1-\eta(y))\bigl(\pi\!+\!\cot^{-1}(y^{-1}u_{0,2}(x,y))\bigr)\!+\!2\pi\mathbin{\mathbb{Z}},x\!+\!2\pi\mathbin{\mathbb{Z}},y\!+\!2\pi\mathbin{\mathbb{Z}}\bigr),&y<0.\end{cases}

Similarly we find that

arg⁡(u0,−2​(x,y)+i​y)={π,y=0,cot−1⁡(y−1​u0,−2​(x,y)),y>0,π+cot−1⁡(y−1​u0,−2​(x,y)),y<0,\arg\bigl(u_{0,-2}(x,y)+iy\bigr)=\begin{cases}\pi,&y=0,\\ \cot^{-1}\bigl(y^{-1}u_{0,-2}(x,y)\bigr),&y>0,\\ \pi+\cot^{-1}\bigl(y^{-1}u_{0,-2}(x,y)\bigr),&y<0,\\ \end{cases}

as u0,−2​(x,0)<0u_{0,-2}(x,0)<0 for all xx, so that

Φ0,−2,0−∘(Φ0,−2,0+)−1:(θ+2πℤ,x+2πℤ,y+2πℤ)↦\displaystyle\Phi^{-}_{0,-2,0}\circ(\Phi^{+}_{0,-2,0})^{-1}:(\theta+2\pi\mathbin{\mathbb{Z}},x+2\pi\mathbin{\mathbb{Z}},y+2\pi\mathbin{\mathbb{Z}})\mapsto
{(θ+π+2πℤ,x+2πℤ,2πℤ),y=0,(θ+(1−η(y))cot−1(y−1u0,−2(x,y))+2πℤ,x+2πℤ,y+2πℤ),y>0,(θ+(1−η(y))(π+cot−1(y−1u0,−2(x,y)))+2πℤ,x+2πℤ,y+2πℤ),y<0.\displaystyle\begin{cases}\bigl(\theta+\pi+2\pi\mathbin{\mathbb{Z}},x+2\pi\mathbin{\mathbb{Z}},2\pi\mathbin{\mathbb{Z}}\bigr),&y=0,\\ \bigl(\theta+(1-\eta(y))\cot^{-1}(y^{-1}u_{0,-2}(x,y))+2\pi\mathbin{\mathbb{Z}},x+2\pi\mathbin{\mathbb{Z}},y+2\pi\mathbin{\mathbb{Z}}\bigr),&y>0,\\ \bigl(\theta+(1-\eta(y))\bigl(\pi\!+\!\cot^{-1}(y^{-1}u_{0,-2}(x,y))\bigr)\!+\!2\pi\mathbin{\mathbb{Z}},x\!+\!2\pi\mathbin{\mathbb{Z}},y\!+\!2\pi\mathbin{\mathbb{Z}}\bigr),&y<0.\end{cases}

From (66) and the equations above we see that the monodromy is

(θ+CLOSE\displaystyle(\theta+ 2πℤ,x+2πℤ,y+2πℤ)↦\displaystyle 2\pi\mathbin{\mathbb{Z}},x+2\pi\mathbin{\mathbb{Z}},y+2\pi\mathbin{\mathbb{Z}})\mapsto
{(θ+(1−η(y))π+2πℤ,x+2πℤ,y+2πℤ),y=0,(θ+(1−η⁡(y))​(cot−1⁡(y−1​u0,2​(x,y))CLOSECLOSE−cot−1(y−1u0,−2(x,y)))+2πℤ,x+2πℤ,y+2πℤ),y≠0.\displaystyle\begin{cases}\bigl(\theta+(1-\eta(y))\pi+2\pi\mathbin{\mathbb{Z}},x+2\pi\mathbin{\mathbb{Z}},y+2\pi\mathbin{\mathbb{Z}}\bigr),&y=0,\\ \begin{gathered}\bigl(\theta+(1-\eta(y))\bigl(\cot^{-1}(y^{-1}u_{0,2}(x,y))\qquad\qquad\qquad\qquad\qquad\\ -\cot^{-1}(y^{-1}u_{0,-2}(x,y))\bigr)+2\pi\mathbin{\mathbb{Z}},x+2\pi\mathbin{\mathbb{Z}},y+2\pi\mathbin{\mathbb{Z}}\bigr),\end{gathered}&y\neq 0.\end{cases}

Note that although this is continuous as a map to (ℝ/2πℤ)3(\mathbin{\mathbb{R}}/2\pi\mathbin{\mathbb{Z}})^{3}, the expression

(1−η⁡(y))​(cot−1⁡(y−1​u0,2​(x,y))−cot−1⁡(y−1​u0,−2​(x,y)))\bigl(1-\eta(y)\bigr)\bigl(\cot^{-1}(y^{-1}u_{0,2}(x,y))-\cot^{-1}(y^{-1}u_{0,-2}(x,y))\bigr)

decreases discontinuously by −2​π-2\pi at y=0y=0, as u0,2​(x,0)>0u_{0,2}(x,0)>0 and u0,−2​(x,0)<0u_{0,-2}(x,0)<0 for all xx. It follows that the monodromy is homotopic to

(θ+2πℤ,x+2πℤ,y+2πℤ)↦(θ+y+2πℤ,x+2πℤ,y+2πℤ),(\theta+2\pi\mathbin{\mathbb{Z}},x+2\pi\mathbin{\mathbb{Z}},y+2\pi\mathbin{\mathbb{Z}})\mapsto(\theta+y+2\pi\mathbin{\mathbb{Z}},x+2\pi\mathbin{\mathbb{Z}},y+2\pi\mathbin{\mathbb{Z}}),

which is a transformation of T3T^{3} with monodromy

(101010001)\begin{pmatrix}1&0&1\\ 0&1&0\\ 0&0&1\end{pmatrix} (67)

with respect to the obvious basis of H1​(T3,ℤ)H_{1}(T^{3};\mathbin{\mathbb{Z}}).

Remark. In the above calculation we defined the fibres N~a,b,c\tilde{N}_{a,b,c} by identifying the two T2T^{2} boundary components of each Na,b,cN_{a,b,c}. This identification (61) works also for the singular fibres N0,b,cN_{0,b,c} for b∈[−1,1]b\in[-1,1], as they are not singular on their boundaries, and is continuous over the set of singular fibres.

This is important, and is what gives the calculation above topological meaning. If we had defined the fibres N~a,b,c\tilde{N}_{a,b,c} only for nonsingular Na,b,cN_{a,b,c}, without the requirement that the identification of boundary components should extend continuously over the singular fibres, then we would have had more topological freedom in choosing how to identify the boundaries of the nonsingular Na,b,cN_{a,b,c} to get N~a,b,c\tilde{N}_{a,b,c}, and the monodromy matrix would depend on this choice.

[03MJ]

9 Global behaviour of SL fibrations

We are now ready to state our picture (still conjectural and incomplete) of what special Lagrangian fibrations of generic almost Calabi–Yau 3-folds should look like, if indeed they exist. Rather than starting from scratch, we begin in §9.1 by reviewing the rather elegant picture of smooth special Lagrangian fibrations f:X→Bf:X\rightarrow B, which has been built up largely by Mark Gross and Wei-Dong Ruan. Then in §9.2 we explain how to modify the Gross–Ruan picture under a small generic deformation of XX. Finally, in §9.3 we draw some conclusions about the SYZ Conjecture.

[03MK]

9.1 The Gross–Ruan picture of smooth SL fibrations

Here is a review of the expected properties of smooth special Lagrangian fibrations of Calabi–Yau 3-folds. Our principal sources are Gross [6, §3] and Ruan [19, §7] for the topology of the singular fibres, and Gross [7, §1] and Ruan [20, §9] for the monodromy matrices. A concise statement may be found in the ‘Precise SYZ mirror conjecture’ of Ruan [20, §9].

Let f:X→𝒮3f:X\rightarrow{\mathcal{S}}^{3} be a smooth special Lagrangian fibration, with fibres Nb=f−1​(b)N_{b}=f^{-1}(b), and generic fibre T3T^{3}. For generic such fibrations, the discriminant Δf\Delta_{f} is thought to be a trivalent graph, made up of smooth edges, and vertices of two kinds, which we shall refer to as positive and negative. The topology and local monodromy for each kind of singular fibre are as follows.

  • (a)

    Let γ\gamma be an edge in Δf\Delta_{f}, and b∈γb\in\gamma. Then NbN_{b} has the topology of T3T^{3} with T2T^{2} collapsed to an 𝒮1{\mathcal{S}}^{1}, and may be written Σ×𝒮1\Sigma\times{\mathcal{S}}^{1}, where Σ\Sigma is a T2T^{2} with an 𝒮1{\mathcal{S}}^{1} collapsed to a point, or equivalently an 𝒮2{\mathcal{S}}^{2} with two points identified. These fibres are called type (2,2)(2,2) by Gross and type II by Ruan. They have Euler characteristic zero.

    The monodromy about each edge γ\gamma in Δf\Delta_{f}, acting on H1(T3;ℤ)≅ℤ3H_{1}(T^{3};\mathbin{\mathbb{Z}})\cong\mathbin{\mathbb{Z}}^{3}, is

    (110010001)\begin{pmatrix}1&1&0\\ 0&1&0\\ 0&0&1\end{pmatrix} (68)

    with respect to a suitable basis of H1​(T3,ℤ)H_{1}(T^{3};\mathbin{\mathbb{Z}}).

  • (b)

    Let bb be a positive vertex in Δf\Delta_{f}. Then NbN_{b} has the topology of T3T^{3} with T2T^{2} collapsed to a point. It has Euler characteristic 1. These fibres are called type (1,2)(1,2) by Gross and type I​I​IIII by Ruan.

    The monodromies around the three edges γ1,γ2,γ3\gamma_{1},\gamma_{2},\gamma_{3} meeting at bb are

    (100110001),(100010−101)and(100−110101)\begin{pmatrix}1&0&0\\ 1&1&0\\ 0&0&1\end{pmatrix},\quad\begin{pmatrix}1&0&0\\ 0&1&0\\ -1&0&1\end{pmatrix}\quad\text{and}\quad\begin{pmatrix}1&0&0\\ -1&1&0\\ 1&0&1\end{pmatrix} (69)

    with respect to a suitable basis of H1​(T3,ℤ)H_{1}(T^{3};\mathbin{\mathbb{Z}}).

    The smooth special Lagrangian fibration of Corollary 4.4 is a local model for the fibration ff near the singular point of a positive singular fibre.

  • (c)

    Let bb be a negative vertex in Δf\Delta_{f}. Then Ruan [19, §7] gives two different possible topologies for NbN_{b}, which he calls type I​III and type I​I~\tilde{II}. His type I​I~\tilde{II} topology agrees with Gross’ proposed type (2,1) fibre [6, §3].

    Both fibres are constructed by taking a fibration π:T3→T2\pi:T^{3}\rightarrow T^{2} with fibre 𝒮1{\mathcal{S}}^{1}, and collapsing the fibres to points over a graph Γ\Gamma in T2T^{2}. In the type I​III case Γ\Gamma has three edges and two vertices, and in the type I​I~\tilde{II} case it has two edges and one vertex. In both cases NbN_{b} has Euler characteristic −1-1.

    The monodromies around the three edges γ1,γ2,γ3\gamma_{1},\gamma_{2},\gamma_{3} meeting at bb are

    (110010001),(10−1010001)and(1−11010001),\begin{pmatrix}1&1&0\\ 0&1&0\\ 0&0&1\end{pmatrix},\quad\begin{pmatrix}1&0&-1\\ 0&1&0\\ 0&0&1\end{pmatrix}\quad\text{and}\quad\begin{pmatrix}1&-1&1\\ 0&1&0\\ 0&0&1\end{pmatrix}, (70)

    with respect to a suitable basis of H1​(T3,ℤ)H_{1}(T^{3};\mathbin{\mathbb{Z}}).

    At present, to the author’s knowledge, there is no known local model for a smooth special Lagrangian fibration (or even a smooth Lagrangian fibration) in the neighbourhood of a codimension three singular point of a negative singular fibre. It may be that no such local model exists. If this is the case then smooth special Lagrangian fibrations may not exist on general Calabi–Yau 3-folds, even with a very nongeneric choice of almost Calabi–Yau metric.

We will refer to the singular fibres over positive and negative vertices as positive and negative singular fibres respectively. Our notation of positive and negative vertices was suggested by David Morrison, and refers to the sign of the Euler characteristic of the singular fibres. Gross’ notation refers to the Betti numbers (b1,b2)(b^{1},b^{2}) of the singular fibres.

In the author’s view, none of the fibre topologies in parts (a)–(c) above can occur as special Lagrangian submanifolds in generic almost Calabi–Yau 3-folds. The fibres of parts (a) and (c) are singular along real curves, and so should be highly nongeneric by the argument given in §3.1. Here is an argument to show that a positive singular fibre, a T3T^{3} with T2T^{2} collapsed to a point, cannot occur as a special Lagrangian 3-fold in a generic almost Calabi–Yau 3-fold.

Let NN be a singular SL 3-fold in XX with the topology of T3T^{3} with T2T^{2} collapsed to a point. The suspension S⁡(T2)S(T^{2}) of T2T^{2} is defined to be T2×[0,1]T^{2}\times[0,1] with the two boundary components T2×{0}T^{2}\times\{0\} and T2×{1}T^{2}\times\{1\} collapsed to two points p0p_{0} and p1p_{1}. We regard NN as an immersion of S⁡(T2)S(T^{2}) in which p0p_{0} and p1p_{1} have the same image.

The singularity of NN is two T2T^{2}-cones meeting at their vertices. According to the author’s theory of SL singularities mentioned in §7.3, generic SL T2T^{2}-cone singularities are modelled on the isomorphic cones L0±L_{0}^{\pm} of (16). So suppose that the singularity of NN is locally modelled on two copies of L0±L_{0}^{\pm}.

Now consider how NN deforms under small generic perturbations of XX as an almost Calabi–Yau 3-fold. According to the author’s theory, a singular SL 3-fold with the topology of S⁡(T2)S(T^{2}) and two singular points modelled on L0±L_{0}^{\pm} should be isolated and stable under small deformations. Thus, as an immersed copy of S⁡(T2)S(T^{2}) we expect NN to be stable under deformations of XX. However, there is no reason for the two singular points p0,p1p_{0},p_{1} of S⁡(T2)S(T^{2}) to coincide when we deform XX.

The condition for this to happen is of real codimension 6 in the space of all almost Calabi–Yau 3-folds. Therefore, singular SL 3-folds with the topology of T3T^{3} with T2T^{2} collapsed to a point should exist only in codimension 6, and not in the generic case. Thus a positive singular fibre is not a feasible model for singular fibres in generic SL fibrations.

Note also that Ruan’s piecewise smooth Lagrangian fibrations defined using gradient flow, described briefly in §3.2, contain positive singular fibres by [19, Th. 2.2]. So the argument above shows that the topological type of Ruan’s fibrations is not quite right to be fibrations of generic almost Calabi–Yau manifolds, although the degree of nongenericity is much less than in the smooth fibration picture.

The author believes that the Gross–Ruan smooth fibration picture is essentially correct at the (degenerate) large complex structure limit, and perhaps also for some nongeneric almost Calabi–Yau structures near the complex limit. It should therefore be a very valuable tool for understanding the topology and symplectic geometry of mirror Calabi–Yau 3-folds, and will presumably give the right answers. For many of the purposes in which one would apply the Gross–Ruan picture, it is irrelevant whether there actually exists such a genuine special Lagrangian fibration or not.

[03ML]

9.2 Modification of this picture for generic ACY 3-folds

We are now ready to say something about what special Lagrangian fibrations of generic almost Calabi–Yau 3-folds might look like. Suppose we start with a smooth Gross–Ruan fibration f:X→Bf:X\rightarrow B, either of a nongeneric almost Calabi–Yau 3-fold or of the degenerate large complex structure limit, and make a small perturbation to a generic almost Calabi–Yau 3-fold. What happens to the fibration?

Near a nonsingular fibre Nb=f−1​(b)N_{b}=f^{-1}(b) of ff, the fibration should remain nonsingular, and the local geometry unchanged. The interesting question is what happens to the singular fibres of ff. The following is the author’s best guess, on the assumption that special Lagrangian fibrations are well-behaved in the generic case. We preface it with some remarks on monodromy and coordinates on the moduli space.

Let f:X→Bf:X\rightarrow B be an SL fibration with generic fibre T3T^{3}. By Theorem 2.9, near a nonsingular fibre NbN_{b} the moduli space of deformations of NbN_{b} is isomorphic to H1(Nb;ℝ)≅ℝ3H^{1}(N_{b};\mathbin{\mathbb{R}})\cong\mathbin{\mathbb{R}}^{3}. But this moduli space is BB, and so near any point in B∖ΔfB\setminus\Delta_{f} we have natural affine coordinates modelled on H1​(T3,ℝ)H^{1}(T^{3};\mathbin{\mathbb{R}}).

However, near a singular fibre NbN_{b} the situation is more complicated because of the monodromy action. Let Nb′N_{b^{\prime}} be a nonsingular fibre near NbN_{b}. Let Γb\Gamma_{b} be the set of monodromies of loops in B∖ΔfB\setminus\Delta_{f} based at b′b^{\prime} and staying in a small neighbourhood of bb. Then Γb\Gamma_{b} is a group acting on H1​(Nb′,ℤ)H_{1}(N_{b^{\prime}};\mathbin{\mathbb{Z}}) and H1​(Nb′,ℝ)H^{1}(N_{b^{\prime}};\mathbin{\mathbb{R}}). Roughly speaking, near bb we can regard BB as a kind of quotient of H1​(Nb′,ℝ)H^{1}(N_{b^{\prime}};\mathbin{\mathbb{R}}) by Γb\Gamma_{b}, so that BB is a kind of orbifold, with the topology of a 3-manifold, but not the smooth structure.

In what follows, as long as we make use of only Γb\Gamma_{b}-invariant objects, we can think of BB as being locally like ℝ3\mathbin{\mathbb{R}}^{3} and mostly ignore the monodromy action. We shall represent elements of H1​(Nb′,ℤ)H_{1}(N_{b^{\prime}};\mathbin{\mathbb{Z}}) by column vectors, and elements of H1​(Nb′,ℝ)H^{1}(N_{b^{\prime}};\mathbin{\mathbb{R}}) by row vectors, upon which the monodromy matrices of equations (68)–(70) act by left and right multiplication respectively.

Here is how generic fibrations might work near the perturbation of the Gross–Ruan singular fibres described in parts (a)–(c) of §9.1.

  • (a)

    The author conjectures that under small deformations, the ‘edges’ in the Gross–Ruan picture will thicken out into thin ‘ribbons’ of the kind described in §8. They are closed subsets of hyperplanes in BB defined locally by [ω]⋅[D]=0[\omega]\cdot[D]=0, where [ω][\omega] is the relative de Rham cohomology class in H1(X,Nb;ℝ)H^{1}(X,N_{b};\mathbin{\mathbb{R}}) and [D][D] a relative homology class in H1(X,Nb;ℤ)H_{1}(X,N_{b};\mathbin{\mathbb{Z}}) depending on the edge, which we expect to be represented by one or more holomorphic discs DD for some b∈Bb\in B, as we discussed in §7.3.

    The situation described in §8, in which the generic fibre has two singular points, is only the simplest possibility. In general we expect the generic singular fibres to contain an even number of singular points, divided equally into two kinds. In codimension one on the ribbon these singular points can appear or disappear in pairs of different kinds, and the edge of the ribbon is where the last two singular points disappear.

    We can give local models for such fibrations by modifying Assumption 8.1, replacing the function cos⁡x\cos x in parts (iii) and (iv) by a more general smooth function g⁡(x)g(x) with period 2​π2\pi and nondegenerate stationary points, modifying part (v) to refer to the stationary points of gg, and dropping part (vi) entirely.

    Observe that the matrices (67) and (68) are conjugate in SL(3,ℤ)\mathop{\rm SL}(3,\mathbin{\mathbb{Z}}). Thus, the monodromy around a ‘ribbon’ that we calculated in §8.2 is the same as that around an edge in the Gross–Ruan picture.

  • (b)

    For positive vertices in the Gross–Ruan picture, the monodromy matrices of (69) all fix the vectors

    𝐯1=(010),𝐯2=(00−1)and𝐯3=(0−11){\bf v}_{1}=\begin{pmatrix}0\\ 1\\ 0\end{pmatrix},\quad{\bf v}_{2}=\begin{pmatrix}0\\ 0\\ -1\end{pmatrix}\quad\text{and}\quad{\bf v}_{3}=\begin{pmatrix}0\\ -1\\ 1\end{pmatrix}

    in H1​(Nb′,ℤ)H_{1}(N_{b^{\prime}};\mathbin{\mathbb{Z}}) and the direction (1 0 0)(1\,0\,0) in H1​(Nb′,ℝ)H^{1}(N_{b^{\prime}};\mathbin{\mathbb{R}}).

    In a generic perturbation of a Gross–Ruan fibration near a positive vertex, the three edges in Δf\Delta_{f} should thicken out into ‘ribbons’ R1,R2,R3R_{1},R_{2},R_{3} lying in the three hyperplanes

    H1={(x1,0,x3):xj∈ℝ},H2={(x1,x2,0):xj∈ℝ}\displaystyle H_{1}=\bigl\{(x_{1},0,x_{3}):x_{j}\in\mathbin{\mathbb{R}}\bigr\},\qquad H_{2}=\bigl\{(x_{1},x_{2},0):x_{j}\in\mathbin{\mathbb{R}}\bigr\}
    andH3={(x1,x2,x3):xj∈ℝ,x2=x3},\displaystyle\text{and}\qquad H_{3}=\bigl\{(x_{1},x_{2},x_{3}):x_{j}\in\mathbin{\mathbb{R}},\quad x_{2}=x_{3}\bigr\},

    which are the hyperplanes dual to 𝐯1,𝐯2,𝐯3{\bf v}_{1},{\bf v}_{2},{\bf v}_{3}, and intersect in the line {(x1,0,0):x1∈ℝ}\bigl\{(x_{1},0,0):x_{1}\in\mathbin{\mathbb{R}}\bigr\}. The ribbons R1,R2,R3R_{1},R_{2},R_{3} intersect in a bounded subinterval of this line, as sketched in Figure 4.

    ∙\textstyle{\bullet}∙\textstyle{\bullet}∙\textstyle{\bullet}R1\textstyle{R_{1}}R2\textstyle{R_{2}}b0\textstyle{\scriptstyle b_{0}}R3\textstyle{R_{3}}......

    Figure 4: Discriminant locus near a perturbation of a positive vertex

    There are two obvious ways for this to happen, in which either R1∩R2∩R3R_{1}\cap R_{2}\cap R_{3} is part of the boundary of each RjR_{j}, or the ribbons RjR_{j} extend a little way beyond their intersection R1∩R2∩R3R_{1}\cap R_{2}\cap R_{3}. The author thinks that the latter option is what actually happens, as in Figure 4.

    For generic points in the intersection R1∩R2∩R3R_{1}\cap R_{2}\cap R_{3} the singularities of the fibres are just finitely many points modelled locally on the T2T^{2}-cones L0±L_{0}^{\pm} of (16). These are divided into three kinds, corresponding to the ribbons R1,R2,R3R_{1},R_{2},R_{3}, according to the homology class of the 𝒮1{\mathcal{S}}^{1} in T3T^{3} that collapses to a point.

    However, at certain special points b0b_{0} in R1∩R2∩R3R_{1}\cap R_{2}\cap R_{3} there will be a new kind of codimension three singularity, when two or three of these singular points of different kinds come together. The author does not have a local model for this singularity, but topologically it may involve a cone on a genus 2 surface. There must be at least one such singular fibre, as it is necessary for the monodromy to work out.

    We expect that when Nb′N_{b^{\prime}} is a nonsingular fibre near the ribbon RjR_{j}, there should exist holomorphic discs DD in XX whose boundary ∂D\partial D in Nb′N_{b^{\prime}} has homology class 𝐯j{\bf v}_{j} in H1​(Nb′,ℤ)H_{1}(N_{b^{\prime}};\mathbin{\mathbb{Z}}). Singularities develop when the area of DD shrinks to zero, which happens on the hyperplane HjH_{j} in BB.

  • (c)

    For negative vertices, the monodromy matrices of (70) all fix the vector (1 0 0)T(1\,0\,0)^{T} in H1​(Nb′,ℤ)H_{1}(N_{b^{\prime}};\mathbin{\mathbb{Z}}) and the hyperplane {(0,x2,x3):xj∈ℝ}\bigl\{(0,x_{2},x_{3}):x_{j}\in\mathbin{\mathbb{R}}\bigr\} in H1​(Nb′,ℝ)H^{1}(N_{b^{\prime}};\mathbin{\mathbb{R}}). In a generic perturbation of a Gross–Ruan fibration near a negative vertex, the three edges in Δf\Delta_{f} should thicken out into ‘ribbons’ which all lie in the same hyperplane HH in BB, isomorphic to {(0,x2,x3):xj∈ℝ}\bigl\{(0,x_{2},x_{3}):x_{j}\in\mathbin{\mathbb{R}}\bigr\} in H1​(Nb′,ℝ)H^{1}(N_{b^{\prime}};\mathbin{\mathbb{R}}). The three ribbons merge together to make a letter YY shape in HH, as sketched in Figure 5.

    Figure 5: Discriminant locus near a perturbation of a negative vertex

    We expect that when Nb′N_{b^{\prime}} is a nonsingular fibre near this part of Δf\Delta_{f}, there should exist an even number of homologous holomorphic discs DD in XX whose boundaries ∂D\partial D in Nb′N_{b^{\prime}} have homology class (1 0 0)T(1\,0\,0)^{T} in H1​(Nb′,ℤ)H_{1}(N_{b^{\prime}};\mathbin{\mathbb{Z}}). Singularities develop when the area of DD shrinks to zero, which happens on the hyperplane HH in BB.

    Calculations by the author, along the lines of §8 but more complicated, show that one can put together a fibration with the topological properties we want using only the local models of §5 and §7. There is no need to include any other kind of singular point.

The author is fairly confident about parts (a) and (c), but rather less happy about part (b). In fact, Ruan’s Lagrangian fibrations by gradient flow look quite like parts (a) and (c) in the relevant regions. Another option in part (b) is that there could be a new kind of codimension two singularity along the line segment R1∩R2∩R3R_{1}\cap R_{2}\cap R_{3}.

[03MM]

9.3 Conclusions

If the speculations of §9.2 are correct, they have important consequences for the SYZ Conjecture. Positive and negative singular fibres are expected to be dual to one another under the mirror transform. That is, if we have dual smooth SL fibrations f:X→Bf:X\rightarrow B and f^:X^→B\hat{f}:\hat{X}\rightarrow B as in the SYZ conjecture, then positive vertices in the discriminant Δf\Delta_{f} of ff in BB should coincide with negative vertices in the discriminant Δf^\Delta_{\smash{\hat{f}}} of f^\hat{f}, and vice versa. One way to see this is that the monodromy matrices in (69) are the transposes of those in (70).

However, after a small generic perturbation of ff and f^\hat{f} near such a vertex in BB, it is clear from Figures 4 and 5 that the discriminant loci Δf\Delta_{f} and Δf^\Delta_{\smash{\hat{f}}} can no longer be identified, because they are not homeomorphic. On this basis we make the following conjecture.

[03MN]
Conjecture 9.1

Let X,X^X,\hat{X} be generic mirror Calabi–Yau 33-folds. Then even if there do exist special Lagrangian fibrations f:X→Bf:X\rightarrow B and f^:X^→B^\hat{f}:\hat{X}\rightarrow\hat{B}, it is not in general possible to homeomorphically identify the bases BB and B^\hat{B} of the fibrations in a way that identifies the discriminants Δf\Delta_{f}, Δf^\Delta_{\smash{\hat{f}}} of f,f^f,\hat{f}, and so that the nonsingular fibres of f,f^f,\hat{f} are 33-tori with dual homology.

This is a kind of counter-conjecture to the SYZ Conjecture, in that it contradicts some of the stronger forms of the SYZ Conjecture that people have written down so far, and if it is true then it will limit the scope of any eventual final formulation of the SYZ Conjecture. The author’s feeling is that while the SYZ Conjecture is clearly morally and spiritually true, it is probably not literally true of genuine special Lagrangian fibrations of holonomy SU(3)\mathop{\rm SU}(3) Calabi–Yau 3-folds, except in some limiting sense in the large complex structure limit.

Finally, we note that the discussion above is based on optimistic assumptions on how well-behaved generic special Lagrangian fibrations are. Here are two ways in which things might go wrong.

  • (i)

    Rather than speaking of a fibration ff, we should instead consider a 3-dimensional family ℳ\mathcal{M} of special Lagrangian 3-folds NN in XX, generically 3-tori, and thought of as the fibres of ff. Hopefully ℳ\mathcal{M} is homeomorphic to a compact 3-manifold without boundary.

    It might be that in some regions of XX there is more than one SL 3-fold in ℳ\mathcal{M} passing through each point. In this case, there will be no map f:X→Bf:X\rightarrow B with fibres ℳ\mathcal{M}. But ℳ\mathcal{M} could still have the property that for each generic point xx in XX the number of elements of ℳ\mathcal{M} passing through xx, counted with signs, is one, so that ℳ\mathcal{M} could be regarded as a ‘fibration’ in a generalized sense.

  • (ii)

    Again, we think of the family ℳ\mathcal{M} rather than the fibration ff. But something worse than (i) might happen. Perhaps there is some new kind of codimension one singularity which means that ℳ\mathcal{M} is a manifold with boundary. The singularities of §7–§8 do not count as boundary singularities, as ℳ\mathcal{M} extends on both sides of them.

    If ℳ\mathcal{M} is a manifold with boundary then the number of elements of ℳ\mathcal{M} passing through x∈Xx\in X, even counted with signs, need not be constant, and some points xx might not lie in any N∈ℳN\in{\mathcal{M}} at all. So the fibration ff would not exist even in the generalized sense above.

The author expects (i) to actually be the rule rather than the exception in general Calabi–Yau 3-folds, but perhaps it does not happen close to the large complex structure limit. Behaviour as in part (i) can arise in a nonsingular part of the ‘fibration’, when the harmonic 1-forms on a nonsingular special Lagrangian T3T^{3} develop zeros, so that neighbouring nonsingular ‘fibres’ intersect one another.

It may also be that the suggestions in part (b) of §9.2 are wrong, and behaviour as in part (ii) above happens instead. It is because the author takes this possibility seriously that we have not made any conjectures that positively assert the existence of special Lagrangian fibrations on generic almost Calabi–Yau 3-folds in this paper, even though it was very tempting to do so.

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