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On the Complex Affine Structures of SYZ Fibration of Del Pezzo Surfaces

Siu-Cheong Lau [email protected] Mathematics and Statistics Department, Boston University, 111 Cummington Mall, Boston MA 02215 Tsung-Ju Lee [email protected] Center of Mathematical Sciences and Applications, 20 Garden St., Cambridge, MA 02138  and  Yu-Shen Lin [email protected] Mathematics and Statistics Department, Boston University, 111 Cummington Mall, Boston MA 02215
Abstract.

Given any smooth cubic curve E2E\subseteq\mathbb{P}^{2}, we show that the complex affine structure of the special Lagrangian fibration of 2E\mathbb{P}^{2}\setminus E constructed by Collins–Jacob–Lin [CJL] coincides with the affine structure used in Carl–Pomperla–Siebert [CPS] for constructing mirror. Moreover, we use the Floer-theoretical gluing method to construct a mirror using immersed Lagrangians, which is shown to agree with the mirror constructed by Carl–Pomperla–Siebert.

1. Introduction

Mirror symmetry is a duality between the symplectic geometry of a Calabi–Yau manifold XX and the complex geometry of its mirror Xˇ\check{X}. With the help of mirror symmetry, one can achieve a lot of enumerative invariants of Calabi–Yau manifolds, which are a priori hard to compute.

To construct the mirror for a Calabi–Yau manifold, Strominger–Yau–Zaslow proposed the following conjectures [SYZ]: First of all, a Calabi–Yau manifold XX near the large complex structure limit admits a special Lagrangian fibration. This is one of the very few geometric descriptions of Calabi–Yau manifolds. Second, the mirror Xˇ\check{X} of XX can be constructed as the dual torus fibration of XX. Third, the Ricci-flat metric on XX is closed to the semi-flat metric, with corrections coming from the holomorphic discs with boundaries on special Lagrangian torus fibres.

For a long time, Strominger–Yau–Zaslow conjecture serves a guiding principle for mirror symmetry. Many of its implications are proved as the building blocks for understanding mirror symmetry. For instance, it provides a geometric way of realizing the homological mirror functor [LYZ]. However, there is very few progress on the original conjecture itself. Only very few examples of special Lagrangian fibrations are known due to technical difficulties of knowing explicit form of Ricci-flat metric. From the conjecture, one need to know the Ricci-flat metric for the existence of special Lagrangian fibration. While the explicit form of the Ricci-flat metric would involve the correction from the holomorphic discs. To retrieve such information, one need to know the boundary conditions, which are provided by the special Lagrangian torus fibres. Thus, the special Lagrangian fibration, the Ricci-flat metric and the correction from holomorphic discs form an iron triangle and firmly linked to each other. Actually, all the examples in the literature are either with respect to the flat metric or the hyperKähler rotation of the holomorphic Lagrangian fibrations. Furthermore, one usually can only track the hyperKähler manifold via Torelli type theorem after hyperKähler rotation rather than writing down the explicit equation.

To get around the analytic difficulties, Kontsevich–Soibelman [KS1], Gross–Siebert [GS1] developed the algebraic alternative to construct the mirror families using rigid analytic spaces. One takes the dual intersection complex BB of the maximal degenerate Calabi–Yau varieties, there is a natural integral affine structures with singularities on BB. By studying the scattering diagrams on BB, one can reconstruct the Calabi–Yau family near the large complex structure limit. It is a folklore theorem that the affine manifold BB is the base for the Strominger–Yau–Zaslow conjecture, while the support of the scattering diagrams are the projection of the holomorphic discs with boundaries on special Lagrangian torus fibres. There are many success of understanding mirror symmetry via this algebraic approach.

On the other hand, one can use Lagrangian Floer theory to construct mirrors and prove homological mirror symmetry. Fukaya [F0] has proposed family Floer homology which was further developed by Tu [T4] and Abouzaid [A2, A3]. The family Floer mirror is constructed as the set of Maurer–Cartan elements for the AA_{\infty} structures of the Lagrangian torus fibres quotient by certain equivalences. As Lagrangian torus fibres bound Maslov index zero holomorphic discs, the Maurer–Cartan elements will jump and induces non-trivial gluing of charts. It is expected that such jumps behave the same way as the cluster transformations associate to the ones in the scattering diagram.

A symplectic realization of the SYZ mirror construction was first illustrated in some inspiring examples by Auroux [A]. Using symplectic geometry, the SYZ mirror construction was realized for toric Calabi–Yau manifolds [CLL] by Chan, Leung and the first named author. They have interesting mirror maps and Gromov-Witten theory. The mirror construction for blowing-up of toric hypersurfaces was realized by Abouzaid-Auroux-Katzarkov [AAK]. Fukaya–Oh–Ohta–Ono [FOOO-T1, FOOO-T2, FOOO-MS] developed the Floer-theoretical construction in great detail for compact toric manifolds, which generalize and strengthen the result of Cho–Oh [CO] for toric Fano manifolds.

In all these cases, the mirrors constructed in symplectic geometry coincide with the ones produced from Gross–Siebert program. The holomorphic discs can be written down explicitly and no scattering of Maslov index zero discs occur.

Singular SYZ fibers are the sources of Maslov index zero holomorphic discs and quantum corrections. In [CHL, CHL-nc], Cho, Hong and the first named author found a way to construct a localized mirror of a Lagrangian immersion by solving the Maurer–Cartan equation for the formal deformations coming from immersed sectors. Moreover, gluing between the local mirror charts based on Fukaya isomorphisms was developed in [CHL-glue]. Applying to singular fibers, it gives a canonical (partial) compactification of the SYZ mirror by gluing the local mirror charts of singular fibers with those of regular tori [HKL].

In general, it is difficult to explicitly compute the Floer theoretical mirror. Maslov index zero discs can glue to new families of Maslov index zero discs, which is analogue of scattering or wall-crossing in Gross–Siebert program. It is in general complicated to control the scattering of Maslov index zero discs.

With the assumption that the Lagrangian fibration is special, one can have extra control of the locus of torus fibres bounding holomorphic discs. They form affine lines with respect to the complex affine structure. In particular, this allows us to study a version of open Gromov–Witten invariants defined by the third author and identified them with the tropical disc counting [L1, L2, L14].

It is reasonable to expect that the Gross–Siebert mirror and the Floer-theoretical mirror are equivalent. The first step toward such statement is to identify the affine manifolds with singularities of the SYZ fibration and the one used in the Gross–Siebert program.

Conjecture 1.1.

Let XtX_{t} be a family of Calabi–Yau toric degeneration X0X_{0} and XtX_{t} admits a special Lagrangian fibration. Then the limit of the complex affine structures of the special Lagrangian fibration coincides with the affine structures on the dual intersection complex of X0X_{0}.

In this paper, we will establish first such a statement for the case of 2\mathbb{P}^{2}.

Theorem 1.2 (=Theorem 3.12).

Conjecture 1.1 holds for the SYZ fibration of X=2EX=\mathbb{P}^{2}\setminus E, where EE is a smooth cubic curve.

The Gross–Siebert type mirror construction of 2E\mathbb{P}^{2}\setminus E is done by Carl–Pomperla–Siebert [CPS] and the mirror is the fiberwise compactification of its Landau–Ginzburg mirror. In particular, it has the following description: First, take the toric variety 2/3\mathbb{P}^{2}/\mathbb{Z}_{3}, whose moment-map polytope is dual to that of 2\mathbb{P}^{2}, see Figure 1. We have the meromorphic function W=z+w+1/zwW=z+w+1/zw on 2/3\mathbb{P}^{2}/\mathbb{Z}_{3}. The pole divisor of WW is the sum of the three toric divisors. The zero divisor of WW intersects with the pole divisor at three points. We blow up 2/3\mathbb{P}^{2}/\mathbb{Z}_{3} at these three points, so that WW induces an elliptic fibration. (We can further blow up the three orbifold points of 2/3\mathbb{P}^{2}/\mathbb{Z}_{3} to make the total space smooth.) Finally we delete the strict transform of the three toric divisors (which is the fiber at \infty) and this defines the mirror space. The Landau–Ginzburg superpotential is the elliptic fibration map induced by WW. It is also worth noticing that the theorem is also achieved by Pierrick Beausseau with a different approach [P]. We refer the readers for the inspiring heuristic discussion there about such an expectation from a different point of view.

Refer to caption
Figure 1. The moment-map polytope of 2\mathbb{P}^{2} and its dual.

For the family Floer mirror, it is glued from torus charts, which are the deformation spaces of Lagrangian torus fibers. Due to scattering of Maslov zero holomorphic discs, there are infinitely many walls and chambers in this case, and each chamber corresponds to a torus chart.

On the other hand, in the Fano situation of this paper, we can use the method in [CHL-glue, HKL] to construct a \mathbb{C}-valued mirror. The special Lagrangian fibration on 2E\mathbb{P}^{2}\setminus E [CJL] has three singular fibers which are nodal tori. Instead of the (infinitely many) torus fibers, we take the monotone moment-map torus together with three monotone Lagrangian immersions (in place of the singular SYZ fibers), and glue their deformation spaces together to construct the mirror.

Theorem 1.3.

For 2E\mathbb{P}^{2}\setminus E, the Floer-theoretical mirror glued from the deformation spaces of the monotone moment-map torus and the three monotone Lagrangian immersions coincides with the Carl–Pomperla–Siebert mirror described above.

More precisely, the gluing construction has to be carried out over the Novikov field

Λ:={i=0ai𝐓Aiai,Ai and increases to +}\Lambda:=\left\{\sum_{i=0}^{\infty}a_{i}\mathbf{T}^{A_{i}}\mid a_{i}\in\mathbb{C},A_{i}\in\mathbb{R}\textrm{ and increases to }+\infty\right\}

so that the Lagrangian deformation spaces have the correct topology and dimension. See Remark 4.10. After we glue up a space over Λ\Lambda using Lagrangian Floer theory, we restrict to \mathbb{C} to get a \mathbb{C}-valued mirror.

Outline of the paper

In Section 2, we review the geometry of the special Lagrangian fibration on 2E\mathbb{P}^{2}\setminus E and the complex affine structure induced from the special Lagrangian fibration in Section . We also describe the affine manifold which is used to construct for mirror in [CPS]. In Section 3, we first explain how to use hyperKähler rotation to reduce the problem to relative periods of an extremal rational elliptic surface, where the geometry can be very explicit. Then we verified various properties of the relative periods for the proof of the main theorem. In Section 4, we carry out the Floer theoretical construction and show that it agrees with Carl–Pomperla–Siebert mirror.

Acknowledgement

The authors would like to thank S.-T. Yau for constant encouragement and the Center of Mathematical Sciences and Applications for the wonderful research environment. The first author expresses his gratitude to Cheol-Hyun Cho, Hansol Hong and Yoosik Kim for the useful joint works. The third author wants to thank Peirrick Beasseau, Tristan Collins, Adam Jacob for related discussion. The first author is supported by Simons Collaboration Grant #580648. The second author is supported by the Center of Mathematical Sciences and Applications. The third author is supported by Simons Collaboration Grant #635846.

2. SYZ Fibration on Del Pezzo Surfaces

We will first review the results in [CJL]: Let YY be a del Pezzo surface or a rational elliptic surface. D|KY|D\in|-K_{Y}| be a smooth anti-canonical divisor and X=YDX=Y\setminus D. There exists a meromorphic volume form Ω\Omega on with simple pole along DD which is unique up to a \mathbb{C}^{\ast}-scaling. Therefore, one can view XX as a log Calabi–Yau surface. Moreover, Tian–Yau proved the following theorem:

Theorem 2.1 ([TY1]).

There exists an exact complete Ricci-flat metric ωTY\omega_{TY} on XX.

We will assume that 2ωTY2=ΩΩ¯2\omega_{TY}^{2}=\Omega\wedge\bar{\Omega} after a suitable scaling of Ω\Omega.

Definition 2.2.

Let XX be a complex manifold with a holomorphic volume form Ω\Omega and a Ricci-flat metric ω\omega. A half dimensional submanifold LL is a special Lagrangian with respect to (ω,Ω)(\omega,\Omega) if ω|L=0\left.\omega\right|_{L}=0 and ImΩ|L=0\left.\mathrm{Im}\Omega\right|_{L}=0.

It is conjectured by Yau and also Auroux [A2] that there exists a special Lagrangian fibration on XX. The conjecture is proved by Colllins–Jacob–Lin earlier.

Theorem 2.3 ([CJL]).

The log Calabi–Yau surface XX admits a special Lagrangian fibration π:XBSYZ\pi:X\rightarrow B_{\mathrm{SYZ}} with respect to ωTY\omega_{TY}.

Although the proof of the existence of special Lagrangian fibration in [CJL] still largely use the hyperKähler structure, an important difference from the earlier examples is that one knows which complex structure can support the special Lagrangian fibration. Moreover, one can use algebraic geometry to understand the complex structure after the hyperKähler rotation.

Theorem 2.4 ([CJL]).

With the above notation and d=(KY)2d=(-K_{Y})^{2}. Let Xˇ\check{X} denotes the underlying topological space of XX with Kähler form and holomorphic volume form

ωˇ\displaystyle\check{\omega} =ReΩ\displaystyle=\mathrm{Re}~{}\Omega
(2.1) Ωˇ\displaystyle\check{\Omega} =ω1ImΩ.\displaystyle=\omega-\sqrt{-1}\cdot\mathrm{Im}~{}\Omega.

Then Xˇ\check{X} admits an elliptic fibration and compactifiation to a rational elliptic surface Yˇ\check{Y} by adding an IdI_{d} singular fibre over \infty.

Xˇ{\check{X}}(Yˇ,Id){(\check{Y},I_{d})}{\mathbb{C}}(1,){(\mathbb{P}^{1},\infty)}

From the asymptotic behavior of Ωˇ\check{\Omega}, one has

Proposition 2.5.

[CJL2] The holomorphic 22-form Ωˇ\check{\Omega} on Xˇ\check{X} coincide with the meromorphic 22-form on Yˇ\check{Y} with simply pole along the fibre over \infty.

In particular, the rational elliptic surface Yˇ\check{Y} has singular configuration I9I13I_{9}I_{1}^{3} for the case Y=2Y=\mathbb{P}^{2} [CJL]. The extremal rational elliptic surfaces have no deformation and thus can be identified by explicit equation. In the case of Y=2Y=\mathbb{P}^{2}, Xˇ\check{X} can actually be realized as the fibrewise compactification of the Landau–Ginzburg mirror

(2.2) W:()2(t1,t2)t1+t2+1t1t2.\displaystyle\begin{split}W\colon(\mathbb{C}^{\ast})^{2}&\longrightarrow\mathbb{C}\\ (t_{1},t_{2})&\mapsto t_{1}+t_{2}+\frac{1}{t_{1}t_{2}}.\end{split}

It is straight-forward to check that WW has three critical values λ0,λ1,λ2\lambda_{0},\lambda_{1},\lambda_{2} and the cross-ratio with \infty is fixed. Thus, we may assume that λi=3ζi\lambda_{i}=3\zeta^{i}, where ζ=exp(2πi/3)\zeta=\exp{(2\pi i/3)}. The fibres of WW are three-punctured elliptic curves. By computing the global monodromy which is conjugating to

[1901],\begin{bmatrix}1&9\\ 0&1\end{bmatrix},

the Lefschetz fibration W:()2W\colon(\mathbb{C}^{\ast})^{2}\rightarrow\mathbb{C} can be compactified to such an extremal rational elliptic surface by adding three sections and an I9I_{9}-fibre at infinity.

Refer to caption
Figure 2. The vanishing cycles in E0E_{0}

There is a 3\mathbb{Z}_{3}-action (x,y)(ζx,ζy)(x,y)\mapsto(\zeta x,\zeta y) on ()2(\mathbb{C}^{\ast})^{2} which induces a 3\mathbb{Z}_{3}-action on the base 1\mathbb{P}^{1} permuting the three critical values. Let E0E_{0} be the fibre over 010\in\mathbb{P}^{1} which is fixed by the 3\mathbb{Z}_{3}-action.

Lemma 2.6 (cf. [AKO]*Lemma 3.1).

We can choose a basis {a,b}\{a,b\} for H1(E0,)2\mathrm{H}_{1}(E_{0},\mathbb{Z})\simeq\mathbb{Z}^{2} and orientations for the vanishing cycles [V0][V_{0}], [V1][V_{1}], [V2][V_{2}] of λ0\lambda_{0}, λ1\lambda_{1}, λ2\lambda_{2} such that [V0][V_{0}], [V1][V_{1}] and [V2][V_{2}] are represented by 2ab-2a-b, a+2ba+2b and aba-b respectively and the vanishing cycle from \infty along the curve O¯\overline{\infty O} in Figure 4 is represented by bb. In particular, we have [V0]+[V1]+[V2]=0[V_{0}]+[V_{1}]+[V_{2}]=0.

Remark 2.7.

We remind the readers that our λi\lambda_{i} is different from the one used in [AKO]. Indeed, V0L0V_{0}\equiv L_{0}, V1L2V_{1}\equiv L_{2} and V2L1V_{2}\equiv-L_{1}, where LiL_{i} is the vanishing cycle defined in [AKO]*Lemma 3.1. However, to make the identification easier, we will use another basis.

We will describe the orientation explicitly in §3.3 (C).

Given a special Lagrangian fibration XBSYZX\rightarrow B_{\mathrm{SYZ}} with respect to (ω,Ω)(\omega,\Omega), we will denote LqL_{q} for the fibre over qBSYZq\in B_{\mathrm{SYZ}}. Let B0B_{0} be the complement of discriminant locus, then there exists an integral affine structure on B0B_{0} [H2] which we will now explain below: Choose a reference fibre Lq0L_{q_{0}} and basis eiH1(Lq0)e_{i}\in\mathrm{H}_{1}(L_{q_{0}}). For a nearby torus fibre LqL_{q} and a path ϕ\phi connecting qq and q0q_{0}, let CiC_{i} be the union of the parallel transport of eie_{i} along ϕ\phi. Then the complex affine coordinate fi(q)f_{i}(q) of qq is defined to be

(2.3) fi(q):=CiImΩ,\displaystyle f_{i}(q):=\int_{C_{i}}\mbox{Im}\Omega,

which is well-defined since Lq,Lq0L_{q},L_{q_{0}} are special Lagrangians. It is straight-forward to check that for a different choice of the basis and paths, the transition function falls in GL(n,)n\mathrm{GL}(n,\mathbb{Z})\rtimes\mathbb{R}^{n}, where n=dimLqn=\mbox{dim}_{\mathbb{R}}L_{q}. Thus, B0B_{0} is an integral affine manifold and we say BSYZB_{\mathrm{SYZ}} is an integral affine manifold with singularities Δ=BSYZB0\Delta=B_{\mathrm{SYZ}}\setminus B_{0}. The above integral affine structure is usually known as the complex affine structure of the special Lagrangian fibration in the context of mirror symmetry.

3. Equivalence of the Two Affine Structures

From now on, we concentrate on the case Y=2Y=\mathbb{P}^{2} with the Landau–Ginzburg potential function (2.2). Recall that 2\mathbb{P}^{2} is defined by the polytope Δ=Conv{(1,1),(2,1),(1,2)}\Delta=\mathrm{Conv}\{(-1,-1),(2,-1),(-1,2)\}. Let =Δ\nabla=\Delta^{\vee} be the dual polytope. We denote by 𝐏\mathbf{P}_{\nabla} the toric variety defined by \nabla and by 𝐏~𝐏\widetilde{\mathbf{P}}_{\nabla}\to\mathbf{P}_{\nabla} the maximal projective crepant partial resolution of 𝐏\mathbf{P}_{\nabla}, which is a resolution in the present case.

We denote by qq the coordinate of the target space of the potential function WW in (2.2) and regard (Wq1)(W-q\cdot 1) as a holomorphic section of the anti-canonical bundle over 𝐏~\widetilde{\mathbf{P}}_{\nabla}. Precisely, the monomials t1t_{1}, t2t_{2}, t11t21t_{1}^{-1}t_{2}^{-1} correspond to the integral points (1,0),(0,1),(1,1)(1,0),(0,1),(-1,-1) in \nabla and the monomial t10t20=1t_{1}^{0}t_{2}^{0}=1 corresponds to the integral point (0,0)(0,0). The subvariety {Wq1=0}𝐏~\{W-q\cdot 1=0\}\subset\widetilde{\mathbf{P}}_{\nabla} gives the desired compactification of our fiber W1(q)W^{-1}(q). The family {Wq1=0}\{W-q\cdot 1=0\} is a pencil spanned by the section 11 and t1+t2+t11t21t_{1}+t_{2}+t_{1}^{-1}t_{2}^{-1}, and can be extended to a family over 1\mathbb{P}^{1}. It is straightforward to check that the sections 11 and t1+t2+t11t21t_{1}+t_{2}+t_{1}^{-1}t_{2}^{-1} intersect at three points. Blowing-up the base locus gives a morphism Yˇ1\check{Y}\to\mathbb{P}^{1}. The fiber at 1\infty\in\mathbb{P}^{1} is a union of proper transforms of toric divisors in 𝐏~\widetilde{\mathbf{P}}_{\nabla}, which is a I9I_{9} fiber. For simplicity, the proper transform of the I9I_{9} fiber in Yˇ\check{Y} is also denoted by I9I_{9}.

Let Xˇ:=YˇI9\check{X}:=\check{Y}\setminus I_{9}. First of all, it is clear that

H4(Yˇ,),H2(Yˇ,)10,andH0(Yˇ,).\mathrm{H}_{4}(\check{Y},\mathbb{Z})\simeq\mathbb{Z},~{}\mathrm{H}_{2}(\check{Y},\mathbb{Z})\simeq\mathbb{Z}^{10},~{}\mbox{and}~{}\mathrm{H}_{0}(\check{Y},\mathbb{Z})\simeq\mathbb{Z}.

Secondly, from the Poincaré duality for orientable manifolds, we have

Hk(Xˇ,)Hc4k(Xˇ,)Hk(Xˇ,),k.\mathrm{H}_{k}(\check{X},\mathbb{Z})\simeq\mathrm{H}^{4-k}_{\mathrm{c}}(\check{X},\mathbb{Z})\simeq\mathrm{H}^{k}(\check{X},\mathbb{Z}),~{}\forall~{}k.

Finally, let UU be the preimage of a small neighborhood around 1\infty\in\mathbb{P}^{1} under Yˇ1\check{Y}\to\mathbb{P}^{1}. I9I_{9} is a retract of UU. Utilizing the Mayer–Vietoris resolution for simple normal crossing varieties, one can easily derive

H2(I9,)9,H1(I9,),andH0(I9,).\mathrm{H}^{2}(I_{9},\mathbb{Z})\simeq\mathbb{Z}^{9},~{}\mathrm{H}^{1}(I_{9},\mathbb{Z})\simeq\mathbb{Z},~{}\mbox{and}~{}\mathrm{H}^{0}(I_{9},\mathbb{Z})\simeq\mathbb{Z}.

Consider the Mayer–Vietoris sequence assicoated to the pair (U,Xˇ)(U,\check{X}), we can show that

H2(Xˇ,)H2(Xˇ,)2\mathrm{H}^{2}(\check{X},\mathbb{C})\simeq\mathrm{H}_{2}(\check{X},\mathbb{C})\simeq\mathbb{C}^{2}

We put Eq={Wq1=0}YˇE_{q}=\{W-q\cdot 1=0\}\subset\check{Y}. It follows that H2(Xˇ,)\mathrm{H}_{2}(\check{X},\mathbb{Z}) is generated by the class of S1×S1()2S^{1}\times S^{1}\subset(\mathbb{C}^{\ast})^{2} and the class of EqE_{q}.

From the construction, the standard toric form

dt1t1dt2t2\frac{\mathrm{d}t_{1}}{t_{1}}\wedge\frac{\mathrm{d}t_{2}}{t_{2}}

on ()2(\mathbb{C}^{\ast})^{2} extends to a meromorphic form on 𝐏~\widetilde{\mathbf{P}}_{\nabla} with poles along the union of toric divisors. Via the pullback further to Yˇ\check{Y}, we obtain a meromorphic 22-form which has poles exactly along I9I_{9}.

In what follows, we set

Ωˇ=1dt1t1dt2t2.\check{\Omega}=\sqrt{-1}\cdot\frac{\mathrm{d}t_{1}}{t_{1}}\wedge\frac{\mathrm{d}t_{2}}{t_{2}}.

The meromorphic top form Ωˇ\check{\Omega} has the property that

ReΩˇ|H2(Xˇ,)0.\mathrm{Re}\left.\check{\Omega}\right|_{\mathrm{H}_{2}(\check{X},\mathbb{Z})}\equiv 0.

We can represent Ωˇ\check{\Omega} in a different way, which turns out to be useful in the sequel. It follows from (2.2) that

dq\displaystyle\mathrm{d}q =dt1+dt2t1dt2+t2dt1(t1t2)2\displaystyle=\mathrm{d}t_{1}+\mathrm{d}t_{2}-\frac{t_{1}\mathrm{d}t_{2}+t_{2}\mathrm{d}t_{1}}{(t_{1}t_{2})^{2}}
=(11t12t2)dt1+(11t1t22)dt2.\displaystyle=\left(1-\frac{1}{t_{1}^{2}t_{2}}\right)\mathrm{d}t_{1}+\left(1-\frac{1}{t_{1}t_{2}^{2}}\right)\mathrm{d}t_{2}.

A direct calculation gives

dqdt1=1t1t22t2Ωˇ1\mathrm{d}q\wedge\mathrm{d}t_{1}=\frac{1-t_{1}t_{2}^{2}}{t_{2}}\frac{\check{\Omega}}{\sqrt{-1}}

and therefore

(3.1) Ωˇ=1t21t1t22dqdt1\check{\Omega}=\sqrt{-1}\cdot\frac{t_{2}}{1-t_{1}t_{2}^{2}}\mathrm{d}q\wedge\mathrm{d}t_{1}

provided that 1t1t2201-t_{1}t_{2}^{2}\neq 0.

3.1. The affine structure of Carl–Pumperla–Siebert

The construction of the mirror of a del Pezzo surface relative to a smooth anti-canonical divisor is studied in [CPS]. We describe the affine manifold with singularities used in [CPS] below. The underlying space is 2\mathbb{R}^{2} topologically. There are three singularities with local monodromy conjugate to

[1101]\begin{bmatrix}1&1\\ 0&1\end{bmatrix}

locating at A=(0,1/2)A^{\prime}=(0,-1/2), B=(1/2,1/2)B^{\prime}=(1/2,1/2) and C=(1/2,0)C^{\prime}=(-1/2,0). To cooperate with the standard affine structure of 2\mathbb{R}^{2} for computation convenience, they introduce cuts and the affine transformation as follows: let

l1+\displaystyle l_{1}^{+} ={(12,y)|y12}\displaystyle=\left\{\left(\frac{1}{2},y\right)\;\middle|\;y\geq\frac{1}{2}\right\}
l1\displaystyle l_{1}^{-} ={(x,12)|x12}\displaystyle=\left\{\left(x,\frac{1}{2}\right)\;\middle|\;x\geq\frac{1}{2}\right\}
l2+\displaystyle l_{2}^{+} ={(x,12)|x0}\displaystyle=\left\{\left(x,-\frac{1}{2}\right)\;\middle|\;x\geq 0\right\}
l2\displaystyle l_{2}^{-} ={(t,12t)|t0}\displaystyle=\left\{\left(-t,-\frac{1}{2}-t\right)\;\middle|\;t\geq 0\right\}
l3+\displaystyle l_{3}^{+} ={(12t,t)|t0}\displaystyle=\left\{\left(-\frac{1}{2}-t,-t\right)\;\middle|\;t\geq 0\right\}
l3\displaystyle l_{3}^{-} ={(12,y)|y0}\displaystyle=\left\{\left(-\frac{1}{2},y\right)\;\middle|\;y\geq 0\right\}

Disgard the sector bounded by li+,lil_{i}^{+},l_{i}^{-}, then glue the cuts by the affine transformations

(3.2) [1413],[2110],[1143]\begin{bmatrix}-1&4\\ -1&3\end{bmatrix},\begin{bmatrix}2&1\\ -1&0\end{bmatrix},\begin{bmatrix}-1&1\\ -4&3\end{bmatrix}

respectively and one reaches the affine manifold in [CPS]. See Figure 3. Notice that we glue the rays in clockwise order.

Refer to caption
Figure 3. The affine plane given in [CPS]
Definition 3.1.

The affine manifold with singularities in Carl–Pumperla–Siebert described above is denoted by BCPSB_{\mathrm{CPS}}.

3.2. A hyperKähler rotation trick

To compute the complex affine coordinates, generally one needs to compute the relative periods for the imaginary part of the holomorphic volume form on XX. Technically, it is not computable generally due to the fact that the special Lagrangian fibration is never explicit. The advantage of the work of Collins–Jacob–Lin is that one knows both the explicit equation of XX and Xˇ\check{X}. From (2.3) and Theorem 2.4, one can compute the complex affine coordinates via the geometry on Xˇ\check{X} with a particular phase for Ωˇ\check{\Omega}. From Mayer–Vietoris sequence, one has H2(Xˇ,)H2(X,)2\mathrm{H}_{2}(\check{X},\mathbb{Z})\cong\mathrm{H}_{2}(X,\mathbb{Z})\cong\mathbb{Z}^{2}. Since ωTY\omega_{TY} is exact, we have ωTY|H2(X,)0\left.\omega_{TY}\right|_{\mathrm{H}_{2}(X,\mathbb{Z})}\equiv 0. Because of the existence of the compact special Lagrangian tori, we have Ω|H2(X,)0\left.\Omega\right|_{\mathrm{H}_{2}(X,\mathbb{Z})}\neq 0. Therefore, the phase of Ωˇ\check{\Omega} need to be chosen such that

ReΩˇ|H2(Xˇ,)0\displaystyle\left.\mbox{Re}~{}\check{\Omega}\right|_{\mathrm{H}_{2}(\check{X},\mathbb{Z})}\equiv 0

from (2.4). To sum up, we have the following lemma:

Lemma 3.2.

We resume the notation introduced in the last paragraph in §2. The complex affine structure of the special Lagrangian fibration in Theorem 2.3 for 2\mathbb{P}^{2} can be computed via

fi(q):=CiImΩˇ\displaystyle f_{i}(q):=\int_{C_{i}}\mathrm{Im}~{}\check{\Omega}

on the extremal rational elliptic surface Yˇ\check{Y} with singular configuration I9I13I_{9}I_{1}^{3}. Here Ωˇ\check{\Omega} is the meromorphic volume form on Yˇ\check{Y} with simple pole along the I9I_{9} fibre and ReΩˇ|H2(Xˇ,)0\mathrm{Re}~{}\check{\Omega}|_{\mathrm{H}_{2}(\check{X},\mathbb{Z})}\equiv 0.

3.3. Relative periods on Yˇ\check{Y}

We analyze the relative periods on Yˇ\check{Y} in more detail in this paragraph. In what follows, the fiber over qq in Yˇ1\check{Y}\to\mathbb{P}^{1} is denoted by EqE_{q}. For simplicity, the points 33, 3ζ3\zeta and 3ζ23\zeta^{2} on q:=1{}\mathbb{C}_{q}:=\mathbb{P}^{1}\setminus\{\infty\} are denoted by AA, BB and CC respectively.

(A) Vanishing cycles

Note that E3E_{3}, E3ζE_{3\zeta} and E3ζ2E_{3\zeta^{2}} are all the singular fibers in Yˇ1\check{Y}\to\mathbb{P}^{1} and each of which is of type I1I_{1}. According to [AKO], after a parallel transport to E0E_{0}, the vanishing cycle for E3ζjE_{3\zeta^{j}} can be represented by a cycle VjV_{j} in E0E_{0} such that the image of VjV_{j} under the projection (t1,t2)t1(t_{1},t_{2})\mapsto t_{1} is given by the arcs δj\delta_{j} drawn in Figure 2.

Note that the cycle class [Vj]H1(E0,)[V_{j}]\in\mathrm{H}_{1}(E_{0},\mathbb{Z}) is only defined up to sign at this moment because we have not fixed the orientation yet. However, once the orientation of V0V_{0} is determined, the 3\mathbb{Z}_{3}-action will uniquely determine the orientations for V1V_{1} and V2V_{2}.

Lemma 3.3.

Suppose the orientation of VjV_{j} is given with respect to the 3\mathbb{Z}_{3}-action. We can accordingly choose an integral basis {c,d}H1(E0,)\{c,d\}\subset\mathrm{H}_{1}(E_{0},\mathbb{Z}) such that d,c=1\langle d,c\rangle=1 and the vanishing cycles [V0][V_{0}], [V1][V_{1}] and [V2][V_{2}] are represented by c2dc-2d, c+dc+d and 2c+d-2c+d, respectively. The presentations are chosen with respect to the 3\mathbb{Z}_{3}-action on the qq-plane q\mathbb{C}_{q} as well.

Proof.

Let {c,d}\{c,d\} be a basis given by

{a=c+db=c\begin{cases}a=-c+d\\ b=c\end{cases}

where {a,b}\{a,b\} is the basis in Lemma 2.6. We get the desired basis. ∎

(B) Lefschetz thimbles

For each jj, we define a simply connected domain

(3.3) Wj:=kj{q:q=rζkwithr3}.W_{j}:=\mathbb{C}\setminus\cup_{k\neq j}\{q:q=r\zeta^{k}~{}\mbox{with}~{}r\geq 3\}.

For qWjq\in W_{j}, let γ\gamma be a smooth curve joint qq and 3ζj3\zeta^{j} contained in WjW_{j}. Let VjE0V_{j}\subset E_{0} be the representatives described in (A). Then the Lefschetz thimble of VjV_{j} along γ\gamma, which is denoted by Γjγ(q)\Gamma^{\gamma}_{j}(q), is the union of the parallel transport of VjV_{j} along the cycle γ\gamma. Precisely,

(3.4) Γjγ(q):=qγVj(q),\Gamma^{\gamma}_{j}(q):=\cup_{q^{\prime}\in\gamma}V_{j}^{(q^{\prime})},

where Vj(q)V_{j}^{(q^{\prime})} is the parallel transport of VjV_{j} along any curve in WjW_{j} connecting 0 and qq and then from qq to qq^{\prime} along γ\gamma.

We shall mention that different representatives V~j\tilde{V}_{j} give different Lefschetz thimbles Γ~jγ(q)\tilde{\Gamma}^{\gamma}_{j}(q) and also that the Lefschetz thimble does depend on the choice of the curve connecting 0 and qq. One proves that in any case their difference is a coboundary. Consequently, by Stokes’ theorem, the integral

(3.5) Γjγ(q)Ωˇ\int_{\Gamma^{\gamma}_{j}(q)}\check{\Omega}

is independent of the choice of the representatives and the curve connecting 0 and qq. However, it is defined only up to a sign because of the orientation.

Refer to caption
Figure 4. The orientation of the cycles. The oriented line segments γ0\vec{\gamma}_{0}, γ1\vec{\gamma}_{1}, and γ2\vec{\gamma}_{2} defined in (3.7) are the oriented line segments AO\overrightarrow{AO}, BO\overrightarrow{BO} and CO\overrightarrow{CO}. For other notation, see the paragraph (D).

(C) Orientations

Recall that δj\delta_{j} is an oriented arc with orientation drawn in Figure 2. From (2.2), we can solve

(3.6) t2±=((qt1)±(qt1)24/t1)/2.t_{2}^{\pm}=\left((q-t_{1})\pm\sqrt{(q-t_{1})^{2}-4/t_{1}}\right)/2.

The orientation of V0V_{0} is chosen in the following manner. First we note that V0V_{0} is set-theoretically equal to the union of the graph of the holomorphic functions t2+t_{2}^{+} and t2t_{2}^{-} along the arc δ0\delta_{0} defined in (3.6). For the graph of t2t_{2}^{-}, we take the induced orientation from δ0\delta_{0}. For the graph of t2+t_{2}^{+}, we shall take the induced orientation from δ0-\delta_{0}. This pins down an orientation of VjV_{j}.

For each jj, let

(3.7) γj:={q:q=rζj,0r3}\vec{\gamma}_{j}:=\left\{q\colon q=r\zeta^{j},~{}0\leq r\leq 3\right\}

be an oriented (from 3ζj3\zeta^{j} towards 0) line segment (consult Figure 4).

We denote by Γjγj(0)\vec{\Gamma}_{j}^{\gamma_{j}}(0) the Lefschetz thimble Γjγj(0)\Gamma_{j}^{\gamma_{j}}(0) with the induced orientation from the S1S^{1}-bundle structure. Precisely, when restricting on {q:q=rζj,0r<3}\{q\colon q=r\zeta^{j},~{}0\leq r<3\}, Γjγj(0)\Gamma_{j}^{\gamma_{j}}(0) becomes an S1S^{1}-bundle whose fibers are equipped with an orientation coming from VjV_{j}. Therefore, it has an induced orientation which can be extended to the whole Γjγj(0)\Gamma_{j}^{\gamma_{j}}(0).

Remark 3.4.

It follows from the construction that the orientations for Γjγj(0)\vec{\Gamma}_{j}^{\gamma_{j}}(0) are compatible with the 3\mathbb{Z}_{3}-action.

Proposition 3.5.

We have, for all jj,

(3.8) Γjγj(0)ImΩˇ+.\int_{\vec{\Gamma}^{\gamma_{j}}_{j}(0)}\mathrm{Im}~{}\check{\Omega}\in\mathbb{R}_{+}.
Corollary 3.6.

We have

(3.9) limqImΓ0γ0(q)Ωˇ=.\lim_{q\to-\infty}\mathrm{Im}\int_{\vec{\Gamma}_{0}^{\gamma_{0}}(q)}\check{\Omega}=\infty.
Proof.

We defer the proofs of Proposition 3.5 and Corollary 3.6 in Appendix A. ∎

Once we pin down the orientation of V0V_{0}, the orientations of VjV_{j} are also uniquely determined. We then pick an integral basis {c,d}H1(E0,)\{c,d\}\subset\mathrm{H}_{1}(E_{0},\mathbb{Z}) such that the vanishing cycles [V0][V_{0}], [V1][V_{1}], and [V2][V_{2}] are represented by c2dc-2d, c+dc+d, and 2c+d-2c+d, respectively as in Lemma 3.3.

(D) Affine structures

We describe the affine structure on \mathbb{C} using the elliptic fibration Xˇ\check{X}\to\mathbb{C}. Consider the set

Ξ1:={q:ImΓ1γ(q)Ωˇ=0,γ:curve contained in {A,C} joining B and q}.\Xi_{1}:=\left\{q\in\mathbb{C}:\mathrm{Im}\int_{\Gamma_{1}^{\gamma}(q)}\check{\Omega}=0,~{}\gamma:\mbox{curve contained in $\mathbb{C}\setminus\{A,C\}$ joining $B$ and $q$}\right\}.

The condition that the imaginary part is equal to zero is independent of the choice of the curve γ\gamma since the monodromy matrices are real. The set Ξ1\Xi_{1} is well-defined. Notice that the set Ξ1{B}\Xi_{1}\setminus\{B\} has two connected components.

Working on the simply connected domain V=W1W2W3V=W_{1}\cap W_{2}\cap W_{3}, we can define the locus

lcd:={Γ1γ(q)Ωˇ+for any parameterized curve γV joining B and q}.l_{-c-d}:=\left\{\int_{\Gamma_{1}^{\gamma}(q)}\check{\Omega}\in\mathbb{R}_{+}~{}\mbox{for any parameterized curve $\gamma\subset V$ joining $B$ and $q$}\right\}.

Similarly we can define another curve l2c+dΞ2l_{-2c+d}\subset\Xi_{2} by requiring that

l2c+d:={Γ2γ(q)Ωˇfor any parameterized curve γV joining C and q}.l_{-2c+d}:=\left\{\int_{\Gamma_{2}^{\gamma}(q)}\check{\Omega}\in\mathbb{R}_{-}~{}\mbox{for any parameterized curve $\gamma\subset V$ joining $C$ and $q$}\right\}.
Remark 3.7.

The above definition explains the notation in Figure 4. However, we have not verified the validity of the intersection point v1v_{1} in Figure 4. We will prove that the curves O¯\overline{O\infty}, lcdl_{-c-d} and l2c+dl_{-2c+d} intersect at one point, where O¯\overline{O\infty} denotes the negative real axis.

We resume the notation given in this subsection and in Figure 4 and Figure 2 without recalling it. To describe the affine structure a little bit more, we need to study the integration over the Lefschetz thimbles.

Definition 3.8.

Let qO¯q\in\overline{O\infty}. We denote by σ0(q)\vec{\sigma}_{0}(q) the oriented curve OA¯Oq¯\overline{OA}\cup\overline{Oq} from AA toward qq, σ1(q)\vec{\sigma}_{1}(q) the oriented curve OB¯Oq¯\overline{OB}\cup\overline{Oq} from AA toward qq and by σ2(q)\vec{\sigma}_{2}(q) the oriented curve OC¯Oq¯\overline{OC}\cup\overline{Oq} from AA toward qq (cf. Figure 5).

For simplicity, we will write Γj(q):=Γjσj(q)(q)\Gamma_{j}(q):=\Gamma_{j}^{\vec{\sigma}_{j}(q)}(q) (see (3.4)), i.e., Γ0(q)\Gamma_{0}(q) is the Lefschetz thimble of the cycle V0V_{0} along σ0(q)\vec{\sigma}_{0}(q), Γ1(q)\Gamma_{1}(q) is the Lefschetz thimble of the cycle V1V_{1} along σ1(q)\vec{\sigma}_{1}(q) and Γ2(q)\Gamma_{2}(q) is the Lefschetz thimble of the cycle V2V_{2} along σ2(q)\vec{\sigma}_{2}(q).

Refer to caption
Figure 5. The curves σj(q)\sigma_{j}(q).
Lemma 3.9.

The map ϕ0(q)=q¯\phi_{0}(q)=\bar{q} fixing OO and AA but exchanging BB and CC is an automorphism of the affine structure.

Proof.

The affine lines are mapped to affine lines via ϕ0\phi_{0}. ∎

In particular, the lemma implies that the fixed locus of ϕ0\phi_{0}, an arc from AA to infinity passing through OO and another arc from AA to infinity without passing through OO, are affine lines.

Corollary 3.10.

The induced map (ϕ0):H1(E0,)H1(E0,)(\phi_{0})_{\ast}\colon\mathrm{H}_{1}(E_{0},\mathbb{Z})\to\mathrm{H}_{1}(E_{0},\mathbb{Z}) under the basis {c,d}\{c,d\} is given by

[1101].\begin{bmatrix}1&1\\ 0&-1\end{bmatrix}.
Proof.

Note that ϕ0\phi_{0} is the complex conjugation. We have (ϕ0)(c2d)=c+2d(\phi_{0})_{\ast}(c-2d)=-c+2d and (ϕ0)(c+d)=2cd(\phi_{0})_{\ast}(c+d)=2c-d by our choice of orientations, which yields the corollary. ∎

Lemma 3.11.

We have

Γ1(q)Γ2(q)Ωˇ,qO¯.\int_{\Gamma_{1}(q)-\Gamma_{2}(q)}\check{\Omega}\in\mathbb{R},~{}\forall~{}q\in\overline{O\infty}.
Proof.

The lemma is proved by using the 2\mathbb{Z}_{2}-symmetry ϕ0\phi_{0}. Since Γ1(q)Γ2(q)\Gamma_{1}(q)-\Gamma_{2}(q) is invariant under ϕ0\phi_{0}, we have

Γ1(q)Γ2(q)Ωˇ=(ϕ01)(Γ1(q)Γ2(q))ϕ0Ωˇ=Γ1(q)Γ2(q)Ωˇ¯\int_{\Gamma_{1}(q)-\Gamma_{2}(q)}\check{\Omega}=\int_{(\phi^{-1}_{0})_{\ast}(\Gamma_{1}(q)-\Gamma_{2}(q))}\phi_{0}^{\ast}\check{\Omega}=\int_{\Gamma_{1}(q)-\Gamma_{2}(q)}\overline{\check{\Omega}}

and the conclusion holds. ∎

We conclude this paragraph by proving the validity of the existence of the triple intersection point v1v_{1} in Figure 4. Let us write

(3.10) F1(q):=Γ1(q)ImΩˇ=Γ1(q)Γ1(0)ImΩˇ+Γ1(0)ImΩˇ=Γ1(q)Γ1(0)ImΩˇ+Γ0(0)ImΩˇ.\displaystyle\begin{split}F_{1}(q):=&\int_{\Gamma_{1}(q)}\mathrm{Im}~{}\check{\Omega}\\ =&\int_{\Gamma_{1}(q)-\Gamma_{1}(0)}\mathrm{Im}~{}\check{\Omega}+\int_{\Gamma_{1}(0)}\mathrm{Im}~{}\check{\Omega}\\ =&\int_{\Gamma_{1}(q)-\Gamma_{1}(0)}\mathrm{Im}~{}\check{\Omega}+\int_{\Gamma_{0}(0)}\mathrm{Im}~{}\check{\Omega}.\end{split}

The last equality in (3.10) holds by the 3\mathbb{Z}_{3}-symmetry on the qq-plane.

For q0q\leq 0,

(3.11) Γ1(q)Γ1(0)=qqO¯V1(q).\Gamma_{1}(q)-\Gamma_{1}(0)=\cup_{q^{\prime}\in\overline{qO}}~{}V_{1}^{(q^{\prime})}.

Consequently, utilizing Lemma 3.11 and the relation 2V1=V0(V2V1)2V_{1}=-V_{0}-(V_{2}-V_{1}), we get

(3.12) Γ1(q)Γ1(0)ImΩˇ=qqO¯V1(q)ImΩˇ=12Γ0(q)Γ0(0)ImΩˇ12Γ2(q)Γ1(q)ImΩˇ=12Γ0(q)Γ0(0)ImΩˇ,\displaystyle\begin{split}\int_{\Gamma_{1}(q)-\Gamma_{1}(0)}\mathrm{Im}~{}\check{\Omega}&=\int_{\cup_{q^{\prime}\in\overline{qO}}~{}V_{1}^{(q^{\prime})}}\mathrm{Im}~{}\check{\Omega}\\ &=-\frac{1}{2}\int_{\Gamma_{0}(q)-\Gamma_{0}(0)}\mathrm{Im}~{}\check{\Omega}-\frac{1}{2}\int_{\Gamma_{2}(q)-\Gamma_{1}(q)}\mathrm{Im}~{}\check{\Omega}\\ &=-\frac{1}{2}\int_{\Gamma_{0}(q)-\Gamma_{0}(0)}\mathrm{Im}~{}\check{\Omega},\end{split}

where the last equality comes from (3.11). Then (3.10) is transformed into

F1(q)=12Γ0(q)ImΩˇ+32Γ0(0)ImΩˇ,forq0.F_{1}(q)=-\frac{1}{2}\int_{\Gamma_{0}(q)}\mathrm{Im}~{}\check{\Omega}+\frac{3}{2}\int_{\Gamma_{0}(0)}\mathrm{Im}~{}\check{\Omega},~{}\mbox{for}~{}q\leq 0.

From Corollary 3.6, we see that F1(q)F_{1}(q)\to-\infty when qq\to-\infty. Together with F1(0)>0F_{1}(0)>0, there exists some v1O¯v_{1}\in\overline{O\infty} such that

F1(v1)=0.F_{1}(v_{1})=0.

Then v1v_{1} is the triple intersection point we are looking for.

3.4. Proof of the Main Theorem

In this paragraph, we will identify the affine manifold with singularities BSYZB_{\mathrm{SYZ}} with BCPSB_{\mathrm{CPS}}. Recall that the base BSYZB_{\mathrm{SYZ}} of the special Lagrangian fibration for 2E\mathbb{P}^{2}\setminus E can be topologically identified with \mathbb{C} and BCPSB_{\mathrm{CPS}} is the affine manifolds constructed in [CPS]. (See §3.1.) We will prove the following main theorem.

Theorem 3.12.

There exists an affine isomorphism between BSYZB_{\mathrm{SYZ}} and BCPSB_{\mathrm{CPS}}.

The affine manifold BSYZB_{\mathrm{SYZ}} has three singularities at AA, BB and CC. Let us study their monodromies in more detail.

Lemma 3.13.

Assume that the vanishing cycle has class pc+qdH1(E0,)pc+qd\in\mathrm{H}_{1}(E_{0},\mathbb{Z}). Then the counter-clockwise monodromy across the branch cut is

[1+pqp2q21pq]\begin{bmatrix}1+pq&-p^{2}\\ q^{2}&1-pq\end{bmatrix}

with respect to the basis {c,d}\{c,d\}.

Proof.

From Picard–Lefschetz formula, the counterclockwise monodromy is given by

(3.13) T(v)=v+δ,vδ\mathrm{T}(v)=v+\langle\delta,v\rangle\delta

where δ\delta is the vanishing cycle and vH1(E0,)v\in\mathrm{H}_{1}(E_{0},\mathbb{Z}). We can compute

{T(c)=c+pc+qd,c(pc+qd)=(1pq)c+q2dT(d)=d+pc+qd,d(pc+qd)=p2c+(1pq)d.\begin{cases}\mathrm{T}(c)=c+\langle pc+qd,c\rangle(pc+qd)=(1-pq)c+q^{2}d\\ \mathrm{T}(d)=d+\langle pc+qd,d\rangle(pc+qd)=-p^{2}c+(1-pq)d.\end{cases}

Notice that the monodromy is conjugate to

[1101]\begin{bmatrix}1&1\\ 0&1\end{bmatrix}

and the vanishing cycle pc+qdpc+qd is invariant under the monodromy. ∎

Corollary 3.14.

The monodromies acting on H1(E0,)\mathrm{H}_{1}(E_{0},\mathbb{Z}) with respect to the basis {c,d}\{c,d\} around AA, BB and CC are given by

(3.14) [1143],[2110]and[1413].\begin{bmatrix}-1&-1\\ 4&3\end{bmatrix},\begin{bmatrix}2&-1\\ 1&0\end{bmatrix}~{}\mbox{and}~{}\begin{bmatrix}-1&4\\ 1&3\end{bmatrix}.
Proof.

Recall that from Lemma 3.3 the vanishing cycles associated with the degenerate fibers AA, BB and CC are given by c2dc-2d, c+dc+d and 2c+d-2c+d. The corollary directly follows from Lemma 3.13. ∎

To write down the affine structure, one needs to introduce one branch cut from each of the three singularities to infinity. Recall that B0=BSYZ{A,B,C}B_{0}=B_{\mathrm{SYZ}}\setminus\{A,B,C\}. Let us fix a reference point uB0u\in B_{0}. Given a loop on the base, the affine monodromies act on TuB0T_{u}B_{0} while the monodromies of the fibration act on H1(Eu,)TuB0\mathrm{H}_{1}(E_{u},\mathbb{Z})\cong T^{\ast}_{u}B_{0}. Therefore, the clockwise affine monodromy action is dual to the counter-clockwise monodromy of the fibration. In particular, the matrix representation of the counter-clockwise monodromy around AA, BB and CC with respect to the dual basis {c,d}\{c,d\} are given by

(3.15) [1143],[2110]and[1413]\begin{bmatrix}-1&-1\\ 4&3\end{bmatrix}^{\intercal},\begin{bmatrix}2&-1\\ 1&0\end{bmatrix}^{\intercal}~{}\mbox{and}~{}\begin{bmatrix}-1&4\\ 1&3\end{bmatrix}^{\intercal}

from Corollary 3.14 .

To compare to BCPSB_{\mathrm{CPS}}, we have further requirements on the branch cuts.

Lemma 3.15.

There exists an affine ray emanating from each of the three singularities such that its tangent is in the monodromy invariant direction at infinity.

Proof.

We will explain the cut emanating from AA and the other two are similar. From Lemma 3.9 and Corollary 3.10, the set {3<q<}\{3<q<\infty\} is an affine line defined by c=(V2V1)/3-c=(V_{2}-V_{1})/3 and the cycle invariant under ϕ0\phi_{0}, which is the vanishing cycle at the infinity by Lemma 2.6 and Lemma 3.3. ∎

Proof of Theorem 3.12.

To match the affine structure on BSYZB_{\mathrm{SYZ}} with BCPSB_{\mathrm{CPS}}, we will take the branch cuts to be the affine rays in Lemma 3.15. Notice that the orientations of vanishing cycles V0,V1,V2V_{0},V_{1},V_{2} are chosen as in Lemma 2.6 and Lemma 3.3 so that they respect the 3\mathbb{Z}_{3}-symmetry on the qq-plane.

Recall we have the identification H1(E0,)cd\mathrm{H}_{1}(E_{0},\mathbb{Z})\cong\mathbb{Z}c\oplus\mathbb{Z}d from Lemma 3.3. We can identify A,B,CBSYZA,B,C\in B_{\mathrm{SYZ}} with A,B,CBCPSA^{\prime},B^{\prime},C^{\prime}\in B_{\mathrm{CPS}} and v1,v2,v3Bv_{1},v_{2},v_{3}\in B with v1,v2,v3v_{1}^{\prime},v_{2}^{\prime},v_{3}^{\prime}. There is an induced affine isomorphism carrying the affine triangle v1v2v3v_{1}v_{2}v_{3} in BSYZB_{\mathrm{SYZ}} to v1v2v3v_{1}^{\prime}v_{2}^{\prime}v_{3}^{\prime} in BCPSB_{\mathrm{CPS}}. Since the affine transformation acrossing the cut in BSYZB_{\mathrm{SYZ}} and BCPSB_{\mathrm{CPS}} are the same from (3.2) and (3.15), the affine isomorphisms glue to an affine isomorphism BSYZBCPSB_{\mathrm{SYZ}}\cong B_{\mathrm{CPS}}. ∎

4. Floer-theoretical gluing construction of mirror geometry

In the previous section, we have well understood the affine structure associated to the special Lagrangian fibration on 2E\mathbb{P}^{2}\setminus E, where EE is a smooth elliptic curve. In this section, we construct the Floer theoretical mirror of 2\mathbb{P}^{2} relative to EE, which is a direct application of the gluing method developed in [CHL-glue, HKL].

The strategy is the following. The special Lagrangian fibration has exactly three singular fibers. Each of these is a nodal torus pinched at one point. However, these singular fibers are located in different energy levels, in the sense that the pseudo-isomorphisms between their formal deformations involve Novikov parameter. The resulting mirror would be defined over Λ\Lambda.

To simplify the situation, we take the following Lagrangians instead of the special Lagrangian fibers. We take a monotone moment-map fiber of 2\mathbb{P}^{2}, and use symplectic reduction by 𝕊1\mathbb{S}^{1} to construct three monotone immersed Lagrangians, which play the role of the above three singular fibers. We consider the weakly unobstructed deformation spaces of these Lagrangians, and glue them together via quasi-isomorphisms in the Fukaya category.

Using these monotone Lagrangians, the gluing relations will be defined over \mathbb{C}, and hence we can reduce to a \mathbb{C}-valued mirror. Moreover, the construction of [CHL-glue] produces a mirror functor from the Fukaya category to the mirror matrix factorization category Fuk(2)MF(Xˇ,W~)\mathrm{Fuk}(\mathbb{P}^{2})\to\mathrm{MF}(\check{X}_{\mathbb{C}},\tilde{W}), which induces a derived equivalence [CHL-toric].

4.1. The Lagrangian objects

Let 𝐋0\mathbf{L}_{0} be the monotone moment-map torus fiber of 2\mathbb{P}^{2} equipped with the toric Kähler form, whose fan is generated by e1,e2e_{1},e_{2} and e3=e1e2e_{3}=-e_{1}-e_{2}, where {e1,e2}𝔱π1(𝐋0)\{e_{1},e_{2}\}\subset\mathfrak{t}\cong\pi_{1}(\mathbf{L}_{0}) is the standard basis. Consider flat connections on 𝐋0\mathbf{L}_{0}, whose holonomies along the loops e1,e2π1(𝐋0)e_{1},e_{2}\in\pi_{1}(\mathbf{L}_{0}) are given by z1,z2z_{1},z_{2} respectively. Let z3=1/z1z2z_{3}=1/z_{1}z_{2} which is the holonomy along e3e_{3}. Denote these flat connections by (z1,z2)\nabla^{(z_{1},z_{2})}.

The flat connections over a Lagrangian are taken over Λ0\Lambda_{0}, with holonomies ziΛ0×z_{i}\in\Lambda_{0}^{\times}, where

Λ0:={i=0ai𝐓Aiai,Ai0 and increases to +}\Lambda_{0}:=\left\{\sum_{i=0}^{\infty}a_{i}\mathbf{T}^{A_{i}}\mid a_{i}\in\mathbb{C},A_{i}\geq 0\textrm{ and increases to }+\infty\right\}

is the Novikov ring, and

Λ0×:={i=0ai𝐓AiΛ0A0=0 and a00}\Lambda_{0}^{\times}:=\left\{\sum_{i=0}^{\infty}a_{i}\mathbf{T}^{A_{i}}\in\Lambda_{0}\mid A_{0}=0\textrm{ and }a_{0}\not=0\right\}

is the group of invertible elements. This ensures the Floer theory for the Lagrangian decorated by a flat connection is convergent over Λ\Lambda.

Following [A], we can ‘push in’ one of the corners of the moment map polytope. Namely, let (i)2\mathbb{C}^{2}_{(i)} be the standard coordinate charts and X(i),Y(i)X^{(i)},Y^{(i)} the corresponding inhomogeneous coordinates for i=0,1,2i=0,1,2. Denote the T2T^{2}-moment map by

μ:2𝔱 with μ1({0})=𝐋0.\mu:\mathbb{P}^{2}\to\mathfrak{t}^{*}\textrm{ with }\mu^{-1}(\{0\})=\mathbf{L}_{0}.

Here the toric Kähler form is taken such that the moment map image is the triangle with vertices (1,1),(1,2),(2,1)(-1,-1),(-1,2),(2,-1) (in the basis {e1,e2}𝔱\{e_{1}^{\vee},e_{2}^{\vee}\}\subset\mathfrak{t}^{*}).

Consider the 𝕊1\mathbb{S}^{1}-action in each direction ei+2ei+1e_{i+2}-e_{i+1} (where the subscript is mod 3). The corresponding moment map is (μ,ei+2ei+1)(\mu,e_{i+2}-e_{i+1}). Moreover, the function X(i)Y(i)X^{(i)}\cdot Y^{(i)} is invariant under this 𝕊1\mathbb{S}^{1}-action and gives a complex coordinate ζ=ζ(i)\zeta=\zeta^{(i)} on the reduced space (i)2𝕊ei+2ei+11\mathbb{C}^{2}_{(i)}\sslash\mathbb{S}^{1}_{e_{i+2}-e_{i+1}}. Using this symplectic reduction, one obtains the following Lagrangian torus fibration.

Proposition 4.1 ([Gross-eg, Goldstein]).

For any cc\in\mathbb{C}, ((μ,ei+2ei+1),|X(i)Y(i)c|)((\mu,e_{i+2}-e_{i+1}),|X^{(i)}\cdot Y^{(i)}-c|) defines a Lagrangian fibration on (i)2=2DiT\mathbb{C}^{2}_{(i)}=\mathbb{P}^{2}-D^{T}_{i} where DiTD^{T}_{i} is the toric divisor corresponding to eie_{i}.

When c=0c=0, this is just isomorphic to the Lagrangian fibration given by the moment map.

We shall take the following Lagrangian objects. In the reduced space (i)2𝕊ei+2ei+11\mathbb{C}^{2}_{(i)}\sslash\mathbb{S}^{1}_{e_{i+2}-e_{i+1}}, 𝐋0\mathbf{L}_{0} is given by a circle of radius r>0r>0 centered at ζ=0\zeta=0. Moreover (μ,ei+2ei+1)=0(\mu,e_{i+2}-e_{i+1})=0 for 𝐋0\mathbf{L}_{0}. For each i=1,2,3i=1,2,3, we take

𝐋i:={|X(i)Y(i)r|=r,(μ,ei+2ei+1)=0}2\mathbf{L}_{i}:=\{|X^{(i)}\cdot Y^{(i)}-r|=r,(\mu,e_{i+2}-e_{i+1})=0\}\subset\mathbb{P}^{2}

which is the singular fiber of the above Lagrangian fibration (for c=r>0c=r>0). 𝐋i\mathbf{L}_{i} is an immersed two-sphere with a single nodal point. We denote the immersion by ιi:𝕊22\iota_{i}:\mathbb{S}^{2}\to\mathbb{P}^{2} whose image is 𝐋i\mathbf{L}_{i}.

For each i=1,2,3i=1,2,3, we also have the Chekanov torus

𝐋i:={|X(i)Y(i)(3r/2)|=r,(μ,ei+2ei+1)=0}2.\mathbf{L}_{i}^{\prime}:=\{|X^{(i)}\cdot Y^{(i)}-(3r/2)|=r,(\mu,e_{i+2}-e_{i+1})=0\}\subset\mathbb{P}^{2}.

See Figure 6.

Refer to caption
Figure 6. The images of the Lagrangians in the reduced space.
Proposition 4.2.

For tt sufficiently small, the Lagrangians 𝐋i\mathbf{L}_{i} and 𝐋i\mathbf{L}_{i}^{\prime} lie in 2Et\mathbb{P}^{2}-E_{t} where Et={xyz+t(x3+y3+z3)=0}2E_{t}=\{xyz+t(x^{3}+y^{3}+z^{3})=0\}\subset\mathbb{P}^{2}.

Proof.

EtE_{t} lies in a neighborhood of the union of toric divisors xyz=0xyz=0. After intersecting with the moment-map level set {(μ,ei+2ei+1)=0}\{(\mu,e_{i+2}-e_{i+1})=0\}, it is a compact set whose image in {}1\mathbb{C}\cup\{\infty\}\cong\mathbb{P}^{1} under X(i)Y(i)X^{(i)}\cdot Y^{(i)} consists of two connected components, one is a compact simply connected region near 0 (but does not contain 0), and one is a compact neighborhood of \infty. For tt small, these two regions are disjoint from the base circles of 𝐋i\mathbf{L}_{i} and 𝐋i\mathbf{L}_{i}^{\prime}. ∎

As explained above, we have the flat connections (z1,z2)\nabla^{(z_{1},z_{2})} on 𝐋0\mathbf{L}_{0}. Now we parametrize the flat connections on the Chekanov tori 𝐋i\mathbf{L}_{i}^{\prime} by fixing the following trivialization of the conic fibrations.

The conic fibration of X(i)Y(i)X^{(i)}\cdot Y^{(i)} restricted to (i)2{Y(i)=0}\mathbb{C}^{2}_{(i)}-\{Y^{(i)}=0\} is trivial, and Y(i)×Y^{(i)}\in\mathbb{C}^{\times} serves as the fiber coordinate. The map

((X(i)Y(i)3r/4)/|X(i)Y(i)3r/4|,Y(i)/|Y(i)|)((X^{(i)}Y^{(i)}-3r/4)/|X^{(i)}Y^{(i)}-3r/4|,Y^{(i)}/|Y^{(i)}|)

gives an identification of 𝐋0\mathbf{L}_{0} and 𝐋i\mathbf{L}_{i}^{\prime} with T2T^{2}. Thus e1,e2,e3π1(𝐋0)e_{1},e_{2},e_{3}\in\pi_{1}(\mathbf{L}_{0}) can be identified as elements in π1(𝐋i)\pi_{1}(\mathbf{L}_{i}^{\prime}).

Let’s denote the holonomy of a flat connection over 𝐋i\mathbf{L}_{i}^{\prime} along ei+1e_{i+1} by zi+1z_{i+1}^{\prime}, and that along the monodromy invariant direction (ei+2ei+1)(e_{i+2}-e_{i+1}) by wi+1w_{i+1}^{\prime}. We shall consider the objects (𝐋i,(zi+1,wi+1))\left(\mathbf{L}_{i}^{\prime},\nabla^{(z_{i+1}^{\prime},w_{i+1}^{\prime})}\right). For 𝐋0\mathbf{L}_{0}, the holonomy of a flat connection along (ei+2ei+1)(e_{i+2}-e_{i+1}) is denoted by wi+1w_{i+1}, which equals to zi+2zi+11z_{i+2}z_{i+1}^{-1}.

In conclusion, we shall consider the objects (𝐋0,(z1,z2)),(𝐋i,(zi+1,wi+1))(\mathbf{L}_{0},\nabla^{(z_{1},z_{2})}),\left(\mathbf{L}_{i}^{\prime},\nabla^{(z_{i+1}^{\prime},w_{i+1}^{\prime})}\right) , and the Lagrangian immersions 𝐋i\mathbf{L}_{i} for i=1,2,3i=1,2,3.

4.2. The Floer theoretical mirror

We construct a mirror out of the objects 𝐋0\mathbf{L}_{0} and 𝐋i\mathbf{L}_{i}. This gives a nice application of the gluing method in [CHL, HKL].

We take a Morse model for the Lagrangian Floer theory. Pearl trajectories, which are formed by holomorphic discs components together with gradient flow lines of a fixed Morse function, were developed in [Oh, BC] for the deformation theory of monotone Lagrangians. In [FOOO-can], the Morse model was developed to general situations using a homotopy between the Morse complex and the singular chain complex. There is also a slightly different formulation in [CW]. Such a Morse model was further developed to apply to a GG-equivariant setting in [LZ, HKLZ]. Fixing the choice of a Morse function ff on a Lagrangian LL and perturbation datum for the pearl trajectories, an AA_{\infty} structure {mk:k0}\{m_{k}:k\in\mathbb{Z}_{\geq 0}\} is constructed on the space of chains (L)\mathcal{F}(L) generated by critical points of ff. Moreover, given a degree-one chain b1(L)b\in\mathcal{F}^{1}(L), one has the deformed AA_{\infty} structure {mkb:k0}\{m_{k}^{b}:k\in\mathbb{Z}_{\geq 0}\} [FOOO-T1]. LL can also be decorated by flat connections \nabla, which produce {mk(L,):k0}\{m_{k}^{(L,\nabla)}:k\in\mathbb{Z}_{\geq 0}\}.

The holomorphic discs bounded by the torus 𝐋02\mathbf{L}_{0}\subset\mathbb{P}^{2} were known due to the classification by [CO]. Moreover, (𝐋0,(z1,z2))(\mathbf{L}_{0},\nabla^{(z_{1},z_{2})}) are weakly unobstructed [FOOO-T1], namely,

m0(𝐋0,(z1,z2))=W𝟏𝐋0m_{0}^{(\mathbf{L}_{0},\nabla^{(z_{1},z_{2})})}=W\cdot\mathbf{1}_{\mathbf{L}_{0}}

where 𝟏𝐋0\mathbf{1}_{\mathbf{L}_{0}} is the unit. The disc potential is given by

W=TA/3(z1+z2+1z1z2)=TA/3(z1+z2+z3)W=T^{A/3}\left(z_{1}+z_{2}+\frac{1}{z_{1}z_{2}}\right)=T^{A/3}\left(z_{1}+z_{2}+z_{3}\right)

where AA is the area of the line class in 2\mathbb{P}^{2}.

For the grading of the Lagrangians, for each i=1,2,3i=1,2,3, we consider the anti-canonical divisor

Di:={X(i)Y(i)=3r/4}{z(i)=0}D_{i}:=\{X^{(i)}Y^{(i)}=3r/4\}\cup\{z^{(i)}=0\}

(where z(i)z^{(i)} is the homogeneous coordinate that defines the toric divisor DiT={z(i)=0}D_{i}^{T}=\{z^{(i)}=0\}).

Lemma 4.3.

𝐋0\mathbf{L}_{0}, 𝐋i\mathbf{L}_{i} and 𝐋i\mathbf{L}_{i}^{\prime} are graded Lagrangians in the complement 2Di\mathbb{P}^{2}-D_{i}.

Proof.

𝐋0\mathbf{L}_{0}, 𝐋i\mathbf{L}_{i} and 𝐋i\mathbf{L}_{i}^{\prime} are isotopic to special Lagrangian fibers with respect to the holomorphic volume form dX(i)dY(i)/(X(i)Y(i)3r/4)dX^{(i)}\wedge dY^{(i)}/(X^{(i)}Y^{(i)}-3r/4) defined on 2Di\mathbb{P}^{2}-D_{i}, and hence they are graded. ∎

Then the Maslov index formula of [CO, A] can be applied and one has the following.

Proposition 4.4 ([CO, A]).

The Maslov index of a disc β\beta bounded by 𝐋0,𝐋i,𝐋i\mathbf{L}_{0},\mathbf{L}_{i},\mathbf{L}_{i}^{\prime} equals to μ(β)=2βDi.\mu(\beta)=2\,\beta\cdot D_{i}.

Now we fix a choice of Morse functions on the Lagrangians. In above we have fixed an identification of 𝐋0\mathbf{L}_{0} and 𝐋i\mathbf{L}_{i}^{\prime} with the standard T2T^{2}. Let’s take a perfect Morse function on T2T^{2} such that the unstable circles of the two degree-one critical points are dual to the 𝕊1\mathbb{S}^{1}-orbits in the directions of e1e_{1} and e2e_{2} respectively. By abuse of notation, we also denote these two degree-one critical points by e1,e2e_{1},e_{2}. The maximum and minimum points are denoted by 𝟏\mathbf{1} and e12e_{12} respectively.

For the immersed Lagrangians 𝐋i\mathbf{L}_{i}, the choice of Morse functions is more subtle and we proceed as follows. First, consider the immersed generators for the Floer theory. The domain of the immersion is 𝕊2\mathbb{S}^{2}. The inverse image of the transverse self-nodal point consists of two points q1,q2𝕊2q_{1},q_{2}\in\mathbb{S}^{2}. The branch jumps q1q2q_{1}\to q_{2} and q2q1q_{2}\to q_{1} are denoted by UiU_{i} and ViV_{i} respectively. See Figure 6. By using the grading in Lemma 4.3, it is easy to see the following.

Lemma 4.5.

Both Ui,ViCF(𝐋i,𝐋i)U_{i},V_{i}\in\mathrm{CF}(\mathbf{L}_{i},\mathbf{L}_{i}) have deg=1\deg=1.

We use Ui,ViU_{i},V_{i} for the Maurer-Cartan deformations of 𝐋i\mathbf{L}_{i}. By using a 2\mathbb{Z}_{2}-symmetry, they can be shown to be unobstructed:

Lemma 4.6 ([HKL]*Lemma 3.3).

uiUi+viViCF(𝐋i,𝐋i)u_{i}U_{i}+v_{i}V_{i}\in\mathrm{CF}(\mathbf{L}_{i},\mathbf{L}_{i}) are bounding cochains for 𝐋i2Di\mathbf{L}_{i}\subset\mathbb{P}^{2}-D_{i}, namely, m0uiUi+viVi=0m_{0}^{u_{i}U_{i}+v_{i}V_{i}}=0, where

(ui,vi)Λ02{val(uivi)=0}.(u_{i},v_{i})\in\Lambda_{0}^{2}-\{\textrm{val}\,(u_{i}v_{i})=0\}.

It is important to take val(uivi)>0\textrm{val}\,(u_{i}v_{i})>0, since there are constant polygons at the nodal point (whose number of UiU_{i} corners must equal to the number of ViV_{i} corners to go back to the same branch) contributing to the Floer theory of 𝐋i\mathbf{L}_{i}. This ensures Novikov convergence of m0uiUi+viVim_{0}^{u_{i}U_{i}+v_{i}V_{i}}.

We construct isomorphisms between (𝐋0,(z1,z2))(\mathbf{L}_{0},\nabla^{(z_{1},z_{2})}) and (𝐋i,uiUi+viVi)(\mathbf{L}_{i},u_{i}U_{i}+v_{i}V_{i}) under suitable gluing relations between (z1,z2)(z_{1},z_{2}) and (ui,vi)(u_{i},v_{i}). Observe that 𝐋i\mathbf{L}_{i} intersects cleanly with 𝐋0\mathbf{L}_{0} (or 𝐋i\mathbf{L}_{i}^{\prime}) at two circle fibers (α,β)(\alpha,\beta) (or (α,β)(\alpha^{\prime},\beta^{\prime})) over the two intersection points of the base loci |ζ|=r|\zeta|=r and |ζr|=r|\zeta-r|=r (or |ζ3r/2|=r|\zeta-3r/2|=r) in the ζ\zeta-plane. Similarly, 𝐋0\mathbf{L}_{0} intersects with 𝐋i\mathbf{L}_{i}^{\prime} at two circles (α′′,β′′)(\alpha^{\prime\prime},\beta^{\prime\prime}). We fix a perfect Morse function on each of these circles. The maximum and minimum points are denoted by α𝟏,α𝐦\alpha\otimes\mathbf{1},\alpha\otimes\mathbf{m} respectively (and similar for β,α,β,α′′,β′′\beta,\alpha^{\prime},\beta^{\prime},\alpha^{\prime\prime},\beta^{\prime\prime}, where 𝐦\mathbf{m} stands for ‘minimum’).

CF(𝐋i,𝐋0)=SpanΛ{α𝟏,α𝐦,β𝟏,β𝐦}\mathrm{CF}(\mathbf{L}_{i},\mathbf{L}_{0})=\mathrm{Span}_{\Lambda}\{\alpha\otimes\mathbf{1},\alpha\otimes\mathbf{m},\beta\otimes\mathbf{1},\beta\otimes\mathbf{m}\}

which have degrees 0,1,1,20,1,1,2 respectively. We can also regard them as generators of CF(𝐋0,𝐋i)\mathrm{CF}(\mathbf{L}_{0},\mathbf{L}_{i}), and they have degrees 1,2,0,11,2,0,1 respectively.

By the projection to the complex ζ\zeta-plane, one can deduce the following (see [HKL]*Section 3.3), which is important for computing m1𝐋i,𝐋0(α𝟏)m_{1}^{\mathbf{L}_{i},\mathbf{L}_{0}}(\alpha\otimes\mathbf{1}) and m1𝐋i,𝐋i(α𝟏)m_{1}^{\mathbf{L}_{i}^{\prime},\mathbf{L}_{i}}(\alpha^{\prime}\otimes\mathbf{1}).

Lemma 4.7.

In 2Di\mathbb{P}^{2}-D_{i}, 𝐋i\mathbf{L}_{i} and 𝐋0\mathbf{L}_{0} (or similarly 𝐋i\mathbf{L}_{i} and 𝐋i\mathbf{L}_{i}^{\prime}) bound exactly two non-constant Maslov-two holomorphic polygons that have output to β𝟏\beta\otimes\mathbf{1} (or β𝟏\beta^{\prime}\otimes\mathbf{1}). One of them has corners at α,β\alpha,\beta (or α,β\alpha^{\prime},\beta^{\prime}). The other has corners at α,β,V\alpha,\beta,V (or α,β,U\alpha^{\prime},\beta^{\prime},U).

The Morse function on 𝐋i\mathbf{L}_{i} that we choose is the following. The boundaries of the above two holomorphic polygons in 𝐋i\mathbf{L}_{i} give two curved segments. We take a perfect Morse function on the domain 𝕊2\mathbb{S}^{2} of 𝐋i\mathbf{L}_{i} such that the two critical points lie in 𝕊2{q1,q2}\mathbb{S}^{2}-\{q_{1},q_{2}\}, and the two flow lines connecting q1,q2q_{1},q_{2} to the minimum are distinct and do not intersect with any of these curve segments.

Then we have the following isomorphisms between the Lagrangian branes.

Theorem 4.8.

α𝟏CF((𝐋0,(z1,z2)),(𝐋i,uiUi+viVi))\alpha\otimes\mathbf{1}\in\mathrm{CF}((\mathbf{L}_{0},\nabla^{(z_{1},z_{2})}),(\mathbf{L}_{i},u_{i}U_{i}+v_{i}V_{i})) is an isomorphism if and only if vi=zi+11v_{i}=z_{i+1}^{-1} and uivi=1+zi1zi+12u_{i}v_{i}=1+z_{i}^{-1}z_{i+1}^{-2} where the subscripts are mod 3.

Proof.

Fix i=1,2,3i=1,2,3. First we consider α′′𝟏CF((𝐋0,(zi+1,wi+1)),(𝐋i,(zi+1,wi+1)))\alpha^{\prime\prime}\otimes\mathbf{1}\in\mathrm{CF}((\mathbf{L}_{0},\nabla^{(z_{i+1},w_{i+1})}),(\mathbf{L}_{i}^{\prime},\nabla^{(z_{i+1}^{\prime},w_{i+1}^{\prime})})) between the tori. m1,u(α′′𝟏)m_{1,u}(\alpha^{\prime\prime}\otimes\mathbf{1}) has degree deg(α′′𝟏)+1μ(u)0\deg(\alpha^{\prime\prime}\otimes\mathbf{1})+1-\mu(u)\geq 0 where μ(u)\mu(u) is the Chern-Weil Maslov index of the strip class uu. Since α′′𝟏\alpha^{\prime\prime}\otimes\mathbf{1} has degree zero and the minimal Maslov index for 𝐋0\mathbf{L}_{0} and 𝐋i\mathbf{L}_{i} is zero, m1(α′′𝟏)m_{1}(\alpha^{\prime\prime}\otimes\mathbf{1}) is merely contributed by strips with Chern-Weil Maslov index zero. We have μ(u)=2uDi\mu(u)=2u\cdot D_{i}. Thus any uu which contributes to m1(α′′𝟏)m_{1}(\alpha^{\prime\prime}\otimes\mathbf{1}) does not intersect with DiD_{i}. We have

m1(α′′𝟏)=(1wi+1wi+11)α′′𝐦+(1+wi+1zi+1zi+11s)β′′𝟏m_{1}(\alpha^{\prime\prime}\otimes\mathbf{1})=(1-w_{i+1}^{\prime}w_{i+1}^{-1})\alpha^{\prime\prime}\otimes\mathbf{m}+(1+w_{i+1}-z_{i+1}^{\prime}z_{i+1}^{-1}s)\beta^{\prime\prime}\otimes\mathbf{1}

where the first term is contributed by the two flow lines from α′′𝟏\alpha^{\prime\prime}\otimes\mathbf{1} to α′′𝐦\alpha^{\prime\prime}\otimes\mathbf{m}, and the second term is contributed from the holomorphic strips from α′′𝟏\alpha^{\prime\prime}\otimes\mathbf{1} to β′′𝟏\beta^{\prime\prime}\otimes\mathbf{1} [Seidel, PT, HKL]. Hence the cocycle condition m1(α′′𝟏)=0m_{1}(\alpha^{\prime\prime}\otimes\mathbf{1})=0 implies wi+1=wi+1=zi+11zi+2=zi1zi+12w_{i+1}^{\prime}=w_{i+1}=z_{i+1}^{-1}z_{i+2}=z_{i}^{-1}z_{i+1}^{-2} and zi+1=zi+1(1+wi+1)z_{i+1}^{\prime}=z_{i+1}(1+w_{i+1}). Moreover, the strips also give m2(β′′×𝟏,α′′×𝟏)=𝟏𝐋0m_{2}(\beta^{\prime\prime}\times\mathbf{1},\alpha^{\prime\prime}\times\mathbf{1})=\mathbf{1}_{\mathbf{L}_{0}} and m2(α′′×𝟏,β′′×𝟏)=𝟏𝐋im_{2}(\alpha^{\prime\prime}\times\mathbf{1},\beta^{\prime\prime}\times\mathbf{1})=\mathbf{1}_{\mathbf{L}_{i}^{\prime}}. Thus α′′×𝟏\alpha^{\prime\prime}\times\mathbf{1} is an isomorphism if and only if the above relations hold.

Now we consider m1(α𝟏)m_{1}(\alpha\otimes\mathbf{1}) and m1(α𝟏)m_{1}(\alpha^{\prime}\otimes\mathbf{1}). We have

m1(α𝟏)=\displaystyle m_{1}(\alpha\otimes\mathbf{1})= (uizi+1)β𝟏+(wi+1f(uivi))α𝐦\displaystyle(u_{i}-z_{i+1}^{\prime})\beta\otimes\mathbf{1}+(w_{i+1}-f(u_{i}v_{i}))\alpha\otimes\mathbf{m}
m1(α𝟏)=\displaystyle m_{1}(\alpha^{\prime}\otimes\mathbf{1})= (vizi+11)β𝟏+(wi+1g(uivi))α𝐦\displaystyle(v_{i}-z_{i+1}^{-1})\beta^{\prime}\otimes\mathbf{1}+(w_{i+1}^{\prime}-g(u_{i}v_{i}))\alpha\otimes\mathbf{m}

for some series ff and gg. Requiring them to be zero implies ui=zi+1u_{i}=z_{i+1}^{\prime}, vi=zi+11v_{i}=z_{i+1}^{-1}, wi+1=f(uivi),wi+1=g(uivi)w_{i+1}=f(u_{i}v_{i}),w_{i+1}^{\prime}=g(u_{i}v_{i}). It easily follows that α\alpha and α\alpha^{\prime} are isomorphisms under the above relations.

Since m2(α,α)=α′′m_{2}(\alpha,\alpha^{\prime})=\alpha^{\prime\prime}, α′′𝟏\alpha^{\prime\prime}\otimes\mathbf{1} is also an isomorphism under the above relations. Thus wi+1=wi+1=zi1zi+12w_{i+1}^{\prime}=w_{i+1}=z_{i}^{-1}z_{i+1}^{-2} and zi+1=zi+1(1+wi+1)z_{i+1}^{\prime}=z_{i+1}(1+w_{i+1}), implying f(uivi)=g(uivi)f(u_{i}v_{i})=g(u_{i}v_{i}) and uivi=1+wi+1u_{i}v_{i}=1+w_{i+1}. Result follows. ∎

According to the above theorem, the formal deformation spaces of 𝐋0\mathbf{L}_{0} and 𝐋i\mathbf{L}_{i} for i=1,2,3i=1,2,3 are glued by the transitions vi=zi+11v_{i}=z_{i+1}^{-1} and uivi=1+zizi+12u_{i}v_{i}=1+z_{i}z_{i+1}^{2}. We denote the resulting space by Xˇ\check{X}. It consists of the chart (Λ0×)2(\Lambda_{0}^{\times})^{2} coming from the torus 𝐋0\mathbf{L}_{0}, and the charts (Λ02)(i){val(uivi)=0}(\Lambda_{0}^{2})_{(i)}-\{\textrm{val}\,(u_{i}v_{i})=0\} coming from the immersed sphere 𝐋i\mathbf{L}_{i} for i=1,2,3i=1,2,3.

Xˇ\check{X} is defined over Λ\Lambda. On the other hand, note that the transition functions do not involve the Novikov parameter 𝐓\mathbf{T}. This is because the base circles of 𝐋0\mathbf{L}_{0}, 𝐋i\mathbf{L}_{i} and 𝐋i\mathbf{L}_{i}^{\prime} in the reduced space are taken to be the same size, so that the symplectic areas of strips are the same. The \mathbb{C}-valued part of Xˇ\check{X} is denoted by Xˇ\check{X}_{\mathbb{C}}, which is the union of the \mathbb{C}-valued parts of the charts of Xˇ\check{X}.

Remark 4.9.

The \mathbb{C}-valued part of the chart (Λ02)(i){val(uivi)=0}(\Lambda_{0}^{2})_{(i)}-\{\textrm{val}\,(u_{i}v_{i})=0\} of the immersed Lagrangian 𝐋i\mathbf{L}_{i} is the singular conic

{(ui,vi)2:uivi=0}={(ui,0):ui×}{(0,vi):vi×}{(0,0)}\{(u_{i},v_{i})\in\mathbb{C}^{2}:u_{i}v_{i}=0\}=\{(u_{i},0):u_{i}\in\mathbb{C}^{\times}\}\cup\{(0,v_{i}):v_{i}\in\mathbb{C}^{\times}\}\cup\{(0,0)\}

whose valuation is {(0,+)}{(+,0)}{(+,+)}\{(0,+\infty)\}\cup\{(+\infty,0)\}\cup\{(+\infty,+\infty)\}. Note that this subset is disconnected under the non-Archimedian topology. Moreover, the \mathbb{C}-valued part of the gluing region with the torus chart (×)2(Λ0×)2(\mathbb{C}^{\times})^{2}\subset(\Lambda_{0}^{\times})^{2} is {(0,vi):vi×}\{(0,v_{i}):v_{i}\in\mathbb{C}^{\times}\}. This is not of the correct complex dimension. Thus we first work over Λ\Lambda to construct the mirror, and then we can restrict to \mathbb{C} to get the \mathbb{C}-valued mirror.

Remark 4.10.

In the above Floer theoretical construction, the mirror is simply glued from one torus chart (×)2(\mathbb{C}^{\times})^{2} and three charts coming from immersed spheres. On the other hand, the corresponding cluster variety consists of infinitely many torus charts.

4.3. Identification with the Carl–Pomperla–Siebert mirror

Now we show that the resulting geometry from the above construction agrees with the Carl–Pomperla–Siebert mirror. This gives Theorem 1.3.

Proposition 4.11.

Xˇ\check{X}_{\mathbb{C}} is the blowing up at three points in the three toric divisors of the toric variety whose fan has the rays generated by (2,1),(1,2)(2,-1),(-1,2) and (1,1)(-1,-1), with the strict transform of the toric divisors removed. W=z1+z2+1z1z2W_{\mathbb{C}}=z_{1}+z_{2}+\frac{1}{z_{1}z_{2}} on (×)2(\mathbb{C}^{\times})^{2} extends to be a proper elliptic fibration on Xˇ\check{X}_{\mathbb{C}} with three I1I_{1}-fibers.

Proof.

The blowing up of the toric chart (V)×(Z)×\mathbb{C}_{(V)}\times\mathbb{C}^{\times}_{(Z)} at (V,Z)=(0,1)(V,Z)=(0,-1) has local charts (U,V)2{UV=1}\mathbb{C}^{2}_{(U,V)}-\{UV=1\} and (V~,Z~)2{Z~=1}\mathbb{C}^{2}_{(\tilde{V},\tilde{Z})}-\{\tilde{Z}=1\} with the change of coordinates V=V~Z~V=\tilde{V}\tilde{Z} and U=V~1U=\tilde{V}^{-1} (where Z~=Z+1\tilde{Z}=Z+1). The strict transform of the toric divisor {V=0}(V)×(Z)×\{V=0\}\subset\mathbb{C}_{(V)}\times\mathbb{C}^{\times}_{(Z)} is given by V~=0\tilde{V}=0, and its complement in the blowing-up is identified with the chart uivi=1+zi1zi+12u_{i}v_{i}=1+z_{i}^{-1}z_{i+1}^{-2} of Xˇ\check{X}_{\mathbb{C}} via Z~=1+zi1zi+12\tilde{Z}=1+z_{i}^{-1}z_{i+1}^{-2}, U=uiU=u_{i}, V=viV=v_{i}. The open torus orbit (V)××(Z)×\mathbb{C}^{\times}_{(V)}\times\mathbb{C}^{\times}_{(Z)} is identified with the torus chart of 𝐋0\mathbf{L}_{0} by V=zi+11V=z_{i+1}^{-1} and Z=zi1zi+12Z=z_{i}^{-1}z_{i+1}^{-2}. This gives the identification between Xˇ\check{X}_{\mathbb{C}} and the blowing-up.

We already know that WW on (×)(z1,z2)2(\mathbb{C}^{\times})^{2}_{(z_{1},z_{2})} gives a fibration whose generic fibers are three-punctured elliptic curves. WW has three critical values, whose fibers are 3-punctured A1A_{1} singular fibers. Below, we see that the partial compactification by the immersed charts (i)2{uivi=1}\mathbb{C}^{2}_{(i)}-\{u_{i}v_{i}=1\} exactly fill in the punctures in all elliptic fibers.

Consider a fiber W=cW=c for cc\in\mathbb{C}. For the chart (i)2{uivi=1}\mathbb{C}^{2}_{(i)}-\{u_{i}v_{i}=1\}, uivi=1+zi+11zi+2u_{i}v_{i}=1+z_{i+1}^{-1}z_{i+2}. Thus zi+2=(uivi1)zi+1=(uivi1)vi1=uivi1z_{i+2}=(u_{i}v_{i}-1)z_{i+1}=(u_{i}v_{i}-1)v_{i}^{-1}=u_{i}-v_{i}^{-1}. Then

W=zi+1+zi+2+1zi+1zi+2=ui+vi2(uivi1)1W=z_{i+1}+z_{i+2}+\frac{1}{z_{i+1}z_{i+2}}=u_{i}+v_{i}^{2}(u_{i}v_{i}-1)^{-1}

in the chart. The fiber is given by

ui(uivi1)+vi2=c(uivi1).u_{i}(u_{i}v_{i}-1)+v_{i}^{2}=c(u_{i}v_{i}-1).

The partial compactification coming from this chart is vi=0v_{i}=0. Thus it adds the point (ui,vi)=(c,0)(u_{i},v_{i})=(c,0) to the fiber. In other words, the coordinate axes vi=0v_{i}=0 are sections of the fibration of WW. The partial compactification adds in these three sections which are exactly the union of three punctures of the elliptic fibers. ∎

We note that the meromorphic functions uiu_{i} for i=1,2,3i=1,2,3 satisfy the following explicit equation.

Proposition 4.12.
(u13+u23+u33)+2u1u2u3i=13(u12u2+u1u22)=0.(u_{1}^{3}+u_{2}^{3}+u_{3}^{3})+2u_{1}u_{2}u_{3}-\sum_{i=1}^{3}(u_{1}^{2}u_{2}+u_{1}u_{2}^{2})=0.
Proof.

We have

(4.1) z0z1z2=1.z_{0}z_{1}z_{2}=1.

Moreover,

(4.2) ui=zi+1(1+zi+11zi+2)=zi+1+zi+2.u_{i}=z_{i+1}(1+z_{i+1}^{-1}z_{i+2})=z_{i+1}+z_{i+2}.

We compute ui3u_{i}^{3}, ui2ui+1,uiui+12u_{i}^{2}u_{i+1},u_{i}u_{i+1}^{2} and u1u2u3u_{1}u_{2}u_{3} using (4.2). It turns out the variables z0,z1,z2z_{0},z_{1},z_{2} can all be eliminated and we obtain the resulting equation.

Appendix A The proof of Proposition 3.5

We resume the notation introduced in §3. Abusing the notation, for q{rζj:r3}q\in\{r\zeta^{j}:r\leq 3\}, let γj\gamma_{j} be the line segment connecting qq and 3ζj3\zeta^{j} and Γjγj(q)\Gamma_{j}^{\gamma_{j}}(q) to denote the set-theoretic union

(A.1) qγjVj(q).\bigcup_{q^{\prime}\in\gamma_{j}}V_{j}^{(q^{\prime})}.

We also denote by γj\vec{\gamma}_{j} the line segment γj\gamma_{j} equipped with an orientation from 3ζj3\zeta^{j} towards to qq and by Γjγj(q)\vec{\Gamma}_{j}^{\gamma_{j}}(q) the set Γjγj(q)\Gamma_{j}^{\gamma_{j}}(q) with the induced orientation as in . The integral

(A.2) Γjγj(q)Ωˇ\int_{\vec{\Gamma}_{j}^{\gamma_{j}}(q)}\check{\Omega}

becomes a function in qWjq\in W_{j}. For simplicity, we put

(A.3) G(q):=Γ0γ0(q)Ωˇ,whereq(,3].G(q):=\int_{\vec{\Gamma}_{0}^{\gamma_{0}}(q)}\check{\Omega},~{}\mbox{where}~{}q\in(-\infty,3]\subset\mathbb{C}.

Proposition 3.5 is an immediate consequence of the following lemma.

Lemma A.1.
Γ0γ0(q)Ωˇ1+forq(,3].\int_{\vec{\Gamma}_{0}^{\gamma_{0}}(q)}\check{\Omega}\in\sqrt{-1}\mathbb{R}_{+}~{}\mbox{for}~{}q\in(-\infty,3].
Proof.

Using Ωˇ\check{\Omega} is d\mathrm{d}-closed and independent of qq, we compute

dG(q)dq=Γ0γ0(q)ιqΩˇ.\displaystyle\begin{split}\frac{\mathrm{d}G(q)}{\mathrm{d}q}&=\int_{\partial\vec{\Gamma}_{0}^{\gamma_{0}}(q)}\iota_{\frac{\partial}{\partial q}}\check{\Omega}.\end{split}

From the construction, Γ0γ0(q)\partial\vec{\Gamma}_{0}^{\gamma_{0}}(q) is equal to V0(q)V_{0}^{(q)} as oriented cycles.

Recall that Eq()2:={(t1,t2)()2:t1+t2+(t1t2)1=q}E_{q}\cap(\mathbb{C}^{\ast})^{2}:=\left\{(t_{1},t_{2})\in(\mathbb{C}^{\ast})^{2}\colon t_{1}+t_{2}+(t_{1}t_{2})^{-1}=q\right\}. Let δ0(q)\delta_{0}(q) be the image of V0(q)V_{0}^{(q)} under the projection

(A.4) ()2,(t1,t2)t1.(\mathbb{C}^{\ast})^{2}\to\mathbb{C}^{\ast},~{}(t_{1},t_{2})\mapsto t_{1}.

For q(,3]q\in(-\infty,3], Eq()2E_{q}\cap(\mathbb{C}^{\ast})^{2}\to\mathbb{C}^{\ast} admits three ramifications: only one of them lies on the real axis and the other two are symmetric with respect to the real axis, denoted by xx and x¯\bar{x}. Here we assume that Im(x)>0\mathrm{Im}(x)>0. xx and x¯\bar{x} are connected through δ0(q)\delta_{0}(q). We equip δ0(q)\delta_{0}(q) with an orientation going from xx to x¯\bar{x}. Note that δ0(0)δ0\delta_{0}(0)\equiv\delta_{0} as oriented cycles.

We can write Γ0γ0(q)=V0(q)=Γ+(q)Γ(q)\partial\vec{\Gamma}_{0}^{\gamma_{0}}(q)=V_{0}^{(q)}=\partial\Gamma^{+}(q)\cup\partial\Gamma^{-}(q), union of the graph of t2+t_{2}^{+} and the graph of t2t_{2}^{-} along δ0(q)\delta_{0}(q) as in the paragraph (C). Then

dG(q)dq\displaystyle\frac{\mathrm{d}G(q)}{\mathrm{d}q} =Γ0γ0(q)ιqΩˇ\displaystyle=\int_{\partial\vec{\Gamma}_{0}^{\gamma_{0}}(q)}\iota_{\frac{\partial}{\partial q}}\check{\Omega}
=Γ+(q)ιqΩˇ+Γ(q)ιqΩˇ\displaystyle=\int_{\partial\Gamma^{+}(q)}\iota_{\frac{\partial}{\partial q}}\check{\Omega}+\int_{\partial\Gamma^{-}(q)}\iota_{\frac{\partial}{\partial q}}\check{\Omega}
(A.5) =δ0(q)1(qt1)24/t1dt1t1+δ0(q)1(qt1)24/t1dt1t1.\displaystyle=\int_{\delta_{0}(q)}\frac{\sqrt{-1}}{\sqrt{(q-t_{1})^{2}-4/t_{1}}}\frac{\mathrm{d}t_{1}}{t_{1}}+\int_{-\delta_{0}(q)}\frac{-\sqrt{-1}}{\sqrt{(q-t_{1})^{2}-4/t_{1}}}\frac{\mathrm{d}t_{1}}{t_{1}}.

We explain the third equality above. Restricting on Γ+(q)\partial\Gamma^{+}(q) or Γ(q)\partial\Gamma^{-}(q) and making use of the equation t12t2+t1t22+1=qt1t2t_{1}^{2}t_{2}+t_{1}t_{2}^{2}+1=qt_{1}t_{2}, we obtain

(A.6) ιqΩˇ|Γ±(q)=1t2±qt1t2±t12t2±2t1(t2±)2dt1=11qt12t2±dt1t1.\displaystyle\begin{split}\left.\iota_{\frac{\partial}{\partial q}}\check{\Omega}\right|_{\partial\Gamma^{\pm}(q)}&=\sqrt{-1}\cdot\frac{t_{2}^{\pm}}{q\cdot t_{1}t_{2}^{\pm}-t_{1}^{2}t_{2}^{\pm}-2t_{1}(t_{2}^{\pm})^{2}}\mathrm{d}t_{1}\\ &=\sqrt{-1}\cdot\frac{1}{q-t_{1}-2t_{2}^{\pm}}\frac{\mathrm{d}t_{1}}{t_{1}}.\end{split}

Also from (3.6), we see that

(A.7) 2t2±+t1q=±(qt1)24/t1.2t_{2}^{\pm}+t_{1}-q=\pm\sqrt{(q-t_{1})^{2}-4/t_{1}}.

Together with the induced orientation on Γ±(q)\partial\Gamma^{\pm}(q), we arrive at the desired equality. Note that the branched cut of z\sqrt{z} in (A.7) is chosen such that

z=exp(12logz),logz=r+1θwithθ[0,2π).\displaystyle\sqrt{z}=\exp\left(\frac{1}{2}{\log z}\right),~{}\log{z}=r+\sqrt{-1}\theta~{}\mbox{with}~{}\theta\in[0,2\pi).

Since both of the integrands in (A) are holomorphic, we can deform the cycle δ0(q)\delta_{0}(q) a little bit. We have the following two cases: (a) 0<q<30<q<3 and (b) q<0q<0.

For the case (a), we can deform δ0(q)\delta_{0}(q) into a circular arc δ0(q)\delta_{0}^{\prime}(q) joining the end points xx and x¯\bar{x} without touching the third ramification point yy, where the integrands have a pole (cf. Figure 7).

Refer to caption
Figure 7. The deformed contour δ0(q)\delta_{0}^{\prime}(q).

Moreover, on the circular arc, we have

(A.8) Im(qt1)24/t10.\mathrm{Im}~{}\sqrt{(q-t_{1})^{2}-4/t_{1}}\geq 0.

Therefore,

δ0(q)1(qt1)24/t1dt1t1\int_{\delta_{0}^{\prime}(q)}\frac{\sqrt{-1}}{\sqrt{(q-t_{1})^{2}-4/t_{1}}}\frac{\mathrm{d}t_{1}}{t_{1}}

has negative imaginary part and so does (A). This implies that the imaginary part of G(q)G(q) decreases.

For the case (b), we can deform δ0(q)\delta_{0}(q) into the contour δ0′′(q)\delta_{0}^{\prime\prime}(q) (cf. Figure 8).

Refer to caption
Figure 8. The deformed contour δ0′′(q)\delta_{0}^{\prime\prime}(q), which is the union of (I)(III)\mathrm{(I)}\sim\mathrm{(III)} and (I)(III)\mathrm{(I)}^{\prime}\sim\mathrm{(III)}^{\prime}.

By symmetry, it suffices to compute the integral over (I)(III)\mathrm{(I)}\sim\mathrm{(III)}. The equation (A.8) still holds for (I) and (III). On the contour (II), with the parameterization t1=1rt_{1}=\sqrt{-1}\cdot r,

(q1r)2+41r=q22qr1r2+41r=(q2r2)+1(4r2qr)\displaystyle\begin{split}(q-\sqrt{-1}r)^{2}+4\frac{\sqrt{-1}}{r}&=q^{2}-2qr\sqrt{-1}-r^{2}+\frac{4\sqrt{-1}}{r}\\ &=(q^{2}-r^{2})+\sqrt{-1}\left(\frac{4}{r}-2qr\right)\end{split}

has positive imaginary part if r>0r>0, which guarantees that (qt1)24/t1\sqrt{(q-t_{1})^{2}-4/t_{1}} has positive real part if r>0r>0. Also we have dt1/t1=dr/r\mathrm{d}t_{1}/t_{1}=\mathrm{d}r/r. These implies again that

(II)1(qt1)24/t1dt1t1\int_{\mathrm{(II)}}\frac{\sqrt{-1}}{\sqrt{(q-t_{1})^{2}-4/t_{1}}}\frac{\mathrm{d}t_{1}}{t_{1}}

has negative imaginary part.

We deduce from above that in both cases, (A) has negative imaginary parts. Together with the fact G(3)=0G(3)=0, it follows that G(q)1+G(q)\in\sqrt{-1}\cdot\mathbb{R}_{+} for q<3q<3. ∎

Corollary A.2.

We have G(0)1+G(0)\in\sqrt{-1}\cdot\mathbb{R}_{+}.

Proof.

This immediately follows from Lemma A.1. ∎

Corollary A.3.

limqG(q)=1\lim_{q\to-\infty}G(q)=\sqrt{-1}\cdot\infty.

Proof.

Assume q<0q<0. We adapt the notation in Figure 8. To compute the integral (A), as in the proof of Lemma A.1, we can deform the path δ0(q)\delta_{0}(q) to δ0′′(q)\delta_{0}^{\prime\prime}(q). We put r:=|x|r:=|x|.

Note that

1(qt1)24/t1dt1t1\frac{-\sqrt{-1}}{\sqrt{(q-t_{1})^{2}-4/t_{1}}}\frac{\mathrm{d}t_{1}}{t_{1}}

has negative imaginary part on the whole (II)\mathrm{(II)}. In particular, we have

(A.9) Imδ0′′(q)1(qt1)24/t1dt1t1Im𝒞1(qt1)24/t1dt1t1,\mathrm{Im}\int_{\delta_{0}^{\prime\prime}(q)}\frac{\sqrt{-1}}{\sqrt{(q-t_{1})^{2}-4/t_{1}}}\frac{\mathrm{d}t_{1}}{t_{1}}\leq\mathrm{Im}\int_{\mathcal{C}}\frac{\sqrt{-1}}{\sqrt{(q-t_{1})^{2}-4/t_{1}}}\frac{\mathrm{d}t_{1}}{t_{1}},

where 𝒞\mathcal{C} is the (clockwise oriented) contour

reiθwithθ[3π4,π2].re^{i\theta}~{}\mbox{with}~{}\theta\in\left[\frac{3\pi}{4},\frac{\pi}{2}\right].

It suffices to estimate the right hand side of (A.9). On 𝒞\mathcal{C}, we have

(A.10) (qt1)24/t1(qt1)2=q2(1rqeiθ)2(q-t_{1})^{2}-4/t_{1}\sim(q-t_{1})^{2}=q^{2}\left(1-\frac{r}{q}e^{i\theta}\right)^{2}

provided |q||q| is large enough. In the meanwhile, r/|q|1r/|q|\sim 1. It is not hard to see that

Im(1(qt1)24/t1)κ|q|,\mathrm{Im}\left(\frac{1}{\sqrt{(q-t_{1})^{2}-4/t_{1}}}\right)\geq\frac{\kappa}{|q|},

for some positive constant κ\kappa. Since 𝒞\mathcal{C} is clockwise oriented, we have

(A.11) Imδ0′′(q)1(qt1)24/t1dt1t1κlength(𝒞)|q|=:κ|q|.\mathrm{Im}\int_{\delta_{0}^{\prime\prime}(q)}\frac{\sqrt{-1}}{\sqrt{(q-t_{1})^{2}-4/t_{1}}}\frac{\mathrm{d}t_{1}}{t_{1}}\leq-\frac{\kappa\cdot\mathrm{length}(\mathcal{C})}{|q|}=:-\frac{\kappa^{\prime}}{|q|}.

This shows that

(A.12) d(ImG(q))dqκqfor allq0\frac{\mathrm{d}(\mathrm{Im}~{}G(q))}{\mathrm{d}q}\leq\frac{\kappa^{\prime}}{q}~{}\mbox{for all}~{}q\ll 0

and therefore limqImG(q)=\lim_{q\to-\infty}\mathrm{Im}~{}G(q)=\infty. ∎

References