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Tropicalization of the Mirror Curve near the Large Radius Limit

Zhaoxing Gu
(Date: December 2022)

Abstract

The mirror of a toric orbifold is an affine curve called the mirror curve. In this paper, firstly, we recall the basic tools in tropical geometry and give a definition of the mirror curve. Then we calculate the tropical spine of the mirror curve for a smooth toric Calabi-Yau 3-fold near the large radius limit. Finally, we recall a special kind of real algebraic curves called the cyclic-M curve and show that under some special choices of parameters near the large radius limit, the mirror curve is a cyclic-M curve. Applying Mikhalkin’s result[14] of cyclic-M curves, we show that the mirror curve is glued from tubes and pairs of pants.

1. Introduction

1.1. Backgrounds of the mirror curve

The mirror of a toric orbifold is an affine curve called the mirror curve. The mirror curve was studied in mirror symmetry by Hori and Vafa for toric Calabi-Yau 3-folds. Let (X,ω)(X,\omega) be a symplectic toric Calabi-Yau 3-fold. There exist three types of mirrors for (X,ω)(X,\omega): Landau-Ginzburg (Givental) mirror, Hori-Vafa mirror, and the mirror curve [11][9].

For the toric Calabi-Yau 3-fold (X,ω)(X,\omega), the mirror B-model is a 3-dimensional Landau-Ginzburg model on ()3(\mathbb{C^{*}})^{3} given by the superpotential

W=H(x,y,q)z.W=H(x,y,q)z.

Here H(x,y,q)=0H(x,y,q)=0 is an affine curve with the parameter qq related to the Kähler parameter of XX given by the mirror map. Another mirror, Hori-Vafa mirror of (X,ω)(X,\omega) is a non-compact Calabi-Yau 3-fold X~\tilde{X} with a holomorphic 3-form Ω\Omega on X~\tilde{X}, where X~\tilde{X} is a hypersurface in 2×()2\mathbb{C}^{2}\times(\mathbb{C^{*}})^{2}, given by

X~={(u,v,x,y)2×()2|uv=H(x,y)},\tilde{X}=\{(u,v,x,y)\in\mathbb{C}^{2}\times(\mathbb{C^{*}})^{2}|uv=H(x,y)\},

and

Ω=ResX~(1uvH(x,y)dudvdxxdyy).\Omega=Res_{\tilde{X}}(\frac{1}{uv-H(x,y)}du\wedge dv\wedge\frac{dx}{x}\wedge\frac{dy}{y}).

These two types of mirrors of a toric Calabi-Yau 3-fold (X,ω)(X,\omega) could be reduced to an affine curve

Cq={(x,y)()2|H(x,y,q)=0}C_{q}=\{(x,y)\in(\mathbb{C^{*}})^{2}|H(x,y,q)=0\}

with the Kähler parameter qq. We define the curve by the mirror curve.

The mirror curve could be used for the prediction of open-closed Gromov-Witten invariants. For example, in [6], the Eynard-Orantin topological recursion provides an algorithm for calculating higher genus invariants for a spectral curve. We can relate the Eynard-Orantin invariants ωg,n\omega_{g,n} of the mirror curve to all genus open-closed Gromov-Witten invariants of the symplectic toric Calabi-Yau 3-fold (X,ω)(X,\omega) by Bouchard-Klemm-Mariño-Pasquetti (BKMP) Remodeling Conjecture [3][4][11][7][6].

Besides, the statement of a version of homological mirror symmetry for a toric Calabi-Yau 3-fold is formulated via the mirror curve. Specifically, for a toric Calabi-Yau 3-fold, the B-model is the matrix factorization, while the A-model is a Fukaya-type category on its mirror curve [15] [1][13][2].

1.2. Main results

For a simplicial toric Calabi-Yau 3-fold XΣX_{\Sigma} defined by a 3-dim fan ΣN3\Sigma\subset N\cong\mathbb{Z}^{3}, all the generators of 1-dim cones lie in a hyperplane NNN^{\prime}\subset N, so a generator corresponds to a lattice point in NN^{\prime}. Thus Σ\Sigma gives a triangulation of Δ\Delta, where Δ\Delta is the convex hull of these lattice points given by 1-dim cones. We define such triangulation by TΣT_{\Sigma}. The first result is that the tropicalization of the mirror curve near the large radius limit gives a subdivision of 2\mathbb{R}^{2}. This subdivision is exactly dual to the triangulation TΣT_{\Sigma}.

Theorem (Theorem 3.4).

The subdivision TT given by the tropical spine is dual to the triangulation TΣT_{\Sigma} of Σ\Sigma near the large radius limit.

Besides, we recall propositions of a special kind of real algebraic curves determined by some Laurent polynomials namely cyclic-M curves in a real toric surface. This kind of curve has the maximal number of connected components in the corresponding real toric surface and intersects the axes of the toric surface in a cyclic order. Here the maximal number of connected components equals one plus the number of lattice points inside the Newton polytope of Laurent polynomial by Harnack’s inequality[10]. We give examples of a non-cyclic-M curve and a cyclic-M curve in Figure 2 and Figure 2.

Refer to caption
Figure 1. Non-cyclic-M curve: 1+x+y0.5x1y1=01+x+y-0.5x^{-1}y^{-1}=0
Refer to caption
Figure 2. cyclic-M curve: 1+x+y0.01x1y1=01+x+y-0.01x^{-1}y^{-1}=0

Mikhalkin has studied cyclic-M curves in manners of tropical geometry. In [14], he has proved the following statements about cyclic-M curves:

Proposition (Proposition 4.4).

Let pp be a Laurent polynomial with real coefficients and A={(x,y)()2|p(x,y)=0}A=\{(x,y)\in(\mathbb{C^{*}})^{2}|p(x,y)=0\}. If A=A()2\mathbb{R}A=A\cap(\mathbb{R^{*}})^{2} is a cyclic-M curve, we define FF to be the locus of critical points of μ|A\mu|_{A}, where μ\mu is the amoeba map. Then we have F=AF=\mathbb{R}A.

Proposition (Proposition 4.5).

Let pp be a Laurent polynomial with real coefficients and A={(x,y)()2|p(x,y)=0}A=\{(x,y)\in(\mathbb{C^{*}})^{2}|p(x,y)=0\}. If A\mathbb{R}A is a cyclic-M curve, then μ(A)=μ(A)\mu(\mathbb{R}A)=\partial\mu(A). Besides, the amoeba map μ\mu is an embedding on A\mathbb{R}A.

Theorem (Theorem 4.6).

Let pp be a Laurent polynomial with real coefficients and A={(x,y)()2|p(x,y)=0}A=\{(x,y)\in(\mathbb{C^{*}})^{2}|p(x,y)=0\}. If A=A()2\mathbb{R}A=A\cap(\mathbb{R^{*}})^{2} is a cyclic-M curve, the topological type of (XΔp;A,l1ln)(\mathbb{R}X_{\Delta_{p}};\mathbb{R}A,l_{1}\cup...\cup l_{n}) is uniquely determined by Δp\Delta_{p}.

The mirror curve is defined by a Laurent polynomial written as

H(x,y,q)=1+x+y+i=4p+3ai(q)xmiyni.H(x,y,q)=1+x+y+\sum\limits_{i=4}^{p+3}a_{i}(q)x^{m_{i}}y^{n_{i}}.

The second result about a mirror curve of a smooth toric Calabi-Yau 3-fold is that under special choices of real parameters, the mirror curve is a cyclic-M curve.

Corollary (Corollary 5.3.4).

Near the large radius limit, with ai(q)<0a_{i}(q)<0 when mi,nim_{i},n_{i} are both odd and ai(q)>0a_{i}(q)>0 when mim_{i} or nin_{i} is even, the mirror curve is a cyclic-M curve.

Finally, we apply Mikhalkin’s result to show the mirror curve of smooth toric Calabi-Yau 3-fold is glued from tubes and pairs of pants, which any vertex in the dual graph of TΣT_{\Sigma} corresponds to a pair of pants and any edge corresponds to a tube. This gluing determines the topology of the mirror curve.

1.3. Outline of the proof

We prove the results in several steps. Beginning in Section 2, we recall tropical geometry and give a definition of the mirror curve. For the first result, we mainly finish the proof by applying the method of tropical geometry. Specifically, in Section 2.6, we will see that generally for a Laurent polynomial of F(z1,,zn)F(z_{1},...,z_{n}), we could construct an injective map ψF\psi_{F} from the connected components of nAF\mathbb{R}^{n}-A_{F} to ΔFn\Delta_{F}\cap\mathbb{Z}^{n}. Then in Section 3, we prove that near the large radius limit, for the mirror curve H(x,y,q)=0H(x,y,q)=0 of a smooth toric Calabi-Yau 3-fold, the previous injective map ψH\psi_{H} is also surjective by constructing the preimage of any lattice point in ΔH\Delta_{H}. Also in Section 3, by introducing the notation of Ronkin function, we show the amoeba of a Laurent polynomial has a canonical deformation retract named tropical spine. Then near the large radius limit, we could calculate the tropical spine of a mirror curve concretely. Further, such a tropical spine gives a dual subdivision of TΣT_{\Sigma}. These steps lead to our first Theorem 3.4.

For the second result, we mainly finish the proof with some symmetry propositions of the distribution rules of coefficients for the mirror curve as given in Section 2.5. In Section 4, we recall Mikhalkin’s result about cyclic-M curves that if A\mathbb{R}A is a cyclic-M curve and AA is the zeroes of the Laurent polynomial pp in ()2(\mathbb{C^{*}})^{2}, then the amoeba map μA\mu_{A} is an embedding on the boundary of amoeba and 2-1 inside the amoeba. This fact explains why we hope the mirror curve is a cyclic-M curve. Because we have already known the deformation retract of a mirror curve’s amoeba, if the mirror curve is a cyclic-M curve, we could locally figure out the topology of the mirror curve. However, generally for the real parameters near the large radius limit, the mirror curve is not a cyclic-M curve. In Section 5, we first give the choice of signs for the parameters in Section 5.1 and explain the motivation for such a choice. Then in Section 5.2, we prove under such a choice of coefficients, any interior lattice point in Newton polytope ΔH\Delta_{H} corresponds to a unique bounded connected component of mirror curve in ()2(\mathbb{R}^{*})^{2}. Thus the mirror curve is an M-curve. Finally, in Section 5.3, we construct arcs connecting any two adjacent points of intersection of the unbounded component and axes of toric surface XΔp\mathbb{R}X_{\Delta_{p}} by the intermediate value theorem. Then we get Corollary 5.3.4.

1.4. Acknowledgement

I would sincerely appreciate my advisor for the undergraduate research Prof. Bohan Fang for his patient guidance and useful suggestions both on the project itself and further math research. I would also thank Prof. Shuai Guo for his frequent discussions with me about the project, his helpful advice, and for inviting me to give the report on such a research project. Besides, I would wish to thank Ce Ji, Kaitai He, Zhiyuan Zhang, Jialiang Lin, and Zhengnan Chen for their valuable discussions about the project. This project is partially supported by an undergraduate research grant at School of Mathematical Sciences, Peking University.

2. Preliminaries on toric varieties, mirror curves, and tropical geometry

In this section, we recall some results in toric variety and tropical geometry, then give the definition of mirror curve. We mainly follow the notation in [7], and we refer to [5][8] for general toric language.

2.1. Subdivision, dual subdivision

In this chapter, we mainly introduce some combinatorial languages which are used for the description of the mirror curve and its tropicalization. We follow the symbol of [16].

Definition 2.1.1.

For a convex set KK in n\mathbb{R}^{n}. A collection TT of nonempty closed convex subsets of KK is called a convex subdivision if it satisfies the following conditions:

  1. (1)

    The union of all sets in TT is equal to KK.

  2. (2)

    If σ\sigma, τT\tau\in T and στ\sigma\cap\tau is nonempty, then στT\sigma\cap\tau\in T

  3. (3)

    If σT\sigma\in T and τ\tau is any subset of σ\sigma, then τT\tau\in T if and only if τ\tau is a face of σ\sigma.

Here a face of a convex set σ\sigma means a set of the form {xσ|ξ,x=supyσξ,y}\{x\in\sigma|\langle\xi,x\rangle=sup_{y\in\sigma}\langle\xi,y\rangle\} for some ξn\xi\in\mathbb{R}^{n}. Since then, we write a subdivision short for a convex subdivision.

In a subdivision TT of KK, we call kk-dimensional subsets kk-cells. If KK is a convex polytope, and all cells of TT are convex polytopes, we call TT a polytopal subdivision. Besides, if TT is a subdivision of a 2-dimensional polytope Δ\Delta, and all 2-dimensional cells of TT are triangles, we call TT a triangulation.

If τσ\tau\subset\sigma, and τ,σ\tau,\sigma are both convex sets, we define the cone generated from τ\tau and σ\sigma by

cone(τ,σ)={t(xy)|xσ,yτ,t0}.cone(\tau,\sigma)=\{t(x-y)|x\in\sigma,y\in\tau,t\geq 0\}.

Clearly, this set is a convex cone. If C is a convex cone, its dual is defined to be the cone Cv={ξn|ξ,x0,xC}C^{v}=\{\xi\in\mathbb{R}^{n}|\langle\xi,x\rangle\leq 0,\forall x\in C\}. Then we will define dual subdivision.

Definition 2.1.2.

Let KK, K0K_{0} be convex sets in n\mathbb{R}^{n}, and let TT, T0T_{0} be convex subdivisions of KK, K0K_{0}. We say that TT and T0T_{0} are dual (to each other) if there exists a bijective map TT0T\to T_{0}, denoted σσ\sigma\to\sigma^{*}, satisfying the following conditions:

  1. (1)

    For σ,τT\sigma,\tau\in T, τσ\tau\subset\sigma if and only if στ\sigma^{*}\subset\tau^{*}

  2. (2)

    If τσ\tau\subset\sigma, then cone(τ,σ)cone(\tau,\sigma) is dual to cone(σ,τ)cone(\sigma^{*},\tau^{*})

Because cone(σ,σ)cone(\sigma,\sigma) is the affine space spanned by σ\sigma, we get σ\sigma and σ\sigma^{*} are orthogonal. Moreover, dim σ\sigma+dim σ=n\sigma^{*}=n. Figure 4 and Figure 4 show a subdivision of 2\mathbb{R}^{2} and its dual subdivision. The dual subdivision is an example of triangulation.

Refer to caption
Figure 3. Division of 2\mathbb{R}^{2}
Refer to caption
Figure 4. Dual Triangulation

2.2. Simplicial toric Calabi-Yau 3-fold and its fan

In this paper, we only consider the simplicial toric Calabi-Yau 3-fold XΣX_{\Sigma} given by a simplicial fan Σ\Sigma in a lattice N3N\cong\mathbb{Z}^{3}. For the convention, we denote Hom(N,)Hom(N,\mathbb{Z}) by MM, then M3M\cong\mathbb{Z}^{3} is also a lattice. We call MM the dual lattice of NN. Besides, by the definition of the toric Calabi-Yau 3-fold, the canonical divisor of XΣX_{\Sigma} is trivial.

It is known that there are two ways to define a general 3-dim toric variety. The first is to use homogeneous coordinates[5]. For any toric 3-fold XX, we could write

X=k+3S()k.X=\frac{\mathbb{C}^{k+3}-S}{(\mathbb{C^{*}})^{k}}.

Here SS is a fixed subset under the action of open dense complex torus ()3X(\mathbb{C}^{*})^{3}\subset X, and k \mathbb{C^{*}}-actions are given by

i:λ(z1,,zk+3)=(λTi,1z1,,λTi,k+3zk+3).\mathbb{C^{*}}_{i}:\lambda*(z_{1},...,z_{k+3})=(\lambda^{T_{i,1}}z_{1},...,\lambda^{T_{i,k+3}}z_{k+3}).

The coefficient matrix

T=(T1,1T1,k+3Tk,1Tk,k+3)T=\left(\begin{array}[]{ccc}T_{1,1}&...&T_{1,k+3}\\ ...&...&...\\ T_{k,1}&...&T_{k,k+3}\\ \end{array}\right)

is called the toric charge for XX. Under such definition, the equivalent description of Calabi-Yau condition is that the sum of elements in any fixed line equals zero, i.e.

XCalabi-Yaua=1k+3Ti,a=0i=1,2,,k.X\quad\text{Calabi-Yau}\Longleftrightarrow\sum\limits_{a=1}^{k+3}T_{i,a}=0\quad\forall i=1,2,...,k.

The second way to define a toric 3-fold is just the original definition given by a 3-dim simplicial fan ΣN3\Sigma\subset N\cong\mathbb{Z}^{3} [8]. For a toric 3-fold XΣX_{\Sigma} which corresponds to the fan Σ\Sigma, we define the d-dimensional cones in Σ\Sigma by Σ(d)\Sigma(d). For the convention, we always write Σ(1)={ρ1,,ρk+3}\Sigma(1)=\{\rho_{1},...,\rho_{k+3}\}, where k+3k+3 is the number of 1-dimensional cones in Σ\Sigma. Besides, we denote the generator of ρi\rho_{i} by bib_{i}.

By definition, XΣX_{\Sigma} contains 𝕋=N()3\mathbb{T}=N\bigotimes\mathbb{C^{*}}\cong(\mathbb{C^{*}})^{3} as an open dense subset. The natural action of 𝕋\mathbb{T} on itself could be extended to XΣX_{\Sigma}. The lattice NN could also be canonically identified with Hom(,𝕋)Hom(\mathbb{C}^{*},\mathbb{T}). NN is so called cocharacter lattice of 𝕋\mathbb{T}. M=Hom(𝕋,)M=Hom(\mathbb{T},\mathbb{C}^{*}) is called the character lattice.

If we define N~=i=1k+3bi~\tilde{N}=\bigoplus\limits_{i=1}^{k+3}\mathbb{Z}\tilde{b_{i}}, then we have a natural group homomorphism ψ:N~N\psi:\tilde{N}\to N, which sends bi~\tilde{b_{i}} to bib_{i}. We denote the kernel of ψ\psi by LL, then we get the exact sequence

0LψN~ϕN0.0\to L\stackrel{{\scriptstyle\psi}}{{\to}}\tilde{N}\stackrel{{\scriptstyle\phi}}{{\to}}N\to 0.

Tensoring \mathbb{C}^{*} in the exact sequence, we have the exact sequence

1GΣ𝕋~𝕋1,1\to G_{\Sigma}\to\tilde{\mathbb{T}}\to\mathbb{T}\to 1,

where 𝕋~()k+3\tilde{\mathbb{T}}\cong(\mathbb{C}^{*})^{k+3} has an action on itself. We extend the action to k+3=\mathbb{C}^{k+3}=Spec [Z1,\mathbb{C}[Z_{1}, ,Z3+k]...,Z_{3+k}]. For any σΣ\sigma\in\Sigma, we consider Zσ=ρiσZiZ_{\sigma}=\prod\limits_{\rho_{i}\notin\sigma}Z_{i}, define Z(Σ)Z(\Sigma) to be the closed subvariety defined by the ideal generated by {Zσ|σΣ}\{Z_{\sigma}|\sigma\in\Sigma\}. Then XΣX_{\Sigma} could be identified with the geometric quotient 3+kZ(Σ)/GΣ\mathbb{C}^{3+k}-Z(\Sigma)/G_{\Sigma}. This is the relation between the two definitions.

Calabi-Yau condition also has a great description under the second definition. The description is that XX Calabi-Yau iff all bib_{i} lie in a hyperplane of NN, or equivalently, there exists a vector e3Me_{3}^{*}\in M which makes e3,bi=1\langle e_{3}^{*},b_{i}\rangle=1 for any i=1,,k+3i=1,...,k+3. Now we choose e1,e2e_{1}^{*},e_{2}^{*} which make {e1,e2,e3}\{e_{1}^{*},e_{2}^{*},e_{3}^{*}\} a basis of MM. Then under the dual basis {e1,e2,e3}\{e_{1},e_{2},e_{3}\}, bib_{i} has the coordinate (mi,ni,1)(m_{i},n_{i},1) in the lattice NN. Since then, we always identify the generator of any 1-dimensional cone bib_{i} with a lattice point (mi,ni)(m_{i},n_{i}) in NN^{\prime}.

For the convention, we define the Calabi-Yau subtorus 𝕋\mathbb{T^{\prime}} of 𝕋\mathbb{T} that

𝕋=ker(e3:𝕋)()2.\mathbb{T^{\prime}}=ker(e_{3}^{*}:\mathbb{T}\to\mathbb{C})\cong(\mathbb{C^{*}})^{2}.

Then N=ker(e3:NZ)N^{\prime}=ker(e_{3}^{*}:N\to Z) could be identified with Hom(,𝕋)Hom(\mathbb{C^{*}},\mathbb{T^{\prime}}). We define PΣNP_{\Sigma}\subset N^{\prime} the convex hull of (mi,ni)(m_{i},n_{i}). Then PΣP_{\Sigma} is a 2-dim convex polytope. The simplicial fan Σ\Sigma also gives a triangulation of PΣP_{\Sigma}. For any σΣ(3)\sigma\in\Sigma(3), σN\sigma\cap N^{\prime} is a triangle. Then a subdivision TΣT_{\Sigma} is given by all these triangles and their faces. Since then, we always use a triangulation TΣT_{\Sigma} to represent a simplicial toric Calabi-Yau 3-fold.

For a general triangulation TΣT_{\Sigma}, XΣX_{\Sigma} is a toric orbifold. In [12], the author introduced the extended stacky fan to deal with the such orbifold case. Mirror curves are also generally defined for simplicial toric Calabi-Yau 3-folds. However, in this paper, we only consider the smooth toric manifold case. Because XΣX_{\Sigma} is smooth iff any cone of Σ\Sigma forms a \mathbb{Z}-basis of NN, since then we assume any triangle in TΣT_{\Sigma} has area 12\frac{1}{2}. In other words, triangulation TΣT_{\Sigma} is the finest. Figure 5 shows a finest triangulation.

Refer to caption
Figure 5. Finest Division

2.3. Toric surface associated to a 2-dimension convex polytope

The mirror curve which we will give a detailed definition later is a complex curve in ()2(\mathbb{C^{*}})^{2} as well as a punctured Riemann surface, which is given by a complex Laurent polynomial in two variables with the parameter qq. Sometimes, we need to compactify it on the toric surface defined by Newton polytope of the polynomial to get a smooth Riemann surface and consider genus or real connected components on the toric surface instead of ()2(\mathbb{C^{*}})^{2} or ()2(\mathbb{R^{*}})^{2}. So in this chapter, we review the definition and some basic facts about the toric surface.

Firstly, we follow the definition in Fulton’s book[8]. Let Δ\Delta be a convex polytope in MM_{\mathbb{R}} with integer vertices A1,A2,,AkA_{1},A_{2},...,A_{k} in counterclockwise order and {Δi=AiAi+1,i=1,2,,k}\{\Delta_{i}=A_{i}A_{i+1},i=1,2,...,k\} be k sides of Δ\Delta, where A1=Ak+1A_{1}=A_{k+1}. For any face of Δ\Delta, specifically, all segments, vertices, and the polytope itself (the first two are called proper faces), we consider their dual cones. If ΔP\Delta_{P} is a face of Δ\Delta, the dual cone σP={vN|v,u1v,u2\sigma_{P}=\{v\in N_{\mathbb{R}}|\langle v,u_{1}\rangle\geq\langle v,u_{2}\rangle, for any u1ΔP,u2Δ}u_{1}\in\Delta_{P},u_{2}\in\Delta\}. It is easy to see that all dual cones form a fan in NN_{\mathbb{R}}. Then the fan defines a 22-dimensional toric variety XΔX_{\Delta}, we called this variety the toric surface associated with convex polytope Δ\Delta. XΔX_{\Delta} contains ()2(\mathbb{C^{*}})^{2} as an open dense subset.

Next we move on to the real toric surface XΔ\mathbb{R}{X_{\Delta}}, which is the closure of ()2(\mathbb{R^{*}})^{2} in XΔX_{\Delta}. For a non-singular algebraic curve on a toric surface XΔX_{\Delta} whose Newton polytope coincides with the polytope Δ\Delta, we could show the genus g of such a curve equals the number of interior lattice points of the Newton polytope by calculating the dimension of global differential forms on the curve[7]. By Harnack’s inequality [10], there are at most g+1 connected components of the curve on the real toric surface.

A more concrete and useful description of the toric surface is given in [7]. Let Δ1\Delta_{1}, …, Δn\Delta_{n} be the sides of the polytope Δ\Delta. We take the dual 1-dimensional cone ρi\rho_{i} of each Δi\Delta_{i}. For ρi=0bi\rho_{i}=\mathbb{Z}_{\geq 0}b_{i}, considering N~=i=1nbi~\tilde{N}=\bigoplus\limits_{i=1}^{n}\mathbb{Z}\tilde{b_{i}} and the natural map ψ:N~N\psi:\tilde{N}\to N, which sends bi~\tilde{b_{i}} to bib_{i}, we have the exact sequence:

0LN~ψN0.\displaystyle 0\to L\to\tilde{N}\stackrel{{\scriptstyle\psi}}{{\to}}N\to 0.

Tensoring \mathbb{C}^{*} on the exact sequence, we have

1GΔ()n()21.\displaystyle 1\to G_{\Delta}\to(\mathbb{C}^{*})^{n}\to(\mathbb{C}^{*})^{2}\to 1.

GΔG_{\Delta} has a natural action on ()n(\mathbb{C}^{*})^{n}. We could extend the action to n\mathbb{C}^{n}. Then we define XΔ=n/GΔX_{\Delta}=\mathbb{C}^{n}/G_{\Delta} by the toric surface, with the open dense subset ()n/GΔ()2(\mathbb{C}^{*})^{n}/G_{\Delta}\cong(\mathbb{C}^{*})^{2}. Moreover, we define li={(z1,,zn)XΔ|zi=0}l_{i}=\{(z_{1},...,z_{n})\in\mathbb{R}X_{\Delta}|z_{i}=0\} under the homogeneous coordinate (z1,,zn)(z_{1},...,z_{n}) to be the axis of the real toric surface XΔ\mathbb{R}X_{\Delta} related to Δi\Delta_{i}. For any i=1,,ni=1,...,n, the axis lil_{i} is a boundary divisor of XΔ\mathbb{R}X_{\Delta}.

2.4. Nef cone

To give the exact definition of the mirror curve, we must firstly introduce the Nef cone with respect to a simplicial fan. One could find the general definition of Nef cone in [5]. But in this paper, still for the convention, we only consider the case of smooth toric Calabi-Yau 3-fold. Recall the exact sequence

0LψN~ϕN0,0\to L\stackrel{{\scriptstyle\psi}}{{\to}}\tilde{N}\stackrel{{\scriptstyle\phi}}{{\to}}N\to 0,

and take Hom(,Z)Hom(-,Z) on the exact sequence of free ZZ-module. We get

0MϕvM~ψvLv0.0\to M\stackrel{{\scriptstyle\phi^{v}}}{{\to}}\tilde{M}\stackrel{{\scriptstyle\psi^{v}}}{{\to}}L^{v}\to 0.

We assume #Σ(1)=p+3\#\Sigma(1)=p+3 and then consider the 𝕋\mathbb{T}-equivalent Poincare dual Di𝕋D_{i}^{\mathbb{T}} of the divisor {Zi=0}\{Z_{i}=0\} in p+3\mathbb{C}^{p+3}. Here Di𝕋D_{i}^{\mathbb{T}} is also the dual basis of bi~\tilde{b_{i}} for i=1,2,..,p+3i=1,2,..,p+3. Next we define Di=ψv(Di𝕋)D_{i}=\psi^{v}(D_{i}^{\mathbb{T}}) in LvL^{v}. For any σΣ(3)\sigma\in\Sigma(3), let IσI_{\sigma} be {i|biσ}\{i|b_{i}\notin\sigma\} and IσI_{\sigma}^{\prime} be {i|biσ}\{i|b_{i}\in\sigma\}. Then {Di|iIσ}\{D_{i}|i\in I_{\sigma}\} form a basis of LvL^{v}.

Definition 2.4.1.

For a σΣ(3)\sigma\in\Sigma(3), we define the Nef cone of σ\sigma to be

Nef~σ={0Di|iIσ}.\tilde{Nef}_{\sigma}=\{\mathbb{R}_{\geq 0}D_{i}|i\in I_{\sigma}\}.

Besides, we define the Nef cone of Σ\Sigma to be

Nef~(Σ)=σΣ(3)Nef~σ.\tilde{Nef}(\Sigma)=\bigcap\limits_{\sigma\in\Sigma(3)}\tilde{Nef}_{\sigma}.

2.5. Mirror curve

In this chapter, we define the mirror curve of a smooth toric Calabi-Yau 3-manifold. For Σ\Sigma, we give any lattice point of PΣP_{\Sigma} a monomial with parameter q=(q1,,qp)q=(q_{1},...,q_{p}). For the convention, we always assume b1=(1,0)b_{1}=(1,0), b2=(0,1)b_{2}=(0,1), b3=(0,0)b_{3}=(0,0). We choose a basis {Hi|i=1,2,,p}\{H_{i}|i=1,2,...,p\} of LvL_{\mathbb{Q}}^{v} in the Nef cone of Σ\Sigma. Then for any σΣ(3)\sigma\in\Sigma(3), because {Di|iIσ}\{D_{i}|i\in I_{\sigma}\} form a basis of LvL_{\mathbb{Q}}^{v}, we could write Hi=jIσsi,jσDjH_{i}=\sum\limits_{j\in I_{\sigma}}s_{i,j}^{\sigma}D_{j} for i=1,2,..,pi=1,2,..,p. Here si,jσs_{i,j}^{\sigma} is a non-negative rational number for any i,j,σi,j,\sigma. We now take H1,,HpH_{1},...,H_{p} which make all si,jσs_{i,j}^{\sigma} non-negative integers and Sσ=[si,jσ]ppS_{\sigma}=[s_{i,j}^{\sigma}]_{p*p} non-degenerate. Then for the parameter qq, we define

aiσ(q)={1iIσj=1p(qj)si,jσiIσa_{i}^{\sigma}(q)=\left\{\begin{array}[]{lcl}1&&{i\in I_{\sigma}^{\prime}}\\ \prod\limits_{j=1}^{p}(q_{j})^{s_{i,j}^{\sigma}}&&{i\in I_{\sigma}}\end{array}\right.

A flag (τ,σ)(\tau,\sigma) of Σ\Sigma consists of two cones σΣ(3)\sigma\in\Sigma(3) and τΣ(2)\tau\in\Sigma(2) with τσ\tau\subset\sigma. Then for any flag (τ,σ)(\tau,\sigma), there exist the unique i1,i2,i3i_{1},i_{2},i_{3} which make Iσ={i1,i2,i3}I_{\sigma}^{\prime}=\{i_{1},i_{2},i_{3}\}, Iτ={i2,i3}I_{\tau}^{\prime}=\{i_{2},i_{3}\}, Iσ={1,2,,p+3}IσI_{\sigma}=\{1,2,...,p+3\}-I_{\sigma}^{\prime}, and Iτ={1,2,,p+3}IτI_{\tau}=\{1,2,...,p+3\}-I_{\tau}^{\prime}, where bi1,bi2,bi3b_{i_{1}},b_{i_{2}},b_{i_{3}} satisfy the counterclockwise order in σ\sigma. For the convention, we call bi3b_{i_{3}} the origin of flag (τ,σ)(\tau,\sigma).

Given a flag (τ,σ)(\tau,\sigma), if 𝒃𝒊𝟏𝒃𝒊𝟑=(mi1,ni1)\boldsymbol{b_{i_{1}}}-\boldsymbol{b_{i_{3}}}=(m_{i_{1}},n_{i_{1}}), 𝒃𝒊𝟐𝒃𝒊𝟑=(mi2,ni2)\boldsymbol{b_{i_{2}}}-\boldsymbol{b_{i_{3}}}=(m_{i_{2}},n_{i_{2}}), we define

e1,(τ,σ)\displaystyle e_{1,(\tau,\sigma)} =mi1e1+ni1e2\displaystyle=m_{i_{1}}e_{1}+n_{i_{1}}e_{2}
e2,(τ,σ)\displaystyle e_{2,(\tau,\sigma)} =mi2e1+ni2e2.\displaystyle=m_{i_{2}}e_{1}+n_{i_{2}}e_{2}.

Then mi1ni2mi2ni1=1m_{i_{1}}n_{i_{2}}-m_{i_{2}}n_{i_{1}}=1. Any lattice point bjb_{j} of PΣP_{\Sigma} could be written mje1,(τ,σ)+nje2,(τ,σ)+bi3m_{j}^{\prime}e_{1,(\tau,\sigma)}+n_{j}^{\prime}e_{2,(\tau,\sigma)}+b_{i_{3}}. We call (mj,nj)(m_{j}^{\prime},n_{j}^{\prime}) the coordinate of bjb_{j} under the flag (τ,σ)(\tau,\sigma).

Definition 2.5.1.

The mirror curve with respect to a given flag (τ,σ)(\tau,\sigma) is the zeroes in ()2(\mathbb{C^{*}})^{2} of following Laurent polynomial:

H(τ,σ)(X(τ,σ),Y(τ,σ),q)=i=1p+3aiσ(q)X(τ,σ)miY(τ,σ)ni.H_{(\tau,\sigma)}(X_{(\tau,\sigma)},Y_{(\tau,\sigma)},q)=\sum\limits_{i=1}^{p+3}a_{i}^{\sigma}(q)X_{(\tau,\sigma)}^{m_{i}^{\prime}}Y_{(\tau,\sigma)}^{n_{i}^{\prime}}.

Specially, when (τ1,σ1)(\tau_{1},\sigma_{1}) satisfies the condition Iσ1={1,2,3},Iτ1={2,3}I_{\sigma_{1}}^{\prime}=\{1,2,3\},I_{\tau_{1}}^{\prime}=\{2,3\}, for the convention, we write H(τ1,σ1)(X(τ1,σ1),Y(τ1,σ1),q)H_{(\tau_{1},\sigma_{1})}(X_{(\tau_{1},\sigma_{1})},Y_{(\tau_{1},\sigma_{1})},q) as H(X,Y,q)H(X,Y,q). From now on, if we talk about a mirror curve without a given flag, then we mean the mirror curve of flag (τ1,σ1)(\tau_{1},\sigma_{1}).

There are many good propositions of the mirror curve. The most elementary and important proposition of the mirror curve is the affine equivalence.

Proposition 2.5.2.

The mirror curves of two different flags (τ1,σ1),(τ2,σ2)(\tau_{1},\sigma_{1}),(\tau_{2},\sigma_{2}) of Σ\Sigma are affine equivalent. Besides, if Iσ1={1,2,3}I_{\sigma_{1}}^{\prime}=\{1,2,3\}, Iτ1={2,3}I_{\tau_{1}}^{\prime}=\{2,3\}, Iσ2={i1,i2,i3}I_{\sigma_{2}}^{\prime}=\{i_{1},i_{2},i_{3}\}, and Iτ2={i2,i3}I_{\tau_{2}}^{\prime}=\{i_{2},i_{3}\}, we could write down the coordinate change concretely.

X(τ2,σ2)\displaystyle X_{(\tau_{2},\sigma_{2})} =XaYbai1(q)ai3(q)\displaystyle=X^{a}Y^{b}\frac{a_{i_{1}}(q)}{a_{i_{3}}(q)}
Y(τ2,σ2)\displaystyle Y_{(\tau_{2},\sigma_{2})} =XcYdai2(q)ai3(q).\displaystyle=X^{c}Y^{d}\frac{a_{i_{2}}(q)}{a_{i_{3}}(q)}.

Under such coordinate transformation, we have the following equivalence

H(X,Y,q)=ai3(q)Xmi3Yni3H(τ2,σ2)(X(τ2,σ2),Y(τ2,σ2),q).H(X,Y,q)=a_{i_{3}}(q)X^{m_{i_{3}}}Y^{n_{i_{3}}}H_{(\tau_{2},\sigma_{2})}(X_{(\tau_{2},\sigma_{2})},Y_{(\tau_{2},\sigma_{2})},q).

Here a,b,c,da,b,c,d is given by

𝒃𝒊𝟏𝒃𝒊𝟑=(a,b)\boldsymbol{b_{i_{1}}}-\boldsymbol{b_{i_{3}}}=(a,b)
𝒃𝒊𝟐𝒃𝒊𝟑=(c,d).\boldsymbol{b_{i_{2}}}-\boldsymbol{b_{i_{3}}}=(c,d).

By the affine equivalence, when we want to study propositions of one fixed flag or we need a fixed flag, we may do the coordinate change and send the three vertices of the flag to (0,0),(0,1),(1,0)(0,0),(0,1),(1,0).

Two deeper and more useful propositions about mirror curves show the distribution rules of ai(q)a_{i}(q) at each lattice point.

Proposition 2.5.3.

In Σ\Sigma, if bi1b_{i_{1}} directly connects bi2b_{i_{2}} by a 1-cell in TΣT_{\Sigma} and 2bi2=bi1+bi32b_{i_{2}}=b_{i_{1}}+b_{i_{3}}, then ai1(q)ai3(q)ai2(q)2\frac{a_{i_{1}}(q)a_{i_{3}}(q)}{a_{i_{2}}(q)^{2}} is a non-constant monomial of qq.

Figure 6 shows this case.

Refer to caption
Figure 6.
Proof.

When i2=3,i1=2i_{2}=3,i_{1}=2, the proof is done because with 𝒃𝒊𝟑=(1,0)\boldsymbol{b_{i_{3}}}=(-1,0), ai3(q)a_{i_{3}}(q) is a non-constant monomial of qq. For the general case, we hope to simplify the case to i2=3,i1=2i_{2}=3,i_{1}=2.

Choose a flag (τ,σ)(\tau,\sigma) which makes Iτ={i1,i2}I_{\tau}=\{i_{1},i_{2}\}, Iσ={i1,i2,j}I_{\sigma}=\{i_{1},i_{2},j\}. Then the coordinate of bi3b_{i_{3}} under the flag (τ,σ)(\tau,\sigma) is (0,1)(0,-1), and ai3(q)a_{i_{3}}^{\prime}(q) is a non-constant monomial of qq. Under the affine coordinate change

X(τ,σ)=XaYbai1(q)ai2(q)X_{(\tau,\sigma)}=X^{a}Y^{b}\frac{a_{i_{1}}(q)}{a_{i_{2}}(q)}
Y(τ,σ)=XcYdaj(q)ai2(q),Y_{(\tau,\sigma)}=X^{c}Y^{d}\frac{a_{j}(q)}{a_{i_{2}}(q)},

we have

ai2(q)Xmi2Yni2ai3(q)X(τ,σ)1=ai3(q)Xmi3Yni3.a_{i_{2}}(q)X^{m_{i_{2}}}Y^{n_{i_{2}}}a_{i_{3}}^{\prime}(q)X_{(\tau,\sigma)}^{-1}=a_{i_{3}}(q)X^{m_{i_{3}}}Y^{n_{i_{3}}}.

Therefore ai1(q)ai3(q)ai2(q)2=ai3(q)\frac{a_{i_{1}}(q)a_{i_{3}}(q)}{a_{i_{2}}(q)^{2}}=a_{i_{3}}^{\prime}(q)

Proposition 2.5.4.

For a flag (τ,σ)(\tau,\sigma) with Iσ={i1,i2,i3}I_{\sigma}^{\prime}=\{i_{1},i_{2},i_{3}\} and Iτ={i2,i3}I_{\tau}^{\prime}=\{i_{2},i_{3}\}, and another vertex bi4b_{i_{4}} which makes i4Iσi_{4}\in I_{\sigma}, ai4(q)(ai3(q))mi+ni1ai1(q)miai2(q)ni\frac{a_{i_{4}}(q)(a_{i_{3}}(q))^{m_{i}^{\prime}+n_{i}^{\prime}-1}}{a_{i_{1}}(q)^{m_{i}^{\prime}}a_{i_{2}}(q)^{n_{i}^{\prime}}} is a non-constant monomial of qq.

Figure 7 shows this case.

Refer to caption
Figure 7.
Proof.

As the proof of Proposition 2.5.3, firstly, the case with Iσ={1,2,3}I_{\sigma}=\{1,2,3\}, Iτ={2,3}I_{\tau}=\{2,3\} is easy. Then we consider the affine coordinate change under flag (τ,σ)(\tau,\sigma). Because bi4b_{i_{4}} has coordinate (mi4,ni4)(m_{i_{4}}^{\prime},n_{i_{4}}^{\prime}), we have

ai4(q)=ai4(q)(ai3(q))mi+niai1(q)miai2(q)ni.a_{i_{4}}^{\prime}(q)=\frac{a_{i_{4}}(q)(a_{i_{3}}(q))^{m_{i}^{\prime}+n_{i}^{\prime}}}{a_{i_{1}}(q)^{m_{i}^{\prime}}a_{i_{2}}(q)^{n_{i}^{\prime}}}.

Remark 2.5.5.

Proposition 2.5.3 could be seen as a special case of Proposition 2.5.4. However, Proposition 2.5.3 does not require a fixed flag, so sometimes it is more convenient to apply Proposition 2.5.3 instead of Proposition 2.5.4.

Remark 2.5.6.

One could also give the definition of the mirror curve with parameter q=(q1,,qp)()pq=(q_{1},...,q_{p})\in(\mathbb{C^{*}})^{p} if we define the smooth toric Calabi-Yau 3-fold XΣX_{\Sigma} with the homogeneous coordinate. Another formal definition of the mirror curve of XΣX_{\Sigma} is given by

Cq={1+x2++x3+p=0|qi=m=23+kxmTim,i=1,,p}.C_{q}=\{1+x_{2}+...+x_{3+p}=0|q_{i}=\prod\limits_{m=2}^{3+k}x_{m}^{T_{i_{m}}},\quad i=1,...,p\}.

We call 1|q|\frac{1}{|q|} the radius of parameter qq. Then people always study propositions of mirror curves with a large radius parameter. For the convention, if we say a statement for the mirror curve holds near the large radius limit, we mean ϵ>0\exists\epsilon>0, for the mirror curve with any qq has a radius larger than 1ϵ\frac{1}{\epsilon}, or equivalently, |q|<ϵ|q|<\epsilon, the statement holds.

Remark 2.5.7.

The importance of such propositions is due to when (mi4,ni4)(0,0)(m_{i_{4}},n_{i_{4}})\neq(0,0), (0,1)(0,1), (1,0)(1,0), especially with an additional condition that mi4m_{i_{4}} and ni4n_{i_{4}} are both non-negative, near the large radius limit, we could easily compare the norm of ai4(q)a_{i_{4}}(q) to the norms of ai1(q)a_{i_{1}}(q), ai2(q)a_{i_{2}}(q), ai3(q)a_{i_{3}}(q).

2.6. Tropical geometry and amoeba

In this chapter, we recall some basic notations and tools of tropical geometry. First, let us recall the notation of amoeba. Consider the map given below.

μ:()nnμ(z1,,zn)=(log|z1|,,log|zn|)\begin{array}[]{lcl}\mu:(\mathbb{C}^{*})^{n}\to\mathbb{R}^{n}\\ \mu(z_{1},...,z_{n})=(log|z_{1}|,...,log|z_{n}|)\end{array}

We define such a map by the amoeba map.

Definition 2.6.1.

Let KFK_{F} be the zeroes in ()n(\mathbb{C^{*}})^{n} of a holomorphic function F(z1,,zn)F(z_{1},...,z_{n}) with n variables. We define the amoeba of FF to be the image μ(KF)\mu(K_{F}). We write the amoeba of FF by AFA_{F}.

Amoeba is the core object of tropical geometry. There are many great propositions about the amoeba. Next, we list one and give a brief idea of the proof. If anyone is interested in the details, he could refer to [17].

Proposition 2.6.2.

If FF is a Laurent polynomial with the Newton polytope ΔF\Delta_{F}. We could define an injective map ψ\psi from the connected components of nAF\mathbb{R}^{n}-A_{F} to ΔFn\Delta_{F}\bigcap\mathbb{Z}^{n}.

Proof.

: We skip some details and write down the proof briefly. For any point x0=(x1,,xn)x_{0}=(x_{1},...,x_{n}) in nAF\mathbb{R}^{n}-A_{F}, we consider μ1(x0)()n\mu^{-1}(x_{0})\subset(\mathbb{C}^{*})^{n} which does not intersect KFK_{F}. Then the degree of loop γi:θF(ex1,,exi+iθ,..,exn)\gamma_{i}:\theta\to F(e^{x_{1}},...,e^{x_{i}+i\theta},..,e^{x_{n}}) gives an integer vF,x0,iv_{F,x_{0},i}. Thus we have constructed a map ψ\psi from nAF\mathbb{R}^{n}-A_{F} to a point of n\mathbb{Z}^{n} given by

ψ(x0)=(vF,x0,1,,vF,x0,n).\psi(x_{0})=(v_{F,x_{0},1},...,v_{F,x_{0},n}).

We write vF,x0v_{F,x_{0}} for short of (vF,x0,1,,vF,x0,n)(v_{F,x_{0},1},...,v_{F,x_{0},n}). Also, we could write the degree as Cauchy integral

vF,x0,i=1(2iπ)nμ1(x0)Fzi(z)1F(z)j=1ndzizi.\displaystyle v_{F,x_{0},i}=\frac{1}{(2i\pi)^{n}}\int_{\mu^{-1}(x_{0})}\frac{\partial F}{\partial z_{i}}(z)\frac{1}{F(z)}\bigwedge\limits_{j=1}^{n}\frac{dz_{i}}{z_{i}}.

It is easy to see that the integer vF,x0,iv_{F,x_{0},i} we just gave is constant on any connected component of nAF\mathbb{R}^{n}-A_{F} because the Cauchy integral changes continuously. Besides, by the integral, we take any preimage point z=(z1,,zn)()nz=(z_{1},...,z_{n})\in(\mathbb{C}^{*})^{n} of x0x_{0} instead of (ex1,,exi+iθ,..,exn)(e^{x_{1}},...,e^{x_{i}+i\theta},..,e^{x_{n}}). Denote such the degree of loop F(z1,,zieiθ,..,zn)F(z_{1},...,z_{i}e^{i\theta},..,z_{n}) by vF,x0,z,iv_{F,x_{0},z,i}. Calculating vF,x0,z,iv_{F,x_{0},z,i} by the Cauchy integral, we get the same result with vF,x0,iv_{F,x_{0},i} because the integral change continuously in torus μ1(x0)\mu^{-1}(x_{0}). Then we define ψ(Cx0)=vF,x0=vF,Cx0\psi(C_{x_{0}})=v_{F,x_{0}}=v_{F,C_{x_{0}}}, where Cx0C_{x_{0}} is the connected component which contains x0x_{0}.

For any lattice point a=(a1,..,an)a=(a_{1},..,a_{n}) n\in\mathbb{Z}^{n}, we know the degree of the loop

γF:θ[0,2π]F(z1eia1θ,,zneianθ)\displaystyle\gamma_{F}:\theta\in[0,2\pi]\to F(z_{1}e^{ia_{1}\theta},...,z_{n}e^{ia_{n}\theta})

is a,vF,Cx0\langle a,v_{F,C_{x_{0}}}\rangle. However, the degree of the loop must be no greater than the degree of γF\gamma_{F} under eiθe^{i\theta}. Thus a,vF,Cx0maxa,ssΔF\langle a,v_{F,C_{x_{0}}}\rangle\leq max\langle a,s\rangle_{s\in\Delta_{F}} for any a,x0a,x_{0}. Then we have ψ(Cx0)=vF,Cx0ΔF\psi(C_{x_{0}})=v_{F,C_{x_{0}}}\in\Delta_{F}.

Next, we will prove the injectivity of ψ\psi. If there exist two components C1C2C_{1}\neq C_{2}, but ψ(C1)=ψ(C2)\psi(C_{1})=\psi(C_{2}), because there exists a line lil_{i} with a rational slope passing x0C1x_{0}\in C_{1} and x1C2x_{1}\in C_{2}. We parametrize such line with the parameter tt, and integer vector a=(a1,,an)a=(a_{1},...,a_{n}). Then lil_{i} could be written (x0,1+a1t,,x0,n+ant)(x_{0,1}+a_{1}t,...,x_{0,n}+a_{n}t). We assume x1x_{1} corresponds to a positive tt in the line. Because the degree of the loop which corresponding (a1,,an)(a_{1},...,a_{n}) at x0x_{0} could also be seen as the link number of the loop of μ1(x0)\mu^{-1}(x_{0}) with degree (a1,,an)(a_{1},...,a_{n}) at each coordinate and KFK_{F}, and lil_{i} has passed the amoeba, the degree increases from x0x_{0} to x1x_{1}. We have shown a,vF,C1<a,vF,C2\langle a,v_{F,C_{1}}\rangle<\langle a,v_{F,C_{2}}\rangle. This is a contradiction. ∎

Since then, for short, if ψ(C)=σ\psi(C)=\sigma, we say that the component CC has the degree σ\sigma. At the end of this chapter, I will introduce the notation of the tropical Laurent polynomial.

Definition 2.6.3.

The tropical Laurent polynomial is the Laurent polynomial under two operations: \boxtimes and \boxplus. For a finite index set JJ and wi{}w_{i}\in\mathbb{R}\cup\{-\infty\}, \boxplus and \boxtimes are defined as follows:

iJwi=max{wi}iJ,\displaystyle\boxplus_{i\in J}w_{i}=max\{w_{i}\}_{i\in J},
iJwi=iJwi.\displaystyle\boxtimes_{i\in J}w_{i}=\sum\limits_{i\in J}w_{i}.

Specifically, the tropical Laurent polynomial with nn variables could be written as

iJaiw1ci1wncin,\displaystyle\boxplus_{i\in J}a_{i}\boxtimes w_{1}^{c_{i_{1}}}\boxtimes...\boxtimes w_{n}^{c_{i_{n}}},

where circ_{i_{r}} is an integer, and wrcirw_{r}^{c_{i_{r}}} is short for wiwiw_{i}\boxplus...\boxplus w_{i} which has total circ_{i_{r}} wiw_{i}.

Because the tropical Laurent polynomial could be written as max{fi}iJmax\{f_{i}\}_{i\in J}, where fj=aj+cj1w1++cjnwnf_{j}=a_{j}+c_{j_{1}}w_{1}+...+c_{j_{n}}w_{n}, we define the tropical hypersurface of a tropical Laurent polynomial to be the union of all the points in ({})n(\mathbb{R}\cup\{-\infty\})^{n} which make at least two iJi\in J, denoted by i1,i2i_{1},i_{2}, satisfy fi1=fi2=max{fi}iJf_{i_{1}}=f_{i_{2}}=max\{f_{i}\}_{i\in J}. It is obvious that the tropical hypersurface consists of some segments, rays, and lines. Actually, the tropical hypersurface is exactly the set of critical points of max{fi}iJmax\{f_{i}\}_{i\in J}. Since then, we write the tropical polynomial short for the tropical Laurent polynomial.

3. Tropical deformation

In this section, we mainly prove that near the large radius limit, the amoeba of the mirror curve H=0H=0 for smooth toric Calabi-Yau 3-fold XΣX_{\Sigma} has a canonical deformation retract which gives the dual subdivision of TΣT_{\Sigma}. We finish the proof by figuring out all connected components of 2AH\mathbb{R}^{2}-A_{H} and directly calculating the tropical spine which we will later give a definition of.

Lemma 3.1.

For any non-zero Laurent polynomial F:()nF:(\mathbb{C^{*}})^{n}\to\mathbb{C} with its amoeba AFA_{F}, AFA_{F} has a tropical hypersurface of τF,Cw1σF,C,1w2σF,C,2wnσF,C,n\boxplus\tau_{F,C}\boxtimes w_{1}^{\sigma_{F,C,1}}\boxtimes w_{2}^{\sigma_{F,C,2}}...\boxtimes w_{n}^{\sigma_{F,C,n}} as a deformation retract. Here the boxplus is done over all connected components of nAF\mathbb{R}^{n}-A_{F} and σF,C\sigma_{F,C} is the degree of CC, τF,C\tau_{F,C} is some constant related to FF and CC. We define this tropical hypersurface by the tropical spine.

Proof.

Firstly, we define the Ronkin function RF:nR_{F}:\mathbb{R}^{n}\to\mathbb{R} as in [17]:

RF(x)\displaystyle R_{F}(x) =(S1)nlog|F(ex+iθ))|dσ(S1)n(θ)\displaystyle=\int_{(S^{1})^{n}}log|F(e^{x+i\theta}))|d\sigma_{(S^{1})^{n}}(\theta)
=1(2π)n[0,2π]nlog|F(ex+iθ)|𝑑θ1𝑑θn.\displaystyle=\frac{1}{(2\pi)^{n}}\int_{[0,2\pi]^{n}}log|F(e^{x+i\theta})|d\theta_{1}...d\theta_{n}.

The symbol dσ(S1)n(θ)d\sigma_{(S^{1})^{n}}(\theta) here is the normalized Haar measure of group (S1)n(S^{1})^{n}. Then RFR_{F} is CC^{\infty} in any connected component of nAF\mathbb{R}^{n}-A_{F} because the integral has no flaw points outside AFA_{F}. The integral is well-defined on n\mathbb{R}^{n} because log|F|log|F| is plurisubharmonic[17] on n\mathbb{R}^{n}, i.e. subharmonic on every complex line. Then RFR_{F} is a convex function. Thus the improper integral at any point gives a finite real value on n\mathbb{R}^{n}.

We calculate the gradient of RF(x)R_{F}(x)

dRF(x)dxi\displaystyle\frac{dR_{F}(x)}{dx_{i}} =Re(1(2π)n[0,2π]nFxjF(ex+iθ)𝑑θ1𝑑θn)\displaystyle=Re(\frac{1}{(2\pi)^{n}}\int_{[0,2\pi]^{n}}\frac{\frac{\partial F}{\partial x_{j}}}{F}(e^{x+i\theta})d\theta_{1}...d\theta_{n})
=Re(1(2iπ)nμ1(x)Fzi(z)1F(z)j=1ndzizi)\displaystyle=Re(\frac{1}{(2i\pi)^{n}}\int_{\mu^{-1}(x)}\frac{\partial F}{\partial z_{i}}(z)\frac{1}{F(z)}\bigwedge\limits_{j=1}^{n}\frac{dz_{i}}{z_{i}})
=Re(σF,C,j)\displaystyle=Re(\sigma_{F,C,j})
=σF,C,j.\displaystyle=\sigma_{F,C,j}.

Then RF(x)=τF,C+σF,C,xR_{F}(x)=\tau_{F,C}+\langle\sigma_{F,C},x\rangle on CC, where τF,C\tau_{F,C} is some constant related to FF and CC.

Because RFR_{F} is convex, if we extend τF,C+σF,C,x\tau_{F,C}+\langle\sigma_{F,C},x\rangle to another component CC^{\prime} of nAF\mathbb{R}^{n}-A_{F} linearly, we have

τF,C+σF,C,x<τF,C+σF,C,xxC.\tau_{F,C}+\langle\sigma_{F,C},x\rangle<\tau_{F,C^{\prime}}+\langle\sigma_{F,C^{\prime}},x\rangle\quad\forall x\in C^{\prime}.

We have shown that the tropical spine lies in the amoeba AFA_{F}. By intuition, the amoeba retracts into the spine. The concrete retracting process is given in [17], one who has interest could find it. ∎

Generally speaking, even we have known that the amoeba of a Laurent polynomial FF has its tropical spine CτF,Cw1σF,C,1wnσF,C,n\boxplus_{C}\tau_{F,C}\boxtimes w_{1}^{\sigma_{F,C,1}}\boxtimes...\boxtimes w_{n}^{\sigma_{F,C,n}} as the deformation retract, it is still hard to calculate the tropical spine because it is hard to know exactly which lattice point in ΔF\Delta_{F} corresponds to a connected component of nAF\mathbb{R}^{n}-A_{F}. Besides, the calculation of the coefficient τF,C\tau_{F,C} is difficult as well. However, the case is easy when one monomial in FF has the largest norm and is larger than the sum of norms of other monomials.

Lemma 3.2.

In a Laurent polynomial

F(z)=σΔFcσzσ,\displaystyle F(z)=\sum\limits_{\sigma\in\Delta_{F}}c_{\sigma}z^{\sigma},

if there exist one monomial cσ0zσ0c_{\sigma_{0}}z^{\sigma_{0}} and a point z0z_{0} in ()n(\mathbb{C}^{*})^{n} making

|cσ0z0σ0|>σΔF,σσ0|cσz0σ|,\displaystyle|c_{\sigma_{0}}z_{0}^{\sigma_{0}}|>\sum\limits_{\sigma\in\Delta_{F},\sigma\neq\sigma_{0}}|c_{\sigma}z_{0}^{\sigma}|,

obviously x0=log|z0|nx_{0}=log|z_{0}|\in\mathbb{R}^{n} lies in nAF\mathbb{R}^{n}-A_{F}. Let Cx0C_{x_{0}} be the connected component of nAF\mathbb{R}^{n}-A_{F} which contains x0x_{0}, Then the degree of Cx0C_{x_{0}} equals σ0\sigma_{0}.

Proof.

: Define

g(z)=σΔF,σσ0(cσzσ)cσ0zσ0=σΔF,σσ0cσcσ0zσσ0.g(z)=\frac{\sum\limits_{\sigma\in\Delta_{F},\sigma\neq\sigma_{0}}(c_{\sigma}z^{\sigma})}{c_{\sigma_{0}}z^{\sigma_{0}}}=\sum\limits_{\sigma\in\Delta_{F},\sigma\neq\sigma_{0}}\frac{c_{\sigma}}{c_{\sigma_{0}}}z^{\sigma-\sigma_{0}}.

We do the direct calculation.

RF(x0)\displaystyle R_{F}(x_{0}) =1(2π)n[0,2π]nlog|F(z0eiθ)|𝑑θ1𝑑θn\displaystyle=\frac{1}{(2\pi)^{n}}\int_{[0,2\pi]^{n}}log|F(z_{0}*e^{i\theta})|d\theta_{1}...d\theta_{n}
=1(2π)n[0,2π]nlog|cσ0z0σ0(1+σΔF,σσ0(cσz0σei<σ,θ>)cσ0z0σ0ei<σ0,θ>)|𝑑θ1𝑑θn\displaystyle=\frac{1}{(2\pi)^{n}}\int_{[0,2\pi]^{n}}log|c_{\sigma_{0}}z_{0}^{\sigma_{0}}(1+\frac{\sum\limits_{\sigma\in\Delta_{F},\sigma\neq\sigma_{0}}(c_{\sigma}z_{0}^{\sigma}e^{i<\sigma,\theta>})}{c_{\sigma_{0}}z_{0}^{\sigma_{0}}e^{i<\sigma_{0},\theta>}})|d\theta_{1}...d\theta_{n}
=log|cσ0|+x0,σ0+Log1(x0)log|1+σΔF,σσ0(cσzσ)cσ0zσ0|𝑑σ(S1)n\displaystyle=log|c_{\sigma_{0}}|+\langle x_{0},\sigma_{0}\rangle+\int_{Log^{-1}(x_{0})}log|1+\frac{\sum\limits_{\sigma\in\Delta_{F},\sigma\neq\sigma_{0}}(c_{\sigma}z^{\sigma})}{c_{\sigma_{0}}z^{\sigma_{0}}}|d\sigma_{(S^{1})^{n}}
=log|cσ0|+x0,σ0+1(2πi)nLog1(x0)log|1+g(z)|dz1dznz1zn.\displaystyle=log|c_{\sigma_{0}}|+\langle x_{0},\sigma_{0}\rangle+\frac{1}{(2\pi i)^{n}}\int_{Log^{-1}(x_{0})}log|1+g(z)|\frac{dz_{1}...dz_{n}}{z_{1}...z_{n}}.

Because |g(z)|<1,zLog1(x0)|g(z)|<1,\forall z\in Log^{-1}(x_{0}), we have

1(2πi)nLog1(x0)log|1+g(z)|dz1dznz1zn\displaystyle\frac{1}{(2\pi i)^{n}}\int_{Log^{-1}(x_{0})}log|1+g(z)|\frac{dz_{1}...dz_{n}}{z_{1}...z_{n}}
=Re(1(2πi)nLog1(x0)log(1+g(z))dz1dznz1zn)\displaystyle=Re(\frac{1}{(2\pi i)^{n}}\int_{Log^{-1}(x_{0})}log(1+g(z))\frac{dz_{1}...dz_{n}}{z_{1}...z_{n}})
=Re(1(2πi)nLog1(x0)k=1+(1)k1g(z)kkdz1dznz1zn)\displaystyle=Re(\frac{1}{(2\pi i)^{n}}\int_{Log^{-1}(x_{0})}\sum\limits_{k=1}^{+\infty}(-1)^{k-1}\frac{g(z)^{k}}{k}\frac{dz_{1}...dz_{n}}{z_{1}...z_{n}})
=Re(1(2πi)nLog1(x0)k=1+(1)k1(σΔF,σσ0cσcσ0zσσ0)kkdz1dznz1zn)\displaystyle=Re(\frac{1}{(2\pi i)^{n}}\int_{Log^{-1}(x_{0})}\sum\limits_{k=1}^{+\infty}(-1)^{k-1}\frac{(\sum\limits_{\sigma\in\Delta_{F},\sigma\neq\sigma_{0}}\frac{c_{\sigma}}{c_{\sigma_{0}}}z^{\sigma-\sigma_{0}})^{k}}{k}\frac{dz_{1}...dz_{n}}{z_{1}...z_{n}})
=Re(1(2πi)nLog1(x0)k=1+(1)k1(σjΔFσ0,j=1,2,..,kcσ1cσkkcσ0k\displaystyle=Re(\frac{1}{(2\pi i)^{n}}\int_{Log^{-1}(x_{0})}\sum\limits_{k=1}^{+\infty}(-1)^{k-1}(\sum\limits_{\sigma_{j}\in\Delta_{F}-\sigma_{0},j=1,2,..,k}\frac{c_{\sigma_{1}}...c_{\sigma_{k}}}{kc_{\sigma_{0}}^{k}}*
zσ1++σkkσ0)dz1dznz1zn).\displaystyle z^{\sigma_{1}+...+\sigma_{k}-k\sigma_{0}})\frac{dz_{1}...dz_{n}}{z_{1}...z_{n}}).

It is known that when σ(1,,1)\sigma\neq(-1,...,-1),

Log1(x0)zσ𝑑z1𝑑zn=0,\displaystyle\int_{Log^{-1}(x_{0})}z^{\sigma}dz_{1}...dz_{n}=0,

and

Log1(x0)dz1dznz1zn=(2πi)n.\displaystyle\int_{Log^{-1}(x_{0})}\frac{dz_{1}...dz_{n}}{z_{1}...z_{n}}=(2\pi i)^{n}.

Thus

1(2πi)nLog1(x0)log|1+g(z)|dz1dznz1zn\displaystyle\frac{1}{(2\pi i)^{n}}\int_{Log^{-1}(x_{0})}log|1+g(z)|\frac{dz_{1}...dz_{n}}{z_{1}...z_{n}}
=Re(1(2πi)nLog1(x0)k=1+(1)k1(σjΔFσ0,j=1,2,..,kcσ1cσkkcσ0k\displaystyle=Re(\frac{1}{(2\pi i)^{n}}\int_{Log^{-1}(x_{0})}\sum\limits_{k=1}^{+\infty}(-1)^{k-1}(\sum\limits_{\sigma_{j}\in\Delta_{F}-\sigma_{0},j=1,2,..,k}\frac{c_{\sigma_{1}}...c_{\sigma_{k}}}{kc_{\sigma_{0}}^{k}}*
zσ1++σkkσ0)dz1dznz1zn)\displaystyle z^{\sigma_{1}+...+\sigma_{k}-k\sigma_{0}})\frac{dz_{1}...dz_{n}}{z_{1}...z_{n}})
=Re(1(2πi)nLog1(x0)(k,σ1++σk=kσ0cσ1cσkkcσ0k)dz1dznz1zn)\displaystyle=Re(\frac{1}{(2\pi i)^{n}}\int_{Log^{-1}(x_{0})}(\sum\limits_{k,\sigma_{1}+...+\sigma_{k}=k\sigma_{0}}\frac{c_{\sigma_{1}}...c_{\sigma_{k}}}{kc_{\sigma_{0}}^{k}})\frac{dz_{1}...dz_{n}}{z_{1}...z_{n}})
=Re(k,σ1++σk=kσ0cσ1cσkkcσ0k).\displaystyle=Re(\sum\limits_{k,\sigma_{1}+...+\sigma_{k}=k\sigma_{0}}\frac{c_{\sigma_{1}}...c_{\sigma_{k}}}{kc_{\sigma_{0}}^{k}}).

Because

σΔF,σσ0|cσcσ0zσσ0|<1,zLog1(x0),\sum\limits_{\sigma\in\Delta_{F},\sigma\neq\sigma_{0}}|\frac{c_{\sigma}}{c_{\sigma_{0}}}z^{\sigma-\sigma_{0}}|<1,\forall z\in Log^{-1}(x_{0}),

then

k,σ1++σk=kσ0|cσ1cσkkcσ0k|\displaystyle\sum\limits_{k,\sigma_{1}+...+\sigma_{k}=k\sigma_{0}}|\frac{c_{\sigma_{1}}...c_{\sigma_{k}}}{kc_{\sigma_{0}}^{k}}|
<k=1+σjΔFσ0,j=1,2,..,k|cσ1cσkkcσ0kzσ1++σkkσ0|\displaystyle<\sum\limits_{k=1}^{+\infty}\sum\limits_{\sigma_{j}\in\Delta_{F}-\sigma_{0},j=1,2,..,k}|\frac{c_{\sigma_{1}}...c_{\sigma_{k}}}{kc_{\sigma_{0}}^{k}}z^{\sigma_{1}+...+\sigma_{k}-k\sigma_{0}}|
=k=1+(1)k1(σΔF,σσ0|cσcσ0zσσ0|)kk<+.\displaystyle=\sum\limits_{k=1}^{+\infty}(-1)^{k-1}\frac{(\sum\limits_{\sigma\in\Delta_{F},\sigma\neq\sigma_{0}}|\frac{c_{\sigma}}{c_{\sigma_{0}}}z^{\sigma-\sigma_{0}}|)^{k}}{k}<+\infty.

Therefore, the series k,σ1++σk=kσ0cσ1cσkkcσ0k\sum\limits_{k,\sigma_{1}+...+\sigma_{k}=k\sigma_{0}}\frac{c_{\sigma_{1}}...c_{\sigma_{k}}}{kc_{\sigma_{0}}^{k}} is absolutely convergent. Then we get

RF(x0)=log|cσ0|+x0,σ0+Re(k,σ1++σk=kσ0cσ1cσkkcσ0k).R_{F}(x_{0})=log|c_{\sigma_{0}}|+\langle x_{0},\sigma_{0}\rangle+Re(\sum\limits_{k,\sigma_{1}+...+\sigma_{k}=k\sigma_{0}}\frac{c_{\sigma_{1}}...c_{\sigma_{k}}}{kc_{\sigma_{0}}^{k}}).

When x0x_{0} makes one point z0z_{0} in μ1(x0)\mu^{-1}(x_{0}) and σ0\sigma_{0} satisfy the condition of Lemma 3.2, which also guarantees all point zz in μ1(x0)\mu^{-1}(x_{0}) satisfy the same condition, there exist a neighborhood of x0x_{0} in n\mathbb{R}^{n}, denoted by Ux0U_{x_{0}} here, making all zμ1(Ux0)z\in\mu^{-1}(U_{x_{0}}) and σ0\sigma_{0} satisfying the condition of Lemma 3.2. Equivalently, the condition of Lemma 3.2 is an open condition on n\mathbb{R}^{n} for x0x_{0}. Then for any xUx0x\in U_{x_{0}}, we have

RF(x)=log|cσ0|+x,σ0+Re(k,σ1++σk=kσ0cσ1cσkkcσ0k).R_{F}(x)=log|c_{\sigma_{0}}|+\langle x,\sigma_{0}\rangle+Re(\sum\limits_{k,\sigma_{1}+...+\sigma_{k}=k\sigma_{0}}\frac{c_{\sigma_{1}}...c_{\sigma_{k}}}{kc_{\sigma_{0}}^{k}}).

Finally, we know that

σF,Cx0\displaystyle\sigma_{F,C_{x_{0}}} =σ0\displaystyle=\sigma_{0}
τF,Cx0\displaystyle\tau_{F,C_{x_{0}}} =log|cσ0|+Re(k,σ1++σk=kσ0cσ1cσkkcσ0k).\displaystyle=log|c_{\sigma_{0}}|+Re(\sum\limits_{k,\sigma_{1}+...+\sigma_{k}=k\sigma_{0}}\frac{c_{\sigma_{1}}...c_{\sigma_{k}}}{kc_{\sigma_{0}}^{k}}).

Applying Lemma 3.2 to the case of the mirror curve near the large radius limit, we have the following theorem:

Theorem 3.3.

Near the large radius limit, for the mirror curve H(X,Y,q)=0H(X,Y,q)=0 of a smooth toric Calabi-Yau 3-fold XΣX_{\Sigma}, the injective map ψ\psi from the connected components of 2AH\mathbb{R}^{2}-A_{H} to ΔHZ2\Delta_{H}\cap Z^{2} is also surjective.

Proof.

When σ=(mi,ni)ΔHZ2\sigma=(m_{i},n_{i})\in\Delta_{H}\cap Z^{2}, by applying Lemma 3.2, we only need to find a point zσ=(xσ,yσ)z_{\sigma}=(x_{\sigma},y_{\sigma}) which makes the norm of ai(q)xσmiyσnia_{i}(q)x_{\sigma}^{m_{i}}y_{\sigma}^{n_{i}} larger than the sum of norms of all other monomials. When σ=(0,0)=(m3,n3)\sigma=(0,0)=(m_{3},n_{3}), zσ=(13,13)z_{\sigma}=(\frac{1}{3},\frac{1}{3}) satisfies the condition near the large radius limit. That is because when zσ=(13,13)z_{\sigma}=(\frac{1}{3},\frac{1}{3}), the sum of all norms of monomials ai(q)xσmiyσnia_{i}(q)x_{\sigma}^{m_{i}}y_{\sigma}^{n_{i}}, i3i\neq 3 is a polynomial of |q||q| with a constant term 23\frac{2}{3}. Near the large radius limit, we have

1>13+13+i=4p+3|ai(q)|3mi+ni.1>\frac{1}{3}+\frac{1}{3}+\sum\limits_{i=4}^{p+3}\frac{|a_{i}(q)|}{3^{m_{i}+n_{i}}}.

Applying Lemma 3.2, we know that (0,0)(0,0) is in the image of ψ\psi.

Next, for any lattice point bib_{i} of ΔHZ2\Delta_{H}\cap Z^{2}, we see it as the origin of a flag (σ,ρ)(\sigma,\rho). Because H(σ,ρ)H_{(\sigma,\rho)} is affine equivalent to H=H(σ0,ρ0)H=H_{(\sigma_{0},\rho_{0})}, the corresponding coordinate change preserves the norm ratio, and such coordinate change gives an isomorphism from ()2(\mathbb{C}^{*})^{2} to ()2(\mathbb{C}^{*})^{2}, the lattice point bib_{i} has the non-empty preimage of ψ\psi. ∎

Now we have found all the connected components of 2AH\mathbb{R}^{2}-A_{H}. Thus the tropical spine of the mirror curve could be written as

(mi,ni)ΔHlog|ai(q)|Re(k,bj1++bjk=kbjiaj1(q)ajk(q)kai(q)k)w1miw2ni.\displaystyle\boxplus_{(m_{i},n_{i})\in\Delta_{H}}log|a_{i}(q)|\boxtimes Re(\sum\limits_{k,b_{j_{1}}+...+b_{j_{k}}=kb_{j_{i}}}\frac{a_{j_{1}}(q)...a_{j_{k}}(q)}{ka_{i}(q)^{k}})\boxtimes w_{1}^{m_{i}}\boxtimes w_{2}^{n_{i}}.

The tropical hypersurface gives a convex subdivision[16] of 2\mathbb{R}^{2} denoted by TT. Here the 2-cells of the subdivision are all linear parts of the tropical polynomials, the 1-cells are all the critical segments, rays, and lines. For this subdivision, we have the following theorem.

Theorem 3.4.

The subdivision TT given by the tropical hypersurface is dual to the triangulation TΣT_{\Sigma} near the large radius limit.

Proof.

We could write the tropical polynomial as

S(w)=maxi=1,2,,p+3{γi+miw1+niw2},S(w)=max_{i=1,2,...,p+3}\{\gamma_{i}+m_{i}w_{1}+n_{i}w_{2}\},

where

γi=log|ai(q)|+Re(k,bj1++bjk=kbjiaj1(q)ajk(q)kai(q)k).\gamma_{i}=log|a_{i}(q)|+Re(\sum\limits_{k,b_{j_{1}}+...+b_{j_{k}}=kb_{j_{i}}}\frac{a_{j_{1}}(q)...a_{j_{k}}(q)}{ka_{i}(q)^{k}}).

First, we construct the duality of all 1-cells of TΣT_{\Sigma} in the subdivision TT. For any two fixed vertices bi1b_{i_{1}} and bi2b_{i_{2}}, we define

σi1,i2={(w1,w2)|S(w)=γi1+mi1w1+ni1w2=γi2+mi2w1+ni2w2}.\displaystyle\sigma_{i_{1},i_{2}}^{*}=\{(w_{1},w_{2})|S(w)=\gamma_{i_{1}}+m_{i_{1}}w_{1}+n_{i_{1}}w_{2}=\gamma_{i_{2}}+m_{i_{2}}w_{1}+n_{i_{2}}w_{2}\}.

Obviously, σi1,i2\sigma_{i_{1},i_{2}}^{*} is either a 1-cell including segment and ray, or an empty set. Thus, we only need to show near the large radius limit, σi1,i2\sigma_{i_{1},i_{2}}^{*} is non-empty iff there’s a 1-cell in TΣT_{\Sigma} which connects bi1b_{i_{1}} and bi2b_{i_{2}}.

In order to calculate the spine, we will show

aj1(q)ajk(q)kai(q)k\frac{a_{j_{1}}(q)...a_{j_{k}}(q)}{ka_{i}(q)^{k}}

is a non-constant monomial of qq for any 𝒃𝒋𝟏++𝒃𝒋𝒌=k𝒃𝒊,jri.\boldsymbol{b_{j_{1}}}+...+\boldsymbol{b_{j_{k}}}=k\boldsymbol{b_{i}},j_{r}\neq i. When i=3i=3, because 𝒃𝒋𝟏++𝒃𝒋𝒌=k𝒃𝒊,\boldsymbol{b_{j_{1}}}+...+\boldsymbol{b_{j_{k}}}=k\boldsymbol{b_{i}}, there must be some jr1,2j_{r}\neq 1,2. Then the case is easy because for any i1,2,3i\neq 1,2,3, ai(q)a_{i}(q) is a non-constant monomial of qq. For a general ii, we consider a flag (σ,τ)(\sigma,\tau) which makes Iσ={t1,t2,i}I_{\sigma}^{\prime}=\{t_{1},t_{2},i\} and contains bib_{i} as the origin b3b_{3}^{\prime}. We assume bjsb_{j_{s}} corresponds to brsb_{r_{s}}^{\prime} under the flag (σ,τ)(\sigma,\tau). Then because 𝒃𝒋𝟏++𝒃𝒋𝒌=k𝒃𝒊,\boldsymbol{b_{j_{1}}}+...+\boldsymbol{b_{j_{k}}}=k\boldsymbol{b_{i}}, we have 𝒃𝒓𝟏++𝒃𝒓𝒌=0.\boldsymbol{b_{r_{1}}^{\prime}}+...+\boldsymbol{b_{r_{k}}^{\prime}}=0. Because

H(σ,τ)(X(σ,τ),Y(σ,τ),q)=1+X(σ,τ)+Y(σ,τ)+w=4p+3aw(q)X(σ,τ)mwY(σ,τ)nw,\displaystyle H_{(\sigma,\tau)}(X_{(\sigma,\tau)},Y_{(\sigma,\tau)},q)=1+X_{(\sigma,\tau)}+Y_{(\sigma,\tau)}+\sum\limits_{w=4}^{p+3}a_{w}^{\prime}(q)X_{(\sigma,\tau)}^{m_{w}^{\prime}}Y_{(\sigma,\tau)}^{n_{w}^{\prime}},

and the monomial at any lattice point coincides with that in H(X,Y,q)H(X,Y,q) under the coordinate change, we have

ars(q)=ajs(q)at1(q)mrsat2(q)nrsai(q)mi+ni+1.a_{r_{s}}^{\prime}(q)=\frac{a_{j_{s}}(q)a_{t_{1}}(q)^{m_{r_{s}}^{\prime}}a_{t_{2}}(q)^{n_{r_{s}}^{\prime}}}{a_{i}(q)^{m_{i}^{\prime}+n_{i}^{\prime}+1}}.

Then because 𝒃𝒓𝟏++𝒃𝒓𝒌=0,\boldsymbol{b_{r_{1}}^{\prime}}+...+\boldsymbol{b_{r_{k}}^{\prime}}=0, we get

aj1(q)ajk(q)ai(q)k=ar1(q)ark(q).\frac{a_{j_{1}}(q)...a_{j_{k}}(q)}{a_{i}(q)^{k}}=a_{r_{1}}^{\prime}(q)...a_{r_{k}}^{\prime}(q).

Now we have reduced the case to i=3i=3. Thus

aj1(q)ajk(q)kai(q)k\frac{a_{j_{1}}(q)...a_{j_{k}}(q)}{ka_{i}(q)^{k}}

is a non-constant polynomial of qq. Near the large radius limit, for any ll, we know that

k<l,bj1++bjk=kbiaj1(q)ajk(q)kai(q)k\sum\limits_{k<l,b_{j_{1}}+...+b_{j_{k}}=kb_{i}}\frac{a_{j_{1}}(q)...a_{j_{k}}(q)}{ka_{i}(q)^{k}}

is a polynomial of qq with the constant 0. Besides, near the large radius limit, there exists z0=(13,13)=(x0,(σ,τ),y0,(σ,τ))z_{0}=(\frac{1}{3},\frac{1}{3})=(x_{0,(\sigma,\tau)},y_{0,(\sigma,\tau)}) making

i3|ai(q)||x0,(σ,τ)|mi|y0,(σ,τ)|ni<34.\sum\limits_{i\neq 3}|a_{i}^{\prime}(q)||x_{0,(\sigma,\tau)}|^{m_{i}^{\prime}}|y_{0,(\sigma,\tau)}|^{n_{i}^{\prime}}<\frac{3}{4}.

Then

kl,bj1++bjk=kbi|aj1(q)ajk(q)kai(q)k|\displaystyle\sum\limits_{k\geq l,b_{j_{1}}+...+b_{j_{k}}=kb_{i}}|\frac{a_{j_{1}}(q)...a_{j_{k}}(q)}{ka_{i}(q)^{k}}|
<kl,|aj1(q)ajk(q)kai(q)k||x0mj1++mjkkmi||y0nj1++njkkni|\displaystyle<\sum\limits_{k\geq l,}|\frac{a_{j_{1}}(q)...a_{j_{k}}(q)}{ka_{i}(q)^{k}}||x_{0}^{m_{j_{1}}+...+m_{j_{k}}-km_{i}}||y_{0}^{n_{j_{1}}+...+n_{j_{k}}-kn_{i}}|
=(i3|ai(q)||x0,(σ,τ)|mi|y0,(σ,τ)|ni)li=0+(1)i+l1(i3|ai(q)||x0,(σ,τ)|mi|y0,(σ,τ)|ni)ii+l\displaystyle=(\sum\limits_{i\neq 3}|a_{i}^{\prime}(q)||x_{0,(\sigma,\tau)}|^{m_{i}^{\prime}}|y_{0,(\sigma,\tau)}|^{n_{i}})^{l}\sum\limits_{i=0}^{+\infty}(-1)^{i+l-1}\frac{(\sum\limits_{i\neq 3}|a_{i}^{\prime}(q)||x_{0,(\sigma,\tau)}|^{m_{i}^{\prime}}|y_{0,(\sigma,\tau)}|^{n_{i}})^{i}}{i+l}
<(34)l(i=0+(34)i)=4(34)l.\displaystyle<(\frac{3}{4})^{l}(\sum\limits_{i=0}^{+\infty}(\frac{3}{4})^{i})=4(\frac{3}{4})^{l}.

We have proved that near the large radius limit, |γilog|ai(q)||<1,i|\gamma_{i}-log|a_{i}(q)||<1,\forall i.

Note that if i1=3,i2=2i_{1}=3,i_{2}=2, then 1<γi1<1-1<\gamma_{i_{1}}<1, 1<γi2<1-1<\gamma_{i_{2}}<1. We consider the point w0=(w1,0,w2,0)=(3,γi1γi2)w_{0}=(w_{1,0},w_{2,0})=(-3,\gamma_{i_{1}}-\gamma_{i_{2}}). Near the large radius limit, any tropical monomial of the tropical polynomial S(w)=maxi=1,..,p+3{γi+miw1+niw2}S(w)=max_{i=1,..,p+3}\{\gamma_{i}+m_{i}w_{1}+n_{i}w_{2}\} is either one of γi1,γi2+w2,γ1+w1\gamma_{i_{1}},\gamma_{i_{2}}+w_{2},\gamma_{1}+w_{1} or one of γi+miw1+niw2,i>3\gamma_{i}+m_{i}w_{1}+n_{i}w_{2},i>3. But we have shown that γi<log|ai(q)|+1\gamma_{i}<log|a_{i}(q)|+1 for all i>3i>3. Thus near the large radius limit, we have γi+miw1,0+niw2,0<2\gamma_{i}+m_{i}w_{1,0}+n_{i}w_{2,0}<-2. When i=1i=1, γ1+w1,0<3+1=2\gamma_{1}+w_{1,0}<-3+1=-2. Besides, γi1=γi2+w2,0>1\gamma_{i_{1}}=\gamma_{i_{2}}+w_{2,0}>-1. Now we have proved that w0σi1,i2w_{0}\in\sigma_{i_{1},i_{2}}^{*} for i1=3i_{1}=3 and i2=2i_{2}=2. Similarly, with the symmetry Proposition 2.5.2, we know that for any (i1,i2)(i_{1},i_{2}) satisfying the condition that bi1b_{i_{1}} connects bi2b_{i_{2}} directly by a 1-cell in TΣT_{\Sigma}, σi1,i2\sigma_{i_{1},i_{2}}^{*} is non-empty near the large radius limit.

On the other hand, if i1=3i_{1}=3 but bi1b_{i_{1}} doesn’t connect bi2b_{i_{2}} directly in TΣT_{\Sigma}, we choose a flag (τ,σ)(\tau,\sigma) contains bi1b_{i_{1}} as the origin, and bj1b_{j_{1}}, bj2b_{j_{2}} as another two vertices making bi2b_{i_{2}} lies in the cone spanned by the flag, i.e. 𝒃𝒊𝟐𝒃𝒊𝟏=λ1e1,(τ,σ)+λ2e2,(τ,σ)\boldsymbol{b_{i_{2}}}-\boldsymbol{b_{i_{1}}}=\lambda_{1}e_{1,(\tau,\sigma)}+\lambda_{2}e_{2,(\tau,\sigma)} with non-negative λ1,λ2\lambda_{1},\lambda_{2}. Because bi1b_{i_{1}} does not connect bi2b_{i_{2}} directly, we know that λ1+λ22\lambda_{1}+\lambda_{2}\geq 2. Figure 8 shows the case.

Refer to caption
Figure 8.

By Proposition 2.5.4, we know that ai2(q)ai1(q)λ1+λ21aj1(q)λ1aj2(q)λ2\frac{a_{i_{2}}(q)a_{i_{1}}(q)^{\lambda_{1}+\lambda_{2}-1}}{a_{j_{1}}(q)^{\lambda_{1}}a_{j_{2}}(q)^{\lambda_{2}}} is a non-constant monomial of qq. Then near the large radius limit, we have

|ai2(q)ai1(q)λ1+λ21aj1(q)λ1aj2(q)λ2|<1e2λ1+2λ2.|\frac{a_{i_{2}}(q)a_{i_{1}}(q)^{\lambda_{1}+\lambda_{2}-1}}{a_{j_{1}}(q)^{\lambda_{1}}a_{j_{2}}(q)^{\lambda_{2}}}|<\frac{1}{e^{2\lambda_{1}+2\lambda_{2}}}.

Taking the logarithm, we get

log|ai2(q)|+(λ1+λ21)log|ai1(q)|λ1log|aj1(q)|λ2log|aj2(q)|<2λ12λ2.log|a_{i_{2}}(q)|+(\lambda_{1}+\lambda_{2}-1)log|a_{i_{1}}(q)|-\lambda_{1}log|a_{j_{1}}(q)|-\lambda_{2}log|a_{j_{2}}(q)|<-2\lambda_{1}-2\lambda_{2}.

However, for any (w1,w2)2(w_{1},w_{2})\in\mathbb{R}^{2},

γi1+mi1w1+ni1w2+(λ1+λ21)(γi2+mi2w1+ni2w2)\displaystyle\gamma_{i_{1}}+m_{i_{1}}w_{1}+n_{i_{1}}w_{2}+(\lambda_{1}+\lambda_{2}-1)(\gamma_{i_{2}}+m_{i_{2}}w_{1}+n_{i_{2}}w_{2})
λ1(γj1+mj1w1+nj1w2)λ2(γj2+mj2w1+nj2w2)\displaystyle-\lambda_{1}(\gamma_{j_{1}}+m_{j_{1}}w_{1}+n_{j_{1}}w_{2})-\lambda_{2}(\gamma_{j_{2}}+m_{j_{2}}w_{1}+n_{j_{2}}w_{2})
=γi1+(λ1+λ21)γi2λ1γj1λ2γj2\displaystyle=\gamma_{i_{1}}+(\lambda_{1}+\lambda_{2}-1)\gamma_{i_{2}}-\lambda_{1}\gamma_{j_{1}}-\lambda_{2}\gamma_{j_{2}}
=log|ai2(q)|+(λ1+λ21)log|ai1(q)|λ1log|aj1(q)|λ2log|aj2(q)|\displaystyle=log|a_{i_{2}}(q)|+(\lambda_{1}+\lambda_{2}-1)log|a_{i_{1}}(q)|-\lambda_{1}log|a_{j_{1}}(q)|-\lambda_{2}log|a_{j_{2}}(q)|
+(log|ai1(q)|γi1)+(λ1+λ21)(log|ai2(q)|γi2)λ1(log|aj1(q)|γj1)\displaystyle+(log|a_{i_{1}}(q)|-\gamma_{i_{1}})+(\lambda_{1}+\lambda_{2}-1)(log|a_{i_{2}}(q)|-\gamma_{i_{2}})-\lambda_{1}(log|a_{j_{1}}(q)|-\gamma_{j_{1}})
λ2(log|aj2(q)|γj2)\displaystyle-\lambda_{2}(log|a_{j_{2}}(q)|-\gamma_{j_{2}})
<2(λ1+λ2)+2(λ1+λ2)=0\displaystyle<-2(\lambda_{1}+\lambda_{2})+2(\lambda_{1}+\lambda_{2})=0

Because λ1+λ211\lambda_{1}+\lambda_{2}-1\geq 1, λ1,λ20\lambda_{1},\lambda_{2}\geq 0, the previous inequality contradicts the fact that γi1+mi1w1+ni1w2=γi2+mi2w1+ni2w2=max{γi+miw1+niw2}i=1,,p+3\gamma_{i_{1}}+m_{i_{1}}w_{1}+n_{i_{1}}w_{2}=\gamma_{i_{2}}+m_{i_{2}}w_{1}+n_{i_{2}}w_{2}=max\{\gamma_{i}+m_{i}w_{1}+n_{i}w_{2}\}_{i=1,...,p+3}. Therefore, we know that σi1,i2\sigma_{i_{1},i_{2}}^{*} is empty near the large radius limit. Now we have constructed all dual 1-cells in TT, then these 1-cells uniquely determine the dual 0-cells and 2-cells. Dual 0-cells are the faces of these 1-cells. Dual 2-cells are those areas bounded by the 1-cells. Figure 10 and Figure 10 show an example. Here Figure 10 gives a toric Calabi-Yau 3-fold with the mirror curve 1+x+y+q1y2+q1q2xy=01+x+y+q_{1}y^{2}+q_{1}q_{2}xy=0. Figure 10 shows the amoeba (red lines) and the tropical spine (black lines) for such a mirror curve.

Refer to caption
Figure 9.
Refer to caption
Figure 10.

Remark 3.5.

One could also give a dual subdivision of TΣT_{\Sigma} by the methods in symplectic geometry[7]. For a symplectic toric Calabi-Yau 3-fold XX, we consider the maximal torus action of 𝕋3()3\mathbb{T}^{3}\subset(\mathbb{C}^{*})^{3} and see the action as a Hamiltonian action. Here one could also see the symplectic metric as the induced symplectic metric given by the Ka¨\ddot{a}hler quotient of the canonical symplectic metric on p+3\mathbb{C}^{p+3}. We denote the moment map by μ𝕋\mu_{\mathbb{T}_{\mathbb{R}}}, where μ𝕋:XM\mu_{\mathbb{T}_{\mathbb{R}}}:X\to M_{\mathbb{R}} after we identify the Lie algebra of 𝕋3\mathbb{T}^{3} with MM_{\mathbb{R}}. Then we take the projection π\pi from MM_{\mathbb{R}} to MM^{\prime}_{\mathbb{R}} and consider the composition μ𝕋=πμ𝕋\mu_{\mathbb{T}_{\mathbb{R}}}^{\prime}=\pi*\mu_{\mathbb{T}_{\mathbb{R}}}. Finally, we define the union of all 1-dimensional and 0-dimensional 𝕋3\mathbb{T}^{3}-orbits of XX by X1X_{1}. Consider the image μ𝕋(X1)\mu_{\mathbb{T}_{\mathbb{R}}}^{\prime}(X_{1}) of X1X_{1} under μ𝕋\mu_{\mathbb{T}_{\mathbb{R}}}^{\prime}. The image is called the toric graph. Actually, the two subdivisions given by the tropical spine and the toric graph of 2\mathbb{R}^{2} are both dual subdivisions of the triangulation TΣT_{\Sigma}.

4. Cyclic-M curve and its amoeba

In Section 1.4, we have introduced the amoeba map μ\mu. Then in Section 3, we have calculated the tropical spine of the amoeba of the mirror curve for a smooth toric Calabi-Yau 3-fold XΣX_{\Sigma} directly. Such the spine gives a dual subdivision of TΣT_{\Sigma}. If we want to figure out deeper propositions of the mirror curve itself, not only the amoeba of the mirror curve, we also wish the amoeba map μ\mu to have some good propositions. For example, we hope μ\mu is locally a two-fold covering map in the interior of the amoeba and an embedding on the boundary. However, such good propositions do not always hold, even for the mirror curve with real coefficients near the large radius limit. Therefore, we must suggest some new requirements for the mirror curve.

In this section, we mainly recall the notation of the cyclic-M curve and the propositions about the cyclic-M curve introduced by Mikhalkin[14]. These propositions also explain why we hope the mirror curve is a cyclic-M curve.

For a non-singular algebraic curve A={(x,y)()2|p(x,y)=0}A=\{(x,y)\in(\mathbb{C}^{*})^{2}|p(x,y)=0\} with the Newton polytope Δp\Delta_{p}, we could do the compactification on the toric surface XΔpX_{\Delta_{p}} and get A¯\bar{A}. For a non-singular real algebraic curve A={(x,y)()2|p(x,y)=0}\mathbb{R}A=\{(x,y)\in(\mathbb{R}^{*})^{2}|p(x,y)=0\}, we could also do the compactification on the real toric surface XΔp\mathbb{R}X_{\Delta_{p}}. [7] shows that if gg is the number of interior lattice points of Δp\Delta_{p}, there exist gg linear-independent differential 1-forms on A¯\bar{A}, and gg is the maximal number. Then the genus of A¯\bar{A} on XΔpX_{\Delta_{p}} equals gg. By Harnack’s inequality[10], A¯=A¯XΔp\mathbb{R}\bar{A}=\bar{A}\cap\mathbb{R}X_{\Delta_{p}} has at most g+1g+1 connected components on the real toric surface XΔp\mathbb{R}X_{\Delta_{p}} which is the closure of ()2(\mathbb{R}^{*})^{2} in XΔpX_{\Delta_{p}}. Now we could give an exact definition of the M-curve.

Definition 4.1.

Let pp be a polynomial with real coefficients and gg be the number of interior lattice points of Δp\Delta_{p}. A non-singular real algebraic curve A={(z1,z2)()2|p(z1,z2)=0}\mathbb{R}A=\{(z_{1},z_{2})\in(\mathbb{R^{*}})^{2}|p(z_{1},z_{2})=0\} is an M-curve iff A¯\mathbb{R}\bar{A} has g+1 connected components on the real toric surface XΔp\mathbb{R}X_{\Delta_{p}}.

Then we explain what is a cyclic-M curve. Here the ‘cyclic’ means the order of an M-curve intersecting the axes of the corresponding real toric surface in a cyclic order. If A\mathbb{R}A is an M-curve and the real toric surface XΔp\mathbb{R}X_{\Delta_{p}} has axes l1,,lnl_{1},...,l_{n}, any connected component of A¯\mathbb{R}\bar{A} is homeomorphic to a circle. Thus, if we want to talk about the cyclic order, we must first assume there is only one component WW of A¯\mathbb{R}\bar{A} intersecting the axes of XΔp\mathbb{R}X_{\Delta_{p}}. Besides, we also require that there exist arcs c1,,cnc_{1},...,c_{n} of WW, which they do not intersect with each other, and cjc_{j} only intersects ljl_{j} with djd_{j} points, where djd_{j} is the number of lattice points on the side of Δp\Delta_{p} corresponding to ljl_{j} minus 1. We define djd_{j} as the integer length of Δp\Delta_{p}. Then djd_{j} is also the degree of pp restricted on ljl_{j}. Finally, we must require the order of these arcs to coincide with the order of sides of Δp\Delta_{p}. We write the definition formally right now.

Definition 4.2.

Let A\mathbb{R}A be an M-curve defined by a polynomial p(x,y)=0p(x,y)=0 with real coefficients and Δp\Delta_{p} be the Newton polytope of pp. We call A\mathbb{R}A an cyclic-M curve iff

  1. (1)

    There is only one connected component WpW_{p} of A¯\mathbb{R}\bar{A} intersecting axes of XΔpX_{\Delta_{p}}.

  2. (2)

    There exist non-intersecting arcs cic_{i} of WpW_{p} intersecting axis lil_{i} at did_{i} points, and not intersecting the other axes, where lil_{i} is the axis defined by the side Δi\Delta_{i} of Δp\Delta_{p}, and did_{i} is the integer length of Δi\Delta_{i}.

  3. (3)

    The order of cic_{i} on WpW_{p} coincides with the order of Δi\Delta_{i} on Δp\Delta_{p}.

Remark 4.3.

An M-curve is not necessarily a cyclic-M curve. For example, Figure 11 gives a non-singular M-curve given by p(z1,z2)=1+z1+z2+qz1z2p(z_{1},z_{2})=1+z_{1}+z_{2}+qz_{1}z_{2}, 0<q<10<q<1. However, this curve is not a cyclic-M curve because the order of Δi\Delta_{i} does not coincide with the order of arc cic_{i} on WpW_{p}.

Refer to caption
Figure 11. 1+z1+z2+0.5z1z2=01+z_{1}+z_{2}+0.5z_{1}z_{2}=0

The cyclic condition is important here because, without this condition, there may exist some inflection points on the boundary of the amoeba of pp, which may destroy the good propositions of the amoeba map.

In 2000, Mikhalkin proved the following propositions and a theorem about cyclic-M curves[14]. For short, we only list the statements here. In the paper[14], one can read the complete proof.

Proposition 4.4.

Let pp be a Laurent polynomial with real coefficients and A={(x,y)()2|p(x,y)=0}A=\{(x,y)\in(\mathbb{C^{*}})^{2}|p(x,y)=0\}. If A=A()2\mathbb{R}A=A\cap(\mathbb{R^{*}})^{2} is a cyclic-M curve, we define FF to be the locus of critical points of μ|A\mu|_{A}, where μ\mu is the amoeba map. Then we have F=AF=\mathbb{R}A.

Proposition 4.5.

Let pp be a Laurent polynomial with real coefficients and A={(x,y)()2|p(x,y)=0}A=\{(x,y)\in(\mathbb{C^{*}})^{2}|p(x,y)=0\}. If A\mathbb{R}A is a cyclic-M curve, then μ(A)=μ(A)\mu(\mathbb{R}A)=\partial\mu(A). Besides, the amoeba map μ\mu is an embedding on A\mathbb{R}A.

Theorem 4.6.

Let pp be a Laurent polynomial with real coefficients and A={(x,y)()2|p(x,y)=0}A=\{(x,y)\in(\mathbb{C^{*}})^{2}|p(x,y)=0\}. If A=A()2\mathbb{R}A=A\cap(\mathbb{R^{*}})^{2} is a cyclic-M curve, the topological type of (XΔp;A,l1ln)(\mathbb{R}X_{\Delta_{p}};\mathbb{R}A,l_{1}\cup...\cup l_{n}) is uniquely determined by Δp\Delta_{p}.

With such propositions, we know that if the mirror curve H(x,y,q)=0H(x,y,q)=0 is a cyclic M-curve, there don’t exist inflection points on the boundary of the amoeba of the mirror curve. Thus every point inside the amoeba has exactly two preimage points, and on the boundary, the amoeba map is an embedding. Then we could figure out the local topology of the mirror curve such that the mirror curve is glued from some pairs of pants and tubes. However, for general choices of qq, the mirror curve H(x,y,q)=0H(x,y,q)=0 isn’t always a cyclic-M curve, in the next section, we will see that under a special family of qq, the mirror curve satisfies the cyclic-M condition.

5. Cyclic M-condition of the mirror curve and its topology

In Section 3, we have calculated the tropical spine of the amoeba of mirror curve for a smooth toric Calabi-Yau 3-fold XΣX_{\Sigma} directly, and such a spine gives a dual subdivision of TΣT_{\Sigma}. Then in Section 4, we recall the propositions introduced by Mikhalkin. The most important one in this paper is that if F=0F=0 is a cyclic-M curve on the real toric surface, then the boundary of the amoeba is exactly the image of zeroes in ()2(\mathbb{R}^{*})^{2} under the amoeba map Besides, the amoeba map is 2-1 in the interior of amoeba and an embedding on the boundary.

However, the mirror curve with general real coefficients does not always satisfy either M-condition or cyclic condition. For example, the mirror curve of Σ1\Sigma_{1},

H1(x,y,q)=1+x+y+qx1y1=0,H_{1}(x,y,q)=1+x+y+qx^{-1}y^{-1}=0,

when q>0q>0, is not an M-curve as we see in Figure 13 and Figure 13. The mirror curve of Σ2\Sigma_{2},

H2(x,y,q)=1+x+y+qxy=0,H_{2}(x,y,q)=1+x+y+qxy=0,

when q>0q>0 doesn’t satisfy the cyclic condition as we see in Figure 15 and Figure 15 as well.

Refer to caption
Figure 12. Σ1\Sigma_{1}
Refer to caption
Figure 13. 1+x+y+qx1y1=01+x+y+qx^{-1}y^{-1}=0
Refer to caption
Figure 14. Σ2\Sigma_{2}
Refer to caption
Figure 15. 1+x+y+qxy=01+x+y+qxy=0

The main goals of this section are to find a special family of coefficients and to prove that these coefficients make the mirror curve a cyclic-M curve. We finish the construction by choosing the positive or negative sign at every lattice point in the fan.

5.1. Expected choices of coefficients in the mirror curve

In this chapter, we mainly show how we choose the positive or negative sign for each ai(q)a_{i}(q) when we expect the mirror curve satisfies the cyclic-M condition. Besides, we also explain the motivations for such a choice.

Firstly, we consider the case TΣT_{\Sigma} only contains four 0-cells: b3(0,0)b_{3}(0,0), b2(0,1)b_{2}(0,1), b1(1,0)b_{1}(1,0), b4(m4,n4)b_{4}(m_{4},n_{4}). Because TΣT_{\Sigma} only contains triangles with area 12\frac{1}{2} as 2-cells, b4b_{4} could only possibly lie in the union of three lines in NN^{\prime}: x=1x=-1, y=1y=-1, x+y=2x+y=2. As shown in the Figure 16, there are only 12 cases.

Refer to caption
Figure 16.

Then S124=SΔb1b2b4=12S_{124}=S_{\Delta_{b_{1}b_{2}b_{4}}}=\frac{1}{2} or S134=12S_{134}=\frac{1}{2} or S234=12S_{234}=\frac{1}{2}. By drawing the mirror curve (we draw two families of cyclic-M curves here in Figure 18 and Figure 18), our expectation must be that ai(q)>0a_{i}(q)>0 when (m4,n4)(m_{4},n_{4}) satisfies the condition m4m_{4} or n4n_{4} is even, and ai(q)<0a_{i}(q)<0 when (m4,n4)(m_{4},n_{4}) satisfies the condition m4m_{4} and n4n_{4} are both odd.

Refer to caption
Figure 17. 1+x+y0.01x1y1=01+x+y-0.01x^{-1}y^{-1}=0
Refer to caption
Figure 18. 1+x+y0.02x1y3=01+x+y-0.02x^{-1}y^{3}=0

Now we consider a general finest triangulation TΣT_{\Sigma}. For any lattice point bi=(mi,ni)b_{i}=(m_{i},n_{i}), there exists a chain of triangles Δ1Δ2Δki\Delta_{1}\to\Delta_{2}\to...\to\Delta_{k_{i}}, where Δ1\Delta_{1}=Δb1b2b3\Delta_{b_{1}b_{2}b_{3}}, Δj\Delta_{j} have exact two vertices the same as Δj+1\Delta_{j+1}, and Δki\Delta_{k_{i}} is the first triangle which contains bib_{i} as a vertex in the chain. Assume the unique vertex which belongs to Δj+1\Delta_{j+1} but does not belong to Δj\Delta_{j} is brj+1b_{r_{j+1}}. Then we have defined a chain of flag (τj,σj)...\to(\tau_{j},\sigma_{j})\to... in Σ\Sigma, where Iτj={s1,s2}I_{\tau_{j}}^{\prime}=\{s_{1},s_{2}\}, Iσj={s1,s2,rj}I_{\sigma_{j}}^{\prime}=\{s_{1},s_{2},r_{j}\}, and bs1,bs2b_{s_{1}},b_{s_{2}} are other two vertices in Δi\Delta_{i}. We could give the expected sign of ars+1(q)a_{r_{s+1}}(q) by taking the affine coordinate change which sends Δs\Delta_{s} to Δ(0,0),(1,0),(0,1)\Delta_{(0,0),(1,0),(0,1)}. Under the affine coordinates change, brs+1b_{r_{s+1}} is sent to a lattice point in the three given lines of the previous Figure 16. Thus we could give the expected sign of ars+1(q)a_{r_{s+1}}^{\prime}(q). Because we already know the expected sign of ae(q)a_{e}(q), where beb_{e} is any vertex of Δs\Delta_{s}, we could calculate the expected sign of ars+1(q)a_{r_{s+1}}(q) by Proposition 2.5.4.

The signs we give by different chains agree on the same point. Besides, the sign of ai(q)a_{i}(q) even only depends on the coordinate of bib_{i} in NN^{\prime}. Actually our expectation is that ai(q)<0a_{i}(q)<0 when mi,nim_{i},n_{i} are both odd, and ai(q)>0a_{i}(q)>0 when mim_{i} or nin_{i} is even for all i=1,2,,p+3i=1,2,...,p+3. We show the fact by direct computation. Given any flag (τ,σ)(\tau,\sigma), we consider the coordinate change.

X(τ,σ)=Xa(τ,σ)Yb(τ,σ)ai1(q)ai3(q)\displaystyle X_{(\tau,\sigma)}=X^{a(\tau,\sigma)}Y^{b(\tau,\sigma)}\frac{a_{i_{1}}(q)}{a_{i_{3}}(q)}
Y(τ,σ)=Xc(τ,σ)Yd(τ,σ)ai2(q)ai3(q)\displaystyle Y_{(\tau,\sigma)}=X^{c(\tau,\sigma)}Y^{d(\tau,\sigma)}\frac{a_{i_{2}}(q)}{a_{i_{3}}(q)}

If Δs\Delta_{s} contains bi1b_{i_{1}}, bi2b_{i_{2}}, bi3b_{i_{3}} as vertices, Δs+1\Delta_{s+1} contains bi1b_{i_{1}}, bi2b_{i_{2}}, bi4b_{i_{4}} as vertices, and bi4b_{i_{4}} has the coordinate (λ1,λ2)(\lambda_{1},\lambda_{2}) under the flag (τs,σs)(\tau_{s},\sigma_{s}), because Δs+1\Delta_{s+1} contains bi1,bi2b_{i_{1}},b_{i_{2}}, we get λ1+λ2=2\lambda_{1}+\lambda_{2}=2.

Next, we calculate the expected sign of ai4(q)a_{i_{4}}(q) by ai1(q)a_{i_{1}}(q), ai2(q)a_{i_{2}}(q), ai3(q)a_{i_{3}}(q). In the mirror curve H(τ,σ)(X(τ,σ),Y(τ,σ),q)=0H_{(\tau,\sigma)}(X_{(\tau,\sigma)},Y_{(\tau,\sigma)},q)=0, the lattice point bi4b_{i_{4}} corresponds to the monomial a4(q)X(τ,σ)λ1Y(τ,σ)λ2a^{\prime}_{4}(q)X_{(\tau,\sigma)}^{\lambda_{1}}Y_{(\tau,\sigma)}^{\lambda_{2}}. By our construction, a4(q)<0a^{\prime}_{4}(q)<0 if λ1\lambda_{1} is odd, and a4(q)>0a^{\prime}_{4}(q)>0 if λ1\lambda_{1} is even. But we know that

ai4(q)=ai3(q)(ai1(q)ai3(q))λ1(ai2(q)ai3(q))λ2a4(q).a_{i_{4}}(q)=a_{i_{3}}(q)(\frac{a_{i_{1}}(q)}{a_{i_{3}}(q)})^{\lambda_{1}}(\frac{a_{i_{2}}(q)}{a_{i_{3}}(q)})^{\lambda_{2}}a^{\prime}_{4}(q).

When λ1\lambda_{1} is even, the sign of ai4(q)a_{i_{4}}(q) is the same as ai3(q)a_{i_{3}}(q), and two coordinate components of bi4bi3b_{i_{4}}-b_{i_{3}} are both even. When λ1\lambda_{1} is odd, we have ai4(q)ai3(q)a_{i_{4}}(q)a_{i_{3}}(q) have the opposite sign of ai1(q)ai2(q)a_{i_{1}}(q)a_{i_{2}}(q). Then we consider (a,b)=e1,(τs,σs)=𝒃𝒊𝟏𝒃𝒊𝟑(a,b)=e_{1,(\tau_{s},\sigma_{s})}=\boldsymbol{b_{i_{1}}}-\boldsymbol{b_{i_{3}}}, and (c,d)=e2,(τs,σs)=𝒃𝒊𝟐𝒃𝒊𝟑(c,d)=e_{2,(\tau_{s},\sigma_{s})}=\boldsymbol{b_{i_{2}}}-\boldsymbol{b_{i_{3}}}. Because adbc=1ad-bc=1, without loss of generality, we assume adad is odd and bb is even. No matter cc is even or odd, we could prove that bi1,bi2,bi3,bi4b_{i_{1}},b_{i_{2}},b_{i_{3}},b_{i_{4}} have different parities by enumeration. Here (s1,s2)(s_{1},s_{2}) and (s3,s4)(s_{3},s_{4}) have different parities means that s1s3s_{1}-s_{3} and s2s4s_{2}-s_{4} have at least one odd integer. Thus by induction, we know ai4(q)<0a_{i_{4}}(q)<0 when mi4,ni4m_{i_{4}},n_{i_{4}} are both odd, and ai4(q)>0a_{i_{4}}(q)>0 when mi4m_{i_{4}} or ni4n_{i_{4}} is even.

Remark 5.1.1.

These choices of signs are preserved under any coordinate change. Specifically, if we fix any flag (τ,σ)(\tau,\sigma) and consider the mirror curve of such a flag given by H(τ,σ)(X(τ,σ),Y(τ,σ),q)=0H_{(\tau,\sigma)}(X_{(\tau,\sigma)},Y_{(\tau,\sigma)},q)=0, where

H(τ,σ)(X(τ,σ),Y(τ,σ),q)=i=1p+3ai(q)X(τ,σ)miY(τ,σ)ni.H_{(\tau,\sigma)}(X_{(\tau,\sigma)},Y_{(\tau,\sigma)},q)=\sum\limits_{i=1}^{p+3}a^{\prime}_{i}(q)X_{(\tau,\sigma)}^{m^{\prime}_{i}}Y_{(\tau,\sigma)}^{n^{\prime}_{i}}.

Then the sign of ai(q)a^{\prime}_{i}(q) given by ai(q)a_{i}(q) under the coordinate change agrees with the original sign we give, that ai(q)>0a^{\prime}_{i}(q)>0 when mim^{\prime}_{i} or nin^{\prime}_{i} is even, and ai(q)<0a^{\prime}_{i}(q)<0 when mim^{\prime}_{i} and nin^{\prime}_{i} are both odd. This could be another explanation for such choices of coefficients.

Remark 5.1.2.

In this chapter, we only explain why we expect that when the sign of ai(q)a_{i}(q) is given above, near the large radius limit, the mirror curve is a cyclic-M curve by some basic examples and bold calculations. However, we have not yet given any strict proof.

5.2. M-curve condition

In this chapter, we prove that under the right coefficient signs we give near the large radius limit, the mirror curve is an M-curve. As we defined before, the mirror curve given by H=0H=0 is an M-curve iff H=0H=0 have g+1g+1 connected components on the corresponding real toric surface. Here gg is the number of interior lattice points in the Newton polytope of HH.

We find these g+1g+1 components now. Firstly, there must exist at least one connected component (and exactly one because all the intersection points at infinity would be patched together) intersecting with the axes of the real toric surface, that is because when you do the coordinate change which sends a certain axis to the y-axis, x=0x=0, the intersections of the mirror curve and the axis x=0x=0 is the zeroes of a Laurent polynomial

f(y)=1+y+iai(q)ymi=0.\displaystyle f(y)=1+y+\sum\limits_{i}a_{i}(q)y^{m_{i}}=0.

Near the large radius limit, we have f(23)>0f(-\frac{2}{3})>0 and f(43)<0f(-\frac{4}{3})<0. By the intermediate value theorem, ff has at least one zero on the axes. Thus the mirror curve intersects with the axes of the real toric surface.

Then we directly find the other gg connected components in ()2(\mathbb{R}^{*})^{2}, which each has a ‘domain term’ corresponding to an interior lattice point of PΣP_{\Sigma}. Later we will explain what is a ‘domain term’. Because Σ\Sigma only contains finite flags and lattice points, the norm of the coordinate of any lattice point under each flag has a maximal value. For the convention, we use DD to stand for an upper bound of such the maximal value. That is to say for any flag (τ,σ)(\tau,\sigma) and a lattice point bjb_{j} in PΣP_{\Sigma}, if the coordinate of bjb_{j} under the flag (τ,σ)(\tau,\sigma) is (mi,ni)(m_{i}^{\prime},n_{i}^{\prime}), then Dmi2+ni2D\geq\sqrt{m_{i}^{\prime 2}+n_{i}^{\prime 2}}.

Theorem 5.2.1.

For the mirror curve H(X,Y,q)=0H(X,Y,q)=0 under the choice of signs given by ai(q)<0a_{i}(q)<0 when mim_{i} and nin_{i} are both odd, and ai(q)>0a_{i}(q)>0 when mim_{i} or nin_{i} is even, near the large radius limit, fixing any interior lattice point bi(mi,ni)b_{i}(m_{i},n_{i}) of Σ\Sigma, there exists a unique connected component WbiW_{b_{i}} of the mirror curve on the real toric surface XPΣX_{P_{\Sigma}} making all points z0=(x0,y0)Wbiz_{0}=(x_{0},y_{0})\in W_{b_{i}} satisfying that

(1+c)|ai(q)x0miy0ni|>|aj(q)x0mjy0nj|ji,\displaystyle(1+c)|a_{i}(q)x_{0}^{m_{i}}y_{0}^{n_{i}}|>|a_{j}(q)x_{0}^{m_{j}}y_{0}^{n_{j}}|\quad\forall j\neq i,

where cc is a positive constant (irrelevant with qq) making

(1+c)2D<43.\displaystyle(1+c)^{2D}<\frac{4}{3}.

For the convention, if WbiW_{b_{i}} and bib_{i} satisfy the condition of Theorem 5.2.1, we call WbiW_{b_{i}} a domain component of bib_{i}, and bib_{i} the domain term of WbiW_{b_{i}}.

Proof.

Without loss of generality, we assume that b3(0,0)b_{3}(0,0) is an interior lattice point of polytope PΣP_{\Sigma} in NN^{\prime}. Then we hope there exists a connected component which is a domain component of b3b_{3}.

Because b3b_{3} is an interior lattice point, first, we claim that

Cb3={(x,y)()2|1+c|ai(q)xmiyni|,i3}\displaystyle C_{b_{3}}=\{(x,y)\in(\mathbb{R}^{*})^{2}|1+c\geq|a_{i}(q)x^{m_{i}}y^{n_{i}}|,\forall i\neq 3\}

is a bounded compact subset in ()2(\mathbb{R}^{*})^{2} with the boundary

Cb3={(x,y)()2|1+c=|ai0(q)xmi0yni0||ai(q)xmiyni|,i0,i}.\displaystyle\partial C_{b_{3}}=\{(x,y)\in(\mathbb{R}^{*})^{2}|1+c=|a_{i_{0}}(q)x^{m_{i_{0}}}y^{n_{i_{0}}}|\geq|a_{i}(q)x^{m_{i}}y^{n_{i}}|,\exists i_{0},\forall i\}.

In ()2(\mathbb{R}^{*})^{2}, Cb3C_{b_{3}} have 4 parts which are

Cb3,++\displaystyle C_{b_{3},++} ={(x,y)Cb3,x>0,y>0},\displaystyle=\{(x,y)\in C_{b_{3}},x>0,y>0\},
Cb3,+\displaystyle C_{b_{3},+-} ={(x,y)Cb3,x>0,y<0},\displaystyle=\{(x,y)\in C_{b_{3}},x>0,y<0\},
Cb3,+\displaystyle C_{b_{3},-+} ={(x,y)Cb3,x<0,y>0},\displaystyle=\{(x,y)\in C_{b_{3}},x<0,y>0\},
Cb3,\displaystyle C_{b_{3},--} ={(x,y)Cb3,x<0,y<0}.\displaystyle=\{(x,y)\in C_{b_{3}},x<0,y<0\}.

We prove our claim now. Obviously, Cb3=Cb3,±±C_{b_{3}}=\bigsqcup C_{b_{3},\pm\pm}. We only need to prove Cb3,++C_{b_{3},++} is compacted, bounded with the boundary

{(x,y)(+)2|1+c=|ai0(q)xmi0yni0||ai(q)xmiyni|,i0,i}.\{(x,y)\in(\mathbb{R}^{+})^{2}|1+c=|a_{i_{0}}(q)x^{m_{i_{0}}}y^{n_{i_{0}}}|\geq|a_{i}(q)x^{m_{i}}y^{n_{i}}|,\exists i_{0},\forall i\}.

Here ‘bounded’ is obvious because |x|1+c,|y|1+c|x|\leq 1+c,|y|\leq 1+c.

To show Cb3,++C_{b_{3},++} is compact, we only need to show its embedding in 2\mathbb{R}^{2} is compact. It is to say Cb3,++C_{b_{3},++} is closed in 2\mathbb{R}^{2}. We only need to prove the closure of Cb3,++{C_{b_{3},++}} in 2\mathbb{R}^{2} doesn’t intersect x=0x=0 or y=0y=0. It suffices to show ϵ0>0,ϵ1>0\exists\epsilon_{0}>0,\epsilon_{1}>0 making any (x0,y0)Cb3,++(x_{0},y_{0})\in C_{b_{3},++} satisfy |x0|>ϵ0,|x1|>ϵ1|x_{0}|>\epsilon_{0},|x_{1}|>\epsilon_{1}.

Refer to caption
Figure 19.

Because b3(0,0)b_{3}(0,0) is the interior point of Σ\Sigma, we assume that b3b_{3} is the vertex of triangle Δ1\Delta_{1}, Δ2\Delta_{2},…, Δn\Delta_{n} in the clockwise order as we show on Figure 19, Δj=Δb3bijbij+1\Delta_{j}=\Delta_{b_{3}b_{i_{j}}b_{i_{j+1}}}, where in+1=i1i_{n+1}=i_{1}, i1=1i_{1}=1 , and i2=2i_{2}=2. Then there are n segments in TΣT_{\Sigma} connecting b3b_{3} and nn other lattice points bi1=b1,bi2=b2,,binb_{i_{1}}=b_{1},b_{i_{2}}=b_{2},...,b_{i_{n}}. There must be two adjacent lattice points of {bir}r=1n\{b_{i_{r}}\}_{r=1...n}, which are denoted by bik,bik+1b_{i_{k}},b_{i_{k+1}}, satisfying that a=(1,1)\vec{a}=(-1,-1) has a non-negative integer linear coefficient combination under 𝒃𝒊𝒌\boldsymbol{b_{i_{k}}} and 𝒃𝒊𝒌+𝟏\boldsymbol{b_{i_{k+1}}}, as we show in Figure 20. That is to say that there exists λ1,λ2\lambda_{1},\lambda_{2}\in\mathbb{N} and 1kn1\leq k\leq n making

a=λ1𝒃𝒊𝒌+λ2𝒃𝒊𝒌+𝟏.\displaystyle\vec{a}=\lambda_{1}\boldsymbol{b_{i_{k}}}+\lambda_{2}\boldsymbol{b_{i_{k+1}}}.

Then we consider the following inequality

43\displaystyle\frac{4}{3} >(1+c)2D\displaystyle>(1+c)^{2D}
(1+c)λ1+λ2\displaystyle\geq(1+c)^{\lambda_{1}+\lambda_{2}}
|aik(q)xmikynik|λ1|aik+1(q)xmik+1ynik+1|λ2\displaystyle\geq|a_{i_{k}}(q)x^{m_{i_{k}}}y^{n_{i_{k}}}|^{\lambda_{1}}|a_{i_{k+1}}(q)x^{m_{i_{k+1}}}y^{n_{i_{k+1}}}|^{\lambda_{2}}
=|aik(q)|λ1|aik+1(q)|λ2|x|1|y|1.\displaystyle=|a_{i_{k}}(q)|^{\lambda_{1}}|a_{i_{k+1}}(q)|^{\lambda_{2}}|x|^{-1}|y|^{-1}.

Because |y|1+c|y|\leq 1+c, we then calculate the lower boundary of |x||x| that

|x|>34(1+c)|aik(q)|λ1|aik+1(q)|λ2.\displaystyle|x|>\frac{3}{4(1+c)}|a_{i_{k}}(q)|^{\lambda_{1}}|a_{i_{k+1}}(q)|^{\lambda_{2}}.

Now we have shown that Cb3,++C_{b_{3},++} is compact with the boundary

Cb3,++={(x,y)(+)2|1+c=|ai0(q)xmi0yni0||ai(q)xmiyni|,i0,i}.\partial C_{b_{3},++}=\{(x,y)\in(\mathbb{R}^{+})^{2}|1+c=|a_{i_{0}}(q)x^{m_{i_{0}}}y^{n_{i_{0}}}|\geq|a_{i}(q)x^{m_{i}}y^{n_{i}}|,\exists i_{0},\forall i\}.
Refer to caption
Figure 20.

Then we want to find a connected component of the mirror curve inside Cb3,C_{b_{3},--}. Near the large radius limit, it is easy to find an interior point (x0,y0)=(13,13)(x_{0},y_{0})=(-\frac{1}{3},-\frac{1}{3}) of Cb3,C_{b_{3},--} which makes H(x0,y0,q)>0H(x_{0},y_{0},q)>0, because

H(13,13,q)=11313+i=4p+3ai(q)(13)mi+ni=13+i=4p+3ai(q)(13)mi+niH(-\frac{1}{3},-\frac{1}{3},q)=1-\frac{1}{3}-\frac{1}{3}+\sum\limits_{i=4}^{p+3}a_{i}(q)(-\frac{1}{3})^{m_{i}+n_{i}}=\frac{1}{3}+\sum\limits_{i=4}^{p+3}a_{i}(q)(-\frac{1}{3})^{m_{i}+n_{i}}

, where (13,13)(-\frac{1}{3},-\frac{1}{3}) is an interior point of Cb3,C_{b_{3},--}. Except 11, all monomials in H(x,y,q)H(x,y,q), taking values at (13,13)(-\frac{1}{3},-\frac{1}{3}), are either 13-\frac{1}{3} or non-constant monomials of qq. Thus near the large radius limit, H(13,13,q)>0H(-\frac{1}{3},-\frac{1}{3},q)>0.

Next, we show that for all (x,y)(x,y) on the boundary Cb3,\partial C_{b_{3},--} of Cb3,C_{b_{3},--}, near the large radius limit, H(x,y,q)<0H(x,y,q)<0. With such a result, by the intermediate value theorem, there exists at least one connected component to be the domain component of b3(0,0)b_{3}(0,0).

Now we consider the mirror curve given by

H(X,Y,q)=1+X+Y+i=4p+3ai(q)XmiYni.H(X,Y,q)=1+X+Y+\sum\limits_{i=4}^{p+3}a_{i}(q)X^{m_{i}}Y^{n_{i}}.

If there exist (x0,y0)(x_{0},y_{0}) and i0i_{0} which make

1+c=|ai0(q)x0mi0y0ni0||ai(q)x0miy0ni|,i=1,2,..,p+3,1+c=|a_{i_{0}}(q)x_{0}^{m_{i_{0}}}y_{0}^{n_{i_{0}}}|\geq|a_{i}(q)x_{0}^{m_{i}}y_{0}^{n_{i}}|,\quad i=1,2,..,p+3,

we could prove bi0b_{i_{0}} must connect b3b_{3} directly by a 1-cell in TΣT_{\Sigma}. If not, there exists Δj\Delta_{j} with vertices b3,bij,bij+1b_{3},b_{i_{j}},b_{i_{j+1}}, which makes 𝒃𝒊𝟎=λ1𝒃𝒊𝒋+λ2𝒃𝒊𝒋+𝟏\boldsymbol{b_{i_{0}}}=\lambda_{1}\boldsymbol{b_{i_{j}}}+\lambda_{2}\boldsymbol{b_{i_{j+1}}}, where λ1,λ2\lambda_{1},\lambda_{2} are non-negative integers and λ1+λ22\lambda_{1}+\lambda_{2}\geq 2 (because bi0b_{i_{0}} doesn’t directly connect b3b_{3}). By Proposition 2.5.4, we know that

ai0(q)a3(q)λ1+λ21aij(q)λ1aij+1(q)λ2=ai0(q)aij(q)λ1aij+1(q)λ2\frac{a_{i_{0}}(q)a_{3}(q)^{\lambda_{1}+\lambda_{2}-1}}{a_{i_{j}}(q)^{\lambda_{1}}a_{i_{j+1}}(q)^{\lambda_{2}}}=\frac{a_{i_{0}}(q)}{a_{i_{j}}(q)^{\lambda_{1}}a_{i_{j+1}}(q)^{\lambda_{2}}}

is a non-constant monomial of qq denoted by fi0(q)f_{i_{0}}(q). Then we get

ai0(q)x0mi0y0ni0(aij(q)x0mijy0nij)λ1(aij+1(q)x0mij+1y0nij+1)λ2=fi0(q).\displaystyle\frac{a_{i_{0}}(q)x_{0}^{m_{i_{0}}}y_{0}^{n_{i_{0}}}}{(a_{i_{j}}(q)x_{0}^{m_{i_{j}}}y_{0}^{n_{i_{j}}})^{\lambda_{1}}(a_{i_{j+1}}(q)x_{0}^{m_{i_{j+1}}}y_{0}^{n_{i_{j+1}}})^{\lambda_{2}}}=f_{i_{0}}(q).

Because near the large radius limit, |fi0(q)|<(1+c)1λ1λ2|f_{i_{0}}(q)|<(1+c)^{1-\lambda_{1}-\lambda_{2}}, we have

1+c\displaystyle 1+c =|ai0(q)x0mi0y0ni0|\displaystyle=|a_{i_{0}}(q)x_{0}^{m_{i_{0}}}y_{0}^{n_{i_{0}}}|
=|fi0(q)||aij(q)x0mijy0nij|λ1|aij+1(q)x0mij+1y0nij+1|λ2\displaystyle=|f_{i_{0}}(q)||a_{i_{j}}(q)x_{0}^{m_{i_{j}}}y_{0}^{n_{i_{j}}}|^{\lambda_{1}}|a_{i_{j+1}}(q)x_{0}^{m_{i_{j+1}}}y_{0}^{n_{i_{j+1}}}|^{\lambda_{2}}
|fi0(q)|(1+c)λ1+λ2\displaystyle\leq|f_{i_{0}}(q)|(1+c)^{\lambda_{1}+\lambda_{2}}
<1+c.\displaystyle<1+c.

This is a contradiction. Thus bi0b_{i_{0}} must directly connect b3b_{3}.

Next, we define

Cb3,,j={(x0,y0)()2|1+c=|aj(q)x0mjy0nj||ai(q)x0miy0ni|,ij}.\partial C_{b_{3},--,j}=\{(x_{0},y_{0})\in(\mathbb{R}^{-})^{2}|1+c=|a_{j}(q)x_{0}^{m_{j}}y_{0}^{n_{j}}|\geq|a_{i}(q)x_{0}^{m_{i}}y_{0}^{n_{i}}|,\forall i\neq j\}.

We have proved Cb3,,j=\partial C_{b_{3},--,j}=\emptyset if bjb_{j} doesn’t directly connect b3b_{3} by 1-cell in TΣT_{\Sigma}. So Cb3,=jVCb3,,j\partial C_{b_{3},--}=\bigcup_{j\in V}\partial C_{b_{3},--,j}, where VV is the index set of each jj which makes bjb_{j} connect b3b_{3} directly by a 1-cell in TΣT_{\Sigma}.

It is enough to prove H(x0,y0,q)<0H(x_{0},y_{0},q)<0 for all points (x0,y0)(x_{0},y_{0}) on Cb3,,j\partial C_{b_{3},--,j} for a fixed jVj\in V near the large radius limit. If (x0,y0)Cb3,,j(x_{0},y_{0})\in\partial C_{b_{3},--,j} for some fixed jVj\in V, then mj,njm_{j},n_{j} could not be even at the same time because TΣT_{\Sigma} is the finest triangulation. Then we have |aj(q)x0mjy0nj|=1+c|a_{j}(q)x_{0}^{m_{j}}y_{0}^{n_{j}}|=1+c. Also, because mj,njm_{j},n_{j} could not be even at the same time, we have (1)mj+njaj(q)<0(-1)^{m_{j}+n_{j}}a_{j}(q)<0. One could prove this by enumerating the 3 cases. Then aj(q)x0mjy0nj=1ca_{j}(q)x_{0}^{m_{j}}y_{0}^{n_{j}}=-1-c. At this time,

H(x0,y0,q)=c+i3,jai(q)(1+c)miy0ni.H(x_{0},y_{0},q)=-c+\sum_{i\neq 3,j}a_{i}(q)(1+c)^{m_{i}}y_{0}^{n_{i}}.

All the bjb_{j} which connects b3b_{3} directly correspond to negative value aj(q)x0mjy0nj<0a_{j}(q)x_{0}^{m_{j}}y_{0}^{n_{j}}<0 because mjm_{j} and njn_{j} couldn’t be even at the same time.

Among all the monomials in H(x0,y0,q)H(x_{0},y_{0},q), any positive one ar(q)x0mry0nra_{r}(q)x_{0}^{m_{r}}y_{0}^{n_{r}} corresponds to a brb_{r}^{\prime} which have two even coordinate components that mrm_{r} and nrn_{r} are both even. If br(0,0)b_{r}^{\prime}\neq(0,0), then there exist bisb_{i_{s}} and bis+1b_{i_{s+1}} which make

𝒃𝒓=λ1𝒃𝒊𝒔+λ2𝒃𝒊𝒔+𝟏,\boldsymbol{b_{r}}=\lambda_{1}\boldsymbol{b_{i_{s}}}+\lambda_{2}\boldsymbol{b_{i_{s+1}}},

where λ1\lambda_{1} and λ2\lambda_{2} are non-negative integers, and λ1+λ22\lambda_{1}+\lambda_{2}\geq 2. By Proposition 2.5.4, we know that

ar(q)x0mry0nr(ais(q)x0misy0nis)λ1(ais+1(q)x0mis+1y0nis+1)λ2\displaystyle\frac{a_{r}(q)x_{0}^{m_{r}}y_{0}^{n_{r}}}{(a_{i_{s}}(q)x_{0}^{m_{i_{s}}}y_{0}^{n_{i_{s}}})^{\lambda_{1}}(a_{i_{s+1}}(q)x_{0}^{m_{i_{s+1}}}y_{0}^{n_{i_{s+1}}})^{\lambda_{2}}}
=\displaystyle= ar(q)ais(q)λ1ais+1(q)λ2\displaystyle\frac{a_{r}(q)}{a_{i_{s}}(q)^{\lambda_{1}}a_{i_{s+1}}(q)^{\lambda_{2}}}

is a non-constant monomial of qq denoted by fr(q)f_{r}(q). Because for any isi_{s}, we have

|ar(q)x0mry0nr|\displaystyle|a_{r}(q)x_{0}^{m_{r}}y_{0}^{n_{r}}|
=\displaystyle= |fr(q)||(ais(q)x0misy0nis)λ1(ais+1(q)x0mis+1y0nis+1)λ2|\displaystyle|f_{r}(q)||(a_{i_{s}}(q)x_{0}^{m_{i_{s}}}y_{0}^{n_{i_{s}}})^{\lambda_{1}}(a_{i_{s+1}}(q)x_{0}^{m_{i_{s+1}}}y_{0}^{n_{i_{s+1}}})^{\lambda_{2}}|
\displaystyle\leq |fr(q)|(1+c)λ1+λ2\displaystyle|f_{r}(q)|(1+c)^{\lambda_{1}+\lambda_{2}}
\displaystyle\leq |fr(q)|(1+c)2D\displaystyle|f_{r}(q)|(1+c)^{2D}
<\displaystyle< 43|fr(q)|\displaystyle\frac{4}{3}|f_{r}(q)|

Therefore, near the large radius limit,

H(x0,y0,q)<c+43r|fr(q)|<0.H(x_{0},y_{0},q)<-c+\frac{4}{3}\sum_{r}|f_{r}(q)|<0.

Then we have found a domain connected component Wb3W_{b_{3}} of b3(0,0)b_{3}(0,0). Generally, we could define WbiW_{b_{i}} by taking the affine coordinate change given by a fixed flag (τ,σ)(\tau,\sigma) which has bib_{i} as the origin, then under the coordinate (X(τ,σ),Y(τ,σ))(X_{(\tau,\sigma)},Y_{(\tau,\sigma)}), we find the connected component WbiW_{b_{i}} which is a domain component of bib_{i}. By the affine equivalence, we could write down this connected component by the coordinate (X,Y)(X,Y). It is easy to see the domain component of bib_{i} is irrelevant to the flag we choose.

We only need to prove that near the large radius limit, any connected component WbiW_{b_{i}} which we have given before could only be the domain component of a unique interior lattice point in PΣP_{\Sigma}. It is a complicated proof. In the beginning, we state a lemma.

Lemma 5.2.2.

Near the large radius limit, any connected component WbiW_{b_{i}} which is the domain component of the interior lattice point bi(mi,ni)b_{i}(m_{i},n_{i}) as we defined previously locates in one of the four components of ()2(\mathbb{R}^{*})^{2}: ()2(\mathbb{R}^{-})^{2}, (+)2(\mathbb{R}^{+})^{2}, (+)()(\mathbb{R}^{+})*(\mathbb{R}^{-}), ()(+)(\mathbb{R}^{-})*(\mathbb{R}^{+}) uniquely determined by the parity of (mi,ni)(m_{i},n_{i}). Specifically, when mim_{i} and nin_{i} are both even, WbiW_{b_{i}} locates in ()2(\mathbb{R}^{-})^{2}. When mim_{i} and nin_{i} are both odd, WbiW_{b_{i}} locates in (+)2(\mathbb{R}^{+})^{2}. When mim_{i} is even and nin_{i} is odd, WbiW_{b_{i}} locates in (+)()(\mathbb{R}^{+})*(\mathbb{R}^{-}). When mim_{i} is odd and nin_{i} is even, WbiW_{b_{i}} locates in ()(+)(\mathbb{R}^{-})*(\mathbb{R}^{+}).

Proof.

Fix an flag (τ,σ)(\tau,\sigma) with Iσ={i1,i2,i3}I_{\sigma}^{\prime}=\{i_{1},i_{2},i_{3}\} and Iτ={i2,i3}I_{\tau}^{\prime}=\{i_{2},i_{3}\}. If

𝒃𝒊𝟏=\displaystyle\boldsymbol{b_{i_{1}}}= 𝒃𝒊𝟑+a𝒆𝟏+b𝒆𝟐\displaystyle\boldsymbol{b_{i_{3}}}+a\boldsymbol{e_{1}}+b\boldsymbol{e_{2}}
𝒃𝒊𝟐=\displaystyle\boldsymbol{b_{i_{2}}}= 𝒃𝒊𝟑+c𝒆𝟏+d𝒆𝟐.\displaystyle\boldsymbol{b_{i_{3}}}+c\boldsymbol{e_{1}}+d\boldsymbol{e_{2}}.

Then for any (x1,y1)Wbi3(x_{1},y_{1})\in W_{b_{i_{3}}}, because (x1,(τ,σ),y1,(τ,σ))(x_{1,(\tau,\sigma)},y_{1,(\tau,\sigma)}) locates in Wb3W_{b_{3}}^{\prime}, we have

x1,(τ,σ)=x1ay1bai1(q)ai3(q)<0\displaystyle x_{1,(\tau,\sigma)}=x_{1}^{a}y_{1}^{b}\frac{a_{i_{1}}(q)}{a_{i_{3}}(q)}<0
y1,(τ,σ)=x1cy1dai2(q)ai3(q)<0,\displaystyle y_{1,(\tau,\sigma)}=x_{1}^{c}y_{1}^{d}\frac{a_{i_{2}}(q)}{a_{i_{3}}(q)}<0,

where we denote the domain component of b3(0,0)b_{3}^{\prime}(0,0) written under the coordinate (X(τ,σ),Y(τ,σ))(X_{(\tau,\sigma)},Y_{(\tau,\sigma)}) of our fixed flag by Wb3W_{b_{3}}^{\prime}.

Because adbc=1ad-bc=1, then the signs of x1x_{1} and y1y_{1} are uniquely determined by a,b,c,da,b,c,d and ai1(q),ai2(q),ai3(q)a_{i_{1}}(q),a_{i_{2}}(q),a_{i_{3}}(q). Next, we finish the proof of the lemma in four cases.

  1. Case 1

    : When mi3m_{i_{3}} and ni3n_{i_{3}} are both even, then ai3(q)>0a_{i_{3}}(q)>0. Because adbc=1ad-bc=1, aa and bb contain at least one odd integer. If aa is even and bb is odd, then mi1m_{i_{1}} is even and ni1n_{i_{1}} is odd. Thus ai1(q)>0a_{i_{1}}(q)>0. Then if x1<0x_{1}<0 and y1<0y_{1}<0, the sign of

    x1ay1bai1(q)ai3(q)x_{1}^{a}y_{1}^{b}\frac{a_{i_{1}}(q)}{a_{i_{3}}(q)}

    is the same as (1)b(-1)^{b}, then we get

    x1ay1bai1(q)ai3(q)<0.x_{1}^{a}y_{1}^{b}\frac{a_{i_{1}}(q)}{a_{i_{3}}(q)}<0.

    Similarly, if aa is odd and bb is even, we have ai1(q)>0a_{i_{1}}(q)>0. When x1<0x_{1}<0 and y1<0y_{1}<0, we have

    x1ay1bai1(q)ai3(q)<0.x_{1}^{a}y_{1}^{b}\frac{a_{i_{1}}(q)}{a_{i_{3}}(q)}<0.

    Besides, if aa and bb are both odd, we have ai1(q)<0a_{i_{1}}(q)<0. When x1<0x_{1}<0 and y1<0y_{1}<0, we have

    x1ay1bai1(q)ai3(q)<0.x_{1}^{a}y_{1}^{b}\frac{a_{i_{1}}(q)}{a_{i_{3}}(q)}<0.

    Then if mi3m_{i_{3}} and ni3n_{i_{3}} are both even, we could prove

    x1ay1bai1(q)ai3(q)<0,x_{1}^{a}y_{1}^{b}\frac{a_{i_{1}}(q)}{a_{i_{3}}(q)}<0,

    and similarly

    x1cy1dai2(q)ai3(q)<0.x_{1}^{c}y_{1}^{d}\frac{a_{i_{2}}(q)}{a_{i_{3}}(q)}<0.

    Because the signs of x1,y1x_{1},y_{1} uniquely determine the sign of x1,(τ,σ),y1,(τ,σ)x_{1,(\tau,\sigma)},y_{1,(\tau,\sigma)}, we know (x1,y1)()2(x_{1},y_{1})\in(\mathbb{R}^{-})^{2}. Thus we get Wbi3()2W_{b_{i_{3}}}\subset(\mathbb{R}^{-})^{2}

  2. Case 2

    : When mi3m_{i_{3}} and ni3n_{i_{3}} are both odd, then ai3(q)<0a_{i_{3}}(q)<0. Because adbc=1ad-bc=1, aa and bb could not be even at the same time, and cc and dd could not be even at the same time as well, we know that ai1(q)>0a_{i_{1}}(q)>0 and ai2(q)>0a_{i_{2}}(q)>0. If x1>0,y1>0x_{1}>0,y_{1}>0,

    x1ay1bai1(q)ai3(q)<0x_{1}^{a}y_{1}^{b}\frac{a_{i_{1}}(q)}{a_{i_{3}}(q)}<0
    x1cy1bai1(q)ai3(q)<0x_{1}^{c}y_{1}^{b}\frac{a_{i_{1}}(q)}{a_{i_{3}}(q)}<0

    satisfy the signs of x1,(τ,σ),y1,(τ,σ)x_{1,(\tau,\sigma)},y_{1,(\tau,\sigma)}. Similarly, we have Wbi3(+)2W_{b_{i_{3}}}\subset(\mathbb{R}^{+})^{2}.

  3. Case 3

    : mi3m_{i_{3}} is odd. ni3n_{i_{3}} is even.

  4. Case 4

    : mi3m_{i_{3}} is even. ni3n_{i_{3}} is odd.

Cases 3 and 4 are just similar, we only prove Lemma 5.2.2 in case 3. Because mi3m_{i_{3}} is odd, and ni3n_{i_{3}} is even, ai3(q)>0a_{i_{3}}(q)>0, where (a,b)(a,b) also have three kinds of parity. When aa is odd, and bb is even, ai1(q)>0a_{i_{1}}(q)>0, then x1<0x_{1}<0 and y1>0y_{1}>0 make

x1ay1bai1(q)ai3(q)<0.x_{1}^{a}y_{1}^{b}\frac{a_{i_{1}}(q)}{a_{i_{3}}(q)}<0.

When aa is even and bb is odd, ai1(q)<0a_{i_{1}}(q)<0. We have

x1ay1bai1(q)ai3(q)<0.x_{1}^{a}y_{1}^{b}\frac{a_{i_{1}}(q)}{a_{i_{3}}(q)}<0.

When aa and bb are both odd, ai1(q)>0a_{i_{1}}(q)>0. We have

x1ay1bai1(q)ai3(q)<0.x_{1}^{a}y_{1}^{b}\frac{a_{i_{1}}(q)}{a_{i_{3}}(q)}<0.

Thus we have proved Wbi3()(+)W_{b_{i_{3}}}\subset(\mathbb{R}^{-})*(\mathbb{R}^{+}).

With Lemma 5.2.2, we only need to show the domain connected components of br1b_{r_{1}} and br2b_{r_{2}} have an empty intersection when (mr1,nr1)(m_{r_{1}},n_{r_{1}}) has the same parity with (mr2,nr2)(m_{r_{2}},n_{r_{2}}). Without loss of generality, we may assume r1=3r_{1}=3 and br1(0,0)b_{r_{1}}(0,0), then mr2m_{r_{2}} and nr2n_{r_{2}} are both even. If (x0,y0)Wbr1Wbr2(x_{0},y_{0})\in W_{b_{r_{1}}}\cap W_{b_{r_{2}}}, then we consider f1=1f_{1}=1, f2=ar2(q)x0mr2y0nr2f_{2}=a_{r_{2}}(q)x_{0}^{m_{r_{2}}}y_{0}^{n_{r_{2}}}. Choose a flag (τ,σ)(\tau,\sigma) which contains br2b_{r_{2}} as the origin. Under the coordinates of (τ,σ)(\tau,\sigma), we assume b3=beb_{3}=b_{e}^{\prime} has the coordinate (me,ne)(m_{e}^{\prime},n_{e}^{\prime}) under the flag (τ,σ)(\tau,\sigma), where me,nem_{e}^{\prime},n_{e}^{\prime} must be even because 𝒃𝒊𝟏𝒃𝒊𝟑\boldsymbol{b_{i_{1}}}-\boldsymbol{b_{i_{3}}} and 𝒃𝒊𝟐𝒃𝒊𝟑\boldsymbol{b_{i_{2}}}-\boldsymbol{b_{i_{3}}} form a \mathbb{Z}-basis of e1e2\mathbb{Z}e_{1}\bigoplus\mathbb{Z}e_{2}. We write that

𝒃𝒊𝟏𝒃𝒊𝟑=a𝒆𝟏+b𝒆𝟐\boldsymbol{b_{i_{1}}}-\boldsymbol{b_{i_{3}}}=a\boldsymbol{e_{1}}+b\boldsymbol{e_{2}}
𝒃𝒊𝟐𝒃𝒊𝟑=c𝒆𝟏+d𝒆𝟐,\boldsymbol{b_{i_{2}}}-\boldsymbol{b_{i_{3}}}=c\boldsymbol{e_{1}}+d\boldsymbol{e_{2}},

and consider

f1=ae(q)X1,(τ,σ)meY1,(τ,σ)ne,f2=1.f_{1}^{\prime}=a_{e}^{\prime}(q)X_{1,(\tau,\sigma)}^{m_{e}^{\prime}}Y_{1,(\tau,\sigma)}^{n_{e}^{\prime}},f_{2}^{\prime}=1.

Here the coordinate change is that

X1,(τ,σ)=x1ay1bai1(q)ai3(q)\displaystyle X_{1,(\tau,\sigma)}=x_{1}^{a}y_{1}^{b}\frac{a_{i_{1}}(q)}{a_{i_{3}}(q)}
Y1,(τ,σ)=x1cy1dai2(q)ai3(q).\displaystyle Y_{1,(\tau,\sigma)}=x_{1}^{c}y_{1}^{d}\frac{a_{i_{2}}(q)}{a_{i_{3}}(q)}.

Therefore, we know

f1=ai3(q)x1mi3y1ni3f1f_{1}=a_{i_{3}}(q)x_{1}^{m_{i_{3}}}y_{1}^{n_{i_{3}}}f_{1}^{\prime}
f2=ai3(q)x1mi3y1ni3f2.f_{2}=a_{i_{3}}(q)x_{1}^{m_{i_{3}}}y_{1}^{n_{i_{3}}}f_{2}^{\prime}.

Then we have

|f1||f2|=|f1||f2|.\frac{|f_{1}|}{|f_{2}|}=\frac{|f_{1}^{\prime}|}{|f_{2}^{\prime}|}.

When (x1,y1)Wb3(x_{1},y_{1})\in W_{b_{3}}, and br2b_{r_{2}} does not connect b3b_{3} directly by any 1-cell in TΣT_{\Sigma}, we have proved

|f2|<43|fr2(q)|,|f_{2}|<\frac{4}{3}|f_{r_{2}}(q)|,

where fr2(q)f_{r_{2}}(q) is a non-constant monomial of qq. Then we have

|f1||f2|>34|fr2(q)|>1\frac{|f_{1}|}{|f_{2}|}>\frac{3}{4|f_{r_{2}}(q)|}>1

near the large radius limit. But we could also similarly prove near the large radius limit,

|f2||f1|>1\frac{|f_{2}^{\prime}|}{|f_{1}^{\prime}|}>1

because (x1,y1)Wbr2(x_{1},y_{1})\in W_{b_{r_{2}}}. Thus we have the following contradiction

1>|f1||f2|=|f1||f2|>1.\displaystyle 1>\frac{|f_{1}^{\prime}|}{|f_{2}^{\prime}|}=\frac{|f_{1}|}{|f_{2}|}>1.

We have finished the proof of Theorem 5.2.1. By Theorem 5.2.1, under our choice of coefficients near the large radius limit, any interior point of PΣP_{\Sigma} is the domain term of a unique connected component on the real toric surface which does not intersect axes of XPΣX_{P_{\Sigma}}. Besides, because there is still one connected component intersecting axes of XPΣX_{P_{\Sigma}}, we get the following corollary.

Corollary 5.2.3.

Near the large radius limit, if ai(q)<0a_{i}(q)<0 when mim_{i} and nin_{i} are both odd, and ai(q)>0a_{i}(q)>0 when mim_{i} or nin_{i} is even, the mirror curve given by H(X,Y,q)=0H(X,Y,q)=0 is an M-curve.

5.3. Cyclic Condition

In this chapter, we show that near the large radius limit, under our choices of coefficients, the mirror curve satisfies the cyclic condition.

If PΣP_{\Sigma} contains sides r1,,rnr_{1},...,r_{n}, and they correspond to axes l1,,lnl_{1},...,l_{n} in the cyclic order, first, we could show under the special coefficients we have fixed, for any ii, lil_{i} intersects with a unique connected component of the mirror curve in did_{i} points, where did_{i} is the integer length of rir_{i}. For the convention, we denote the only connected component intersecting with axes by WW and call it the unbounded component.

Theorem 5.3.1.

Near the large radius limit, with ai(q)<0a_{i}(q)<0 when mim_{i} and nin_{i} are both odd, and ai(q)>0a_{i}(q)>0 when mim_{i} or nin_{i} is even, if lil_{i} is an axis of XPΣ\mathbb{R}X_{P_{\Sigma}} corresponding to side rir_{i} with integer length did_{i}, then the unbounded component WW of the mirror curve H(X,Y,q)=0H(X,Y,q)=0 intersects with lil_{i} in did_{i} points.

Proof.

Given any flag (τ,σ)(\tau,\sigma), we consider the affine coordinate change

X(τ,σ)=Xa(τ,σ)Yb(τ,σ)ai1(q)ai3(q),\displaystyle X_{(\tau,\sigma)}=X^{a(\tau,\sigma)}Y^{b(\tau,\sigma)}\frac{a_{i_{1}}(q)}{a_{i_{3}}(q)},
Y(τ,σ)=Xc(τ,σ)Yd(τ,σ)ai2(q)ai3(q).\displaystyle Y_{(\tau,\sigma)}=X^{c(\tau,\sigma)}Y^{d(\tau,\sigma)}\frac{a_{i_{2}}(q)}{a_{i_{3}}(q)}.

Under this coordinate change, the sides of ΔH\Delta_{H} are sent to the sides of ΔH(τ,σ)\Delta_{H_{(\tau,\sigma)}}, and any axis would be sent to a new axis in the new real toric surface XΔH(τ,σ)\mathbb{R}X_{\Delta_{H_{(\tau,\sigma)}}} defined by ΔH(τ,σ)\Delta_{H_{(\tau,\sigma)}}. Then without loss of generality, we could assume that l1l_{1} is the axis corresponding to the side r1r_{1} of PΣP_{\Sigma} containing b3(0,0),bjk(0,k)b_{3}(0,0),b_{j_{k}}(0,k) as two vertices, and other lattice points in Σ\Sigma outside r1r_{1} has the coordinate (m,n)(m,n) with m>0m>0 as shown in Figure 21. It is sufficient to show the mirror curve intersects with l1l_{1} in kk different points.

Refer to caption
Figure 21. The polytope given by Σ\Sigma

Then l1l_{1} is the yaxisy-axis at this time, by restricting H(x,y,q)H(x,y,q) on l1l_{1}, we get

H|l1(y)=1+y+r=2kajr(q)yr=r=0kajr(q)yr,\displaystyle H|_{l_{1}}(y)=1+y+\sum\limits_{r=2}^{k}a_{j_{r}}(q)y^{r}=\sum\limits_{r=0}^{k}a_{j_{r}}(q)y^{r},

where jrj_{r} is the index which corresponds to vertex (0,r)(0,r). But by our choice of coefficients that all ajr(q)>0a_{j_{r}}(q)>0 with mjr=0m_{j_{r}}=0, H|l1H|_{l_{1}} only have negative zeroes.

Next, we show that H|l1H|_{l_{1}} has exactly kk different negative zeroes near the large radius limit. For any fixed 0rk10\leq r\leq k-1, by Proposition 2.5.3,

br(q)=ajr+1(q)ajr1(q)ajr(q)2b_{r}(q)=\frac{a_{j_{r+1}}(q)a_{j_{r-1}}(q)}{a_{j_{r}}(q)^{2}}

is a non-constant monomial of qq. Moreover, if we choose any flag (τ,σ)(\tau,\sigma) which contains (0,r)(0,r) as the origin and Iτ={jr,jr+1}I_{\tau}=\{j_{r},j_{r+1}\}, then under such a flag, bjt=(0,t)b_{j_{t}}=(0,t) has the coordinate (0,tr)(0,t-r). By Proposition 2.5.4, we get

br,t(q)=ajt(q)ajr(q)(ajr+1(q)ajr(q))rtb_{r,t}(q)=\frac{a_{j_{t}}(q)}{a_{j_{r}}(q)}*(\frac{a_{j_{r+1}}(q)}{a_{j_{r}}(q)})^{r-t}

is a non-constant monomial of qq when tr,r+1t\neq r,r+1.

Then we calculate

H|l1(2ajr(q)ajr+1(q))\displaystyle H|_{l_{1}}(-2\frac{a_{j_{r}}(q)}{a_{j_{r+1}}(q)}) =t=0kajt(q)(2ajr(q)ajr+1(q))t\displaystyle=\sum\limits_{t=0}^{k}a_{j_{t}}(q)(-2\frac{a_{j_{r}}(q)}{a_{j_{r+1}}(q)})^{t}
=ajr(q)r+1ajr+1(q)r((2)r+tr,r+1(2)tbr,t(q)),\displaystyle=\frac{a_{j_{r}}(q)^{r+1}}{a_{j_{r+1}}(q)^{r}}(-(-2)^{r}+\sum\limits_{t\neq r,r+1}(-2)^{t}b_{r,t}(q)),

and

H|l1(12ajr(q)ajr+1(q))\displaystyle H|_{l_{1}}(-\frac{1}{2}\frac{a_{j_{r}}(q)}{a_{j_{r+1}}(q)}) =t=0kajt(q)(12ajr(q)ajr+1(q))t\displaystyle=\sum\limits_{t=0}^{k}a_{j_{t}}(q)(-\frac{1}{2}\frac{a_{j_{r}}(q)}{a_{j_{r+1}}(q)})^{t}
=ajr(q)r+1ajr+1(q)r((12)r+1+tr,r+1(12)tbr,t(q)).\displaystyle=\frac{a_{j_{r}}(q)^{r+1}}{a_{j_{r+1}}(q)^{r}}(-(-\frac{1}{2})^{r+1}+\sum\limits_{t\neq r,r+1}(-\frac{1}{2})^{t}b_{r,t}(q)).

Near the large radius limit, we have

|tr,r+1(12)tbr,t(q)|<12r+1|\sum\limits_{t\neq r,r+1}(-\frac{1}{2})^{t}b_{r,t}(q)|<\frac{1}{2^{r+1}}
|tr,r+1(2)tbr,t(q)|<2r.|\sum\limits_{t\neq r,r+1}(-2)^{t}b_{r,t}(q)|<2^{r}.

So H|l1(2ajr(q)ajr+1(q))H|_{l_{1}}(-2\frac{a_{j_{r}}(q)}{a_{j_{r+1}}(q)}) has the same sign with (1)r+1ajr(q)r+1ajr+1(q)r(-1)^{r+1}\frac{a_{j_{r}}(q)^{r+1}}{a_{j_{r+1}}(q)^{r}}, and H|l1(12ajr(q)ajr+1(q))H|_{l_{1}}(-\frac{1}{2}\frac{a_{j_{r}}(q)}{a_{j_{r+1}}(q)}) has the same sign with (1)rajr(q)r+1ajr+1(q)r(-1)^{r}\frac{a_{j_{r}}(q)^{r+1}}{a_{j_{r+1}}(q)^{r}}. We have shown that they have the opposite signs, by the intermediate value theorem, there exists at least a zero of H|l1H|_{l_{1}} in (2ajr(q)ajr+1(q),12ajr(q)ajr+1(q))(-2\frac{a_{j_{r}}(q)}{a_{j_{r+1}}(q)},-\frac{1}{2}\frac{a_{j_{r}}(q)}{a_{j_{r+1}}(q)}).

Because br(q)=ajr+1(q)ajr1(q)ajr(q)2b_{r}(q)=\frac{a_{j_{r+1}}(q)a_{j_{r-1}}(q)}{a_{j_{r}}(q)^{2}} is a non-constant monomial for any rr, then near the large radius limit, we have |br(q)|<15|b_{r}(q)|<\frac{1}{5}. Therefore, 12ajr(q)ajr+1(q)<2ajr1(q)ajr(q)-\frac{1}{2}\frac{a_{j_{r}}(q)}{a_{j_{r+1}}(q)}<-2\frac{a_{j_{r-1}}(q)}{a_{j_{r}}(q)} for any rr. We have seen that the kk intervals

(2ajr(q)ajr+1(q),12ajr(q)ajr+1(q))r=0,,k1(-2\frac{a_{j_{r}}(q)}{a_{j_{r+1}}(q)},-\frac{1}{2}\frac{a_{j_{r}}(q)}{a_{j_{r+1}}(q)})\quad r=0,...,k-1

don’t intersect with each other. Thus we have proved H|l1H|_{l_{1}} has kk different zeroes. ∎

After we get Theorem 5.3.1, we also hope that for any axis lil_{i}, there exists an arc uiu_{i} of the unbounded component WW intersects lil_{i} at did_{i} points and doesn’t intersect other axes as we show in Figure 22. Actually, we have the following theorem.

Refer to caption
Figure 22. An example when di=4d_{i}=4
Theorem 5.3.2.

Near the large radius limit, with ai(q)<0a_{i}(q)<0 when mi,nim_{i},n_{i} are both odd and ai(q)>0a_{i}(q)>0 when mim_{i} or nin_{i} is even, if lil_{i} is an axis of XPΣ\mathbb{R}X_{P_{\Sigma}} corresponding to side rir_{i} with integer length did_{i}, then their exists an arc of WW which intersecting with the axis lil_{i} in did_{i} points and not intersecting with other axes.

Proof.

Similarly as the proof of Theorem 5.3.1, without loss of generality, we assume l1l_{1} is the axis corresponding to the side r1r_{1} of PΣP_{\Sigma} containing b3(0,0),bjk(0,k)b_{3}(0,0),b_{j_{k}}(0,k) as the two vertices, and other lattice points in PΣP_{\Sigma} outside r1r_{1} has coordinate (m,n)(m,n) with m>0m>0.

We denote kk negative zeroes of H|l1H|_{l_{1}} by s1s_{1},…, sks_{k}, where srs_{r} is the zero lies in (2ajr(q)ajr+1(q),12ajr(q)ajr+1(q))(-2\frac{a_{j_{r}}(q)}{a_{j_{r+1}}(q)},-\frac{1}{2}\frac{a_{j_{r}}(q)}{a_{j_{r+1}}(q)}), and we assume Ar=(0,sr)A_{r}=(0,s_{r}). Then we hope to construct an arc that only intersects l1l_{1} with the points ArA_{r} and Ar+1A_{r+1} and doesn’t intersect with the other axes.

Now let us construct the arc connecting ArA_{r} and Ar+1A_{r+1}. We choose a flag (τ,σ)(\tau,\sigma) which contains bjrb_{j_{r}} as the origin and makes Iτ={jr,jr+1}I_{\tau}^{\prime}=\{j_{r},j_{r+1}\}. Consider the affine coordinate change under this flag

X(τ,σ)=XaYbaw(q)ajr(q)\displaystyle X_{(\tau,\sigma)}=X^{a}Y^{b}\frac{a_{w}(q)}{a_{j_{r}}(q)}
Y(τ,σ)=Yajr+1(q)ajr(q).\displaystyle Y_{(\tau,\sigma)}=Y\frac{a_{j_{r+1}}(q)}{a_{j_{r}}(q)}.

Then for e=1,,ke=1,...,k, under the coordinate (X(τ,σ),Y(τ,σ))(X_{(\tau,\sigma)},Y_{(\tau,\sigma)}), Ae=(0,ajr(q)ajr+1(q)se)A_{e}=(0,\frac{a_{j_{r}}(q)}{a_{j_{r+1}}(q)}s_{e}). We denote ajr(q)ajr+1(q)se\frac{a_{j_{r}}(q)}{a_{j_{r+1}}(q)}s_{e} by ses_{e}^{\prime}. Then all zeroes of H(τ,σ)|X(τ,σ)=0H_{(\tau,\sigma)}|_{X_{(\tau,\sigma)}=0} are {se|e=1,..,k}\{s_{e}^{\prime}|e=1,..,k\}. Because under the flag (τ,σ)(\tau,\sigma), bjrb_{j_{r}} has the coordinate (0,0)(0,0), and bjr+1b_{j_{r+1}} has the coordinate (0,1)(0,1) with ajr(q)=ajr+1(q)=1a_{j_{r}}^{\prime}(q)=a_{j_{r+1}}^{\prime}(q)=1, we know that sr+1(2ajr+2(q),12ajr+2(q))s_{r+1}^{\prime}\in(-2a_{j_{r+2}}^{\prime}(q),-\frac{1}{2}a_{j_{r+2}}^{\prime}(q)), and sr(2,12)s_{r}^{\prime}\in(-2,-\frac{1}{2}). Now we only need to construct the arc under the coordinate (X(τ,σ),Y(τ,σ))(X_{(\tau,\sigma)},Y_{(\tau,\sigma)}).

We consider all lattice points bl1b_{l_{1}}, …, blwb_{l_{w}} connecting bjr+1b_{j_{r+1}} directly. Under the flag (τ,σ)(\tau,\sigma), blcb_{l_{c}} must have the coordinate (mlc,nlc)(m_{l_{c}}^{\prime},n_{l_{c}}^{\prime}) where mlc0m_{l_{c}}^{\prime}\geq 0, and mlc,nlcm_{l_{c}}^{\prime},n_{l_{c}}^{\prime} could not be even at the same time for c=1,,wc=1,...,w. Then for any c=1,..,wc=1,..,w, we have (1)mlc+nlcalcσ(q)<0(-1)^{m_{l_{c}}^{\prime}+n_{l_{c}}^{\prime}}a_{l_{c}}^{\sigma}(q)<0. Thus alcσ(q)xmlcynlc<0a_{l_{c}}^{\sigma}(q)x^{m_{l_{c}}^{\prime}}y^{n_{l_{c}}^{\prime}}<0 when x<0x<0 and y<0y<0.

For y[sr,sr+1]y\in[s_{r}^{\prime},s_{r+1}^{\prime}], we define g(y)g(y) to be the unique negative ss which makes

max{|alcσ(q)smlcynlc|}=3.max\{|a_{l_{c}}^{\sigma}(q)s^{m_{l_{c}}^{\prime}}y^{n_{l_{c}}^{\prime}}|\}=3.

Here the existence and uniqueness of ss are due to the fact mlc0m_{l_{c}}^{\prime}\geq 0, and at least one cc makes mlc>0m_{l_{c}}^{\prime}>0 which makes

max{|alcσ(q)smlcynlc|}max\{|a_{l_{c}}^{\sigma}(q)s^{m_{l_{c}}^{\prime}}y^{n_{l_{c}}^{\prime}}|\}

increase monotonically strictly with respect to |s||s| without an upper bound. Then we define AA to be the index set of the lattice points which do not connect bjrb_{j_{r}} directly. Similarly as the point (1,1)(-1,-1) in Figure 20, for any point bi(mi,ni)b_{i}(m_{i}^{\prime},n_{i}^{\prime}), there exists a flag (τ1,σ1)(\tau_{1},\sigma_{1}) containing bjrb_{j_{r}} as the origin, and the two coordinate components of bib_{i}, denoted by mi′′m_{i}^{\prime\prime} and ni′′n_{i}^{\prime\prime}, are both non-negative. For y[sr,sr+1]y\in[s_{r}^{\prime},s_{r+1}^{\prime}], because y<0y<0 and g(y)<0g(y)<0, we have

alcσ(q)g(y)mlcynlc<0c=1,,w.a_{l_{c}}^{\sigma}(q)g(y)^{m_{l_{c}}^{\prime}}y^{n_{l_{c}}^{\prime}}<0\quad\forall c=1,...,w.

Then

H(τ,σ)(g(y),y,q)\displaystyle H_{(\tau,\sigma)}(g(y),y,q) =i=1p+3aiσ(q)g(y)miyni\displaystyle=\sum\limits_{i=1}^{p+3}a_{i}^{\sigma}(q)g(y)^{m_{i}^{\prime}}y^{n_{i}^{\prime}}
=1+c=1walcσ(q)g(y)mlcynlc+iAaiσ(q)g(y)miyni\displaystyle=1+\sum\limits_{c=1}^{w}a_{l_{c}}^{\sigma}(q)g(y)^{m_{l_{c}}^{\prime}}y^{n_{l_{c}}^{\prime}}+\sum\limits_{i\in A}a_{i}^{\sigma}(q)g(y)^{m_{i}^{\prime}}y^{n_{i}^{\prime}}
<13+iA|aiσ(q)g(y)miyni|.\displaystyle<1-3+\sum\limits_{i\in A}|a_{i}^{\sigma}(q)g(y)^{m_{i}^{\prime}}y^{n_{i}^{\prime}}|.

By Proposition 2.5.4, for any ii, there exists a non-constant monomial bi(q)b_{i}(q) and c1,c2c_{1},c_{2}, makes

|aiσ(q)g(y)miyni|\displaystyle|a_{i}^{\sigma}(q)g(y)^{m_{i}^{\prime}}y^{n_{i}^{\prime}}| =|bi(q)(alc1(q)g(y)mc1ync1)mi′′(alc2(q)g(y)mc2ync2)ni′′|\displaystyle=|b_{i}(q)(a_{l_{c_{1}}}(q)g(y)^{m_{c_{1}}^{\prime}}y^{n_{c_{1}}^{\prime}})^{m_{i}^{\prime\prime}}(a_{l_{c_{2}}}(q)g(y)^{m_{c_{2}}^{\prime}}y^{n_{c_{2}}^{\prime}})^{n_{i}^{\prime\prime}}|
3mi′′+ni′′|bi(q)|\displaystyle\leq 3^{m_{i}^{\prime\prime}+n_{i}^{\prime\prime}}|b_{i}(q)|
<32D|bi(q)|.\displaystyle<3^{2D}|b_{i}(q)|.

Finally, near the large radius limit, we get

H(τ,σ)(g(y),y,q)<2+32DiA|bi(q)|<0.H_{(\tau,\sigma)}(g(y),y,q)<-2+3^{2D}\sum\limits_{i\in A}|b_{i}(q)|<0.

However, because near the large radius limit, for 12[sr,sr+1]-\frac{1}{2}\in[s_{r}^{\prime},s_{r+1}^{\prime}], it is obvious that H(τ,σ)(0,12,q)>0H_{(\tau,\sigma)}(0,-\frac{1}{2},q)>0, we have proved

H(τ,σ)(0,y,q)>0y(sr,sr+1).H_{(\tau,\sigma)}(0,y,q)>0\quad\forall y\in(s_{r}^{\prime},s_{r+1}^{\prime}).

By the intermediate value theorem, for any fixed y[sr,sr+1]y\in[s_{r}^{\prime},s_{r+1}^{\prime}], there exists z(g(y),0]z\in(g(y),0] making H(τ,σ)(z,y,q)=0H_{(\tau,\sigma)}(z,y,q)=0. Denote the non-positive zero of H(τ,σ)(,y)H_{(\tau,\sigma)}(\quad,y) with the least norm by h(y)h(y). Then g(y)h(y)0g(y)\leq h(y)\leq 0 for all y[sr,sr+1]y\in[s_{r}^{\prime},s_{r+1}^{\prime}]. Besides, h(y)=0h(y)=0 iff y=sry=s_{r}^{\prime} or y=sr+1y=s_{r+1}^{\prime}. Finally, because H(τ,σ)(X,Y,q)H_{(\tau,\sigma)}(X,Y,q) is a Laurent polynomial with respect to X,YX,Y, h(y)h(y) is a smooth function with respect to y[sr,sr+1]y\in[s_{r}^{\prime},s_{r+1}^{\prime}]. We have constructed an arc connecting ArA_{r} and Ar+1A_{r+1} with the parameterization given by (h(y),y),y[sr,sr+1](h(y),y),\quad y\in[s_{r}^{\prime},s_{r+1}^{\prime}]. ∎

Now, it suffices to show there exists an arc connecting two adjacent axes. We have the following theorem.

Theorem 5.3.3.

Near the large radius limit, with ai(q)<0a_{i}(q)<0 when mim_{i} and nin_{i} are both odd, and ai(q)>0a_{i}(q)>0 when mim_{i} or nin_{i} is even, if lil_{i} and li+1l_{i+1} are two axes of XPΣ\mathbb{R}X_{P_{\Sigma}} corresponding to two adjacent sides rir_{i}, ri+1r_{i+1} in PΣP_{\Sigma}, then there exists an arc of WW only intersecting with these two axes.

Proof.

Still without loss of generality, we assume lil_{i} and li+1l_{i+1} are the axes corresponding to side rir_{i}, ri+1r_{i+1}, where rir_{i} is the segment having the two vertices b3(0,0)b_{3}(0,0) and bjk(0,k)b_{j_{k}}(0,k), and ri+1r_{i+1} having the two vertices b3(0,0)b_{3}(0,0) and ble(ew1,ew2)b_{l_{e}}(ew_{1},ew_{2}). Here ee is an integer, w1w_{1} and w2w_{2} are coprime, and w1>0w_{1}>0, w20w_{2}\leq 0, as we show in Figure 23.

Refer to caption
Figure 23.

Then lil_{i} is the y-axis, because H|yaxis=1+y+aj2(q)y2++ajk(q)ykH|_{y-axis}=1+y+a_{j_{2}}(q)y^{2}+...+a_{j_{k}}(q)y^{k} has the zero with the least norm in (2,12)(-2,-\frac{1}{2}) near the large radius limit. We denote this zero by ss. Thus H(0,t,q)>0H(0,t,q)>0 for st<0s\leq t<0.

Next, we consider all lattice points bl1b_{l_{1}}, …, blwb_{l_{w}} connecting b3b_{3} directly, similarly, for any fixed t[s,0)t\in[s,0),

v(|x|)=max{|alc(q)xmlctnlc|}v(|x|)=max\{|a_{l_{c}}(q)x^{m_{l_{c}}}t^{n_{l_{c}}}|\}

increases monotonically strictly with |x||x| increasing without an upper boundary. We still define g(t)g(t) to be the unique negative xx which makes

max{|alc(q)xmlctnlc|}=3.max\{|a_{l_{c}}(q)x^{m_{l_{c}}}t^{n_{l_{c}}}|\}=3.

Similarly, if we define AA to be the index set that corresponds to all lattices which do not connect b3b_{3} directly, we have

H(g(t),t,q)\displaystyle H(g(t),t,q) =i=1p+3ai(q)g(t)mitni\displaystyle=\sum\limits_{i=1}^{p+3}a_{i}(q)g(t)^{m_{i}}t^{n_{i}}
=1+c=1walc(q)g(t)mlctnlc+iAai(q)g(t)mitni\displaystyle=1+\sum\limits_{c=1}^{w}a_{l_{c}}(q)g(t)^{m_{l_{c}}}t^{n_{l_{c}}}+\sum\limits_{i\in A}a_{i}(q)g(t)^{m_{i}}t^{n_{i}}
<13+iA|ai(q)g(t)mitni|\displaystyle<1-3+\sum\limits_{i\in A}|a_{i}(q)g(t)^{m_{i}}t^{n_{i}}|

However, similarly, by Proposition 2.5.4, for any ii, there exist a non-constant monomial bi(q)b_{i}(q) and c1,c2c_{1},c_{2}, making

|ai(q)g(t)mitni|\displaystyle|a_{i}(q)g(t)^{m_{i}}t^{n_{i}}| =|bi(q)(alc1(q)g(t)mc1tnc1)mi(alc2(q)g(t)mc2tnc2)ni|\displaystyle=|b_{i}(q)(a_{l_{c_{1}}}(q)g(t)^{m_{c_{1}}}t^{n_{c_{1}}})^{m_{i}^{\prime}}(a_{l_{c_{2}}}(q)g(t)^{m_{c_{2}}}t^{n_{c_{2}}})^{n_{i}^{\prime}}|
3mi+ni|bi(q)|\displaystyle\leq 3^{m_{i}^{\prime}+n_{i}^{\prime}}|b_{i}(q)|
<32D|bi(q)|.\displaystyle<3^{2D}|b_{i}(q)|.

Finally, near the large radius limit, we get

H(g(t),t,q)<2+32DiA|bi(q)|<0.H(g(t),t,q)<-2+3^{2D}\sum\limits_{i\in A}|b_{i}(q)|<0.

Then by the intermediate value theorem, letting h(t)h(t) be the non-positive zero of H(,t,q)H(\quad,t,q) with the least norm, we have h(t)[g(t),0]h(t)\in[g(t),0]. Besides, h(t)=0h(t)=0 iff t=st=s.

Finally, we consider the arc (h(t),t)(h(t),t) with the parameter t[s,0)t\in[s,0). Because H(h(t),t,q)=0H(h(t),t,q)=0 for all t[s,0)t\in[s,0), then

0\displaystyle 0 =i=1p+3ai(q)h(t)mitni\displaystyle=\sum\limits_{i=1}^{p+3}a_{i}(q)h(t)^{m_{i}}t^{n_{i}}
=i=0eali(q)(h(t)w1tw2)i+jliaj(q)h(t)mjtnj.\displaystyle=\sum\limits_{i=0}^{e}a_{l_{i}}(q)(h(t)^{w_{1}}t^{w_{2}})^{i}+\sum\limits_{j\neq l_{i}}a_{j}(q)h(t)^{m_{j}}t^{n_{j}}.

Thus, for any jlij\neq l_{i}, there exist positive integer numbers k1,jk_{1,j}, k2,jk_{2,j}, k3,jk_{3,j} which make k1,j(w1,w2)+k2,j(0,1)=k3,j(mj,nj)k_{1,j}(w_{1},w_{2})+k_{2,j}(0,1)=k_{3,j}(m_{j},n_{j}). Then

|aj(q)h(t)mjtnj|=|aj(q)||t|k2,jk3,j|h(t)w1tw2|k1,jk3,j.|a_{j}(q)h(t)^{m_{j}}t^{n_{j}}|=|a_{j}(q)||t|^{\frac{k_{2,j}}{k_{3,j}}}|h(t)^{w_{1}}t^{w_{2}}|^{\frac{k_{1,j}}{k_{3,j}}}.

Therefore, near the large radius limit, if we denote ee different zeroes of

i=0eali(q)xi\sum\limits_{i=0}^{e}a_{l_{i}}(q)x^{i}

by u1u_{1}, …, ueu_{e} with |u1|<<|ue||u_{1}|<...<|u_{e}|, where there exist ee different zeroes because we could see

i=0eali(q)xi\sum\limits_{i=0}^{e}a_{l_{i}}(q)x^{i}

as HH restricted on axis li+1l_{i+1}, we have

0=H(h(t),t,q)\displaystyle 0=H(h(t),t,q) =i=0eali(q)(h(t)w1tw2)i+jliaj(q)h(t)mjtnj\displaystyle=\sum\limits_{i=0}^{e}a_{l_{i}}(q)(h(t)^{w_{1}}t^{w_{2}})^{i}+\sum\limits_{j\neq l_{i}}a_{j}(q)h(t)^{m_{j}}t^{n_{j}}
i=0eali(q)(h(t)w1tw2)i+jli|aj(q)||t|k2,jk3,j|h(t)w1tw2|k1,jk3,j.\displaystyle\leq\sum\limits_{i=0}^{e}a_{l_{i}}(q)(h(t)^{w_{1}}t^{w_{2}})^{i}+\sum\limits_{j\neq l_{i}}|a_{j}(q)||t|^{\frac{k_{2,j}}{k_{3,j}}}|h(t)^{w_{1}}t^{w_{2}}|^{\frac{k_{1,j}}{k_{3,j}}}.

Similarly, we could prove

jli|aj(q)||t|k2,jk3,j|h(t)w1tw2|k1,jk3,j\displaystyle-\sum\limits_{j\neq l_{i}}|a_{j}(q)||t|^{\frac{k_{2,j}}{k_{3,j}}}|h(t)^{w_{1}}t^{w_{2}}|^{\frac{k_{1,j}}{k_{3,j}}} i=0eali(q)(h(t)w1tw2)i\displaystyle\leq\sum\limits_{i=0}^{e}a_{l_{i}}(q)(h(t)^{w_{1}}t^{w_{2}})^{i}
jli|aj(q)||t|k2,jk3,j|h(t)w1tw2|k1,jk3,j.\displaystyle\leq\sum\limits_{j\neq l_{i}}|a_{j}(q)||t|^{\frac{k_{2,j}}{k_{3,j}}}|h(t)^{w_{1}}t^{w_{2}}|^{\frac{k_{1,j}}{k_{3,j}}}.

Because |h(t)w1tw2|3|al1(q)||h(t)^{w_{1}}t^{w_{2}}|\leq\frac{3}{|a_{l_{1}}(q)|}, take the limit of tt tending to 0, we get

limt0i=0eali(q)(h(t)w1tw2)i=0.lim_{t\to 0}\sum\limits_{i=0}^{e}a_{l_{i}}(q)(h(t)^{w_{1}}t^{w_{2}})^{i}=0.

Finally, because h(t)h(t) corresponds to the zero with the least norm, we have

limt0h(t)w1tw2=u1.lim_{t\to 0}h(t)^{w_{1}}t^{w_{2}}=u_{1}.

If we write such an arc by the homogeneous coordinate, for the parameter t[s,0)t\in[s,0), the arc is given as (1,1,.,h(t)tw2w1,t1w1,,1)(1,1,....,h(t)*t^{\frac{w_{2}}{w_{1}}},t^{\frac{1}{w_{1}}},...,1). Here we choose a fixed branch of x1w1x^{\frac{1}{w_{1}}}. Then

limt0h(t)tw2w1=u11w1.lim_{t\to 0}h(t)t^{\frac{w_{2}}{w_{1}}}=u_{1}^{\frac{1}{w_{1}}}.

Because for any branch of x1w1x^{\frac{1}{w_{1}}}, we have (1,1,,u11w1,0,1,,1)(1,1,...,u_{1}^{\frac{1}{w_{1}}},0,1,...,1) corresponding to the same point in the toric surface (one could see this by considering the group action on p+3\mathbb{C}^{p+3}), we could naturally extend the arc with the parameter t[s,0]t\in[s,0]. Besides, such an extended arc only intersects with the axes lil_{i}, li+1l_{i+1}. ∎

With the previous three theorems, we have shown the corollary given below.

Corollary 5.3.4.

Near the large radius limit, with ai(q)<0a_{i}(q)<0 when mim_{i} and nin_{i} are both odd, and ai(q)>0a_{i}(q)>0 when mim_{i} or nin_{i} is even, the mirror curve is a cyclic M-curve.

With the corollary, we could give a refinement of the topology of the mirror curve near the large radius limit. Because we have already calculated the tropicalization of the mirror curve near the large radius limit which is dual to the subdivision TΣT_{\Sigma} given by Σ\Sigma. For any bounded 2-cell CC in the subdivision given by the tropicalization, there exists an oval contains in CC. Besides, for unbounded 2-cell CC^{\prime}, there exists an unbounded convex half circle contains in CC^{\prime}, as we show in Figure 24.

Refer to caption
Figure 24.

Then because the amoeba map is an embedding on the boundary of the amoeba and 2-1 in the interior of the amoeba, we could show that the mirror curve under such special coefficients is glued by tubes and pairs of pants. Any vertex corresponds to a pair of pants, and any edge corresponds to a tube, as we show in Figure 26 and Figure 26. Finally, because qq is a flat family of parameters[7] near the large radius limit, we have seen that, for a general qq, the mirror curve is glued from tubes and pairs of pants, and these tubes and pairs of pants move smoothly with the change of the parameter q()pq\in(\mathbb{C^{*}})^{p} near the large radius limit.

Remark 5.3.5.

This result is only a refinement because the topological type of a non-singular algebraic curve on a toric surface is uniquely determined by its genus. However, near the large radius limit, we have shown how to glue these tubes and pairs of pants concretely. This gives us the local way to see the topology of the mirror curve.

Refer to caption
Figure 25. 1+x+y0.01x1y1=01+x+y-0.01x^{-1}y^{-1}=0
Refer to caption
Figure 26. Topology of Mirror curve

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