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3.2. Asymptotes for the first order ansatz [0427]

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3.2. Asymptotes for the first order ansatz

This Section is concerned with obtaining refined asymptotes of α~1\tilde{\alpha}_{1}, α~2\tilde{\alpha}_{2}, α~3\tilde{\alpha}_{3}; a summary can be found at the end of the Section. We define the average functions

(3.5) {α¯1​(μ1,μ2,y)=∫01α~1​(μ1,μ2,x+−1​y)​dx,α¯2​(μ1,μ2,y)=∫01α~2​(μ1,μ2,x+−1​y)​dx,α¯3​(μ1,μ2,y)=∫01α~3​(μ1,μ2,x+−1​y)​dx.\begin{cases}\bar{\alpha}_{1}(\mu_{1},\mu_{2},y)=\int_{0}^{1}\tilde{\alpha}_{1}(\mu_{1},\mu_{2},x+\sqrt{-1}y)dx,\\ \bar{\alpha}_{2}(\mu_{1},\mu_{2},y)=\int_{0}^{1}\tilde{\alpha}_{2}(\mu_{1},\mu_{2},x+\sqrt{-1}y)dx,\\ \bar{\alpha}_{3}(\mu_{1},\mu_{2},y)=\int_{0}^{1}\tilde{\alpha}_{3}(\mu_{1},\mu_{2},x+\sqrt{-1}y)dx.\end{cases}

The main goal in this Section is to prove exponential decay estimate for α~i−α¯i\tilde{\alpha}_{i}-\bar{\alpha}_{i} outside a tubular neighbourhood of 𝔇i\mathfrak{D}_{i}.

Proposition 3.3.

(Leading order asymptote) The formulae for α¯i\bar{\alpha}_{i} are explicitly given as

(3.6) {α¯1=12​a22​{log⁡2−γE−log⁡(1A​|(μ1,μ2,y)|a′−a22A​(μ2+a12a22​μ1))}α¯2=12​a11​{log⁡2−γE−log⁡(1A​|(μ1,μ2,y)|a′−a11A​(μ1+a12a11​μ2))}α¯3=12​a11+2​a12+a22{log2−γE−log(1A|(μ1,μ2,y)|a′+a11​μ1+a12​μ2+a21​μ1+a22​μ2A​a11+2​a12+a22)}\begin{cases}\bar{\alpha}_{1}=&\frac{1}{2\sqrt{a_{22}}}\{\log 2-\gamma_{E}-\log\left(\frac{1}{\sqrt{A}}|(\mu_{1},\mu_{2},y)|_{a}^{\prime}-\frac{\sqrt{a_{22}}}{\sqrt{A}}(\mu_{2}+\frac{a_{12}}{a_{22}}\mu_{1})\right)\}\\ \bar{\alpha}_{2}=&\frac{1}{2\sqrt{a_{11}}}\{\log 2-\gamma_{E}-\log\left(\frac{1}{\sqrt{A}}|(\mu_{1},\mu_{2},y)|_{a}^{\prime}-\frac{\sqrt{a_{11}}}{\sqrt{A}}(\mu_{1}+\frac{a_{12}}{a_{11}}\mu_{2})\right)\}\\ \bar{\alpha}_{3}=&\frac{1}{2\sqrt{a_{11}+2a_{12}+a_{22}}}\{\log 2-\gamma_{E}\\ &-\log\left(\frac{1}{\sqrt{A}}|(\mu_{1},\mu_{2},y)|_{a}^{\prime}+\frac{a_{11}\mu_{1}+a_{12}\mu_{2}+a_{21}\mu_{1}+a_{22}\mu_{2}}{\sqrt{A}\sqrt{a_{11}+2a_{12}+a_{22}}}\right)\}\end{cases}

where γE=limn→∞∑k=1n1k−log⁡n\gamma_{E}=\lim_{n\to\infty}\sum_{k=1}^{n}\frac{1}{k}-\log n is the Euler constant.

Proof.

We will focus on α¯1\bar{\alpha}_{1}. The periodic version of equation (2.7) on ℝμ1,μ22×(S1×ℝ)η\mathbb{R}^{2}_{\mu_{1},\mu_{2}}\times(S^{1}\times\mathbb{R})_{\eta} is the measure equation

(Δaα~1)A3/2dμ1∧dμ2∧dx∧dy=−2πA∫𝔇1dμ2.(\Delta_{a}\tilde{\alpha}_{1})A^{3/2}d\mu_{1}\wedge d\mu_{2}\wedge dx\wedge dy=-2\pi\sqrt{A}\int_{\mathfrak{D}_{1}}d\mu_{2}.

Integrating in the periodic xx-variable from 0 to 1,

(3.7) (Δa′α¯1)dVola′=−2π∫𝔇1dμ2,(\Delta_{a}^{\prime}\bar{\alpha}_{1})d\text{Vol}_{a}^{\prime}=-2\pi\int_{\mathfrak{D}_{1}}d\mu_{2},

where Δa′\Delta_{a}^{\prime} is the Laplacian of the metric ga′=ai​j​d​μi​d​μj+A​d​y2g_{a}^{\prime}=a_{ij}d\mu_{i}d\mu_{j}+Ady^{2} on ℝμ1,μ22×ℝ\mathbb{R}^{2}_{\mu_{1},\mu_{2}}\times\mathbb{R}, whose volume form is d​Vola′=A​d​μ1∧d​μ2∧d​yd\text{Vol}_{a}^{\prime}=Ad\mu_{1}\wedge d\mu_{2}\wedge dy.

Now the basic strategy is to build a function satisfying the same measure equation and then compare. For a large positive cutoff Λ\Lambda, we calculate the Green representation

−14​π∫0Λ−2​π|(μ1,μ2−s,y)|a′ds=12​a22sinh−1(sAa222​μ12+Aa22​y2)|s=−μ2−a12a22​μ1s=−μ2−a12a22​μ1+Λ.\begin{split}&-\frac{1}{4\pi}\int_{0}^{\Lambda}\frac{-2\pi}{|(\mu_{1},\mu_{2}-s,y)|_{a}^{\prime}}ds=\frac{1}{2\sqrt{a_{22}}}\sinh^{-1}\left(\frac{s}{\sqrt{\frac{A}{a_{22}^{2}}\mu_{1}^{2}+\frac{A}{a_{22}}y^{2}}}\right)|_{s=-\mu_{2}-\frac{a_{12}}{a_{22}}\mu_{1}}^{s=-\mu_{2}-\frac{a_{12}}{a_{22}}\mu_{1}+\Lambda}.\end{split}

If we subtract 12​a22​log⁡(2​Λ)\frac{1}{2\sqrt{a_{22}}}\log(2\Lambda) and take the limit Λ→∞\Lambda\to\infty, we obtain the function

−12​a22​log⁡(1a22​|(μ1,μ2,y)|a′−μ2−a12a22​μ1)-\frac{1}{2\sqrt{a_{22}}}\log\left(\frac{1}{\sqrt{a_{22}}}|(\mu_{1},\mu_{2},y)|_{a}^{\prime}-\mu_{2}-\frac{a_{12}}{a_{22}}\mu_{1}\right)

which by construction satisfies the same measure equation as (3.7).

We claim that this function differs from α¯1\bar{\alpha}_{1} by a constant. By the Liouville theorem, it suffices to show that the function α¯1\bar{\alpha}_{1} on ℝ2×ℝ\mathbb{R}^{2}\times\mathbb{R} has the logarithmic growth estimate

α¯1≤CA−1/4{log(1+A−3/4ϱ)+|log(1a22−1​μ12+y2)|+1}\bar{\alpha}_{1}\leq CA^{-1/4}\{\log(1+A^{-3/4}\varrho)+|\log(\frac{1}{a_{22}^{-1}\mu_{1}^{2}+y^{2}})|+1\}

which is easy to deduce from Lemma 3.2.

Now to pin down the constant, we can evaluate α¯1\bar{\alpha}_{1} for μ1=μ2=0,y≠0\mu_{1}=\mu_{2}=0,y\neq 0. Then the arctan\arctan term drops out, and

α¯1​(0,0,y)=12​a22​limΛ→+∞{∫0Λ1x2+y2​dx−∑n=1Λ1n}=12​a22​limΛ→∞{sinh−1⁡(Λ|y|)−log⁡Λ−γE}=12​a22​(log⁡(2|y|)−γE)\begin{split}\bar{\alpha}_{1}(0,0,y)&=\frac{1}{2\sqrt{a_{22}}}\lim_{\Lambda\to+\infty}\{\int_{0}^{\Lambda}\frac{1}{\sqrt{x^{2}+y^{2}}}dx-\sum_{n=1}^{\Lambda}\frac{1}{n}\}\\ &=\frac{1}{2\sqrt{a_{22}}}\lim_{\Lambda\to\infty}\{\sinh^{-1}(\frac{\Lambda}{|y|})-\log\Lambda-\gamma_{E}\}\\ &=\frac{1}{2\sqrt{a_{22}}}(\log(\frac{2}{|y|})-\gamma_{E})\end{split}

Comparing the expressions give the formula for α¯1\bar{\alpha}_{1}. ∎

Lemma 3.4.

The difference α~1−α¯1\tilde{\alpha}_{1}-\bar{\alpha}_{1} satisfies the following estimate: if either y2+a22−1​μ12≳1y^{2}+a_{22}^{-1}\mu_{1}^{2}\gtrsim 1 or μ2≲−A1/4\mu_{2}\lesssim-A^{1/4}, namely if distga′​(⋅,𝔇1)≳A1/2\text{dist}_{g_{a}^{\prime}}(\cdot,\mathfrak{D}_{1})\gtrsim A^{1/2}, then |α~1−α¯1|≤CA−1/4|\tilde{\alpha}_{1}-\bar{\alpha}_{1}|\leq CA^{-1/4}. Similar bounds hold for α~i−α¯i\tilde{\alpha}_{i}-\bar{\alpha}_{i} for i=1,2,3i=1,2,3.

Proof.

We notice in advance that α~1\tilde{\alpha}_{1} and α¯1\bar{\alpha}_{1} are periodic in η\eta, so it suffices to assume |x|≤1/2|x|\leq 1/2. The main idea of a variant of Cauchy’s integral test for convergence.

Using the fact that |∂2α1∂x2|≤C​a22(μ12+a22​|η|2)3/2|\frac{\partial^{2}\alpha_{1}}{\partial x^{2}}|\leq C\frac{a_{22}}{(\mu_{1}^{2}+a_{22}|\eta|^{2})^{3/2}}, and the mean value type inequality

f(0)−∫−1/21/2f(s)ds≤Csup|s|≤1/2|f′′(s)|,f(0)-\int_{-1/2}^{1/2}f(s)ds\leq C\sup_{|s|\leq 1/2}|f^{\prime\prime}(s)|,

we deduce that for |η|2+μ12a22≳1|\eta|^{2}+\frac{\mu_{1}^{2}}{a_{22}}\gtrsim 1,

|α1(μ1,μ2,η)−∫x−1/2x+1/2α1(μ1,μ2,s+−1y)ds|≤CA−1/4(|η|2+μ12a22)−3/2|\alpha_{1}(\mu_{1},\mu_{2},\eta)-\int_{x-1/2}^{x+1/2}\alpha_{1}(\mu_{1},\mu_{2},s+\sqrt{-1}y)ds|\leq CA^{-1/4}(|\eta|^{2}+\frac{\mu_{1}^{2}}{a_{22}})^{-3/2}

Thus for |x|≤1/2|x|\leq 1/2,

|∑n∈ℤ∖{0}{α1​(μ1,μ2,η+n)−∫x−1/2x+1/2α1​(μ1,μ2,s+n+−1​y)​ds}|≤CA−1/4∑|n|≠0(|η+n|2+μ12a22)−3/2≤CA−1/4,\begin{split}&|\sum_{n\in\mathbb{Z}\setminus\{0\}}\{\alpha_{1}(\mu_{1},\mu_{2},\eta+n)-\int_{x-1/2}^{x+1/2}\alpha_{1}(\mu_{1},\mu_{2},s+n+\sqrt{-1}y)ds\}|\\ &\leq CA^{-1/4}\sum_{|n|\neq 0}(|\eta+n|^{2}+\frac{\mu_{1}^{2}}{a_{22}})^{-3/2}\leq CA^{-1/4},\end{split}

and the sum converges to zero as μ12+|η|2→∞\mu_{1}^{2}+|\eta|^{2}\to\infty.

In particular if y2+a22−1​μ12≳1y^{2}+a_{22}^{-1}\mu_{1}^{2}\gtrsim 1, then adding the above two inequalities already implies the bound

|α~1−α¯1|=|∑n∈ℤ{α1(μ1,μ2,η+n)−∫x−1/2x+1/2α1(μ1,μ2,s+n+−1y)ds}|≤CA−1/4,\begin{split}|\tilde{\alpha}_{1}-\bar{\alpha}_{1}|&=|\sum_{n\in\mathbb{Z}}\{\alpha_{1}(\mu_{1},\mu_{2},\eta+n)-\int_{x-1/2}^{x+1/2}\alpha_{1}(\mu_{1},\mu_{2},s+n+\sqrt{-1}y)ds\}|\leq CA^{-1/4},\end{split}

and that |α~1−α¯1||\tilde{\alpha}_{1}-\bar{\alpha}_{1}| converges to zero as μ12+|η|2→∞\mu_{1}^{2}+|\eta|^{2}\to\infty.

If however y2+a22−1​μ12≪1y^{2}+a_{22}^{-1}\mu_{1}^{2}\ll 1 but μ2≲−A1/4\mu_{2}\lesssim-A^{1/4}, then we can make

a22​μ2+a12​μ1A1/2​μ12+a22​|η|2≲−1,\frac{a_{22}\mu_{2}+a_{12}\mu_{1}}{A^{1/2}\sqrt{\mu_{1}^{2}+a_{22}|\eta|^{2}}}\lesssim-1,

and the Taylor expansion of arctan\arctan will ensure |α1​(μ1,μ2,η)|≤C−μ2|\alpha_{1}(\mu_{1},\mu_{2},\eta)|\leq\frac{C}{-\mu_{2}}, so

|α1(μ1,μ2,η)−∫x−1/2x+1/2α1(μ1,μ2,s+−1y)ds|≤Cμ2−1≤CA−1/4,|\alpha_{1}(\mu_{1},\mu_{2},\eta)-\int_{x-1/2}^{x+1/2}\alpha_{1}(\mu_{1},\mu_{2},s+\sqrt{-1}y)ds|\leq C\mu_{2}^{-1}\leq CA^{-1/4},

from which we again deduce |α~1−α¯1|≤CA−1/4|\tilde{\alpha}_{1}-\bar{\alpha}_{1}|\leq CA^{-1/4}. ∎

Proposition 3.5.

(Exponential decay for higher Fourier modes in the first order ansatz) If distga′​(⋅,𝔇1)≳A1/2\text{dist}_{g_{a}^{\prime}}(\cdot,\mathfrak{D}_{1})\gtrsim A^{1/2}, then

(3.8) |α~1−α¯1|≤CA−3/4distga′(⋅,𝔇1)exp(−2πA−1/2distga′(⋅,𝔇1)).|\tilde{\alpha}_{1}-\bar{\alpha}_{1}|\leq CA^{-3/4}\text{dist}_{g_{a}^{\prime}}(\cdot,\mathfrak{D}_{1})\exp(-2\pi A^{-1/2}\text{dist}_{g_{a}^{\prime}}(\cdot,\mathfrak{D}_{1})).

Similar bounds hold for α~i−α¯i\tilde{\alpha}_{i}-\bar{\alpha}_{i} for i=1,2,3i=1,2,3.

Proof.

We focus on the region {distga′(⋅,𝔇1)≳A1/2}\{\text{dist}_{g_{a}^{\prime}}(\cdot,\mathfrak{D}_{1})\gtrsim A^{1/2}\}. The key idea is that α~1−α¯1\tilde{\alpha}_{1}-\bar{\alpha}_{1} is Δa\Delta_{a}-harmonic , bounded and has no zero Fourier mode in the S1S^{1} direction defined by the xx-variable, so the exponential decay follows from Fourier analysis. We remark that similar ideas have appeared in the recent paper [13].

We perform Fourier decomposition in the S1S^{1} direction

α~1−α¯1=∑n≠0hn​(μ1,μ2,y)​e2​π​i​n​x,\tilde{\alpha}_{1}-\bar{\alpha}_{1}=\sum_{n\neq 0}h_{n}(\mu_{1},\mu_{2},y)e^{2\pi inx},

Parseval identity combined with Lemma 3.4 shows

∑n|hn|2=∫01|α~1−α¯1|2dx≤CA−1/2.\sum_{n}|h_{n}|^{2}=\int_{0}^{1}|\tilde{\alpha}_{1}-\bar{\alpha}_{1}|^{2}dx\leq CA^{-1/2}.

Now Δa\Delta_{a}-harmonicity translates into the 3-dimensional Helmholtz equations:

Δa′​hn−4​π2​n2​A−1​hn=0.\Delta_{a}^{\prime}h_{n}-4\pi^{2}n^{2}A^{-1}h_{n}=0.

The remaining task is conceptually speaking to estimate the Dirichlet Green’s function for the Helmholtz equation on the noncompact 3-dimensional domain {distga′(⋅,𝔇1)≳A1/2}\{\text{dist}_{g_{a}^{\prime}}(\cdot,\mathfrak{D}_{1})\gtrsim A^{1/2}\}. In practice, building an upper barrier for the Green’s function suffices for our purpose.

Recall ϱ=|(μ1,μ2,y)|a′\varrho=|(\mu_{1},\mu_{2},y)|_{a}^{\prime} is the distance function for the Euclidean metric ga′g_{a}^{\prime} on ℝμ1,μ22×ℝy\mathbb{R}^{2}_{\mu_{1},\mu_{2}}\times\mathbb{R}_{y}. By simple direct computation, for any κ>0\kappa>0,

(Δa′−4​π2​n2​A−1)​e−κ​ϱ≤(κ2−4​π2​n2​A−1)​e−κ​ϱ,(\Delta_{a}^{\prime}-4\pi^{2}n^{2}A^{-1})e^{-\kappa\varrho}\leq(\kappa^{2}-4\pi^{2}n^{2}A^{-1})e^{-\kappa\varrho},

so for kn=2π|n|A−1/2k_{n}=2\pi|n|A^{-1/2}, the function e−kn​ϱe^{-k_{n}\varrho} is a supersolution of the Helmholtz equation. Now we build a barrier function

hn′(μ1,μ2,y)=A−1/2∫0∞e−kn​|(μ1,μ2−s,y)|a′ds,h_{n}^{\prime}(\mu_{1},\mu_{2},y)=A^{-1/2}\int_{0}^{\infty}e^{-k_{n}|(\mu_{1},\mu_{2}-s,y)|_{a}^{\prime}}ds,

whose singularity lies on 𝔇1\mathfrak{D}_{1}. Since hn′h_{n}^{\prime} is a positive superposition of supersolutions, it must be itself a supersolution. Other basic properties are:

  • •

    On {distga′(⋅,𝔇1)≥A1/2}\{\text{dist}_{g_{a}^{\prime}}(\cdot,\mathfrak{D}_{1})\geq A^{1/2}\}, using the saddle point method for Laplace type integrals

    0≤hn′≤CA−3/4distga′(⋅,𝔇1)exp(−kndistga′(⋅,𝔇1)).0\leq h_{n}^{\prime}\leq CA^{-3/4}\text{dist}_{g_{a}^{\prime}}(\cdot,\mathfrak{D}_{1})\exp(-k_{n}\text{dist}_{g_{a}^{\prime}}(\cdot,\mathfrak{D}_{1})).
  • •

    On the boundary of {distga′(⋅,𝔇1)≥A1/2}\{\text{dist}_{g_{a}^{\prime}}(\cdot,\mathfrak{D}_{1})\geq A^{1/2}\}, we have hn′≥A−1/4C​|n|h_{n}^{\prime}\geq\frac{A^{-1/4}}{C|n|}.

Since |hn|≤CA−1/4|h_{n}|\leq CA^{-1/4} by the Parseval identity, the comparison principle implies

hn≤C|n|hn′≤CA−3/4|n|distga′(⋅,𝔇1)exp(−kndistga′(⋅,𝔇1)).\begin{split}h_{n}\leq C|n|h_{n}^{\prime}\leq CA^{-3/4}|n|\text{dist}_{g_{a}^{\prime}}(\cdot,\mathfrak{D}_{1})\exp(-k_{n}\text{dist}_{g_{a}^{\prime}}(\cdot,\mathfrak{D}_{1})).\end{split}

Thus on {distga′(⋅,𝔇1)≥A1/2}\{\text{dist}_{g_{a}^{\prime}}(\cdot,\mathfrak{D}_{1})\geq A^{1/2}\}, the desired bound on |α~1−α¯1||\tilde{\alpha}_{1}-\bar{\alpha}_{1}| follows by summing over these estimates over nn. It is worth commenting that we expect the exponential decay rate to be sharp. ∎

Remark 3.4.

The periodicity condition is responsible for the exponential decay. Its effect becomes significant when η∼1\eta\sim 1, which is compatible with the length scale |μ→|a∼A1/2|\vec{\mu}|_{a}\sim A^{1/2}, or distga′​(⋅,𝔇)∼A1/2\text{dist}_{g_{a}^{\prime}}(\cdot,\mathfrak{D})\sim A^{1/2}. The geometric significance of exponential decay is that the ansatz models the transition from fully quantum into semiflat behaviour (cf. review Section 1.3).

Next we ask for fine asymptote as we move far along 𝔇i\mathfrak{D}_{i}.

Lemma 3.6.

We have the identity

α~1​(μ1,μ2,η)+α~1​(−μ1,−μ2,−η)=12​μ12+a22​|η|2+∑n∈ℤ∖{0}{12​μ12+a22​|η+n|2−12​a22​|n|}\begin{split}&\tilde{\alpha}_{1}(\mu_{1},\mu_{2},\eta)+\tilde{\alpha}_{1}(-\mu_{1},-\mu_{2},-\eta)\\ =&\frac{1}{2\sqrt{\mu_{1}^{2}+a_{22}|\eta|^{2}}}+\sum_{n\in\mathbb{Z}\setminus\{0\}}\{\frac{1}{2\sqrt{\mu_{1}^{2}+a_{22}|\eta+n|^{2}}}-\frac{1}{2\sqrt{a_{22}}|n|}\}\end{split}

where the RHS is recognized as the main part of the complex 2-dimensional Ooguri-Vafa potential. Similarly with 𝔇i\mathfrak{D}_{i} for i=1,2,3i=1,2,3.

Proof.

Clear from α1​(μ1,μ2,η)+α1​(−μ1,−μ2,−η)=12​μ12+a22​|η|2.\alpha_{1}(\mu_{1},\mu_{2},\eta)+{\alpha}_{1}(-\mu_{1},-\mu_{2},-\eta)=\frac{1}{2\sqrt{\mu_{1}^{2}+a_{22}|\eta|^{2}}}. ∎

The utility of this Lemma is that for distga​(⋅,𝔇1)≲A1/2,|μ→|a≳A1/2\text{dist}_{g_{a}}(\cdot,\mathfrak{D}_{1})\lesssim A^{1/2},|\vec{\mu}|_{a}\gtrsim A^{1/2}, namely if we move far from the origin along 𝔇1\mathfrak{D}_{1}, then up to exponentially small errors

α~1​(−μ1,−μ2,−η)∼α¯1​(−μ1,−μ2,−η)=12​a22​{log⁡2−γE−log⁡(1A​|(μ1,μ2,y)|a′+a22A​(μ2+a12a22​μ1))}\begin{split}&\tilde{\alpha}_{1}(-\mu_{1},-\mu_{2},-\eta)\sim\bar{\alpha}_{1}(-\mu_{1},-\mu_{2},-\eta)\\ &=\frac{1}{2\sqrt{a_{22}}}\{\log 2-\gamma_{E}-\log\left(\frac{1}{\sqrt{A}}|(\mu_{1},\mu_{2},y)|_{a}^{\prime}+\frac{\sqrt{a_{22}}}{\sqrt{A}}(\mu_{2}+\frac{a_{12}}{a_{22}}\mu_{1})\right)\}\end{split}

by Proposition 3.5, so the Lemma provides very precise asymptote for α~1​(μ1,μ2,η)\tilde{\alpha}_{1}(\mu_{1},\mu_{2},\eta) along 𝔇1\mathfrak{D}_{1}.

The refined asymptotic behaviour of α~i\tilde{\alpha}_{i} is summarised as

  • •

    Near the origin α~i∼αi\tilde{\alpha}_{i}\sim\alpha_{i}. This is designed to match the asymptote of the Taub-NUT type metric on ℂ3\mathbb{C}^{3} from Chapter 2.

  • •

    Sufficiently far from 𝔇i\mathfrak{D}_{i}, the α~i\tilde{\alpha}_{i} is modelled by an elementary logarithmic function α¯i\bar{\alpha}_{i} up to exponentially small fluctuation.

  • •

    Near 𝔇i\mathfrak{D}_{i} and far from the origin, the α~i\tilde{\alpha}_{i} agrees with the 2-dimensional Ooguri-Vafa potential, up to an elementary logarithmic function and some exponentially small fluctuation.

We comment that although α~i\tilde{\alpha}_{i} is defined globally over ℝμ1,μ22×(S1×ℝ)η\mathbb{R}^{2}_{\mu_{1},\mu_{2}}\times(S^{1}\times\mathbb{R})_{\eta}, the Kähler ansatz is only defined over a finite region and is incomplete, because A+w~A+\tilde{w} becomes negative when α~i∼α¯i≳A1/2\tilde{\alpha}_{i}\sim\bar{\alpha}_{i}\gtrsim A^{1/2}, which happens when log(A−1/2ϱ)≳A3/4.\log(A^{-1/2}\varrho)\gtrsim A^{3/4}. Conversely for a fixed 0<ϵ0≪10<\epsilon_{0}\ll 1 independent of AA, the Kähler ansatz is positive definite on

(3.9) M+={log(A−1/2ϱ)<ϵ0A3/4}.M^{+}=\{\log(A^{-1/2}\varrho)<\epsilon_{0}A^{3/4}\}.

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