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Closed lagrangian self-shrinkers in \R4\R^{4} symmetric with respect to a hyperplane

Jaehoon Lee Jaehoon Lee, Department of Mathematical Sciences, Seoul National University, Seoul 08826, Korea jaehoon.lee@snu.ac.kr
Abstract.

In this paper, we prove that the closed Lagrangian self-shrinkers in \R4\R^{4} which are symmetric with respect to a hyperplane are given by the products of Abresch-Langer curves. As a corollary, we obtain a new geometric characterization of the Clifford torus as the unique embedded closed Lagrangian self-shrinker symmetric with respect to a hyperplane in \R4\R^{4}.

Key words and phrases:
Lagrangian self-shrinker, Clifford torus, Reflection symmetry, Lawson conjecture, Rigidity
2020 Mathematics Subject Classification:
Primary 53C42; Secondary 53D12

1. Introduction

A self-shrinker of the mean curvature flow is defined to be an immersed submanifold in the Euclidean space, F:Mn\Rn+kF:M^{n}\to\R^{n+k}, which satisfies the quasilinear elliptic system

H=F.\displaystyle\vec{H}=-F^{\perp}. (1.1)

Here, H\vec{H} is the mean curvature vector given by the trace of the second fundamental form and \perp means the projection onto the normal bundle of MnM^{n}.

It is well known that the blow-up limit at the Type I singularity of the mean curvature flow is a self-shrinker. Self-shrinkers themselves also provide self-similar solutions of the mean curvature flow that shrink to the origin. Furthermore, if we consider the Euclidean space as a weighted Riemannian manifold with the Gaussian density e|x|22e^{-\frac{|x|^{2}}{2}}, the solution of (1.1) corresponds to a minimal submanifold in a weighted sense. For these reasons, it is important to understand the geometry of self-shrinkers.

Abresch and Langer [1] completely determined closed self-shrinking planar curves. These curves are called Abresch-Langer curves and note that they have reflection symmetry. Moreover, there is a positive constant associated with each curve so that if two Abresch-Langer curves have the same constants, then they are the same up to a rigid motion (see Lemma 2.1). However, unlike the case of curves, the situation becomes more complicated, so it is hard to expect a complete classification in higher dimensions.

On the other hand, the mean curvature flow preserves the Lagrangian condition in Kähler-Einstein manifolds, including the Euclidean space (see [11]). Since the mean curvature flow corresponds to the negative gradient flow for a volume functional, it provides a potential way to obtain a volume minimizer. For instance, special Lagrangian submanifolds are volume minimizing in a Calabi-Yau manifold, so the Lagrangian mean curvature flow plays a significant role in the construction of these examples. However, the development of finite-time singularities is the main difficulty of this method (see for instance [9]). Therefore, in order to manage possible singularities, it is necessary to study Lagrangian self-shrinkers.

In this paper, we consider Lagrangian self-shrinkers in \R42\R^{4}\simeq\mathbb{C}^{2}. Since Lagrangian self-shrinking sphere cannot exist by the theorem of Smoczyk [12], the simplest example is the surface of genus 1. Many immersed Lagrangian self-shrinking tori were constructed: products of Abresch-Langer curves, Anciaux’s tori (see [2]), and Lee-Wang’s tori (see [6], [7]).

One interesting observation we would like to emphasize is that all known embedded examples of closed Lagrangian self-shrinkers in 2\mathbb{C}^{2} become the Clifford torus. This is not true in n\mathbb{C}^{n}(n3n\geq 3) since two or more different embedded Lagrangian self-shrinkers can be found in Anciaux’s examples (see [2]). Moreover, as the normal and tangent bundles of a Lagrangian submanifold are diffeomorphic and the self-intersection number is given by the Euler characteristic of the normal bundle, one can conclude that embedded Lagrangian surfaces in 2\mathbb{C}^{2} should have genus 1. Therefore, it is natural to ask whether the Clifford torus is the only embedded example in 2\mathbb{C}^{2}:

Question 1.1.

Is the Clifford torus unique as an embedded Lagrangian self-shrinker in 2\mathbb{C}^{2}?

This question is analogous to Lawson’s conjecture that whether the Clifford torus is the only embedded minimal torus in S3S^{3}. The Lawson conjecture was proved by Brendle [3], by clever use of the maximum principle for two-point functions on a given surface. However, due to the increased codimension, it is not easy to apply the maximum principle in our case. But, assuming a particular symmetry condition, we obtain a positive answer for Question 1.1.

Before we state the main results, we recall some rigidity results on the Clifford torus as a Lagrangian self-shrinker. Castro and Lerma [4] characterized Lee-Wang’s tori as compact Hamiltonian stationary Lagrangian self-shrinkers in 2\mathbb{C}^{2} and the Clifford torus was characterized as the only embedded example among them. In [5], they proved that if a compact Lagrangian self-shrinker satisfies either |H|2=const|\vec{H}|^{2}=const or |H|22|\vec{H}|^{2}\leq 2 or |H|22|\vec{H}|^{2}\geq 2, then it is the Clifford torus. They also proved that a compact Lagrangian self-shrinker without change of sign on the Gauss curvature and satisfying |σ|22|\sigma|^{2}\leq 2 is the Clifford torus. Here, σ\sigma denotes the second fundamental form. Then Li and Wang [8] generalized previous results into two directions: the Clifford torus is the unique compact Lagrangian self-shrinker with |σ|22|\sigma|^{2}\leq 2, and if a compact Lagrangian self-shrinker has no sign change on the Gauss curvature, then it is one of the products of Abresch-Langer curves.

Now we recall the result of Ros related to Lawson’s conjecture, which states that the Clifford torus is the unique embedded minimal torus in S3S^{3} symmetric with respect to four pairwise orthogonal hyperplanes in \R4\R^{4} (see Theorem 6 in [10]). Since the almost complex structure does not commute with reflections in general, we could expect that there would be a non-trivial restriction on a Lagrangian submanifold if we assume the reflection symmetry. Motivated by this, we study Lagrangian self-shrinkers symmetric with respect to a hyperplane in \R4\R^{4}.

Then we have the following theorem.

Theorem 1.2.

Let F:Σ2\R42F:\Sigma^{2}\to\R^{4}\simeq\mathbb{C}^{2} be a closed Lagrangian self-shrinker symmetric with respect to a hyperplane PP. Then Σ2\Sigma^{2} is given by the product of two Abresch-Langer curves.

We remark that it requires only one hyperplane of symmetry in Theorem 1.2, while Ros’ theorem assumed four orthogonal hyperplanes of symmetry. For the proof of Theorem 1.2, we were not able to apply the method of Ros [10] due to the high codimension. Instead, we observe that each Lagrangian self-shrinker with reflection symmetry satisfies global relations which are similar to transcendental relations (2.4) on Abresch-Langer curves (see Proposition 4.3). By using such relations, we prove that Σ2\Sigma^{2} is flat. Then, by the result of Li and Wang (see Proposition 2.2), we could finish the proof. We also show that global relations on a product of Abresch-Langer curves coincide with the transcendental relation on each curve.

Since the Clifford torus is the only embedded self-shrinker among the products of Abresch-Langer curves, we obtain a new geometric characterization of the Clifford torus as a Lagrangian self-shrinker:

Theorem 1.3.

A closed embedded Lagrangian self-shrinker symmetric with respect to a hyperplane in \R4\R^{4} is the Clifford torus.

The paper is organized as follows. In Section 2 we provide some basic definitions and show that a hyperplane of symmetry can be assumed to be the coordinate hyperplane {x1=0}\{x_{1}=0\} in a way that preserves the Lagrangian condition. We also recall two previous results that play an important role in this paper. In the next section, we compute local equations for Lagrangian self-shrinkers with reflection symmetry in terms of isothermal coordinates. Then we obtain global relations in Section 4. Finally, we prove the main results in Section 5.

Acknowledgements

The author would like to express his gratitude to Jaigyoung Choe for helpful discussions and thoughtful encouragement. This work was supported in part by NRF-2018R1A2B6004262.

2. Preliminaries

Identify \R4\R^{4} with 2\mathbb{C}^{2} via (x1,x2,x3,x4)(x1+ix2,x3+ix4)\left(x_{1},x_{2},x_{3},x_{4}\right)\leftrightarrow\left(x_{1}+ix_{2},x_{3}+ix_{4}\right), where i=1i=\sqrt{-1}. We use the almost complex structure JJ on \R4\R^{4} which corresponds to the multiplication of ii in 2\mathbb{C}^{2}. Let ,\left\langle\ ,\ \right\rangle be the standard hermitian product in 2\mathbb{C}^{2}. Then the Euclidean inner product in \R4\R^{4} is given by the real part of ,\left\langle\ ,\ \right\rangle under the identification.

The Kähler form ω\omega on (\R4,J)\left(\R^{4},J\right) is given by

ω=dx1dx2+dx3dx4,\displaystyle\omega=\textup{d}x_{1}\wedge\textup{d}x_{2}+\textup{d}x_{3}\wedge\textup{d}x_{4},

where xix_{i}’s are coordinate functions of \R4\R^{4}. An immersion F:Σ2\R4F:\Sigma^{2}\to\R^{4} is called a Lagrangian if

Fω=0,\displaystyle F^{*}\omega=0, (2.1)

and we call F:Σ2\R4F:\Sigma^{2}\to\R^{4} a Lagrangian self-shrinker if it satisfies (1.1) and the Lagrangian condition (2.1).

For arbitrary pΣp\in\Sigma, one can always find local isothermal coordinates xx, yy in a neighborhood of pp such that

|Fx|=|Fy|,FxFy,\displaystyle|F_{x}|=|F_{y}|,\ F_{x}\perp F_{y}, (2.2)

where the lower indices denote partial derivatives. In terms of the isothermal coordinates, the Lagrangian condition (2.1) is equivalent to

JFxFy.\displaystyle JF_{x}\perp F_{y}. (2.3)

Now let F:Σ2\R4F:\Sigma^{2}\to\R^{4} be a Lagrangian self-shrinker symmetric with respect to a hyperplane PP. First, we claim that PP contains the origin OO. Indeed, by the reflection symmetry, Σ\Sigma and its reflected surface shrink to the same point along the mean curvature flow. As the surface shrinks to the origin, OO should be invariant under the reflection, which implies that OPO\in P.

Let ν\R42\nu\in\R^{4}\simeq\mathbb{C}^{2} be the unit normal vector of PP. Then there exists a unitary matrix GU(2)G\in U(2) such that

Gν=(1,0)2.\displaystyle G\cdot\nu=(1,0)\in\mathbb{C}^{2}.

The unitary group U(2)U(2) can be identified as a subgroup of O(4)O(4) consisting of elements which commute with JJ, so there is an orthogonal transformation G~O(4)\tilde{G}\in O(4) corresponding to GG. Then G~\tilde{G} sends PP to the coordinate hyperplane {x1=0}\{x_{1}=0\}. Moreover, it preserves Lagrangian submanifolds since it commutes with JJ. Thus, G~F:Σ2\R4\tilde{G}\circ F:\Sigma^{2}\to\R^{4} is a Lagrangian self-shrinker symmetric to {x1=0}\{x_{1}=0\}. Therefore it suffices to consider Lagrangian self-shrinkers F:Σ2\R4F:\Sigma^{2}\to\R^{4} symmetric with respect to {x1=0}\{x_{1}=0\}. This family of self-shrinkers will be denoted by \mathscr{F}.

Lagrangian self-shrinkers with reflection symmetry can be easily found in the products of Abresch-Langer curves. For later use, we recall two results on Abresch-Langer curves and their product self-shrinkers. The first result is about the transcendental relation on those curves (see Theorem A in [1] and Lemma 5.3 in [13]).

Lemma 2.1 (Lemma 5.3 in [13]).

Let Γ\R2\Gamma\subset\R^{2} be one of the Abresch-Langer curves. Then there exists a positive constant cΓc_{\Gamma} such that

ker22=cΓ\displaystyle ke^{-\frac{r^{2}}{2}}=c_{\Gamma} (2.4)

holds everywhere on Γ\Gamma, where rr is the distance from the origin and kk is the curvature. If two Abresch-Langer curves Γ1\Gamma_{1} and Γ2\Gamma_{2} have the same constants, i.e., cΓ1=cΓ2c_{\Gamma_{1}}=c_{\Gamma_{2}}, then (up to a rigid motion) Γ1=Γ2\Gamma_{1}=\Gamma_{2}. Moreover, the critical values kck_{c} of the curvature kk satisfy kcekc22=cΓk_{c}e^{-\frac{k_{c}^{2}}{2}}=c_{\Gamma}.

The second one is about the characterization of products of Abresch-Langer curves as Lagrangian self-shrinkers with constant Gauss curvature in \R4\R^{4} (see Proposition 5.6 in [8]).

Proposition 2.2 (Proposition 5.6 in [8]).

Let F:Σ2\R4F:\Sigma^{2}\to\R^{4} be a compact Lagrangian self-shrinker with constant Gauss curvature KK. Then K=0K=0 and Σ2\Sigma^{2} is given by the product of two Abresch-Langer curves.

Throughout this paper, the gradient and Laplacian on a given surface will be denoted by \nabla and Δ\Delta, respectively.

3. Local Equations

Let F:Σ2\R42F:\Sigma^{2}\to\R^{4}\simeq\mathbb{C}^{2} be a closed Lagrangian self-shrinker symmetric with respect to {x1=0}\{x_{1}=0\}, i.e., FF\in\mathscr{F}. Using isothermal coordinates, we obtain the following local equations:

Proposition 3.1.

Suppose that F:Σ22F:\Sigma^{2}\to\mathbb{C}^{2} is given by F=(A,B)F=(A,B) for some complex-valued functions AA and BB. Then

  1. (1)

    |Ax|=|By||A_{x}|=|B_{y}|, |Ay|=|Bx||A_{y}|=|B_{x}|,

  2. (2)

    AxAy¯+BxBy¯=0A_{x}\bar{A_{y}}+B_{x}\bar{B_{y}}=0, and AxAy¯A_{x}\bar{A_{y}}, BxBy¯B_{x}\bar{B_{y}} are real-valued,

  3. (3)

    (ΔA+A)Ax¯(\Delta A+A)\bar{A_{x}}, (ΔA+A)Ay¯(\Delta A+A)\bar{A_{y}}, (ΔB+B)Bx¯(\Delta B+B)\bar{B_{x}}, (ΔB+B)By¯(\Delta B+B)\bar{B_{y}} are real-valued,

hold true on all of Σ2\Sigma^{2}, where x,yx,y are local isothermal coordinates.

Proof.

Since the coordinates are assumed to be isothermal, from (2.2) we have

FxFy\displaystyle F_{x}\perp F_{y} Re(AxAy¯+BxBy¯)=0,\displaystyle\Leftrightarrow\mbox{Re}(A_{x}\bar{A_{y}}+B_{x}\bar{B_{y}})=0, (3.1)
|Fx|2=|Fy|2\displaystyle|F_{x}|^{2}=|F_{y}|^{2} |Ax|2+|Bx|2=|Ay|2+|By|2,\displaystyle\Leftrightarrow|A_{x}|^{2}+|B_{x}|^{2}=|A_{y}|^{2}+|B_{y}|^{2}, (3.2)

and the Lagrangian condition (2.3) implies

JFxFy\displaystyle JF_{x}\perp F_{y} Re(iAxAy¯+iBxBy¯)=0Im(AxAy¯+BxBy¯)=0.\displaystyle\Leftrightarrow\mbox{Re}(iA_{x}\bar{A_{y}}+iB_{x}\bar{B_{y}})=0\Leftrightarrow\mbox{Im}(A_{x}\bar{A_{y}}+B_{x}\bar{B_{y}})=0. (3.3)

Combining (3.1) and (3.3), we obtain

AxAy¯+BxBy¯=0,\displaystyle A_{x}\bar{A_{y}}+B_{x}\bar{B_{y}}=0, (3.4)

and then with (3.2), we conclude that

|Ax|=|By|,|Ay|=|Bx|.\displaystyle|A_{x}|=|B_{y}|,\ |A_{y}|=|B_{x}|. (3.5)

On the other hand, since Σ2\Sigma^{2} has the reflection symmetry with respect to x1x_{1}-hyperplane, the same equations hold when we replace AA by A¯-\bar{A}.

Now substituting AA by A¯-\bar{A} in (3.4) gives

Ax¯Ay+BxBy¯=0.\displaystyle\bar{A_{x}}A_{y}+B_{x}\bar{B_{y}}=0. (3.6)

Hence we get AxAy¯=Ax¯AyA_{x}\bar{A_{y}}=\bar{A_{x}}A_{y} and BxBy¯=Bx¯ByB_{x}\bar{B_{y}}=\bar{B_{x}}B_{y} from (3.4) and (3.6), which imply that AxAy¯A_{x}\bar{A_{y}} and BxBy¯B_{x}\bar{B_{y}} are real-valued.

In order to prove (3), we compute each term in (1.1), H=F\vec{H}=-F^{\perp}, directly. Let λ|Fx|2=|Fy|2\lambda\coloneqq|F_{x}|^{2}=|F_{y}|^{2}. As {1λFx,1λFy}\left\{\frac{1}{\sqrt{\lambda}}F_{x},\frac{1}{\sqrt{\lambda}}F_{y}\right\} form an orthonormal frame, the mean curvature vector can be expressed as

H\displaystyle\vec{H} =(ΔF)\displaystyle=\left(\Delta F\right)^{\perp}
=ΔFReΔF,FxλFxReΔF,FyλFy\displaystyle=\Delta F-\frac{\mbox{Re}\langle\Delta F,F_{x}\rangle}{\lambda}F_{x}-\frac{\mbox{Re}\langle\Delta F,F_{y}\rangle}{\lambda}F_{y}
=(ΔARe(ΔAAx¯+ΔBBx¯)λAxRe(ΔAAy¯+ΔBBy¯)λAy,\displaystyle=\left(\Delta A-\frac{\mbox{Re}(\Delta A\bar{A_{x}}+\Delta B\bar{B_{x}})}{\lambda}A_{x}-\frac{\mbox{Re}(\Delta A\bar{A_{y}}+\Delta B\bar{B_{y}})}{\lambda}A_{y},\right.
ΔBRe(ΔAAx¯+ΔBBx¯)λBxRe(ΔAAy¯+ΔBBy¯)λBy),\displaystyle\left.\ \ \ \ \ \ \ \Delta B-\frac{\mbox{Re}(\Delta A\bar{A_{x}}+\Delta B\bar{B_{x}})}{\lambda}B_{x}-\frac{\mbox{Re}(\Delta A\bar{A_{y}}+\Delta B\bar{B_{y}})}{\lambda}B_{y}\right), (3.7)

and similarly the normal part of the position vector is given by

F\displaystyle F^{\perp} =FReF,FxλFxReF,FyλFy\displaystyle=F-\frac{\mbox{Re}\langle F,F_{x}\rangle}{\lambda}F_{x}-\frac{\mbox{Re}\langle F,F_{y}\rangle}{\lambda}F_{y}
=(ARe(AAx¯+BBx¯)λAxRe(AAy¯+BBy¯)λAy,\displaystyle=\left(A-\frac{\mbox{Re}(A\bar{A_{x}}+B\bar{B_{x}})}{\lambda}A_{x}-\frac{\mbox{Re}(A\bar{A_{y}}+B\bar{B_{y}})}{\lambda}A_{y},\right.
BRe(AAx¯+BBx¯)λBxRe(AAy¯+BBy¯)λBy).\displaystyle\left.\ \ \ \ \ \ \ B-\frac{\mbox{Re}(A\bar{A_{x}}+B\bar{B_{x}})}{\lambda}B_{x}-\frac{\mbox{Re}(A\bar{A_{y}}+B\bar{B_{y}})}{\lambda}B_{y}\right). (3.8)

Let u~Ax¯Ay\tilde{u}\coloneqq\bar{A_{x}}A_{y}, which is a real-valued function. Clearly, BxBy¯=u~B_{x}\bar{B_{y}}=-\tilde{u}, by (3.4). From (3.5), |Ay|=|Bx||A_{y}|=|B_{x}|, we may write

λ=|Ax|2+|Ay|2.\displaystyle\lambda=|A_{x}|^{2}+|A_{y}|^{2}.

Since FF is an immersion, λ0\lambda\neq 0 and either Ax0A_{x}\neq 0 or Ay0A_{y}\neq 0 hold. In both cases, a similar argument applies, so we may assume that Ax0A_{x}\neq 0. Then we have the following relations:

Ay=uAx,Bx=uBy,\displaystyle A_{y}=uA_{x},\ B_{x}=-uB_{y},

where uu~|Ax|2u\coloneqq\frac{\tilde{u}}{|A_{x}|^{2}} is also real-valued. By the above relations,

Re(ΔAAx¯+ΔBBx¯)Ax+Re(ΔAAy¯+ΔBBy¯)Ay\displaystyle\mbox{Re}(\Delta A\bar{A_{x}}+\Delta B\bar{B_{x}})A_{x}+\mbox{Re}(\Delta A\bar{A_{y}}+\Delta B\bar{B_{y}})A_{y}
=Re(ΔAAx¯uΔBBy¯)Ax+Re(uΔAAx¯+ΔBBy¯)(uAx)\displaystyle=\mbox{Re}(\Delta A\bar{A_{x}}-u\Delta B\bar{B_{y}})A_{x}+\mbox{Re}(u\Delta A\bar{A_{x}}+\Delta B\bar{B_{y}})(uA_{x})
=(1+u2)Re(ΔAAx¯)Ax\displaystyle=(1+u^{2})\mbox{Re}(\Delta A\bar{A_{x}})A_{x}
=λ|Ax|2Re(ΔAAx¯)Ax,\displaystyle=\frac{\lambda}{|A_{x}|^{2}}\mbox{Re}(\Delta A\bar{A_{x}})A_{x},

and we compute

ΔARe(ΔAAx¯+ΔBBx¯)λAxRe(ΔAAy¯+ΔBBy¯)λAy=(ΔAAx¯ΔA¯Ax)2|Ax|2Ax.\displaystyle\Delta A-\frac{\mbox{Re}(\Delta A\bar{A_{x}}+\Delta B\bar{B_{x}})}{\lambda}A_{x}-\frac{\mbox{Re}(\Delta A\bar{A_{y}}+\Delta B\bar{B_{y}})}{\lambda}A_{y}=\frac{(\Delta A\bar{A_{x}}-\Delta\bar{A}A_{x})}{2|A_{x}|^{2}}A_{x}.

By applying similar computations to (3.7) and (3.8), we obtain

H=((ΔAAx¯ΔA¯Ax)2|Ax|2Ax,(ΔBBy¯ΔB¯By)2|By|2By)\displaystyle\vec{H}=\left(\frac{(\Delta A\bar{A_{x}}-\Delta\bar{A}A_{x})}{2|A_{x}|^{2}}A_{x},\ \frac{(\Delta B\bar{B_{y}}-\Delta\bar{B}B_{y})}{2|B_{y}|^{2}}B_{y}\right)

and

F=((AAx¯A¯Ax)2|Ax|2Ax,(BBy¯B¯By)2|By|2By).\displaystyle F^{\perp}=\left(\frac{(A\bar{A_{x}}-\bar{A}A_{x})}{2|A_{x}|^{2}}A_{x},\ \frac{(B\bar{B_{y}}-\bar{B}B_{y})}{2|B_{y}|^{2}}B_{y}\right).

Consequently, (1.1), H=F\vec{H}=-F^{\perp}, is equivalent to

(ΔA+A)Ax¯=(ΔA¯+A¯)Ax\displaystyle(\Delta A+A)\bar{A_{x}}=(\Delta\bar{A}+\bar{A})A_{x}

and

(ΔB+B)By¯=(ΔB¯+B¯)By,\displaystyle(\Delta B+B)\bar{B_{y}}=(\Delta\bar{B}+\bar{B})B_{y},

which imply that (ΔA+A)Ax¯(\Delta A+A)\bar{A_{x}} and (ΔB+B)By¯(\Delta B+B)\bar{B_{y}} are real-valued. Since AxAy¯A_{x}\bar{A_{y}} and BxBy¯B_{x}\bar{B_{y}} are also real-valued, (3) is proved. ∎

4. Global Relations

In this section, we prove that Lagrangian self-shrinkers in \mathscr{F} have a special property analogous to the transcendental relation on Abresch-Langer curves as in Lemma 2.1. From local equations in Proposition 3.1, we obtain the following lemma:

Lemma 4.1.

With the same notation in Proposition 3.1, suppose that |A|>0|A|>0 in a neighborhood of pΣ2p\in\Sigma^{2}. Let A=reiθA=re^{i\theta} be a locally given polar representation of AA. Then r4|θ|2=Cer2r^{4}|\nabla\theta|^{2}=Ce^{r^{2}} for some constant CC.

Proof.

By a straightforward calculation, we have

Ax=(rx+irθx)eiθ,Ay=(ry+irθy)eiθ,\displaystyle A_{x}=\left(r_{x}+ir\theta_{x}\right)e^{i\theta},\ A_{y}=\left(r_{y}+ir\theta_{y}\right)e^{i\theta},

where x,yx,y are isothermal coordinates. It then follows from (2) in Proposition 3.1

Im(AxAy¯)r=θxryrxθy=0,\displaystyle\frac{\mbox{Im}(A_{x}\bar{A_{y}})}{r}=\theta_{x}r_{y}-r_{x}\theta_{y}=0,

which implies that r\nabla r and θ\nabla\theta are linearly dependent. Moreover, |r|2+r2|θ|2=1|\nabla r|^{2}+r^{2}|\nabla\theta|^{2}=1 implies that either |r|0|\nabla r|\neq 0 or |θ|0|\nabla\theta|\neq 0. We treat both cases separately as follows.

First, assume that |r|0|\nabla r|\neq 0. We may write θ=μr\nabla\theta=\mu\nabla r for some function μ\mu. From this we derive

Δθ=μΔr+μr,\displaystyle\Delta\theta=\mu\Delta r+\nabla\mu\cdot\nabla r,

and we compute

ΔA+A\displaystyle\Delta A+A =(Δr+rr|θ|2+2irθ+irΔθ)eiθ\displaystyle=\left(\Delta r+r-r|\nabla\theta|^{2}+2i\nabla r\cdot\nabla\theta+ir\Delta\theta\right)e^{i\theta}
=(Δr+rrμ2|r|2+2iμ|r|2+irμΔr+irrμ)eiθ.\displaystyle=\left(\Delta r+r-r\mu^{2}|\nabla r|^{2}+2i\mu|\nabla r|^{2}+ir\mu\Delta r+ir\nabla r\cdot\nabla\mu\right)e^{i\theta}.

Thus,

(ΔA+A)Ax¯\displaystyle(\Delta A+A)\bar{A_{x}}
=(Δr+rrμ2|r|2+2iμ|r|2+irμΔr+irrμ)(rxirθx)\displaystyle=\left(\Delta r+r-r\mu^{2}|\nabla r|^{2}+2i\mu|\nabla r|^{2}+ir\mu\Delta r+ir\nabla r\cdot\nabla\mu\right)\left(r_{x}-ir\theta_{x}\right)
=(Δr+(r+r3μ2rμ2)|r|2+2iμ|r|2+irμΔr+irrμ)(1irμ)rx,\displaystyle=\left(\Delta r+(r+r^{3}\mu^{2}-r\mu^{2})|\nabla r|^{2}+2i\mu|\nabla r|^{2}+ir\mu\Delta r+ir\nabla r\cdot\nabla\mu\right)\left(1-ir\mu\right)r_{x},

where we used 1=(1+r2μ2)|r|21=\left(1+r^{2}\mu^{2}\right)|\nabla r|^{2} and θx=μrx\theta_{x}=\mu r_{x} in the last equality.

Taking the imaginary part, we deduce from (3) in Proposition 3.1 that

Im((ΔA+A)Ax¯)=0\displaystyle\mbox{Im}\left((\Delta A+A)\bar{A_{x}}\right)=0
(rrμ+(2μr2μ+r2μ3r4μ3)|r|2)rx=0.\displaystyle\Leftrightarrow\left(r\nabla r\cdot\nabla\mu+\left(2\mu-r^{2}\mu+r^{2}\mu^{3}-r^{4}\mu^{3}\right)|\nabla r|^{2}\right)r_{x}=0. (4.1)

By a similar computation, we also have

Im((ΔA+A)Ay¯)=0\displaystyle\mbox{Im}\left((\Delta A+A)\bar{A_{y}}\right)=0
(rrμ+(2μr2μ+r2μ3r4μ3)|r|2)ry=0.\displaystyle\Leftrightarrow\left(r\nabla r\cdot\nabla\mu+\left(2\mu-r^{2}\mu+r^{2}\mu^{3}-r^{4}\mu^{3}\right)|\nabla r|^{2}\right)r_{y}=0. (4.2)

Since |r|0|\nabla r|\neq 0, (4) and (4) imply that

rrμ+(2μr2μ+r2μ3r4μ3)|r|2=0.\displaystyle r\nabla r\cdot\nabla\mu+\left(2\mu-r^{2}\mu+r^{2}\mu^{3}-r^{4}\mu^{3}\right)|\nabla r|^{2}=0. (4.3)

On the other hand, θxy=μyrx+μrxy=μxry+μryx=θyx\theta_{xy}=\mu_{y}r_{x}+\mu r_{xy}=\mu_{x}r_{y}+\mu r_{yx}=\theta_{yx} implies

μyrxμxry=0.\displaystyle\mu_{y}r_{x}-\mu_{x}r_{y}=0.

Then μ\nabla\mu and r\nabla r are linearly dependent so that (4.3) is equivalent to

rμ+(2μr2μ+r2μ3r4μ3)r=0.\displaystyle r\nabla\mu+\left(2\mu-r^{2}\mu+r^{2}\mu^{3}-r^{4}\mu^{3}\right)\nabla r=0. (4.4)

Now we use (4.4) to compute

(r2μe12r21+r2μ2)\displaystyle\nabla\left(\frac{r^{2}\mu}{e^{\frac{1}{2}r^{2}}\sqrt{1+r^{2}\mu^{2}}}\right)
=e12r21+r2μ2(2rμr+r2μ)r2μ(re12r21+r2μ2r+e12r2r2μμ+rμ2r1+r2μ2)er2(1+r2μ2)\displaystyle=\frac{e^{\frac{1}{2}r^{2}}\sqrt{1+r^{2}\mu^{2}}\left(2r\mu\nabla r+r^{2}\nabla\mu\right)-r^{2}\mu\left(re^{\frac{1}{2}r^{2}}\sqrt{1+r^{2}\mu^{2}}\nabla r+e^{\frac{1}{2}r^{2}}\frac{r^{2}\mu\nabla\mu+r\mu^{2}\nabla r}{\sqrt{1+r^{2}\mu^{2}}}\right)}{e^{r^{2}}\left(1+r^{2}\mu^{2}\right)}
=(1+r2μ2)(2rμr+r2μ)r3μ(1+r2μ2)rr4μ2μr3μ3re12r2(1+r2μ2)32\displaystyle=\frac{\left(1+r^{2}\mu^{2}\right)\left(2r\mu\nabla r+r^{2}\nabla\mu\right)-r^{3}\mu\left(1+r^{2}\mu^{2}\right)\nabla r-r^{4}\mu^{2}\nabla\mu-r^{3}\mu^{3}\nabla r}{e^{\frac{1}{2}r^{2}}\left(1+r^{2}\mu^{2}\right)^{\frac{3}{2}}}
=re12r2(1+r2μ2)32(rμ+(2μr2μ+r2μ3r4μ3)r)\displaystyle=\frac{r}{e^{\frac{1}{2}r^{2}}\left(1+r^{2}\mu^{2}\right)^{\frac{3}{2}}}\left(r\nabla\mu+\left(2\mu-r^{2}\mu+r^{2}\mu^{3}-r^{4}\mu^{3}\right)\nabla r\right)
=0.\displaystyle=0.

Therefore we conclude that

(r2μe12r21+r2μ2)2=r4μ2er2(1+r2μ2)=r4|θ|2er2\displaystyle\left(\frac{r^{2}\mu}{e^{\frac{1}{2}r^{2}}\sqrt{1+r^{2}\mu^{2}}}\right)^{2}=\frac{r^{4}\mu^{2}}{e^{r^{2}}\left(1+r^{2}\mu^{2}\right)}=\frac{r^{4}|\nabla\theta|^{2}}{e^{r^{2}}}

is a constant.

For the case |θ|0|\nabla\theta|\neq 0, there exists a function η\eta such that r=ηθ\nabla r=\eta\nabla\theta. Then, a similar argument yields

(r2e12r2r2+η2)=0,\displaystyle\nabla\left(\frac{r^{2}}{e^{\frac{1}{2}r^{2}}\sqrt{r^{2}+\eta^{2}}}\right)=0,

which again implies that

(r2e12r2r2+η2)2=r4er2(r2+η2)=r4|θ|2er2\displaystyle\left(\frac{r^{2}}{e^{\frac{1}{2}r^{2}}\sqrt{r^{2}+\eta^{2}}}\right)^{2}=\frac{r^{4}}{e^{r^{2}}(r^{2}+\eta^{2})}=\frac{r^{4}|\nabla\theta|^{2}}{e^{r^{2}}}

is a constant. ∎

Next, we prove that the constant in the previous lemma cannot be zero.

Lemma 4.2.

For pΣ2p\in\Sigma^{2} with |A|>0|A|>0, let r4|θ|2=Cer2r^{4}|\nabla\theta|^{2}=Ce^{r^{2}} at pp. Then C>0C>0.

Proof.

Suppose that there exists a point pΣ2p\in\Sigma^{2} such that |A|>0|A|>0 and r4|θ|2=0r^{4}|\nabla\theta|^{2}=0 at pp. Let Ω\Omega be the connected component of Σ2{|A|>0}\Sigma^{2}\cap\{|A|>0\} which contains pp. Then Lemma 4.1 implies that Ω\Omega is an open set and locally every point shares the same constant in the above lemma. From the connectedness of Ω\Omega, we conclude that all points of Ω\Omega share the same constant. Hence r4|θ|2=0r^{4}|\nabla\theta|^{2}=0 in Ω\Omega.

Since r=|A|>0r=|A|>0 in Ω\Omega, we have |θ|=0|\nabla\theta|=0 in Ω\Omega. Let γ=γ(t)\gamma=\gamma(t) be the integral curve of r\nabla r with γ(0)=p\gamma(0)=p. Then

r(γ(T))r(γ(0))\displaystyle r(\gamma(T))-r(\gamma(0)) =0Tddtr(γ(t))dt\displaystyle=\int_{0}^{T}\frac{\textup{d}}{\textup{d}t}r(\gamma(t))\textup{d}t
=0Tr(γ(t))γ˙(t)dt\displaystyle=\int_{0}^{T}\nabla r(\gamma(t))\cdot\dot{\gamma}(t)\textup{d}t
=0T|r|2dt=T,\displaystyle=\int_{0}^{T}|\nabla r|^{2}\textup{d}t\ =\ T,

where we used |r|2=|r|2+r2|θ|2=1|\nabla r|^{2}=|\nabla r|^{2}+r^{2}|\nabla\theta|^{2}=1 in the last equality.

If the integral curve stays inside Ω\Omega, then rr increases along the curve by the amount of TT increases. This is impossible since rr is bounded on Σ2\Sigma^{2}. Thus, we may deduce that γ(t)\gamma(t) approaches the boundary point of Ω\Omega. However, by the definition of Ω\Omega, rr should vanish at the boundary point. This is also a contradiction as rr is continuous and increases along γ\gamma. Therefore, such pΣ2p\in\Sigma^{2} does not exist. ∎

Finally, we obtain the following proposition.

Proposition 4.3 (Global Relations).

Let F:Σ22F:\Sigma^{2}\to\mathbb{C}^{2} be a closed Lagrangian self-shrinker in \mathscr{F}, given by F=(A,B)F=(A,B). Then, |A|>0|A|>0 and |B|>0|B|>0 on Σ2\Sigma^{2}. Moreover, there exist constants C1,C2>0C_{1},\ C_{2}>0 such that

r14|θ1|2=C1er12,r24|θ2|2=C2er22\displaystyle r_{1}^{4}|\nabla\theta_{1}|^{2}=C_{1}e^{r_{1}^{2}},\ r_{2}^{4}|\nabla\theta_{2}|^{2}=C_{2}e^{r_{2}^{2}} (4.5)

on all of Σ2\Sigma^{2}, where A=r1eiθ1A=r_{1}e^{i\theta_{1}} and B=r2eiθ2B=r_{2}e^{i\theta_{2}} are polar representations.

Proof.

If |A||A| vanishes at every point of Σ2\Sigma^{2}, then Σ2\Sigma^{2} should be contained in a 22-plane. It is impossible, so there exists a point pΣ2p\in\Sigma^{2} with |A|>0|A|>0. Then, by Lemma 4.1 and 4.2, there exists a positive constant C1C_{1} such that r14|θ1|2=C1er12r_{1}^{4}|\nabla\theta_{1}|^{2}=C_{1}e^{r_{1}^{2}} in a neighborhood of pp.

Let UU be the maximal subset of Σ2\Sigma^{2} consisting of points which share the same constant C1C_{1}, i.e., r14|θ1|2=C1er12r_{1}^{4}|\nabla\theta_{1}|^{2}=C_{1}e^{r_{1}^{2}} in UU. Since pUp\in U by the definition of C1C_{1}, UU is non-empty. Moreover, by Lemma 4.1, there exists a neighborhood for each point qUq\in U such that all points in the neighborhood share the same constant. Thus, UU is an open set.

Next, we prove that UU is also a closed subset by proving U=\partial U=\emptyset. Suppose the contrary. That is, assume that xUx\in\partial U. If r1(x)>0r_{1}(x)>0, then by Lemma 4.1 and 4.2, there exists a neighborhood of xx, VV, and a positive constant C0C_{0} such that r14|θ1|2=C0er12r_{1}^{4}|\nabla\theta_{1}|^{2}=C_{0}e^{r_{1}^{2}} in VV. By the definition of the boundary point, we have VUV\cap U\neq\emptyset and VUcV\cap U^{c}\neq\emptyset. From VUV\cap U\neq\emptyset, we deduce that C0=C1C_{0}=C_{1}. This implies that VUV\subseteq U and VUc=V\cap U^{c}=\emptyset, which is a contradiction. Thus, r1(x)=0r_{1}(x)=0.

On the other hand, from |r1|2+r12|θ1|2=1|\nabla r_{1}|^{2}+r_{1}^{2}|\nabla\theta_{1}|^{2}=1 we derive

|12r12|2=r12C1er120\displaystyle|\nabla\frac{1}{2}r_{1}^{2}|^{2}=r_{1}^{2}-C_{1}e^{r_{1}^{2}}\geq 0

in UU. The last inequality holds, if and only if

C11e\displaystyle C_{1}\leq\frac{1}{e}

and

rmin(C1)r1rmax(C1),\displaystyle r_{min}(C_{1})\leq r_{1}\leq r_{max}(C_{1}),

where rmin(C1)r_{min}(C_{1}) and rmax(C1)r_{max}(C_{1}) are two solutions of r2=C1er2r^{2}=C_{1}e^{r^{2}}.

By the continuity of r1r_{1}, we conclude that 0=r1(x)rmin(C1)>00=r_{1}(x)\geq r_{min}(C_{1})>0, which is a contradiction. Therefore U=\partial U=\emptyset and UU is closed.

Since UU is a non-empty open and closed subset in the connected surface, UU must be equal to Σ2\Sigma^{2} and we deduce that r14|θ1|2=C1er12r_{1}^{4}|\nabla\theta_{1}|^{2}=C_{1}e^{r_{1}^{2}} on all of Σ2\Sigma^{2}. The same method can be applied to BB and we finish the proof. ∎

Remark 4.4.

Although θ1\theta_{1} and θ2\theta_{2} are defined up to multiples of 2π2\pi, θ1\nabla\theta_{1} and θ2\nabla\theta_{2} are well-defined on Σ2\Sigma^{2}.

Next, we compute explicit constants on products of Abresch-Langer curves. All self-shrinkers in this family have reflection symmetry so that Proposition 4.3 can be applied. We observe that each constant coincides with the one that appeared in Lemma 2.1. The precise computation would be done as follows.

Let Γ1\Gamma_{1} and Γ2\Gamma_{2} be the Abresch-Langer curves associated with the constants cΓ1c_{\Gamma_{1}} and cΓ2c_{\Gamma_{2}} as in Lemma 2.1. Suppose Γ1\Gamma_{1} and Γ2\Gamma_{2} are given by γ1(s)\gamma_{1}(s) and γ2(t)\gamma_{2}(t), respectively, where ss and tt are arc-length parametrizations. Consider the Lagrangian self-shrinker Γ1×Γ2\R2×\R2=\R4\Gamma_{1}\times\Gamma_{2}\subset\R^{2}\times\R^{2}=\R^{4}. If we write γ1(s)=r1(s)eiθ1(s)\gamma_{1}(s)=r_{1}(s)e^{i\theta_{1}(s)}, then

|γ1˙|2=r1˙2+r12θ1˙2=1,\displaystyle|\dot{\gamma_{1}}|^{2}=\dot{r_{1}}^{2}+r_{1}^{2}\dot{\theta_{1}}^{2}=1, (4.6)

where the upper dot denotes the derivative with respect to ss. As Γ1×Γ2\R4\Gamma_{1}\times\Gamma_{2}\subset\R^{4} is given by the product, we have

|θ1|2=θ1˙2\displaystyle|\nabla\theta_{1}|^{2}=\dot{\theta_{1}}^{2}

so that

C1r14|θ1|2er12=r14θ1˙2er12=r12(1r1˙2)er12,\displaystyle C_{1}\coloneqq\frac{r_{1}^{4}|\nabla\theta_{1}|^{2}}{e^{r_{1}^{2}}}=\frac{r_{1}^{4}\dot{\theta_{1}}^{2}}{e^{r_{1}^{2}}}=\frac{r_{1}^{2}(1-\dot{r_{1}}^{2})}{e^{r_{1}^{2}}}, (4.7)

where we have used (4.6) in the last step. A direct computation gives

γ1=γ1Re(γ1γ1˙¯)γ1˙=(r1(1r1˙2)ir12r1˙θ1˙)eiθ1,\displaystyle\gamma_{1}^{\perp}=\gamma_{1}-\mbox{Re}(\gamma_{1}\bar{\dot{\gamma_{1}}})\dot{\gamma_{1}}=\big{(}r_{1}(1-\dot{r_{1}}^{2})-ir_{1}^{2}\dot{r_{1}}\dot{\theta_{1}}\big{)}e^{i\theta_{1}},

and then with (4.6), we obtain

kΓ12=|γ1¨|2=|γ1|2=r12(1r1˙2)2+r14r1˙2θ1˙2=r12(1r1˙2).\displaystyle k_{\Gamma_{1}}^{2}=|\ddot{\gamma_{1}}|^{2}=|\gamma_{1}^{\perp}|^{2}=r_{1}^{2}(1-\dot{r_{1}}^{2})^{2}+r_{1}^{4}\dot{r_{1}}^{2}\dot{\theta_{1}}^{2}=r_{1}^{2}(1-\dot{r_{1}}^{2}). (4.8)

We deduce from (4.7) and (4.8) that

C1=r12(1r1˙2)er12=kΓ12er12=cΓ12,\displaystyle C_{1}=\frac{r_{1}^{2}(1-\dot{r_{1}}^{2})}{e^{r_{1}^{2}}}=\frac{k_{\Gamma_{1}}^{2}}{e^{r_{1}^{2}}}=c_{\Gamma_{1}}^{2},

and similarly C2=cΓ22C_{2}=c_{\Gamma_{2}}^{2}.

5. Proof of the Main Results

In this section, we prove the main results of this paper.

Proof of Theorem 1.2.

We may assume that FF\in\mathscr{F}. Let pΣ2p\in\Sigma^{2} and suppose that the immersion is given by F(x,y)=(A(x,y),B(x,y))F(x,y)=(A(x,y),B(x,y)), where xx and yy are isothermal coordinates near pp. By Propostion 4.3, |A||A| and |B||B| never vanish on Σ2\Sigma^{2} and we may consider polar representations in a neighborhood of pp as follows:

A(x,y)=r1(x,y)eiθ1(x,y),B(x,y)=r2(x,y)eiθ2(x,y).\displaystyle A(x,y)=r_{1}(x,y)e^{i\theta_{1}(x,y)},\ B(x,y)=r_{2}(x,y)e^{i\theta_{2}(x,y)}.

Again by Proposition 4.3, we know that |θ1|>0|\nabla\theta_{1}|>0 and |θ2|>0|\nabla\theta_{2}|>0.

Then, as in the proof of Lemma 4.1, there exist functions η1\eta_{1} and η2\eta_{2} such that

r1=η1θ1,r2=η2θ2.\displaystyle\nabla r_{1}=\eta_{1}\nabla\theta_{1},\ \nabla r_{2}=\eta_{2}\nabla\theta_{2}. (5.1)

From (1) and (2) in Proposition 3.1, we derive

|Ax|=|By|\displaystyle|A_{x}|=|B_{y}| (η12+r12)θ1x2=(η22+r22)θ2y2,\displaystyle\Leftrightarrow(\eta_{1}^{2}+r_{1}^{2})\theta_{1x}^{2}=(\eta_{2}^{2}+r_{2}^{2})\theta_{2y}^{2},
|Ay|=|Bx|\displaystyle|A_{y}|=|B_{x}| (η12+r12)θ1y2=(η22+r22)θ2x2,\displaystyle\Leftrightarrow(\eta_{1}^{2}+r_{1}^{2})\theta_{1y}^{2}=(\eta_{2}^{2}+r_{2}^{2})\theta_{2x}^{2},
AxAy¯+BxBy¯=0\displaystyle A_{x}\bar{A_{y}}+B_{x}\bar{B_{y}}=0 (η12+r12)θ1xθ1y+(η22+r22)θ2xθ2y=0,\displaystyle\Leftrightarrow(\eta_{1}^{2}+r_{1}^{2})\theta_{1x}\theta_{1y}+(\eta_{2}^{2}+r_{2}^{2})\theta_{2x}\theta_{2y}=0,

which gives

θ1xθ2x+θ1yθ2y=0.\displaystyle\theta_{1x}\theta_{2x}+\theta_{1y}\theta_{2y}=0.

Therefore we conclude that

θ1θ2=0.\displaystyle\nabla\theta_{1}\cdot\nabla\theta_{2}=0. (5.2)

Since θ1\nabla\theta_{1} and θ2\nabla\theta_{2} are non-vanishing and orthogonal, θ1\theta_{1} and θ2\theta_{2} give rise to local coordinates near pp. In terms of θ1\theta_{1} and θ2\theta_{2}, we may write A=r1(θ1,θ2)eiθ1A=r_{1}(\theta_{1},\theta_{2})e^{i\theta_{1}}. Then, by (5.1) and (5.2),

r1θ2=η1θ1θ2=0.\displaystyle\nabla r_{1}\cdot\nabla\theta_{2}=\eta_{1}\nabla\theta_{1}\cdot\nabla\theta_{2}=0.

This proves that r1r_{1} is independent of θ2\theta_{2}. Similarly

r2θ1=η2θ2θ1=0,\displaystyle\nabla r_{2}\cdot\nabla\theta_{1}=\eta_{2}\nabla\theta_{2}\cdot\nabla\theta_{1}=0,

and r2r_{2} is independent of θ1\theta_{1}.

Therefore we proved that Σ2\Sigma^{2} is locally given by the product of two curves, parametrized by θ1\theta_{1} and θ2\theta_{2}, respectively, in a neighborhood of pp. This implies that Σ2\Sigma^{2} is flat at pp. Since pp was arbitrary, we conclude that Σ2\Sigma^{2} is flat. Then, by the result of Li and Wang (see Proposition 2.2), Σ2\Sigma^{2} is the product of two Abresch-Langer curves. ∎

The unit circle is the only embedded curve in the examples of Abresch and Langer. Therefore we can characterize the Clifford torus as the unique embedded self-shrinker in the products of Abresch-Langer curves, and Theorem 1.3 follows directly from Theorem 1.2.

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