ScalingStacks

6 A class of U ( 1 ) -invariant SL 3-folds in ℂ 3 [03LD]

Original official author HTML, exact retained edition. Historical TeX conversion verdicts remain unchanged. Cited-edition alignment and mathematical self-containment are not assessed.

Complete original source context · Original author HTML

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

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

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

We shall assume that NN may be written

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

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

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

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

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

6.1 Finding the equations on uu and vv

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

Proposition 6.1

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

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

Then

  • (a)

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

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

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

  • (b)

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

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

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

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

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

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

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

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

Lemma 6.2

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

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

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

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

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

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

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

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

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

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

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

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

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

Proposition 6.3

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

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

Proposition 6.4

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

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

Proposition 6.5

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

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

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

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

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

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

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

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

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

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

Lemma 6.6

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

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

Proposition 6.7

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

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

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

  • (a)

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

  • (b)

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

  • (c)

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

  • (d)

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

  • (e)

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

  • (i)

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

  • (ii)

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

  • (iii)

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

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

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

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

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

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

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

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

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

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

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

Proposition 6.8

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

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

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

  • (a)

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

  • (b)

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

  • (c)

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

  • (d)

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

  • (e)

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

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

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

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

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

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

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

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

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

6.4 Isolated singularities of solutions to (32)

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

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

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

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

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

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

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

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

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

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

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

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

Lemma 6.13

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

Here is a conjecture on isolated singularities.

Conjecture 6.14

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

  • (a)

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

  • (b)

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

  • (c)

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

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

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

  • (d)

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

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

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

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

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

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

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

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

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

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

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

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

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

6.5 Geometric interpretation

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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

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