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4.12. Special Lagrangian geometry [0473]

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4.12. Special Lagrangian geometry

This Section is an informal discussion concerning special Lagrangian 3-tori L≃T3L\simeq T^{3} on the negative vertex Mν−M^{-}_{\nu}.

The generic special Lagrangian 3-tori LL are expected to be isotopic to the T3T^{3} lying over the 2-tori in the 5-dimensional base defined by

(4.33) (y1,y2,μ)=const.(y_{1},y_{2},\mu)=\text{const}.

The Lagrangian requirement then imposes a homological constraint in the light of Proposition 4.34:

(4.34) ∫T2ω−=Im​(a2​1¯)=0,\int_{T^{2}}\omega_{-}=\text{Im}(a_{2\bar{1}})=0,

or equivalently (ap​q¯)(a_{p\bar{q}}) is real symmetric. The interpretation is that the Ooguri-Vafa type metrics we constructed on the negative vertex can be the metric model for the SYZ fibration only if the homological constraint is satisfied; when this fails, they may still be the local model for other types of degenerating 3-fold Calabi-Yau metrics which do not admit a global special Lagrangian 3-torus fibration.

From now on in this Section we assume the homological constraint, and proceed to speculate on the geometric features of the special Lagrangian 3-tori LL, without attempting to prove existence results.

First, notice that outside a tubular neighbourhood of the singular locus SS, the metric g−g_{-} is a perturbation of the flat model gflatg_{\text{flat}} (cf. Example 1.6), namely the generalised Gibbons-Hawking construction applied to the constant solution

V=A,Wp​q¯=ap​q¯.V=A,\quad W^{p\bar{q}}=a_{p\bar{q}}.

On the flat model it is elementary to check that the map to ℝ3\mathbb{R}^{3} defined by (y1,y2,μ)(y_{1},y_{2},\mu) have special Lagrangian fibres, which are flat 3-tori invariant under the S1S^{1}-action. In other words, to crudest approximation the map

(4.35) Mν−→(y1,y2,μ)ℝ3M^{-}_{\nu}\xrightarrow{(y_{1},y_{2},\mu)}\mathbb{R}^{3}

is an approximate special Lagrangian fibration. Most of these T3T^{3}-fibres stay far away from the curvature radius along SS, so it is likely that in the generic region these T3T^{3} can be perturbed into a genuine special Lagrangian fibration with respect to the Calabi-Yau structure (g−,ω−,J,Ω)(g_{-},\omega_{-},J,\Omega), while maintaining the S1S^{1}-invariance.

Near SS the features of the special Lagrangians LL have strong resonance with Joyce’s work [14] (cf. Section 1.1.5). It is natural to expect LL to be S1S^{1}-invariant. Around P∈SP\in S, the Calabi-Yau structure is transversely modelled on gNUTg_{\text{NUT}} (cf. Section 4.5), so the S1S^{1}-reduction of the special Lagrangian condition

ω−|L=0,Im​(Ω−)|L=0\omega_{-}|_{L}=0,\quad\text{Im}(\Omega_{-})|_{L}=0

approximately reads:

(4.36) {μ=constant,{(A+12​μ2+|ξ1|2)​d​ξ1∧d​ξ¯1+A​d​ξ2∧d​ξ¯2}|L/S1=0,Im​(d​ξ1∧d​ξ2)|L/S1=0.\begin{cases}\mu=\text{constant},\\ \{(A+\frac{1}{2\sqrt{\mu^{2}+|\xi_{1}|^{2}}})d\xi_{1}\wedge d\bar{\xi}_{1}+Ad\xi_{2}\wedge d\bar{\xi}_{2}\}|_{L/S^{1}}=0,\\ \text{Im}(d\xi_{1}\wedge d\xi_{2})|_{L/S^{1}}=0.\end{cases}

To render the analogy with Joyce [14] more transparent, we introduce real variables x~1,x~2,u~1,u~2\tilde{x}_{1},\tilde{x}_{2},\tilde{u}_{1},\tilde{u}_{2} such that ξ1=x~1−−1​u~1,ξ2=x~2+−1​u~2.\xi_{1}=\tilde{x}_{1}-\sqrt{-1}\tilde{u}_{1},\xi_{2}=\tilde{x}_{2}+\sqrt{-1}\tilde{u}_{2}. Representing LL locally by

u~1=u~1​(x~1,x~2),u~2=u~2​(x~1,x~2),μ=constant,\tilde{u}_{1}=\tilde{u}_{1}(\tilde{x}_{1},\tilde{x}_{2}),\quad\tilde{u}_{2}=\tilde{u}_{2}(\tilde{x}_{1},\tilde{x}_{2}),\quad\mu=\text{constant},

then (4.36) takes the form of the nonlinear Cauchy-Riemann equation

(4.37) ∂u~1∂x~1=∂u~2∂x~2,∂u~1∂x~2=−(1+12​A​μ2+x~12+u~12)​∂u~1∂x~2,\frac{\partial\tilde{u}_{1}}{\partial\tilde{x}_{1}}=\frac{\partial\tilde{u}_{2}}{\partial\tilde{x}_{2}},\quad\frac{\partial\tilde{u}_{1}}{\partial\tilde{x}_{2}}=-(1+\frac{1}{2A\sqrt{\mu^{2}+\tilde{x}_{1}^{2}+\tilde{u}_{1}^{2}}})\frac{\partial\tilde{u}_{1}}{\partial\tilde{x}_{2}},

which is very similar to the key equations in [14]. Morever LL should asymptotically match up with fibres of (4.35) at far distance from SS, described by the affine condition (4.33).

We can use this information to speculate on the nature of singularities in line with Joyce [14]. For μ≠0\mu\neq 0 the equations are nonsingular, so the special Lagrangians LL will be smooth. When μ=0\mu=0 the T3T^{3}-fibres of (4.35) intersect SS if and only if (y1,y2)(y_{1},y_{2}) lies in the amoeba Im​(S)\text{Im}(S), and we expect a perturbation of such fibres to produce special Lagrangians LL with singularities. In the subcase where (y1,y2)(y_{1},y_{2}) lies in the interior of the amoeba, there are two transverse intersection points L∩SL\cap S, at which we expect to create a pair of special Lagrangian T2T^{2}-cone singularities. At the boundary of the amoeba these two intersection points merge together, and the singularities disappear outside the amoeba.

The fine details of a special Lagrangian LL near a transverse intersection point with SS is conjecturally modelled by an entire solution to the nonlinear Cauchy-Riemann equation (4.37) over ℝx~1,x~22\mathbb{R}^{2}_{\tilde{x}_{1},\tilde{x}_{2}}, which has a local special Lagrangian T2T^{2}-cone singularity at the origin and is asymptotic to (4.33) at infinity. LL is then obtained by gluing this local picture to the corresponding fibres of (4.35) away from SS.

A salient feature of Joyce [14] is that the special Lagrangian fibration can fail to be defined by smooth maps (cf. Section 1.1.5). This is compatible with this Chapter. The key point is that the absence of an a priori smooth topology forces us to work with tensors of low regularity (cf. Section 4.5), and the smooth structure along SS only emerges a posteriori after solving the Monge-Ampère equation. Thus one neither expects to produce a model special Lagrangian fibration defined by smooth maps, nor expects smoothness properties to persist after perturbation inside function spaces of low regularity.

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