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2.2 Special Lagrangian m -folds in Calabi–Yau m -folds [03KJ]

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2.2 Special Lagrangian mm-folds in Calabi–Yau mm-folds

Now special Lagrangian submanifolds in ℂm\mathbin{\mathbb{C}}^{m} are the local model for special Lagrangian submanifolds in Calabi–Yau manifolds. We adopt the following definition of Calabi–Yau manifolds, which is not the usual one, but will be useful for our purposes.

Definition 2.5 Let m⩾2m\geqslant 2. A Calabi–Yau mm-fold, or CY mm-fold for short, is a quadruple (X,J,ω,Ω)(X,J,\omega,\Omega) such that (X,J)(X,J) is a compact mm-dimensional complex manifold, ω\omega the Kähler form of a Kähler metric gg on XX, and Ω\Omega a non-vanishing holomorphic (m,0)(m,0)-form on XX which satisfies

ωm/m!=(−1)m⁡(m−1)/2​(i/2)m​Ω∧Ω¯.\omega^{m}/m!=(-1)^{m(m-1)/2}(i/2)^{m}\Omega\wedge\bar{\Omega}. (7)

Then for each x∈Xx\in X there exists an isomorphism TxX≅ℂmT_{x}X\cong\mathbin{\mathbb{C}}^{m} that identifies gx,ωxg_{x},\omega_{x} and Ωx\Omega_{x} with the flat versions g,ω,Ωg,\omega,\Omega on ℂm\mathbin{\mathbb{C}}^{m} in (1).

Generally we will refer to a Calabi–Yau mm-fold as XX, taking J,ω,ΩJ,\omega,\Omega as given. Note that if (X,J,ω,Ω)(X,J,\omega,\Omega) is a CY mm-fold and θ∈[0,2​π)\theta\in[0,2\pi) then (X,J,ω,ei​θ​Ω)(X,J,\omega,{\rm e}^{i\theta}\Omega) is also a CY mm-fold. It can be shown that gg is Ricci-flat with holonomy group Hol(g){\textstyle\mathop{\rm Hol}}(g) contained in SU(m)\mathop{\rm SU}(m), and that ∇ω=∇Ω=0\nabla\omega=\nabla\Omega=0, where ∇\nabla is the Levi-Civita connection of gg. Furthermore, as Ω\Omega is a nonvanishing section of the canonical bundle KX=Λm,0​XK_{X}=\Lambda^{m,0}X of XX, we see that KXK_{X} is trivial, so that the first Chern class c1​(X)c_{1}(X) is zero.

Here is how to construct examples of Calabi–Yau manifolds. Using algebraic geometry one can find many examples of compact complex manifolds (X,J)(X,J) with c1​(X)=0c_{1}(X)=0, for instance as hypersurfaces in toric varieties. If XX is simply-connected, KXK_{X} is trivial, and has a nonvanishing holomorphic section Ω\Omega.

If XX admits Kähler metrics, then as c1​(X)=0c_{1}(X)=0 Yau’s solution of the Calabi Conjecture shows that there exists a unique Ricci-flat Kähler metric gg in each Kähler class, with Kähler form ω\omega. It then follows that ∇ω=∇Ω=0\nabla\omega=\nabla\Omega=0, and therefore that ωm\omega^{m} is a constant multiple of Ω∧Ω¯\Omega\wedge\bar{\Omega}. We can rescale Ω\Omega by a constant factor to make (7) hold, and then (X,J,ω,Ω)(X,J,\omega,\Omega) is a CY mm-fold.

We move on to discuss special Lagrangian submanifolds of Calabi–Yau manifolds. Following Definition 2.1, we define:

Definition 2.6 Let (X,J,ω,Ω)(X,J,\omega,\Omega) be a Calabi–Yau mm-fold with metric gg, and NN an oriented real mm-dimensional submanifold of XX. We call NN a special Lagrangian submanifold, or SL mm-fold for short, if NN is calibrated with respect to ReΩ\mathop{\rm Re}\Omega.

Then Proposition 2.3 gives:

Proposition 2.7

Let (X,J,ω,Ω)(X,J,\omega,\Omega) be a Calabi–Yau mm-fold, and NN a real mm-dimensional submanifold of XX. Then there is a unique orientation on NN making it into an SL mm-fold if and only if ω|N≡0\omega|_{N}\equiv 0 and ImΩ|N≡0\mathop{\rm Im}\Omega|_{N}\equiv 0.

Now ω\omega and ImΩ\mathop{\rm Im}\Omega are closed forms on XX, and so if NN is an mm-dimensional submanifold of XX then we can consider the de Rham cohomology classes [ω|N][\omega|_{N}] in H2​(N,ℝ)H^{2}(N,\mathbin{\mathbb{R}}) and [ImΩ|N][\mathop{\rm Im}\Omega|_{N}] in Hm​(N,ℝ)H^{m}(N,\mathbin{\mathbb{R}}). Clearly, by the proposition, these have to be zero for NN to be an SL mm-fold. Furthermore, they are invariant under continuous deformations of NN as a submanifold in XX, and so they have to be zero for any deformation of NN to be special Lagrangian. So we prove:

Corollary 2.8

Let (X,J,ω,Ω)(X,J,\omega,\Omega) be a Calabi–Yau mm-fold, and NN a compact mm-dimensional submanifold of XX. Then there exists a special Lagrangian submanifold N′N^{\prime} of XX isotopic to NN in XX only if [ω|N]=0[\omega|_{N}]=0 in H2​(N,ℝ)H^{2}(N,\mathbin{\mathbb{R}}) and [ImΩ|N]=0[\mathop{\rm Im}\Omega|_{N}]=0 in Hm​(N,ℝ)H^{m}(N,\mathbin{\mathbb{R}}).

This gives us a cohomological obstruction to finding special Lagrangian submanifolds in XX. The deformation theory of special Lagrangian submanifolds was studied by McLean [14, §3], who proved the following result.

Theorem 2.9

Let (X,J,ω,Ω)(X,J,\omega,\Omega) be a Calabi–Yau mm-fold, and NN a compact special Lagrangian submanifold of XX. Then the moduli space ℳ\mathcal{M} of special Lagrangian submanifolds in XX is near NN a smooth manifold of dimension b1​(N)b^{1}(N), the first Betti number of NN.

The idea in the proof of this theorem is that an infinitesimal deformation of NN as a submanifold in XX corresponds to a section of the normal bundle ν\nu of NN in XX. But because NN is Lagrangian, contracting with ω\omega gives an isomorphism between the vector bundles ν\nu and T∗​NT^{*}N over NN. So there is a 1-1 correspondence between infinitesimal deformations of NN in XX and 1-forms α\alpha on NN.

McLean shows that α\alpha corresponds to an infinitesimal deformation of NN as an SL submanifold if and only if d​α=d∗​α=0{\rm d}\alpha={\rm d}^{*}\alpha=0. But as NN is compact, by Hodge theory the vector space of 1-forms α\alpha with d​α=d∗​α=0{\rm d}\alpha={\rm d}^{*}\alpha=0 is isomorphic to H1​(N,ℝ)H^{1}(N,\mathbin{\mathbb{R}}), and so has dimension b1​(N)b^{1}(N).

Our next result concerns the stability of compact special Lagrangian submanifolds NN under small deformations of the underlying Calabi–Yau mm-fold (X,J,ω,Ω)(X,J,\omega,\Omega). McLean does not discuss this question, but it can be answered by the same techniques used to prove Theorem 2.9.

Theorem 2.10

Let (X,J,ω,Ω)(X,J,\omega,\Omega) be a Calabi–Yau mm-fold, and NN a compact special Lagrangian mm-fold in XX. Suppose (X,J~,ω~,Ω~)(X,\tilde{J},\tilde{\omega},\tilde{\Omega}) is a nearby Calabi–Yau structure on XX. Provided (X,J~,ω~,Ω~)(X,\tilde{J},\tilde{\omega},\tilde{\Omega}) is sufficiently close to (X,J,ω,Ω)(X,J,\omega,\Omega), there exists a special Lagrangian mm-fold N~\tilde{N} in (X,J~,ω~,Ω~)(X,\tilde{J},\tilde{\omega},\tilde{\Omega}) close to NN in XX if and only if [ω~|N]=0[\tilde{\omega}|_{N}]=0 in H2​(N,ℝ)H^{2}(N,\mathbin{\mathbb{R}}) and [ImΩ~|N]=0[\mathop{\rm Im}\tilde{\Omega}|_{N}]=0 in Hm​(N,ℝ)H^{m}(N,\mathbin{\mathbb{R}}).

Note that the condition [ω~|N]=0[\tilde{\omega}|_{N}]=0 in H2​(N,ℝ)H^{2}(N,\mathbin{\mathbb{R}}) is automatically satisfied if the image of H2​(N,ℝ)H_{2}(N,\mathbin{\mathbb{R}}) in H2​(X,ℝ)H_{2}(X,\mathbin{\mathbb{R}}) is zero, and the condition [ImΩ~|N]=0[\mathop{\rm Im}\tilde{\Omega}|_{N}]=0 can always be satisfied by choosing the phase of Ω~\tilde{\Omega} correctly. So the conditions [ω~|N]=[ImΩ~|N]=0[\tilde{\omega}|_{N}]=[\mathop{\rm Im}\tilde{\Omega}|_{N}]=0 are often not very stringent.

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