1: why is it called mirror symmetry?
Mirror symmetry is a proposed duality between symplectic geometry and complex geometry. In one of its most familiar forms, it starts with a Calabi--Yau manifold \(X\) and predicts another Calabi--Yau manifold \(\check X\), called a mirror, whose complex geometry records symplectic information about \(X\) and whose symplectic geometry records complex information about \(X\). The mirror is not determined by the Hodge numbers alone; the Hodge-number symmetry is the first visible numerical shadow of a stronger correspondence. This slogan is a useful entry point into the more categorical form of mirror symmetry discussed in HMS for Fanos. In the Calabi--Yau setting, the mirror symmetry conjectures predict two related kinds of data:- to a suitable symplectic or Kähler Calabi--Yau manifold \(X\), a complex Calabi--Yau manifold \(\check X\) called a mirror of \(X\);
- a dictionary translating symplectic invariants of \(X\) into complex invariants of \(\check X\), and conversely.
definition 0.0.1
In these notes, a Calabi--Yau \(n\)-fold is a compact connected Kähler manifold \(X\) of complex dimension \(n\) whose canonical bundle \[ K_X:=\Lambda^n(T^{1,0}X)^* \] is holomorphically trivial. Equivalently, \(X\) admits a nowhere-vanishing holomorphic volume form \[ \Omega\in H^0(X,K_X). \] Thus a Calabi--Yau manifold carries compatible complex and symplectic data:- an integrable complex structure \(J:TX\to TX\);
- a Kähler form \(\omega\in \Omega^2(X)\), which in particular makes \(X\) a symplectic manifold;
- a holomorphic volume form \(\Omega\) trivializing \(K_X\).
theorem 0.0.2
Let \((X,J)\) be a compact Kähler manifold of complex dimension \(n\) with \(c_1(TX)=0\) in \(H^2(X;\RR)\). For every Kähler class \[ \alpha\in H^{1,1}(X;\RR) \] there is a unique Kähler form \(\omega\in\alpha\) whose Ricci form is zero. If \(K_X\) is holomorphically trivial, then with respect to this metric a nowhere-vanishing holomorphic \(n\)-form is parallel, and the holonomy is contained in \(SU(n)\). Conversely, a Kähler metric with holonomy contained in \(SU(n)\) is Ricci-flat and admits a parallel nowhere-vanishing holomorphic \(n\)-form.0.1: Hodge diamond and deformation
definition 0.0.3
This definition uses the Hodge decomposition. The Hodge diamond of a compact Kähler manifold \(X\) of complex dimension \(n\) is the array of Hodge numbers \(h^{p,q}(X)=\dim_{\CC}H^{p,q}(X)\) arranged so that entries with fixed \(p+q\) lie on the same row and reflection across the vertical axis interchanges the two indices. Thus the row indexed by \(k\) contains the numbers corresponding to the summands in \[ H^k(X;\CC)=\bigoplus_{p+q=k}H^{p,q}(X). \] For a threefold, the diamond has rows \[ \begin{array}{ccccccc} &&& h^{0,0} &&&\\ && h^{1,0} && h^{0,1} &&\\ & h^{2,0} && h^{1,1} && h^{0,2} &\\ h^{3,0} && h^{2,1} && h^{1,2} && h^{0,3}\\ & h^{3,1} && h^{2,2} && h^{1,3} &\\ && h^{3,2} && h^{2,3} &&\\ &&& h^{3,3} &&& \end{array} \] The diamond is not extra structure beyond the Hodge decomposition; it is a compact way of displaying the dimensions of its summands.- complex conjugation gives \[ h^{p,q}(X)=h^{q,p}(X); \]
- Serre duality gives \[ h^{p,q}(X)=h^{n-p,n-q}(X); \]
- together, these equalities imply that the usual Hodge diamond is symmetric across both the vertical and horizontal axes.
0.0.1: \(h^{1,1}\) and the K\"ahler cone
definition 0.0.4
Let \(X\) be a compact Kähler manifold. Under the Hodge decomposition, the real \((1,1)\)-cohomology is \[ H^{1,1}(X;\RR):=H^{1,1}(X;\CC)\cap H^2(X;\RR). \] The K\"ahler cone of \(X\) is \[ \mathcal K_X :=\{[\omega]_{\mathrm{dR}}\in H^{1,1}(X;\RR)\mid \omega \text{ is a Kähler form on }X\}. \] It is an open convex cone in \(H^{1,1}(X;\RR)\). A point of \(\mathcal K_X\) is the de Rham cohomology class of a compatible symplectic form on the fixed complex manifold \(X\). In mirror symmetry one often uses the complexified K\"ahler parameter \[ [B]+i[\omega]\in H^2(X;\CC), \] where \([B]\in H^2(X;\RR)\) is usually considered modulo integral classes.0.0.2: \(h^{2,1}\) and complex deformation
definition 0.0.1
Let \(X\) be a compact complex manifold. A first-order deformation of the complex structure on \(X\) is a flat deformation of \(X\) over the dual numbers \(\CC[\epsilon]/(\epsilon^2)\), together with an identification of the special fiber with \(X\). Equivalence classes of first-order deformations are naturally identified with the Kodaira--Spencer group \[ H^1(X,T_X), \] where \(T_X=T^{1,0}X\) is the holomorphic tangent bundle. Analytically, after choosing a splitting, a nearby almost complex structure may be represented by a Beltrami differential \[ s\in \Omega^{0,1}(X,T_X). \] The integrability condition is the Maurer--Cartan equation \[ \bar\partial s+\frac{1}{2}[s,s]=0. \] To first order this reduces to \(\bar\partial s=0\), and infinitesimal changes of coordinates change \(s\) by elements of \(\bar\partial\Omega^0(X,T_X)\). Thus the Zariski tangent space to the deformation functor or Kuranishi space is \(H^1(X,T_X)\), while obstruction classes naturally take values in \(H^2(X,T_X)\).- The condition that the new almost complex structure be integrable is the Maurer--Cartan equation \[ \bar\partial s+\frac{1}{2}[s,s]=0. \] To first order, this becomes \(\bar\partial s=0\).
- Some deformations of complex structure arise from pulling back by a diffeomorphism. Infinitesimally, these lie in the image of \[ \bar\partial: \Omega^0(X,T_X^{1,0})\to \Omega^{0,1}(X,T_X^{1,0}). \]
- Therefore, the space of first-order deformations of complex structure is \[ \frac{\ker(\bar\partial: \Omega^{0,1}(X,T_X^{1,0})\to \Omega^{0,2}(X,T_X^{1,0}))} {\operatorname{im}(\bar\partial: \Omega^{0}(X,T_X^{1,0})\to \Omega^{0,1}(X,T_X^{1,0}))} =H^{0,1}(X,T_X^{1,0})=H^1(X,T_X). \] On a Calabi--Yau \(n\)-fold, contraction with a holomorphic volume form identifies \(T_X\) with \(\Omega_X^{n-1}\). Thus \[ H^1(X,T_X)\simeq H^1(X,\Omega_X^{n-1})\simeq H^{n-1,1}(X). \] For a Calabi--Yau threefold, this is \(H^{2,1}(X)\).
0.2: the mirror flip
This is the elementary origin of the name ``mirror symmetry.'' If \(X\) and \(\check X\) are mirror Calabi--Yau \(n\)-folds, then the expected numerical relation is \[ h^{p,q}(X)=h^{n-p,q}(\check X). \] For Calabi--Yau threefolds satisfying the simplifying vanishing used above, this says in particular that variations of Kähler or symplectic structure on \(X\) should correspond to variations of complex structure on \(\check X\), and conversely. Since the dimensions of these two deformation spaces are governed by Hodge numbers, one expects \[ h^{1,1}(X)=h^{2,1}(\check X),\qquad h^{2,1}(X)=h^{1,1}(\check X). \] Pictorially, for threefolds this mirror relation exchanges the vertical \(h^{1,1}\) entries with the horizontal \(h^{2,1}\) entries:2: constructing mirror manifolds and implications
The Hodge-number flip explains the name, but it does not yet explain where the mirror should come from. The next layer of the story is constructive: one tries to build the mirror family by degenerating \(X\) to a combinatorial, toric, or affine limit, dualizing the relevant data, and then smoothing the result. The constructions below are schematic, but the point is precise: mirror symmetry is usually a statement about matched families near boundary points of moduli, not just about two isolated manifolds.1.1: constructing mirrors
The first examples of mirror symmetry involved Calabi--Yau hypersurfaces in projective space. Let \(H\subset \CP^n\) be a smooth hypersurface of degree \(d\), so \(H\) has complex dimension \(n-1\). We can compute its first Chern class using the exact sequence \[ 0 \to T^{1,0}H\to T^{1,0}\CP^n|_H\to N_{H/\CP^n}\to 0. \] This tells us that \[ c(T\CP^n)|_H=c(TH)\cdot c(N_{H/\CP^n}). \] Suppose that the hypersurface has degree \(d\), and let \(h=c_1(\mathcal O_{\CP^n}(1))|_H\). Then \[ c(T\CP^n)|_H=(1+h)^{n+1},\qquad c(N_{H/\CP^n})=1+dh. \] Therefore, \[ 1+(n+1)h+\cdots=(1+c_1(TH)+\cdots)(1+dh), \] so \[ c_1(TH)=(n+1-d)h. \] Equivalently, by adjunction, \[ K_H\simeq \mathcal O_H(d-n-1). \] Thus \(d=n+1\) is necessary and sufficient for \(H\) to have trivial canonical bundle. If \(H\) is smooth, a degree \(n+1\) hypersurface in \(\CP^n\) is a compact Kähler manifold with trivial canonical bundle, hence is Calabi--Yau in the sense of definition 0.0.1. The quintic threefold in \(\CP^4\) is the standard example.definition 1.0.1
Let \[ \pi:\mathcal X^*\to \Delta^* \] be a one-parameter family of Calabi--Yau \(n\)-folds over a punctured disc. Parallel transport around the puncture gives a monodromy operator \[ T:H^n(X_t;\QQ)\to H^n(X_t;\QQ). \] After replacing the punctured disc by a finite cover if necessary, assume that the monodromy is unipotent, and write \(T\) for this unipotent monodromy. Then one can define \[ N:=\log T=(T-I)-\frac{(T-I)^2}{2}+\frac{(T-I)^3}{3}-\cdots . \] The series is finite because \(T-I\) is nilpotent. In this introductory convention, a boundary point \(t=0\) is called a large complex-structure limit, or a maximally unipotent monodromy point, if \[ N^n\neq 0 \] on \(H^n(X_t;\QQ)\). Equivalently, \(N\) has nilpotency index \(n+1\), the maximum possible for a weight-\(n\) variation of Hodge structure. More refined definitions also impose conditions on the limiting mixed Hodge structure; the maximally unipotent monodromy criterion is the part used in this introductory discussion.- find a toric or toroidal degeneration of the family to \(X_0\);
- construct a mirror degeneration \(\check X_0\) using the dual toric or affine-combinatorial data;
- deform or smooth \(\check X_0\) to obtain the mirror family \(\check{\mathcal X}\), and match the deformation parameters using the mirror map.
- The SYZ proposal interprets mirror symmetry as fiberwise \(T\)-duality, which suggests looking at dual tori.
- Homological mirror symmetry suggests that a Lagrangian torus fiber equipped with a flat unitary local system should correspond to a skyscraper sheaf at a point of the mirror. Thus torus fibrations are natural objects to examine.
- The topological calculation below shows why dualizing torus fibers exchanges the two Hodge numbers.
definition 1.0.2
Let \((X,\omega,\Omega)\) be a Calabi--Yau \(n\)-fold with its Ricci-flat Kähler metric, and assume that \(\Omega\) is normalized with respect to this metric. For \(\theta\in \RR/2\pi\ZZ\), an oriented real \(n\)-dimensional submanifold \(L\subset X\) is special Lagrangian of phase \(\theta\) if \[ \omega|_L=0,\qquad \operatorname{Im}(e^{-i\theta}\Omega)|_L=0, \] and \[ \operatorname{Re}(e^{-i\theta}\Omega)|_L=\operatorname{vol}_L \] as positive volume forms on \(L\). A special Lagrangian torus fibration of phase \(\theta\) is a continuous map \[ f:X\to B \] to a real \(n\)-dimensional base such that, over a dense open subset \(B_0\subset B\), the restriction \[ f^{-1}(B_0)\to B_0 \] is a smooth fiber bundle whose fibers are \(n\)-tori that are special Lagrangian submanifolds of phase \(\theta\). In the SYZ setting, nontrivial compact examples are expected to have singular fibers over a discriminant locus \(\Delta=B\setminus B_0\).definition 1.0.3
Let \[ f:X_0\to B_0 \] be a smooth torus fibration with fibers \(F_b\simeq V_b/\Lambda_b\), where \(V_b\) is a real vector space and \(\Lambda_b\subset V_b\) is a lattice. The dual torus fibration is \[ \check f:\check X_0\to B_0, \qquad \check F_b:=\check f^{-1}(b)=\operatorname{Hom}(\Lambda_b,U(1)) \simeq H^1(F_b;\RR)/H^1(F_b;\ZZ). \] Fiberwise, \[ H_1(\check F_b;\ZZ)\simeq H^1(F_b;\ZZ), \qquad H^1(\check F_b;\ZZ)\simeq H_1(F_b;\ZZ). \] If the three-torus fibers are oriented, then Poincar\'e duality, with respect to the chosen orientations, gives the useful identifications \[ H^1(\check F_b;\CC)\simeq H^2(F_b;\CC), \qquad H^2(\check F_b;\CC)\simeq H^1(F_b;\CC). \] These fiberwise identifications induce the corresponding dual local systems over \(B_0\).3: where to go from here?
If mirror symmetry relates deformations of symplectic structures to deformations of complex structures, then symplectic and complex invariants should have related deformation theories. One of the original predictions of mirror symmetry was an equality between two different Yukawa couplings.definition 2.0.1
We use the genus-zero Gromov--Witten invariants from genus-zero Gromov--Witten invariant. Let \(X\) be a smooth projective Calabi--Yau threefold. The \(A\)-model Yukawa coupling is the formal trilinear form on divisor classes \(\alpha_1,\alpha_2,\alpha_3\in H^{1,1}(X;\CC)\) given by \[ \langle \alpha_1,\alpha_2,\alpha_3\rangle_A = \int_X\alpha_1\wedge\alpha_2\wedge\alpha_3 + \sum_{0\neq \beta\in H_2(X;\ZZ)_{\mathrm{eff}}} \langle \alpha_1,\alpha_2,\alpha_3\rangle_{0,\beta}\,q^\beta. \] The first term is the classical triple intersection product. The remaining terms are genus-zero Gromov--Witten quantum corrections. If the complexified Kähler parameter is \([B]+i[\omega]\), then one common convention is \[ q^\beta=\exp\left(2\pi i\int_\beta(B+i\omega)\right). \] Different sign conventions for \(q^\beta\) appear in the literature.definition 2.0.2
Let \(\check X\) be a compact Calabi--Yau threefold, and choose a nowhere-vanishing holomorphic volume form \(\Omega\). The \(B\)-model Yukawa coupling associated to \(\Omega\) is the symmetric trilinear form on first-order complex-structure deformations \[ H^1(\check X,T_{\check X})^{\otimes 3}\to \CC \] defined by \[ \langle a_1,a_2,a_3\rangle_B = \int_{\check X}\Omega\wedge \big((a_1\wedge a_2\wedge a_3)\lrcorner\,\Omega\big). \] Here the \(a_i\) may be represented by \((0,1)\)-forms with values in \(T_{\check X}\), and contraction with \(\Omega\) identifies the \(\wedge^3T_{\check X}\) factor with \(\mathcal O_{\check X}\). In a family, these couplings can be described equivalently in terms of the variation of Hodge structure on \(H^3(\check X)\).definition 2.0.3
Let \(X\) and \(\check X\) be a proposed mirror pair of Calabi--Yau manifolds. Given chosen boundary points in the complexified Kähler moduli of \(X\) and the complex-structure moduli of \(\check X\), a mirror map is a local analytic or formal identification of the corresponding parameter spaces: \[ \text{complexified Kähler parameters of }X \quad\leftrightarrow\quad \text{complex-structure parameters of }\check X. \] Depending on convention, either this identification or its inverse is called the mirror map. Near a large-radius limit on the \(A\)-side and a large complex-structure limit on the \(B\)-side, this identification is usually normalized using flat coordinates on the \(B\)-model side obtained from periods of the holomorphic volume form on \(\check X\). It is the coordinate change used to compare \(A\)-model structures on \(X\) with \(B\)-model structures on \(\check X\).Connections
Uses
- why is it called mirror symmetry?article / art:whyMirrorSymmetryIntro
- constructing mirror manifolds and implicationsarticle / art:constructingMirrorManifolds
- where to go from here?article / art:mirrorSymmetryYukawaCouplings
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