ConceptComplete

Moduli Spaces - Core Definitions

Moduli spaces parametrize families of geometric objects, encoding how structures can vary while preserving essential properties. For Calabi-Yau manifolds, the moduli spaces of Kähler and complex structures form the geometric foundation for mirror symmetry.

DefinitionModuli Space

A moduli space M\mathcal{M} for a class of geometric objects is a space whose points correspond to isomorphism classes of those objects. Local coordinates on M\mathcal{M} parametrize continuous families of deformations.

For a moduli problem to be well-posed, we require:

  1. A notion of family (flat morphisms)
  2. An equivalence relation (isomorphism)
  3. Representability or existence of a coarse moduli space

For Calabi-Yau threefolds XX, two primary moduli spaces arise naturally from the geometry. The complex structure moduli space Mc\mathcal{M}_c parametrizes complex structures preserving the Calabi-Yau condition, while the Kähler moduli space MK\mathcal{M}_K parametrizes Kähler forms modulo diffeomorphism.

DefinitionComplex Structure Moduli Space

The complex structure moduli space Mc\mathcal{M}_c of a Calabi-Yau manifold XX is the space of complex structures on the underlying smooth manifold that preserve c1=0c_1 = 0, modulo diffeomorphisms isotopic to the identity.

The tangent space at a point [X]Mc[X] \in \mathcal{M}_c is: T[X]McH1(X,TX)H2,1(X)T_{[X]}\mathcal{M}_c \cong H^1(X, T_X) \cong H^{2,1}(X)

where the isomorphism follows from Dolbeault cohomology and Serre duality.

The dimension of Mc\mathcal{M}_c equals h2,1(X)h^{2,1}(X) near smooth points. Infinitesimal deformations are controlled by the Kodaira-Spencer map, which associates to each tangent vector a class in H1(X,TX)H^1(X,T_X).

DefinitionKähler Moduli Space

The Kähler moduli space MK\mathcal{M}_K parametrizes Kähler classes [ω]H1,1(X,R)[\omega] \in H^{1,1}(X,\mathbb{R}) with ω\omega a positive (1,1)(1,1)-form. The tangent space is: T[ω]MKH1,1(X,R)T_{[\omega]}\mathcal{M}_K \cong H^{1,1}(X,\mathbb{R})

The dimension of MK\mathcal{M}_K is h1,1(X)h^{1,1}(X).

The Kähler cone KXH1,1(X,R)\mathcal{K}_X \subset H^{1,1}(X,\mathbb{R}) consists of classes [ω][\omega] representable by Kähler forms. This is an open convex cone whose boundary corresponds to degenerate geometries.

Remark

The total moduli space M=Mc×MK\mathcal{M} = \mathcal{M}_c \times \mathcal{M}_K has dimension h2,1+h1,1h^{2,1} + h^{1,1}. Mirror symmetry exchanges these two factors: for a mirror pair (X,X)(X, X^\vee), the complex structure moduli of XX correspond to Kähler moduli of XX^\vee and vice versa.

ExampleQuintic Threefold Moduli

For the quintic threefold X5X_5, we have h2,1=101h^{2,1} = 101 and h1,1=1h^{1,1} = 1. Thus dimMc=101\dim\mathcal{M}_c = 101 while dimMK=1\dim\mathcal{M}_K = 1. The mirror quintic X5X_5^\vee has h2,1=1h^{2,1} = 1 and h1,1=101h^{1,1} = 101, demonstrating the moduli space exchange.

The geometry of these moduli spaces is highly constrained. They carry natural metric structures (Weil-Petersson and special Kähler metrics) and admit canonical coordinates related to period integrals and Yukawa couplings.