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Calabi-Yau Space


A Calabi-Yau space, in its metric formulation, is a Kähler manifold whose Riemannian metric has holonomy group contained in SU(n), where n is its complex dimension. Calabi-Yau spaces are important in string theory, where one model posits the geometry of the universe to consist of a ten-dimensional space of the form M×V, where M is a four dimensional manifold (space-time) and V is a six dimensional compact Calabi-Yau space. They are related to Kummer surfaces. Although the main application of Calabi-Yau spaces is in theoretical physics, they are also interesting from a purely mathematical standpoint. Consequently, they go by slightly different names, depending mostly on context, such as Calabi-Yau manifolds or Calabi-Yau varieties.

Although the definition can be generalized to any dimension, they are usually considered to have three complex dimensions. Since their complex structure may vary, it is convenient to think of them as having six real dimensions and a fixed smooth structure.

A Calabi-Yau metric has a nonvanishing spinor whose covariant derivative vanishes. The existence of a nonvanishing Dirac-harmonic spinor alone does not imply Calabi-Yau holonomy. In the complex-geometric description, the canonical bundle is trivial.

Consider the local situation using coordinates. In R^6, pick coordinates x_1,x_2,x_3 and y_1,y_2,y_3 so that

 z_j=x_j+iy_j
(1)

gives it the structure of C^3. Then

 phi_z=dz_1 ^ dz_2 ^ dz_3
(2)

is a local bundle section of the canonical bundle. A unitary change of coordinates w=Az, where A is a unitary matrix, transforms phi by detA, i.e.,

 phi_w=detAphi_z.
(3)

If the linear transformation A has determinant 1, that is, it is a special unitary transformation, then phi is consistently defined as phi_z or as phi_w.

On a Calabi-Yau manifold V, such a phi can be defined globally, and the Lie group SU(3) is very important in the theory. In fact, one of the many equivalent definitions, coming from Riemannian geometry, says that a Calabi-Yau manifold is a 2n-dimensional manifold whose holonomy group reduces to SU(n). Such a manifold has a calibration form given locally by the real part of its parallel complex volume form, whose algebraic form is

 dz_1 ^ ... ^ dz_n.
(4)

A closed calibration form of this algebraic type alone does not imply Calabi-Yau holonomy. Often, the extra assumptions that V is simply connected and/or compact are made.

Calabi-Yau manifolds and their moduli spaces have interesting geometric properties. Compact Calabi-Yau manifolds have Hodge diamonds with intrinsic symmetries. Mirror symmetry instead relates the Hodge numbers of different Calabi-Yau manifolds. For a mirror pair X,Y of complex dimension n, it predicts the relation

 h^(p,q)(X)=h^(n-p,q)(Y).
(5)

This exchange is distinct from the intrinsic symmetries of either Hodge diamond.


See also

Algebraic Variety, Calabi-Yau Variety, Canonical Bundle, Complex Manifold, Harmonic, K3 Surface, Kähler Form, Lie Group, Mirror Pair, Moduli Space, Spinor

Portions of this entry contributed by Todd Rowland

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Cite this as:

Weisstein, Eric W., with contributions by Todd Rowland. "Calabi-Yau Space." From MathWorld--A Wolfram Resource. https://mathworld.wolfram.com/Calabi-YauSpace.html

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