# Kähler manifold

In mathematics and especially differential geometry, a **Kähler manifold** is a manifold with three mutually compatible structures: a complex structure, a Riemannian structure, and a symplectic structure. The concept was first studied by Jan Arnoldus Schouten and David van Dantzig in 1930, and then introduced by Erich Kähler in 1933. The terminology has been fixed by André Weil. **Kähler geometry** refers to the study of Kähler manifolds, their geometry and topology, as well as the study of structures and constructions that can be performed on Kähler manifolds, such as the existence of special connections like Hermitian Yang–Mills connections, or special metrics such as Kähler–Einstein metrics.

Every smooth complex projective variety is a Kähler manifold. Hodge theory is a central part of algebraic geometry, proved using Kähler metrics.

Since Kähler manifolds are equipped with several compatible structures, they can be described from different points of view:

A Kähler manifold is a symplectic manifold (*X*, *ω*) equipped with an integrable almost-complex structure *J* which is compatible with the symplectic form ω, meaning that the bilinear form

on the tangent space of *X* at each point is symmetric and positive definite (and hence a Riemannian metric on *X*).^{[1]}

A Kähler manifold is a complex manifold *X* with a Hermitian metric *h* whose associated 2-form *ω* is closed. In more detail, *h* gives a positive definite Hermitian form on the tangent space *TX* at each point of *X*, and the 2-form *ω* is defined by

Equivalently, a Kähler manifold *X* is a Hermitian manifold of complex dimension *n* such that for every point *p* of *X*, there is a holomorphic coordinate chart around *p* in which the metric agrees with the standard metric on **C**^{n} to order 2 near *p*.^{[2]} That is, if the chart takes *p* to 0 in **C**^{n}, and the metric is written in these coordinates as *h*_{ab} = (∂/∂*z*_{a},
∂/∂*z*_{b}), then

Since the 2-form *ω* is closed, it determines an element in de Rham cohomology *H*^{2}(*X*, **R**), known as the **Kähler class**.

A Kähler manifold is a Riemannian manifold *X* of even dimension 2*n* whose holonomy group is contained in the unitary group U(*n*).^{[3]} Equivalently, there is a complex structure *J* on the tangent space of *X* at each point (that is, a real linear map from *TX* to itself with *J*^{2} = −1) such that *J* preserves the metric *g* (meaning that *g*(*Ju*, *Jv*) = *g*(*u*, *v*)) and *J* is preserved by parallel transport.

A smooth real-valued function ρ on a complex manifold is called strictly plurisubharmonic if the real closed (1,1)-form

For a compact Kähler manifold *X*, the volume of a closed complex subspace of *X* is determined by its homology class. In a sense, this means that the geometry of a complex subspace is bounded in terms of its topology. (This fails completely for real submanifolds.) Explicitly, **Wirtinger's formula** says that

where *Y* is an *r*-dimensional closed complex subspace and *ω* is the Kähler form.^{[5]} Since *ω* is closed, this integral depends only on the class of *Y* in *H*_{2r}(*X*, **R**). These volumes are always positive, which expresses a strong positivity of the Kähler class *ω* in *H*^{2}(*X*, **R**) with respect to complex subspaces. In particular, *ω*^{n} is not zero in *H*^{2n}(*X*, **R**), for a compact Kähler manifold *X* of complex dimension *n*.

A related fact is that every closed complex subspace *Y* of a compact Kähler manifold *X* is a minimal submanifold (outside its singular set). Even more: by the theory of calibrated geometry, *Y* minimizes volume among all (real) cycles in the same homology class.

If *X* is Kähler, then these Laplacians are all the same up to a constant:^{[6]}

Further, for a compact Kähler manifold *X*, Hodge theory gives an interpretation of the splitting above which does not depend on the choice of Kähler metric. Namely, the cohomology *H*^{r}(*X*, **C**) of *X* with complex coefficients splits as a direct sum of certain coherent sheaf cohomology groups:^{[7]}

The group on the left depends only on *X* as a topological space, while the groups on the right depend on *X* as a complex manifold. So this **Hodge decomposition theorem** connects topology and complex geometry for compact Kähler manifolds.

A simple consequence of Hodge theory is that every odd Betti number *b*_{2a+1} of a compact Kähler manifold is even, by Hodge symmetry. This is not true for compact complex manifolds in general, as shown by the example of the Hopf surface, which is diffeomorphic to *S*^{1} × *S*^{3} and hence has *b*_{1} = 1.

The "Kähler package" is a collection of further restrictions on the cohomology of compact Kähler manifolds, building on Hodge theory. The results include the Lefschetz hyperplane theorem, the hard Lefschetz theorem, and the Hodge-Riemann bilinear relations.^{[8]} A related result is that every compact Kähler manifold is formal in the sense of rational homotopy theory.^{[9]}

The question of which groups can be fundamental groups of compact Kähler manifolds, called **Kähler groups**, is wide open. Hodge theory gives many restrictions on the possible Kähler groups.^{[10]} The simplest restriction is that the abelianization of a Kähler group must have even rank, since the Betti number *b*_{1} of a compact Kähler manifold is even. (For example, the integers **Z** cannot be the fundamental group of a compact Kähler manifold.) Extensions of the theory such as non-abelian Hodge theory give further restrictions on which groups can be Kähler groups.

Without the Kähler condition, the situation is simple: Clifford Taubes showed that every finitely presented group arises as the fundamental group of some compact complex manifold of dimension 3.^{[11]} (Conversely, the fundamental group of any closed manifold is finitely presented.)

The Kodaira embedding theorem characterizes smooth complex projective varieties among all compact Kähler manifolds. Namely, a compact complex manifold *X* is projective if and only if there is a Kähler form *ω* on *X* whose class in *H*^{2}(*X*, **R**) is in the image of the integral cohomology group *H*^{2}(*X*, **Z**). (Because a positive multiple of a Kähler form is a Kähler form, it is equivalent to say that *X* has a Kähler form whose class in *H*^{2}(*X*, **R**) is in *H*^{2}(*X*, **Q**).) Equivalently, *X* is projective if and only if there is a holomorphic line bundle *L* on *X* with a hermitian metric whose curvature form ω is positive (since ω is then a Kähler form that represents the first Chern class of *L* in *H*^{2}(*X*, **Z**)).

Every compact complex curve is projective, but in complex dimension at least 2, there are many compact Kähler manifolds that are not projective; for example, most compact complex tori are not projective. One may ask whether every compact Kähler manifold can at least be deformed (by continuously varying the complex structure) to a smooth projective variety. Kunihiko Kodaira's work on the classification of surfaces implies that every compact Kähler manifold of complex dimension 2 can indeed be deformed to a smooth projective variety. Claire Voisin found, however, that this fails in dimensions at least 4. She constructed a compact Kähler manifold of complex dimension 4 that is not even homotopy equivalent to any smooth complex projective variety.^{[12]}

One can also ask for a characterization of compact Kähler manifolds among all compact complex manifolds. In complex dimension 2, Kodaira and Yum-Tong Siu showed that a compact complex surface has a Kähler metric if and only if its first Betti number is even.^{[13]} Thus "Kähler" is a purely topological property for compact complex surfaces. Hironaka's example shows, however, that this fails in dimensions at least 3. In more detail, the example is a 1-parameter family of smooth compact complex 3-folds such that most fibers are Kähler (and even projective), but one fiber is not Kähler. Thus a compact Kähler manifold can be diffeomorphic to a non-Kähler complex manifold.

A Kähler manifold is called **Kähler–Einstein** if it has constant Ricci curvature. Equivalently, the Ricci curvature tensor is equal to a constant λ times the metric tensor, Ric = *λg*. The reference to Einstein comes from general relativity, which asserts in the absence of mass that spacetime is a 4-dimensional Lorentzian manifold with zero Ricci curvature. See the article on Einstein manifolds for more details.

Although Ricci curvature is defined for any Riemannian manifold, it plays a special role in Kähler geometry: the Ricci curvature of a Kähler manifold *X* can be viewed as a real closed (1,1)-form that represents *c*_{1}(*X*) (the first Chern class of the tangent bundle) in *H*^{2}(*X*, **R**). It follows that a compact Kähler–Einstein manifold *X* must have canonical bundle *K*_{X} either anti-ample, homologically trivial, or ample, depending on whether the Einstein constant λ is positive, zero, or negative. Kähler manifolds of those three types are called Fano, Calabi–Yau, or with ample canonical bundle (which implies general type), respectively. By the Kodaira embedding theorem, Fano manifolds and manifolds with ample canonical bundle are automatically projective varieties.

Shing-Tung Yau proved the Calabi conjecture: every smooth projective variety with ample canonical bundle has a Kähler–Einstein metric (with constant negative Ricci curvature), and every Calabi–Yau manifold has a Kähler–Einstein metric (with zero Ricci curvature). These results are important for the classification of algebraic varieties, with applications such as the Miyaoka–Yau inequality for varieties with ample canonical bundle and the Beauville–Bogomolov decomposition for Calabi–Yau manifolds.^{[14]}

By contrast, not every smooth Fano variety has a Kähler–Einstein metric (which would have constant positive Ricci curvature). However, Xiuxiong Chen, Simon Donaldson, and Song Sun proved the Yau–Tian–Donaldson conjecture: a smooth Fano variety has a Kähler–Einstein metric if and only if it is K-stable, a purely algebro-geometric condition.

In situations where there cannot exist a Kähler–Einstein metric, it is possible to study mild generalizations including constant scalar curvature Kähler metrics and extremal Kähler metrics. When a Kähler–Einstein metric can exist, these broader generalizations are automatically Kähler–Einstein.

The deviation of a Riemannian manifold *X* from the standard metric on Euclidean space is measured by sectional curvature, which is a real number associated to any real 2-plane in the tangent space of *X* at a point. For example, the sectional curvature of the standard metric on **CP**^{n} (for *n* ≥ 2) varies between 1/4 and 1. For a Hermitian manifold (for example, a Kähler manifold), the **holomorphic sectional curvature** means the sectional curvature restricted to complex lines in the tangent space. This behaves more simply, in that **CP**^{n} has holomorphic sectional curvature equal to 1. At the other extreme, the open unit ball in **C**^{n} has a complete Kähler metric with holomorphic sectional curvature equal to −1. (With this metric, the ball is also called **complex hyperbolic space**.)

The holomorphic sectional curvature is closely tied to the properties of *X* as a complex manifold. For example, every Hermitian manifold *X* with holomorphic sectional curvature bounded above by a negative constant is Kobayashi hyperbolic.^{[15]} It follows that every holomorphic map **C** → *X* is constant.

A remarkable feature of complex geometry is that holomorphic sectional curvature decreases on complex submanifolds.^{[16]} (The same goes for a more general concept, holomorphic bisectional curvature.) For example, every complex submanifold of **C**^{n} (with the induced metric from **C**^{n}) has holomorphic sectional curvature ≤ 0.