ScalingStacks

1 Background [029P]

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1 Background

We begin by reviewing some basic notions in Kahler geometry. The author’s view of this subject is coloured by an analogy with gauge theory so, while it is only indirectly relevant, we will begin with that.

1.1 Gauge theory and holomorphic bundles.

Here we consider a complex vector bundle EE over a complex manifold XX. We want to study the interaction between two structures

  • •

    A hermitian metric on EE;

  • •

    A holomorphic structure on EE, which can be defined by a ∂¯\overline{\partial}-operator

    ∂¯:Ω0​(E)→Ω0,1​(E).\overline{\partial}:\Omega^{0}(E)\rightarrow\Omega^{0,1}(E).

A basic fact is that given both of these structures there is a unique compatible unitary connection, in the sense that the ∂¯\overline{\partial}-operator is the (0,1)(0,1)-component of the covariant derivative. Now there are two ways of setting up the theory. In the first—the traditional point of view in complex geometry, as is [14] for example—we fix a holomorphic structure and consider the various Hermitian metrics. Then we have, for example, the formula

Fh=∂¯​(h−1​∂h)F_{h}=\overline{\partial}(h^{-1}\partial h) (1)

for the curvature tensor in a local holomorphic trivialisation, where the metric is defined by a matrix-valued function hh. In the second point of view—closer to what one does in general Yang-Mills theory—we fix the Hermitian metric and consider various ∂¯\overline{\partial}-operators. We can identify the set of these operators with the space 𝒜{\cal A} of unitary connections on EE. This point of view brings in two infinite dimensional groups. First, the group U⁡(E)U(E) of unitary automorphisms of EE and second the group G​L​(E)GL(E) of general linear automorphisms. Then G​L​(E)GL(E) acts on the space of ∂¯\overline{\partial}-operators by conjugation, and hence on the set 𝒜{\cal A} of connections. The ∂¯\overline{\partial}-operators which define equivalent holomorphic structures are exactly those which are in the same orbit of the G​L​(E)GL(E)-action.

The advantage of this second point of view comes when studying the “jumping” of holomorphic structures. This arises from the fact that the G​L​(E)GL(E) orbits are not usually closed in 𝒜{\cal A}. Fix a Kahler metric on the base space XX and use this to define the Yang-Mills functional: the L2L^{2} norm of the curvature. When one seeks Yang-Mills connections compatible with a given holomorphic structure ℰ{\cal E} one attempts to minimise this functional over a G​L​(E)GL(E) orbit in 𝒜{\cal A}. But it may happen that there is no minimum, in the simplest case because the infimum is achieved at a point in 𝒜{\cal A} in the closure but not in the orbit itself. Then one finds a Yang-Mills connection not on the original holomorphic bundle ℰ{\cal E}, but on another one ℰ′{\cal E}^{\prime}, such that there are arbitrarily small deformations of ℰ′{\cal E}^{\prime} which are isomorphic to ℰ{\cal E}. This lies at the root of the solution of the link between Yang-Mills theory and stability of holomorphic bundles expressed by the Kobayashi-Hitchin conjecture [3], [33], [7].

1.2 Symplectic and complex structures

Now we pass on to Kahler geometry. We study the interaction between two structures on an underlying manifold MM: a complex structure and a symplectic form. We require these to be algebraically compatible in the sense that the symplectic form is the imaginary part of a hermitian metric. As before there are two points of view we can take. In the first—the conventional point of view in complex differential geometry—we fix the complex structure and vary the Kahler form. If we choose a reference form ω0\omega_{0} and vary in the fixed cohomology class then (at least when MM is compact) any other form can be represented by a Kahler potential, in the shape

ωψ=ω0+i​∂∂¯​ψ.\omega_{\psi}=\omega_{0}+i\partial\overline{\partial}\psi.

For the alternative point of view we fix a symplectic form ω\omega and consider the space 𝒥{\cal J} of algebraically-compatible almost-complex structures on MM. Then the group SDiff{\rm SDiff} of symplectomorphisms of (M,ω)(M,\omega) acts on 𝒥{\cal J}, and this is the analogue of the unitary gauge group U⁡(E)U(E) in the previous case. We consider the subset 𝒥int{\cal J}_{{\rm int}} of integrable almost complex structures, which is preserved by SDiff{\rm SDiff}. This is partitioned into equivalence classes under the relation J1∼J2J_{1}\sim J_{2} if (M,J1),(M,J2)(M,J_{1}),(M,J_{2}) are isomorphic as complex manifolds. Although the group SDiff{\rm SDiff} does not have a true complexification one can argue that the equivalence classes in 𝒥int{\cal J}_{{\rm int}} are formally the orbits of such a (mythical) complexified group, in the sense that they behave that way at the level of tangent spaces and Lie algebras [8].

1.3 The equations

The focus of this article is on the existence question for four different kinds of special Kahler metrics, working within a fixed Kahler class on a compact manifold.

  1. 1.

    Extremal Kahler metrics The definition is due to Calabi [6]. They are critical points (and in fact local minima) of the Calabi functional

    ∫M|Riem⁡(ω)|2​d​μω,\int_{M}|{\rm Riem}(\omega)|^{2}d\mu_{\omega},

    where ω\omega varies over the Kahler metrics in a fixed Kahler class and Riem{\rm Riem} is the Riemann curvature tensor. The Euler-Lagrange equation is

    ∂¯​(grad​Sω)=0,\overline{\partial}({\rm grad}S_{\omega})=0,

    where grad{\rm grad} is the gradient operator defined by ω\omega and S⁡(ω)S(\omega) is the scalar curvature. In other words, the vector field grad​Sω{\rm grad}S_{\omega} should be a holomorphic vector field. On the face of it, this is a sixth order partial differential equation for the Kahler potential ψ\psi.

  2. 2.

    Constant scalar curvature Kahler metrics These are just those with SωS_{\omega} constant. Certainly they are extremal metrics (since the gradient vanishes), and if it happens that MM has no non-trivial holomorphic vector fields then an extremal metric must have constant scalar curvature.

  3. 3.

    Kahler-Einstein metrics By definition these are those where the Ricci tensor is a multiple λ​ω\lambda\omega. We will only consider the case when λ\lambda is positive (the zero and negative cases being completely understood through the results of Yau and Aubin). By rescaling there is no loss in supposing that λ=1\lambda=1. Solutions can only exist when MM is a “Fano” manifold and the class [ω][\omega] is −c1​(M)-c_{1}(M).

  4. 4.

    Kahler-Ricci solitons These again occur only in the Fano case. They are metrics for which

    Ric−ω=Lv​ω,{\rm Ric}-\omega=L_{v}\omega,

    where LvL_{v} is the Lie derivative along a holomorphic vector field vv.

Obviously a Kahler-Einstein metric has constant scalar curvature. There is no simple relation between the other two classes—extremal metrics and Kahler-Ricci solitons— but they can each be thought of as variants of the theory which take account of the possible holomorphic vector fields on the manifold. All this is elucidated by the theory of the Futaki invariant. We will not go in to this in detail here, since we will see later how the theory works in explicit examples. Suffice it to say that in either situation the relevant holomorphic vector field which can be determined a priori from standard topological data. More precisely, the vector field it determined once we fix a maximal compact connected subgroup of the group of holomorphic automorphisms. In either situation, an extremal metric or Kahler-Ricci soliton will necessarily be Einstein/constant scalar curvature if the Futaki invariant vanishes.

There is. of course, as yet no general existence theory for these structures but at the conjectural level one can see a detailed analogy with the Yang-Mills case. We do not want to go into this further here—partly because there is a comprehensive recent survey article [24]—but proceed with our study of special classes of manifolds.

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