Locally, a Kähler metric is the complex Hessian of a real Kähler potential. Adding a holomorphic function and its complex conjugate to leaves the metric unchanged.
A Kähler-Einstein metric is a Kähler metric whose Ricci tensor satisfiesfor a real constant . Equivalently, its Ricci form satisfies , where is the Kähler form. It combines the compatibility of complex and Riemannian geometry with an Einstein curvature condition.
In holomorphic coordinates, take . The Ricci form is . A constant positive Hermitian matrix therefore gives : the flat metric on , and its quotient by a full lattice, are Ricci-flat examples. The Fubini-Study metric on Complex projective space gives a positive- example, with the numerical value depending on the metric normalization.
The equation is a nonlinear condition on a local Kähler potential, through the logarithmic determinant of its complex Hessian. This is why complex Monge-Ampère equations enter existence questions. Not every Kähler metric satisfies the Einstein condition.[ref]
Lectures on Kähler Geometry by Andrei Moroianu. Sections 11 and 13, Ricci form and Kähler-Einstein condition
A Hodge metric is a Kähler metric whose Kähler form represents an integral cohomology class in real de Rham cohomology. Equivalently, its periods over integral two-cycles are integers. Some conventions require the class of to be integral instead; this changes the normalization but not existence.
At any point of a Kähler manifold, a complex-linear coordinate change normalizes the Hermitian metric matrix. Closedness makes its holomorphic first derivatives symmetric in the two unbarred indices. A quadratic holomorphic coordinate change removes those derivatives, and Hermitian symmetry removes the antiholomorphic derivatives. Conversely, having this first-order normalization at every point makes the fundamental Hermitian form closed.
For a Kähler metric with complex structure , the associated real two-form is . It has type , is positive in the sense for , and is closed. Conversely a real closed positive form determines a Kähler metric. A local geometric Kähler potential writes it as .
On a nonempty compact Kähler manifold of complex dimension , the Kähler form is closed and . If for , then ; Stokes theorem contradicts the positive integral. Thus the de Rham cohomology is nonzero in every even degree through .
For a closed real form, the Poincaré lemma gives a real one-form with . Its part is -closed, so the Dolbeault-Poincaré lemma gives . Reality gives , hence . Positivity is a separate requirement for this form to define a metric.
A smooth real rotation-invariant potential is constant on every positive-radius circle, so its logarithmic-radius function is smooth on . Off the origin, . Since is smooth on the entire plane, this coefficient extends smoothly through the origin. A finite Taylor expansion, rather than a convergent series assumption, gives .
For a potential already smooth on all of , the associated form is a Kähler form exactly when the displayed two positivity conditions hold. The first gives a positive metric coefficient off the origin; the second is positivity of . The associated real metric is . Positivity away from the origin alone permits a degenerate metric at the origin.
A geometric Kähler potential is locally a real smooth function with for the Kähler form. Its complex Hessian must be positive definite to define a Kähler metric. Conventions sometimes absorb a factor of into . Potentials differing by the real part of a holomorphic function determine the same form. This topic concerns ordinary complex geometry; the existing undisambiguated Kähler potential entry concerns superfields.
For and , a geometric Kähler potential with derivative defines a Kähler metric on . Its tangential and radial eigenvalues are and . Their product is , giving the same Riemannian volume form as , although the metric is different. This construction makes preservation of volume compatible with anisotropic stretching.
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