Kretschmann scalar


In the theory of Lorentzian manifolds, particularly in the context of applications to general relativity, the Kretschmann scalar is a quadratic scalar invariant. It was introduced by Erich Kretschmann.

Definition

The Kretschmann invariant is
where is the Riemann [curvature tensor] and is the Christoffel symbol. Because it is a sum of squares of tensor components, this is a quadratic invariant.
Einstein summation convention with raised and lowered indices is used above and throughout the article. An explicit summation expression is

Examples

For a Schwarzschild black hole of mass, the Kretschmann scalar is
where is the gravitational constant.
For a general FRW spacetime with metric
the Kretschmann scalar is

Relation to other invariants

Another possible invariant is
where is the Weyl tensor, the conformal curvature tensor which is also the completely traceless part of the Riemann tensor. In dimensions this is related to the Kretschmann invariant by
where is the Ricci curvature tensor and is the Ricci scalar curvature. The Ricci tensor vanishes in vacuum spacetimes, and hence there the Riemann tensor and the Weyl tensor coincide, as do their invariants.

Gauge theory invariants

The Kretschmann scalar and the Chern-Pontryagin scalar
where is the left dual of the Riemann tensor, are mathematically analogous to the familiar invariants of the electromagnetic field tensor
Generalising from the gauge theory of electromagnetism to general non-abelian gauge theory, the first of these invariants is
an expression proportional to the Yang–Mills Lagrangian. Here is the curvature of a covariant derivative, and is a trace form. The Kretschmann scalar arises from taking the connection to be on the frame bundle.