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. Because it is a sum of squares of tensor components, this is a quadratic invariant.
Relation to other invariants
Another possible invariant (which has been employed for example in writing the gravitational term of the Lagrangian for some higher-order gravity theories of gravitation) 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 (obtained by taking successive traces of the Riemann tensor).
The Kretschmann scalar and the Chern-Pontryagin scalar
where is the left dual of the Riemann tensor, are mathematically analogous (to some extent, physically analogous) to the familiar invariants of the electromagnetic field tensor
See also
- Carminati-McLenaghan invariants, for a set of invariants.
- Classification of electromagnetic fields, for more about the invariants of the electromagnetic field tensor.
- Curvature invariant, for curvature invariants in Riemannian and pseudo-Riemannian geometry in general.
- Curvature invariant (general relativity).
- Ricci decomposition, for more about the Riemann and Weyl tensor.