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 Ernst Kretschmann.

Definition

The Kretschmann invariant is

$K=R_{abcd}\,R^{abcd}$

where $R_{abcd}$ 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

$C_{abcd}\,C^{abcd}$

where $C_{abcd}$ is the Weyl tensor, the conformal curvature tensor which is also the completely traceless part of the Riemann tensor. This is related to the Kretschmann invariant by

$R_{abcd}\,R^{abcd}=C_{abcd}\,C^{abcd}-2R_{ab}\,R^{ab}+{\frac {R^{2}}{3}}$

where $R^{ab}$ is the Ricci curvature tensor and $R$ is the Ricci scalar curvature (obtained by taking successive traces of the Riemann tensor).

The Kretschmann scalar and the Chern-Pontryagin scalar

$R_{abcd}\,{{}^{\star }\!R}^{abcd}$

where ${{}^{\star }R}^{abcd}$ 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

$F_{ab}\,F^{ab},\;\;F_{ab}\,{{}^{\star }\!F}^{ab}$

See also

• Curvature invariant (general relativity)
• Curvature invariant, for curvature invariants in Riemannian and pseudo-Riemannian geometry in general.
• Ricci decomposition, for more about the Riemann and Weyl tensor.
• Carminati-McLenaghan invariants, for a set of invariants.
• Classification of electromagnetic fields, for more about the invariants of the electromagnetic field tensor.