Ricci decomposition

Let (M,g) be a Riemannian or pseudo-Riemannian n-manifold. Consider its Riemann curvature, as a (0,4)-tensor field. This article will follow the sign convention

${\displaystyle R_{ijkl}=g_{lp}{\Big (}\partial _{i}\Gamma _{jk}^{p}-\partial _{j}\Gamma _{ik}^{p}+\Gamma _{iq}^{p}\Gamma _{jk}^{q}-\Gamma _{jq}^{p}\Gamma _{ik}^{q}{\Big )};}$

written multilinearly, this is the convention

${\displaystyle \operatorname {Rm} (W,X,Y,Z)=g{\Big (}\nabla _{W}\nabla _{X}Y-\nabla _{X}\nabla _{W}Y-\nabla _{[W,X]}Y,Z{\Big )}.}$

With this convention, the Ricci tensor is a (0,2)-tensor field defined by R_jk=g^ilR_ijkl and the scalar curvature is defined by R=g^jkR_jk. (Note that this is the less common sign convention for the Ricci tensor; it is more standard to define it by contracting either the first and third or the second and fourth indices, which yields a Ricci tensor with the opposite sign. Under that more common convention, the signs of the Ricci tensor and scalar must be changed in the equations below.) Define the traceless Ricci tensor

${\displaystyle Z_{jk}=R_{jk}-{\frac {1}{n}}Rg_{jk},}$

and then define three (0,4)-tensor fields S, E, and W by

${\displaystyle {\begin{aligned}S_{ijkl}&={\frac {R}{n(n-1)}}{\big (}g_{il}g_{jk}-g_{ik}g_{jl}{\big )}\\E_{ijkl}&={\frac {1}{n-2}}{\big (}Z_{il}g_{jk}-Z_{jl}g_{ik}-Z_{ik}g_{jl}+Z_{jk}g_{il}{\big )}\\W_{ijkl}&=R_{ijkl}-S_{ijkl}-E_{ijkl}.\end{aligned}}}$

The "Ricci decomposition" is the statement

${\displaystyle R_{ijkl}=S_{ijkl}+E_{ijkl}+W_{ijkl}.}$

As stated, this is vacuous since it is just a reorganization of the definition of W. The importance of the decomposition is in the properties of the three new tensors S, E, and W.

Terminological note. The tensor W is called the Weyl tensor. The notation W is standard in mathematics literature, while C is more common in physics literature. The notation R is standard in both, while there is no standardized notation for S, Z, and E.

One can compute the "norm formulas"

${\displaystyle {\begin{aligned}S_{ijkl}S^{ijkl}&={\frac {2R^{2}}{n(n-1)}}\\E_{ijkl}E^{ijkl}&={\frac {4R_{ij}R^{ij}}{n-2}}-{\frac {4R^{2}}{n(n-2)}}\\W_{ijkl}W^{ijkl}&=R_{ijkl}R^{ijkl}-{\frac {4R_{ij}R^{ij}}{n-2}}+{\frac {2R^{2}}{(n-1)(n-2)}}\end{aligned}}}$

and the "trace formulas"

${\displaystyle {\begin{aligned}g^{il}S_{ijkl}&={\frac {1}{n}}Rg_{jk}\\g^{il}E_{ijkl}&=R_{jk}-{\frac {1}{n}}Rg_{jk}\\g^{il}W_{ijkl}&=0.\end{aligned}}}$

Mathematically, the Ricci decomposition is the decomposition of the space of all tensors having the symmetries of the Riemann tensor into its irreducible representations for the action of the orthogonal group (Besse 1987, Chapter 1, §G). Let V be an n-dimensional vector space, equipped with a metric tensor (of possibly mixed signature). Here V is modeled on the cotangent space at a point, so that a curvature tensor R (with all indices lowered) is an element of the tensor product V⊗V⊗V⊗V. The curvature tensor is skew symmetric in its first and last two entries:

${\displaystyle R(x,y,z,w)=-R(y,x,z,w)=-R(x,y,w,z)\,}$

and obeys the interchange symmetry

${\displaystyle R(x,y,z,w)=R(z,w,x,y),\,}$

for all x,y,z,w ∈ V^∗. As a result, R is an element of the subspace ${\displaystyle S^{2}\Lambda ^{2}V}$, the second symmetric power of the second exterior power of V. A curvature tensor must also satisfy the Bianchi identity, meaning that it is in the kernel of the linear map ${\displaystyle b:S^{2}\Lambda ^{2}V\to \Lambda ^{4}V}$ given by

${\displaystyle b(R)(x,y,z,w)=R(x,y,z,w)+R(y,z,x,w)+R(z,x,y,w).\,}$

The space RV = ker b in S²Λ²V is the space of algebraic curvature tensors. The Ricci decomposition is the decomposition of this space into irreducible factors. The Ricci contraction mapping

${\displaystyle c:S^{2}\Lambda ^{2}V\to S^{2}V}$

is given by

${\displaystyle c(R)(x,y)=\operatorname {tr} R(x,\cdot ,y,\cdot ).}$

This associates a symmetric 2-form to an algebraic curvature tensor. Conversely, given a pair of symmetric 2-forms h and k, the Kulkarni–Nomizu product of h and k

${\displaystyle (h{~\wedge \!\!\!\!\!\!\!\!\;\bigcirc ~}k)(x,y,z,w)=h(x,z)k(y,w)+h(y,w)k(x,z)-h(x,w)k(y,z)-h(y,z)k(x,w)}$

produces an algebraic curvature tensor.

If n ≥ 4, then there is an orthogonal decomposition into (unique) irreducible subspaces

RV = SV ⊕ EV ⊕ CV

where

${\displaystyle \mathbf {S} V=\mathbb {R} g{~\wedge \!\!\!\!\!\!\!\!\;\bigcirc ~}g}$, where ${\displaystyle \mathbb {R} }$ is the space of real scalars

${\displaystyle \mathbf {E} V=g{~\wedge \!\!\!\!\!\!\!\!\;\bigcirc ~}S_{0}^{2}V}$, where S²
₀V is the space of trace-free symmetric 2-forms

${\displaystyle \mathbf {C} V=\ker c\cap \ker b.}$

The parts S, E, and C of the Ricci decomposition of a given Riemann tensor R are the orthogonal projections of R onto these invariant factors. In particular,

${\displaystyle R=S+E+C}$

is an orthogonal decomposition in the sense that

${\displaystyle |R|^{2}=|S|^{2}+|E|^{2}+|C|^{2}.}$

This decomposition expresses the space of tensors with Riemann symmetries as a direct sum of the scalar submodule, the Ricci submodule, and Weyl submodule, respectively. Each of these modules is an irreducible representation for the orthogonal group (Singer & Thorpe 1969), and thus the Ricci decomposition is a special case of the splitting of a module for a semisimple Lie group into its irreducible factors. In dimension 4, the Weyl module decomposes further into a pair of irreducible factors for the special orthogonal group: the self-dual and antiself-dual parts W⁺ and W⁻.

The Ricci decomposition can be interpreted physically in Einstein's theory of general relativity, where it is sometimes called the Géhéniau-Debever decomposition. In this theory, the Einstein field equation

${\displaystyle G_{ab}=8\pi \,T_{ab}}$

where ${\displaystyle T_{ab}}$ is the stress–energy tensor describing the amount and motion of all matter and all nongravitational field energy and momentum, states that the Ricci tensor—or equivalently, the Einstein tensor—represents that part of the gravitational field which is due to the immediate presence of nongravitational energy and momentum. The Weyl tensor represents the part of the gravitational field which can propagate as a gravitational wave through a region containing no matter or nongravitational fields. Regions of spacetime in which the Weyl tensor vanishes contain no gravitational radiation and are also conformally flat.

• Bel decomposition of the Riemann tensor
• Conformal geometry
• Petrov classification
• Plebanski tensor
• Ricci calculus
• Schouten tensor
• Trace-free Ricci tensor

• Besse, Arthur L. (1987), Einstein manifolds, Ergebnisse der Mathematik und ihrer Grenzgebiete (3) [Results in Mathematics and Related Areas (3)], vol. 10, Berlin, New York: Springer-Verlag, pp. xii+510, ISBN 978-3-540-15279-8.
• Sharpe, R.W. (1997), Differential Geometry: Cartan's Generalization of Klein's Erlangen Program, Springer-Verlag, New York, ISBN 0-387-94732-9. Section 6.1 discusses the decomposition. Versions of the decomposition also enter into the discussion of conformal and projective geometries, in chapters 7 and 8.
• Singer, I.M.; Thorpe, J.A. (1969), "The curvature of 4-dimensional Einstein spaces", Global Analysis (Papers in Honor of K. Kodaira), Univ. Tokyo Press, pp. 355–365.