In semi-Riemannian geometry, the Ricci decomposition is a way of breaking up the Riemann curvature tensor of a pseudo-Riemannian manifold into pieces with useful individual algebraic properties. This decomposition is of fundamental importance in Riemannian- and pseudo-Riemannian geometry.
The pieces appearing in the decomposition
The decomposition is
The three pieces are:
- the scalar part, the tensor
- the semi-traceless part, the tensor
- the fully traceless part, the Weyl tensor
Each piece possesses all the algebraic symmetries of the Riemann tensor itself, but has additional properties.
The scalar part
The semi-traceless part
is constructed algebraically using the metric tensor and the traceless part of the Ricci tensor
where is the metric tensor.
The Weyl tensor or conformal curvature tensor is completely traceless, in the sense that taking the trace, or contraction, over any pair of indices gives zero. Hermann Weyl showed that this tensor measures the deviation of a semi-Riemannian manifold from conformal flatness; if it vanishes, the manifold is (locally) conformally equivalent to a flat manifold.
No additional differentiation is needed anywhere in this construction.
In the case of a Lorentzian manifold, , the Einstein tensor has, by design, a trace which is just the negative of the Ricci scalar, and one may check that the traceless part of the Einstein tensor agrees with the traceless part of the Ricci tensor.
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 Template:Harv. 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:
and obeys the interchange symmetry
for all x,y,z,w ∈ V∗. As a result R is an element of the subspace S2Λ2V, 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
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
is given by
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
produces an algebraic curvature tensor.
If n > 4, then there is an orthogonal decomposition into (unique) irreducible subspaces
- RV = SV ⊕ EV ⊕ CV
- , where is the space of real scalars
- , where STemplate:SuV is the space of trace-free symmetric 2-forms
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,
is an orthogonal decomposition in the sense that
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 Template:Harv, 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
where 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
|CitationClass=book }} See section 2.6 for the decomposition. This book uses opposite signature but the same Landau-Lifshitz spacelike sign convention used in the Wikipedia.
|CitationClass=book }} See section 6.7 for a discussion of the decomposition (but note different sign conventions).
|CitationClass=book }} See section 3.2 for a discussion of the decomposition.
|CitationClass=citation }}. 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.