Ricci Decomposition
   HOME

TheInfoList



OR:

In the mathematical fields of Riemannian and pseudo-Riemannian geometry, the Ricci decomposition is a way of breaking up the Riemann curvature tensor of a Riemannian or pseudo-Riemannian manifold into pieces with special algebraic properties. This decomposition is of fundamental importance in Riemannian and pseudo-Riemannian geometry.


Definition of the 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 :R_=g_\Big(\partial_i\Gamma_^p-\partial_j\Gamma_^p+\Gamma_^p\Gamma_^q-\Gamma_^p\Gamma_^q\Big); written multilinearly, this is the convention :\operatorname(W,X,Y,Z)=g\Big(\nabla_W\nabla_XY-\nabla_X\nabla_WY-\nabla_Y,Z\Big). With this convention, the Ricci tensor is a (0,2)-tensor field defined by ''Rjk''=''gilRijkl'' and the scalar curvature is defined by ''R''=''gjkRjk.'' Define the traceless Ricci tensor :Z_=R_-\fracRg_, and then define three (0,4)-tensor fields ''S'', ''E'', and ''W'' by :\begin S_&=\frac\big(g_g_-g_g_\big)\\ E_&=\frac\big(Z_g_-Z_g_-Z_g_+Z_g_\big)\\ W_&=R_-S_-E_. \end The "Ricci decomposition" is the statement :R_=S_+E_+W_. 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 In differential geometry, the Weyl curvature tensor, named after Hermann Weyl, is a measure of the curvature of spacetime or, more generally, a pseudo-Riemannian manifold. Like the Riemann curvature tensor, the Weyl tensor expresses the tidal forc ...
. 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''.


Basic properties


Properties of the pieces

Each of the tensors ''S'', ''E'', and ''W'' has the same algebraic symmetries as the Riemann tensor. That is: :\begin S_&=-S_=-S_=S_\\ E_&=-E_=-E_=E_\\ W_&=-W_=-W_=W_ \end together with :\begin S_+S_+S_&=0\\ E_+E_+E_&=0\\ W_+W_+W_&=0. \end The Weyl tensor has the additional symmetry that it is completely traceless: :g^W_=0.
Hermann Weyl Hermann Klaus Hugo Weyl, (; 9 November 1885 – 8 December 1955) was a German mathematician, theoretical physicist and philosopher. Although much of his working life was spent in Zürich, Switzerland, and then Princeton, New Jersey, he is assoc ...
showed that ''W'' has the remarkable property of measuring the deviation of a Riemannian or pseudo-Riemannian manifold from local conformal flatness; if it is zero, then ''M'' can be covered by charts relative to which ''g'' has the form ''gij=ef''δ''ij'' for some function ''f'' defined chart by chart.


Properties of the decomposition

One may check that the Ricci decomposition is orthogonal in the sense that :S_E^=S_W^=E_W^=0, recalling the general definition T^=g^g^g^g^T_. This has the consequence, which could be proved directly, that :R_R^=S_S^+E_E^+W_W^. Terminological note. It would be symbolically clean to present this orthogonality as saying :\langle S,E\rangle_g=\langle S,W\rangle_g=\langle E,W\rangle_g=0, together with :, \operatorname, _g^2=, S, _g^2+, E, _g^2+, W, _g^2. However, there is an unavoidable ambiguity with such notation depending on whether one views \operatorname,S,E,W as multilinear maps T_pM\times T_pM\times T_pM\times T_pM\to\mathbb or as linear maps \wedge^2T_pM\to\wedge^2T_pM, in which case the corresponding norms and inner products would differ by a constant factor. Although this would not lead to any inconsistencies in the above equations, since all terms would be changed by the same factor, it can lead to confusion in more involved contexts. For this reason, the index notation can often be easier to understand.


Related formulas

One can compute the "norm formulas" :\begin S_S^&=\frac\\ E_E^&=\frac-\frac\\ W_W^&=R_R^-\frac+\frac \end and the "trace formulas" :\begin g^S_&=\fracRg_\\ g^E_&=R_-\fracRg_\\ g^W_&=0. \end


Mathematical explanation of the decomposition

Mathematically, the Ricci decomposition is the decomposition of the space of all tensors having the symmetries of the Riemann tensor into its
irreducible representation In mathematics, specifically in the representation theory of groups and algebras, an irreducible representation (\rho, V) or irrep of an algebraic structure A is a nonzero representation that has no proper nontrivial subrepresentation (\rho, _W,W ...
s for the action of the
orthogonal group In mathematics, the orthogonal group in dimension , denoted , is the Group (mathematics), group of isometry, distance-preserving transformations of a Euclidean space of dimension that preserve a fixed point, where the group operation is given by ...
. Let ''V'' be an ''n''-dimensional vector space, equipped with a
metric tensor In the mathematical field of differential geometry, a metric tensor (or simply metric) is an additional structure on a manifold (such as a surface) that allows defining distances and angles, just as the inner product on a Euclidean space allows ...
(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: :R(x,y,z,w)=-R(y,x,z,w)=-R(x,y,w,z)\, and obeys the interchange symmetry :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 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 b: S^2\Lambda^2 V \to \Lambda^4 V given by :b(R)(x,y,z,w) = R(x,y,z,w) + R(y,z,x,w) + R(z,x,y,w).\, The space in ''S''2Λ2''V'' is the space of algebraic curvature tensors. The Ricci decomposition is the decomposition of this space into irreducible factors. The Ricci contraction mapping :c : S^2\Lambda^2 V \to S^2V is given by :c(R)(x,y) = \operatornameR(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'' :(h 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 : where :\mathbfV = \mathbb g g, where \mathbb is the space of real scalars :\mathbfV = g S^2_0V, where ''S'V'' is the space of trace-free symmetric 2-forms :\mathbfV = \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, :R = S + E + C is an orthogonal decomposition in the sense that :, 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 In mathematics, specifically in the representation theory of groups and algebras, an irreducible representation (\rho, V) or irrep of an algebraic structure A is a nonzero representation that has no proper nontrivial subrepresentation (\rho, _W,W ...
for the
orthogonal group In mathematics, the orthogonal group in dimension , denoted , is the Group (mathematics), group of isometry, distance-preserving transformations of a Euclidean space of dimension that preserve a fixed point, where the group operation is given by ...
, 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 In mathematics, the orthogonal group in dimension , denoted , is the group of distance-preserving transformations of a Euclidean space of dimension that preserve a fixed point, where the group operation is given by composing transformations. T ...
: the
self-dual In mathematics, a duality translates concepts, theorems or mathematical structures into other concepts, theorems or structures, in a Injective function, one-to-one fashion, often (but not always) by means of an Involution (mathematics), involutio ...
and antiself-dual parts ''W''+ and ''W''.


Physical interpretation

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 : G_ = 8 \pi \, T_ where T_ is the
stress–energy tensor The stress–energy tensor, sometimes called the stress–energy–momentum tensor or the energy–momentum tensor, is a tensor physical quantity that describes the density and flux of energy and momentum in spacetime, generalizing the stress ...
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 Gravitational waves are waves of the intensity of gravity generated by the accelerated masses of an orbital binary system that propagate as waves outward from their source at the speed of light. They were first proposed by Oliver Heaviside in 1 ...
through a region containing no matter or nongravitational fields. Regions of spacetime in which the Weyl tensor vanishes contain no
gravitational radiation Gravitational waves are waves of the intensity of gravity generated by the accelerated masses of an orbital binary system that propagate as waves outward from their source at the speed of light. They were first proposed by Oliver Heaviside in 1 ...
and are also conformally flat.


See also

*
Bel decomposition In semi-Riemannian geometry, the Bel decomposition, taken with respect to a specific timelike congruence, is a way of breaking up the Riemann tensor of a pseudo-Riemannian manifold into lower order tensors with properties similar to the electric ...
of the Riemann tensor * Conformal geometry *
Petrov classification In differential geometry and theoretical physics, the Petrov classification (also known as Petrov–Pirani–Penrose classification) describes the possible algebraic symmetries of the Weyl tensor at each event in a Lorentzian manifold. It is mos ...
*
Plebanski tensor The Plebanski tensor is an order 4 tensor in general relativity constructed from the trace-free Ricci tensor. It was first defined by Jerzy Plebański in 1964. Let S_ be the trace-free Ricci tensor: :S_=R_-\fracRg_. Then the Plebanski tensor ...
*
Ricci calculus In mathematics, Ricci calculus constitutes the rules of index notation and manipulation for tensors and tensor fields on a differentiable manifold, with or without a metric tensor or connection. It is also the modern name for what used to be cal ...
*
Schouten tensor In Riemannian geometry the Schouten tensor is a second-order tensor introduced by Jan Arnoldus Schouten defined for by: :P=\frac \left(\mathrm -\frac g\right)\, \Leftrightarrow \mathrm=(n-2) P + J g \, , where Ric is the Ricci tensor (defined by ...
*
Trace-free Ricci tensor In differential geometry, the Ricci curvature tensor, named after Gregorio Ricci-Curbastro, is a geometric object which is determined by a choice of Riemannian or pseudo-Riemannian metric on a manifold. It can be considered, broadly, as a measur ...


References

*. * . 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. * . {{DEFAULTSORT:Ricci Decomposition Differential geometry Riemannian geometry Tensors in general relativity