Ricci tensor


Definition.

The Ricci curvature tensor is a rank 2, symmetric tensorMathworldPlanetmath that arises naturally in pseudo-Riemannian geometry. Let (M,gi⁢j) be a smooth, n-dimensional pseudo-Riemannian manifold, and let Rij⁢k⁢l denote the corresponding Riemann curvature tensorMathworldPlanetmath. The Ricci tensor Ri⁢j is commonly defined as the following contractionPlanetmathPlanetmath of the full curvature tensor:

Ri⁢j=Rk.i⁢k⁢j

The index symmetryPlanetmathPlanetmath of Ri⁢j, so defined, follows from the symmetry properties of the Riemann curvature. To wit,

Ri⁢j=Rk=i⁢k⁢jRk⁢i=kjRk=j⁢k⁢iRj⁢i.

It is also convenient to regard the Ricci tensor as a symmetric bilinear formMathworldPlanetmath. To that end for vector-fields X,Y we will write

Ric⁡(X,Y)=Xi⁢Yj⁢Ri⁢j.

Related objects.

Contracting the Ricci tensor, we obtain an important scalar invariantMathworldPlanetmath

R=Ri,i

called the scalar curvature, and sometimes also called the Ricci scalar. Closely related to the Ricci tensor is the tensor

Gi⁢j=Ri⁢j-12⁢R⁢gi⁢j,

called the Einstein tensor. The Einstein tensor is also known as the trace-reversed Ricci tensor owing to the fact that

Gi=i-R.

Another related tensor is

Si⁢j=Ri⁢j-1n⁢R⁢gi⁢j.

This is called the trace-free Ricci tensor, owing to the fact that the above definition implies that

Si=i0.

Geometric interpretation.

In Riemannian geometry, the Ricci tensor represents the average value of the sectional curvatureMathworldPlanetmath along a particular direction. Let

Kx⁢(u,v)=Rx⁢(u,v,v,u)gx⁢(u,u)⁢gx⁢(v,v)-gx⁢(u,v)2

denote the sectional curvature of M along the plane spanned by vectors u,v∈Tx⁢M. Fix a point x∈M and a tangent vectorMathworldPlanetmath v∈Tx⁢M, and let

Sx⁢(v)={u∈Tx⁢M:gx⁢(u,u)=1,gx⁢(u,v)=0}

denote the n-2 dimensional sphere of those unit vectorsMathworldPlanetmath at x that are perpendicularMathworldPlanetmathPlanetmath to v. Let μx denote the natural (n-2)-dimensional volume measure on Tx⁢M, normalized so that

∫Sx⁢(v)μx=1.

In this way, the quantity

∫Sx⁢(v)Kx⁢(⋅,v)⁢μx,

describes the average value of the sectional curvature for all planes in Tx⁢M that contain v. It is possible to show that

Ricx⁡(v,v)=(1-n)⁢∫Sx⁢(v)Kx⁢(⋅,v)⁢μx,

thereby giving us the desired geometric interpretationMathworldPlanetmathPlanetmath.

Decomposition of the curvature tensor.

For n≥3, the Ricci tensor can be characterized in terms of the decomposition of the full curvature tensor into three covariantly defined summands, namely

Fi⁢j⁢k⁢l =1n-2⁢(Sj⁢l⁢gi⁢k+Si⁢k⁢gj⁢l-Si⁢l⁢gj⁢k-Sj⁢k⁢gi⁢l),
Ei⁢j⁢k⁢l =1n⁢(n-1)⁢R⁢(gj⁢l⁢gi⁢k-gi⁢l⁢gj⁢k),
Wi⁢j⁢k⁢l =Ri⁢j⁢k⁢l-Fi⁢j⁢k⁢l-Ei⁢j⁢k⁢l.

The Wi⁢j⁢k⁢l is called the Weyl curvature tensor. It is the conformally invariant, trace-free part of the curvature tensor. Indeed, with the above definitions, we have

Wk=i⁢k⁢j0.

The Ei⁢j⁢k⁢l and Fi⁢j⁢k⁢l correspond to the trace-free part of the Ricci curvature tensor, and to the Ricci scalar. Indeed, we can recover Si⁢j and R from Ei⁢j⁢k⁢l and Fi⁢j⁢k⁢l as follows:

Si⁢j =Fk,i⁢k⁢j
Ei⁢ji⁢j =R.

Relativity.

The Ricci tensor also plays an important role in the theory of general relativity. In this keystone application, M is a 4-dimensional pseudo-Riemannian manifold with signaturePlanetmathPlanetmathPlanetmathPlanetmath (3,1). The Einstein field equations assert that the energy-momentum tensor is proportional to the Einstein tensor. In particular, the equation

Ri⁢j=0

is the field equation for a vacuum space-time. In geometry, a pseudo-Riemannian manifold that satisfies this equation is called Ricci-flat. It is possible to prove that a manifoldMathworldPlanetmath is Ricci flat if and only if locally, the manifold, is conformally equivalent to flat space.

Title Ricci tensor
Canonical name RicciTensor
Date of creation 2013-03-22 15:02:38
Last modified on 2013-03-22 15:02:38
Owner rmilson (146)
Last modified by rmilson (146)
Numerical id 9
Author rmilson (146)
Entry type Definition
Classification msc 83C05
Defines scalar curvature
Defines Einstein tensor
Defines ricci scalar
Defines Weyl tensor
Defines Weyl curvature tensor