Ricci tensor
Definition.
The Ricci curvature tensor is a rank 2, symmetric tensor that
arises naturally in pseudo-Riemannian geometry. Let (M,gij) be a
smooth, n-dimensional pseudo-Riemannian manifold, and let
Rijkl denote the corresponding Riemann curvature tensor
. The
Ricci tensor Rij is commonly defined as the following contraction
of the full curvature tensor:
Rij=Rk.ikj |
The index symmetry of Rij, so defined, follows from the symmetry
properties of the Riemann curvature. To wit,
Rij=Rk=ikjRki=kjRk=jkiRji. |
It is also convenient to regard the Ricci tensor as a symmetric bilinear
form. To that end for vector-fields X,Y we will write
Ric(X,Y)=XiYjRij. |
Related objects.
Contracting the Ricci tensor, we obtain an important scalar invariant
R=Ri,i |
called the scalar curvature, and sometimes also called the Ricci scalar. Closely related to the Ricci tensor is the tensor
Gij=Rij-12Rgij, |
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
Sij=Rij-1nRgij. |
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 curvature 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∈TxM. Fix a point x∈M and a tangent vector
v∈TxM, and let
Sx(v)={u∈TxM:gx(u,u)=1,gx(u,v)=0} |
denote the n-2 dimensional
sphere of those unit vectors at x that are perpendicular
to v.
Let μx denote the natural
(n-2)-dimensional volume measure on TxM, 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 TxM 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 interpretation.
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
Fijkl | =1n-2(Sjlgik+Sikgjl-Silgjk-Sjkgil), | ||
Eijkl | =1n(n-1)R(gjlgik-gilgjk), | ||
Wijkl | =Rijkl-Fijkl-Eijkl. |
The Wijkl 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=ikj0. |
The Eijkl and Fijkl correspond to the trace-free part of the Ricci curvature tensor, and to the Ricci scalar. Indeed, we can recover Sij and R from Eijkl and Fijkl as follows:
Sij | =Fk,ikj | ||
Eijij | =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 signature
(3,1). The Einstein field equations assert that the energy-momentum
tensor is proportional to the Einstein tensor. In particular, the
equation
Rij=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 manifold 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 |