Physics:Contracted Bianchi identities

From HandWiki

In general relativity and tensor calculus, the contracted Bianchi identities are:[1]

ρRρμ=12μR

where Rρμ is the Ricci tensor, R the scalar curvature, and ρ indicates covariant differentiation.

These identities are named after Luigi Bianchi, although they had been already derived by Aurel Voss in 1880.[2] In the Einstein field equations, the contracted Bianchi identity ensures consistency with the vanishing divergence of the matter stress–energy tensor.

Proof

Start with the Bianchi identity[3]

Rabmn;+Rabm;n+Rabn;m=0.

Contract both sides of the above equation with a pair of metric tensors:

gbngam(Rabmn;+Rabm;n+Rabn;m)=0,
gbn(Rmbmn;Rmbm;n+Rmbn;m)=0,
gbn(Rbn;Rb;nRbmn;m)=0,
Rnn;Rn;nRnmn;m=0.

The first term on the left contracts to yield a Ricci scalar, while the third term contracts to yield a mixed Ricci tensor,

R;Rn;nRm;m=0.

The last two terms are the same (changing dummy index n to m) and can be combined into a single term which shall be moved to the right,

R;=2Rm;m,

which is the same as

mRm=12R.

Swapping the index labels l and m on the left side yields

Rm=12mR.

See also

Notes

References