Contracted Bianchi identities

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

∇ρRρμ=12∇μR

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] and independently by Gregorio Ricci-Curbastro in 1889.[3]Template:Reference page 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[4]

Rabmn;ℓ+Rabℓm;n+Rabnℓ;m=0.

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

gbngam(Rabmn;ℓ+Rabℓm;n+Rabnℓ;m)=0,
gbn(Rmbmn;ℓ−Rmbmℓ;n+Rmbnℓ;m)=0,
gbn(Rbn;ℓ−Rbℓ;n−Rbmnℓ;m)=0,
Rnn;ℓ−Rnℓ;n−Rnmnℓ;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;ℓ−Rnℓ;n−Rmℓ;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;ℓ=2Rmℓ;m,

which is the same as

∇mRmℓ=12∇ℓR.

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

∇ℓRℓm=12∇mR.

See also

Template:Div col

Template:Div col end

Notes

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References


Template:Mathanalysis-stub Template:Relativity-stub