In general relativity and tensor calculus, the contracted Bianchi identities are:
\nabla\rho
\rho} | |
{R | |
\mu |
={1\over2}\nabla\muR
where
\rho} | |
{R | |
\mu |
R
\nabla\rho
These identities are named after Luigi Bianchi, although they had been already derived by Aurel Voss in 1880. In the Einstein field equations, the contracted Bianchi identity ensures consistency with the vanishing divergence of the matter stress–energy tensor.
Start with the Bianchi identity[1]
Rabmn;\ell+Rab\ell+Rabn\ell;m=0.
Contract both sides of the above equation with a pair of metric tensors:
gbngam(Rabmn;\ell+Rab\ell+Rabn\ell;m)=0,
gbn(Rm{}bmn;\ell-Rm{}bm\ell;n+Rm{}bn\ell;m)=0,
gbn(Rbn;\ell-Rb\ell;n-Rb{}m{}n\ell;m)=0,
Rn{}n;\ell-Rn{}\ell;n-Rnm{}n\ell;m=0.
R;\ell-Rn{}\ell;n-Rm{}\ell;m=0.
R;\ell=2Rm{}\ell;m,
\nablamRm{}\ell={1\over2}\nabla\ellR.
\nabla\ellR\ell{}m={1\over2}\nablamR.