Proofs involving covariant derivatives

From Infogalactic: the planetary knowledge core
Jump to: navigation, search

This article contains proof of formulas in Riemannian geometry that involve the Christoffel symbols.

Contracted Bianchi identities

Proof

Start with the Bianchi identity[1]

 R_{abmn;l} + R_{ablm;n} + R_{abnl;m} = 0\,\!.

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

  g^{bn} g^{am} (R_{abmn;l} + R_{ablm;n} + R_{abnl;m}) = 0,\,\!
 g^{bn} (R^m {}_{bmn;l} - R^m {}_{bml;n} + R^m {}_{bnl;m}) = 0,\,\!
 g^{bn} (R_{bn;l} - R_{bl;n} - R_b {}^m {}_{nl;m}) = 0,\,\!
 R^n {}_{n;l} - R^n {}_{l;n} - R^{nm} {}_{nl;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} - R^n {}_{l;n} - R^m {}_{l;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} = 2 R^m {}_{l;m},\,\!

which is the same as

 \nabla_m R^m {}_l = {1 \over 2} \nabla_l R\,\!.

Swapping the index labels l and m yields

 \nabla_l R^l {}_m = {1 \over 2} \nabla_m R\,\!,      Q.E.D.     (return to article)

The covariant divergence of the Einstein tensor vanishes

Proof

The last equation in Proof 1 above can be expressed as

 \nabla_l R^l {}_m - {1 \over 2} \delta^l {}_m \nabla_l R = 0\,\!

where δ is the Kronecker delta. Since the mixed Kronecker delta is equivalent to the mixed metric tensor,

 \delta^l {}_m = g^l {}_m,\,\!

and since the covariant derivative of the metric tensor is zero (so it can be moved in or out of the scope of any such derivative), then

 \nabla_l R^l {}_m - {1 \over 2} \nabla_l g^l {}_m R = 0.\,\!

Factor out the covariant derivative

 \nabla_l \left(R^l {}_m - {1 \over 2} g^l {}_m R\right) = 0,\,\!

then raise the index m throughout

 \nabla_l \left(R^{lm} - {1 \over 2} g^{lm} R\right) = 0.\,\!

The expression in parentheses is the Einstein tensor, so [1]

 \nabla_l G^{lm} = 0,\,\!     Q.E.D.    (return to article)

this means that the covariant divergence of the Einstein tensor vanishes.

See also

References

  1. 1.0 1.1 Lua error in package.lua at line 80: module 'strict' not found.

Books

  • Lua error in package.lua at line 80: module 'strict' not found.
  • Lua error in package.lua at line 80: module 'strict' not found.
  • Lua error in package.lua at line 80: module 'strict' not found.
  • Lua error in package.lua at line 80: module 'strict' not found.
  • Lua error in package.lua at line 80: module 'strict' not found.
  • Lua error in package.lua at line 80: module 'strict' not found.
  • Lua error in package.lua at line 80: module 'strict' not found.


<templatestyles src="Asbox/styles.css"></templatestyles>