What is a covariant derivative

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SUMMARY

The covariant derivative, denoted as D, is a coordinate-dependent adjustment to the ordinary derivative that ensures the partial derivatives of coordinate unit vectors are zero. This adjustment is facilitated by a linear operator known as the connection, represented by the Christoffel symbols, \(\Gamma^i_{\ jk}\). The covariant derivative of the metric tensor \(g_{ij}\) is zero, and it maintains the tensorial nature of any tensor it operates on. Furthermore, a vector \(V^i\) is parallel transported along a curve \(x^i(s)\) if its covariant directional derivative in the direction of the tangent \(T^i(s)\) is zero.

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Definition/Summary

Covariant derivative, D, is a coordinate-dependent adjustment to ordinary derivative which makes each partial derivative of each coordinate unit vector zero: D\hat{\mathbf{e}}_i/\partial x_j\ =\ 0

The adjustment is made by a linear operator known both as the connection, \Gamma^i_{\ jk}, and as the Christoffel symbol, \{^{\ i\ }_{j\ k}\}.

Covariant derivative of the metric (g_{ij}) is zero.

Covariant derivative (unlike ordinary derivative) of any tensor is also a tensor (with an extra covariant index).

A vector V^i is parallel transported along a curve x^i(s) with tangent T^i(s) if its covariant directional derivative in the direction of that tangent is zero: (T.D)V^i/ds\ =\ 0

Equations

\frac{DV^i}{\partial x^j}\left(\text{also written}\ \frac{DV^i}{Dx^j}\ \text{or}\ \nabla_jV^i\ \text{or}\ V^i_{\ ;\,j}\right)\ =\ \frac{\partial V^i}{\partial x^j}\ -\ \Gamma^i_{\ jk}V^k

\frac{D\,(a^i\hat{\mathbf{e}}_i)}{\partial x^j}\ =\ 0\ \text{for constant}\ a^i

\frac{Dg^{ij}}{\partial x^k}\ =\ 0

\Gamma^i_{\ jk}\ =\ \Gamma^i_{\ kj}

\Gamma^i_{\ jk}\ =\ \{^{\ i\ }_{j\ k}\}\ =\ \frac{1}{2}\,g^{il}\left(\frac{\partial g_{jl}}{\partial x^k}\ +\ \frac{\partial g_{kl}}{\partial x^j}\ -\ \frac{\partial g_{jk}}{\partial x^l}\right)

Parallel transport of a vector V^i along a curve x^i(s):

\frac{dx^j}{ds}\frac{DV^i}{\partial x^j}\ =\ 0\ \ \text{or}\ \ dV^i = -\Gamma^i_{\ jk}V^kdx^j

Geodesic deviation equation:

\frac{D^2\,\delta x^{\alpha}}{d\tau^2}\ =\ -\,R^{\alpha}_{\ \mu\beta\sigma}\,V^{\mu}\,V^{\sigma}\,\delta x^{\beta}

Extended explanation



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