Geometric meaning of Christoffel symbol

 

 Covariant derivative

 

Since direction of basis vector might differ between two distinct points on curvature, we have to compare the difference of two vectors by setting their starting points on a single point.

 

Let A^i+dA^i(A^i+\delta A^i) be a vector which we moved vector A^i (parallel to curvature) from P_1 to P_2.

The difference we are looking for is

DA^i=A^i+dA^i-(A^i+\delta A^i)=dA^i-\delta A^i

     Let us define   \delta A^i=-\Gamma_{kl}^iu^kdx^l   and   A_{;l}^i=\frac{DA^i}{dx^l}.

 

(We will see later that this \Gamma_{kl}^i corresponds to the Cristoffel symbol we saw in geodesic equation.)

then                  A_{;l}^i=A_{,l}^i+\Gamma_{ik}^iA^k

since scalar is invariant,   \delta(u_iu^i)=0,  A_{i;l}=A_{i,l}-\Gamma_{il}^kA_k.

 

 

 Riemann tensor

 

Let us calculate difference the vector make while we move it parallel to infinitely small closed curve on curvature. It is,

\Delta A_k=\oint\Gamma_{kl}^iA_idx^l,  then  \frac{\partial A_i}{\partial x^l}=\Gamma_{il}^nA_n.

 

Thus     \Delta A_k=\frac{1}2(\frac{\partial \Gamma_{km}^lA_i}{\partial x^l}-\frac{\partial \Gamma_{kl}^iA_i}{\partial x^m})\Delta f^{lm}   (\because Stokes theorem) 

         =\frac{1}2(\frac{\partial \Gamma_{km}^i}{\partial x^l}-\frac{\partial \Gamma_{kl}^i}{\partial x^m}+\Gamma_{nl}^i\Gamma_{km}^n-\Gamma_{nm}^i\Gamma_{kl}^n)A_i\Delta f^{lm}

and here we define

Riemann tensor: R_{klm}^i=\frac{1}2(\frac{\partial \Gamma_{km}^i}{\partial x^l}-\frac{\partial \Gamma_{kl}^i}{\partial x^m}+\Gamma_{nl}^i\Gamma_{km}^n-\Gamma_{nm}^i\Gamma_{kl}^n)

 

 

 Relation between Riemann tensor and Cristoffel symbol

 

Since scalar is invariant during parallel translation,

(g_{mn}+g_{mn,b}dx^b)(A^m-\Gamma_{ab}^mA^adx^b)(A^{n}-\Gamma_{ab}^nA^adx^b)=g_{mn}A^mA^n

Since coefficent of dx^b is zero,

g_{mn,b}=g_{an}\Gamma_{mb}^a+g_{ma}\Gamma_{nb}^a=\Gamma_{nmb}+\Gamma_{mnb}

        also  g_{mb,n}=\Gamma_{bmn}+\Gamma_{mbn},  g_{bn,m}=\Gamma_{mnb}+\Gamma_{bnm}.

 

thus        \Gamma_{bn}^c=g^{cn}\Gamma_{cbn}=\frac{1}2g^{cm}(g_{an,m}+g_{ma,n}-g_{nm,a}).

 

Later we will use the results of these long calculations when we calculate the radius of blackhole; event horizon.

 

 

 Reference

The Classical Theory of Fields (L.D.Landau and E.M.Lifshitz)