The Mathematical Theory of RelativityEddington, Arthur Stanley, Sir
Science
The Mathematical Theory of Relativity
Eddington, Arthur Stanley, Sir
Relativity (Physics)
Formulae analogous to~\Eq{(34.3)} can be obtained for the second derivatives
of a tensor~$A_{...\mu..}$ instead of for a vector~$A_{\mu}$. The result is easily found to be
\[
A_{...\mu..\nu\sigma} - A_{...\mu..\sigma\nu} = \sum B_{\mu\sigma\nu}^{\epsilon} A_{...\epsilon..},
\Tag{(34.8)}
\]
the summation being taken over all the suffixes~$\mu$ of the original tensor.
The corresponding formulae for contravariant tensors follow at once, since
the $g^{\mu\nu}$ behave as constants in covariant differentiation, and suffixes may be
raised on both sides of~\Eq{(34.8)}.
\PageSep{74}
\Section{35.}{Miscellaneous formulae}
The following are needed for subsequent use--- \\
Since
\begin{gather*}
g_{\mu\nu} g^{\mu\alpha} = \text{$0$ or $1$,} \\
g^{\mu\alpha} \, dg_{\mu\nu} + g_{\mu\nu}\, dg^{\mu\alpha} = 0.
\end{gather*}
Hence
\begin{align*}
g^{\mu\alpha}\, g^{\nu\beta} \, dg_{\mu\nu}
&= -g_{\mu\nu}\, g^{\nu\beta}\, dg^{\mu\alpha}
= -g_{\mu}^{\beta}\, dg^{\mu\alpha} \\
&= -dg^{\alpha\beta}.
\Tag{(35.11)}
\end{align*}
Similarly
\[
dg_{\alpha\beta} = -g_{\mu\alpha} g_{\nu\beta}\, dg^{\mu\nu}.
\Tag{(35.12)}
\]
Multiplying by~$A^{\alpha\beta}$, we have by the rule for lowering suffixes
\begin{align*}
A^{\alpha\beta}\, dg_{\alpha\beta}
&= -(g_{\mu\alpha} g_{\nu\beta}A^{\alpha\beta})\, dg^{\mu\nu} \\
&= -A_{\mu\nu}\, dg^{\mu\nu}
= -A_{\alpha\beta}\, dg^{\alpha\beta}.
\Tag{(35.2)}
\end{align*}
For any tensor~$B_{\alpha\beta}$ other than the fundamental tensor the corresponding
formula would be
\[
A^{\alpha\beta}\, dB_{\alpha\beta} = A_{\alpha\beta}\, dB^{\alpha\beta}
\]
by~\Eq{(26.3)}. The exception for $B_{\alpha\beta} = g_{\alpha\beta}$ arises because a change~$dg_{\alpha\beta}$ has an
additional indirect effect through altering the operation of raising and lowering
suffixes.
Again $dg$~is formed by taking the differential of each~$g_{\mu\nu}$ and multiplying
by its co-factor~$g · g^{\mu\nu}$ in the determinant. Thus
\[
\frac{dg}{g} = g^{\mu\nu}\, dg_{\mu\nu} = -g_{\mu\nu}\, dg^{\mu\nu}.
\Tag{(35.3)}
\]
The contracted $3$-index symbol
\index{Three-index symbol!contracted}%
\begin{align*}
\{\mu\sigma, \sigma\}
&= \tfrac{1}{2} g^{\sigma\lambda} \left\{
\frac{\dd g_{\mu\lambda}}{\dd x_{\sigma}}
+ \frac{\dd g_{\sigma\lambda}}{\dd x_{\mu}}
- \frac{\dd g_{\mu\sigma}}{\dd x_{\lambda}}\right\} \\
&= \tfrac{1}{2} g^{\sigma\lambda}\, \frac{\dd g_{\sigma\lambda}}{\dd x_{\mu}}.
\end{align*}
The other two terms cancel by interchange of the dummy suffixes $\sigma$ and~$\lambda$.
Hence by~\Eq{(35.3)}
\begin{align*}
\{\mu\sigma, \sigma\}
&= \frac{1}{2g}\, \frac{\dd g}{\dd x_{\mu}} \\
&= \frac{\dd}{\dd x_{\mu}} \log \sqrt{-g}.
\Tag{(35.4)}
\end{align*}
We use $\sqrt{-g}$ because $g$~is always negative for real coordinates.
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