I am interested in the behavior of the proper volume when we switch the frame of reference. For example, I know that the proper volume element for the Schwarzschild and Kerr black holes may be extracted easily from the formulae:
$V=\sqrt{g}dr d\theta d\phi = \frac{r^{5/2} \sin (\theta )}{\sqrt{r-2 m}}$
(Where we only picked the spatial components of the $g_{\mu \nu}$ for the determinant)
However, I am interested in seeing how this proper volume changes when according to different observers. For example, I know that the local frame of reference can be expressed with a tetrad:
$e^m_\mu=\left( \begin{array}{cccc} \sqrt{\frac{r-2 m}{r}} & 0 & 0 & 0 \\ 0 & \sqrt{\frac{r^2}{r^2-2 m r}} & 0 & 0 \\ 0 & 0 & \sqrt{r^2} & 0 \\ 0 & 0 & 0 & \sqrt{r^2} \sin (\theta ) \\ \end{array} \right)$
Which fulfills: $e_{c}{}^{b} e_{e}{}^{d} g_{bd} = \eta_{c e}$ (the tetrad transformation into the local frame of reference)
Now I am interested in finding out what the proper volume $V_{\rm local}$ is in this local frame of reference given by the tetrad. Is this possible?