In the weak field limit of general relativity (with matter described by a perfect fluid consisting only of dust), we have the following correspondences:
- $00$-component of the Einstein field equations (EFEs) $\leftrightarrow$ Poisson's equation $\nabla^2\phi = 4\pi G \rho$;
- spatial components of the geodesic equation $\leftrightarrow$ force equation $\vec{g} = -\vec{\nabla}\phi$,
where $\phi$ is the Newtonian gravitational potential. My question is about the other components of the EFEs and geodesic equation. In the several textbooks I have consulted these are not worked out or discussed. The remaining $0$-component of the geodesic equation reduces nicely to $0=0$ and hence does not add anything. Similarly for the mixed $0i$-components of the EFEs. But the $ij$-components of the EFEs do not seem to reduce to a triviality. In fact, we obtain an equation of the form (schematically)
$$\sum \partial_i\partial_j h_{\mu\nu} = 0,$$
where the sum represents the fact that there are several of these terms with permuted indices (some of which are contracted over). This equation constrains the spatial and mixed components $h_{ij}, h_{0i}$ in terms of $h_{00} = 2 \phi/c^2$. Does this represent anything physical? Since the $h_{ij}, h_{0i}$ components do not enter in the (approximate) geodesic equation for massive particles in the Newtonian limit, the equation has no bearing on the movement of (massive) test particles, at least. I'm wondering whether it is still relevant in any way.