Gtr needed for galactic gravitation? No.
notknowing said:
The motivation for my question is related to the missing mass problem (in galaxies). Usually one compares the observed rotation curves (of stars) to the rotation curve based on a Newtonian potential and which reveals the well-known discrepancy. I was wondering whether there could be some extra GR-related terms (leading to an extra effective "force" towards the galaxy centre) which could mimic "extra matter". Has this been investigated in detail ? Would the corrections be so small that they can be ruled out to explain the galaxy rotation curves ?
I was too rushed to say this before, but at the averaged matter densities at galactic scales inferred from visible matter (shining stars), Newtonian gravitation should be quite adequate to determine the rotation curve. Thus, the observed rotation curves would be a huge problem for any theory of gravitation constructed to fit solar system scale data. Either gravitation behaves
very differently at galactic scales (for various reasons, hardly anyone buys this as the explanation), or there's some mass-energy we don't yet know about associated with galaxies. The lensing observations discussed by Sean Carroll at his blog and in other places provides some very convincing if indirect evidence that there's nothing wrong with gtr (or other "close mimics") at galactic scales; rather, it seems that there is indeed some mass-energy that corresponds to something we haven't yet identified. Actually, quite a lot of mass-energy.
So the best short answer to your question of whether relativistic corrections to Newtonian gravitation have any relevance to the galactic rotation curve problem is probably "no".
As for a centrally directed "gravitational force" associated with a disk which is a bit stronger (in the equatorial plane) than the "gravitational force" for an equal mass spherical object, that's true in Newtonian gravitation, but doesn't help at all with the rotation curve problem. There is nothing mysterious about this; the equipotentials look like spheres at large radii but nearer the object they look more like the shape of the equal-mass surfaces in the matter distribution inside the object; in this case, they look more like a disk, i.e. they become flattened and look like nested oblate spheroids near the disk. These are "more closely packed" in the equatorial plane near the disk, so the force is a big greater. Something similar happens in gtr and other such theories.
notknowing said:
One could for instance use the derived metric to obtain the path of a small test body just outside of the disk.
If you are back to the Neugebauer-Meinel exact solution modeling (in gtr) a rigidly rotating disk of dust, then, sure, in principle you can determine the geodesics of the vacuum exterior (everything outside a certain disk in the equatorial plane).