Reference frames in General Relativity and the galactic rotation curves
Filipe Costa  1@  , José Natário  1  , Francisco Frutos-Alfaro  2  , Michael Soffel  3  
1 : CAMGSD - IST Lisbon
2 : Space Research Center (CINESPA), University of Costa Rica, San José
3 : Lohrmann Observatory, Dresden TU

The physical interpretation of the exact solutions of the Einstein field equations is, in general, a challenging task, part of the difficulties lying in the significance of the coordinate system. I will discuss the extension of the International Astronomical Union (IAU) reference system to the exact theory. It will be seen that such an extension, retaining some of its crucial properties, can be achieved in a special class of spacetimes, admitting non-shearing congruences of observers which, at infinity, have zero vorticity and acceleration. As applications, we consider the FLRW solution, the Kerr and NUT black hole spacetimes, the van Stockum rotating dust cylinder, spinning cosmic strings and, finally, we debunk the so-called Balasin-Grumiller (BG) model, and the claims that the galactic rotation curves can be explained through gravitomagnetic effects without the need for Dark Matter. It is shown to be completely inappropriate as a galactic model: its dust is actually static with respect to the asymptotic inertial frame, its gravitomagnetic effects arise from unphysical singularities along the axis, and the rotation curves obtained are merely down to an invalid choice of reference frame -- the congruence of zero angular momentum observers, which are being dragged by the singularities. The same type of flaws are seen to affect other akin gravitomagnetic "galactic models" in the literature.


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