There has been much speculation that the Schwarzschild field harbors regions of gravitational repulsion, witnessed by a positive acceleration. The criterion is that the radial velocity should be greater than B/31/2 , where B=(1-R/r), and R is the Schwarzschild radius. The radial velocity can, therefore, surpass the velocity of light. To avoid this, one usually claims that "local observers cannot detect gravitational repulsion, apparently because their measuring instruments are affected by gravity, whereas distant observers, whose instruments are not affected by the gravitational field, can measure a positive value for the acceleration of gravity." (McGruder, Phys. Rev. D 25 (1982) 3191) Apart from the fact that this would provide a means for the observers to distinguish their position through measurement (something outlawed in non-Euclidean geometries), the gravitational field of a distant observer is unaffected by gravity why should he measure a positive acceleration?

The assumption that the metric coefficients depend only r and not on t implies that the fields are completely static. So how do accelerations and velocities come in the description?

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