How strong is the gravity of general relativity?
How much radial force is required to keep a particle with mass $m$ at a certain distance $r$ from a black hole with mass $M$? We know that Newtonian gravity $$f=\frac{GmM}{r^2}$$ provides a good approximation of the force, $f$, for low energy cases. But what is the exact difference a) for a far-away observer, and b) within the reference frame of the particle?