Can General Relativity be "translated" to a language of forces in the analogous way that Newtonian gravity can be formulated in geometric terms? I know from "Gravitation" of Misner, Thorne and Wheeler(MTW) that Newtonian gravity can be formulated in a geometric language. Can we do the reverse for General Relativity? That is, could General Relativity be formulated or translated to a language of forces?  
 A: In some special cases like the Schwarzschild-case it can, the equation of motion for a massless test particle then becomes:
$$\ddot{r}(t) = -\frac{G\cdot M}{r(t)^2} + r(t)\cdot \dot{{\theta}}(t)^2 {\color{red} {- \frac{3\cdot G\cdot M\cdot \dot{{\theta}}(t)^2}{c^2}}}$$
for the radial acceleration,
$$\ddot{{\theta}}(t) = -2\cdot \dot{r}(t)/r(t)\cdot \dot{{\theta}}(t)$$
for the angular acceleration and
$${\color{red} {\dot{{\tau}}(t) = \frac{\sqrt{c^2\cdot r(t)-c^2\cdot  r_s +r(t)\cdot r \dot{(t)}^2- r_s\cdot  r(t)^2\cdot \dot{\theta}(t)^2+r(t)^3\cdot \dot{\theta}(t)^2}}{c\cdot \sqrt{r(t)- r_s } \cdot\sqrt{1-\frac{ r_s }{r(t)}}}}}$$
for the time dilation.
The newtonian equation of motion is the same, but without the red terms.
The transformation from the local velocity to the local coordinate speed is
$$\dot{r} = \frac{v_{\parallel}\color{green}{\cdot \sqrt{1-r_s/r}}}{\color{blue}{ \sqrt{ 1-v^2/c^2}}}$$
with an extra term in the numerator for the gravitational length contraction for the radial, and
$$\dot{\theta} = \frac{ v_{\perp}}{\color{blue}{ \sqrt{ 1-v^2/c^2}}\cdot r}$$
for the angular component (with newton the blue and green terms vanish) where $\perp$ stands for the transversal and $\parallel$ for the radial component, so by Pythagoras $v^2=v_{\perp}^2+v_{\parallel}^2$ .
To get the shapiro-delayed velocity as observed by a field-free observer you multiply $v_{\parallel}$ with $1-r_s/r$ and $v_{\perp}$ with $\sqrt{1-r_s/r}$.
In other cases where you have more than 2 bodies of which one's mass is neglible it might be a different story, but if you have only one significant mass and almost massless test particles you can describe it in an almost newtonian way, like in the Schwarzschild oder Kerr case.
But I have no idea how you would deal with a full relativistic n-body simulation, that might be a little more complicated than with Newton.
A: This is like asking whether Statistical mechanics can be reformulated in terms of Thermodynamics. Statistical mechanics is the microscopic description that puts Thermodynamics on a firmer ground. In the same fashion what Newton called a force is what you get when curvatures in space-time are low and change very slowly and velocities are well below the speed of light. 
One of the major lessons of GR is that even gravity is a fictitious force. It is on the same grounds as Coriolis force and centrifugal force. What you are asking for is a reformulation of a fundamental theory of space-time in terms of fictitious forces. 
