Typically, a three body problem is extremely hard to put into numerical form. If someone has a numerical solution for a three body problem it would have to involve one force, where vectors would be used to solve the problem. The Sun, Earth and moon are a three body problem. The force involved in each case is that of gravitation. Trying to describe the motion of the Earth with a numerical solution is not straight forward. In the case of Hydrogen, one electron orbits a proton- a two body system. Bohr's theory was a solution to this two body problem, it equated electrostatic force or coulomb's law with an inward centripetal force. In the case of Helium, we have two electrons and one nucleus, a three body problem. In this case a solution is extremely difficult, because we have to consider not only the attraction between the electrons and the proton, but also electron-electron repulsion.
In order to be relevant we really need to know what three body problem you are referring too.