Solving the Three-Body Problem via the Dual Rotational Current Model

This paper presents a deterministic solution to the Three-Body Problem based exclusively on the ”Dual Rotational Current Model.” Unlike classical mechanics which relies on point- mass attraction leading to chaotic variables, this model treats celestial bodies as nodes of concentrated magnetic currents within a symmetrical helical medium. By applying the principles of flux density and dual torque balance, trajectory prediction becomes a matter of calculating the geometric equilibrium of the vacuum fabric.