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

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