JorgeM
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The discussion centers on the application of electromagnetic (EM) fields in solving the classical three-body problem. By knowing the positions and velocities of bodies along with the EM-field parameters, such as the electric field vector ##\vec{E}(t)## and magnetic field vector ##\vec{B}(t)##, one can compute the dynamics of the system over time. When approximating the speed of light to infinity (##c \to \infty##), the problem simplifies to a classical three-body scenario with an added Coulomb force. However, incorporating magnetic forces based on body positions may compromise the model's invariance under Galileo and Lorentz transformations.
PREREQUISITESPhysicists, mathematicians, and engineers interested in advanced dynamics, particularly those exploring the intersection of classical mechanics and electromagnetic theory.