Simulation of the Radiation Reaction Orbits of a Classical Relativistic Charged Particle with Generalized Off-Shell Lorentz Force
Figure 13
The smaller scale polygonal orbit and its propagation. One can observe the cycling polygonal orbit “filling” the oval frame in a star-like pattern (a). There is also a sinusoidal propagation (b). Time step: 10-10 GeV-1. The scale is about 12 times smaller than the one in Figures 12(b)–12(d).
