Number density of accelerated leptons in the orbital plane. Results for energies of 1.5 GeV (bottom), 485.5 GeV (middle), and 5467.7 GeV (top) as indicated above the corresponding plots. We show our results for eight different orbital phases of the second orbit as indicated in the plot. In each case, we depict a range of densities from the peak value at periastron to a factor of 10⁻⁵ of this value. Additionally, the white arrows indicate the direction towards the observer. An example for corresponding fluid quantities is shown in Fig. B.1 in Appendix B.