Number density of accelerated leptons shown in contrast with different fluid quantities in the orbital plane for an orbital phase of φ = 0.41 during the second orbit. We show the accelerated leptons on the upper left for an energy of 485.5 GeV (see also Fig. 1). Additionally, we show the representative fluid quantities in the form of the mass density (upper right), the thermal pressure (lower left) and the absolute value of the spatial component of the fluid’s four velocity (lower right).