Signature of Plausible Accreting Supermassive Black Holes in Mrk 261/262 and Mrk 266
Figure 10
EH: event horizon, AD: accretion disk, SPC: superdense protomatter core, and PC: protomatter core. (a) The phenomenological model of AGN with the central stationary black hole. The meaningless singularity occurs at the center inside of the black hole. Either the Kruskal continuation of the metric for a Schwarzschild black hole or the Kerr metric shows that the static observers do not exist inside the horizon. Any timelike world line inside the EH must strike the central singularity which wholly absorbs the infalling particles. This disables an accumulation of matter in the central part, and, thus, neither a growth of black hole nor an increase of its mass-energy density occur at accretion of outside matter. (b) The microscopic model of AGN with central stable SPC, due to which the stable equilibrium holds in outward layers too and, thus, now an accumulation of matter allowed around SPC inside the EH. The static observers can exist inside the EH. The SPC accommodates the highest energy scale >1021 eV in PC. With time, an infalling matter forms PD around PC tapering off faster at reaching out the thin edge of EH. At this, metric singularity cutoff [6, 7] is switched on and the neutrinos of huge energies may escape through the vista to the outside world.
