COLLIMATED ESCAPING VORTICAL POLAR e−e+ JETS INTRINSICALLY PRODUCED BY ROTATING BLACK HOLES AND PENROSE PROCESSES

In this paper, I present results from theoretical and numerical (Monte Carlo) N-particle fully relativistic 4-D analysis of Penrose scattering processes (Compton and γγ −→ ee) in the ergosphere of a supermassive or stellar mass Kerr (rotating) black hole. Specifically, the escape conditions and the escaping orbits of the Penrose pair production (γγ −→ ee) electrons are analyzed, revealing that these particles escape along collimated, jet geodesic trajectories encircling the polar axis. Such collimated vortical tightly wound coil-like trajectories of relativistic particles are inherent properties of rotating black holes. The helical polar angles of escape for these ee pairs range from ∼ 40 to ∼ 0.5 (for the highest energy particles). These jet distributions appear to be consistent with the astrophysical jets of active galactic nuclei (AGNs) and galactic black holes, and suggest a mechanism for precollimation within the inner radius of the dynamically stable accretion disk. Subject headings: acceleration of particles—black hole physics: jets: general— gravitation—relativity