Macroscale fast flow and magnetic-field generation in two-temperature relativistic electron–ion plasmas of astrophysical objects

We have shown the simultaneous generation of macro-scale fast flows and strong magnetic fields in 2-temperature relativistic electron-ion plasmas astrophysical objects due to Unified Reverse Dynamo/Dynamo mechanism. The resulting dynamical field amplification and/or flow acceleration is directly proportional initial turbulent kinetic/magnetic (magnetic) energy; process very sensitive relativistically hot fraction temperature magneto-fluid coupling. It shown, that for realistic physical parameters White Dwarfs accreting / Binary systems there always exists such a real solution dispersion relation which formation dispersive super-Alfv\'enic flow/outflow with Alfv\'en Mach number $> 10^6$ super-strong guaranteed.