http://arxiv.org/abs/2112.09673
We have shown the simultaneous generation of macro-scale fast flows and strong magnetic fields in the 2-temperature relativistic electron-ion plasmas of astrophysical objects due to Unified Reverse Dynamo/Dynamo mechanism. The resulting dynamical magnetic field amplification and/or flow acceleration is directly proportional to the initial turbulent kinetic/magnetic (magnetic) energy; the process is very sensitive to relativistically hot electron-ion fraction temperature and magneto-fluid coupling. It is shown, that for realistic physical parameters of White Dwarfs accreting hot astrophysical flow / Binary systems there always exists such a real solution of dispersion relation for which the formation of dispersive strong super-Alfv\’enic macro-scale flow/outflow with Alfv\’en Mach number $> 10^6$ and/or generation of super-strong magnetic fields is guaranteed.
K. Kotorashvili and N. Shatashvili
Mon, 20 Dec 21
55/59
Comments: 15 pages of two-column text, 10 figures, accepted for publication in Astrophysics and Space Science, manuscript number ASTR-D-21-00328R1
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