The Chronology of High-k Magnetic Modes - From Small-Scale Dynamo to Driven Stationary Magnetized Turbulence

Explore the evolution of high-k magnetic modes in astrophysical plasmas through this 45-minute conference talk examining the progression from small-scale dynamo processes to driven stationary magnetized turbulence. Delve into the complex magnetic field dynamics that occur in extreme astrophysical environments around black holes and neutron stars, where relativistic effects become crucial. Learn about the chronological development of magnetic modes at small scales and understand how these processes contribute to the spectacular phenomena observed in exotic relativistic objects. Discover the theoretical framework connecting small-scale magnetic field generation through dynamo mechanisms to the sustained turbulent magnetic states that characterize these extreme plasma environments. Gain insights into the fundamental plasma physics underlying some of the most energetic and puzzling astrophysical phenomena, including the magnetic processes that may explain recent observational discoveries such as black hole imaging and Fast Radio Bursts.