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Explore particle acceleration mechanisms in three-dimensional turbulent magnetic reconnection through this 43-minute conference talk by Masahiro Hoshino from the University of Tokyo. Delve into the complex plasma physics processes that occur in extreme astrophysical environments around black holes and neutron stars, where relativistic, radiative, and quantum electrodynamics effects become crucial. Examine how magnetic reconnection operates under these extreme conditions and its role in accelerating particles to high energies. Learn about the theoretical frameworks and computational approaches used to understand these nonlinear plasma processes in three-dimensional turbulent systems. Discover the connections between laboratory plasma physics and astrophysical phenomena, including insights relevant to understanding Fast Radio Bursts and accretion processes near event horizons. Gain perspective on current research challenges in extreme plasma physics and the interdisciplinary approaches needed to advance our understanding of particle acceleration in cosmic environments.
