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Explore how radiative relativistic turbulence functions as an in situ pair-plasma source in blazar jets through this 19-minute conference talk by John Mehlhaff from Washington University. Examine the complex plasma processes occurring in extreme astrophysical environments around black holes and neutron stars, where relativistic, radiative, and quantum electrodynamics effects become critically important. Learn about the challenges posed by recent observational discoveries, including event-horizon scale images of accreting black holes and Fast Radio Bursts, and how these phenomena require new understanding of nonlinear plasma processes like magnetic reconnection and shocks under extreme conditions. Discover the interdisciplinary approach needed to advance research in this field, combining insights from observational and theoretical high-energy astrophysics, plasma theory, computational physics, and experimental laser-plasma studies. Gain insights into the current progress and future strategic directions for understanding extreme plasma behavior in relativistic astrophysical objects.
