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Explore quasi-3D kinetic simulations of particle acceleration in relativistic magnetized jets through this 22-minute conference talk by Gabrielle Guttormsen from UCLA. Delve into the complex plasma processes occurring around exotic relativistic astrophysical objects like black holes and neutron stars, examining how magnetic reconnection and shocks operate under extreme conditions where relativistic, radiative, and QED effects become significant. Learn about computational approaches to understanding particle acceleration mechanisms in relativistic jets, which are crucial for explaining spectacular phenomena such as the first images of accreting black holes at event-horizon scales and enigmatic Fast Radio Bursts. Discover how kinetic simulations provide insights into nonlinear plasma processes that challenge our current understanding of high-energy astrophysical environments. Gain knowledge about the intersection of plasma theory, computational physics, and observational astrophysics in studying extreme plasma conditions that cannot be replicated in terrestrial laboratories.
