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Explore high-energy neutrino emission from radiatively inefficient accretion flows through advanced 3D general relativistic magnetohydrodynamic (GRMHD) simulations in this 33-minute conference talk by Tomohisa Kawashima from NIT Ichinoseki. Delve into the complex plasma processes occurring around black holes and neutron stars, where extreme relativistic, radiative, and quantum electrodynamic effects become crucial for understanding exotic astrophysical phenomena. Learn how cutting-edge computational modeling reveals the mechanisms behind neutrino production in accretion flows that radiate inefficiently, providing insights into some of the most energetic processes in the universe. Discover the intersection of plasma physics, high-energy astrophysics, and computational methods as they apply to understanding the behavior of matter under the most extreme conditions found near compact objects. Gain understanding of how magnetic reconnection and shock processes operate in relativistic environments and their role in generating high-energy particles and neutrinos that can be detected by Earth-based observatories.
