Collisionless Shock & Accretion Disk

[HEDS9-06] High-energy neutrino emission from collisionless shocks in black hole coronae

*Minh Nhat Ly¹, Takayoshi Sano¹, Yoshiyuki Inoue^2,3,4, Youichi Sakawa¹, Yasuhiko Sentoku¹ (1. Institute of Laser Engineering, Osaka University, 2. Department of Earth and Space Science, Graduate School of Science, Osaka University, 3. Interdisciplinary Theoretical & Mathematical Science Program (iTHEMS), RIKEN, 4. Kavli Institute for the Physics and Mathematics of the Universe (WPI), UTIAS, The University of Tokyo)

Diffusive shock acceleration scenario has been proposed to explain proton acceleration leading to high-energy neutrino production in black hole corona. Here, we employ PIC simulations of collisionless shocks using parameters derived from NGC 1068 coronae to thoroughly examine this scenario