Speaker
Description
This work is dedicated to develop the most detailed comprehensive numerical framework to date, combining magnetohydrodynamics (MHD) and Monte-Carlo simulations to derive the multi-wavelength (MWL) and multi-messenger spectra from the magnetized environment of galaxy clusters. Special attention will be given to Perseus-like clusters hosting active galactic nuclei (AGNs). We will study Propagation of the cosmic ray (CR) in the ICM through multi-dimensional Monte-carlo simulations, considering all relevant interaction processes. Machine learning and data analysis techniques is the essential part of the research work to ensure the robustness and timely production of research products. This work is suitable to appropriately interpret the observed emissions from clusters and provide source distribution constraints for various observation facilities such as CTA, HAWC, LHAASO, IceCube-Gen2, TA, and Pierre Auger Observatory, etc.
