Magnetic Fields in Galaxy Clusters - Insights from Synchrotron and X-Ray Intensity Gradients

Explore a 33-minute conference talk on magnetic fields in galaxy clusters, presented by Yue Hu from UW Madison at the Kavli Institute for Theoretical Physics. Delve into the analysis of synchrotron and X-ray intensity gradients to gain insights into the complex magnetic field structures within galaxy clusters. Learn about the latest advancements in observational and theoretical studies of astrophysical turbulence, covering topics such as turbulent dynamo, magnetic reconnection, and plasma physics. Understand the significance of turbulence across various astrophysical environments, from stellar interiors to the intra-cluster medium. Discover how this research contributes to broader discussions on star formation, cosmic rays, accretion, and galaxy formation and evolution.