Multi-Phase Turbulence - The Interaction Between Radiative Cooling and Turbulence

Explore the complex interplay between radiative cooling and turbulence in multi-phase environments through this 28-minute conference talk by Peng Oh from UCSB. Delivered as part of the "Turbulence in the Universe" conference at the Kavli Institute for Theoretical Physics, the presentation delves into the crucial role of turbulence in various astrophysical settings, from stellar interiors to the intra-cluster medium. Gain insights into recent advancements in observational and theoretical studies of astrophysical turbulence, and understand how these developments have influenced multiple branches of astronomy. The talk contributes to a broader discussion on topics such as turbulent dynamo, magnetic reconnection, plasma physics, and astrophysical applications of magnetized turbulence, fostering interdisciplinary collaboration among experts in astrophysics and physics.