Turbulence-Driven Magnetic Reconnection & Cosmic Ray Acceleration

Explore a 31-minute conference talk on turbulence-driven magnetic reconnection and cosmic ray acceleration presented by Elisabete M. de Gouveia Dal Pino from the University of São Paulo. Delivered as part of the "Turbulence in the Universe" conference at the Kavli Institute for Theoretical Physics, this presentation delves into the crucial role of turbulence in various astrophysical environments across vast scales. Gain insights into recent advances in observational and theoretical studies of astrophysical turbulence and their impact on multiple branches of astronomy. Discover how this interdisciplinary discussion covers topics such as turbulent dynamo, magnetic reconnection, plasma physics, space physics, numerical simulations, laboratory turbulence, observational techniques, and astrophysical applications of magnetized turbulence including star formation, cosmic rays, accretion, and galaxy formation and evolution.