Title
How Turbulence Accelerates Cosmic Rays and Amplifies B-fields in the ICM
Abstract
I address the role of turbulence in accelerating cosmic rays in cluster radio halos, and whether matching the observations requires fine tuning. I also consider how turbulence induced by shock-clump interactions amplify B-fields, and implications for radio relics.
Suggested Citation
Oh, Peng.
(2016).
How Turbulence Accelerates Cosmic Rays and Amplifies B-fields in the ICM.
Retrieved from the University of Minnesota Digital Conservancy,
https://hdl.handle.net/11299/182011.