Oh, Peng2016-08-302016-08-302016-08-23https://hdl.handle.net/11299/182011I 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.enICMFTPIHow Turbulence Accelerates Cosmic Rays and Amplifies B-fields in the ICMPresentation