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How Turbulence Accelerates Cosmic Rays and Amplifies B-fields in the ICM
Oh, Peng (2016)
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https://hdl.handle.net/11299/182011
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Title
How Turbulence Accelerates Cosmic Rays and Amplifies B-fields in the ICM
Authors
Issue Date
2016-08-23
Type
Presentation
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.
Keywords
ICM
Appears in collections
Physics of the Intracluster Medium: Theory and Computation 2016 [31]
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.
Content distributed via the University of Minnesota's Digital Conservancy may be subject to additional license and use restrictions applied by the depositor.