How Turbulence Accelerates Cosmic Rays and Amplifies B-fields in the ICM

Oh, Peng
2016-08-23
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How Turbulence Accelerates Cosmic Rays and Amplifies B-fields in the ICM

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2016-08-23

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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.

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Physics of the Intracluster Medium: Theory and Computation 2016

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Oh, Peng. (2016). How Turbulence Accelerates Cosmic Rays and Amplifies B-fields in the ICM. Retrieved from the University Digital Conservancy, https://hdl.handle.net/11299/182011.

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