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Models of particle acceleration in galaxy clusters by MHD turbulence
Published online by Cambridge University Press: 21 October 2010
Abstract
Present radio data provide indirect evidence that diffuse radio emission in the central cluster regions may originate from turbulent-acceleration of relativistic particles. I was invited to discuss models of particle acceleration by MHD turbulence in clusters and in these pages I briefly touch the main points of my talk.
Keywords
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 466 - 467
- Copyright
- Copyright © International Astronomical Union 2010