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Models of particle acceleration in galaxy clusters by MHD turbulence

Published online by Cambridge University Press:  21 October 2010

G. Brunetti
G. Brunetti*
Affiliation:
INAF Istituto di Radioastronomia, via P. Gobetti 101, I–40129, Bologna, Italy email: brunetti@ira.inaf.it
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Abstract

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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

acceleration of particlesradiation mechanisms: nonthermalturbulencegalaxies: clusters: general
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

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