Published in

Cambridge University Press (CUP), Proceedings of the International Astronomical Union, H15(5), p. 466-467, 2009

DOI: 10.1017/s1743921310010306

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Models of particle acceleration in galaxy clusters by MHD turbulence

Journal article published in 2009 by G. Brunetti ORCID
This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

Full text: Unavailable

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Data provided by SHERPA/RoMEO

Abstract

AbstractPresent 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.

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