Title of article
Models of particle acceleration in galaxy clusters by MHD turbulence
Author/Authors
G. Brunetti، نويسنده ,
Issue Information
روزنامه با شماره پیاپی سال 2009
Pages
2
From page
466
To page
467
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
radiation mechanisms: nonthermal , galaxies: clusters: general , turbulence , acceleration of particles
Journal title
Proceedings of the International Astronomical Union
Serial Year
2009
Journal title
Proceedings of the International Astronomical Union
Record number
674775
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