Magnetic Fields, Turbulence and Cosmic Rays in Galaxy Clusters

Details Magnetic Fields, Turbulence and Cosmic Rays in Galaxy Clusters Magnetic Fields, Turbulence and Cosmic Rays in Galaxy Clusters

Aug 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011scgg.conf....7d&link_type=abstract

"Structure in Clusters and Groups of Galaxies in the Chandra Era, 2011 Chandra Science Workshop held July 12-14, 2011. Edited by

Computer Science

Scientific paper

In galaxy clusters, non-thermal components such as magnetic field, turbulence and high energy particles keep a record of the processes acting since early times till now. These components play key roles by controlling transport processes inside the cluster atmosphere and therefore have to be understood in detail. Although including them in simulations is extremely challenging as the structures in and around clusters are quite complex and span a very large dynamic range in scales, it allows us to put constrains on turbulence and the presence of cosmic rays in galaxy clusters by comparing in detail the induced radio emission in these simulations with observations.

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