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arXiv · 1005.3699

Non-thermal emission from galaxy clusters: a Pandora's vase for astrophysics

C. Ferrari
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Abstract

The existence of cosmic rays and weak magnetic fields in the intracluster volume has been well proven by deep radio observations of galaxy clusters. However a detailed physical characterization of the non-thermal component of large scale-structures, relevant for high-precision cosmology, is still missing. I will show the importance of combining numerical and theoretical works with cluster observations by a new-generation of radio, Gamma- and X-ray instruments.

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C. Ferrari. 2010-05-20. Non-thermal emission from galaxy clusters: a Pandora's vase for astrophysics. https://arxiv.org/abs/1005.3699

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