Gamma ray emission and stochastic particle acceleration in galaxy clusters

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dc.creatorBrunetti, G.
dc.creatorBlasi, P.
dc.creatorCassano, R.
dc.creatorGabici, S.
dc.date2008-11-06
dc.date.accessioned2026-07-07T12:43:17Z
dc.date.available2026-07-07T12:43:17Z
dc.descriptionFERMI (formely GLAST) will shortly provide crucial information on relativistic particles in galaxy clusters. We discuss non-thermal emission in the context of general calculations in which relativistic particles (protons and secondary electrons due to proton-proton collisions) interact with MHD turbulence generated in the cluster volume during cluster mergers. Diffuse cluster-scale radio emission (Radio Halos) and hard X-rays are produced during massive mergers while gamma ray emission, at some level, is expected to be common in galaxy clusters.
dc.description4 pages, 2 Figure, proc. of the 4th Heidelberg International Symposium on High Energy Gamma-ray Astronomy
dc.identifierhttps://arxiv.org/abs/0811.1010
dc.identifierhttp://arxiv.org/abs/0811.1010
dc.identifierAIP Conf.Proc.1085:628-631,2009
dc.identifierdoi:10.1063/1.3076753
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/220371
dc.subjectAstrophysics
dc.titleGamma ray emission and stochastic particle acceleration in galaxy clusters
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