Non-thermal Emissions from Cool Cores Heated by Cosmic-Rays in Galaxy Clusters
Authors: Yutaka Fujita, Yutaka Ohira
http://arxiv.org/abs/1111.4208
Abstract: We study non-thermal emissions from cool cores in galaxy clusters. We adopted a recent model, in which cosmic-rays (CRs) prevail in the cores and stably heat them through CR streaming. The non-thermal emissions come from the interaction between CR protons and intracluster medium (ICM). Comparison between the theoretical predictions and radio observations shows that the overall CR spectra must be steep, and most of the CRs in the cores are low-energy CRs. Assuming that the CRs are injected through AGN activities, we study the nature of the shocks that are responsible for the CR acceleration. The steep CR spectra are likely to reflect the fact that the shocks travel in hot ICM with fairly small Much numbers. We also study the dependence on the CR streaming velocity. The results indicate that synchrotron emissions from secondary electrons should be observed as radio mini-halos in the cores. In particular, low-frequency observations (e.g. LOFAR) are promising. On the other hand, the steepness of the spectra makes it difficult to detect non-thermal X-ray and gamma-ray emissions from the cores. The low-energy CRs may be heating optical filaments observed in the cores.
Comments: Cosmic Rays from AGN propagate via Alfven waves (at low Mach numbers) through the intracluster medium and heat it. The paper is well structured, the only problem is the collection of plots in the end, which makes reading a bit annoying.
