BEXCO - Room F(201/202/203/204)
[CRD026] Acceleration and Evolution of Cosmic Ray Electrons During Radio-Galaxy-Cluster-Shock Encounters
Radio Galaxies (radio-loud AGNs) are common in galaxy cluster media (ICMs). In addition to their potential thermodynamical roles, these AGN may also serve to illuminate important ICM dynamical features, especially ICM shocks. Those interactions are revealed most clearly by radio synchrotron emissions from associated AGN Cosmic Ray Electrons (CRe). Here we report results from "MHD+CR" simulations of AGN-shock encounters and specifically on resultant shock acceleration (DSA) of the CRe and observable consequences. We find, in particular, that even modest-strength ICM shocks (M_s ~ 3-4) may lead to significant and observable DSA of the AGn CRe. This work has impact on both the nature of large scale cluster radio emissions, including so-called radio relics and our understanding of AGN-ICM-shock dynamics.