Abstract:Dark Matter annihilation is a possible source of relativistic electrons in galaxy clusters; these electrons, interacting with intra-cluster magnetic fields, can contribute to the diffuse radio emission observed in several clusters. We explore the possibility that Dark Matter annihilation can be at the origin of the radio emission in the cluster A520. We find that, if a radio emission of Dark Matter origin is present in this cluster, it can be observed in a region in the NE part of the cluster, whereas we expec… Show more
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