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Exact solutions of the perturbations equations in the magnetized LambdaCDM scenario are presented. They apply during the dark ages and, more specifically, after the baryons are freed from the drag of ...
IceCube as a three-dimensional air-shower array covers an energy range of the cosmic-ray spectrum from below 1 PeV to approximately 1 EeV. This talk is a brief review of the function and goals of IceT...
Shocks that arise from baryonic in-fall and merger events during the structure formation are believed to be a source of cosmic rays. These "struc- ture formation cosmic rays" (SFCRs) would essential...

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