http://arxiv.org/abs/1601.04867
We will review the production of neutrinos with PeV energies and above. Discussing two possible sources of this radiation: the propagation of ultra high energy cosmic rays and the decay of super heavy dark matter. The discussion will focus on the theoretical expectations on neutrino fluxes and on the detection capabilities of present and future experiments.
R. Aloisio
Wed, 20 Jan 16
55/58
Comments: 5 pages, 4 pdf figures, contribution to the proceedings of the TAUP 2015 conference
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