Super-GZK neutrinos

Details Super-GZK neutrinos Super-GZK neutrinos

May 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006jphcs..39..393r&link_type=abstract

Journal of Physics: Conference Series, Volume 39, Issue 1, pp. 393-399 (2006).

Physics

1

Scientific paper

In the upcoming decade, observatories for cosmic neutrinos will open up a huge window in energy from 107 GeV to 1017 GeV, much above the Greisen-Zatsepin-Kuzmin (GZK) cutoff at about 4×1010 GeV, expected for cosmic protons and nuclei due to inelastic interactions with the cosmic microwave background photons. In this review, we discuss in particular the possibilities to use extremely energetic cosmic neutrinos as a diagnostic of astrophysical processes, as a tool for particle physics beyond the Standard Model, and as a probe of cosmology.

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