Ultrahigh Energy Neutrinos

Details Ultrahigh Energy Neutrinos Ultrahigh Energy Neutrinos

2003-02-19

arxiv.org/abs/hep-ph/0302178v1

Int.J.Mod.Phys. A18 (2003) 4085-4096

Physics

High Energy Physics

High Energy Physics - Phenomenology

7 pages, presented at Neutrinos and Implications for Physics Beyond the Standard Model, Stony Brook, NY, October 11-13, 2002

Scientific paper

10.1142/S0217751X03017385

The ultrahigh energy neutrino cross section is well understood in the standard model for neutrino energies up to 10$^{12}$ GeV. Test of neutrino oscillations ($\nu_\mu\leftrightarrow\nu_\tau$) from extragalactic sources of neutrinos are possible with large underground detectors. Measurments of horizontal air shower event rates at neutrino energies above 10$^{10}$ GeV will be able to constrain nonstandard model contributions to the neutrino-nucleon cross section, e.g., from mini-black hole production.

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