Tracing Very High Energy Tau Neutrinos from Cosmological Sources in Ice

Details Tracing Very High Energy Tau Neutrinos from Cosmological Sources in Ice Tracing Very High Energy Tau Neutrinos from Cosmological Sources in Ice

Jan 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004lbeh.conf..298j&link_type=abstract

THE LAUNCHING OF LA BELLE EPOQUE OF HIGH ENERGY PHYSICS AND COSMOLOGY A Festschrift for Paul Frampton in His 60th Year and Memor

Physics

High Energy Physics

Scientific paper

Astrophysical sources of ultrahigh energy neutrinos yield tau neutrino fluxes due to neutrino oscillations. We study in detail the contribution of tau neutrinos with energies above 106 GeV relative to the contribution of the other flavors. We consider several different initial neutrino fluxes and include tau neutrino regeneration in transit through the Earth and energy loss of charged leptons. We discuss signals of tau neutrinos in detectors such as IceCube, RICE and ANITA.

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