Characteristics of upward-going EeV Tau Neutrino Airshowers

Details Characteristics of upward-going EeV Tau Neutrino Airshowers Characteristics of upward-going EeV Tau Neutrino Airshowers

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....3.1210k&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

Scientific paper

We calculate the properties of the Cerenkov light emitted by upward-going extensive air showers (EAS) through Monte Carlo Simulation. Cerenkov light spectrum, lateral distribution, and arrival time distributions are calculated for a wide range of energies, zenith angles and atmospheric conditions, assuming observation by a satellite with a 100 km orbital height. The resulting simulations indicate that it may be feasible to detect upward-going tau neutrino showers from space with a fairly large aperture (100 km2 sr) for energies above 10 PeV.

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