Detecting Very High Energy Neutrinos by the Telescope Array

Details Detecting Very High Energy Neutrinos by the Telescope Array Detecting Very High Energy Neutrinos by the Telescope Array

2002-04-09

arxiv.org/abs/astro-ph/0204167v2

Astropart.Phys. 19 (2003) 37-46

Astronomy and Astrophysics

Astrophysics

15pages, 9 figures, 3 tables

Scientific paper

10.1016/S0927-6505(02)00191-3

We present the cosmic neutrino detecting potential of the Telescope Array for quasihorizontally downward and upward air showers initiated by very high energy neutrinos penetrating the air and the Earth respectively. We adopted model predictions for extraterrestrial neutrino fluxes from active galactic nuclei, gamma-ray bursters, Greisen photo production, the collapse of topological defects, and Z-bursts. The Telescope Array, using a large array of bright and wide field-of-view flourescence telescopes, can esplore these very high energy cosmic neutrino sources.

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