Extremely High Energy Neutrino Detection by the Telescope Array

Details Extremely High Energy Neutrino Detection by the Telescope Array Extremely High Energy Neutrino Detection by the Telescope Array

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....3.1255y&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

The Telescope Array detector (TA) which aims at measuring air showers in-duced by Extremely High Energy (EHE) cosmic rays by the air uorescence has also capability of detecting EHE cosmic neutrinos. The fine resolution of geometry of air showers makes it possible to identify deeply penetrating down-ward showers and upgoing showers induced by EHE neutrinos. We show the expected sensitivity for detection of cosmic neutrinos with energies beyond 10 19 eV which interact in air or rock initiating those anomalous air showers.

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