Physics
Scientific paper
Aug 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....3.1142y&link_type=abstract
Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int
Physics
6
Scientific paper
We have made a systematic search for air shower events induced possibly by Ultra-high Energy (UHE) cosmic neutrinos by the Akeno Giant Air Shower Array. The lateral distribution of secondary shower particle densities and their shower front curvature are found to be closely related to atmospheric depth of the shower maximum which makes it possible to discriminate anomaly penetrating air shower events from the regular hadron induced air showers. The present analysis has indicated no significant enhancement on intensity of deeply penetrating air showers within the detector resolution. The resultant upper bound on UHE νe flux with energies greater than 3 × 1017 eV is 5.7 × 10-10 m-2 sec-1 sr-1 for J(E)˜ E-2 with 95 % C.L.
Chikawa Michiyuki
Fukushima Masatoshi
Hayashida Naokai
Honda Katsuya
Inoue Naoya
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