Cosmic neutrino events in HiRes I detector

Details Cosmic neutrino events in HiRes I detector Cosmic neutrino events in HiRes I detector

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002phdt........20k&link_type=abstract

Thesis (PhD). THE UNIVERSITY OF UTAH, Source DAI-B 63/06, p. 2874, Dec 2002, 79 pages.

Computer Science

Scientific paper

High energy cosmic neutrino events (≥1015 eV)—deeply penetrating events in the atmosphere and upward-going events from the Earth surface—are searched for with the HiRes I detector located at Dugway Proving Grounds in Utah. The detector acceptance for the neutrino events is calculated using a Monte Carlo simulation for neutrino events in the atmosphere or below the surface of the Earth and a parton model for the neutrino cross section. The events rates in the HiRes I detector for various cosmic neutrino spectrum models, such as AGN-M95, AGN-SS91, AGN-P96, and GRB-WB, are estimated and compared with HiRes I data.

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