Observation of high energy atmospheric neutrinos with AMANDA

Details Observation of high energy atmospheric neutrinos with AMANDA Observation of high energy atmospheric neutrinos with AMANDA

Dec 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..549..823k&link_type=abstract

INTERSECTIONS OF PARTICLE AND NUCLEAR PHYSICS: 7th Conference. AIP Conference Proceedings, Volume 549, pp. 823-827 (2000).

Other

Neutrino, Muon, Pion, And Other Elementary Particles, Cosmic Rays, Neutrino, Muon, Pion, And Other Elementary Particle Detectors, Cosmic Ray Detectors

Scientific paper

In 1997 the Antarctic Muon and Neutrino Detector Array (AMANDA) started operating with 10 strings. In an analysis of data taken during the first year of operation 188 atmospheric neutrino candidates were found. Their zenith angle distribution agrees with expectations based on Monte Carlo simulations. A preliminary upper limit is given on a diffuse flux of high energy neutrinos of astrophysical origin. .

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