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Observation of high energy atmospheric neutrinos with AMANDA
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2000 (English)In: AIP Conference Proceedings, American Institute of Physics (AIP), 2000, no 549, 823-827 p.Conference paper, Published paper (Refereed)
Abstract [en]

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.

Place, publisher, year, edition, pages
American Institute of Physics (AIP), 2000. no 549, 823-827 p.
Keyword [en]
cosmic ray apparatus, cosmic ray neutrinos, Monte Carlo methods, neutrino detection
National Category
Physical Sciences
Research subject
Physics, Astroparticle Physics
Identifiers
URN: urn:nbn:se:lnu:diva-29486OAI: oai:DiVA.org:lnu-29486DiVA: diva2:654070
Conference
7th Conference on the Intersection of Particles and Nuclear Physics. Quebec City, Que., Canada, 22-28 May 2000
Available from: 2013-10-07 Created: 2013-10-07 Last updated: 2013-10-09Bibliographically approved

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Carius, Staffan

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