Measurement of Atmospheric Neutrinos at the Sudbury Neutrino Observatory

Details Measurement of Atmospheric Neutrinos at the Sudbury Neutrino Observatory Measurement of Atmospheric Neutrinos at the Sudbury Neutrino Observatory

Aug 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009nupha.827..498s&link_type=abstract

Nuclear Physics A, Volume 827, Issue 1-4, p. 498-500c.

Physics

Nuclear Physics

Ordinary Neutrinos (Nuw Bosons, Cosmic Rays, Neutrino Mass And Mixing

Scientific paper

The Sudbury Neutrino Observatory consists of a 1 kiloton heavy water Cherenkov detector able to detect and reconstruct high-energy muons created from cosmic ray showers and atmospheric neutrino interactions. By measuring the flux of through-going muons as a function of zenith angle, the SNO experiment can distinguish between the oscillated and un-oscillated portion of the neutrino flux. This report describes SNO's measurements of the flux of cosmic ray muons and neutrino-induced muon flux at a depth of 5890 meters water equivalent.

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