Measurement of Atmospheric Neutrinos at the Sudbury Neutrino Observatory

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 experime...

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Bibliografiska uppgifter
Huvudupphovsman: Formaggio, Joseph A
Övriga upphovsmän: Massachusetts Institute of Technology. Department of Physics
Materialtyp: Artikel
Språk:en_US
Publicerad: Elsevier B.V. 2009
Länkar:http://hdl.handle.net/1721.1/49855
https://orcid.org/0000-0002-3757-9883