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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Main Author: Formaggio, Joseph A
Other Authors: Massachusetts Institute of Technology. Department of Physics
Format: Article
Language:en_US
Published: Elsevier B.V. 2009
Online Access:http://hdl.handle.net/1721.1/49855
https://orcid.org/0000-0002-3757-9883
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author Formaggio, Joseph A
author2 Massachusetts Institute of Technology. Department of Physics
author_facet Massachusetts Institute of Technology. Department of Physics
Formaggio, Joseph A
author_sort Formaggio, Joseph A
collection MIT
description 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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spelling mit-1721.1/498552023-02-26T08:01:41Z Measurement of Atmospheric Neutrinos at the Sudbury Neutrino Observatory Formaggio, Joseph A Massachusetts Institute of Technology. Department of Physics Massachusetts Institute of Technology. Laboratory for Nuclear Science Formaggio, Joseph A Formaggio, Joseph A. 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. 2009-11-25T16:21:11Z 2009-11-25T16:21:11Z 2009-07 Article http://purl.org/eprint/type/SubmittedJournalArticle 0375-9474 http://hdl.handle.net/1721.1/49855 Formaggio, J.A. “Measurement of Atmospheric Neutrinos at the Sudbury Neutrino Observatory.” Nuclear Physics A 827.1-4 (2009): 498c-500c. https://orcid.org/0000-0002-3757-9883 en_US http://dx.doi.org/10.1016/j.nuclphysa.2009.05.143 Nuclear Physics A Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. application/pdf Elsevier B.V. Joseph A. Formaggio
spellingShingle Formaggio, Joseph A
Measurement of Atmospheric Neutrinos at the Sudbury Neutrino Observatory
title Measurement of Atmospheric Neutrinos at the Sudbury Neutrino Observatory
title_full Measurement of Atmospheric Neutrinos at the Sudbury Neutrino Observatory
title_fullStr Measurement of Atmospheric Neutrinos at the Sudbury Neutrino Observatory
title_full_unstemmed Measurement of Atmospheric Neutrinos at the Sudbury Neutrino Observatory
title_short Measurement of Atmospheric Neutrinos at the Sudbury Neutrino Observatory
title_sort measurement of atmospheric neutrinos at the sudbury neutrino observatory
url http://hdl.handle.net/1721.1/49855
https://orcid.org/0000-0002-3757-9883
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