Measurement of the rate of ve + d → p + p + e- interactions produced by 8B solar neutrinos at the sudbury neutrino observatory

The 8B flux from elastic scattering (ES) and charged current (CC) of electrons was recorded at the Sudbury Neutrino Observatory (SNO) between November 2, 1999 and January 15, 2001. Data were partitioned into two sets then analyzed. As a result, the first direct indication of a nonelectron flavor com...

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Príomhchruthaitheoirí: Ahmad, Q, Allen, R, Andersen, T, Anglin, J, Bühler, G, Barton, J, Beier, E, Bercovitch, M, Bigu, J, Biller, S, Black, R, Blevis, I, Bardman, R, Boger, J, Bonvin, E, Boulay, MG, Bowler, MG, Bowles, T, Brice, S, Browne, M, Bullard, T, Burritt, T, Cameron, K, Cameron, J, Chan, Y
Formáid: Journal article
Teanga:English
Foilsithe / Cruthaithe: 2001
_version_ 1826296993781121024
author Ahmad, Q
Allen, R
Andersen, T
Anglin, J
Bühler, G
Barton, J
Beier, E
Bercovitch, M
Bigu, J
Biller, S
Black, R
Blevis, I
Bardman, R
Boger, J
Bonvin, E
Boulay, MG
Bowler, MG
Bowles, T
Brice, S
Browne, M
Bullard, T
Burritt, T
Cameron, K
Cameron, J
Chan, Y
author_facet Ahmad, Q
Allen, R
Andersen, T
Anglin, J
Bühler, G
Barton, J
Beier, E
Bercovitch, M
Bigu, J
Biller, S
Black, R
Blevis, I
Bardman, R
Boger, J
Bonvin, E
Boulay, MG
Bowler, MG
Bowles, T
Brice, S
Browne, M
Bullard, T
Burritt, T
Cameron, K
Cameron, J
Chan, Y
author_sort Ahmad, Q
collection OXFORD
description The 8B flux from elastic scattering (ES) and charged current (CC) of electrons was recorded at the Sudbury Neutrino Observatory (SNO) between November 2, 1999 and January 15, 2001. Data were partitioned into two sets then analyzed. As a result, the first direct indication of a nonelectron flavor component in the solar neutrino flux was established.
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spelling oxford-uuid:cc455c4a-e6bd-45cf-8396-42e530f8b2a62022-03-27T07:20:44ZMeasurement of the rate of ve + d → p + p + e- interactions produced by 8B solar neutrinos at the sudbury neutrino observatoryJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:cc455c4a-e6bd-45cf-8396-42e530f8b2a6EnglishSymplectic Elements at Oxford2001Ahmad, QAllen, RAndersen, TAnglin, JBühler, GBarton, JBeier, EBercovitch, MBigu, JBiller, SBlack, RBlevis, IBardman, RBoger, JBonvin, EBoulay, MGBowler, MGBowles, TBrice, SBrowne, MBullard, TBurritt, TCameron, KCameron, JChan, YThe 8B flux from elastic scattering (ES) and charged current (CC) of electrons was recorded at the Sudbury Neutrino Observatory (SNO) between November 2, 1999 and January 15, 2001. Data were partitioned into two sets then analyzed. As a result, the first direct indication of a nonelectron flavor component in the solar neutrino flux was established.
spellingShingle Ahmad, Q
Allen, R
Andersen, T
Anglin, J
Bühler, G
Barton, J
Beier, E
Bercovitch, M
Bigu, J
Biller, S
Black, R
Blevis, I
Bardman, R
Boger, J
Bonvin, E
Boulay, MG
Bowler, MG
Bowles, T
Brice, S
Browne, M
Bullard, T
Burritt, T
Cameron, K
Cameron, J
Chan, Y
Measurement of the rate of ve + d → p + p + e- interactions produced by 8B solar neutrinos at the sudbury neutrino observatory
title Measurement of the rate of ve + d → p + p + e- interactions produced by 8B solar neutrinos at the sudbury neutrino observatory
title_full Measurement of the rate of ve + d → p + p + e- interactions produced by 8B solar neutrinos at the sudbury neutrino observatory
title_fullStr Measurement of the rate of ve + d → p + p + e- interactions produced by 8B solar neutrinos at the sudbury neutrino observatory
title_full_unstemmed Measurement of the rate of ve + d → p + p + e- interactions produced by 8B solar neutrinos at the sudbury neutrino observatory
title_short Measurement of the rate of ve + d → p + p + e- interactions produced by 8B solar neutrinos at the sudbury neutrino observatory
title_sort measurement of the rate of ve d p p e interactions produced by 8b solar neutrinos at the sudbury neutrino observatory
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