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Measurement of the Total ActiveB8Solar Neutrino Flux at the Sudbury Neutrino Observatory with Enhanced Neutral Current Sensitivity

Authors :
R. L. Helmer
P. J. Doe
R. L. Hahn
Monica Dunford
A. W. P. Poon
R. MacLellan
S. R. Elliott
R. W. Ollerhead
E. D. Hallman
G. T. Ewan
J. Maneira
I. T. Lawson
W. B. Handler
Y. Takeuchi
J. F. Wilkerson
J. Boger
J. J. Simpson
D. Waller
Reda Tafirout
Darren Grant
Christopher C. M. Kyba
Yuen-Dat Chan
B. L. Wall
C. K. Hargrove
P. Skensved
C. E. Okada
David A. Sinclair
G. A. Cox
Eric B. Norman
F. A. Duncan
R. S. Dosanjh
B. A. Moffat
K. Graham
E. Rollin
J. R. Leslie
M. W.E. Smith
B. T. Cleveland
J. M. Wouters
R. G. Stokstad
Chris Waltham
M. A. Howe
Malcolm M. Fowler
C. Ouellet
S. M. Oser
H. Fergani
Guthrie Miller
J. A. Dunmore
J. Farine
A. J. Noble
X. Chen
X. Dai
G. Tešić
N. West
A. V. Krumins
R. Lange
S. J. M. Peeters
V. L. Rusu
K.K.S. Miknaitis
W. J. Heintzelman
M.G. Boulay
S. J. Brice
A. S. Hamer
K. T. Lesko
G. McGregor
A. L. Hallin
J. R. Wilson
C. Mifflin
T. V. Bullard
R. J. Hemingway
S. McGee
M. Kos
E. D. Earle
S. D. Biller
Bernie G. Nickel
H. Wan Chan Tseung
I. Levine
N. S. Oblath
E. W. Beier
C. A. Duba
H. Labranche
A. B. McDonald
D. L. Wark
M. R. Dragowsky
F. Dalnoki-Veress
M. H. Schwendener
M. G. Bowler
A. D. Marino
B. G. Fulsom
J. C. Hall
J. Law
R. G. H. Robertson
C. J. Sims
Kai Zuber
C. W. Nally
Andrew Hime
B. C. Robertson
G. Doucas
J. B. Wilhelmy
T. Kutter
C. J. Virtue
N. Gagnon
John L. Orrell
L. C. Stonehill
S. N. Ahmed
R. Hazama
T. J. Bowles
Joseph A. Formaggio
N. McCauley
Minfang Yeh
N. A. Jelley
M. Thorman
R. Van Berg
O. Simard
Hal Evans
K. Frame
Alain Bellerive
K. M. Heeger
M. L. Chen
M. A. Thomson
J. Heise
F. Fleurot
A. E. Anthony
S. Luoma
P. Jagam
Joshua R. Klein
R. G. Van de Water
N. Starinsky
H. B. Mak
S. S.E. Rosendahl
P. J. Harvey
S. Majerus
Source :
Physical Review Letters. 92
Publication Year :
2004
Publisher :
American Physical Society (APS), 2004.

Abstract

The Sudbury Neutrino Observatory has precisely determined the total active (nu(x)) B-8 solar neutrino flux without assumptions about the energy dependence of the nu(e) survival probability. The measurements were made with dissolved NaCl in heavy water to enhance the sensitivity and signature for neutral-current interactions. The flux is found to be 5.21+/-0.27(stat)+/-0.38(syst)x10(6) cm(-2) s(-1), in agreement with previous measurements and standard solar models. A global analysis of these and other solar and reactor neutrino results yields Deltam(2)=7.1(-0.6)(+1.2)x10(-5) eV(2) and theta= 32.5(-2.3)(+2.4) degrees. Maximal mixing is rejected at the equivalent of 5.4 standard deviations.

Details

ISSN :
10797114 and 00319007
Volume :
92
Database :
OpenAIRE
Journal :
Physical Review Letters
Accession number :
edsair.doi...........d5363f907634e6f3fe75310597220384
Full Text :
https://doi.org/10.1103/physrevlett.92.181301