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Measurement of the total active 8B solar neutrino flux at the Sudbury Neutrino Observatory with enhanced neutral current sensitivity.

Authors :
Ahmed SN
Anthony AE
Beier EW
Bellerive A
Biller SD
Boger J
Boulay MG
Bowler MG
Bowles TJ
Brice SJ
Bullard TV
Chan YD
Chen M
Chen X
Cleveland BT
Cox GA
Dai X
Dalnoki-Veress F
Doe PJ
Dosanjh RS
Doucas G
Dragowsky MR
Duba CA
Duncan FA
Dunford M
Dunmore JA
Earle ED
Elliott SR
Evans HC
Ewan GT
Farine J
Fergani H
Fleurot F
Formaggio JA
Fowler MM
Frame K
Fulsom BG
Gagnon N
Graham K
Grant DR
Hahn RL
Hall JC
Hallin AL
Hallman ED
Hamer AS
Handler WB
Hargrove CK
Harvey PJ
Hazama R
Heeger KM
Heintzelman WJ
Heise J
Helmer RL
Hemingway RJ
Hime A
Howe MA
Jagam P
Jelley NA
Klein JR
Kos MS
Krumins AV
Kutter T
Kyba CC
Labranche H
Lange R
Law J
Lawson IT
Lesko KT
Leslie JR
Levine I
Luoma S
MacLellan R
Majerus S
Mak HB
Maneira J
Marino AD
McCauley N
McDonald AB
McGee S
McGregor G
Mifflin C
Miknaitis KK
Miller GG
Moffat BA
Nally CW
Nickel BG
Noble AJ
Norman EB
Oblath NS
Okada CE
Ollerhead RW
Orrell JL
Oser SM
Ouellet C
Peeters SJ
Poon AW
Robertson BC
Robertson RG
Rollin E
Rosendahl SS
Rusu VL
Schwendener MH
Simard O
Simpson JJ
Sims CJ
Sinclair D
Skensved P
Smith MW
Starinsky N
Stokstad RG
Stonehill LC
Tafirout R
Takeuchi Y
Tesić G
Thomson M
Thorman M
Van Berg R
Van de Water RG
Virtue CJ
Wall BL
Waller D
Waltham CE
Tseung HW
Wark DL
West N
Wilhelmy JB
Wilkerson JF
Wilson JR
Wouters JM
Yeh M
Zuber K
Source :
Physical review letters [Phys Rev Lett] 2004 May 07; Vol. 92 (18), pp. 181301. Date of Electronic Publication: 2004 May 03.
Publication Year :
2004

Abstract

The Sudbury Neutrino Observatory has precisely determined the total active (nu(x)) 8B 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) x 10(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(+1.2)(-0.6) x 10(-5) eV(2) and theta=32.5(+2.4)(-2.3) degrees. Maximal mixing is rejected at the equivalent of 5.4 standard deviations.

Details

Language :
English
ISSN :
0031-9007
Volume :
92
Issue :
18
Database :
MEDLINE
Journal :
Physical review letters
Publication Type :
Academic Journal
Accession number :
15169480
Full Text :
https://doi.org/10.1103/PhysRevLett.92.181301