Measurement of the total active8B solar neutrino flux at the Sudbury Neutrino Observatory with enhanced neutral current sensitivity
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Ahmed, S N
j
Anthony, A E
o
Beier, E W
i
Bellerive, A
c
Biller, S D
h
Boger, J
b
Boulay, M G
g
Bowler, M G
h
Bowles, T J
g
Brice, S J
g
Bullard, T V
n
Chan, Y D
f
Chen, M
j
Chen, X
f
Cleveland, B T
h
Cox, G A
n
Dai, X
c,h
Dalnoki Veress, F
c
Doe, P J
n
Dosanjh, R S
c
Doucas, G
h
Dragowsky, M R
g
Duba, C A
n
Duncan, F A
j
Dunford, M
i
Dunmore, J A
h
Earle, E D
j
Elliott, S R
g
Evans, H C
j
Ewan, G T
j
Farine, J
c,e
Fergani, H
h
Fleurot, F
e
Formaggio, J A
n
Fowler, M M
g
Frame, K
c,h
Fulsom, B G
j
Gagnon, N
f,g,h,n
Graham, K
j
Grant, D R
c
Hahn, R L
b
Hall, J C
o
Hallin, A L
j
Hallman, E D
e
Hamer, A S
g
Handler, W B
j
Hargrove, C K
c
Harvey, P J
j
Hazama, R
n
Heeger, K M
f
Heintzelman, W J
i
Heise, J
g
Helmer, R L
a,m
Hemingway, R J
c
Hime, A
g
Howe, M A
n
Jagam, P
d
Jelley, N A
h
Klein, J R
i,o
Kos, M S
j
Krumins, A V
j
Kutter, T
a
Kyba, C C M
i
Labranche, H
d
Lange, R
b
Law, J
d
Lawson, I T
d
Lesko, K T
f
Leslie, J R
j
Levine, I
c,p
Luoma, S
e
MacLellan, R
j
Majerus, S
h
Mak, H B
j
Maneira, J
j
Marino, A D
f
McCauley, N
i
McDonald, A B
j
McGee, S
n
McGregor, G
h
Mifflin, C
c
Miknaitis, K K S
n
Miller, G G
g
Moffat, B A
j
Nally, C W
a
Nickel, B G
d
Noble, A J
c,j,m
Norman, E B
f
Oblath, N S
n
Okada, C E
f
Ollerhead, R W
d
Orrell, J L
n
Oser, S M
a,i
Ouellet, C
j
Peeters, S J M
h
Poon, A W P
f
Robertson, B C
j
Robertson, R G H
n
Rollin, E
c
Rosendahl, S S E
f
Rusu, V L
i
Schwendener, M H
e
Simard, O
c
Simpson, J J
d
Sims, C J
h
Sinclair, D
c,m
Skensved, P
j
Smith, M W E
n
Starinsky, N
c
Stokstad, R G
f
Stonehill, L C
n
Tafirout, R
e
Takeuchi, Y
j
Tesic G
c
Thomson, M
j
Thorman, M
h
van Berg, R
i
van de Water, R G
g
Virtue, C J
e
Wall, B L
n
Waller, D
c
Waltham, C E
a
Wan Chan Tseung, H
h
Wark, D L
k,l
West, N
h
Wilhelmy, J B
g
Wilkerson, J F
n
Wilson, J R
h
Wouters, J M
g
Yeh, M
b
Zuber, K
h
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SNO Collaboration, Q. R. Ahmad et al., Phys. Rev. Lett. 87, 071301 (2001).
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Ahmad, Q.R.1
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2942689121
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note
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ij the angle between hits i and j from the event position and N the number of hits.
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2942665353
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A small correction to EGS4 was made to allow for the neglect of the Mott terms in the electron scattering cross section and other approximations in the treatment of multiple scattering. We thank D.W. O. Rogers for providing EGSnrc simulations.
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SNO Collaboration, Phys. Rev. Lett. 89, 011302 (2002).
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0037048001
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A (0.5%), theoretical cross section (1% for CC and NC, 0.3% for CC/NC), S. Nakamura et al. Nucl. Phys. A707, 561 (2002 ) , and radiative corrections (0.3% for CC, 0.1% for NC), A. Kurylov, M. J. Ramsey-Musolf, and P. Vogel, Phys. Rev. C 65, 055501 (2002).
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Nakamura, S.1
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4243487078
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A (0.5%), theoretical cross section (1% for CC and NC, 0.3% for CC/NC), S. Nakamura et al. Nucl. Phys. A707, 561 (2002 ) , and radiative corrections (0.3% for CC, 0.1% for NC), A. Kurylov, M. J. Ramsey-Musolf, and P. Vogel, Phys. Rev. C 65, 055501 (2002).
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Phys. Rev. C
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Kurylov, A.1
Ramsey-Musolf, M.J.2
Vogel, P.3
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2942676376
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hep neutrinos could also be present in the measured fluxes; the SSM contribution would be 0.5%
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hep neutrinos could also be present in the measured fluxes; the SSM contribution would be 0.5%.
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0000163416
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Electron neutrino cross sections are used to calculate all fluxes. The ES cross section is from J. N. Bahcall et al., Phys. Rev. D 51, 6146 (1995).
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Phys. Rev. D
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Bahcall, J.N.1
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note
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A hypothesis test similar to [3] disfavors no flavor transformation at greater than the equivalent of 7σ
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0000883579
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Z. Maki, N. Nakagawa, and S. Sakata, Prog. Theor. Phys. 28, 870 (1962); V. Gribov and B. Pontecorvo, Phys. Lett B 28, 493 (1969): S.P. Mikheyev and A.Yu. Smirnov, Sov. J. Nucl. Phys. 42, 913 (1985) ; L. Wolfenstein, Phys. Rev. D 17, 2369 (1978).
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33744534117
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Z. Maki, N. Nakagawa, and S. Sakata, Prog. Theor. Phys. 28, 870 (1962); V. Gribov and B. Pontecorvo, Phys. Lett B 28, 493 (1969): S.P. Mikheyev and A.Yu. Smirnov, Sov. J. Nucl. Phys. 42, 913 (1985) ; L. Wolfenstein, Phys. Rev. D 17, 2369 (1978).
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Gribov, V.1
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Z. Maki, N. Nakagawa, and S. Sakata, Prog. Theor. Phys. 28, 870 (1962); V. Gribov and B. Pontecorvo, Phys. Lett B 28, 493 (1969): S.P. Mikheyev and A.Yu. Smirnov, Sov. J. Nucl. Phys. 42, 913 (1985) ; L. Wolfenstein, Phys. Rev. D 17, 2369 (1978).
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Mikheyev, S.P.1
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Z. Maki, N. Nakagawa, and S. Sakata, Prog. Theor. Phys. 28, 870 (1962); V. Gribov and B. Pontecorvo, Phys. Lett B 28, 493 (1969): S.P. Mikheyev and A.Yu. Smirnov, Sov. J. Nucl. Phys. 42, 913 (1985) ; L. Wolfenstein, Phys. Rev. D 17, 2369 (1978).
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T. Kirsten, in Proceedings of the XXth International Conference on Neutrino Physics and Astrophysics, Munich, 2002 [Nucl. Phys. B, Proc. Suppl. 118, 33 (2003)].
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See the SNO website, http://sno.phy.queensu.ca, for details.
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SNO Website
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