Direct Evidence for Neutrino Flavor Transformation from Neutral-Current Interactions in the Sudbury Neutrino Observatory
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Ahmad, Q R
q
Allen, R C
d
Andersen, T C
f
D Anglin, J
j
Barton, J C
k
Beier, E W
l
Bercovitch, M
j
Bigu, J
g
Biller, S D
k
Black, R A
k
Blevis, I
e
Boardman, R J
k
Boger, J
c
Bonvin, E
n
Boulay, M G
i,n
Bowler, M G
k
Bowles, T J
i
Brice, S J
i,k
Browne, M C
i,q
Bullard, T V
q
Buhler G
d
Cameron, J
k
Chan, Y D
h
Chen, H H
d
Chen, M
n
Chen, X
h,k
Cleveland, B T
k
Clifford, E T H
n
Cowan, J H M
g
Cowen, D F
l
Cox, G A
q
Dai, X
k
Dalnoki Veress, F
e
Davidson, W F
j
Doe, P J
d,i,q
Doucas, G
k
Dragowsky, M R
h,i
Duba, C A
q
Duncan, F A
n
Dunford, M
l
Dunmore, J A
k
Earle, E D
a,n
Elliott, S R
i,q
Evans, H C
n
Ewan, G T
n
Farine, J
e,g
Fergani, H
k
Ferraris, A P
k
Ford, R J
n
Formaggio, J A
q
Fowler, M M
i
Frame, K
k
Frank, E D
l
Frati, W
l
Gagnon, N
h,i,k,q
Germani, J V
q
Gil, S
b
Graham, K
n
Grant, D R
e
Hahn, R L
c
Hallin, A L
n
Hallman, E D
g
Hamer, A S
i,n
Hamian, A A
q
Handler, W B
n
Haq, R U
g
Hargrove, C K
e
Harvey, P J
n
Hazama, R
q
Heeger, K M
q
Heintzelman, W J
l
Heise, J
b,i
Helmer, R L
b,p
Hepburn, J D
n
Heron, H
k
Hewett, J
g
Hime, A
i
Howe, M
q
Hykawy, J G
g
Isaac, M C P
h
Jagam, P
f
Jelley, N A
k
Jillings, C
n
Jonkmans, G
a,g
Kazkaz, K
q
Keener, P T
l
Klein, J R
l
Knox, A B
k
Komar, R J
b
Kouzes, R
m
Kutter, T
b
Kyba, C C M
l
Law, J
f
Lawson, I T
f
Lay, M
k
Lee, H W
n
Lesko, K T
h
Leslie, J R
n
Levine, I
e
Locke, W
k
Luoma, S
g
Lyon, J
k
Majerus, S
k
Mak, H B
n
Maneira, J
n
Manor, J
q
Marino, A D
h
McCauley, N
k,l
McDonald, A B
m,n
McDonald, D S
l
McFarlane, K
e
McGregor, G
k
Meijer Drees, R
q
Mifflin, C
e
Miller, G G
i
Milton, G
a
Moffat, B A
n
Moorhead, M
k
Nally, C W
b
Neubauer, M S
l
Newcomer, F M
l
Ng, H S
b
Noble, A J
e,p
Norman, E B
h
Novikov, V M
e
O'Neill, M
e
Okada, C E
h
Ollerhead, R W
f
Omori, M
k
Orrell, J L
q
Oser, S M
l
Poon, A W P
b,h,i,q
Radcliffe, T J
n
Roberge, A
g
Robertson, B C
n
Robertson, R G H
i,q
Rosendahl, S S E
h
Rowley, J K
c
Rusu, V L
l
Saettler, E
g
Schaffer, K K
q
Schwendener, M H
g
Schulke A
h
Seifert, H
g,i,q
Shatkay, M
e
Simpson, J J
f
Sims, C J
k
Sinclair, D
e,p
Skensved, P
n
Smith, A R
h
Smith, M W E
q
Spreitzer, T
l
Starinsky, N
e
Steiger, T D
q
Stokstad, R G
h
Stonehill, L C
q
Storey, R S
j
Sur, B
a,n
Tafirout, R
g
Tagg, N
f,k
Tanner, N W
k
Taplin, R K
k
Thorman, M
k
Thornewell, P M
k
Trent, P T
k
Tserkovnyak, Y I
b
Van Berg, R
l
Van de Water, R G
i,l
Virtue, C J
g
Waltham, C E
b
Wang, J X
f
Wark, D L
i,k,o
West, N
k
Wilhelmy, J B
i
Wilkerson, J F
i,q
Wilson, J R
k
Wittich, P
l
Wouters, J M
i
Yeh, M
c
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0027592333
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M.-Q. Liu, H. W. Lee, and A. B. McDonald, Nucl. Instrum. Methods Phys. Res., Sect. A 329, 291 (1993).
-
(1993)
Nucl. Instrum. Methods Phys. Res., Sect. A
, vol.329
, pp. 291
-
-
Liu, M.-Q.1
Lee, H.W.2
McDonald, A.B.3
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0002026307
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We note that this rate of neutron events also leads to a lower bound on the proton lifetime for “invisible” modes based on the free neutron that would be left in deuterium [V. I. Tretyak and Yu. G. Zdesenko, Phys. Lett. B 505, 59 (2001)]
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(2001)
Phys. Lett. B
, vol.505
, pp. 59
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Tretyak, V.I.1
Zdesenko, Y.G.2
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33646635124
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The possible contribution of this mechanism to the solar neutrino NC background is ignored
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in excess of (Formula presented) years, approximately 3 orders of magnitude more restrictive than previous limits [J. Evans and R. Steinberg, Science 197, 989 (1977)]. The possible contribution of this mechanism to the solar neutrino NC background is ignored.
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(1977)
Science
, vol.197
, pp. 989
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Evans, J.1
Steinberg, R.2
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Cross section uncertainty includes (Formula presented) uncertainty (Formula presented), difference between NSGK [S. Nakamura, T. Sato, V. Gudkov, and K. Kubodera, Phys. Rev. C 63, 034617 (2001)]
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(2001)
Phys. Rev. C
, vol.63
, pp. 34617
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Nakamura, S.1
Sato, T.2
Gudkov, V.3
Kubodera, K.4
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in SNO's calculations (Formula presented), radiative correction uncertainties [ (Formula presented) for CC, (Formula presented) for NC; A. Kurylov, M. J. Ramsey-Musolf, and P. Vogel, Phys. Rev. C 65, 055501 (2002)]
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(2002)
Phys. Rev. C
, vol.65
, pp. 55501
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Kurylov, A.1
Ramsey-Musolf, M.J.2
Vogel, P.3
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85038323882
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arXiv:nucl-th/0201062
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uncertainty associated with neglect of real photons in SNO ( (Formula presented) for CC), and theoretical cross section uncertainty [ (Formula presented), S. Nakamura, arXiv:nucl-th/0201062 (to be published)].
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Nakamura, S.1
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85038273415
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This change of variables allows a direct test of the null hypothesis of no flavor transformation (Formula presented) without requiring calculation of the CC, ES, and NC signal correlations
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This change of variables allows a direct test of the null hypothesis of no flavor transformation (Formula presented) without requiring calculation of the CC, ES, and NC signal correlations.
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