Combined analysis of all three phases of solar neutrino data from the Sudbury Neutrino Observatory

B. Aharmim; S. N. Ahmed; A. E. Anthony; N. Barros; E. W. Beier; A. Bellerive; B. Beltran; M. Bergevin; S. D. Biller; K. Boudjemline; M. G. Boulay; B. Cai; Y. D. Chan; D. Chauhan; M. Chen; B. T. Cleveland; G. A. Cox; X. Dai; H. Deng; J. A. Detwiler; M. Dimarco; P. J. Doe; G. Doucas; P. L. Drouin; F. A. Duncan; M. Dunford; E. D. Earle; S. R. Elliott; H. C. Evans; G. T. Ewan; J. Farine; H. Fergani; F. Fleurot; R. J. Ford; J. A. Formaggio; N. Gagnon; J. Tm Goon; K. Graham; E. Guillian; S. Habib; R. L. Hahn; A. L. Hallin; E. D. Hallman; P. J. Harvey; R. Hazama; W. J. Heintzelman; J. Heise; R. L. Helmer; A. Hime; C. Howard; M. Huang; P. Jagam; B. Jamieson; N. A. Jelley; M. Jerkins; K. J. Keeter; J. R. Klein; L. L. Kormos; M. Kos; C. Kraus; C. B. Krauss; A. Kruger; T. Kutter; C. C.M. Kyba; R. Lange; J. Law; I. T. Lawson; K. T. Lesko; J. R. Leslie; J. C. Loach; R. Maclellan; S. Majerus; H. B. Mak; J. Maneira; R. Martin; N. McCauley; A. B. McDonald; S. R. McGee; M. L. Miller; B. Monreal; J. Monroe; B. G. Nickel; A. J. Noble; H. M. O'Keeffe; N. S. Oblath; R. W. Ollerhead; G. D. Orebi Gann; S. M. Oser; R. A. Ott; S. J.M. Peeters; A. W.P. Poon; G. Prior; S. D. Reitzner; K. Rielage; B. C. Robertson; R. G.H. Robertson; R. C. Rosten; M. H. Schwendener; J. A. Secrest; S. R. Seibert; O. Simard; J. J. Simpson; P. Skensved; T. J. Sonley; L. C. Stonehill; G. Tešić; N. Tolich; T. Tsui; R. Van Berg; B. A. Vandevender; C. J. Virtue; H. Wan Chan Tseung; D. L. Wark; P. J.S. Watson; J. Wendland; N. West; J. F. Wilkerson; J. R. Wilson; J. M. Wouters; A. Wright; M. Yeh; F. Zhang; K. Zuber

doi:10.1103/PhysRevC.88.025501

Combined analysis of all three phases of solar neutrino data from the Sudbury Neutrino Observatory

B. Aharmim, S. N. Ahmed, A. E. Anthony, N. Barros, E. W. Beier, A. Bellerive, B. Beltran, M. Bergevin, S. D. Biller, K. Boudjemline, M. G. Boulay, B. Cai, Y. D. Chan, D. Chauhan, M. Chen, B. T. Cleveland, G. A. Cox, X. Dai, H. Deng, J. A. DetwilerM. Dimarco, P. J. Doe, G. Doucas, P. L. Drouin, F. A. Duncan, M. Dunford, E. D. Earle, S. R. Elliott, H. C. Evans, G. T. Ewan, J. Farine, H. Fergani, F. Fleurot, R. J. Ford, J. A. Formaggio, N. Gagnon, J. Tm Goon, K. Graham, E. Guillian, S. Habib, R. L. Hahn, A. L. Hallin, E. D. Hallman, P. J. Harvey, R. Hazama, W. J. Heintzelman, J. Heise, R. L. Helmer, A. Hime, C. Howard, M. Huang, P. Jagam, B. Jamieson, N. A. Jelley, M. Jerkins, K. J. Keeter, J. R. Klein, L. L. Kormos, M. Kos, C. Kraus, C. B. Krauss, A. Kruger, T. Kutter, C. C.M. Kyba, R. Lange, J. Law, I. T. Lawson, K. T. Lesko, J. R. Leslie, J. C. Loach, R. Maclellan, S. Majerus, H. B. Mak, J. Maneira, R. Martin, N. McCauley, A. B. McDonald, S. R. McGee, M. L. Miller, B. Monreal, J. Monroe, B. G. Nickel, A. J. Noble, H. M. O'Keeffe, N. S. Oblath, R. W. Ollerhead, G. D. Orebi Gann, S. M. Oser, R. A. Ott, S. J.M. Peeters, A. W.P. Poon, G. Prior, S. D. Reitzner, K. Rielage, B. C. Robertson, R. G.H. Robertson, R. C. Rosten, M. H. Schwendener, J. A. Secrest, S. R. Seibert, O. Simard, J. J. Simpson, P. Skensved, T. J. Sonley, L. C. Stonehill, G. Tešić, N. Tolich, T. Tsui, R. Van Berg, B. A. Vandevender, C. J. Virtue, H. Wan Chan Tseung, D. L. Wark, P. J.S. Watson, J. Wendland, N. West, J. F. Wilkerson, J. R. Wilson, J. M. Wouters, A. Wright, M. Yeh, F. Zhang, K. Zuber

Biochemistry, Chemistry, & Physics

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Abstract

We report results from a combined analysis of solar neutrino data from all phases of the Sudbury Neutrino Observatory (SNO). By exploiting particle identification information obtained from the proportional counters installed during the third phase, this analysis improved background rejection in that phase of the experiment. The combined analysis of the SNO data resulted in a total flux of active neutrino flavors from 8B decays in the Sun of (5.25±0.16(stat.)-0.13+0.11(syst.))×106cm^-2s ^-1, while a two-flavor neutrino oscillation analysis yielded Δm212=(5.6-1.4+1.9)×10^-5eV2 and tan2θ₁₂= 0.427-0.029+0.033. A three-flavor neutrino oscillation analysis combining the SNO result with results of all other solar neutrino experiments and reactor neutrino experiments yielded Δm212=(7.46-0.19+0.20)×10 ^-5eV2, tan2θ₁₂=0.443-0.025+0.030, and sin2θ₁₃=(2.49-0.32+0.20)×10^-2.

Original language	English
Article number	025501
Journal	Physical Review C - Nuclear Physics
Volume	88
Issue number	2
DOIs	https://doi.org/10.1103/PhysRevC.88.025501
State	Published - Aug 1 2013

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10.1103/PhysRevC.88.025501

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Aharmim, B., Ahmed, S. N., Anthony, A. E., Barros, N., Beier, E. W., Bellerive, A., Beltran, B., Bergevin, M., Biller, S. D., Boudjemline, K., Boulay, M. G., Cai, B., Chan, Y. D., Chauhan, D., Chen, M., Cleveland, B. T., Cox, G. A., Dai, X., Deng, H., ... Zuber, K. (2013). Combined analysis of all three phases of solar neutrino data from the Sudbury Neutrino Observatory. Physical Review C - Nuclear Physics, 88(2), Article 025501. https://doi.org/10.1103/PhysRevC.88.025501

@article{912ed24a83164135bcf98fcd1cf261eb,

title = "Combined analysis of all three phases of solar neutrino data from the Sudbury Neutrino Observatory",

abstract = "We report results from a combined analysis of solar neutrino data from all phases of the Sudbury Neutrino Observatory (SNO). By exploiting particle identification information obtained from the proportional counters installed during the third phase, this analysis improved background rejection in that phase of the experiment. The combined analysis of the SNO data resulted in a total flux of active neutrino flavors from 8B decays in the Sun of (5.25±0.16(stat.)-0.13+0.11(syst.))×106cm-2s -1, while a two-flavor neutrino oscillation analysis yielded Δm212=(5.6-1.4+1.9)×10-5eV2 and tan2θ12= 0.427-0.029+0.033. A three-flavor neutrino oscillation analysis combining the SNO result with results of all other solar neutrino experiments and reactor neutrino experiments yielded Δm212=(7.46-0.19+0.20)×10 -5eV2, tan2θ12=0.443-0.025+0.030, and sin2θ13=(2.49-0.32+0.20)×10-2.",

author = "B. Aharmim and Ahmed, {S. N.} and Anthony, {A. E.} and N. Barros and Beier, {E. W.} and A. Bellerive and B. Beltran and M. Bergevin and Biller, {S. D.} and K. Boudjemline and Boulay, {M. G.} and B. Cai and Chan, {Y. D.} and D. Chauhan and M. Chen and Cleveland, {B. T.} and Cox, {G. A.} and X. Dai and H. Deng and Detwiler, {J. A.} and M. Dimarco and Doe, {P. J.} and G. Doucas and Drouin, {P. L.} and Duncan, {F. A.} and M. Dunford and Earle, {E. D.} and Elliott, {S. R.} and Evans, {H. C.} and Ewan, {G. T.} and J. Farine and H. Fergani and F. Fleurot and Ford, {R. J.} and Formaggio, {J. A.} and N. Gagnon and Goon, {J. Tm} and K. Graham and E. Guillian and S. Habib and Hahn, {R. L.} and Hallin, {A. L.} and Hallman, {E. D.} and Harvey, {P. J.} and R. Hazama and Heintzelman, {W. J.} and J. Heise and Helmer, {R. L.} and A. Hime and C. Howard and M. Huang and P. Jagam and B. Jamieson and Jelley, {N. A.} and M. Jerkins and Keeter, {K. J.} and Klein, {J. R.} and Kormos, {L. L.} and M. Kos and C. Kraus and Krauss, {C. B.} and A. Kruger and T. Kutter and Kyba, {C. C.M.} and R. Lange and J. Law and Lawson, {I. T.} and Lesko, {K. T.} and Leslie, {J. R.} and Loach, {J. C.} and R. Maclellan and S. Majerus and Mak, {H. B.} and J. Maneira and R. Martin and N. McCauley and McDonald, {A. B.} and McGee, {S. R.} and Miller, {M. L.} and B. Monreal and J. Monroe and Nickel, {B. G.} and Noble, {A. J.} and O'Keeffe, {H. M.} and Oblath, {N. S.} and Ollerhead, {R. W.} and {Orebi Gann}, {G. D.} and Oser, {S. M.} and Ott, {R. A.} and Peeters, {S. J.M.} and Poon, {A. W.P.} and G. Prior and Reitzner, {S. D.} and K. Rielage and Robertson, {B. C.} and Robertson, {R. G.H.} and Rosten, {R. C.} and Schwendener, {M. H.} and Secrest, {J. A.} and Seibert, {S. R.} and O. Simard and Simpson, {J. J.} and P. Skensved and Sonley, {T. J.} and Stonehill, {L. C.} and G. Te{\v s}i{\'c} and N. Tolich and T. Tsui and {Van Berg}, R. and Vandevender, {B. A.} and Virtue, {C. J.} and {Wan Chan Tseung}, H. and Wark, {D. L.} and Watson, {P. J.S.} and J. Wendland and N. West and Wilkerson, {J. F.} and Wilson, {J. R.} and Wouters, {J. M.} and A. Wright and M. Yeh and F. Zhang and K. Zuber",

year = "2013",

month = aug,

day = "1",

doi = "10.1103/PhysRevC.88.025501",

language = "English",

volume = "88",

journal = "Physical Review C - Nuclear Physics",

issn = "0556-2813",

publisher = "American Physical Society",

number = "2",

}

Aharmim, B, Ahmed, SN, Anthony, AE, Barros, N, Beier, EW, Bellerive, A, Beltran, B, Bergevin, M, Biller, SD, Boudjemline, K, Boulay, MG, Cai, B, Chan, YD, Chauhan, D, Chen, M, Cleveland, BT, Cox, GA, Dai, X, Deng, H, Detwiler, JA, Dimarco, M, Doe, PJ, Doucas, G, Drouin, PL, Duncan, FA, Dunford, M, Earle, ED, Elliott, SR, Evans, HC, Ewan, GT, Farine, J, Fergani, H, Fleurot, F, Ford, RJ, Formaggio, JA, Gagnon, N, Goon, JT, Graham, K, Guillian, E, Habib, S, Hahn, RL, Hallin, AL, Hallman, ED, Harvey, PJ, Hazama, R, Heintzelman, WJ, Heise, J, Helmer, RL, Hime, A, Howard, C, Huang, M, Jagam, P, Jamieson, B, Jelley, NA, Jerkins, M, Keeter, KJ, Klein, JR, Kormos, LL, Kos, M, Kraus, C, Krauss, CB, Kruger, A, Kutter, T, Kyba, CCM, Lange, R, Law, J, Lawson, IT, Lesko, KT, Leslie, JR, Loach, JC, Maclellan, R, Majerus, S, Mak, HB, Maneira, J, Martin, R, McCauley, N, McDonald, AB, McGee, SR, Miller, ML, Monreal, B, Monroe, J, Nickel, BG, Noble, AJ, O'Keeffe, HM, Oblath, NS, Ollerhead, RW, Orebi Gann, GD, Oser, SM, Ott, RA, Peeters, SJM, Poon, AWP, Prior, G, Reitzner, SD, Rielage, K, Robertson, BC, Robertson, RGH, Rosten, RC, Schwendener, MH, Secrest, JA, Seibert, SR, Simard, O, Simpson, JJ, Skensved, P, Sonley, TJ, Stonehill, LC, Tešić, G, Tolich, N, Tsui, T, Van Berg, R, Vandevender, BA, Virtue, CJ, Wan Chan Tseung, H, Wark, DL, Watson, PJS, Wendland, J, West, N, Wilkerson, JF, Wilson, JR, Wouters, JM, Wright, A, Yeh, M, Zhang, F & Zuber, K 2013, 'Combined analysis of all three phases of solar neutrino data from the Sudbury Neutrino Observatory', Physical Review C - Nuclear Physics, vol. 88, no. 2, 025501. https://doi.org/10.1103/PhysRevC.88.025501

TY - JOUR

T1 - Combined analysis of all three phases of solar neutrino data from the Sudbury Neutrino Observatory

AU - Aharmim, B.

AU - Ahmed, S. N.

AU - Anthony, A. E.

AU - Barros, N.

AU - Beier, E. W.

AU - Bellerive, A.

AU - Beltran, B.

AU - Bergevin, M.

AU - Biller, S. D.

AU - Boudjemline, K.

AU - Boulay, M. G.

AU - Cai, B.

AU - Chan, Y. D.

AU - Chauhan, D.

AU - Chen, M.

AU - Cleveland, B. T.

AU - Cox, G. A.

AU - Dai, X.

AU - Deng, H.

AU - Detwiler, J. A.

AU - Dimarco, M.

AU - Doe, P. J.

AU - Doucas, G.

AU - Drouin, P. L.

AU - Duncan, F. A.

AU - Dunford, M.

AU - Earle, E. D.

AU - Elliott, S. R.

AU - Evans, H. C.

AU - Ewan, G. T.

AU - Farine, J.

AU - Fergani, H.

AU - Fleurot, F.

AU - Ford, R. J.

AU - Formaggio, J. A.

AU - Gagnon, N.

AU - Goon, J. Tm

AU - Graham, K.

AU - Guillian, E.

AU - Habib, S.

AU - Hahn, R. L.

AU - Hallin, A. L.

AU - Hallman, E. D.

AU - Harvey, P. J.

AU - Hazama, R.

AU - Heintzelman, W. J.

AU - Heise, J.

AU - Helmer, R. L.

AU - Hime, A.

AU - Howard, C.

AU - Huang, M.

AU - Jagam, P.

AU - Jamieson, B.

AU - Jelley, N. A.

AU - Jerkins, M.

AU - Keeter, K. J.

AU - Klein, J. R.

AU - Kormos, L. L.

AU - Kos, M.

AU - Kraus, C.

AU - Krauss, C. B.

AU - Kruger, A.

AU - Kutter, T.

AU - Kyba, C. C.M.

AU - Lange, R.

AU - Law, J.

AU - Lawson, I. T.

AU - Lesko, K. T.

AU - Leslie, J. R.

AU - Loach, J. C.

AU - Maclellan, R.

AU - Majerus, S.

AU - Mak, H. B.

AU - Maneira, J.

AU - Martin, R.

AU - McCauley, N.

AU - McDonald, A. B.

AU - McGee, S. R.

AU - Miller, M. L.

AU - Monreal, B.

AU - Monroe, J.

AU - Nickel, B. G.

AU - Noble, A. J.

AU - O'Keeffe, H. M.

AU - Oblath, N. S.

AU - Ollerhead, R. W.

AU - Orebi Gann, G. D.

AU - Oser, S. M.

AU - Ott, R. A.

AU - Peeters, S. J.M.

AU - Poon, A. W.P.

AU - Prior, G.

AU - Reitzner, S. D.

AU - Rielage, K.

AU - Robertson, B. C.

AU - Robertson, R. G.H.

AU - Rosten, R. C.

AU - Schwendener, M. H.

AU - Secrest, J. A.

AU - Seibert, S. R.

AU - Simard, O.

AU - Simpson, J. J.

AU - Skensved, P.

AU - Sonley, T. J.

AU - Stonehill, L. C.

AU - Tešić, G.

AU - Tolich, N.

AU - Tsui, T.

AU - Van Berg, R.

AU - Vandevender, B. A.

AU - Virtue, C. J.

AU - Wan Chan Tseung, H.

AU - Wark, D. L.

AU - Watson, P. J.S.

AU - Wendland, J.

AU - West, N.

AU - Wilkerson, J. F.

AU - Wilson, J. R.

AU - Wouters, J. M.

AU - Wright, A.

AU - Yeh, M.

AU - Zhang, F.

AU - Zuber, K.

PY - 2013/8/1

Y1 - 2013/8/1

N2 - We report results from a combined analysis of solar neutrino data from all phases of the Sudbury Neutrino Observatory (SNO). By exploiting particle identification information obtained from the proportional counters installed during the third phase, this analysis improved background rejection in that phase of the experiment. The combined analysis of the SNO data resulted in a total flux of active neutrino flavors from 8B decays in the Sun of (5.25±0.16(stat.)-0.13+0.11(syst.))×106cm-2s -1, while a two-flavor neutrino oscillation analysis yielded Δm212=(5.6-1.4+1.9)×10-5eV2 and tan2θ12= 0.427-0.029+0.033. A three-flavor neutrino oscillation analysis combining the SNO result with results of all other solar neutrino experiments and reactor neutrino experiments yielded Δm212=(7.46-0.19+0.20)×10 -5eV2, tan2θ12=0.443-0.025+0.030, and sin2θ13=(2.49-0.32+0.20)×10-2.

AB - We report results from a combined analysis of solar neutrino data from all phases of the Sudbury Neutrino Observatory (SNO). By exploiting particle identification information obtained from the proportional counters installed during the third phase, this analysis improved background rejection in that phase of the experiment. The combined analysis of the SNO data resulted in a total flux of active neutrino flavors from 8B decays in the Sun of (5.25±0.16(stat.)-0.13+0.11(syst.))×106cm-2s -1, while a two-flavor neutrino oscillation analysis yielded Δm212=(5.6-1.4+1.9)×10-5eV2 and tan2θ12= 0.427-0.029+0.033. A three-flavor neutrino oscillation analysis combining the SNO result with results of all other solar neutrino experiments and reactor neutrino experiments yielded Δm212=(7.46-0.19+0.20)×10 -5eV2, tan2θ12=0.443-0.025+0.030, and sin2θ13=(2.49-0.32+0.20)×10-2.

UR - http://www.scopus.com/inward/record.url?scp=84883473826&partnerID=8YFLogxK

U2 - 10.1103/PhysRevC.88.025501

DO - 10.1103/PhysRevC.88.025501

M3 - Article

AN - SCOPUS:84883473826

SN - 0556-2813

VL - 88

JO - Physical Review C - Nuclear Physics

JF - Physical Review C - Nuclear Physics

IS - 2

M1 - 025501

ER -

Combined analysis of all three phases of solar neutrino data from the Sudbury Neutrino Observatory

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