Measurement of the cosmic ray and neutrino-induced muon flux at the Sudbury neutrino observatory

B. Aharmim; S. N. Ahmed; T. C. Andersen; A. E. Anthony; N. Barros; E. W. Beier; A. Bellerive; B. Beltran; M. Bergevin; S. D. Biller; K. Boudjemline; M. G. Boulay; T. H. Burritt; B. Cai; Y. D. Chan; M. Chen; M. C. Chon; B. T. Cleveland; G. A. Cox-Mobrand; C. A. Currat; X. Dai; F. Dalnoki-Veress; H. Deng; J. Detwiler; P. J. Doe; R. S. Dosanjh; G. Doucas; P. L. Drouin; F. A. Duncan; M. Dunford; S. R. Elliott; H. C. Evans; G. T. Ewan; J. Farine; H. Fergani; F. Fleurot; R. J. Ford; J. A. Formaggio; N. Gagnon; J. T.M. Goon; K. Graham; D. R. Grant; E. Guillian; S. Habib; R. L. Hahn; A. L. Hallin; E. D. Hallman; C. K. Hargrove; P. J. Harvey; R. Hazama; K. M. Heeger; W. J. Heintzelman; J. Heise; R. L. Helmer; R. J. Hemingway; R. Henning; A. Hime; C. Howard; M. A. Howe; M. Huang; B. Jamieson; N. A. Jelley; J. R. Klein; M. Kos; A. Krüger; C. Kraus; C. B. Krauss; T. Kutter; C. C.M. Kyba; R. Lange; J. Law; I. T. Lawson; K. T. Lesko; J. R. Leslie; I. Levine; J. C. Loach; S. Luoma; R. MacLellan; S. Majerus; H. B. Mak; J. Maneira; A. D. Marino; R. Martin; N. McCauley; A. B. McDonald; S. McGee; C. Mifflin; M. L. Miller; B. Monreal; J. Monroe; A. J. Noble; N. S. Oblath; C. E. Okada; H. M. O'Keeffe; Y. Opachich; G. D.Orebi Gann; S. M. Oser; R. A. Ott; S. J.M. Peeters; A. W.P. Poon; G. Prior; K. Rielage; B. C. Robertson; R. G.H. Robertson; E. Rollin; M. H. Schwendener; J. A. Secrest; S. R. Seibert; O. Simard; J. J. Simpson; D. Sinclair; P. Skensved; M. W.E. Smith; T. J. Sonley; T. D. Steiger; L. C. Stonehill; N. Tagg; G. Tešić; N. Tolich; T. Tsui; R. G.Van De Water; B. A. Vandevender; C. J. Virtue; D. Waller; C. E. Waltham; H. Wan Chan Tseung; D. L. Wark; P. 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/PhysRevD.80.012001

Measurement of the cosmic ray and neutrino-induced muon flux at the Sudbury neutrino observatory

B. Aharmim
, S. N. Ahmed
, T. C. Andersen
, A. E. Anthony
, N. Barros
, E. W. Beier
, A. Bellerive
, B. Beltran
, M. Bergevin
, S. D. Biller
, K. Boudjemline
, M. G. Boulay
, T. H. Burritt
, B. Cai
, Y. D. Chan
, M. Chen
, M. C. Chon
, B. T. Cleveland
, G. A. Cox-Mobrand
, C. A. Currat

X. Dai, F. Dalnoki-Veress, H. Deng, J. Detwiler, P. J. Doe, R. S. Dosanjh, G. Doucas, P. L. Drouin, F. A. Duncan, M. Dunford, S. R. Elliott, H. C. Evans, G. T. Ewan, J. Farine, H. Fergani, F. Fleurot, R. J. Ford, J. A. Formaggio, N. Gagnon, J. T.M. Goon, K. Graham, D. R. Grant, E. Guillian, S. Habib, R. L. Hahn, A. L. Hallin, E. D. Hallman, C. K. Hargrove, P. J. Harvey, R. Hazama, K. M. Heeger, W. J. Heintzelman, J. Heise, R. L. Helmer, R. J. Hemingway, R. Henning, A. Hime, C. Howard, M. A. Howe, M. Huang, B. Jamieson, N. A. Jelley, J. R. Klein, M. Kos, A. Krüger, C. Kraus, C. B. Krauss, T. Kutter, C. C.M. Kyba, R. Lange, J. Law, I. T. Lawson, K. T. Lesko, J. R. Leslie, I. Levine, J. C. Loach, S. Luoma, R. MacLellan, S. Majerus, H. B. Mak, J. Maneira, A. D. Marino, R. Martin, N. McCauley, A. B. McDonald, S. McGee, C. Mifflin, M. L. Miller, B. Monreal, J. Monroe, A. J. Noble, N. S. Oblath, C. E. Okada, H. M. O'Keeffe, Y. Opachich, G. D.Orebi Gann, S. M. Oser, R. A. Ott, S. J.M. Peeters, A. W.P. Poon, G. Prior, K. Rielage, B. C. Robertson, R. G.H. Robertson, E. Rollin, M. H. Schwendener, J. A. Secrest, S. R. Seibert, O. Simard, J. J. Simpson, D. Sinclair, P. Skensved, M. W.E. Smith, T. J. Sonley, T. D. Steiger, L. C. Stonehill, N. Tagg, G. Tešić, N. Tolich, T. Tsui, R. G.Van De Water, B. A. Vandevender, C. J. Virtue, D. Waller, C. E. Waltham, H. Wan Chan Tseung, D. L. Wark, P. 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

Laurentian University
Queen's University Kingston
University of Guelph
University of Texas at Austin
Laboratório de Instrumentação e Física Experimental de Partículas
University of Pennsylvania
Carleton University
University of Alberta
Berkeley National Laboratory
University of Oxford
Los Alamos National Laboratory
University of Washington
Wells Fargo
Princeton University
SNOLAB
The University of Chicago
Massachusetts Institute of Technology
Louisiana State University
Case Western Reserve University
Brookhaven National Laboratory
Hiroshima University
University of Wisconsin–Madison
University of British Columbia
TRIUMF
University of North Carolina at Chapel Hill
Indiana University South Bend
University of Colorado Boulder
University of Liverpool
University of California at Santa Barbara
Remote Sensing Lab.
University of California, Davis
University of Sussex
CERN
University of Utah
Otterbein University
Imperial College London
Rutherford Appleton Laboratory
Technische Universität Dresden

Research output: Contribution to journal › Article › peer-review

60 Scopus citations

Abstract

Results are reported on the measurement of the atmospheric neutrino-induced muon flux at a depth of 2 kilometers below the Earth's surface from 1229 days of operation of the Sudbury Neutrino Observatory (SNO). By measuring the flux of through-going muons as a function of zenith angle, the SNO experiment can distinguish between the oscillated and unoscillated portion of the neutrino flux. A total of 514 muonlike events are measured between -1≤cos θzenith≤0.4 in a total exposure of 2.30×1014cm2s. The measured flux normalization is 1.22±0.09 times the Bartol three-dimensional flux prediction. This is the first measurement of the neutrino-induced flux where neutrino oscillations are minimized. The zenith distribution is consistent with previously measured atmospheric neutrino oscillation parameters. The cosmic ray muon flux at SNO with zenith angle cos θzenith>0.4 is measured to be (3.31±0.01(stat)±0.09(sys))×10-10μ/s/cm2.

Original language	English
Article number	012001
Journal	Physical Review D - Particles, Fields, Gravitation and Cosmology
Volume	80
Issue number	1
DOIs	https://doi.org/10.1103/PhysRevD.80.012001
State	Published - Jul 10 2009

Scopus Subject Areas

Nuclear and High Energy Physics
Physics and Astronomy (miscellaneous)

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10.1103/PhysRevD.80.012001

Cite this

Aharmim, B., Ahmed, S. N., Andersen, T. C., Anthony, A. E., Barros, N., Beier, E. W., Bellerive, A., Beltran, B., Bergevin, M., Biller, S. D., Boudjemline, K., Boulay, M. G., Burritt, T. H., Cai, B., Chan, Y. D., Chen, M., Chon, M. C., Cleveland, B. T., Cox-Mobrand, G. A., ... Zuber, K. (2009). Measurement of the cosmic ray and neutrino-induced muon flux at the Sudbury neutrino observatory. Physical Review D - Particles, Fields, Gravitation and Cosmology, 80(1), Article 012001. https://doi.org/10.1103/PhysRevD.80.012001

@article{834ecc72ae104cb0a0d5783862cfe4ae,

title = "Measurement of the cosmic ray and neutrino-induced muon flux at the Sudbury neutrino observatory",

abstract = "Results are reported on the measurement of the atmospheric neutrino-induced muon flux at a depth of 2 kilometers below the Earth's surface from 1229 days of operation of the Sudbury Neutrino Observatory (SNO). By measuring the flux of through-going muons as a function of zenith angle, the SNO experiment can distinguish between the oscillated and unoscillated portion of the neutrino flux. A total of 514 muonlike events are measured between -1≤cos θzenith≤0.4 in a total exposure of 2.30×1014cm2s. The measured flux normalization is 1.22±0.09 times the Bartol three-dimensional flux prediction. This is the first measurement of the neutrino-induced flux where neutrino oscillations are minimized. The zenith distribution is consistent with previously measured atmospheric neutrino oscillation parameters. The cosmic ray muon flux at SNO with zenith angle cos θzenith>0.4 is measured to be (3.31±0.01(stat)±0.09(sys))×10-10μ/s/cm2.",

author = "B. Aharmim and Ahmed, \{S. N.\} and Andersen, \{T. C.\} 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 Burritt, \{T. H.\} and B. Cai and Chan, \{Y. D.\} and M. Chen and Chon, \{M. C.\} and Cleveland, \{B. T.\} and Cox-Mobrand, \{G. A.\} and Currat, \{C. A.\} and X. Dai and F. Dalnoki-Veress and H. Deng and J. Detwiler and Doe, \{P. J.\} and Dosanjh, \{R. S.\} and G. Doucas and Drouin, \{P. L.\} and Duncan, \{F. A.\} and M. Dunford 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. T.M.\} and K. Graham and Grant, \{D. R.\} and E. Guillian and S. Habib and Hahn, \{R. L.\} and Hallin, \{A. L.\} and Hallman, \{E. D.\} and Hargrove, \{C. K.\} and Harvey, \{P. J.\} and R. Hazama and Heeger, \{K. M.\} and Heintzelman, \{W. J.\} and J. Heise and Helmer, \{R. L.\} and Hemingway, \{R. J.\} and R. Henning and A. Hime and C. Howard and Howe, \{M. A.\} and M. Huang and B. Jamieson and Jelley, \{N. A.\} and Klein, \{J. R.\} and M. Kos and A. Kr{\"u}ger and C. Kraus and Krauss, \{C. B.\} 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 I. Levine and Loach, \{J. C.\} and S. Luoma and R. MacLellan and S. Majerus and Mak, \{H. B.\} and J. Maneira and Marino, \{A. D.\} and R. Martin and N. McCauley and McDonald, \{A. B.\} and S. McGee and C. Mifflin and Miller, \{M. L.\} and B. Monreal and J. Monroe and Noble, \{A. J.\} and Oblath, \{N. S.\} and Okada, \{C. E.\} and O'Keeffe, \{H. M.\} and Y. Opachich and Gann, \{G. D.Orebi\} and Oser, \{S. M.\} and Ott, \{R. A.\} and Peeters, \{S. J.M.\} and Poon, \{A. W.P.\} and G. Prior and K. Rielage and Robertson, \{B. C.\} and Robertson, \{R. G.H.\} and E. Rollin and Schwendener, \{M. H.\} and Secrest, \{J. A.\} and Seibert, \{S. R.\} and O. Simard and Simpson, \{J. J.\} and D. Sinclair and P. Skensved and Smith, \{M. W.E.\} and Sonley, \{T. J.\} and Steiger, \{T. D.\} and Stonehill, \{L. C.\} and N. Tagg and G. Te{\v s}i{\'c} and N. Tolich and T. Tsui and \{De Water\}, \{R. G.Van\} and Vandevender, \{B. A.\} and Virtue, \{C. J.\} and D. Waller and Waltham, \{C. E.\} and Tseung, \{H. Wan Chan\} and Wark, \{D. L.\} and P. Watson 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 = "2009",

month = jul,

day = "10",

doi = "10.1103/PhysRevD.80.012001",

language = "English",

volume = "80",

journal = "Physical Review D - Particles, Fields, Gravitation and Cosmology",

issn = "1550-7998",

publisher = "American Physical Society",

number = "1",

}

Aharmim, B, Ahmed, SN, Andersen, TC, Anthony, AE, Barros, N, Beier, EW, Bellerive, A, Beltran, B, Bergevin, M, Biller, SD, Boudjemline, K, Boulay, MG, Burritt, TH, Cai, B, Chan, YD, Chen, M, Chon, MC, Cleveland, BT, Cox-Mobrand, GA, Currat, CA, Dai, X, Dalnoki-Veress, F, Deng, H, Detwiler, J, Doe, PJ, Dosanjh, RS, Doucas, G, Drouin, PL, Duncan, FA, Dunford, M, Elliott, SR, Evans, HC, Ewan, GT, Farine, J, Fergani, H, Fleurot, F, Ford, RJ, Formaggio, JA, Gagnon, N, Goon, JTM, Graham, K, Grant, DR, Guillian, E, Habib, S, Hahn, RL, Hallin, AL, Hallman, ED, Hargrove, CK, Harvey, PJ, Hazama, R, Heeger, KM, Heintzelman, WJ, Heise, J, Helmer, RL, Hemingway, RJ, Henning, R, Hime, A, Howard, C, Howe, MA, Huang, M, Jamieson, B, Jelley, NA, Klein, JR, Kos, M, Krüger, A, Kraus, C, Krauss, CB, Kutter, T, Kyba, CCM, Lange, R, Law, J, Lawson, IT, Lesko, KT, Leslie, JR, Levine, I, Loach, JC, Luoma, S, MacLellan, R, Majerus, S, Mak, HB, Maneira, J, Marino, AD, Martin, R, McCauley, N, McDonald, AB, McGee, S, Mifflin, C, Miller, ML, Monreal, B, Monroe, J, Noble, AJ, Oblath, NS, Okada, CE, O'Keeffe, HM, Opachich, Y, Gann, GDO, Oser, SM, Ott, RA, Peeters, SJM, Poon, AWP, Prior, G, Rielage, K, Robertson, BC, Robertson, RGH, Rollin, E, Schwendener, MH, Secrest, JA, Seibert, SR, Simard, O, Simpson, JJ, Sinclair, D, Skensved, P, Smith, MWE, Sonley, TJ, Steiger, TD, Stonehill, LC, Tagg, N, Tešić, G, Tolich, N, Tsui, T, De Water, RGV, Vandevender, BA, Virtue, CJ, Waller, D, Waltham, CE, Tseung, HWC, Wark, DL, Watson, P, Wendland, J, West, N, Wilkerson, JF, Wilson, JR, Wouters, JM, Wright, A, Yeh, M, Zhang, F & Zuber, K 2009, 'Measurement of the cosmic ray and neutrino-induced muon flux at the Sudbury neutrino observatory', Physical Review D - Particles, Fields, Gravitation and Cosmology, vol. 80, no. 1, 012001. https://doi.org/10.1103/PhysRevD.80.012001

TY - JOUR

T1 - Measurement of the cosmic ray and neutrino-induced muon flux at the Sudbury neutrino observatory

AU - Aharmim, B.

AU - Ahmed, S. N.

AU - Andersen, T. C.

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 - Burritt, T. H.

AU - Cai, B.

AU - Chan, Y. D.

AU - Chen, M.

AU - Chon, M. C.

AU - Cleveland, B. T.

AU - Cox-Mobrand, G. A.

AU - Currat, C. A.

AU - Dai, X.

AU - Dalnoki-Veress, F.

AU - Deng, H.

AU - Detwiler, J.

AU - Doe, P. J.

AU - Dosanjh, R. S.

AU - Doucas, G.

AU - Drouin, P. L.

AU - Duncan, F. A.

AU - Dunford, M.

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. T.M.

AU - Graham, K.

AU - Grant, D. R.

AU - Guillian, E.

AU - Habib, S.

AU - Hahn, R. L.

AU - Hallin, A. L.

AU - Hallman, E. D.

AU - Hargrove, C. K.

AU - Harvey, P. J.

AU - Hazama, R.

AU - Heeger, K. M.

AU - Heintzelman, W. J.

AU - Heise, J.

AU - Helmer, R. L.

AU - Hemingway, R. J.

AU - Henning, R.

AU - Hime, A.

AU - Howard, C.

AU - Howe, M. A.

AU - Huang, M.

AU - Jamieson, B.

AU - Jelley, N. A.

AU - Klein, J. R.

AU - Kos, M.

AU - Krüger, A.

AU - Kraus, C.

AU - Krauss, C. B.

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 - Levine, I.

AU - Loach, J. C.

AU - Luoma, S.

AU - MacLellan, R.

AU - Majerus, S.

AU - Mak, H. B.

AU - Maneira, J.

AU - Marino, A. D.

AU - Martin, R.

AU - McCauley, N.

AU - McDonald, A. B.

AU - McGee, S.

AU - Mifflin, C.

AU - Miller, M. L.

AU - Monreal, B.

AU - Monroe, J.

AU - Noble, A. J.

AU - Oblath, N. S.

AU - Okada, C. E.

AU - O'Keeffe, H. M.

AU - Opachich, Y.

AU - Gann, G. D.Orebi

AU - Oser, S. M.

AU - Ott, R. A.

AU - Peeters, S. J.M.

AU - Poon, A. W.P.

AU - Prior, G.

AU - Rielage, K.

AU - Robertson, B. C.

AU - Robertson, R. G.H.

AU - Rollin, E.

AU - Schwendener, M. H.

AU - Secrest, J. A.

AU - Seibert, S. R.

AU - Simard, O.

AU - Simpson, J. J.

AU - Sinclair, D.

AU - Skensved, P.

AU - Smith, M. W.E.

AU - Sonley, T. J.

AU - Steiger, T. D.

AU - Stonehill, L. C.

AU - Tagg, N.

AU - Tešić, G.

AU - Tolich, N.

AU - Tsui, T.

AU - De Water, R. G.Van

AU - Vandevender, B. A.

AU - Virtue, C. J.

AU - Waller, D.

AU - Waltham, C. E.

AU - Tseung, H. Wan Chan

AU - Wark, D. L.

AU - Watson, P.

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 - 2009/7/10

Y1 - 2009/7/10

N2 - Results are reported on the measurement of the atmospheric neutrino-induced muon flux at a depth of 2 kilometers below the Earth's surface from 1229 days of operation of the Sudbury Neutrino Observatory (SNO). By measuring the flux of through-going muons as a function of zenith angle, the SNO experiment can distinguish between the oscillated and unoscillated portion of the neutrino flux. A total of 514 muonlike events are measured between -1≤cos θzenith≤0.4 in a total exposure of 2.30×1014cm2s. The measured flux normalization is 1.22±0.09 times the Bartol three-dimensional flux prediction. This is the first measurement of the neutrino-induced flux where neutrino oscillations are minimized. The zenith distribution is consistent with previously measured atmospheric neutrino oscillation parameters. The cosmic ray muon flux at SNO with zenith angle cos θzenith>0.4 is measured to be (3.31±0.01(stat)±0.09(sys))×10-10μ/s/cm2.

AB - Results are reported on the measurement of the atmospheric neutrino-induced muon flux at a depth of 2 kilometers below the Earth's surface from 1229 days of operation of the Sudbury Neutrino Observatory (SNO). By measuring the flux of through-going muons as a function of zenith angle, the SNO experiment can distinguish between the oscillated and unoscillated portion of the neutrino flux. A total of 514 muonlike events are measured between -1≤cos θzenith≤0.4 in a total exposure of 2.30×1014cm2s. The measured flux normalization is 1.22±0.09 times the Bartol three-dimensional flux prediction. This is the first measurement of the neutrino-induced flux where neutrino oscillations are minimized. The zenith distribution is consistent with previously measured atmospheric neutrino oscillation parameters. The cosmic ray muon flux at SNO with zenith angle cos θzenith>0.4 is measured to be (3.31±0.01(stat)±0.09(sys))×10-10μ/s/cm2.

UR - https://www.scopus.com/pages/publications/69549138371

U2 - 10.1103/PhysRevD.80.012001

DO - 10.1103/PhysRevD.80.012001

M3 - Article

AN - SCOPUS:69549138371

SN - 1550-7998

VL - 80

JO - Physical Review D - Particles, Fields, Gravitation and Cosmology

JF - Physical Review D - Particles, Fields, Gravitation and Cosmology

IS - 1

M1 - 012001

ER -

Measurement of the cosmic ray and neutrino-induced muon flux at the Sudbury neutrino observatory

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