C
C. J. Virtue
Researcher at Laurentian University
Publications - 3
Citations - 497
C. J. Virtue is an academic researcher from Laurentian University. The author has contributed to research in topics: Neutrino oscillation & Neutrino. The author has an hindex of 3, co-authored 3 publications receiving 425 citations. Previous affiliations of C. J. Virtue include Imperial College London.
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Journal ArticleDOI
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,Alain Bellerive,B. Beltran,M. Bergevin,M. Bergevin,S. D. Biller,K. Boudjemline,K. Boudjemline,Mark Guy Boulay,Bei Cai,Yuen-Dat Chan,D. Chauhan,M. L. Chen,B. T. Cleveland,G. A. Cox,X. Dai,X. Dai,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,Steven Elliott,Steven Elliott,Hal Evans,G. T. Ewan,J. Farine,J. Farine,H. Fergani,F. Fleurot,R. J. Ford,Joseph A. Formaggio,Joseph A. Formaggio,N. Gagnon,J. Tm. Goon,K. Graham,K. Graham,E. Guillian,S. Habib,R. L. Hahn,A. L. Hallin,E. D. Hallman,P. J. Harvey,Ryuta Hazama,W. J. Heintzelman,J. Heise,J. Heise,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. Krüger,T. Kutter,Christopher 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. D. Martin,N. McCauley,A. B. McDonald,S. McGee,M. L. Miller,Benjamin Monreal,Jocelyn 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,Keith Rielage,B. C. Robertson,R. G. H. Robertson,Rachel Rosten,M. H. Schwendener,J. A. Secrest,S. Seibert,Olivier Simard,J. J. Simpson,P. Skensved,T. 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,Peter Watson,J. Wendland,N. West,J. F. Wilkerson,J. R. Wilson,J. M. Wouters,A. Wright,Minfang Yeh,F. Zhang,Kai Zuber +132 more
TL;DR: In this paper, a combined analysis of solar neutrino data from all phases of the Sudbury Neutrino Observatory was presented, which showed that particle identification information obtained from the proportional counters installed during the third phase improved background rejection in that phase of the experiment.
Journal Article
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,Alain Bellerive,B. Beltran,M. Bergevin,S. D. Biller,K. Boudjemline,Mark Guy Boulay,Bei Cai,Yuen-Dat Chan,D. Chauhan,M. L. 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,Steven Elliott,Hal Evans,G. T. Ewan,J. Farine,H. Fergani,F. Fleurot,R. J. Ford,Joseph 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,Ryuta 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. Krüger,T. Kutter,Christopher 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. D. Martin,N. McCauley,A. B. McDonald,S. McGee,M. L. Miller,Benjamin Monreal,Jocelyn 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,Keith Rielage,B. C. Robertson,R. G. H. Robertson,Rachel Rosten,M. H. Schwendener,J. A. Secrest,S. Seibert,Olivier Simard,J. J. Simpson,P. Skensved,T. 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,Peter Watson,J. Wendland,N. West,J. F. Wilkerson,J. R. Wilson,J. M. Wouters,A. Wright,Minfang Yeh,F. Zhang,Kai Zuber +122 more
TL;DR: In this paper, a combined analysis of solar neutrino data from all phases of the Sudbury Neutrino Observatory was presented, which showed that particle identification information obtained from the proportional counters installed during the third phase improved background rejection in that phase of the experiment.
Journal ArticleDOI
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,Alain Bellerive,B. Beltran,B. Beltran,M. Bergevin,M. Bergevin,S. D. Biller,K. Boudjemline,M.G. Boulay,M.G. Boulay,T.H. Burritt,Bei Cai,Yuen-Dat Chan,M. L. Chen,M. C. Chon,B. T. Cleveland,G.A. Cox-Mobrand,C. A. Currat,C. A. Currat,X. Dai,X. Dai,X. Dai,F. Dalnoki-Veress,F. Dalnoki-Veress,H. Deng,J. A. Detwiler,J. A. Detwiler,P. J. Doe,R. S. Dosanjh,G. Doucas,P.-L. Drouin,F. A. Duncan,Monica Dunford,Monica Dunford,Steven Elliott,Steven Elliott,Hal Evans,G. T. Ewan,J. Farine,H. Fergani,F. Fleurot,R. J. Ford,Joseph A. Formaggio,Joseph A. Formaggio,N. Gagnon,J. T.M. Goon,K. Graham,Darren Grant,Darren Grant,E. Guillian,S. Habib,S. Habib,R. L. Hahn,A. L. Hallin,A. L. Hallin,E. D. Hallman,C. K. Hargrove,P. J. Harvey,R. Hazama,R. Hazama,K. M. Heeger,K. M. Heeger,W. J. Heintzelman,J. Heise,J. Heise,J. Heise,R. L. Helmer,R. J. Hemingway,Reyco Henning,Andrew Hime,C. Howard,C. Howard,M. A. Howe,M. Huang,M. Huang,B. Jamieson,N. A. Jelley,Joshua R. Klein,Joshua R. Klein,M. Kos,A. Krüger,C. Kraus,C. B. Krauss,C. B. Krauss,T. Kutter,Christopher C. M. Kyba,R. Lange,J. Law,I. T. Lawson,K. T. Lesko,J. R. Leslie,I. Levine,I. Levine,J. C. Loach,J. C. Loach,S. Luoma,R. MacLellan,S. Majerus,H. B. Mak,J. Maneira,A. D. Marino,A. D. Marino,R. D. Martin,N. McCauley,N. McCauley,N. McCauley,A. B. McDonald,S. McGee,C. Mifflin,M. L. Miller,M. L. Miller,Benjamin Monreal,Benjamin Monreal,Jocelyn Monroe,A. J. Noble,N. S. Oblath,C. E. Okada,H. M. O'Keeffe,Y. Opachich,Y. Opachich,G. D. Orebi Gann,S. M. Oser,R. A. Ott,S. J. M. Peeters,S. J. M. Peeters,A. W. P. Poon,G. Prior,G. Prior,Keith Rielage,Keith Rielage,B. C. Robertson,R. G. H. Robertson,E. Rollin,M. H. Schwendener,J. A. Secrest,S. R. Seibert,S. R. Seibert,O. Simard,J. J. Simpson,David A. Sinclair,David A. Sinclair,P. Skensved,M. W.E. Smith,M. W.E. Smith,T. J. Sonley,T. J. Sonley,T. D. Steiger,L. C. Stonehill,L. C. Stonehill,N. Tagg,N. Tagg,N. Tagg,G. Tešić,N. Tolich,N. Tolich,T. Tsui,R. G. Van de Water,R. G. Van de Water,B.A. VanDevender,C. J. Virtue,C. J. Virtue,D. Waller,Chris Waltham,H. Wan Chan Tseung,D. L. Wark,Peter Watson,J. Wendland,N. West,J. F. Wilkerson,J. R. Wilson,J. M. Wouters,A. Wright,Minfang Yeh,F. Zhang,Kai Zuber,Kai Zuber +180 more
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 un-oscillated portion of the neutrino flux. A total of 514 muon-like events are measured between -1 {le} cos {theta}{sub zenith} 0.4 in a total exposure of 2.30 x 10{sup 14} cm{sup 2} s. 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 {theta}{sub zenith} > 0.4 is measured to be (3.31 {+-} 0.01 (stat.) {+-} 0.09 (sys.)) x 10{sup -10} {micro}/s/cm{sup 2}.