Y
Y. Takeuchi
Researcher at Queen's University
Publications - 5
Citations - 1114
Y. Takeuchi is an academic researcher from Queen's University. The author has contributed to research in topics: Sudbury Neutrino Observatory & Neutrino. The author has an hindex of 5, co-authored 5 publications receiving 1082 citations.
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Journal ArticleDOI
Measurement of the total active B-8 solar neutrino flux at the Sudbury Neutrino Observatory with enhanced neutral current sensitivity
S. N. Ahmed,A. E. Anthony,E. W. Beier,Alain Bellerive,S. D. Biller,J. Boger,M.G. Boulay,M. G. Bowler,T. J. Bowles,S. J. Brice,T. V. Bullard,Yuen-Dat Chan,M. L. Chen,X. Chen,B. T. Cleveland,G. A. Cox,X. Dai,X. Dai,F. Dalnoki-Veress,P. J. Doe,R. S. Dosanjh,G. Doucas,M. R. Dragowsky,C. A. Duba,F. A. Duncan,Monica Dunford,J. A. Dunmore,E. D. Earle,S. R. Elliott,Hal Evans,G. T. Ewan,J. Farine,J. Farine,H. Fergani,F. Fleurot,Joseph A. Formaggio,Malcolm M. Fowler,K. Frame,K. Frame,B. G. Fulsom,N. Gagnon,K. Graham,Darren Grant,R. L. Hahn,J. C. Hall,A. L. Hallin,E. D. Hallman,A. S. Hamer,W. B. Handler,C. K. Hargrove,P. J. Harvey,R. Hazama,K. M. Heeger,W. J. Heintzelman,J. Heise,R. L. Helmer,R. L. Helmer,R. J. Hemingway,Andrew Hime,M. A. Howe,P. Jagam,N. A. Jelley,Joshua R. Klein,Joshua R. Klein,M. Kos,A. V. Krumins,T. Kutter,Christopher C. M. Kyba,H. Labranche,R. Lange,J. Law,I. T. Lawson,K. T. Lesko,J. R. Leslie,I. Levine,I. Levine,S. Luoma,R. MacLellan,S. Majerus,H. B. Mak,J. Maneira,A. D. Marino,N. McCauley,A. B. McDonald,S. McGee,G. McGregor,C. Mifflin,K.K.S. Miknaitis,Guthrie Miller,B. A. Moffat,C. W. Nally,Bernie G. Nickel,A. J. Noble,A. J. Noble,A. J. Noble,Eric B. Norman,N. S. Oblath,C. E. Okada,R. W. Ollerhead,John L. Orrell,S. M. Oser,S. M. Oser,C. Ouellet,S. J. M. Peeters,A. W. P. Poon,B. C. Robertson,R. G. H. Robertson,E. Rollin,S. S.E. Rosendahl,V. L. Rusu,M. H. Schwendener,O. Simard,J. J. Simpson,C. J. Sims,David A. Sinclair,David A. Sinclair,P. Skensved,M. W.E. Smith,N. Starinsky,R. G. Stokstad,L. C. Stonehill,Reda Tafirout,Y. Takeuchi,G. Tešić,M. A. Thomson,M. Thorman,R. Van Berg,R. G. Van de Water,C. J. Virtue,B. L. Wall,D. Waller,Chris Waltham,H. Wan Chan Tseung,D. L. Wark,D. L. Wark,N. West,J. B. Wilhelmy,J. F. Wilkerson,J. R. Wilson,J. M. Wouters,Minfang Yeh,Kai Zuber +141 more
TL;DR: The Sudbury Neutrino Observatory has precisely determined the total active (nu(x) 8B solar neutrino flux without assumptions about the energy dependence of the nu(e) survival probability.
Journal Article
Electron energy spectra, fluxes, and day-night asymmetries of boron-8 solar neutrinos from the 391-day salt phase sno data set
B. Aharmim,S. N. Ahmed,A. E. Anthony,E. W. Beier,Alain Bellerive,M. Bergevin,S. D. Biller,J. Boger,M.G. Boulay,M. G. Bowler,T. V. Bullard,Yuen-Dat Chan,Min Chen,X. Chen,B. T. Cleveland,G. A. Cox,C. Currat,X. Dai,F. Dalnoki-Veress,H. Deng,P. J. Doe,R. S. Dosanjh,G. Doucas,C. A. Duba,F. A. Duncan,Monica Dunford,J. A. Dunmore,E. D. Earle,S. R. Elliott,Hal Evans,G. T. Ewan,J. Farine,H. Fergani,F. Fleurot,Joseph A. Formaggio,K. Frame,W. Frati,B. G. Fulsom,N. Gagnon,K. Graham,Darren Grant,R. L. Hahn,J. C. Hall,A. L. Hallin,E. D. Hallman,W. B. Handler,C. K. Hargrove,P. J. Harvey,Ryuta Hazama,K. M. Heeger,L. Heelan,W. J. Heintzelman,J. Heise,R. L. Helmer,R. J. Hemingway,Andrew Hime,C. Howard,Howe,M. Huang,P. Jagam,N. A. Jelley,Joshua R. Klein,L. L. Kormos,Kos,A. Krüger,C. Kraus,C. B. Krauss,A. V. Krumins,T. Kutter,Christopher C. M. Kyba,H. Labranche,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,N. McCauley,A. B. McDonald,S. McGee,G. McGregor,C. Mifflin,K.K.S. Miknaitis,B. A. Moffat,C. W. Nally,Neubauer,Bernie G. Nickel,A. J. Noble,Eric B. Norman,N. S. Oblath,C. E. Okada,R. W. Ollerhead,John L. Orrell,S. M. Oser,C. Ouellet,S. J. M. Peeters,A. W. P. Poon,Keith Rielage,B. C. Robertson,R. G. H. Robertson,E. Rollin,S. S.E. Rosendahl,V. L. Rusu,M. H. Schwendener,S. R. Seibert,O. Simard,J. J. Simpson,C. J. Sims,David A. Sinclair,P. Skensved,M. W.E. Smith,N. Starinsky,R. G. Stokstad,L. C. Stonehill,Reda Tafirout,Y. Takeuchi,G. Tešić,Marcus J. Thomson,M. Thorman,T. Tsui,R. Van,Van Berg,de Water,C. J. Virtue,B. L. Wall,D. Waller,Chris Waltham,H. Wan,Chan Tseung,D. L. Wark,J. Wendland,N. West,J. F. Wilkerson,J. R. Wilson,Peter Wittich,J. M. Wouters,A. Wright,Minfang Yeh,Kai Zuber +145 more
TL;DR: Aharmim et al. as discussed by the authors reported the results of the complete salt phase of the Sudbury Neutrino Observatory experiment in which NaCl was dissolved in the D_2O target.
Journal ArticleDOI
Determination of the νe and total B8 solar neutrino fluxes using the Sudbury Neutrino Observatory Phase I data set
B. Aharmim,Q. R. Ahmad,S. N. Ahmed,R. C. Allen,T. C. Andersen,J. D. Anglin,G. Bühler,J. C. Barton,E. W. Beier,M. Bercovitch,M. Bergevin,M. Bergevin,J. Bigu,S. D. Biller,R. A. Black,I. Blevis,R. J. Boardman,J. Boger,E. Bonvin,M.G. Boulay,M.G. Boulay,M. G. Bowler,T. J. Bowles,S. J. Brice,M. C. Browne,M. C. Browne,T. V. Bullard,T.H. Burritt,J. Cameron,Yuen-Dat Chan,Herbert H. Chen,M. L. Chen,X. Chen,B. T. Cleveland,J. H.M. Cowan,D. F. Cowen,G. A. Cox,C. A. Currat,X. Dai,X. Dai,X. Dai,F. Dalnoki-Veress,W. F. Davidson,H. Deng,M. DiMarco,P. J. Doe,G. Doucas,M. R. Dragowsky,C. A. Duba,F. A. Duncan,Monica Dunford,J. A. Dunmore,E. D. Earle,Steven Elliott,Steven Elliott,Hal Evans,G. T. Ewan,J. Farine,H. Fergani,A. P. Ferraris,F. Fleurot,R. J. Ford,J. A. Formaggio,Malcolm M. Fowler,K. Frame,K. Frame,E. D. Frank,W. Frati,N. Gagnon,J. V. Germani,J. V. Germani,Salvador Gil,A. Goldschmidt,J. T.M. Goon,K. Graham,Darren Grant,E. Guillian,R. L. Hahn,A. L. Hallin,E. D. Hallman,A. S. Hamer,A. S. Hamer,A. A. Hamian,W. B. Handler,R. U. Haq,C. K. Hargrove,P. J. Harvey,Ryuta Hazama,K. M. Heeger,W. J. Heintzelman,J. Heise,J. Heise,J. Heise,R. L. Helmer,Reyco Henning,J. D. Hepburn,H. Heron,J. Hewett,Andrew Hime,C. Howard,M. A. Howe,M. Huang,J. G. Hykaway,M. C.P. Isaac,P. Jagam,B. Jamieson,N. A. Jelley,C. Jillings,G. Jonkmans,G. Jonkmans,K. Kazkaz,P. T. Keener,Klaus Kirch,Joshua R. Klein,A. B. Knox,R. J. Komar,L. L. Kormos,M. Kos,Richard T. Kouzes,A. Krüger,C. Kraus,C. B. Krauss,T. Kutter,Christopher C. M. Kyba,H. Labranche,R. Lange,J. Law,I. T. Lawson,M. Lay,H. W. Lee,K. T. Lesko,J. R. Leslie,I. Levine,J. C. Loach,W. Locke,S. Luoma,J. Lyon,R. MacLellan,S. Majerus,H. B. Mak,J. Maneira,A. D. Marino,R. D. Martin,N. McCauley,A. B. McDonald,D. S. McDonald,K. McFarlane,S. McGee,G. McGregor,R. Meijer Drees,H. Mes,C. Mifflin,K. K.S. Miknaitis,M. L. Miller,G. Milton,B. A. Moffat,Benjamin Monreal,M. Moorhead,M. Moorhead,B. Morrissette,C. W. Nally,Mark Neubauer,F. M. Newcomer,H. S. Ng,Bernie G. Nickel,A. J. Noble,E. B. Norman,V. M. Novikov,N. S. Oblath,C. E. Okada,H. M. O'Keeffe,R. W. Ollerhead,M. Omori,John L. Orrell,S. M. Oser,R. A. Ott,S. J. M. Peeters,A. W. P. Poon,G. Prior,S. D. Reitzner,Keith Rielage,Keith Rielage,A. Roberge,B. C. Robertson,R. G. H. Robertson,S. S.E. Rosendahl,J. K. Rowley,V. L. Rusu,E. Saettler,A. Schülke,M. H. Schwendener,J. A. Secrest,H. Seifert,H. Seifert,H. Seifert,M. Shatkay,J. J. Simpson,C. J. Sims,David A. Sinclair,David A. Sinclair,P. Skensved,Alan R. Smith,M. W.E. Smith,M. W.E. Smith,N. Starinsky,T. D. Steiger,R. G. Stokstad,L. C. Stonehill,L. C. Stonehill,R. S. Storey,Bhaskar Sur,Bhaskar Sur,Reda Tafirout,N. Tagg,Y. Takeuchi,N.W. Tanner,R. K. Taplin,M. Thorman,P. M. Thornewell,P. M. Thornewell,P. M. Thornewell,N. Tolich,P. T. Trent,Y. I. Tserkovnyak,T. Tsui,C. D. Tunnell,R. Van Berg,R. G. Van de Water,R. G. Van de Water,C. J. Virtue,T. J. Walker,B. L. Wall,Chris Waltham,H. Wan Chan Tseung,J. X. Wang,D. L. Wark,J. Wendland,N. West,J. B. Wilhelmy,J. F. Wilkerson,J. R. Wilson,Peter Wittich,J. M. Wouters,A. Wright,Minfang Yeh,Kai Zuber +245 more
TL;DR: The phase I data set of the Sudbury Neutrino Observatory (SNO) as discussed by the authors is based on a 0.65 kt-year exposure of heavy water to the solar 8B neutrino flux.
Journal ArticleDOI
Constraints on nucleon decay via invisible modes from the Sudbury Neutrino Observatory.
S. N. Ahmed,A. E. Anthony,E. W. Beier,Alain Bellerive,S. D. Biller,J. Boger,M.G. Boulay,M. G. Bowler,T. J. Bowles,S. J. Brice,T. V. Bullard,Yuen-Dat Chan,M. L. Chen,X. Chen,B. T. Cleveland,G. A. Cox,X. Dai,X. Dai,F. Dalnoki-Veress,P. J. Doe,R. S. Dosanjh,G. Doucas,M. R. Dragowsky,C. A. Duba,F. A. Duncan,Monica Dunford,J. A. Dunmore,E. D. Earle,S. R. Elliott,Hal Evans,G. T. Ewan,J. Farine,J. Farine,H. Fergani,F. Fleurot,Joseph A. Formaggio,Malcolm M. Fowler,K. Frame,K. Frame,W. Frati,B. G. Fulsom,N. Gagnon,K. Graham,Darren Grant,R. L. Hahn,J. C. Hall,A. L. Hallin,E. D. Hallman,A. S. Hamer,W. B. Handler,C. K. Hargrove,P. J. Harvey,R. Hazama,K. M. Heeger,W. J. Heintzelman,J. Heise,R. L. Helmer,R. L. Helmer,R. J. Hemingway,Andrew Hime,M. A. Howe,P. Jagam,N. A. Jelley,Joshua R. Klein,Joshua R. Klein,M. Kos,A. V. Krumins,T. Kutter,Christopher C. M. Kyba,H. Labranche,R. Lange,J. Law,I. T. Lawson,K. T. Lesko,J. R. Leslie,I. Levine,I. Levine,S. Luoma,R. MacLellan,S. Majerus,H. B. Mak,J. Maneira,A. D. Marino,N. McCauley,A. B. McDonald,S. McGee,G. McGregor,C. Mifflin,K.K.S. Miknaitis,Guthrie Miller,B. A. Moffat,C. W. Nally,Mark Neubauer,Bernie G. Nickel,A. J. Noble,A. J. Noble,A. J. Noble,Eric B. Norman,N. S. Oblath,C. E. Okada,R. W. Ollerhead,John L. Orrell,S. M. Oser,S. M. Oser,C. Ouellet,S. J. M. Peeters,A. W. P. Poon,B. C. Robertson,R. G. H. Robertson,E. Rollin,S. S.E. Rosendahl,V. L. Rusu,M. H. Schwendener,O. Simard,J. J. Simpson,C. J. Sims,David A. Sinclair,David A. Sinclair,P. Skensved,M. W.E. Smith,N. Starinsky,R. G. Stokstad,L. C. Stonehill,Reda Tafirout,Y. Takeuchi,G. Tešić,M. A. Thomson,M. Thorman,R. Van Berg,R. G. Van de Water,C. J. Virtue,B. L. Wall,D. Waller,Chris Waltham,H. Wan Chan Tseung,D. L. Wark,N. West,J. B. Wilhelmy,J. F. Wilkerson,J. R. Wilson,Peter Wittich,J. M. Wouters,Minfang Yeh,Kai Zuber +143 more
TL;DR: Data from the Sudbury Neutrino Observatory have been used to constrain the lifetime for nucleon decay to "invisible" modes, such as n-->3nu, which is about an order of magnitude more stringent than previous constraints on invisible proton-decay modes and 400 timesMore stringent than similar neutron modes.
Journal ArticleDOI
Electron antineutrino search at the Sudbury Neutrino Observatory
B. Aharmim,S. N. Ahmed,E. W. Beier,Alain Bellerive,S. D. Biller,J. Boger,M.G. Boulay,T. J. Bowles,S. J. Brice,T. V. Bullard,Yuen-Dat Chan,M. L. Chen,Xiaobo Chen,B. T. Cleveland,G. A. Cox,X. Dai,X. Dai,F. Dalnoki-Veress,P. J. Doe,R. S. Dosanjh,G. Doucas,M. R. Dragowsky,C. A. Duba,F. A. Duncan,Monica Dunford,J. A. Dunmore,E. D. Earle,S. R. Elliott,Hal Evans,G. T. Ewan,J. Farine,J. Farine,H. Fergani,F. Fleurot,Joseph A. Formaggio,Malcolm M. Fowler,K. Frame,K. Frame,K. Frame,W. Frati,B. G. Fulsom,N. Gagnon,K. Graham,Darren Grant,R. L. Hahn,A. L. Hallin,E. D. Hallman,A. S. Hamer,W. B. Handler,C. K. Hargrove,P. J. Harvey,R. Hazama,K. M. Heeger,W. J. Heintzelman,J. Heise,R. L. Helmer,R. L. Helmer,R. J. Hemingway,Andrew Hime,M. A. Howe,P. Jagam,N. A. Jelley,Joshua R. Klein,Joshua R. Klein,L. L. Kormos,M. S. Kos,M. S. Kos,A. Krüger,C. B. Krauss,A. V. Krumins,T. Kutter,Christopher C. M. Kyba,H. Labranche,R. Lange,J. Law,I. T. Lawson,K. T. Lesko,J. R. Leslie,I. Levine,S. Luoma,R. MacLellan,S. Majerus,H. B. Mak,J. Maneira,A. D. Marino,N. McCauley,A. B. McDonald,S. McGee,G. McGregor,C. Mifflin,K.K.S. Miknaitis,Guthrie Miller,B. A. Moffat,C. W. Nally,Mark Neubauer,B. G. Nickel,A. J. Noble,A. J. Noble,A. J. Noble,Eric B. Norman,N. S. Oblath,C. E. Okada,R. W. Ollerhead,John L. Orrell,S. M. Oser,S. M. Oser,C. Ouellet,S. J. M. Peeters,A. W. P. Poon,Keith Rielage,B. C. Robertson,R. G. H. Robertson,E. Rollin,S. S.E. Rosendahl,V. L. Rusu,M. H. Schwendener,O. Simard,J. J. Simpson,C. J. Sims,David A. Sinclair,David A. Sinclair,P. Skensved,M. W.E. Smith,N. Starinsky,R. G. Stokstad,L. C. Stonehill,Reda Tafirout,Y. Takeuchi,G. Tešić,M. A. Thomson,T. Tsui,R. Van Berg,R. G. Van de Water,C. J. Virtue,B. L. Wall,D. Waller,Chris Waltham,H. Wan Chan Tseung,D. L. Wark,N. West,J. B. Wilhelmy,J. F. Wilkerson,J. R. Wilson,Peter Wittich,J. M. Wouters,Minfang Yeh,Kai Zuber +146 more
TL;DR: In this paper, the upper limits on the (ν) over bar (e) flux at the Sudbury Neutrino Observatory have been set based on the charged-current reaction on deuterium, which produces a positron and two neutrons in coincidence.