B
Bhaskar Sur
Researcher at Chalk River Laboratories
Publications - 72
Citations - 6298
Bhaskar Sur is an academic researcher from Chalk River Laboratories. The author has contributed to research in topics: Neutrino & Sudbury Neutrino Observatory. The author has an hindex of 16, co-authored 72 publications receiving 5849 citations. Previous affiliations of Bhaskar Sur include Atomic Energy of Canada Limited & Queen's University.
Papers
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Journal ArticleDOI
Direct evidence for neutrino flavor transformation from neutral current interactions in the Sudbury Neutrino Observatory
Q. R. Ahmad,R. C. Allen,T. C. Andersen,J. D. Anglin,J. C. Barton,E. W. Beier,M. Bercovitch,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,S. J. Brice,M. C. Browne,M. C. Browne,T. V. Bullard,G. Bühler,J. Cameron,Yuen-Dat Chan,Herbert H. Chen,M. L. Chen,Xin Chen,Xin Chen,B. T. Cleveland,E. T.H. Clifford,J. H.M. Cowan,D. F. Cowen,G. A. Cox,X. Dai,F. Dalnoki-Veress,W. F. Davidson,P. J. Doe,P. J. Doe,P. J. Doe,G. Doucas,M. R. Dragowsky,M. R. Dragowsky,C. A. Duba,F. A. Duncan,Monica Dunford,J. A. Dunmore,E. D. Earle,E. D. Earle,Steven Elliott,Steven Elliott,Hal Evans,G. T. Ewan,J. Farine,J. Farine,H. Fergani,A. P. Ferraris,R. J. Ford,Joseph A. Formaggio,M. M. Fowler,K. Frame,E.D. Frank,W. Frati,N. Gagnon,J. V. Germani,Salvador Gil,K. Graham,Darren Grant,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,R. Hazama,K. M. Heeger,W. J. Heintzelman,J. Heise,J. Heise,R. L. Helmer,R. L. Helmer,J. D. Hepburn,H. Heron,J. Hewett,Andrew Hime,M. A. Howe,J. G. Hykawy,M. C.P. Isaac,P. Jagam,N. A. Jelley,C. Jillings,G. Jonkmans,G. Jonkmans,K. Kazkaz,P. T. Keener,Joshua R. Klein,A. B. Knox,R. J. Komar,Richard T. Kouzes,T. Kutter,Christopher C. M. Kyba,J. Law,I. T. Lawson,M. Lay,H. W. Lee,K. T. Lesko,J. R. Leslie,I. Levine,W. Locke,S. Luoma,J. Lyon,S. Majerus,H. B. Mak,J. Maneira,J. Manor,A. D. Marino,N. McCauley,N. McCauley,A. B. McDonald,A. B. McDonald,D. S. McDonald,K. McFarlane,G. McGregor,R. Meijer Drees,C. Mifflin,G. G. Miller,G. Milton,B. A. Moffat,M. Moorhead,C. W. Nally,Mark Neubauer,F.M. Newcomer,H. S. Ng,A. J. Noble,A. J. Noble,Eric B. Norman,V. M. Novikov,M. O'Neill,C. E. Okada,R. W. Ollerhead,M. Omori,John L. Orrell,S. M. Oser,A. W. P. Poon,T. J. Radcliffe,A. Roberge,B. C. Robertson,R. G. H. Robertson,R. G. H. Robertson,S. S.E. Rosendahl,J. K. Rowley,V. L. Rusu,E. Saettler,K. K. Schaffer,M. H. Schwendener,Anett Schulke,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,T. Spreitzer,N. Starinsky,T. D. Steiger,R. G. Stokstad,L. C. Stonehill,R. S. Storey,Bhaskar Sur,Bhaskar Sur,Reda Tafirout,N. Tagg,N. Tagg,N. W. Tanner,R. K. Taplin,M. Thorman,P. M. Thornewell,P. T. Trent,Y. I. Tserkovnyak,R. Van Berg,R. G. Van de Water,R. G. Van de Water,C. J. Virtue,Chris Waltham,J. X. Wang,D. L. Wark,D. L. Wark,D. L. Wark,N. West,J. B. Wilhelmy,J. F. Wilkerson,J. F. Wilkerson,J. R. Wilson,Peter Wittich,J. M. Wouters,Minfang Yeh +205 more
TL;DR: Observations of neutral-current nu interactions on deuterium in the Sudbury Neutrino Observatory are reported, providing strong evidence for solar nu(e) flavor transformation.
Journal ArticleDOI
Measurement of the rate of ve + d → p + p + e- interactions produced by 8B solar neutrinos at the sudbury neutrino observatory
Q. R. Ahmad,R. C. Allen,T. C. Andersen,J. D. Anglin,G. Bühler,J. C. Barton,J. C. Barton,E. W. Beier,M. Bercovitch,J. Bigu,S. D. Biller,R. A. Black,I. Blevis,R. J. Bardman,J. Boger,E. Bonvin,Mark Guy Boulay,M. G. Bowler,T. J. Bowles,S. J. Brice,S. J. Brice,M. C. Browne,T. V. Bullard,T.H. Burritt,T.H. Burritt,K. Cameron,J. Cameron,Yuen-Dat Chan,M. L. Chen,Herbert H. Chen,Xin Chen,Xin Chen,M. C. Chon,B. T. Cleveland,E. T.H. Clifford,E. T.H. Clifford,J. H.M. Cowan,D. F. Cowen,G. A. Cox,Y. Dai,X. Dai,F. Dalnoki-Veress,W. F. Davidson,P. J. Doe,P. J. Doe,P. J. Doe,G. Doucas,M. R. Dragowsky,M. R. Dragowsky,C. A. Duba,F. A. Duncan,J. A. Dunmore,E. D. Earle,E. D. Earle,Steven Elliott,Steven Elliott,Hal Evans,G. T. Ewan,J. Farine,H. Fergani,A. P. Ferraris,R. J. Ford,M. M. Fowler,K. Frame,E.D. Frank,W. Frati,J. V. Germani,J. V. Germani,Salvador Gil,A. Goldschmidt,Darren Grant,R. L. Hahn,A. L. Hallin,E. D. Hallman,A. S. Hamer,A. S. Hamer,A. A. Hamian,R. U. Haq,C. K. Hargrove,P. J. Harvey,R. Hazama,R. Heaton,K. M. Heeger,W. J. Heintzelman,J. Heise,R. L. Helmer,R. L. Helmer,J. D. Hepburn,J. D. Hepburn,H. Heron,J. Hewett,Andrew Hime,M. A. Howe,J. G. Hykawy,M. C.P. Isaac,P. Jagam,N. A. Jelley,C. Jillings,G. Jonkmans,G. Jonkmans,J. Karn,P. T. Keener,Klaus Kirch,Joshua R. Klein,A. B. Knox,R. J. Komar,R. J. Komar,Richard T. Kouzes,T. Kutter,Christopher C. M. Kyba,J. Law,I. T. Lawson,M. Lay,H. W. Lee,K. T. Lesko,J. R. Leslie,I. Levine,W. Locke,M. M. Lowry,S. Luoma,J. Lyon,S. Majerus,H. B. Mak,A. D. Marino,N. McCauley,A. B. McDonald,A. B. McDonald,D. S. McDonald,K. McFarlane,G. McGregor,W. McLatchie,R. Meijer Drees,H. Mes,C. Mifflin,G. G. Miller,G. Milton,B. A. Moffat,M. Moorhead,M. Moorhead,C. W. Nally,Mark Neubauer,F.M. Newcomer,H. S. Ng,A. J. Noble,A. J. Noble,Eric B. Norman,V. M. Novikov,M. O'Neill,C. E. Okada,R. W. Ollerhead,M. Omori,John L. Orrell,S. M. Oser,A. W. P. Poon,T. J. Radcliffe,A. Roberge,B. C. Robertson,R. G. H. Robertson,R. G. H. Robertson,J. K. Rowley,V. L. Rusu,E. Saettler,K. K. Schaffer,A. Schuelke,M. H. Schwendener,H. Seifert,H. Seifert,H. Seifert,M. Shatkay,J. J. Simpson,David A. Sinclair,P. Skensved,Alan R. Smith,M. W.E. Smith,N. Starinsky,T. D. Steiger,R. G. Stokstad,R. S. Storey,Bhaskar Sur,Bhaskar Sur,Reda Tafirout,N. Tagg,N. W. Tanner,R. K. Taplin,M. Thorman,P. M. Thornewell,P. M. Thornewell,P. M. Thornewell,P. T. Trent,P. T. Trent,Y. I. Tserkovnyak,R. Van Berg,R. G. Van de Water,R. G. Van de Water,C. J. Virtue,Chris Waltham,J. X. Wang,D. L. Wark,N. West,J. B. Wilhelmy,J. F. Wilkerson,J. F. Wilkerson,J. R. Wilson,Peter Wittich,J. M. Wouters,Minfang Yeh +205 more
TL;DR: In this paper, the total flux of 8B neutrinos was determined to be (5.44±0.99)×106 cm−2 s−1, in close agreement with the predictions of solar models.
Journal ArticleDOI
Measurement of Day and Night Neutrino Energy Spectra at SNO and Constraints on Neutrino Mixing Parameters
Q. R. Ahmad,R. C. Allen,T. C. Andersen,J. D. Anglin,J. C. Barton,E. W. Beier,M. Bercovitch,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,S. J. Brice,M. C. Browne,M. C. Browne,T. V. Bullard,G. Bühler,J. Cameron,Yuen-Dat Chan,Herbert H. Chen,M. L. Chen,Xin Chen,Xin Chen,B. T. Cleveland,E. T.H. Clifford,J. H.M. Cowan,D. F. Cowen,G. A. Cox,X. Dai,F. Dalnoki-Veress,W. F. Davidson,P. J. Doe,P. J. Doe,P. J. Doe,G. Doucas,M. R. Dragowsky,M. R. Dragowsky,C. A. Duba,F. A. Duncan,Monica Dunford,J. A. Dunmore,E. D. Earle,E. D. Earle,Steven Elliott,Steven Elliott,Hal Evans,G. T. Ewan,J. Farine,J. Farine,H. Fergani,A. P. Ferraris,R. J. Ford,Joseph A. Formaggio,M. M. Fowler,K. Frame,E.D. Frank,W. Frati,N. Gagnon,J. V. Germani,Salvador Gil,K. Graham,Darren Grant,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,R. Hazama,K. M. Heeger,W. J. Heintzelman,J. Heise,J. Heise,R. L. Helmer,R. L. Helmer,J. D. Hepburn,H. Heron,J. Hewett,Andrew Hime,M. A. Howe,J. G. Hykawy,M. C.P. Isaac,P. Jagam,N. A. Jelley,C. Jillings,G. Jonkmans,G. Jonkmans,K. Kazkaz,P. T. Keener,Joshua R. Klein,A. B. Knox,R. J. Komar,Richard T. Kouzes,T. Kutter,Christopher C. M. Kyba,J. Law,I. T. Lawson,M. Lay,H. W. Lee,K. T. Lesko,J. R. Leslie,I. Levine,W. Locke,S. Luoma,J. Lyon,S. Majerus,H. B. Mak,J. Maneira,J. Manor,A. D. Marino,N. McCauley,N. McCauley,A. B. McDonald,A. B. McDonald,D. S. McDonald,K. McFarlane,G. McGregor,R. Meijer Drees,C. Mifflin,G. G. Miller,G. Milton,B. A. Moffat,M. Moorhead,C. W. Nally,Mark Neubauer,F.M. Newcomer,H. S. Ng,A. J. Noble,A. J. Noble,Eric B. Norman,V. M. Novikov,M. O'Neill,C. E. Okada,R. W. Ollerhead,M. Omori,John L. Orrell,S. M. Oser,A. W. P. Poon,T. J. Radcliffe,A. Roberge,B. C. Robertson,R. G. H. Robertson,R. G. H. Robertson,S. S.E. Rosendahl,J. K. Rowley,V. L. Rusu,E. Saettler,K. K. Schaffer,M. H. Schwendener,Anett Schulke,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,T. Spreitzer,N. Starinsky,T. D. Steiger,R. G. Stokstad,L. C. Stonehill,R. S. Storey,Bhaskar Sur,Bhaskar Sur,Reda Tafirout,N. Tagg,N. Tagg,N.W. Tanner,R. K. Taplin,M. Thorman,P. M. Thornewell,P. T. Trent,Y. I. Tserkovnyak,R. Van Berg,R. G. Van de Water,R. G. Van de Water,C. J. Virtue,Chris Waltham,J. X. Wang,D. L. Wark,D. L. Wark,D. L. Wark,N. West,J. B. Wilhelmy,J. F. Wilkerson,J. F. Wilkerson,J. R. Wilson,Peter Wittich,J. M. Wouters,Minfang Yeh +205 more
TL;DR: The Sudbury Neutrino Observatory (SNO) has measured day and night solar neutrino energy spectra and rates, and a global solar neutRino analysis in terms of matter-enhanced oscillations of two active flavors strongly favors the large mixing angle solution.
Journal ArticleDOI
Search for dark matter with a 231-day exposure of liquid argon using DEAP-3600 at SNOLAB
R. Ajaj,P. Amaudruz,G. R. Araujo,M. Baldwin,M. Batygov,B. Beltran,C. E. Bina,J. Bonatt,Mark Guy Boulay,B. Broerman,J. F. Bueno,P. M. Burghardt,A. Butcher,Bei Cai,Stefano Cavuoti,Min Chen,Y. Chen,B. T. Cleveland,D. Cranshaw,K. Dering,J. DiGioseffo,Luca Doria,F. A. Duncan,M. Dunford,A. Erlandson,N. Fatemighomi,G. Fiorillo,S. Florian,A. Flower,R. J. Ford,R. Gagnon,D. Gallacher,E. A. Garcés,S. Garg,P. Giampa,D. Goeldi,V. V. Golovko,P. Gorel,K. Graham,Darren Grant,A. L. Hallin,M. Hamstra,P. J. Harvey,C. Hearns,A. Joy,C. Jillings,O. Kamaev,G. Kaur,A. Kemp,I. Kochanek,M. Kuźniak,S. Langrock,F. La Zia,B. Lehnert,Xiujiang Li,J. Lidgard,T. Lindner,O. Litvinov,J. Lock,Giuseppe Longo,Peter Majewski,A. B. McDonald,T. McElroy,T. McGinn,J. B. McLaughlin,R. Mehdiyev,C. Mielnichuk,Jocelyn Monroe,P. Nadeau,C. M. Nantais,C. Ng,A. J. Noble,E. O'Dwyer,C. Ouellet,P. Pasuthip,S. J. M. Peeters,M. C. Piro,T. Pollmann,E. T. Rand,C. Rethmeier,F. Retiere,N. Seeburn,K. Singhrao,P. Skensved,B. C. Smith,N. J. T. Smith,T. Sonley,J. Soukup,R. Stainforth,C. Stone,V. Strickland,Bhaskar Sur,J. Tang,E. Vázquez-Jáuregui,Laurelle Maria Veloce,S. Viel,J. Walding,M. Waqar,Martin Ward,S. Westerdale,J. Willis,A. Zuñiga-Reyes +101 more
TL;DR: DEAP-3600 is a single-phase liquid argon (LAr) direct-detection dark matter experiment, operating 2 km underground at SNOLAB (Sudbury, Canada) as discussed by the authors.
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.