A
A. J. Noble
Researcher at Queen's University
Publications - 58
Citations - 3699
A. J. Noble is an academic researcher from Queen's University. The author has contributed to research in topics: Dark matter & Sudbury Neutrino Observatory. The author has an hindex of 24, co-authored 51 publications receiving 3467 citations. Previous affiliations of A. J. Noble include Carleton University & TRIUMF.
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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 ArticleDOI
Dark Matter Search Results from the PICO-2L C3F8 Bubble Chamber.
C. Amole,Miguel Ardid,David M. Asner,D. Baxter,E. Behnke,P. S. Bhattacharjee,H. Borsodi,M. Bou-Cabo,S. J. Brice,Daniel Broemmelsiek,K. Clark,J. I. Collar,P. S. Cooper,M. Crisler,C. E. Dahl,C. E. Dahl,S. Daley,Madhusmita Das,F. Debris,N. Dhungana,J. Farine,Ivan Felis,R. Filgas,M. Fines-Neuschild,Francoise Girard,G. Giroux,M. Hai,J. Hall,O. Harris,C. M. Jackson,M. Jin,C. B. Krauss,M. Lafrenière,M. Laurin,I. Lawson,I. Levine,W. H. Lippincott,E. Mann,J. P. Martin,Deepam Maurya,Pitam Mitra,R. Neilson,R. Neilson,A. J. Noble,A. Plante,R. B. Podviianiuk,Shashank Priya,A. E. Robinson,M. Ruschman,O. Scallon,O. Scallon,S. Seth,Andrew Sonnenschein,N. Starinski,I. Stekl,E. Vázquez-Jáuregui,E. Vázquez-Jáuregui,J. Wells,U. Wichoski,V. Zacek,Jie Zhang +60 more
TL;DR: These data provide the most sensitive direct detection constraints on WIMP-proton spin-dependent scattering to date, with significant sensitivity at low W IMP masses for spin-independent WIMp-nucleon scattering.
Journal ArticleDOI
Independent Measurement of the Total Active 8B Solar Neutrino Flux Using an Array of 3He Proportional Counters at the Sudbury Neutrino Observatory
B. Aharmim,S. N. Ahmed,J. F. Amsbaugh,A. E. Anthony,J. Banar,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. J. Bowles,M. C. Browne,M. C. Browne,T. V. Bullard,T.H. Burritt,Bei Cai,Yuen-Dat Chan,D. Chauhan,M. L. Chen,B. T. Cleveland,G. A. Cox-Mobrand,C. Currat,X. Dai,X. Dai,X. Dai,H. Deng,J. A. Detwiler,J. A. Detwiler,M. DiMarco,P. J. Doe,G. Doucas,P.-L. Drouin,C. A. Duba,F. A. Duncan,Monica Dunford,E. D. Earle,Steven Elliott,Steven Elliott,Hal Evans,G. T. Ewan,J. Farine,H. Fergani,F. Fleurot,R. J. Ford,Joseph A. Formaggio,Joseph A. Formaggio,Malcolm M. Fowler,N. Gagnon,J. V. Germani,J. V. Germani,A. Goldschmidt,J. T.M. Goon,K. Graham,K. Graham,E. Guillian,S. Habib,S. Habib,R. L. Hahn,A. L. Hallin,A. L. Hallin,E. D. Hallman,A. A. Hamian,G. C. Harper,P. J. Harvey,R. Hazama,K. M. Heeger,W. J. Heintzelman,J. Heise,J. Heise,J. Heise,R. L. Helmer,Reyco Henning,Andrew Hime,C. Howard,C. Howard,M. A. Howe,M. Huang,M. Huang,P. Jagam,B. Jamieson,N. A. Jelley,K. J. Keeter,Joshua R. Klein,L. L. Kormos,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,J. C. Loach,J. C. Loach,R. MacLellan,S. Majerus,H. B. Mak,J. Maneira,R. D. Martin,K. McBryde,N. McCauley,N. McCauley,A. B. McDonald,S. McGee,C. Mifflin,Guthrie Miller,M. L. Miller,Benjamin Monreal,Jocelyn Monroe,B. Morissette,A. W. Myers,Bernie G. Nickel,A. J. Noble,N. S. Oblath,H. M. O'Keeffe,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,Keith Rielage,B. C. Robertson,R. G. H. Robertson,E. Rollin,M. H. Schwendener,J. A. Secrest,S. R. Seibert,O. Simard,J. J. Simpson,L. Sinclair,P. Skensved,M. W.E. Smith,M. W.E. Smith,T. D. Steiger,L. C. Stonehill,L. C. Stonehill,G. Tešić,P. M. Thornewell,P. M. Thornewell,N. Tolich,N. Tolich,T. Tsui,C. D. Tunnell,T. D. Van Wechel,R. Van Berg,B.A. VanDevender,C. J. Virtue,T. J. Walker,B. L. Wall,D. Waller,H. Wan Chan Tseung,J. Wendland,N. West,J. B. Wilhelmy,J. F. Wilkerson,J. R. Wilson,J. M. Wouters,A. Wright,Minfang Yeh,F. Zhang,Kai Zuber +174 more
TL;DR: The Sudbury Neutrino Observatory (SNO) used an array of He3 proportional counters to measure the rate of neutral-current interactions in heavy water and precisely determined the total active (x) B8 solar neutrino flux as discussed by the authors.
Journal ArticleDOI
Constraints on Low-Mass WIMP Interactions on $^{19}F$ from PICASSO
S. Archambault,E. Behnke,Pijushpani Bhattacharjee,S. Bhattacharya,X. Dai,Mala Das,A. Davour,F. Debris,N. Dhungana,J. Farine,S. Gagnebin,G. Giroux,E. Grace,C. M. Jackson,A. Kamaha,C. B. Krauss,S. Kumaratunga,M. Lafrenière,M. Laurin,I. Lawson,L. Lessard,I. Levine,C. Levy,R. MacDonald,D. Marlisov,J. P. Martin,P. Mitra,A. J. Noble,M.-C. Piro,R. Podviyanuk,Stanislav Pospisil,Satyajit Saha,O. Scallon,S. Seth,N. Starinski,I. Stekl,U. Wichoski,T. Xie,V. Zacek +38 more
TL;DR: In this article, the PICASSO dark matter search experiment at SNOLAB was used to detect weakly interacting massive particles (WIMPs) with masses below 10 GeV/c 2.
Journal ArticleDOI
Low-energy-threshold analysis of the Phase I and Phase II data sets of the Sudbury Neutrino Observatory
B. Aharmim,L. C. Stonehill,L. C. Stonehill,J. R. Leslie,J. F. Wilkerson,H. Fergani,S. R. Seibert,S. R. Seibert,H. M. O'Keeffe,H. M. O'Keeffe,A. B. McDonald,B. L. Wall,Benjamin Monreal,Benjamin Monreal,Monica Dunford,Monica Dunford,R. J. Ford,D. L. Wark,D. L. Wark,J. Tm. Goon,T. J. Sonley,T. J. Sonley,O. Simard,C. B. Krauss,Andrew Hime,I. T. Lawson,Yuen-Dat Chan,M. Kos,D. Waller,C. D. Tunnell,R. L. Hahn,R. D. Martin,R. D. Martin,Minfang Yeh,T. Kutter,E. Guillian,J. Heise,W. J. Heintzelman,F. Zhang,A. E. Anthony,A. E. Anthony,R. L. Helmer,Mark Guy Boulay,X. Dai,X. Dai,X. Dai,J. Maneira,Joseph A. Formaggio,Joseph A. Formaggio,F. Fleurot,N. Barros,N. A. Jelley,M. Huang,M. Huang,B. C. Robertson,T.H. Burritt,J. Law,J. Farine,J. Farine,G. Tešić,K. T. Lesko,N. McCauley,N. McCauley,N. McCauley,B.A. VanDevender,Steven Elliott,Steven Elliott,A. Wright,M. L. Chen,K. J. Keeter,S. J. M. Peeters,S. J. M. Peeters,M. DiMarco,E. D. Earle,N. Gagnon,S. D. Reitzner,Kai Zuber,Kai Zuber,K. Graham,K. Graham,R. G. H. Robertson,B. Beltran,M. Bergevin,M. Bergevin,B. T. Cleveland,H. Deng,Alain Bellerive,C. Howard,B. Morissette,Christopher C. M. Kyba,J. C. Loach,J. C. Loach,C. Kraus,E. W. Beier,T. Tsui,G. Prior,G. Prior,R. A. Ott,Hal Evans,P.-L. Drouin,Jocelyn Monroe,G. T. Ewan,A. W. P. Poon,D. Chauhan,P. J. Harvey,R. MacLellan,S. McGee,G. D. Orebi Gann,G. D. Orebi Gann,S. Majerus,Bei Cai,Keith Rielage,Keith Rielage,S. M. Oser,N. West,B. Jamieson,Joshua R. Klein,Joshua R. Klein,I. Levine,I. Levine,L. L. Kormos,E. D. Hallman,David A. Sinclair,David A. Sinclair,S. Habib,S. D. Biller,Bernie G. Nickel,G. Doucas,A. L. Hallin,G. A. Cox,A. J. Noble,A. J. Noble,P. J. Doe,N. S. Oblath,Howe,R. Van Berg,J. A. Secrest,J. A. Secrest,M. H. Schwendener,C. J. Virtue,C. A. Duba,J. A. Detwiler,J.M. Wouters,J.M. Wouters,S. N. Ahmed,R. Hazama,R. Hazama,H. Wan Chan Tseung,H. Wan Chan Tseung,M. L. Miller,M. L. Miller,K. Boudjemline,J. R. Wilson,P. Skensved,H. B. Mak,F. A. Duncan,N. Tolich +156 more
TL;DR: In this paper, a joint analysis of Phase I and Phase II data from the Sudbury Neutrino Observatory is reported, where the total flux of active-flavor neutrinos from 8B decay in the Sun measured using the neutral current (NC) reaction, with no constraint on the 8B neutrino energy spectrum, is found to be FNC=5.5 MeV, the lowest analysis threshold yet achieved with water Cherenkov detector data.