M. Lay
University of Oxford
9 Papers
128 Citations
M. Lay is an academic researcher from University of Oxford. The author has contributed to research in topics: Sudbury Neutrino Observatory & Neutrino. The author has an hindex of 7, co-authored 9 publications.
Chat about Author
Papers
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.
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.
2K
•Journal Article
Sudbury neutrino observatory
J. Boger,R. L. Hahn,J. K. Rowley,A.L. Carter,B. Hollebone,D. Kessler,I. Blevis,F. Dalnoki-Veress,A. Dekok,J. Farine,Darren Grant,C. K. Hargrove,G. Laberge,I. Levine,K. McFarlane,H. Mes,A.T. Noble,V. M. Novikov,M. O'Neill,M. Shatkay,C. Shewchuk,David A. Sinclair,E. T.H. Clifford,R. Deal,E. D. Earle,E. Gaudette,G. Milton,Bhaskar Sur,J. Bigu,J. H.M. Cowan,D.L. Cluff,E. D. Hallman,R. U. Haq,J. Hewett,J. G. Hykawy,G. Jonkmans,R. Michaud,A. Roberge,J. Roberts,E. Saettler,M. H. Schwendener,H. Seifert,D. Sweezey,Reda Tafirout,C. J. Virtue,D.N. Beck,Yuen-Dat Chan,Xin Chen,M. R. Dragowsky,F.W. Dycus,J. Gonzalez,M. C.P. Isaac,Y. Kajiyama,G.W. Koehler,K. T. Lesko,M.C. Moebus,Eric B. Norman,C. E. Okada,A. W. P. Poon,P. Purgalis,A. Schuelke,Alan R. Smith,R. G. Stokstad,S. Turner,I. Zlimen,J.M. Anaya,T. J. Bowles,S. J. Brice,E.I. Esch,Malcolm M. Fowler,A. Goldschmidt,Andrew Hime,A.F. McGirt,G. G. Miller,W.A. Teasdale,J. B. Wilhelmy,J. M. Wouters,J. D. Anglin,M. Bercovitch,W.F. Davidson,R. S. Storey,S. D. Biller,R. A. Black,R. J. Boardman,M. G. Bowler,J. Cameron,B. T. Cleveland,A. P. Ferraris,G. Doucas,H. Heron,C. Howard,N. A. Jelley,A. B. Knox,M. Lay,W. Locke,J. Lyon,S. Majerus,M. Moorhead,M. Omori +98 more
117
Direct Evidence for Neutrino Flavor Transformation from Neutral‐Current Interactions in SNO
A. B. McDonald,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. Bowler,T. J. Bowles,S. J. Brice,M. C. Browne,T. V. Bullard,G. Bühler,J. Cameron,Yuen-Dat Chan,Herbert H. Chen,Min Chen,X. 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,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,H. Fergani,A. P. Ferraris,R. J. Ford,Joseph A. Formaggio,Malcolm 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. A. Hamian,W. B. Handler,R. U. Haq,C. K. Hargrove,P. J. Harvey,Ryuta Hazama,K. M. Heeger,W. J. Heintzelman,John Heise,R. L. Helmer,J. D. Hepburn,H. Heron,J.L. Hewett,Andrew Hime,M. A. Howe,J. G. Hykawy,M. C.P. Isaac,P. Jagam,N. A. Jelley,C. Jillings,G. Jonkmans,K. Kazkaz,P. T. Keener,Jochen Klein,A. Knox,R. J. Komar,Richard T. Kouzes,T. Kutter,Christopher C. M. Kyba,J. Law,I. Lawson,M. Lay,H. W. Lee,K. T. Lesko,J. R. Leslie,Ilan Levine,W. Locke,S. Luoma,J. Lyon,S. Majerus,H. B. Mak,J. Maneira,J. Manor,A. D. Marino,N. McCauley,D. S. McDonald,K. McFarlane,G. McGregor,R. Meijer Drees,C. Mifflin,Guthrie Miller,G. Milton,B. A. Moffat,M. Moorhead,C. W. Nally,Mark Neubauer,F. M. Newcomer,H. S. Ng,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,S. S.E. Rosendahl,J. K. Rowley,V. L. Rusu,E. Saettler,K. K. Schaffer,M. H. Schwendener,Anett Schulke,H. Seifert,M. Shatkay,J. J. Simpson,C. J. Sims,David A. Sinclair,P. Skensved,A. R. Smith,M. W.E. Smith,T. Spreitzer,N. Starinsky,T. D. Steiger,R. G. Stokstad,L. C. Stonehill,R. S. Storey,Bhaskar Sur,Reda Tafirout,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,C. J. Virtue,Chris Waltham,J. X. Wang,D. L. Wark,N. West,J. B. Wilhelmy,J. F. Wilkerson,James R. Wilson,Peter Wittich,J. M. Wouters,Minfang Yeh +178 more
- 14 Nov 2002
TL;DR: The Sudbury Neutrino Observatory (SNO) is a 1,000 tonne heavy water Cerenkov-based neutrino detector situated 2,000 meters underground in INCO's Creighton Mine near Sudbury, Ontario, Canada.
14
Solar neutrino observations at the Sudbury Neutrino Observatory
A. W. P. Poon,Neubauer,M. Omori,T. C. Andersen,L. C. Stonehill,J. R. Leslie,Salvador Gil,M. Shatkay,M. Lay,J. V. Germani,H. B. Mak,H. Fergani,T. D. Steiger,E. Bonvin,J. Lyon,J. D. Hepburn,Monica Dunford,R. Ford,E.D. Frank,D. F. Cowen,J. Cameron,J. K. Rowley,V. L. Rusu,N. West,Eric B. Norman,Y. I. Tserkovnyak,M. O'Neill,C. W. Nally,C. E. Okada,C. Jillings,M. C.P. Isaac,H. S. Ng,Bhaskar Sur,J. Boger,A. D. Marino,B. C. Robertson,G. Milton,A. Hime,I. Lawson,S. S.E. Rosendahl,M. L. Chen,John L. Orrell,R. C. Allen,R. L. Hahn,G. G. Miller,M. M. Fowler,T. J. Radcliffe,Minfang Yeh,T. Kutter,Peter Wittich,J. Law,J. F. Wilkerson,W. J. Heintzelman,W. Frati,W. Locke,R. L. Helmer,P. T. Keener,K. Frame,M.G. Boulay,X. Dai,J. Maneira,M. W.E. Smith,K. McFarlane,E. T.H. Clifford,Joseph A. Formaggio,D. S. McDonald,N. A. Jelley,J. Hewett,J. Bigu,I. Blevis,R. Meijer Drees,J. A. Dunmore,K. K. Schaffer,J. Heise,J. Farine,Xin Chen,P. M. Thornewell,K. T. Lesko,N. McCauley,Steven Elliott,M. C. Browne,Y.D. Chan,J. B. Wilhelmy,R. S. Storey,C. Mifflin,A. Roberge,M. G. Bowler,M. Moorhead,H. W. Lee,A. A. Hamian,P. Jagam,R. J. Boardman,E. D. Earle,N. Gagnon,K. Kazkaz,B. A. Moffat,A. B. McDonald,W.F. Davidson,K. Graham,R. G. H. Robertson,T. V. Bullard,T.J. Bowles,B. T. Cleveland,R. W. Ollerhead,C. K. Hargrove,J. C. Barton,Christopher C. M. Kyba,M. Bercovitch,N.W. Tanner,J. Manor,S. Luoma,E. W. Beier,J. H.M. Cowan,Alan R. Smith,Anett Schulke,Hal Evans,J. G. Hykawy,Darren Grant,R. G. Stokstad,Richard T. Kouzes,G. T. Ewan,N. Tagg,A. Knox,T. Spreitzer,Reda Tafirout,R. A. Black,Richard George Van de Water,K. M. Heeger,P. J. Harvey,F.M. Newcomer,S. Majerus,Q. R. Ahmad,G. Bühler,G. Jonkmans,A. S. Hamer,R. K. Taplin,S. M. Oser,P. T. Trent,David A. Sinclair,Joshua R. Klein,J. X. Wang,I. Levine,E. D. Hallman,J.D. Anglin,Chris Waltham,S. D. Biller,H. Seifert,G. Doucas,A. L. Hallin,G. A. Cox,A. J. Noble,M. Thorman,J. J. Simpson,E. Saettler,Herbert H. Chen,P. J. Doe,G. McGregor,V. M. Novikov,R. Van Berg,C. J. Sims,R. U. Haq,H. Heron,M. H. Schwendener,C. J. Virtue,R. J. Komar,C. A. Duba,M. R. Dragowsky,J. M. Wouters,S. J. Brice,W. B. Handler,J. R. Wilson,P. Skensved,Ryuta Hazama,A. P. Ferraris,F. A. Duncan,N. Starinsky,D. L. Wark,F. Dalnoki-Veress +177 more
- 01 Jan 2002
TL;DR: The Sudbury Neutrino Observatory (SNO) is a 1000-tonne heavy water Cherenkov detector as discussed by the authors, which allows simultaneous measurements of the νe flux from B decay in the Sun and the total flux of all active neutrino species through the charged-current and the neutralcurrent interactions on the deuterons.
2