Measurement of Day and Night Neutrino Energy Spectra at SNO and Constraints on Neutrino Mixing Parameters

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ID: 267946
2002
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Abstract
The Sudbury Neutrino Observatory (SNO) has measured day and night solar neutrino energy spectra and rates. For charged current events, assuming an undistorted 8B spectrum, the night minus day rate is 14.0%±6.3%−1.4+1.5% of the average rate. If the total flux of active neutrinos is additionally constrained to have no asymmetry, the νe asymmetry is found to be 7.0%±4.9%−1.2+1.3%. A global solar neutrino analysis in terms of matter-enhanced oscillations of two active flavors strongly favors the large mixing angle solution.
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Authors Q. R. Ahmad,R. C. Allen,Thomas 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,Y. D. Chan,H. H. Chen,M. Chen,X. Chen,B. T. Cleveland,E. T. H. Clifford,J. H. M. Cowan,D. F. Cowen,G. A. Cox,X. Dai,Ferenc (Jacob Rolf) Dalnoki-Veress,W. F. Davidson,P. J. Doe,G. Doucas,M. R. Dragowsky,C. A. Duba,F. A. Duncan,M. Dunford,J. A. Dunmore,E. D. Earle,S. R. Elliott,H. C. Evans,G. T. Ewan,J. Farine,H. Fergani,A. P. Ferraris,R. J. Ford,J. A. Formaggio,M. M. Fowler,K. Frame,E. D. Frank,W. Frati,N. Gagnon,J. V. Germani,S. Gil,K. Graham,D. R. 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,R. Hazama,K. M. Heeger,W. J. Heintzelman,J. Heise,R. L. Helmer,J. D. Hepburn,H. Heron,J. Hewett,A. Hime,M. Howe,J. G. Hykawy,M. C. P. Isaac,Formaggio Ja,N. A. Jelley,C. Jillings,G. Jonkmans,K. Kazkaz,P. T. Keener,J. R. Klein,A. B. Knox,R. J. Komar,R. Kouzes,T. Kutter,Christopher 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,Jose Maneira,J. Manor,A. D. Marino,N. McCauley,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,M. S. Neubauer,F. M. Newcomer,H. S. Ng,A. J. Noble,E. B. Norman,V. M. Novikov,M. O'neill,C. E. Okada,R. W. Ollerhead,M. Omori,John 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,A. Schülke,H. Seifert,M. Shatkay,J. J. Simpson,Neubauer Ms,D. 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,B. Sur,R. 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,C. E. Waltham,J.-X. Wang,D. L. Wark,N. West,J. B. Wilhelmy,J. F. Wilkerson,Jeanne Wilson,P. Wittich,J. M. Wouters,Minfang Yeh;Q. R. Ahmad;R. C. Allen;Thomas 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;Y. D. Chan;H. H. Chen;M. Chen;X. Chen;B. T. Cleveland;E. T. H. Clifford;J. H. M. Cowan;D. F. Cowen;G. A. Cox;X. Dai;Ferenc (Jacob Rolf) Dalnoki-Veress;W. F. Davidson;P. J. Doe;G. Doucas;M. R. Dragowsky;C. A. Duba;F. A. Duncan;M. Dunford;J. A. Dunmore;E. D. Earle;S. R. Elliott;H. C. Evans;G. T. Ewan;J. Farine;H. Fergani;A. P. Ferraris;R. J. Ford;J. A. Formaggio;M. M. Fowler;K. Frame;E. D. Frank;W. Frati;N. Gagnon;J. V. Germani;S. Gil;K. Graham;D. R. 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;R. Hazama;K. M. Heeger;W. J. Heintzelman;J. Heise;R. L. Helmer;J. D. Hepburn;H. Heron;J. Hewett;A. Hime;M. Howe;J. G. Hykawy;M. C. P. Isaac;Formaggio Ja;N. A. Jelley;C. Jillings;G. Jonkmans;K. Kazkaz;P. T. Keener;J. R. Klein;A. B. Knox;R. J. Komar;R. Kouzes;T. Kutter;Christopher 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;Jose Maneira;J. Manor;A. D. Marino;N. McCauley;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;M. S. Neubauer;F. M. Newcomer;H. S. Ng;A. J. Noble;E. B. Norman;V. M. Novikov;M. O'neill;C. E. Okada;R. W. Ollerhead;M. Omori;John 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;A. Schülke;H. Seifert;M. Shatkay;J. J. Simpson;Neubauer Ms;D. 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;B. Sur;R. 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;C. E. Waltham;J.-X. Wang;D. L. Wark;N. West;J. B. Wilhelmy;J. F. Wilkerson;Jeanne Wilson;P. Wittich;J. M. Wouters;Minfang Yeh;
Journal physical review letters
Year 2002
DOI
10.1103/physrevlett.89.011302
URL
https://sciprofiles.com/publication/view/8cd27a643d28eff62d0df12f1670a25e
Keywords
solar energy oscillations spectrum solar neutrinos particle physics cosmic ray nuclear astrophysics

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