Tests of Lorentz invariance at the Sudbury Neutrino Observatory

B. Aharmim; S. N. Ahmed; A. E. Anthony; N. Barros; E. W. Beier; A. Bellerive; B. Beltran; M. Bergevin; S. D. Biller; E. Blucher; Richard Bonventre; K. Boudjemline; M.G. Boulay; B. Cai; E. J. Callaghan; J. Caravaca; Y. D. Chan; D. Chauhan; M. Chen; B. T. Cleveland; G. A. Cox; X. Dai; H. Deng; F. B. Descamps; J. A. Detwiler; P. J. Doe; G. Doucas; P.-L. Drouin; M. Dunford; S.R. Elliott; H. C. Evans; G. T. Ewan; J. Farine; H. Fergani; F. Fleurot; R. J. Ford; J. A. Formaggio; N. Gagnon; K. Gilje; J. Tm. Goon; K. Graham; E. Guillian; S. Habib; R. L. Hahn; A. L. Hallin; E. D. Hallman; P. J. Harvey; R. Hazama; W. J. Heintzelman; J. Heise; R. L. Helmer; A. Hime; C. Howard; M. Huang; P. Jagam; B. Jamieson; N.A. Jelley; M. Jerkins; C. Kéfélian; K. J. Keeter; J. R. Klein; L. L. Kormos; M. Kos; A. Krüger; C. Kraus; C. B. Krauss; T. Kutter; C. C. M. Kyba; K. Labe; B. J. Land; R. Lange; A. Latorre; J. Law; I. T. Lawson; K. T. Lesko; J. R. Leslie; I. Levine; J. C. Loach; R. MacLellan; S. Majerus; H. B. Mak; J. Maneira; R.D. Martin; A. Mastbaum; N. McCauley; A. B. McDonald; S. R. McGee; M. L. Miller; B. Monreal; J. Monroe; B. G. Nickel; A. J. Noble; H.M. O’Keeffe; N. Oblath; C. E. Okada; 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; K. Rielage; B. C. Robertson; R.G. Hamish Robertson; M. H. Schwendener; J. A. Secrest; S.R. Seibert; O. Simard; D. Sinclair; P. Skensved; T. J. Sonley; L. C. Stonehill; G. Tešić; N. Tolich; T. Tsui; R. Van Berg; B. A. VanDevender; C. J. Virtue; B. L. Wall; D. Waller; H. Wan Chan Tseung; D. L. Wark; J. Wendland; N. West; John F. Wilkerson; T. Winchester; J. R. Wilson; A. Wright; M. Yeh; F. Zhang; K. Zuber; SNO Collaboration;B. Aharmim;S. N. Ahmed;A. E. Anthony;N. Barros;E. W. Beier;A. Bellerive;B. Beltran;M. Bergevin;S. D. Biller;E. Blucher;Richard Bonventre;K. Boudjemline;M.G. Boulay;B. Cai;E. J. Callaghan;J. Caravaca;Y. D. Chan;D. Chauhan;M. Chen;B. T. Cleveland;G. A. Cox;X. Dai;H. Deng;F. B. Descamps;J. A. Detwiler;P. J. Doe;G. Doucas;P.-L. Drouin;M. Dunford;S.R. Elliott;H. C. Evans;G. T. Ewan;J. Farine;H. Fergani;F. Fleurot;R. J. Ford;J. A. Formaggio;N. Gagnon;K. Gilje;J. Tm. Goon;K. Graham;E. Guillian;S. Habib;R. L. Hahn;A. L. Hallin;E. D. Hallman;P. J. Harvey;R. Hazama;W. J. Heintzelman;J. Heise;R. L. Helmer;A. Hime;C. Howard;M. Huang;P. Jagam;B. Jamieson;N.A. Jelley;M. Jerkins;C. Kéfélian;K. J. Keeter;J. R. Klein;L. L. Kormos;M. Kos;A. Krüger;C. Kraus;C. B. Krauss;T. Kutter;C. C. M. Kyba;K. Labe;B. J. Land;R. Lange;A. Latorre;J. Law;I. T. Lawson;K. T. Lesko;J. R. Leslie;I. Levine;J. C. Loach;R. MacLellan;S. Majerus;H. B. Mak;J. Maneira;R.D. Martin;A. Mastbaum;N. McCauley;A. B. McDonald;S. R. McGee;M. L. Miller;B. Monreal;J. Monroe;B. G. Nickel;A. J. Noble;H.M. O’Keeffe;N. Oblath;C. E. Okada;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;K. Rielage;B. C. Robertson;R.G. Hamish Robertson;M. H. Schwendener;J. A. Secrest;S.R. Seibert;O. Simard;D. Sinclair;P. Skensved;T. J. Sonley;L. C. Stonehill;G. Tešić;N. Tolich;T. Tsui;R. Van Berg;B. A. VanDevender;C. J. Virtue;B. L. Wall;D. Waller;H. Wan Chan Tseung;D. L. Wark;J. Wendland;N. West;John F. Wilkerson;T. Winchester;J. R. Wilson;A. Wright;M. Yeh;F. Zhang;K. Zuber;SNO Collaboration;

doi:10.1103/physrevd.98.112013

Tests of Lorentz invariance at the Sudbury Neutrino Observatory

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ID: 115445

2018

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Experimental tests of Lorentz symmetry in systems of all types are critical for ensuring that the basic assumptions of physics are well founded. Data from all phases of the Sudbury Neutrino Observatory, a kiloton-scale heavy water Cherenkov detector, are analyzed for possible violations of Lorentz symmetry in the neutrino sector. Such violations would appear as one of eight possible signal types in the detector: six seasonal variations in the solar electron neutrino survival probability differing in energy and time dependence and two shape changes to the oscillated solar neutrino energy spectrum. No evidence for such signals is observed, and limits on the size of such effects are established in the framework of the standard model extension, including 38 limits on previously unconstrained operators and improved limits on 16 additional operators. This makes limits on all minimal, Dirac-type Lorentz violating operators in the neutrino sector available for the first time.

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Autores	B. Aharmim,S. N. Ahmed,A. E. Anthony,N. Barros,E. W. Beier,A. Bellerive,B. Beltran,M. Bergevin,S. D. Biller,E. Blucher,Richard Bonventre,K. Boudjemline,M.G. Boulay,B. Cai,E. J. Callaghan,J. Caravaca,Y. D. Chan,D. Chauhan,M. Chen,B. T. Cleveland,G. A. Cox,X. Dai,H. Deng,F. B. Descamps,J. A. Detwiler,P. J. Doe,G. Doucas,P.-L. Drouin,M. Dunford,S.R. Elliott,H. C. Evans,G. T. Ewan,J. Farine,H. Fergani,F. Fleurot,R. J. Ford,J. A. Formaggio,N. Gagnon,K. Gilje,J. Tm. Goon,K. Graham,E. Guillian,S. Habib,R. L. Hahn,A. L. Hallin,E. D. Hallman,P. J. Harvey,R. Hazama,W. J. Heintzelman,J. Heise,R. L. Helmer,A. Hime,C. Howard,M. Huang,P. Jagam,B. Jamieson,N.A. Jelley,M. Jerkins,C. Kéfélian,K. J. Keeter,J. R. Klein,L. L. Kormos,M. Kos,A. Krüger,C. Kraus,C. B. Krauss,T. Kutter,C. C. M. Kyba,K. Labe,B. J. Land,R. Lange,A. Latorre,J. Law,I. T. Lawson,K. T. Lesko,J. R. Leslie,I. Levine,J. C. Loach,R. MacLellan,S. Majerus,H. B. Mak,J. Maneira,R.D. Martin,A. Mastbaum,N. McCauley,A. B. McDonald,S. R. McGee,M. L. Miller,B. Monreal,J. Monroe,B. G. Nickel,A. J. Noble,H.M. O’Keeffe,N. Oblath,C. E. Okada,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,K. Rielage,B. C. Robertson,R.G. Hamish Robertson,M. H. Schwendener,J. A. Secrest,S.R. Seibert,O. Simard,D. Sinclair,P. Skensved,T. J. Sonley,L. C. Stonehill,G. Tešić,N. Tolich,T. Tsui,R. Van Berg,B. A. VanDevender,C. J. Virtue,B. L. Wall,D. Waller,H. Wan Chan Tseung,D. L. Wark,J. Wendland,N. West,John F. Wilkerson,T. Winchester,J. R. Wilson,A. Wright,M. Yeh,F. Zhang,K. Zuber,SNO Collaboration;B. Aharmim;S. N. Ahmed;A. E. Anthony;N. Barros;E. W. Beier;A. Bellerive;B. Beltran;M. Bergevin;S. D. Biller;E. Blucher;Richard Bonventre;K. Boudjemline;M.G. Boulay;B. Cai;E. J. Callaghan;J. Caravaca;Y. D. Chan;D. Chauhan;M. Chen;B. T. Cleveland;G. A. Cox;X. Dai;H. Deng;F. B. Descamps;J. A. Detwiler;P. J. Doe;G. Doucas;P.-L. Drouin;M. Dunford;S.R. Elliott;H. C. Evans;G. T. Ewan;J. Farine;H. Fergani;F. Fleurot;R. J. Ford;J. A. Formaggio;N. Gagnon;K. Gilje;J. Tm. Goon;K. Graham;E. Guillian;S. Habib;R. L. Hahn;A. L. Hallin;E. D. Hallman;P. J. Harvey;R. Hazama;W. J. Heintzelman;J. Heise;R. L. Helmer;A. Hime;C. Howard;M. Huang;P. Jagam;B. Jamieson;N.A. Jelley;M. Jerkins;C. Kéfélian;K. J. Keeter;J. R. Klein;L. L. Kormos;M. Kos;A. Krüger;C. Kraus;C. B. Krauss;T. Kutter;C. C. M. Kyba;K. Labe;B. J. Land;R. Lange;A. Latorre;J. Law;I. T. Lawson;K. T. Lesko;J. R. Leslie;I. Levine;J. C. Loach;R. MacLellan;S. Majerus;H. B. Mak;J. Maneira;R.D. Martin;A. Mastbaum;N. McCauley;A. B. McDonald;S. R. McGee;M. L. Miller;B. Monreal;J. Monroe;B. G. Nickel;A. J. Noble;H.M. O’Keeffe;N. Oblath;C. E. Okada;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;K. Rielage;B. C. Robertson;R.G. Hamish Robertson;M. H. Schwendener;J. A. Secrest;S.R. Seibert;O. Simard;D. Sinclair;P. Skensved;T. J. Sonley;L. C. Stonehill;G. Tešić;N. Tolich;T. Tsui;R. Van Berg;B. A. VanDevender;C. J. Virtue;B. L. Wall;D. Waller;H. Wan Chan Tseung;D. L. Wark;J. Wendland;N. West;John F. Wilkerson;T. Winchester;J. R. Wilson;A. Wright;M. Yeh;F. Zhang;K. Zuber;SNO Collaboration;
Revista	physical review d
Ano	2018
DOI	10.1103/physrevd.98.112013 Buscando DOI...
URL	https://sciprofiles.com/publication/view/ee6382cbd9d53bbf608286190833d96b https://doi.org/10.1103/physrevd.98.112013
Palabras Clave	model survival solar neutrino detector observatory sudbury lorentz symmetry

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