M. R. Dragowsky
Los Alamos National Laboratory
21 Papers
400 Citations
M. R. Dragowsky is an academic researcher from Los Alamos National Laboratory. The author has contributed to research in topics: Sudbury Neutrino Observatory & Solar neutrino. The author has an hindex of 15, co-authored 21 publications. Previous affiliations of M. R. Dragowsky include Case Western Reserve University & Lawrence Berkeley National Laboratory.
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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
Search for weakly interacting massive particles with the first five-tower data from the cryogenic dark matter search at the soudan underground laboratory.
Z. Ahmed,D. S. Akerib,S. Arrenberg,M. J. Attisha,C. N. Bailey,Laura Baudis,D. A. Bauer,J. Beaty,P. L. Brink,T. Bruch,R. Bunker,S. Burke,Blas Cabrera,David O. Caldwell,Jodi Cooley,P. Cushman,F. DeJongh,M. R. Dragowsky,L. Duong,J. Emes,Enectali Figueroa-Feliciano,Jeffrey P. Filippini,Matthew Fritts,R. J. Gaitskell,Sunil Golwala,Darren Grant,J. Hall,R. Hennings-Yeomans,S. A. Hertel,Donald J. Holmgren,Martin E. Huber,R. Mahapatra,Vuk Mandic,Kevin A. McCarthy,N. Mirabolfathi,H. N. Nelson,L. Novak,R. W. Ogburn,M. Pyle,X. Qiu,E. J. Ramberg,W. Rau,A. Reisetter,Tarek Saab,Bernard Sadoulet,Bernard Sadoulet,J. Sander,R. Schmitt,R. W. Schnee,D. N. Seitz,B. Serfass,Adam Sirois,K. M. Sundqvist,M. Tarka,Astrid Tomada,G. Wang,S. J. Yellin,S. J. Yellin,J. Yoo,Betty A. Young +59 more
TL;DR: In this article, the authors report results from the Cryogenic Dark Matter Search at the Soudan Underground Laboratory (CDMS II) featuring the full complement of 30 detectors, and a blind analysis of data taken between October 2006 and July 2007 sets an upper limit on the weakly interacting massive particle (WIMP) nucleon spin-independent cross section of 6.6 x 10^(-44) cm^2.
529
•Posted Content
After LUX: The LZ Program
D.C. Malling,D. S. Akerib,Henrique Araujo,X. Bai,S. Bedikian,Ethan Bernard,A. Bernstein,A. W. Bradley,Sidney Cahn,M. C. Carmona-Benitez,D. Carr,J.J. Chapman,K. Clark,T. Classen,T. Coffey,A. Curioni,A. Currie,S. Dazeley,L. de Viveiros,M. R. Dragowsky,E. Druszkiewicz,C. H. Faham,S. Fiorucci,R. J. Gaitskell,K.R. Gibson,C. R. Hall,M. Hanhardt,B. Holbrook,M. Ihm,R.G. Jacobsen,L. Kastens,K. Kazkaz,Richard Lander,N.A. Larsen,C. Lee,David Leonard,K. T. Lesko,A. Lindote,M.I. Lopes,A. Lyashenko,P. Majewski,R. L. Mannino,Daniel McKinsey,Dongming Mei,J. Mock,M. Morii,A. St. J. Murphy,H. N. Nelson,F. Neves,James Nikkel,M. Pangilinan,P. Phelps,L. Reichhart,T. A. Shutt,C. Silva,W. Skulski,V. N. Solovov,P. Sorensen,J. Spaans,T.M. Stiegler,T. J. Sumner,Robert Svoboda,M. Sweany,Matthew Szydagis,J. Thomson,Mani Tripathi,J.R. Verbus,N. Walsh,R. C. Webb,J.T. White,M. Wlasenko,F.L.H. Wolfs,M. Woods,Chao Zhang +73 more
TL;DR: The LZ program consists of two stages of direct dark matter searches using liquid Xe detectors, the first stage will be a 1.5-3 tonne detector, while the last stage is a 20-tonne detector as mentioned in this paper, which will probe spin-independent interaction cross sections as low as 5E-49 cm2 for 100 GeV WIMPs.
155
•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
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