D
D.C. Malling
Researcher at Brown University
Publications - 39
Citations - 4459
D.C. Malling is an academic researcher from Brown University. The author has contributed to research in topics: Dark matter & Large Underground Xenon experiment. The author has an hindex of 19, co-authored 37 publications receiving 4065 citations.
Papers
More filters
Journal ArticleDOI
First results from the LUX dark matter experiment at the Sanford Underground Research Facility
D. S. Akerib,Henrique Araujo,X. Bai,A. J. Bailey,J. Balajthy,S. Bedikian,Ethan Bernard,A. Bernstein,Alexander Bolozdynya,A. W. Bradley,D. Byram,Sidney Cahn,M. C. Carmona-Benitez,C. Chan,J.J. Chapman,A. A. Chiller,C. Chiller,K. Clark,T. Coffey,A. Currie,A. Curioni,Steven Dazeley,L. de Viveiros,A. Dobi,J. E. Y. Dobson,E. M. Dragowsky,E. Druszkiewicz,B. N. Edwards,C. H. Faham,S. Fiorucci,C. E. Flores,R. J. Gaitskell,V. M. Gehman,C. Ghag,K.R. Gibson,Murdock Gilchriese,C. R. Hall,M. Hanhardt,S. A. Hertel,M. Horn,D. Q. Huang,M. Ihm,R. G. Jacobsen,L. Kastens,K. Kazkaz,R. Knoche,S. Kyre,R. L. Lander,N. A. Larsen,C. Lee,David Leonard,K. T. Lesko,A. Lindote,M.I. Lopes,A. Lyashenko,D.C. Malling,R. L. Mannino,Daniel McKinsey,Dongming Mei,J. Mock,M. Moongweluwan,J. A. Morad,M. Morii,A. St. J. Murphy,C. Nehrkorn,H. N. Nelson,F. Neves,James Nikkel,R. A. Ott,M. Pangilinan,P. D. Parker,E. K. Pease,K. Pech,P. Phelps,L. Reichhart,T. A. Shutt,C. Silva,W. Skulski,C. Sofka,V. N. Solovov,P. Sorensen,T.M. Stiegler,K. O'Sullivan,T. J. Sumner,Robert Svoboda,M. Sweany,Matthew Szydagis,D. J. Taylor,B. P. Tennyson,D. R. Tiedt,Mani Tripathi,S. Uvarov,J.R. Verbus,N. Walsh,R. C. Webb,J. T. White,D. White,M. S. Witherell,M. Wlasenko,F.L.H. Wolfs,M. Woods,Chao Zhang +101 more
TL;DR: The first WIMP search data set is reported, taken during the period from April to August 2013, presenting the analysis of 85.3 live days of data, finding that the LUX data are in disagreement with low-mass W IMP signal interpretations of the results from several recent direct detection experiments.
Journal ArticleDOI
Improved limits on scattering of weakly interacting massive particles from reanalysis of 2013 LUX data
D. S. Akerib,Henrique Araujo,X. Bai,A. J. Bailey,J. Balajthy,P. Beltrame,Ethan Bernard,A. Bernstein,T. P. Biesiadzinski,E. M. Boulton,A. W. Bradley,R. Bramante,Sidney Cahn,M. C. Carmona-Benitez,C. Chan,J.J. Chapman,A.A. Chiller,C. Chiller,A. Currie,J. E. Cutter,T. J. R. Davison,L. de Viveiros,A. Dobi,J. E. Y. Dobson,E. Druszkiewicz,B. N. Edwards,C. H. Faham,S. Fiorucci,R. J. Gaitskell,V. M. Gehman,C. Ghag,K.R. Gibson,M. G. D. Gilchriese,C. R. Hall,M. Hanhardt,S. J. Haselschwardt,S. A. Hertel,D. P. Hogan,M. Horn,D. Q. Huang,C. M. Ignarra,M. Ihm,R.G. Jacobsen,W. Ji,K. Kazkaz,D. Khaitan,R. Knoche,N.A. Larsen,C. Lee,B. G. Lenardo,K. T. Lesko,A. Lindote,M.I. Lopes,D.C. Malling,A. Manalaysay,R. L. Mannino,M. F. Marzioni,Daniel McKinsey,D. M. Mei,J. Mock,M. Moongweluwan,J. A. Morad,A. St. J. Murphy,C. Nehrkorn,H. N. Nelson,F. Neves,K. O'Sullivan,K. C. Oliver-Mallory,R. A. Ott,K. J. Palladino,M. Pangilinan,E. K. Pease,P. Phelps,L. Reichhart,C. Rhyne,S. Shaw,T. A. Shutt,C. Silva,V. N. Solovov,P. Sorensen,S. Stephenson,T. J. Sumner,Matthew Szydagis,D. J. Taylor,W. C. Taylor,B. P. Tennyson,P. A. Terman,D. R. Tiedt,W. H. To,Mani Tripathi,L. Tvrznikova,S. Uvarov,J.R. Verbus,R. C. Webb,J. T. White,T. J. Whitis,M. S. Witherell,F.L.H. Wolfs,K. Yazdani,Sarah Young,Chao Zhang +100 more
TL;DR: This new analysis incorporates several advances: single-photon calibration at the scintillation wavelength, improved event-reconstruction algorithms, a revised background model including events originating on the detector walls in an enlarged fiducial volume, and new calibrations from decays of an injected tritium β source and from kinematically constrained nuclear recoils down to 1.1 keV.
Journal ArticleDOI
The Large Underground Xenon (LUX) experiment
D. S. Akerib,X. Bai,S. Bedikian,Ethan Bernard,A. Bernstein,Alexander Bolozdynya,A. W. Bradley,D. Byram,Sidney Cahn,C. Camp,M. C. Carmona-Benitez,D. Carr,J.J. Chapman,A. A. Chiller,C. Chiller,K. Clark,T. Classen,T. Coffey,A. Curioni,E. Dahl,S. Dazeley,L. de Viveiros,A. Dobi,E. M. Dragowsky,E. Druszkiewicz,B. N. Edwards,C.H. Faham,S. Fiorucci,R. J. Gaitskell,K.R. Gibson,Murdock Gilchriese,C. R. Hall,M. Hanhardt,B. Holbrook,M. Ihm,R. G. Jacobsen,L. Kastens,K. Kazkaz,R. Knoche,S. Kyre,J. Kwong,R. L. Lander,N. A. Larsen,C. Lee,David Leonard,K. T. Lesko,A. Lindote,M.I. Lopes,A. Lyashenko,D.C. Malling,R. L. Mannino,Z. Marquez,Daniel McKinsey,Dongming Mei,J. Mock,M. Moongweluwan,M. Morii,H. N. Nelson,F. Neves,James Nikkel,M. Pangilinan,P.D. Parker,E. K. Pease,K. Pech,P. Phelps,A. Rodionov,P. Roberts,Alexander Shei,T. A. Shutt,C. Silva,W. Skulski,V. N. Solovov,C. Sofka,P. Sorensen,J. Spaans,T.M. Stiegler,D. Stolp,Robert Svoboda,M. Sweany,Matthew Szydagis,D. J. Taylor,J. Thomson,Mani Tripathi,S. Uvarov,J.R. Verbus,N. Walsh,R. C. Webb,D. White,J. T. White,T. J. Whitis,M. Wlasenko,F.L.H. Wolfs,M. Woods,Chao Zhang +93 more
TL;DR: The Large Underground Xenon (LUX) detector as mentioned in this paper is a dual-phase Xenon detector with a spin independent cross-section per nucleon of 2 × 10 − 46 cm 2, equivalent to ∼ 1 event / 100 kg / month in the inner 100-kg fiducial volume (FV) of the 370-kg detector.
ReportDOI
LUX-ZEPLIN (LZ) Conceptual Design Report
D. S. Akerib,D. S. Akerib,R. M. Preece,V. Bugaev,T. K. Edberg,Hoff,Patrick Bauer,A. Currie,J. Mock,D. White,V. M. Gehman,S. D. Worm,M. F. Marzioni,D. Markley,C. M. Ignarra,E. M. Boulton,Sergey Burdin,Bhawna Gomber,C. E. Dahl,E. Druszkiewicz,Eli Woods,S. A. Hertel,Daniel McKinsey,P.R. Scovell,T.W. Hurteau,Olevitch,T. A. Shutt,T. J. R. Davison,K. C. Oliver-Mallory,P. Ford,B. Holbrook,C. Ghag,K. Sundarnath,B. N. Edwards,A. Khazov,R.M. Gerhard,J.S. Saba,M. Elnimr,A.A. Chiller,S. Balashov,Wolfgang Lorenzon,L. Reichhart,J. Busenitz,Carl W. Akerlof,V. B. Francis,A. Konovalov,Matthew Szydagis,Mikkel B. Johnson,J. Reichenbacher,H. Kraus,Wenzhao Wei,Laura Manenti,M. Cascella,D. Woodward,Minfang Yeh,C. Carels,S. Luitz,Witherell,W. Skulski,Sridhara Dasu,X. Ji,W. T. Emmet,N.J. Gantos,J. E. Cutter,A. Tomás,K. O'Sullivan,F. G. O'Neill,J. E. Y. Dobson,J. Thomson,J. H. Buckley,K.J. Thomas,I. Stancu,M.J. Barry,T.J. Martin,A. Lindote,M. E. Monzani,R. Bunker,K. T. Lesko,Chao Zhang,Mani Tripathi,S. J. Haselschwardt,L. Tvrznikova,P. A. Terman,Duncan Carlsmith,M. R. While,D. Khaitan,R.G. Jacobsen,J. O'Dell,A. Harris,E. K. Pease,J. Va’vra,J. Lin,K. Skarpaas,Elena Korolkova,S.K. Young,W. Craddock,T. J. Whitis,B. N. Ratcliff,M. C. Carmona-Benitez,J. Liu,R. J. Gaitskell,C. Chiller,H.J. Krebs,K. Kazkaz,N.A. Larsen,R. Bramante,M. G. D. van der Grinten,Richard Rosero,C. R. Hall,E. Holtom,C. Lee,C. O. Vuosalo,V. N. Solovov,C. Rhyne,T. J. Sumner,S. Powell,P. Beltrame,R. C. Webb,M. G. D. Gilchriese,C. Fu,J. A. Morad,S. Kyre,D. R. Tiedt,L. de Viveiros,B. P. Tennyson,D. Q. Huang,C. Silva,A. Bernstein,T. P. Biesiadzinski,J. Balajthy,J.P. Rodrigues,S. J. Patton,M.R. Stark,F.-T. Liao,S. Stephenson,W. H. Lippincott,Yue Meng,K. Pushkin,L. Wang,Michael Schubnell,X. Bai,K. J. Palladino,D.Yu. Akimov,W. H. To,A. V. Kumpan,Alexander Bolozdynya,A. St. J. Murphy,A. Dobi,D. J. Taylor,A.V. Khromov,Ethan Bernard,K. E. Boast,D.C. Malling,P. Sorensen,Peter Majewski,F. Neves,F.L.H. Wolfs,V.V. Sosnovtsev,A. J. Bailey,H. N. Nelson,S. Shaw,J. J. Cherwinka,M.I. Lopes,X. Liu,E. H. Miller,C. Chan,V. A. Kudryavtsev,J.R. Verbus,R. L. Mannino,Dongming Mei,C. H. Faham,S. Uvarov,T.M. Stiegler,R. W. Schnee,M. Pangilinan,Henrique Araujo,S. Alsum,W. J. Wisniewski,H. J. Rose,K. Kamdin,M. Sarychev,A. Manalaysay,W. Ji,J. Yin,W. C. Taylor,W. R. Edwards,J.P. da Cunha,Y. Ju,A. Piepke,W.L. Waldron,C. E. Tull,B. G. Lenardo,Ben Carlson,S. Fiorucci,James Nikkel +194 more
TL;DR: The design and performance of the LUX-ZEPLIN (LZ) detector is described as of March 2015 in this Conceptual Design Report as mentioned in this paper. And the LZ detector will be located at the Sanford Underground Research Facility in South Dakota.
Journal ArticleDOI
Results on the Spin-Dependent Scattering of Weakly Interacting Massive Particles on Nucleons from the Run 3 Data of the LUX Experiment.
D. S. Akerib,Henrique Araujo,X. Bai,A. J. Bailey,J. Balajthy,P. Beltrame,Ethan Bernard,A. Bernstein,T. P. Biesiadzinski,E. M. Boulton,A. W. Bradley,R. Bramante,Sidney Cahn,M. C. Carmona-Benitez,C. Chan,J.J. Chapman,A.A. Chiller,C. Chiller,A. Currie,J. E. Cutter,T. J. R. Davison,L. de Viveiros,A. Dobi,J. E. Y. Dobson,E. Druszkiewicz,B. N. Edwards,C. H. Faham,S. Fiorucci,R. J. Gaitskell,V. M. Gehman,C. Ghag,K.R. Gibson,M. G. D. Gilchriese,C. R. Hall,M. Hanhardt,S. J. Haselschwardt,S. A. Hertel,D. P. Hogan,M. Horn,D. Q. Huang,C. M. Ignarra,M. Ihm,R.G. Jacobsen,W. Ji,K. Kazkaz,D. Khaitan,R. Knoche,N.A. Larsen,C. Lee,B. G. Lenardo,K. T. Lesko,A. Lindote,M.I. Lopes,D.C. Malling,A. Manalaysay,R. L. Mannino,M. F. Marzioni,Daniel McKinsey,D. M. Mei,J. Mock,M. Moongweluwan,J. A. Morad,A. St. J. Murphy,C. Nehrkorn,H. N. Nelson,F. Neves,K. O'Sullivan,K. C. Oliver-Mallory,R. A. Ott,K. J. Palladino,M. Pangilinan,E. K. Pease,P. Phelps,L. Reichhart,C. Rhyne,S. Shaw,T. A. Shutt,C. Silva,V. N. Solovov,P. Sorensen,S. Stephenson,T. J. Sumner,Matthew Szydagis,D. J. Taylor,W. C. Taylor,B. P. Tennyson,P. A. Terman,D. R. Tiedt,W. H. To,Mani Tripathi,L. Tvrznikova,S. Uvarov,J.R. Verbus,R. C. Webb,J. T. White,T. J. Whitis,Michael S. Witherell,F.L.H. Wolfs,K. Yazdani,Sarah Young,Chao Zhang +100 more
TL;DR: The spin-dependent WIMP-neutron limit is the most sensitive constraint to date.