9 Papers
30 Citations
E. Dahl is an academic researcher from Case Western Reserve University. The author has contributed to research in topics: Dark matter & Large Underground Xenon experiment. The author has an hindex of 4, co-authored 8 publications.
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Papers
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.
Status of the LUX dark matter search
S. Fiorucci,D. S. Akerib,S. Bedikian,A. Bernstein,Alexander Bolozdynya,A. W. Bradley,D. Carr,J.J. Chapman,K. Clark,T. Classen,A. Curioni,E. Dahl,S. Dazeley,L. de Viveiros,E. Druszkiewicz,R. J. Gaitskell,C. R. Hall,C. Hernandez Faham,B. Holbrook,L. Kastens,Kareem Kazkaz,Richard Lander,K. T. Lesko,D.C. Malling,R. L. Mannino,Daniel McKinsey,Dongming Mei,J. Mock,James Nikkel,P. Phelps,U. Schroeder,T. A. Shutt,W. Skulski,P. Sorensen,J. Spaans,T.M. Stiegler,Robert Svoboda,M. Sweany,J. Thomson,Jan Toke,Mani Tripathi,N. Walsh,R. C. Webb,J.T. White,F.L.H. Wolfs,M. Woods,Chao Zhang +46 more
- 05 Mar 2010
TL;DR: The Large Underground Xenon (LUX) dark matter search experiment is currently being deployed at the Homestake Laboratory in South Dakota as discussed by the authors, and the main elements of design which make the experiment a very strong competitor in the field of direct detection, as well as an easily scalable concept.
3D Position Sensitive XeTPC for Dark Matter Search
J. Angle,Elena Aprile,F. Arneodo,Laura Baudis,A. Bernstein,Alexander Bolozdynya,Luis Coelho,E. Dahl,L. DeViveiros,A. D. Ferella,L.M.P. Fernandes,S. Fiorucci,R. J. Gaitskell,K. L. Giboni,R. Gomez,R. Hasty,J. Kwong,J. A. M. Lopes,N. Madden,A. Manalaysay,A. Manzur,Daniel McKinsey,M. E. Monzani,Kaixuan Ni,Uwe Oberlack,J. Orboeck,G. Plante,Joaquim M. F. dos Santos,P. Shagin,T. A. Shutt,P. Sorensen,C. Winant,Masaki Yamashita +32 more
- 01 Nov 2007
TL;DR: In this paper, the technique to realize 3D position sensitivity in a two-phase Xenon time projection chamber (XeTPC) is described, and a prototype detector (XENON3) is presented.
3D Position Sensitive XeTPC for Dark Matter Search
J. Angle,Elena Aprile,F. Arneodo,Laura Baudis,A. Bernstein,Alexander Bolozdynya,Luis Coelho,E. Dahl,L. DeViveiros,A. D. Ferella,L.M.P. Fernandes,S. Fiorucci,R. J. Gaitskell,K. L. Giboni,R. Gomez,R. Hasty,J. Kwong,J. A. M. Lopes,N. Madden,A. Manalaysay,A. Manzur,Daniel McKinsey,M. E. Monzani,Kaixuan Ni,Uwe Oberlack,J. Orboeck,G. Plante,Joaquim M. F. dos Santos,P. Shagin,T. A. Shutt,P. Sorensen,C. Winant,Masaki Yamashita +32 more
TL;DR: In this article, the technique to realize 3D position sensitivity in a two-phase Xenon time projection chamber (XeTPC) for dark matter search is described, and results from a prototype detector (XENON3) are presented.
A search for weakly interacting dark matter with the LUX experiment
C. R. Hall,D. S. Akerib,X. Bai,S. Bedikian,Adam Bernstein,Alexander Bolozdynya,A. W. Bradley,Sidney Cahn,D. Carr,J.J. Chapman,K. Clark,T. Classen,A. Curioni,E. Dahl,Steven Dazeley,L. de Viveiros,M. R. Dragowsky,E. Druszkiewicz,C.H. Faham,S. Fiorucci,R. J. Gaitskell,M. Hanhardt,B. Holbrook,L. Kastens,Kareem Kazkaz,R. L. Lander,C. Lee,David Leonard,K. T. Lesko,A. Lyashenko,D.C. Malling,R. L. Mannino,Daniel McKinsey,Dongming Mei,J. Mock,M. Morii,James Nikkel,P. Phelps,U. Schroeder,T. A. Shutt,W. Skulski,P. Sorensen,J. Spaans,T.M. Stiegler,Robert Svoboda,M. Sweany,J. Thomson,J. Toke,Mani Tripathi,J.R. Verbus,N. Walsh,R. C. Webb,J. T. White,F. L. H. Wolfs,M. Woods,Chao Zhang +55 more
- 01 Jan 2010
TL;DR: The LUX experiment as discussed by the authors is the largest experiment of its type ever attempted, and it is expected to improve upon current experimental sensitivities by two orders of magnitude, and first data is expected in 2011.
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