The Large Underground Xenon (LUX) experiment

D. S. Akerib; X. Bai; S. Bedikian; E. Bernard; A. Bernstein; A. Bolozdynya; A. Bradley; D. Byram; S. B. Cahn; C. Camp; M. C. Carmona-Benitez; D. Carr; J. J. Chapman; A. Chiller; C. Chiller; K. Clark; T. Classen; T. Coffey; A. Curioni; E. Dahl; S. Dazeley; L. De Viveiros; A. Dobi; E. Dragowsky; E. Druszkiewicz; B. Edwards; C. H. Faham; S. Fiorucci; R. J. Gaitskell; K. R. Gibson; M. Gilchriese; C. Hall; M. Hanhardt; B. Holbrook; M. Ihm; R. G. Jacobsen; L. Kastens; K. Kazkaz; R. Knoche; S. Kyre; J. Kwong; R. Lander; N. A. Larsen; C. Lee; D. S. Leonard; K. T. Lesko; A. Lindote; M. I. Lopes; A. Lyashenko; D. C. Malling; R. Mannino; Z. Marquez; D. N. McKinsey; D. M. Mei; J. Mock; M. Moongweluwan; M. Morii; H. Nelson; F. Neves; J. A. Nikkel; M. Pangilinan; P. D. Parker; E. K. Pease; K. Pech; P. Phelps; A. Rodionov; P. Roberts; A. Shei; T. Shutt; C. Silva; W. Skulski; V. N. Solovov; C. J. Sofka; P. Sorensen; J. Spaans; T. Stiegler; D. Stolp; R. Svoboda; M. Sweany; M. Szydagis; D. Taylor; J. Thomson; M. Tripathi; S. Uvarov; J. R. Verbus; N. Walsh; R. Webb; D. White; J. T. White; T. J. Whitis; M. Wlasenko; F. L.H. Wolfs; M. Woods; C. Zhang

doi:10.1016/j.nima.2012.11.135

The Large Underground Xenon (LUX) experiment

D. S. Akerib, X. Bai, S. Bedikian, E. Bernard, A. Bernstein, A. Bolozdynya, A. Bradley, D. Byram, S. B. Cahn, C. Camp, M. C. Carmona-Benitez, D. Carr, J. J. Chapman, A. Chiller, C. Chiller, K. Clark, T. Classen, T. Coffey, A. Curioni, E. DahlS. Dazeley, L. De Viveiros, A. Dobi, E. Dragowsky, E. Druszkiewicz, B. Edwards, C. H. Faham, S. Fiorucci, R. J. Gaitskell, K. R. Gibson, M. Gilchriese, C. Hall, M. Hanhardt, B. Holbrook, M. Ihm, R. G. Jacobsen, L. Kastens, K. Kazkaz, R. Knoche, S. Kyre, J. Kwong, R. Lander, N. A. Larsen, C. Lee, D. S. Leonard, K. T. Lesko, A. Lindote, M. I. Lopes, A. Lyashenko, D. C. Malling, R. Mannino, Z. Marquez, D. N. McKinsey, D. M. Mei, J. Mock, M. Moongweluwan, M. Morii, H. Nelson, F. Neves, J. A. Nikkel, M. Pangilinan, P. D. Parker, E. K. Pease, K. Pech, P. Phelps, A. Rodionov, P. Roberts, A. Shei, T. Shutt, C. Silva, W. Skulski, V. N. Solovov, C. J. Sofka, P. Sorensen, J. Spaans, T. Stiegler, D. Stolp, R. Svoboda, M. Sweany, M. Szydagis, D. Taylor, J. Thomson, M. Tripathi, S. Uvarov, J. R. Verbus, N. Walsh, R. Webb, D. White, J. T. White, T. J. Whitis, M. Wlasenko, F. L.H. Wolfs, M. Woods, C. Zhang

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Abstract

The Large Underground Xenon (LUX) collaboration has designed and constructed a dual-phase xenon detector, in order to conduct a search for Weakly Interacting Massive Particles (WIMPs), a leading dark matter candidate. The goal of the LUX detector is to clearly detect (or exclude) WIMPS with a spin independent cross-section per nucleon of 2×10^-46cm2, equivalent to ∼1event/100kg/month in the inner 100-kg fiducial volume (FV) of the 370-kg detector. The overall background goals are set to have <1 background events characterized as possible WIMPs in the FV in 300 days of running. This paper describes the design and construction of the LUX detector.

Original language	English (US)
Pages (from-to)	111-126
Number of pages	16
Journal	Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
Volume	704
DOIs	https://doi.org/10.1016/j.nima.2012.11.135
State	Published - 2013

All Science Journal Classification (ASJC) codes

Nuclear and High Energy Physics
Instrumentation

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10.1016/j.nima.2012.11.135

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Akerib, D. S., Bai, X., Bedikian, S., Bernard, E., Bernstein, A., Bolozdynya, A., Bradley, A., Byram, D., Cahn, S. B., Camp, C., Carmona-Benitez, M. C., Carr, D., Chapman, J. J., Chiller, A., Chiller, C., Clark, K., Classen, T., Coffey, T., Curioni, A., ... Zhang, C. (2013). The Large Underground Xenon (LUX) experiment. Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, 704, 111-126. https://doi.org/10.1016/j.nima.2012.11.135

@article{edf9e297972b4ff09779768cfe218cf2,

title = "The Large Underground Xenon (LUX) experiment",

abstract = "The Large Underground Xenon (LUX) collaboration has designed and constructed a dual-phase xenon detector, in order to conduct a search for Weakly Interacting Massive Particles (WIMPs), a leading dark matter candidate. The goal of the LUX detector is to clearly detect (or exclude) WIMPS with a spin independent cross-section per nucleon of 2×10-46cm2, equivalent to ∼1event/100kg/month in the inner 100-kg fiducial volume (FV) of the 370-kg detector. The overall background goals are set to have <1 background events characterized as possible WIMPs in the FV in 300 days of running. This paper describes the design and construction of the LUX detector.",

author = "Akerib, \{D. S.\} and X. Bai and S. Bedikian and E. Bernard and A. Bernstein and A. Bolozdynya and A. Bradley and D. Byram and Cahn, \{S. B.\} and C. Camp and Carmona-Benitez, \{M. C.\} and D. Carr and Chapman, \{J. J.\} and A. Chiller and C. Chiller and K. Clark and T. Classen and T. Coffey and A. Curioni and E. Dahl and S. Dazeley and \{De Viveiros\}, L. and A. Dobi and E. Dragowsky and E. Druszkiewicz and B. Edwards and Faham, \{C. H.\} and S. Fiorucci and Gaitskell, \{R. J.\} and Gibson, \{K. R.\} and M. Gilchriese and C. Hall and M. Hanhardt and B. Holbrook and M. Ihm and Jacobsen, \{R. G.\} and L. Kastens and K. Kazkaz and R. Knoche and S. Kyre and J. Kwong and R. Lander and Larsen, \{N. A.\} and C. Lee and Leonard, \{D. S.\} and Lesko, \{K. T.\} and A. Lindote and Lopes, \{M. I.\} and A. Lyashenko and Malling, \{D. C.\} and R. Mannino and Z. Marquez and McKinsey, \{D. N.\} and Mei, \{D. M.\} and J. Mock and M. Moongweluwan and M. Morii and H. Nelson and F. Neves and Nikkel, \{J. A.\} and M. Pangilinan and Parker, \{P. D.\} and Pease, \{E. K.\} and K. Pech and P. Phelps and A. Rodionov and P. Roberts and A. Shei and T. Shutt and C. Silva and W. Skulski and Solovov, \{V. N.\} and Sofka, \{C. J.\} and P. Sorensen and J. Spaans and T. Stiegler and D. Stolp and R. Svoboda and M. Sweany and M. Szydagis and D. Taylor and J. Thomson and M. Tripathi and S. Uvarov and Verbus, \{J. R.\} and N. Walsh and R. Webb and D. White and White, \{J. T.\} and Whitis, \{T. J.\} and M. Wlasenko and Wolfs, \{F. L.H.\} and M. Woods and C. Zhang",

note = "Funding Information: This work was partially supported by the U.S. Department of Energy (DOE) under award numbers DE-FG02-08ER41549 , DE-FG02-91ER40688 , DOE , DE-FG02-95ER40917 , DE-FG02-91ER40674 , DE-FG02-11ER41738 , DE-SC0006605 , DE-AC02- 05CH11231 , DE-AC52-07NA27344 , the U.S. National Science Foundation under award numbers PHYS-0750671 , PHY-0801536 , PHY-1004661 , PHY-1102470 , PHY-1003660 , the Research Corporation grant RA0350 , the Center for Ultra-low Background Experiments in the Dakotas (CUBED) , and the South Dakota School of Mines and Technology (SDSMT) . LIP-Coimbra acknowledges funding from Funda{\c c}{\~a}o para a Ci{\^e}ncia e Tecnologia (FCT) through the project-grant CERN/FP/123610/2011 . We gratefully acknowledge the logistical and technical support and the access to laboratory infrastructure provided to us by the Sanford Underground Research Facility (SURF) and its personnel at Lead, South Dakota.",

year = "2013",

doi = "10.1016/j.nima.2012.11.135",

language = "English (US)",

volume = "704",

pages = "111--126",

journal = "Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment",

issn = "0168-9002",

publisher = "Elsevier B.V.",

}

Akerib, DS, Bai, X, Bedikian, S, Bernard, E, Bernstein, A, Bolozdynya, A, Bradley, A, Byram, D, Cahn, SB, Camp, C, Carmona-Benitez, MC, Carr, D, Chapman, JJ, Chiller, A, Chiller, C, Clark, K, Classen, T, Coffey, T, Curioni, A, Dahl, E, Dazeley, S, De Viveiros, L, Dobi, A, Dragowsky, E, Druszkiewicz, E, Edwards, B, Faham, CH, Fiorucci, S, Gaitskell, RJ, Gibson, KR, Gilchriese, M, Hall, C, Hanhardt, M, Holbrook, B, Ihm, M, Jacobsen, RG, Kastens, L, Kazkaz, K, Knoche, R, Kyre, S, Kwong, J, Lander, R, Larsen, NA, Lee, C, Leonard, DS, Lesko, KT, Lindote, A, Lopes, MI, Lyashenko, A, Malling, DC, Mannino, R, Marquez, Z, McKinsey, DN, Mei, DM, Mock, J, Moongweluwan, M, Morii, M, Nelson, H, Neves, F, Nikkel, JA, Pangilinan, M, Parker, PD, Pease, EK, Pech, K, Phelps, P, Rodionov, A, Roberts, P, Shei, A, Shutt, T, Silva, C, Skulski, W, Solovov, VN, Sofka, CJ, Sorensen, P, Spaans, J, Stiegler, T, Stolp, D, Svoboda, R, Sweany, M, Szydagis, M, Taylor, D, Thomson, J, Tripathi, M, Uvarov, S, Verbus, JR, Walsh, N, Webb, R, White, D, White, JT, Whitis, TJ, Wlasenko, M, Wolfs, FLH, Woods, M & Zhang, C 2013, 'The Large Underground Xenon (LUX) experiment', Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment, vol. 704, pp. 111-126. https://doi.org/10.1016/j.nima.2012.11.135

TY - JOUR

T1 - The Large Underground Xenon (LUX) experiment

AU - Akerib, D. S.

AU - Bai, X.

AU - Bedikian, S.

AU - Bernard, E.

AU - Bernstein, A.

AU - Bolozdynya, A.

AU - Bradley, A.

AU - Byram, D.

AU - Cahn, S. B.

AU - Camp, C.

AU - Carmona-Benitez, M. C.

AU - Carr, D.

AU - Chapman, J. J.

AU - Chiller, A.

AU - Chiller, C.

AU - Clark, K.

AU - Classen, T.

AU - Coffey, T.

AU - Curioni, A.

AU - Dahl, E.

AU - Dazeley, S.

AU - De Viveiros, L.

AU - Dobi, A.

AU - Dragowsky, E.

AU - Druszkiewicz, E.

AU - Edwards, B.

AU - Faham, C. H.

AU - Fiorucci, S.

AU - Gaitskell, R. J.

AU - Gibson, K. R.

AU - Gilchriese, M.

AU - Hall, C.

AU - Hanhardt, M.

AU - Holbrook, B.

AU - Ihm, M.

AU - Jacobsen, R. G.

AU - Kastens, L.

AU - Kazkaz, K.

AU - Knoche, R.

AU - Kyre, S.

AU - Kwong, J.

AU - Lander, R.

AU - Larsen, N. A.

AU - Lee, C.

AU - Leonard, D. S.

AU - Lesko, K. T.

AU - Lindote, A.

AU - Lopes, M. I.

AU - Lyashenko, A.

AU - Malling, D. C.

AU - Mannino, R.

AU - Marquez, Z.

AU - McKinsey, D. N.

AU - Mei, D. M.

AU - Mock, J.

AU - Moongweluwan, M.

AU - Morii, M.

AU - Nelson, H.

AU - Neves, F.

AU - Nikkel, J. A.

AU - Pangilinan, M.

AU - Parker, P. D.

AU - Pease, E. K.

AU - Pech, K.

AU - Phelps, P.

AU - Rodionov, A.

AU - Roberts, P.

AU - Shei, A.

AU - Shutt, T.

AU - Silva, C.

AU - Skulski, W.

AU - Solovov, V. N.

AU - Sofka, C. J.

AU - Sorensen, P.

AU - Spaans, J.

AU - Stiegler, T.

AU - Stolp, D.

AU - Svoboda, R.

AU - Sweany, M.

AU - Szydagis, M.

AU - Taylor, D.

AU - Thomson, J.

AU - Tripathi, M.

AU - Uvarov, S.

AU - Verbus, J. R.

AU - Walsh, N.

AU - Webb, R.

AU - White, D.

AU - White, J. T.

AU - Whitis, T. J.

AU - Wlasenko, M.

AU - Wolfs, F. L.H.

AU - Woods, M.

AU - Zhang, C.

N1 - Funding Information: This work was partially supported by the U.S. Department of Energy (DOE) under award numbers DE-FG02-08ER41549 , DE-FG02-91ER40688 , DOE , DE-FG02-95ER40917 , DE-FG02-91ER40674 , DE-FG02-11ER41738 , DE-SC0006605 , DE-AC02- 05CH11231 , DE-AC52-07NA27344 , the U.S. National Science Foundation under award numbers PHYS-0750671 , PHY-0801536 , PHY-1004661 , PHY-1102470 , PHY-1003660 , the Research Corporation grant RA0350 , the Center for Ultra-low Background Experiments in the Dakotas (CUBED) , and the South Dakota School of Mines and Technology (SDSMT) . LIP-Coimbra acknowledges funding from Fundação para a Ciência e Tecnologia (FCT) through the project-grant CERN/FP/123610/2011 . We gratefully acknowledge the logistical and technical support and the access to laboratory infrastructure provided to us by the Sanford Underground Research Facility (SURF) and its personnel at Lead, South Dakota.

PY - 2013

Y1 - 2013

N2 - The Large Underground Xenon (LUX) collaboration has designed and constructed a dual-phase xenon detector, in order to conduct a search for Weakly Interacting Massive Particles (WIMPs), a leading dark matter candidate. The goal of the LUX detector is to clearly detect (or exclude) WIMPS with a spin independent cross-section per nucleon of 2×10-46cm2, equivalent to ∼1event/100kg/month in the inner 100-kg fiducial volume (FV) of the 370-kg detector. The overall background goals are set to have <1 background events characterized as possible WIMPs in the FV in 300 days of running. This paper describes the design and construction of the LUX detector.

AB - The Large Underground Xenon (LUX) collaboration has designed and constructed a dual-phase xenon detector, in order to conduct a search for Weakly Interacting Massive Particles (WIMPs), a leading dark matter candidate. The goal of the LUX detector is to clearly detect (or exclude) WIMPS with a spin independent cross-section per nucleon of 2×10-46cm2, equivalent to ∼1event/100kg/month in the inner 100-kg fiducial volume (FV) of the 370-kg detector. The overall background goals are set to have <1 background events characterized as possible WIMPs in the FV in 300 days of running. This paper describes the design and construction of the LUX detector.

UR - https://www.scopus.com/pages/publications/84872289226

UR - https://www.scopus.com/inward/citedby.url?scp=84872289226&partnerID=8YFLogxK

U2 - 10.1016/j.nima.2012.11.135

DO - 10.1016/j.nima.2012.11.135

M3 - Article

AN - SCOPUS:84872289226

SN - 0168-9002

VL - 704

SP - 111

EP - 126

JO - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment

JF - Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment

ER -

The Large Underground Xenon (LUX) experiment

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