Corpus ID: 117043383

# After LUX: The LZ Program

@article{Malling2011AfterLT,
title={After LUX: The LZ Program},
author={D. C. Malling and D. S. Akerib and Henrique Ara{\'u}jo and Xinzhan Bai and Sourpouhi Bedikian and Ethan P. Bernard and Adam Bernstein and A. Bradley and Sydney B. Cahn and M. C. Carmona-Benitez and D. Carr and J. J. Chapman and Ken Clark and Timothy M. Classen and Tyler Coffey and Alessandro Curioni and A. Currie and Steven A. Dazeley and Luiz de Viveiros and Michael Raymond Dragowsky and Eryk Druszkiewicz and Carlos Faham and S. Fiorucci and R. J. Gaitskell and K. R. Gibson and Christopher Hall and Mark Hanhardt and Britt Holbrook and M. O. Ihm and Robert G Jacobsen and L. W. Kastens and K. Kazkaz and Richard L. Lander and N. A. Larsen and Chien-Hsiung Lee and David Leonard and Kevin T. Lesko and A. Lindote and M. I. Lopes and Alexey V. Lyashenko and Paweł Majewski and Rachel Mannino and D. N. Mckinsey and Dongming Mei and Jeremy A. Mock and Masahiro Morii and A. St. J. Murphy and H. Nelson and Fernando A. Das Neves and J. A. Nikkel and Monica Pangilinan and Patrick R. Phelps and Lea Reichhart and Thomas Alan Shutt and C. Silva and Wojtek Skulski and V. N. Solovov and Peter Sorensen and Jason D. Spaans and Tyana Stiegler and Timothy J Sumner and Robert C. Svoboda and Melinda Sweany and Matthew Szydagis and J. A. Thomson and M. Tripathi and James Verbus and Nicholas Walsh and Robert C. Webb and J. T. White and Michal Wlasenko and F. L. H. Wolfs and Michael Woods and C. Zhang},
journal={arXiv: Instrumentation and Methods for Astrophysics},
year={2011}
}
• D. Malling, +71 authors C. Zhang
• Published 1 October 2011
• Physics
• arXiv: Instrumentation and Methods for Astrophysics
Author(s): Malling, DC; Akerib, DS; Araujo, HM; Bai, X; Bedikian, S; Bernard, E; Bernstein, A; Bradley, A; Cahn, SB; Carmona-Benitez, MC; Carr, D; Chapman, JJ; Clark, K; Classen, T; Coffey, T; Curioni, A; Currie, A; Dazeley, S; Viveiros, L de; Dragowsky, M; Druszkiewicz, E; Faham, CH; Fiorucci, S; Gaitskell, RJ; Gibson, KR; Hall, C; Hanhardt, M; Holbrook, B; Ihm, M; Jacobsen, RG; Kastens, L; Kazkaz, K; Lander, R; Larsen, N; Lee, C; Leonard, D; Lesko, K; Lindote, A; Lopes, MI; Lyashenko, A… Expand
111 Citations

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#### References

SHOWING 1-10 OF 12 REFERENCES
Calibration of a Liquid Xenon Detector with Kr-83m
• Physics
• 2009
We report the preparation of a $^{83}\mathrm{Kr}{}^{m}$ source and its use in calibrating a liquid xenon detector. $^{83}\mathrm{Kr}{}^{m}$ atoms were produced through the decay of $^{83}\mathrm{Rb}$Expand
Study of a zirconium getter for purification of xenon gas
Abstract Oxygen, nitrogen and methane purification efficiencies for a common zirconium getter are measured in 1050 Torr of xenon gas. Starting with impurity concentrations near 10 −6  g/g, the outletExpand
Scintillating properties of frozen new liquid scintillators
Abstract The light emission from scintillators which are liquid at room temperature was studied in the interval between +20°C and −120°C where the phase transition from liquid to solid takes place.Expand
Dark matter results from 100 live days of XENON100 data.
The XENON100 detector, installed underground at the Laboratori Nazionali del Gran Sasso of INFN, Italy, finds no evidence for dark matter, leading to the most stringent limit on dark matter interactions today. Expand
A 83Krm Source for Use in Low-background Liquid Xenon Time Projection Chambers
• Materials Science, Physics
• 2009
We report the testing of a charcoal-based Kr-83m source for use in calibrating a low background two-phase liquid xenon detector. Kr-83m atoms produced through the decay of Rb-83 are introduced into aExpand
Neutrino coherent scattering rates at direct dark matter detectors
Neutrino-induced recoil events may constitute a background to direct dark matter searches, particularly for those detectors that strive to reach the ton-scale and beyond. This paper discusses theExpand
Observation of two-neutrino double-beta decay in 136Xe with the EXO-200 detector.
The observed decay rate provides new input to matrix element calculations and to the search for the more interesting neutrinoless double-beta decay, the most sensitive probe for the existence of Majorana particles and the measurement of the neutrino mass scale. Expand
Muon-induced background study for underground laboratories
• Physics
• 2004
We provide a comprehensive study of the cosmic-ray muon flux and induced activity as a function of overburden along with a convenient parametrization of the salient fluxes and differentialExpand
Observation of Two-Neutrino Double-Beta Decay in 136Xe with EXO-200.
• arXiv:1108.4193v1 [nucl-ex]
• 2011
Construction of the LUX Dark Matter Experiment at the Sanford Underground Science and Engineering Laboratory