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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
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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.
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Abstract: 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 will be a 20 tonne detector. Both devices will benefit tremendously from research and development performed for the LUX experiment, a 350 kg liquid Xe dark matter detector currently operating at the Sanford Underground Laboratory. In particular, the technology used for cryogenics and electrical feedthroughs, circulation and purification, low-background materials and shielding techniques, electronics, calibrations, and automated control and recovery systems are all directly scalable from LUX to the LZ detectors. Extensive searches for potential background sources have been performed, with an emphasis on previously undiscovered background sources that may have a significant impact on tonne-scale detectors. The LZ detectors will probe spin-independent interaction cross sections as low as 5E-49 cm2 for 100 GeV WIMPs, which represents the ultimate limit for dark matter detection with liquid xenon technology.
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TL;DR: 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.
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Neutrino Coherent Scattering Rates at Direct Dark Matter Detectors
TL;DR: In this article, the expected neutrino-induced background spectrum due to several of the most important sources, including solar, atmospheric, and diffuse supernova neutrinos, was discussed.
Scintillating properties of frozen new liquid scintillators
G. I. Britvich,F. Galeazzi,S.V. Golovkin,G. Martellotti,A.M. Medvedkov,Gianni Penso,A.S. Solovjev,V.G. Vasil'chenko +7 more
TL;DR: In this article, the decay time of scintillation light was measured at +20°C and −120°C, where the phase transition from liquid to solid takes place.
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