Pith. sign in

REVIEW 1 cited by

The Large Underground Xenon (LUX) Experiment

Not yet reviewed by Pith; the record is open.

Re-run · record.json Download PDF Read on arXiv ↗

This paper has not been read by Pith yet. Machine review is queued; the pith claim, tier, and objections will appear here once it completes.

SPECIMEN: schema-true, not a live event

T0 review · schema-true

One-sentence machine reading of the paper's core claim.

pith:XXXXXXXX · record.json · timestamp

arxiv 1211.3788 v2 pith:PPEBLQPV submitted 2012-11-16 physics.ins-det hep-ex

D. S. Akerib , X. Bai , S. Bedikian , E. Bernard , A. Bernstein , A. Bolozdynya , A. Bradley , D. Byram
show 86 more authors
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
This is my paper · ORCID
classification physics.ins-dethep-ex
keywords detectorwimpsxenonbackgroundlargeundergroundcandidatecharacterized
verification ladder T0 review T1 audit T2 compute T3 formal

Signed reviews

No signed human review yet.

0 comments
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 $2\times 10^{-46}$ cm$^{2}$, equivalent to $\sim$1 event/100 kg/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.

Discussion (0). Continue with ORCID to comment.

Forward citations

Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. First direct detection constraint on mirror dark matter kinetic mixing using LUX 2013 data

    hep-ex 2019-08 conditional novelty 6.0 of 10

    A search of 95 live-days of LUX 2013 data finds no mirror dark matter electron recoils, giving 90% confidence upper limits on kinetic mixing for mirror electron temperatures 0.1-0.9 keV and excluding temperatures abov...

Pith tools