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@article{Akerib:2017:10.1103/PhysRevLett.118.021303,
author = {Akerib, DS and Alsum, S and Araujo, HM and Bai, X and Bailey, AJ and Balajthy, J and Beltrame, P and Bernard, EP and Bernstein, A and Biesiadzinski, TP and Boulton, EM and Bramante, R and Bras, P and Byram, D and Cahn, SB and Carmona-Benitez, MC and Chan, C and Chiller, AA and Chiller, C and Currie, A and Cutter, JE and Davison, TJR and Dobi, A and Dobson, JEY and Druszkiewicz, E and Edwards, BN and Faham, CH and Fiorucci, S and Gaitskell, RJ and Gehman, VM and Ghag, C and Gibson, KR and Gilchriese, MGD and Hall, CR and Hanhardt, M and Haselschwardt, SJ and Hertel, SA and Hogan, DP and Horn, M and Huang, DQ and Ignarra, CM and Ihm, M and Jacobsen, RG and Ji, W and Kamdin, K and Kazkaz, K and Khaitan, D and Knoche, R and Larsen, NA and Lee, C and Lenardo, BG and Lesko, KT and Lindote, A and Lopes, MI and Manalaysay, A and Mannino, RL and Marzioni, MF and McKinsey, DN and Mei, D-M and Mock, J and Moongweluwan, M and Morad, JA and Murphy, ASJ and Nehrkorn, C and Nelson, HN and Neves, F an},
doi = {10.1103/PhysRevLett.118.021303},
journal = {Physical Review Letters},
title = {Results from a search for dark matter in the complete LUX exposure},
url = {http://dx.doi.org/10.1103/PhysRevLett.118.021303},
volume = {118},
year = {2017}
}

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TY  - JOUR
AB  - We report constraints on spin-independent weakly interacting massive particle (WIMP)-nucleon scattering using a 3.35×104  kg day exposure of the Large Underground Xenon (LUX) experiment. A dual-phase xenon time projection chamber with 250 kg of active mass is operated at the Sanford Underground Research Facility under Lead, South Dakota (USA). With roughly fourfold improvement in sensitivity for high WIMP masses relative to our previous results, this search yields no evidence of WIMP nuclear recoils. At a WIMP mass of 50  GeV c−2, WIMP-nucleon spin-independent cross sections above 2.2×10−46  cm2 are excluded at the 90% confidence level. When combined with the previously reported LUX exposure, this exclusion strengthens to 1.1×10−46  cm2 at 50  GeV c−2.
AU  - Akerib,DS
AU  - Alsum,S
AU  - Araujo,HM
AU  - Bai,X
AU  - Bailey,AJ
AU  - Balajthy,J
AU  - Beltrame,P
AU  - Bernard,EP
AU  - Bernstein,A
AU  - Biesiadzinski,TP
AU  - Boulton,EM
AU  - Bramante,R
AU  - Bras,P
AU  - Byram,D
AU  - Cahn,SB
AU  - Carmona-Benitez,MC
AU  - Chan,C
AU  - Chiller,AA
AU  - Chiller,C
AU  - Currie,A
AU  - Cutter,JE
AU  - Davison,TJR
AU  - Dobi,A
AU  - Dobson,JEY
AU  - Druszkiewicz,E
AU  - Edwards,BN
AU  - Faham,CH
AU  - Fiorucci,S
AU  - Gaitskell,RJ
AU  - Gehman,VM
AU  - Ghag,C
AU  - Gibson,KR
AU  - Gilchriese,MGD
AU  - Hall,CR
AU  - Hanhardt,M
AU  - Haselschwardt,SJ
AU  - Hertel,SA
AU  - Hogan,DP
AU  - Horn,M
AU  - Huang,DQ
AU  - Ignarra,CM
AU  - Ihm,M
AU  - Jacobsen,RG
AU  - Ji,W
AU  - Kamdin,K
AU  - Kazkaz,K
AU  - Khaitan,D
AU  - Knoche,R
AU  - Larsen,NA
AU  - Lee,C
AU  - Lenardo,BG
AU  - Lesko,KT
AU  - Lindote,A
AU  - Lopes,MI
AU  - Manalaysay,A
AU  - Mannino,RL
AU  - Marzioni,MF
AU  - McKinsey,DN
AU  - Mei,D-M
AU  - Mock,J
AU  - Moongweluwan,M
AU  - Morad,JA
AU  - Murphy,ASJ
AU  - Nehrkorn,C
AU  - Nelson,HN
AU  - Neves,F
AU  - O'Sullivan,K
AU  - Oliver-Mallory,KC
AU  - Palladino,KJ
AU  - Pease,EK
AU  - Phelps,P
AU  - Reichhart,L
AU  - Rhyne,C
AU  - Shaw,S
AU  - Shutt,TA
AU  - Silva,C
AU  - Solmaz,M
AU  - Solovov,VN
AU  - Sorensen,P
AU  - Stephenson,S
AU  - Sumner,TJ
AU  - Szydagis,M
AU  - Taylor,DJ
AU  - Taylor,WC
AU  - Tennyson,BP
AU  - Terman,PA
AU  - Tiedt,DR
AU  - To,WH
AU  - Tripathi,M
AU  - Tvrznikova,L
AU  - Uvarov,S
AU  - Verbus,JR
AU  - Webb,RC
AU  - White,JT
AU  - Whitis,TJ
AU  - Witherell,MS
AU  - Wolfs,FLH
AU  - Xu,J
AU  - Yazdani,K
AU  - Young,SK
AU  - Zhang,C
DO  - 10.1103/PhysRevLett.118.021303
PY  - 2017///
SN  - 1079-7114
TI  - Results from a search for dark matter in the complete LUX exposure
T2  - Physical Review Letters
UR  - http://dx.doi.org/10.1103/PhysRevLett.118.021303
UR  - http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=WOS:000391926900002&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=1ba7043ffcc86c417c072aa74d649202
UR  - http://hdl.handle.net/10044/1/45091
VL  - 118
ER  -

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