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First Dark Matter Search Results from the LUX-ZEPLIN (LZ) Experiment.

Authors :
Aalbers J
Akerib DS
Akerlof CW
Al Musalhi AK
Alder F
Alqahtani A
Alsum SK
Amarasinghe CS
Ames A
Anderson TJ
Angelides N
Araújo HM
Armstrong JE
Arthurs M
Azadi S
Bailey AJ
Baker A
Balajthy J
Balashov S
Bang J
Bargemann JW
Barry MJ
Barthel J
Bauer D
Baxter A
Beattie K
Belle J
Beltrame P
Bensinger J
Benson T
Bernard EP
Bhatti A
Biekert A
Biesiadzinski TP
Birch HJ
Birrittella B
Blockinger GM
Boast KE
Boxer B
Bramante R
Brew CAJ
Brás P
Buckley JH
Bugaev VV
Burdin S
Busenitz JK
Buuck M
Cabrita R
Carels C
Carlsmith DL
Carlson B
Carmona-Benitez MC
Cascella M
Chan C
Chawla A
Chen H
Cherwinka JJ
Chott NI
Cole A
Coleman J
Converse MV
Cottle A
Cox G
Craddock WW
Creaner O
Curran D
Currie A
Cutter JE
Dahl CE
David A
Davis J
Davison TJR
Delgaudio J
Dey S
de Viveiros L
Dobi A
Dobson JEY
Druszkiewicz E
Dushkin A
Edberg TK
Edwards WR
Elnimr MM
Emmet WT
Eriksen SR
Faham CH
Fan A
Fayer S
Fearon NM
Fiorucci S
Flaecher H
Ford P
Francis VB
Fraser ED
Fruth T
Gaitskell RJ
Gantos NJ
Garcia D
Geffre A
Gehman VM
Genovesi J
Ghag C
Gibbons R
Gibson E
Gilchriese MGD
Gokhale S
Gomber B
Green J
Greenall A
Greenwood S
van der Grinten MGD
Gwilliam CB
Hall CR
Hans S
Hanzel K
Harrison A
Hartigan-O'Connor E
Haselschwardt SJ
Hernandez MA
Hertel SA
Heuermann G
Hjemfelt C
Hoff MD
Holtom E
Hor JY
Horn M
Huang DQ
Hunt D
Ignarra CM
Jacobsen RG
Jahangir O
James RS
Jeffery SN
Ji W
Johnson J
Kaboth AC
Kamaha AC
Kamdin K
Kasey V
Kazkaz K
Keefner J
Khaitan D
Khaleeq M
Khazov A
Khurana I
Kim YD
Kocher CD
Kodroff D
Korley L
Korolkova EV
Kras J
Kraus H
Kravitz S
Krebs HJ
Kreczko L
Krikler B
Kudryavtsev VA
Kyre S
Landerud B
Leason EA
Lee C
Lee J
Leonard DS
Leonard R
Lesko KT
Levy C
Li J
Liao FT
Liao J
Lin J
Lindote A
Linehan R
Lippincott WH
Liu R
Liu X
Liu Y
Loniewski C
Lopes MI
Lopez Asamar E
López Paredes B
Lorenzon W
Lucero D
Luitz S
Lyle JM
Majewski PA
Makkinje J
Malling DC
Manalaysay A
Manenti L
Mannino RL
Marangou N
Marzioni MF
Maupin C
McCarthy ME
McConnell CT
McKinsey DN
McLaughlin J
Meng Y
Migneault J
Miller EH
Mizrachi E
Mock JA
Monte A
Monzani ME
Morad JA
Morales Mendoza JD
Morrison E
Mount BJ
Murdy M
Murphy ASJ
Naim D
Naylor A
Nedlik C
Nehrkorn C
Neves F
Nguyen A
Nikoleyczik JA
Nilima A
O'Dell J
O'Neill FG
O'Sullivan K
Olcina I
Olevitch MA
Oliver-Mallory KC
Orpwood J
Pagenkopf D
Pal S
Palladino KJ
Palmer J
Pangilinan M
Parveen N
Patton SJ
Pease EK
Penning B
Pereira C
Pereira G
Perry E
Pershing T
Peterson IB
Piepke A
Podczerwinski J
Porzio D
Powell S
Preece RM
Pushkin K
Qie Y
Ratcliff BN
Reichenbacher J
Reichhart L
Rhyne CA
Richards A
Riffard Q
Rischbieter GRC
Rodrigues JP
Rodriguez A
Rose HJ
Rosero R
Rossiter P
Rushton T
Rutherford G
Rynders D
Saba JS
Santone D
Sazzad ABMR
Schnee RW
Scovell PR
Seymour D
Shaw S
Shutt T
Silk JJ
Silva C
Sinev G
Skarpaas K
Skulski W
Smith R
Solmaz M
Solovov VN
Sorensen P
Soria J
Stancu I
Stark MR
Stevens A
Stiegler TM
Stifter K
Studley R
Suerfu B
Sumner TJ
Sutcliffe P
Swanson N
Szydagis M
Tan M
Taylor DJ
Taylor R
Taylor WC
Temples DJ
Tennyson BP
Terman PA
Thomas KJ
Tiedt DR
Timalsina M
To WH
Tomás A
Tong Z
Tovey DR
Tranter J
Trask M
Tripathi M
Tronstad DR
Tull CE
Turner W
Tvrznikova L
Utku U
Va'vra J
Vacheret A
Vaitkus AC
Verbus JR
Voirin E
Waldron WL
Wang A
Wang B
Wang JJ
Wang W
Wang Y
Watson JR
Webb RC
White A
White DT
White JT
White RG
Whitis TJ
Williams M
Wisniewski WJ
Witherell MS
Wolfs FLH
Wolfs JD
Woodford S
Woodward D
Worm SD
Wright CJ
Xia Q
Xiang X
Xiao Q
Xu J
Yeh M
Yin J
Young I
Zarzhitsky P
Zuckerman A
Zweig EA
Source :
Physical review letters [Phys Rev Lett] 2023 Jul 28; Vol. 131 (4), pp. 041002.
Publication Year :
2023

Abstract

The LUX-ZEPLIN experiment is a dark matter detector centered on a dual-phase xenon time projection chamber operating at the Sanford Underground Research Facility in Lead, South Dakota, USA. This Letter reports results from LUX-ZEPLIN's first search for weakly interacting massive particles (WIMPs) with an exposure of 60 live days using a fiducial mass of 5.5 t. A profile-likelihood ratio analysis shows the data to be consistent with a background-only hypothesis, setting new limits on spin-independent WIMP-nucleon, spin-dependent WIMP-neutron, and spin-dependent WIMP-proton cross sections for WIMP masses above 9  GeV/c^{2}. The most stringent limit is set for spin-independent scattering at 36  GeV/c^{2}, rejecting cross sections above 9.2×10^{-48}  cm at the 90% confidence level.

Details

Language :
English
ISSN :
1079-7114
Volume :
131
Issue :
4
Database :
MEDLINE
Journal :
Physical review letters
Publication Type :
Academic Journal
Accession number :
37566836
Full Text :
https://doi.org/10.1103/PhysRevLett.131.041002