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First dark matter search results from the LUX-ZEPLIN (LZ) experiment

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PhysRevLett.131.041002.pdfPublished version9.61 MBAdobe PDFView/Open
Title: First dark matter search results from the LUX-ZEPLIN (LZ) experiment
Authors: Aalbers, J
Akerib, DS
Akerlof, CW
Musalhi, AKA
Alder, F
Alqahtani, A
Alsum, SK
Amarasinghe, CS
Ames, A
Anderson, TJ
Angelides, N
Araujo, 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
Bras, P
Buckley, JH
V. Bugaev, V
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
V. Converse, M
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
Grinten, MGDVD
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-K
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
V. Korolkova, E
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, F-T
Liao, J
Lin, J
Lindote, A
Linehan, R
Lippincott, WH
Liu, R
Liu, X
Liu, Y
Loniewski, C
Lopes, MI
Asamar, EL
Paredes, BL
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
Mendoza, JDM
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
Tomas, 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
Item Type: Journal Article
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/c2. The most stringent limit is set for spin-independent scattering at 36  GeV/c2, rejecting cross sections above 9.2×10−48  cm2 at the 90% confidence level.
Issue Date: 28-Jul-2023
Date of Acceptance: 7-Jun-2023
URI: http://hdl.handle.net/10044/1/113169
DOI: 10.1103/PhysRevLett.131.041002
ISSN: 0031-9007
Publisher: American Physical Society
Journal / Book Title: Physical Review Letters
Volume: 131
Issue: 4
Copyright Statement: Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.
Publication Status: Published
Article Number: 041002
Online Publication Date: 2023-07-28
Appears in Collections:Physics
High Energy Physics



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