Projected WIMP sensitivity of the LUX-ZEPLIN dark matter experiment

Akerib, D. S.; Akerlof, C. W.; Alsum, S. K.; Araújo, H. M.; Arthurs, M.; Bai, X.; Bailey, A. J.; Balajthy, J.; Balashov, S.; Bauer, D.; Belle, J.; Beltrame, P.; Benson, T.; Bernard, E. P.; Biesiadzinski, T. P.; Boast, K. E.; Boxer, B.; Brás, P.; Buckley, J. H.; Bugaev, V. V.; Burdin, S.; Busenitz, J. K.; Carels, C.; Carlsmith, D. L.; Carlson, B.; Carmona-Benitez, M. C.; Chan, C.; Cherwinka, J. J.; Cole, A.; Cottle, A.; Craddock, W. W.; Currie, A.; Cutter, J. E.; Dahl, C. E.; de Viveiros, L.; Dobi, A.; Dobson, J. E.  Y.; Druszkiewicz, E.; Edberg, T. K.; Edwards, W. R.; Fan, A.; Fayer, S.; Fiorucci, S.; Fruth, T.; Gaitskell, R. J.; Genovesi, J.; Ghag, C.; Gilchriese, M. G.  D.; van der Grinten, M. G.  D.; Hall, C. R.; Hans, S.; Hanzel, K.; Haselschwardt, S. J.; Hertel, S. A.; Hillbrand, S.; Hjemfelt, C.; Hoff, M. D.; Hor, J. Y-K.; Huang, D. Q.; Ignarra, C. M.; Ji, W.; Kaboth, A. C.; Kamdin, K.; Keefner, J.; Khaitan, D.; Khazov, A.; Kim, Y. D.; Kocher, C. D.; Korolkova, E. V.; Kraus, H.; Krebs, H. J.; Kreczko, L.; Krikler, B.; Kudryavtsev, V. A.; Kyre, S.; Lee, J.; Lenardo, B. G.; Leonard, D. S.; Lesko, K. T.; Levy, C.; Li, J.; Liao, J.; Liao, F. -T.; Lin, J.; Lindote, A.; Linehan, R.; Lippincott, W. H.; Liu, X.; Lopes, M. I.; López Paredes, B.; Lorenzon, W.; Luitz, S.; Lyle, J. M.; Majewski, P.; Manalaysay, A.; Mannino, R. L.; Maupin, C.; McKinsey, D. N.; Meng, Y.; Miller, E. H.; Mock, J.; Monzani, M. E.; Morad, J. A.; Morrison, E.; Mount, B. J.; Murphy, A. St.  J.; Nelson, H. N.; Neves, F.; Nikoleyczik, J.; O’Sullivan, K.; Olcina, I.; Olevitch, M. A.; Oliver-Mallory, K. C.; Palladino, K. J.; Patton, S. J.; Pease, E. K.; Penning, B.; Piepke, A.; Powell, S.; Preece, R. M.; Pushkin, K.; Ratcliff, B. N.; Reichenbacher, J.; Rhyne, C. A.; Richards, A.; Rodrigues, J. P.; Rosero, R.; Rossiter, P.; Saba, J. S.; Sarychev, M.; Schnee, R. W.; Schubnell, M.; Scovell, P. R.; Shaw, S.; Shutt, T. A.; Silk, J. J.; Silva, C.; Skarpaas, K.; Skulski, W.; Solmaz, M.; Solovov, V. N.; Sorensen, P.; Stancu, I.; Stark, M. R.; Stiegler, T. M.; Stifter, K.; Szydagis, M.; Taylor, W. C.; Taylor, R.; Taylor, D. J.; Temples, D.; Terman, P. A.; Thomas, K. J.; Timalsina, M.; To, W. H.; Tomás, A.; Tope, T. E.; Tripathi, M.; Tull, C. E.; Tvrznikova, L.; Utku, U.; Va’vra, J.; Vacheret, A.; Verbus, J. R.; Voirin, E.; Waldron, W. L.; Watson, J. R.; Webb, R. C.; White, D. T.; Whitis, T. J.; Wisniewski, W. J.; Witherell, M. S.; Wolfs, F. L.  H.; Woodward, D.; Worm, S. D.; Yeh, M.; Yin, J.; Young, I.

doi:10.1103/PhysRevD.101.052002

Title: Projected WIMP sensitivity of the LUX-ZEPLIN dark matter experiment

Journal Article · Wed Mar 04 00:00:00 EST 2020 · Physical Review D

DOI:https://doi.org/10.1103/PhysRevD.101.052002· OSTI ID:1605156

Akerib, D. S.; Akerlof, C. W.; Alsum, S. K.; Araújo, H. M.; Arthurs, M.; Bai, X.; Bailey, A. J.; Balajthy, J.; Balashov, S.; Bauer, D.; Belle, J.; Beltrame, P.; Benson, T.; Bernard, E. P.; Biesiadzinski, T. P.; Boast, K. E.; Boxer, B.; Brás, P.; Buckley, J. H.; Bugaev, V. V. more »

LUX-ZEPLIN (LZ) is a next-generation dark matter direct detection experiment that will operate 4850 feet underground at the Sanford Underground Research Facility (SURF) in Lead, South Dakota, USA. Using a two-phase xenon detector with an active mass of 7 tonnes, LZ will search primarily for low-energy interactions with weakly interacting massive particles (WIMPs), which are hypothesized to make up the dark matter in our galactic halo. In this paper, the projected WIMP sensitivity of LZ is presented based on the latest background estimates and simulations of the detector. For a 1000 live day run using a 5.6-tonne fiducial mass, LZ is projected to exclude at 90% confidence level spin-independent WIMP-nucleon cross sections above 1.4×10-48 cm2 for a 40 GeV/c2 mass WIMP. Additionally, a 5σ discovery potential is projected, reaching cross sections below the exclusion limits of recent experiments. For spin-dependent WIMP-neutron(-proton) scattering, a sensitivity of 2.3×10-43 cm2 (7.1×10-42 cm2) for a 40 GeV/c2 mass WIMP is expected. With underground installation well underway, LZ is on track for commissioning at SURF in 2020.

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Research Organization:: Univ. of California, Santa Barbara, CA (United States); Univ. of California, Berkeley, CA (United States); Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States); SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States); Univ. of Michigan, Ann Arbor, MI (United States)

Sponsoring Organization:: USDOE Office of Science (SC), High Energy Physics (HEP); National Science Foundation (NSF); UK Science & Technology Facilities Council; Portuguese Foundation for Science and Technology (FCT); Institute for Basic Science, Korea

Contributing Organization:: LUX-ZEPLIN Collaboration

Grant/Contract Number:: SC0011702; AC02-05CH11231; SC0020216; SC0012704; SC0010010; AC02-07CH11359; SC0012161; SC0014223; FG02-13ER42020; SC0009999; NA0003180; SC0010072; SC0015708; SC0006605; FG02-10ER46709; UW PRJ82AJ; SC0013542; AC02-76SF00515; SC0019066; AC52-07NA27344; SC0012447; SC0018982; SC0019193

OSTI ID:: 1605156

Alternate ID(s):: OSTI ID: 1603208; OSTI ID: 1604732; OSTI ID: 1633961; OSTI ID: 1671746; OSTI ID: 1756453

Journal Information:: Physical Review D, Vol. 101, Issue 5; ISSN 2470-0010

Publisher:: American Physical Society (APS)Copyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 123 works

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Observation of Coherent Elastic Neutrino-Nucleus Scattering Akimov, D.; Albert, J. B.; An, P. arXiv https://doi.org/10.48550/arxiv.1708.01294	text	January 2017
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