Simulations of events for the LUX-ZEPLIN (LZ) dark matter experiment

Akerib, D. S.; Akerlof, C. W.; Alqahtani, A.; Alsum, S. K.; Anderson, T. J.; Angelides, N.; Araújo, H. M.; Armstrong, J. E.; Arthurs, M.; Bai, X.; Balajthy, J.; Balashov, S.; Bang, J.; Bauer, D.; Baxter, A.; Bensinger, J.; Bernard, E. P.; Bernstein, A.; Bhatti, A.; Biekert, A.; Biesiadzinski, T. P.; Birch, H. J.; Boast, K. E.; Boxer, B.; Brás, P.; Buckley, J. H.; Bugaev, V. V.; Burdin, S.; Busenitz, J. K.; Cabrita, R.; Carels, C.; Carlsmith, D. L.; Carmona-Benitez, M. C.; Cascella, M.; Chan, C.; Chott, N. I.; Cole, A.; Cottle, A.; Cutter, J. E.; Dahl, C. E.; Viveiros, L. de; Dobson, J. E.Y.; Druszkiewicz, E.; Edberg, T. K.; Eriksen, S. R.; Fan, A.; Fayer, S.; Fiorucci, S.; Flaecher, H.; Fraser, E. D.; Fruth, T.; Gaitskell, R. J.; Genovesi, J.; Ghag, C.; Gibson, E.; Gilchriese, M. G.D.; Gokhale, S.; van der Grinten, M. G.D.; Hall, C. R.; Harrison, A.; Haselschwardt, S. J.; Hertel, S. A.; Hor, J. Y-K.; Horn, M.; Huang, D. Q.; Ignarra, C. M.; Jahangir, O.; Ji, W.; Johnson, J.; Kaboth, A. C.; Kamaha, A. C.; Kamdin, K.; Kazkaz, K.; Khaitan, D.; Khazov, A.; Khurana, I.; Kocher, C. D.; Korley, L.; Korolkova, E. V.; Kras, J.; Kraus, H.; Kravitz, S.; Kreczko, L.; Krikler, B.; Kudryavtsev, V. A.; Leason, E. A.; Lee, J.; 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, R.; Liu, X.; Loniewski, C.; Lopes, M. I.; López Paredes, B.; Lorenzon, W.; Luitz, S.; Lyle, J. M.; Majewski, P. A.; Manalaysay, A.; Manenti, L.; Mannino, R. L.; Marangou, N.; Marzioni, M. F.; McKinsey, D. N.; McLaughlin, J.; Meng, Y.; Miller, E. H.; Mizrachi, E.; Monte, A.; Monzani, M. E.; Morad, J. A.; Morrison, E.; Mount, B. J.; Murphy, A. St.J.; Naim, D.; Naylor, A.; Nedlik, C.; Nehrkorn, C.; Nelson, H. N.; Neves, F.; Nikoleyczik, J. A.; Nilima, A.; Olcina, I.; Oliver-Mallory, K. C.; Pal, S.; Palladino, K. J.; Palmer, J.; Parveen, N.; Pease, E. K.; Penning, B.; Pereira, G.; Piepke, A.; Pushkin, K.; Reichenbacher, J.; Rhyne, C. A.; Richards, A.; Riffard, Q.; Rischbieter, G. R.C.; Rosero, R.; Rossiter, P.; Rutherford, G.; Santone, D.; Sazzad, A. B.M.R.; Schnee, R. W.; Schubnell, M.; Scovell, P. R.; Seymour, D.; Shaw, S.; Shutt, T. A.; Silk, J. J.; Silva, C.; Smith, R.; Solmaz, M.; Solovov, V. N.; Sorensen, P.; Stancu, I.; Stevens, A.; Stifter, K.; Sumner, T. J.; Swanson, N.; Szydagis, M.; Tan, M.; Taylor, W. C.; Taylor, R.; Temples, D. J.; Terman, P. A.; Tiedt, D. R.; Timalsina, M.; Tomás, A.; Tripathi, M.; Tronstad, D. R.; Turner, W.; Tvrznikova, L.; Utku, U.; Vacheret, A.; Vaitkus, A.; Wang, J. J.; Wang, W.; Watson, J. R.; Webb, R. C.; White, R. G.; Whitis, T. J.; Wolfs, F. L.H.; Woodward, D.; Xiang, X.; Xu, J.; Yeh, M.; Zarzhitsky, P.

doi:10.1016/j.astropartphys.2020.102480

Title: Simulations of events for the LUX-ZEPLIN (LZ) dark matter experiment

Journal Article · Tue Jun 16 00:00:00 EDT 2020 · Astroparticle Physics

DOI:https://doi.org/10.1016/j.astropartphys.2020.102480· OSTI ID:1767431

Akerib, D. S.; Akerlof, C. W.; Alqahtani, A.; Alsum, S. K.; Anderson, T. J.; Angelides, N.; Araújo, H. M.; Armstrong, J. E.; Arthurs, M.; Bai, X.; Balajthy, J.; Balashov, S.; Bang, J.; Bauer, D.; Baxter, A.; Bensinger, J.; Bernard, E. P.; Bernstein, A.; Bhatti, A.; Biekert, A. more »

The LUX-ZEPLIN dark matter search aims to achieve a sensitivity to the WIMP-nucleon spin-independent cross-section down to (1-2) $$\times$$ $$10^{-12}$$ pb at a WIMP mass of 40 GeV/$c^2$. Here, this paper describes the simulations framework that, along with radioactivity measurements, was used to support this projection, and also to provide mock data for validating reconstruction and analysis software. Of particular note are the event generators, which allow us to model the background radiation, and the detector response physics used in the production of raw signals, which can be converted into digitized waveforms similar to data from the operational detector. Inclusion of the detector response allows us to process simulated data using the same analysis routines as developed to process the experimental data.

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Research Organization:: SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States); Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States); Univ. of Michigan, Ann Arbor, MI (United States); Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States); Univ. of Alabama, Tuscaloosa, AL (United States); Univ. of Rochester, NY (United States)

Sponsoring Organization:: USDOE Office of Science (SC), Basic Energy Sciences (BES); USDOE Office of Science (SC), High Energy Physics (HEP)

Contributing Organization:: LUX-ZEPLIN (LZ) Collaboration

Grant/Contract Number:: AC02-05CH11231; SC0020216; SC0012704; SC0010010; AC02-07CH11359; SC0012161; SC0014223; FG02-13ER42020; SC0009999; NA0003180; SC0011702; SC0010072; SC0015708; SC0006605; FG02-10ER46709; SC0013542; AC02-76SF00515; SC0018982; SC0019066; AC52-07NA27344; SC0012447; SC0019193; SC0008475

OSTI ID:: 1767431

Alternate ID(s):: OSTI ID: 1604733; OSTI ID: 1778397; OSTI ID: 1797373; OSTI ID: 1830751; OSTI ID: 1839636; OSTI ID: 1869519

Report Number(s):: LLNL-JRNL-833901; TRN: US2206364

Journal Information:: Astroparticle Physics, Vol. 125; ISSN 0927-6505

Publisher:: ElsevierCopyright Statement

Country of Publication:: United States

Language:: English

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