Cosmogenic production of $^{37}$Ar in the context of the LUX-ZEPLIN experiment

Aalbers, J.; Akerib, D. S.; Musalhi, A. K. Al; Alder, F.; Alsum, S. K.; Amarasinghe, C. S.; Ames, A.; Anderson, T. J.; Angelides, N.; Araújo, H. M.; Armstrong, J. E.; Arthurs, M.; Bai, X.; Baker, A.; Balajthy, J.; Balashov, S.; Bang, J.; Bargemann, J. W.; Bauer, D.; Baxter, A.; Beattie, K.; Bernard, E. P.; Bhatti, A.; Biekert, A.; Biesiadzinski, T. P.; Birch, H. J.; Blockinger, G. M.; Bodnia, E.; Boxer, B.; Brew, C. A. J.; Brás, P.; Burdin, S.; Busenitz, J. K.; Buuck, M.; Cabrita, R.; Carmona-Benitez, M. C.; Cascella, M.; Chan, C.; Chawla, A.; Chen, H.; Chott, N. I.; Cole, A.; Converse, M. V.; Cottle, A.; Cox, G.; Creaner, O.; Cutter, J. E.; Dahl, C. E.; David, A.; de Viveiros, L.; Dobson, J. E. Y.; Druszkiewicz, E.; Eriksen, S. R.; Fan, A.; Fayer, S.; Fearon, N. M.; 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.; Gwilliam, C. B.; Hall, C. R.; Haselschwardt, S. J.; Hertel, S. A.; Horn, M.; Huang, D. Q.; Hunt, D.; Ignarra, C. M.; Jahangir, O.; James, R. S.; Ji, W.; Johnson, J.; Kaboth, A. C.; Kamaha, A. C.; Kamdin, K.; Khaitan, D.; Khazov, A.; Khurana, I.; Kodroff, D.; Korley, L.; Korolkova, E. V.; Kraus, H.; Kravitz, S.; Kreczko, L.; Kudryavtsev, V. A.; Leason, E. A.; Leonard, D. S.; Lesko, K. T.; Levy, C.; Lee, J.; Lin, J.; Lindote, A.; Linehan, R.; Lippincott, W. H.; Liu, X.; Lopes, M. I.; Asamar, E. Lopez; Lopez-Paredes, B.; Lorenzon, W.; Luitz, S.; Majewski, P. A.; Manalaysay, A.; Manenti, L.; Mannino, R. L.; Marangou, N.; McCarthy, M. E.; McKinsey, D. N.; McLaughlin, J.; Miller, E. H.; Mizrachi, E.; Monte, A.; Monzani, M. E.; Morad, J. A.; Mendoza, J. D. Morales; Morrison, E.; Mount, B. J.; Murphy, A. St. J.; Naim, D.; Naylor, A.; Nedlik, C.; Nelson, H. N.; Neves, F.; Nikoleyczik, J. A.; Nilima, A.; Olcina, I.; Oliver-Mallory, K.; Pal, S.; Palladino, K. J.; Palmer, J.; Parveen, N.; Patton, S. J.; Pease, E. K.; Penning, B.; Pereira, G.; Perry, E.; Pershing, J.; Piepke, A.; Porzio, D.; Qie, Y.; Reichenbacher, J.; Rhyne, C. A.; Richards, A.; Riffard, Q.; Riffard, %Q.; Rischbieter, G. R. C.; Rosero, R.; Rossiter, P.; Rushton, T.; Santone, D.; Sazzad, A. B. M. R.; Schnee, R. W.; Scovell, P. R.; Shaw, S.; Shutt, T. A.; Silk, J. J.; Silva, C.; Sinev, G.; Smith, R.; Solmaz, M.; Solovov, V. N.; Sorensen, P.; Soria, J.; Stancu, I.; Stevens, A.; Stifter, K.; Suerfu, B.; Sumner, T. J.; Swanson, N.; Szydagis, M.; Taylor, W. C.; Taylor, R.; Temples, D. J.; Terman, P. A.; Tiedt, D. R.; Timalsina, M.; To, W. H.; Tong, Z.; Tovey, D. R.; Trask, M.; Tripathi, M.; Tronstad, D. R.; Turner, W.; Utku, U.; Vaitkus, A.; Wang, B.; Wang, Y.; Wang, J. J.; Wang, W.; Watson, J. R.; Webb, R. C.; White, R. G.; Whitis, T. J.; Williams, M.; Wolfs, F. L. H.; Woodford, S.; Woodward, D.; Wright, C. J.; Xia, Q.; Xiang, X.; Xu, J.; Yeh, M.

doi:10.48550/arxiv.2201.02858

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Radioactive Isotopes In Fluid Detectors1

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2022

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“…The sea-level cosmogenic production rate in argon has been measured using neutron beam irradiation [245], and the production rate in xenon has been estimated in Ref. [246]. 39 Ar is a pure β emitter that is relatively long-lived (268 yr) and is a dominant background source for Ar-based DM detectors.…”

Section: Radioactive Isotopes In Fluid Detectorsmentioning

confidence: 99%

Snowmass2021 Cosmic Frontier White Paper: Calibrations and backgrounds for dark matter direct detection

Baxter¹,

Bunker²,

Shaw³

et al. 2022

Preprint

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Future dark matter direct detection experiments will reach unprecedented levels of sensitivity. Achieving this sensitivity will require more precise models of signal and background rates in future detectors. Improving the precision of signal and background modeling goes hand-in-hand with novel calibration techniques that can probe rare processes and lower threshold detector response. The goal of this white paper is to outline community needs to meet the background and calibration requirements of nextgeneration dark matter direct detection experiments.

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Section: Radioactive Isotopes In Fluid Detectorsmentioning

confidence: 99%