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Aalbers, J.; Akerib, D. S.; Alder, F.; Ames, A.; Anderson, T. J.; Angelides, N.; Araújo, H. M.; Armstrong, J. E.; Baker, A.; Bang, J.; Bargemann, J. W.; Baxter, A.; Bhatti, A.; Biekert, A.; Biesiadzinski, T. P.; Brás, P.; Busenitz, J. K.; Buuck, M.; Cascella, M.; Chan, C.; Chawla, A.; Cole, A.; Cottle, A.; Cox, G.; Creaner, O.; Dahl, C. E.; Dobson, J. E. Y.; Druszkiewicz, E.; Eriksen, S. R.; Fan, A.; Fayer, S.; Fraser, E. D.; Fruth, T.; Genovesi, J.; Gibson, E.; Gilchriese, M. G. D.; van der Grinten, M. G. D.; Hall, C. R.; Hertel, S. A.; Ignarra, C. M.; Johnson, J.; Khaitan, D.; Korolkova, E. V.; Kudryavtsev, V. A.; Leason, E. A.; Lesko, K. T.; Levy, C.; Linehan, R.; Lippincott, W. H.; Lopes, M. I.; Lopez Asamar, E.; Lopez-Paredes, B.; Majewski, P. A.; McKinsey, D. N.; Mizrachi, E.; Morad, J. A.; Morales Mendoza, J. D.; Murphy, A. J.; Nedlik, C.; Nelson, H. N.; Neves, F.; Nikoleyczik, J. A.; Olcina, I.; Palladino, K. J.; Parveen, N.; Pease, E. K.; Penning, B.; Pereira, G.; Piepke, A.; Porzio, D.; Qie, Y.; Rischbieter, G. R. C.; Rosero, R.; Rushton, T.; Santone, D.; Schnee, R. W.; Solovov, V. N.; Sorensen, P.; Stifter, K.; Suerfu, B.; Szydagis, M.; Taylor, R.; Temples, D. J.; Terman, P. A.; Tiedt, D. R.; Timalsina, M.; Tong, Z.; Tovey, D. R.; Tronstad, D. R.; Turner, W.; Utku, U.; Wang, J. J.; Wang, W.; Watson, J. R.; Webb, R. C.; White, R. G.; Wolfs, F. L. H.; Xia, Q.; Xu, J.; Yeh, M.
Physical review. D, 04/2022, Letnik: 105, Številka: 8Journal Article
We estimate the amount of Ar37 produced in natural xenon via cosmic-ray-induced spallation, an inevitable consequence of the transportation and storage of xenon on the Earth’s surface. We then calculate the resulting Ar37 concentration in a 10-tonne payload (similar to that of the LUX-ZEPLIN experiment) assuming a representative schedule of xenon purification, storage, and delivery to the underground facility. Using the spallation model by Silberberg and Tsao, the sea-level production rate of Ar37 in natural xenon is estimated to be 0.024 atoms/kg/day. Assuming the xenon is successively purified to remove radioactive contaminants in 1-tonne batches at a rate of 1 tonne/month, the average Ar37 activity after 10 tons are purified and transported underground is 0.058-0.090 μBq/kg, depending on the degree of argon removal during above-ground purification. Such cosmogenic Ar37 will appear as a noticeable background in the early science data, while decaying with a 35-day half-life. This newly noticed production mechanism of Ar37 should be considered when planning for future liquid-xenon-based experiments.
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