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arXiv 1904.02112physics.ins-dethep-ex
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桑福德地下研究设施戴维斯洞穴中Gamma Ray背景的测量

Measurement of the Gamma Ray Background in the Davis Cavern at the Sanford Underground Research Facility

D. S. Akerib, C. W. Akerlof, S. K. Alsum, N. Angelides, H. M. Araújo, J. E. Armstrong, M. Arthurs, X. Bai, J. Balajthy, S. Balashov, A. Baxter, E. P. Bernard, A… 展开作者

D. S. Akerib, C. W. Akerlof, S. K. Alsum, N. Angelides, H. M. Araújo, J. E. Armstrong, M. Arthurs, X. Bai, J. Balajthy, S. Balashov, A. Baxter, E. P. Bernard, A. Biekert, T. P. Biesiadzinski, K. E. Boast, B. Boxer, P. Brás, J. H. Buckley, V. V. Bugaev, S. Burdin, J. K. Busenitz, C. Carels, D. L. Carlsmith, M. C. Carmona-Benitez, M. Cascella, C. Chan, A. Cole, A. Cottle, J. E. Cutter, C. E. Dahl, L. de Viveiros, J. E. Y. Dobson, E. Druszkiewicz, T. K. Edberg, A. Fan, S. Fiorucci, H. Flaecher, T. Fruth, R. J. Gaitskell, J. Genovesi, C. Ghag, M. G. D. Gilchriese, S. Gokhale, M. G. D. van der Grinten, C. R. Hall, S. Hans, J. Harrison, S. J. Haselschwardt, S. A. Hertel, J. Y-K. Hor, M. Horn, D. Q. Huang, C. M. Ignarra, O. Jahangir, W. Ji, J. Johnson, A. C. Kaboth, K. Kamdin, D. Khaitan, A. Khazov, W. T. Kim, C. D. Kocher, L. Korley, E. V. Korolkova, J. Kras, H. Kraus, S. W. Kravitz, L. Kreczko, B. Krikler, V. A. Kudryavtsev, E. A. Leason, J. Lee, D. S. Leonard, K. T. Lesko, C. Levy, J. Li, J. Liao, F. -T. Liao, J. Lin, A. Lindote, R. Linehan, W. H. Lippincott, R. Liu, X. Liu, C. Loniewski, M. I. Lopes, B. López Paredes, W. Lorenzon, S. Luitz, J. M. Lyle, P. A. Majewski, A. Manalaysay, L. Manenti, R. L. Mannino, N. Marangou, M. F. Marzioni, D. N. McKinsey, J. McLaughlin, Y. Meng, E. H. Miller, M. E. Monzani, J. A. Morad, E. Morrison, B. J. Mount, A. St. J. Murphy, D. Naim, A. Naylor, C. Nedlik, C. Nehrkorn, H. N. Nelson, F. Neves, J. Nikoleyczik, A. Nilima, I. Olcina, K. C. Oliver-Mallory, S. Pal, K. J. Palladino, E. K. Pease, B. P. Penning, G. Pereira, A. Piepke, K. Pushkin, J. Reichenbacher, C. A. Rhyne, Q. Riffard, G. R. C. Rischbieter, J. P. Rodrigues, R. Rosero, P. Rossiter, G. Rutherford, A. B. M. R. Sazzad, R. W. Schnee, M. Schubnell, P. R. Scovell, D. Seymour, S. Shaw, T. A. Shutt, J. J. Silk, C. Silva, M. Solmaz, V. N. Solovov, P. Sorensen, I. Stancu, A. Stevens, T. M. Stiegler, K. Stifter, M. Szydagis, W. C. Taylor, R. Taylor, D. Temples, P. A. Terman, D. R. Tiedt, M. Timalsina, A Tomás, M. Tripathi, L. Tvrznikova, U. Utku, S. Uvarov, A. Vacheret, J. J. Wang, J. R. Watson, R. C. Webb, R. G. White, T. J. Whitis, F. L. H. Wolfs, D. Woodward, J. Yin

摘要:

由于宇宙射线通过地球时会衰减,深地下环境是低背景搜索的理想场所。然而,它们受到周围岩石中$^{40}$ K和$^{238}$ U和$^{232}$ Th衰变链发射的$γ$ -射线的背景影响。LUX-ZEPLIN(LZ)实验将寻找暗物质粒子与位于南达科他州Lead的Sanford Underground Research Facility的Davis校园内的液体氙TPC的相互作用,该实验位于4,850英尺的高度。为了确定洞穴背景,在不同位置用碘化钠探测器和铅屏蔽进行了现场$γ$射线测量。对于无屏蔽测量,积分计数率(0- 3300 keV)在596 Hz到1355 Hz之间变化,对应于$1.9\pm0.4$ ~ $γ~$ cm $^{-2}$ s $^{-1}$ .洞穴壁中产生的放射性可表征为$220\pm60$ ~Bq/kg的$^{40}$ K、$29\pm15$ ~Bq/kg的$^{238}$ U和$13\pm3$ ~Bq/kg的$^{232}$ Th。

英文摘要:

Deep underground environments are ideal for low background searches due to the attenuation of cosmic rays by passage through the earth. However, they are affected by backgrounds from $γ$-rays emitted by $^{40}$K and the $^{238}$U and $^{232}$Th decay chains in the surrounding rock. The LUX-ZEPLIN (LZ) experiment will search for dark matter particle interactions with a liquid xenon TPC located within the Davis campus at the Sanford Underground Research Facility, Lead, South Dakota, at the 4,850-foot level. In order to characterise the cavern background, in-situ $γ$-ray measurements were taken with a sodium iodide detector in various locations and with lead shielding. The integral count rates (0--3300~keV) varied from 596~Hz to 1355~Hz for unshielded measurements, corresponding to a total flux in the cavern of $1.9\pm0.4$~$γ~$cm$^{-2}$s$^{-1}$. The resulting activity in the walls of the cavern can be characterised as $220\pm60$~Bq/kg of $^{40}$K, $29\pm15$~Bq/kg of $^{238}$U, and $13\pm3$~Bq/kg of $^{232}$Th.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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