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

**Authors:** D.S. Akerib, C.W. Akerlof, S.K. Alsum, N. Angelides, H.M. Ara\'ujo,, 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. Br\'as,, 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. L\'opez 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 Tom\'as, 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, and J. Yin

arXiv: 1904.02112 · 2019-11-18

## TL;DR

This study measures gamma-ray backgrounds in the Davis Cavern at Sanford Underground Research Facility to inform low-background experiments like LUX-ZEPLIN, revealing specific activity levels of natural isotopes and gamma fluxes.

## Contribution

It provides the first in-situ gamma-ray background characterization of the Davis Cavern, including activity levels of key isotopes and gamma flux measurements for underground physics experiments.

## Key findings

- Gamma flux in the cavern ranges from 596 Hz to 1355 Hz.
- Activities of $^{40}$K, $^{238}$U, and $^{232}$Th were quantified.
- Total gamma flux is approximately 1.9 gamma/cm²/s.

## Abstract

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 $\gamma$-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 $\gamma$-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 $1.9\pm0.4$~$\gamma~$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.

## Full text

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## Figures

15 figures with captions in the complete paper: https://tomesphere.com/paper/1904.02112/full.md

## References

30 references — full list in the complete paper: https://tomesphere.com/paper/1904.02112/full.md

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Source: https://tomesphere.com/paper/1904.02112