- Main
Measurement of the gamma ray background in the Davis cavern at the Sanford Underground Research Facility
- Akerib, DS;
- Akerlof, CW;
- Alsum, SK;
- Angelides, N;
- Araújo, HM;
- Armstrong, JE;
- Arthurs, M;
- Bai, X;
- Balajthy, J;
- Balashov, S;
- Baxter, A;
- Bernard, EP;
- Biekert, A;
- Biesiadzinski, TP;
- Boast, KE;
- Boxer, B;
- Brás, P;
- Buckley, JH;
- Bugaev, VV;
- Burdin, S;
- Busenitz, JK;
- Carels, C;
- Carlsmith, DL;
- Carmona-Benitez, MC;
- Cascella, M;
- Chan, C;
- Cole, A;
- Cottle, A;
- Cutter, JE;
- Dahl, CE;
- de Viveiros, L;
- Dobson, JEY;
- Druszkiewicz, E;
- Edberg, TK;
- Fan, A;
- Fiorucci, S;
- Flaecher, H;
- Fruth, T;
- Gaitskell, RJ;
- Genovesi, J;
- Ghag, C;
- Gilchriese, MGD;
- Gokhale, S;
- van der Grinten, MGD;
- Hall, CR;
- Hans, S;
- Harrison, J;
- Haselschwardt, SJ;
- Hertel, SA;
- Hor, JY-K;
- Horn, M;
- Huang, DQ;
- Ignarra, CM;
- Jahangir, O;
- Ji, W;
- Johnson, J;
- Kaboth, AC;
- Kamdin, K;
- Khaitan, D;
- Khazov, A;
- Kim, WT;
- Kocher, CD;
- Korley, L;
- Korolkova, EV;
- Kras, J;
- Kraus, H;
- Kravitz, SW;
- Kreczko, L;
- Krikler, B;
- Kudryavtsev, VA;
- Leason, EA;
- Lee, J;
- Leonard, DS;
- Lesko, KT;
- Levy, C;
- Li, J;
- Liao, J;
- Liao, F-T;
- Lin, J;
- Lindote, A;
- Linehan, R;
- Lippincott, WH;
- Liu, R;
- Liu, X;
- Loniewski, C;
- Lopes, MI;
- Paredes, B López;
- Lorenzon, W;
- Luitz, S;
- Lyle, JM;
- Majewski, PA;
- Manalaysay, A;
- Manenti, L;
- Mannino, RL;
- Marangou, N;
- Marzioni, MF;
- McKinsey, DN;
- McLaughlin, J;
- Meng, Y;
- Miller, EH;
- Monzani, ME;
- Morad, JA;
- Morrison, E;
- Mount, BJ;
- Murphy;
- Naim, D;
- Naylor, A;
- Nedlik, C;
- Nehrkorn, C;
- Nelson, HN;
- Neves, F;
- Nikoleyczik, J;
- Nilima, A;
- Olcina, I;
- Oliver-Mallory, KC;
- Pal, S;
- Palladino, KJ;
- Pease, EK;
- Penning, BP;
- Pereira, G;
- Piepke, A;
- Pushkin, K;
- Reichenbacher, J;
- Rhyne, CA;
- Riffard, Q;
- Rischbieter, GRC;
- Rodrigues, JP;
- Rosero, R;
- Rossiter, P;
- Rutherford, G;
- Sazzad, ABMR;
- Schnee, RW;
- Schubnell, M;
- Scovell, PR;
- Seymour, D;
- Shaw, S;
- Shutt, TA;
- Silk, JJ;
- Silva, C;
- Solmaz, M;
- Solovov, VN;
- Sorensen, P;
- Stancu, I;
- Stevens, A;
- Stiegler, TM;
- Stifter, K;
- Szydagis, M;
- Taylor, WC;
- Taylor, R;
- Temples, D;
- Terman, PA;
- Tiedt, DR;
- Timalsina, M;
- Tomás, A;
- Tripathi, M;
- Tvrznikova, L;
- Utku, U;
- Uvarov, S;
- Vacheret, A;
- Wang, JJ;
- Watson, JR;
- Webb, RC;
- White, RG;
- Whitis, TJ;
- Wolfs, FLH;
- Woodward, D;
- Yin, J;
- Collaboration)
Published Web Location
https://doi.org/10.1016/j.astropartphys.2019.102391Abstract
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 40K and the 238U and 232Th 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 4850-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 from the cavern walls of 1.9 ± 0.4 γ cm − 2 s − 1 . The resulting activity in the walls of the cavern can be characterised as 220 ± 60 Bq/kg of 40K, 29 ± 15 Bq/kg of 238U, and 13 ± 3 Bq/kg of 232Th.
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