Cosmogenic production of Ar 37 in the context of the LUX-ZEPLIN experiment
- Aalbers, J.
- Akerib, D.S.
- Al, Musalhi A.K.
- Alder, F.
- Alsum, S.K.
- Amarasinghe, C.S.
- Ames, A.
- Anderson, T.J.
- Angelides, N.
- Araujo, 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.
- Bras, 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 Douglas
- Lesko, K.T.
- Levy, C.
- Jaison Lee
- Lin, J.
- Lindote, A.
- Linehan, R.
- Lippincott, W.H.
- Liu, X.
- Lopes, M.I.
- Lopez, Asamar E.
- 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.
- Morales, Mendoza J.D.
- 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.
- 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. Suerfu
- Williams, M.
- Wolfs, F.L.H.
- Woodford, S.
- Woodward, D.
- Wright, C.J.
- Xia, Q.
- Xiang, X.
- Xu, J.
- Yeh, M.
DOIAbstract
© 2022 authors. Published by the American Physical Society.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, t...
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