# Identification of Radiopure Titanium for the LZ Dark Matter Experiment   and Future Rare Event Searches

**Authors:** D.S. Akerib, C.W. Akerlof, D. Yu. Akimov, S.K. Alsum, H.M. Ara\'ujo,, I.J. Arnquist, M. Arthurs, X. Bai, A.J. Bailey, J. Balajthy, S. Balashov,, M.J. Barry, J. Belle, P. Beltrame, T. Benson, E.P. Bernard, A. Bernstein,, T.P. Biesiadzinski, K.E. Boast, A. Bolozdynya, B. Boxer, R. Bramante, P., Br\'as, J.H. Buckley, V.V. Bugaev, R. Bunker, S. Burdin, J.K. Busenitz, C., Carels, D.L. Carlsmith, B. Carlson, M.C. Carmona-Benitez, C. Chan, J.J., Cherwinka, A.A. Chiller, C. Chiller, A. Cottle, R. Coughlen, W.W. Craddock,, A. Currie, C.E. Dahl, T.J.R. Davison, A. Dobi, J.E.Y. Dobson, E., Druszkiewicz, T.K. Edberg, W.R. Edwards, W.T. Emmet, C.H. Faham, S. Fiorucci,, T. Fruth, R.J. Gaitskell, N.J. Gantos, V.M. Gehman, R.M. Gerhard, C. Ghag,, M.G.D. Gilchriese, B. Gomber, C.R. Hall, S. Hans, K. Hanzel, S.J., Haselschwardt, S.A. Hertel, S. Hillbrand, C. Hjemfelt, M.D. Hoff, B., Holbrook, E. Holtom, E.W. Hoppe, J.Y-K. Hor, M. Horn, D.Q. Huang, T.W., Hurteau, C.M. Ignarra, R.G. Jacobsen, W. Ji, A. Kaboth, K. Kamdin, K. Kazkaz,, D. Khaitan, A. Khazov, A.V. Khromov, A.M. Konovalov, E.V. Korolkova, M., Koyuncu, H. Kraus, H.J. Krebs, V.A. Kudryavtsev, A.V. Kumpan, S. Kyre, C., Lee, H.S. Lee, J. Lee, D.S. Leonard, R. Leonard, K.T. Lesko, C. Levy, F.-T., Liao, J. Lin, A. Lindote, R.E. Linehan, W.H. Lippincott, X. Liu, M.I. Lopes,, B. Lopez Paredes, W. Lorenzon, S. Luitz, P. Majewski, A. Manalaysay, L., Manenti, R.L. Mannino, D.J. Markley, T.J. Martin, M.F. Marzioni, C.T., McConnell, D.N. McKinsey, D.-M. Mei, Y. Meng, E.H. Miller, E.Mizrachi, J., Mock, M.E. Monzani, J.A. Morad, B.J. Mount, A.St.J. Murphy, C. Nehrkorn, H.N., Nelson, F. Neves, J.A. Nikkel, J. O'Dell, K. O'Sullivan, I. Olcina, M.A., Olevitch, K.C. Oliver-Mallory, K.J. Palladino, E.K. Pease, A. Piepke, S., Powell, R.M. Preece, K. Pushkin, B.N. Ratcliff, J. Reichenbacher, L., Reichhart, C.A. Rhyne, A. Richards, J.P. Rodrigues, H.J. Rose, R. Rosero, P., Rossiter, J.S. Saba, M. Sarychev, R.W. Schnee, M. Schubnell, P.R. Scovell, S., Shaw, T.A. Shutt, C. Silva, K. Skarpaas, W. Skulski, M. Solmaz, V.N. Solovov,, P. Sorensen, V.V. Sosnovtsev, I. Stancu, M.R. Stark, S. Stephenson, T.M., Stiegler, K. Stifter, T.J. Sumner, M. Szydagis, D.J. Taylor, W.C. Taylor, D., Temples, P.A. Terman, K.J. Thomas, J.A. Thomson, D.R. Tiedt, M. Timalsina,, W.H. To, A. Tom\'as, T.E. Tope, M. Tripathi, L. Tvrznikova, J. Va'vra, A., Vacheret, M.G.D. van der Grinten, J.R. Verbus, C.O. Vuosalo, W.L. Waldron, R., Wang, R. Watson, R.C. Webb, W.-Z. Wei, M. While, D.T. White, T.J. Whitis,, W.J. Wisniewski, M.S. Witherell, F.L.H. Wolfs, D. Woodward, S. Worm, J. Xu,, M. Yeh, J. Yin, and C. Zhang

arXiv: 1702.02646 · 2017-09-28

## TL;DR

This study identifies and characterizes radiopure titanium with extremely low radioactivity levels suitable for constructing the LZ dark matter detector cryostat, significantly reducing background noise in rare event searches.

## Contribution

The paper reports the selection and detailed radioassay of titanium with unprecedented low radioactivity levels for use in dark matter detectors, enabling improved sensitivity in rare event searches.

## Key findings

- Titanium with record low radioactivity levels was identified.
- Monte Carlo simulations show minimal background contribution from the titanium cryostat.
- The low-radioactivity titanium enables more sensitive future dark matter experiments.

## Abstract

The LUX-ZEPLIN (LZ) experiment will search for dark matter particle interactions with a detector containing a total of 10 tonnes of liquid xenon within a double-vessel cryostat. The large mass and proximity of the cryostat to the active detector volume demand the use of material with extremely low intrinsic radioactivity. We report on the radioassay campaign conducted to identify suitable metals, the determination of factors limiting radiopure production, and the selection of titanium for construction of the LZ cryostat and other detector components. This titanium has been measured with activities of $^{238}$U$_{e}$~$<$1.6~mBq/kg, $^{238}$U$_{l}$~$<$0.09~mBq/kg, $^{232}$Th$_{e}$~$=0.28\pm 0.03$~mBq/kg, $^{232}$Th$_{l}$~$=0.25\pm 0.02$~mBq/kg, $^{40}$K~$<$0.54~mBq/kg, and $^{60}$Co~$<$0.02~mBq/kg (68\% CL). Such low intrinsic activities, which are some of the lowest ever reported for titanium, enable its use for future dark matter and other rare event searches. Monte Carlo simulations have been performed to assess the expected background contribution from the LZ cryostat with this radioactivity. In 1,000 days of WIMP search exposure of a 5.6-tonne fiducial mass, the cryostat will contribute only a mean background of $0.160\pm0.001$(stat)$\pm0.030$(sys) counts.

## Figures

9 figures with captions in the complete paper: https://tomesphere.com/paper/1702.02646/full.md

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Source: https://tomesphere.com/paper/1702.02646