Identification of radiopure titanium for the LZ dark matter experiment and future rare event searches

dc.contributor.author Akerib, D. S.
dc.contributor.author Akerlof, C. W.
dc.contributor.author Akimov, D. Yu
dc.contributor.author Alsum, S. K.
dc.contributor.author Araújo, H. M.
dc.contributor.author Arnquist, I. J.
dc.contributor.author Arthurs, M.
dc.contributor.author Bai, X.
dc.contributor.author Bailey, A. J.
dc.contributor.author Balajthy, J.
dc.contributor.author Balashov, S.
dc.contributor.author Barry, M. J.
dc.contributor.author Belle, J.
dc.contributor.author Beltrame, P.
dc.contributor.author Benson, T.
dc.contributor.author Bernard, E. P.
dc.contributor.author Bernstein, A.
dc.contributor.author Biesiadzinski, T. P.
dc.contributor.author Boast, K. E.
dc.contributor.author Bolozdynya, A.
dc.contributor.author Boxer, B.
dc.contributor.author Bramante, R.
dc.contributor.author Brás, P.
dc.contributor.author Buckley, J. H.
dc.contributor.author Bugaev, V. V.
dc.contributor.author Bunker, R.
dc.contributor.author Burdin, S.
dc.contributor.author Busenitz, J. K.
dc.contributor.author Carels, C.
dc.contributor.author Carlsmith, D. L.
dc.contributor.author Carlson, B.
dc.contributor.author Carmona-Benitez, M. C.
dc.contributor.author Chan, C.
dc.contributor.author Cherwinka, J. J.
dc.contributor.author Chiller, A. A.
dc.contributor.author Chiller, C.
dc.contributor.author Cottle, A.
dc.contributor.author Coughlen, R.
dc.contributor.author Craddock, W. W.
dc.contributor.author Currie, A.
dc.contributor.author Dahl, C. E.
dc.contributor.author Davison, T. J.R.
dc.contributor.author Dobi, A.
dc.contributor.author Dobson, J. E.Y.
dc.contributor.author Druszkiewicz, E.
dc.contributor.author Edberg, T. K.
dc.contributor.author Edwards, W. R.
dc.contributor.author Emmet, W. T.
dc.contributor.author Faham, C. H.
dc.contributor.author Fiorucci, S.
dc.contributor.author Fruth, T.
dc.contributor.author Gaitskell, R. J.
dc.contributor.author Gantos, N. J.
dc.contributor.author Gehman, V. M.
dc.contributor.author Gerhard, R. M.
dc.contributor.author Ghag, C.
dc.contributor.author Gilchriese, M. G.D.
dc.contributor.author Gomber, B.
dc.contributor.author Hall, C. R.
dc.contributor.author Hans, S.
dc.contributor.author Hanzel, K.
dc.contributor.author Haselschwardt, S. J.
dc.contributor.author Hertel, S. A.
dc.contributor.author Hillbrand, S.
dc.contributor.author Hjemfelt, C.
dc.contributor.author Hoff, M. D.
dc.contributor.author Holbrook, B.
dc.contributor.author Holtom, E.
dc.contributor.author Hoppe, E. W.
dc.contributor.author Hor, J. Y.K.
dc.contributor.author Horn, M.
dc.contributor.author Huang, D. Q.
dc.contributor.author Hurteau, T. W.
dc.contributor.author Ignarra, C. M.
dc.contributor.author Jacobsen, R. G.
dc.contributor.author Ji, W.
dc.contributor.author Kaboth, A.
dc.contributor.author Kamdin, K.
dc.contributor.author Kazkaz, K.
dc.contributor.author Khaitan, D.
dc.contributor.author Khazov, A.
dc.contributor.author Khromov, A. V.
dc.contributor.author Konovalov, A. M.
dc.contributor.author Korolkova, E. V.
dc.contributor.author Koyuncu, M.
dc.contributor.author Kraus, H.
dc.contributor.author Krebs, H. J.
dc.contributor.author Kudryavtsev, V. A.
dc.contributor.author Kumpan, A. V.
dc.contributor.author Kyre, S.
dc.contributor.author Lee, C.
dc.contributor.author Lee, H. S.
dc.contributor.author Lee, J.
dc.contributor.author Leonard, D. S.
dc.contributor.author Leonard, R.
dc.contributor.author Lesko, K. T.
dc.contributor.author Levy, C.
dc.contributor.author Liao, F. T.
dc.contributor.author Lin, J.
dc.contributor.author Lindote, A.
dc.date.accessioned 2022-03-27T06:51:38Z
dc.date.available 2022-03-27T06:51:38Z
dc.date.issued 2017-11-01
dc.description.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 238Ue < 1.6 mBq/kg, 238Ul < 0.09 mBq/kg, 232The=0.28±0.03 mBq/kg, 232Thl=0.25±0.02 mBq/kg, 40K < 0.54 mBq/kg, and 60Co < 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 ± 0.001(stat) ± 0.030(sys) counts.
dc.identifier.citation Astroparticle Physics. v.96
dc.identifier.issn 09276505
dc.identifier.uri 10.1016/j.astropartphys.2017.09.002
dc.identifier.uri https://www.sciencedirect.com/science/article/abs/pii/S0927650517300592
dc.identifier.uri https://dspace.uohyd.ac.in/handle/1/10403
dc.title Identification of radiopure titanium for the LZ dark matter experiment and future rare event searches
dc.type Journal. Article
dspace.entity.type
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