UCL Discovery Stage
UCL home » Library Services » Electronic resources » UCL Discovery Stage

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

Akerib, DS; Akerlof, CW; Akimov, DY; Alsum, SK; Araújo, HM; Arnquist, IJ; Arthurs, M; ... Zhang, C; + view all (2017) Identification of Radiopure Titanium for the LZ Dark Matter Experiment and Future Rare Event Searches. Astroparticle Physics , 96 pp. 1-10. 10.1016/j.astropartphys.2017.09.002. Green open access

[thumbnail of Dobson_1-s2.0-S0927650517300592-main.pdf]
Preview
Text
Dobson_1-s2.0-S0927650517300592-main.pdf - Accepted Version

Download (779kB) | Preview

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.

Type: Article
Title: Identification of Radiopure Titanium for the LZ Dark Matter Experiment and Future Rare Event Searches
Open access status: An open access version is available from UCL Discovery
DOI: 10.1016/j.astropartphys.2017.09.002
Publisher version: http://doi.org/10.1016/j.astropartphys.2017.09.002
Language: English
Additional information: © 2017 Elsevier B.V. All rights reserved. This version is the author accepted manuscript. For information on re-use, please refer to the publisher’s terms and conditions.
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy
URI: https://discovery-pp.ucl.ac.uk/id/eprint/1552516
Downloads since deposit
2,916Downloads
Download activity - last month
Download activity - last 12 months
Downloads by country - last 12 months

Archive Staff Only

View Item View Item