pith. sign in

arxiv: 1702.02646 · v5 · pith:F3PXD3MWnew · submitted 2017-02-08 · ⚛️ physics.ins-det · hep-ex

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

D.S. Akerib , C.W. Akerlof , D. Yu. Akimov , S.K. Alsum , H.M. Ara\'ujo , I.J. Arnquist , M. Arthurs , X. Bai
show 197 more authors
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 C. Zhang
This is my paper
classification ⚛️ physics.ins-det hep-ex
keywords cryostattitaniumdarkdetectormatteractivitiesbackgroundbeen
0
0 comments X p. Extension
pith:F3PXD3MW Add to your LaTeX paper What is a Pith Number?
\usepackage{pith}
\pithnumber{F3PXD3MW}

Prints a linked pith:F3PXD3MW badge after your title and writes the identifier into PDF metadata. Compiles on arXiv with no extra files. Learn more

read the original 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.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.