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Development of the liquid level meters for the PandaX dark matter detector

Development of the liquid level meters for the PandaX dark matter detector
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摘要 The two-phase xenon detector is at the frontier of dark matter direct search. This kind of detector uses liquid xenon as the sensitive target and is operated in two-phase (liquid/gas) mode, where the liquid level needs to be monitored and controlled in sub-millimeter precision. In this paper, we present a detailed design and study of two kinds of level meters for the PandaX dark matter detector. The long level meter is used to monitor the overall liquid level while short level meters are used to monitor the inclination of the detector. These level meters are cylindrical capacitors that are custom-made from two concentric metal tubes. Their capacitance values are read out by a universal transducer interface chip and are recorded by the PandaX slow control system. We present the developments that lead to level meters with long-term stability and sub-millimeter precision. Fluctuations (standard deviations) of less than 0.02 mm for the short level meters and less than 0.2 mm for the long level meter were achieved during a few days of test operation. The two-phase xenon detector is at the frontier of dark matter direct search. This kind of detector uses liquid xenon as the sensitive target and is operated in two-phase (liquid/gas) mode, where the liquid level needs to be monitored and controlled in sub-millimeter precision. In this paper, we present a detailed design and study of two kinds of level meters for the PandaX dark matter detector. The long level meter is used to monitor the overall liquid level while short level meters are used to monitor the inclination of the detector. These level meters are cylindrical capacitors that are custom-made from two concentric metal tubes. Their capacitance values are read out by a universal transducer interface chip and are recorded by the PandaX slow control system. We present the developments that lead to level meters with long-term stability and sub-millimeter precision. Fluctuations (standard deviations) of less than 0.02 mm for the short level meters and less than 0.2 mm for the long level meter were achieved during a few days of test operation.
出处 《Chinese Physics C》 SCIE CAS CSCD 2014年第5期53-57,共5页 中国物理C(英文版)
基金 Supported by National Science Foundation of China(11055003,11175117) Science and Technology Commission of Shanghai Municipality(11PJ1405300) Ministry of Science and Technology of China(2010CB833005)
关键词 liquid level meter XENON dark matter liquid level meter, xenon, dark matter
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参考文献6

  • 1GONG H, Giboni K L, JI X, TAN A, ZHAO L. The Cryogenic System for the PandaX Dark Matter Search Experiment, 2013 JINST 8 P 01002[arXiv:1207.510.
  • 2Aprile E, Alfonsi M, Arisaka K et al. (XENON100 collaboration). Phys. Rev. Lett., 2012, 109: 181301[arXiv:1207.598.
  • 3Plante G. The XENON100 Dark Matter Experiment: Design, Construction, Calibration and 2010 Search Results with Improved Measurement of the Scintillation Response of Liquid Xenon to Low-Energy Nuclear Recoils. PhD Thesis. Columbia University, New York, 2012.
  • 4Smartec Company. http://www.smartec-sensors.com/en/pro-ducts/uti-interface-en.html.
  • 5Schmidt W F. The Basic Properties of Liquid Xenon as Related to its Application in Radiation Detectors, in Technique and Application of Xenon Detectors. Proceedings of the International Workshop. Edited by Suzuki Y, Nakahata M, Koshio Y, Moriyama S. Singerpore: World Scientific, 2002.
  • 6MDC Vacuum Products. http://www.mdcvacuum.com/ displaypart.aspx?p=680502.
  • 1SONG Jianlan.Tracking the Voice of Dark Matter in Space[J].Bulletin of the Chinese Academy of Sciences,2015,29(4):209-210.
  • 2K.A.Olive,K.Agashe,C.Amsler,M.Antonelli,J.-F.Arguin,D.M.Asner,H.Baer,H.R.Band,R.M.Barnett,T.Basaglia,C.W.Bauer,J.J.Beatty,V.I.Belousov,J.Beringer,G.Bernardi,S.Bethke,H.Bichsel,O.Biebe,E.Blucher,S.Blusk,G.Brooijmans,O.Buchmueller,V.Burkert,M.A.Bychkov,R.N.Cahn,M.Carena,A.Ceccucci,A.Cerr,D.Chakraborty,M.-C.Chen,R.S.Chivukula,K.Copic,G.Cowan,O.Dahl,G.D'Ambrosio,T.Damour,D.de Florian,A.de Gouvea,T.DeGrand,P.de Jong,G.Dissertor,B.A.Dobrescu,M.Doser,M.Drees,H.K.Dreiner,D.A.Edwards,S.Eidelman,J.Erler,V.V.Ezhela,W.Fetscher,B.D.Fields,B.Foster,A.Freitas,T.K.Gaisser,H.Gallagher,L.Garren,H.-J.Gerber,G.Gerbier,T.Gershon,T.Gherghetta,S.Golwala,M.Goodman,C.Grab,A.V.Gritsan,C.Grojean,D.E.Groom,M.Grnewald,A.Gurtu,T.Gutsche,H.E.Haber,K.Hagiwara,C.Hanhart,S.Hashimoto,Y.Hayato,K.G.Hayes,M.Heffner,B.Heltsley,J.J.Hernandez-Rey,K.Hikasa,A.Hocker,J.Holder,A.Holtkamp,J.Huston,J.D.Jackson,K.F.Johnson,T.Junk,M.Kado,D.Karlen,U.F.Katz,S.R.Klein,E.Klempt,R.V.Kowalewski,F.Krauss,M.Kreps,B.Krusche,Yu.V.Kuyanov,Y.Kwon,O.Lahav,J.Laiho,P.Langacker,A.Liddle,Z.Ligeti,C.-J.Lin,T.M.Liss,L.Littenberg,K.S.Lugovsky,S.B.Lugovsky,F.Maltoni,T.Mannel,A.V.Manohar,W.J.Marciano,A.D.Martin,A.Masoni,J.Matthews,D.Milstead,P.Molaro,K.Monig,F.Moortgat,M.J.Mortonson,H.Murayama,K.Nakamura,M.Narain,P.Nason,S.Navas,M.Neubert,P.Nevski,Y.Nir,L.Pape,J.Parsons,C.Patrignani,J.A.Peacock,M.Pennington,S.T.Petcov,Kavli IPMU,A.Piepke,A.Pomarol,A.Quadt,S.Raby,J.Rademacker,G.Raffel,B.N.Ratcliff,P.Richardson,A.Ringwald,S.Roesler,S.Rolli,A.Romaniouk,L.J.Rosenberg,J,L.Rosner,G.Rybka,C.T.Sachrajda,Y.Sakai,G.P.Salam,S.Sarkar,F.Sauli,O.Schneider,K.Scholberg,D.Scott,V.Sharma,S.R.Sharpe,M.Silari,T.Sjostrand,P.Skands,J.G.Smith,G.F.Smoot,S.Spanier,H.Spieler,C.Spiering,A.Stahl,T.Stanev,S.L.Stone,T.Sumiyoshi,M.J.Syphers,F.Takahashi,M.Tanabashi,J.Terning,L.Tiator,M.Titov,N.P.Tkachenko,N.A.Tornqvist,D.Tovey,G.Valencia,G.Venanzoni,M.G.Vincter,P.Vogel,A.Vogt,S.P.Wakely,W.Walkowiak,C.W.Walter,D.R.Ward,G.Weiglein,D.H.Weinberg,E.J.Weinberg,M.White,L.R.Wiencke,C.G.Wohl,L.Wolfenstein,J.Womersley,C.L.Woody,R.L.Workman,A.Yamamoto,W.-M.Yao,G.P.Zeller,O.V.Zenin,J.Zhang,R.-Y.Zhu,F.Zimmermann,P.A.Zyla,G.Harper,V.S.Lugovsky,P.Schaffner.DARK MATTER[J].Chinese Physics C,2014,38(9):353-360.
  • 3Chang Jin.Status and Perspectives of Dark Matter Searches in China[J].空间科学学报,2010,30(5):422-423.
  • 4HUANG Jin-feng NI Bang-fa GUAN Yong-jing TIIAN Wei-zhi ZHANG Gui-ying ZHAO Chang-jun GAO Si-ze HUANG Dong-hui XIAO Cai-jin LIU Cun-xiong ZHANG Hai-qing SUN Hong-chao YUAN Guo- jun LIU Chao.Preliminary Design of A Superheated Droplet Detection Device for Search of Dark Matter[J].Annual Report of China Institute of Atomic Energy,2010(1):136-137.
  • 5ZHANG Gui-ying NI Bang-fa ZHAO Chang-jun GAO Si-ze HUANG Jin-feng TIAN Wei-zhi WANG Ping-sheng HUANG Dong-hui LIU Cun-xiong XIAO Cai-jin ZHANG Hai-qing SUN Hong-chao LIU Chao.Preliminary Study on Bubble Detectors for Dark Matter Search[J].Annual Report of China Institute of Atomic Energy,2010(1):133-134.
  • 6CHANG Jin,FAN Yizhong.Indirect Searches of Dark Matter in Space[J].Bulletin of the Chinese Academy of Sciences,2011,25(3):161-163.
  • 7XIAO MengJiao,XIAO Xiang,ZHAO Li,CAO XiGuang,CHEN Xun,CHEN YunHua,CUI XiangYi,FANG DeQing,FU ChangBo,GIBONI Karl L.,GONG HaoWei,GUO GuoDong,HU Jie,HUANG XingTao,JI XiangDong,JU YongLin,LEI SiAo,LI ShaoLi,LIN Qing,LIU HuaXuan,LIU JiangLai,LIU Xiang,LORENZON Wolfgang,MA YuGang,MAO YaJun,NI KaiXuan,PUSHKIN Kirill,REN XiangXiang,SCHUBNELL Michael,SHEN ManBing,STEPHENSON Scott,TAN AnDi,TARL Greg,WANG HongWei,WANG JiMin,WANG Meng,WANG XuMing,WANG Zhou,WEI YueHuan,WU ShiYong,XIE PengWei,YOU YingHui,ZENG XiongHui,ZHANG Hua,ZHANG Tao,ZHU ZhongHua.First dark matter search results from the PandaX-Ⅰ experiment[J].Science China(Physics,Mechanics & Astronomy),2014,57(11):2024-2030. 被引量:13
  • 8暗物质的运动模式[J].大科技(科学之谜)(A),2006(4):35-35.
  • 9Yan Ma Yanmin Niu Min Lei.Design and Study of the Active Router Structure[J].通讯和计算机(中英文版),2005,2(9):75-78.
  • 10Bing-Lin Young.A survey of dark matter and related topics in cosmology[J].Frontiers of physics,2017,12(2):1-219. 被引量:1

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