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Search for Dark Matter at CJPL with PANDAX. Kirill Pushkin for the PANDAX Collaboration, 10 th Rencontres du Vietnam, Very High Energy Phenomena in the Universe, August 3-9, 2014. Contents. Introduction Experiment Commissioning. Data taking. Prospects and summary.
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Search for Dark Matter at CJPL with PANDAX Kirill Pushkin for the PANDAX Collaboration, 10th Rencontres du Vietnam, Very High Energy Phenomena in the Universe, August 3-9, 2014
Contents • Introduction • Experiment • Commissioning. Data taking. • Prospects and summary
The PANDAX Collaboration • Collaboration started in 2009 (includes ~40 people) • 7 institutions Shanghai Jiao Tong University, Shandong University, Shanghai Institute of Applied Physics, CAS, Beijing University, Yalong Hydropower Co., Ltd. http://pandax.org University of Michigan (USA) University of Maryland (USA)
China JinPingUnderground Laboratory (CJPL) • μ – veto system unnecessary • compact shielding structure possible • easy access by road • future plans for CJPL II • ~2400 m overburden of rock • Deepest underground lab in operation 6720 m.w.e. ~57 muons/(year x m2) • Low radioactivity marble rock • Easy access – located in the middle of the 18 km tunnel
CJPL SURF SURF
The PANDAX laboratory Ge counting station Xe detector Storage bottles with Gas Xenon
The PANDAX Detector • Dual phase Xe detector • Probing WIMP-nucleon cross section • Designed for 1 T fiducial mass
III stages for PANDAX Stage I Stage III Stage I: 125 kg xenon target, 400 kg total mass Stage II: 500 kg xenon target, 1.3T total mass Stage III: 1.5 ton target, 3T total mass Stage II
External shielding Passive shield Rn purge with N2 gas • Reduces background from surrounding • rocks and concrete • Passive shield allows accommodating • a large, 1T, scale detector • Continuous flush with boiled-off LN2 • Levels of Rn achieved < 1 Bq/m3 (limited by the • sensitivity of the used Rn detector
Cryogenics Cooling power ~180 W (-96 degrees of Celsius) LN cooling Pulse Tube Refrigerator Heat exchanger
Stage I TPC Detector characteristics: • TPC radius: 30 cm • Drift length: 15.4 cm • Total Xenon mass: 400 kg • Sensitive target: Xe mass: 125 kg • Fiducial volume: Xe mass 37 kg • Top PMTs array (1”, R8520): 143 • Bottom PMTs array (3”, R11410): 37
Background control: Detector materials counting Use materials with low radioactivity: 238U, 232Th, 40K, 60Co
PMT calibration with LEDs • LED calibrations: • 2 Teflon ball diffusers on top PMT array • LED and diffusers are coupled to optical fibers and feedthroughs • Gains balanced at ~2x106
Calibration data system We can insert a gamma or neutron source into the tubing to calibrate the detector 3D position reconstruction important for further background reduction
Xenon purity • Electron lifetime ~262 us (drift time 20-80 us)
S2 vs S1 light anticorrelation 80 keV (Xe-131) 40 keV (Xe-129)
Radioactive background: Kr in Xe Radioisotope Kr-85, T1/2=10.756 years. Beta maximum energy decay 687 keV • We employ a home made distillation column to remove Kr from gaseous Xe. • We use an ultrasensitive Purity Analysis System based on RGA (MKS E-Vision 2). • The amount of Kr-84 in our Xe after the distillation is of the order of ppt which can be subsequently recalculated into the amount of Kr-85 in Xe. Kr-Xe distillation system
Calibration measurements of Kr-84 in Xe gas Purity Analysis System Measured by K. Pushkin and He Min
Sensitivity projection (Stage I after 100 days of taking data) Leffcutoff below 3 keV Leff no cut off below 3 keV Stay tuned for the Physics Results (17 days Dark Matter data paper will be released VERY SOON)
Upgrade: Stage II • Goals: • Upgrade in preparations. Stay tuned for more exciting news • Sensitivity reach 2x10-46 cm2 at 100 GeV • with 54000 kg-day.
Summary • PANDAX has made a good progress in the past year. Currently, the experiment is taking data. • Stay tuned for the coming 17 days Dark Matter data paper (expected to appear VERY SOON on arXiv). • Currently, we are upgrading the detector, Stage I, to Stage II.