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Columbia Astrophysics Laboratory

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Presentation on theme: "Columbia Astrophysics Laboratory"— Presentation transcript:

1 Columbia Astrophysics Laboratory
Cryogenics and Cryostat Design Karl-Ludwig Giboni Columbia Astrophysics Laboratory XENON1T Meeting Zuerich, 27 February, 2010

2 Mass Increase by factor 10 – 20, but not simple scale up.
XENON100 : 50 kg fiducial. 170 kg total XENON1T : 1000kg fiducial, 2400 kg total Mass Increase by factor 10 – 20, but not simple scale up. Main reason for changes: Cryostat : 1. Size Shield with Water or Liquid Scintillator Opening to Top Copper design for lower background Limited cooling Power Cryogenics : 1. Limited cooling Power Filling and Recovery time Long time storage Recirculation Rate

3 i.e. servicing detector in situ.
Size Instead of 170 kg there will be 2.5T filling the cryostat, i.e stronger support structures needed Access to interior has to be easier than XENON100, but pieces to be moved are bulkier and heavier. Shield with Water or Liquid Scintillator Early assumption started from passive (Lead-Poly) design Many ideas not easily applicable to water or L.S. shield Large water shield might be to high to remove detector from top, i.e. servicing detector in situ. Safety issues must be addressed

4 Limited Cooling Power We will never have 10 PTRs. Maximum 2. We need spare cooler, i.e. 2 coolers including the spare. Thinner supporting materials (Copper?, Titanium?) Better thermal insulation Cryostat design is not only influenced by shield, but also by TPC design However, we should not forget the lessons learned from XENON10 and XENON100

5 Filling and Recovery Time
For 170 kg we need about 2.5 days, i.e. about 1 month for 2.4 ton, but limited cooling power. If we store xenon in liquid form, transfer rate 100 liter(liquid)/hour with Barber Nichols pump, as in MEG, i.e. fill time < 1 day. Similar time for recovery in liquid form. Time to prepare liquid for filling, e..g. Krypton removal, during experiment set up time. Long Term Storage We cannot handle battery of 50 2A cylinders underground. Concept similar to MEG. Transfer xenon to liquid dewar for storage. 1000 liter dewar with PTR for cooling. Low thermal losses (< 20 W) Design by Taiyo Nissan Sanso. Without cooling: Pressure rise over 45 hours is < 1 atm? No additional emergency storage necessary.

6 MEG Set Up Detector Liquid Storage Tank Purification System
Gas Storage Tank We want 2 dewars for off-line xenon circulation for purification and Krypton removal

7 Liquid Storage Gas Storage 1 Tank 1000 liter <20 W Thermal Loss 1 PTR 8 Tanks 250 liter each 60 bars 360 kg each

8 Pressure Rise in Liquid Tank with No Cooling
0.9 atm in 44 hours

9 Recirculation Rate Cooling power will be very limited in XENON1T.
During recirculation 1 PTR (200 W) We have to cover heat losses in detector, and leave some room for PID regulator. New tests at Nevis with small system Small PTR with limited cooling power (29 W total) Commercial brazed plate exchanger All stainless steel, copper brazed Similar model, but different manufacturer Used for small PET test system at KEK

10 Flat Plate Model FG3X8-20, GEA PHE Systems
Cooling Power Limit for PDC08: 29 W Heat Losses: 12.5 W Slope: 0.34 W/SLPM Offset: 2.26 W Efficiency: 96.6 %

11 Extrapolation to PC150 PTR, i.e. XENON100
Without other limitations the flow rate would be limited to 250 – 300 SLPM. If these rates are possible, liquid recirculation would be not necessary, and too difficult For the cryogenics there is a baseline concept, but this also still requires some work. Of course, there might be concepts which are better suited, but the development time is limited.


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