Status of Corrado and GeMPI III SpectrometersStatus of Corrado and GeMPI III Spectrometers W....

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Status of Corrado and GeMPI III Spectrometers W. Hampel, Mark Heisel , G.Heusser, M. Laubenstein, W. Maneschg, S. Schönert and H. Simgen Gerda Collaboration Meeting Ringberg Castle, February 2007

Transcript of Status of Corrado and GeMPI III SpectrometersStatus of Corrado and GeMPI III Spectrometers W....

Status of Corrado and GeMPI III Spectrometers

W. Hampel, Mark Heisel, G.Heusser, M. Laubenstein, W. Maneschg, S. Schönert and H. Simgen

Gerda Collaboration MeetingRingberg Castle, February 2007

12/02/07 2Mark Heisel – MPI für Kernphysik, Heidelberg

Design of Corrado

located in Low-Level-Lab (15m w.e.) at MPIK in Heidelberg

coaxial, p-type0.96 kgwith aluminum cap

HP Ge-crystal:

sample camber (20x20x35 cm3):allows for N2 flushing from dewer evaporationpassive shielding:5cm Cu and 15-20cm Pb

active shielding:MWPC in anticoincidence~104μ/min @40ms dead time

expected sensitivity:

~10µBq/kg

12/02/07 3Mark Heisel – MPI für Kernphysik, Heidelberg

Status of Corradoassembly of detector, shielding system and electronics completed early this year

the first spectra have been taken (see next slide)MC-model of geometry is available

upcoming activities:fine tuning of electronics(optimising efficiency and resolution of crystal and veto)dead layer determinationlong background measurement

Corrado is expected to be ready for screening in 5-8 weeks

12/02/07 4Mark Heisel – MPI für Kernphysik, Heidelberg

First BG-spectrum of Corrado

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without veto (3.8 days)

with veto (1.9 days)

background supression by veto is 88% - to be improved

total count rate (40-2700 keV) is slighty worse than in Dario (with veto):

no line-BG observed (yet):

Dario 2.5 cpd/chnCorrado 3.8 cpd/chn

Tl-208 (@2615 keV):Dario 13.1 cpdCorrado ≤ 3 cpd

12/02/07 5Mark Heisel – MPI für Kernphysik, Heidelberg

Design of GeMPI III

located at LNGS (3500m w.e.)customized HP Ge-crystal in LENS-copper cryostat & roman lead as FET-shield:

sample chamber (25x25x25 cm3):passive shielding:5cm Cu and 20cm Pbradon tight steel casing with airlock

constantly flushed with boil off nitrogen

coaxial, p-type2.2 kg

12/02/07 6Mark Heisel – MPI für Kernphysik, Heidelberg

12/02/07 7Mark Heisel – MPI für Kernphysik, Heidelberg

12/02/07 8Mark Heisel – MPI für Kernphysik, Heidelberg

12/02/07 9Mark Heisel – MPI für Kernphysik, Heidelberg

12/02/07 10Mark Heisel – MPI für Kernphysik, Heidelberg

12/02/07 11Mark Heisel – MPI für Kernphysik, Heidelberg

12/02/07 12Mark Heisel – MPI für Kernphysik, Heidelberg

12/02/07 13Mark Heisel – MPI für Kernphysik, Heidelberg

12/02/07 14Mark Heisel – MPI für Kernphysik, Heidelberg

12/02/07 15Mark Heisel – MPI für Kernphysik, Heidelberg

12/02/07 16Mark Heisel – MPI für Kernphysik, Heidelberg

12/02/07 17Mark Heisel – MPI für Kernphysik, Heidelberg

12/02/07 18Mark Heisel – MPI für Kernphysik, Heidelberg

12/02/07 19Mark Heisel – MPI für Kernphysik, Heidelberg

12/02/07 20Mark Heisel – MPI für Kernphysik, Heidelberg

12/02/07 21Mark Heisel – MPI für Kernphysik, Heidelberg

very first spectrum of GeMPI III

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mainly 222Rn (214Bi) lines from air in sample chamber visible (expected)

resolution worsened from 2.68keV (FWHM @1333keV) to ~4keV

high 207Bi contamination! 570keV: 171+/-18 cts 1064keV: 108+/-13 cts

latest bad news:

only 4.6 days counting

- counts at 2615keV (208Tl) (could be 208Bi as well)- x-rays from Pb/Bi- maybe 137Cs

12/02/07 22Mark Heisel – MPI für Kernphysik, Heidelberg

where does the 207Bi come from?ratio of counts:

in comparision with the 214Bi from the air in the chamber (1120keV / 609keV)

5cm Cu changes R by factor >2, 5cm Pb by factor >30.

i.e. 207Bi lies inside of shieldingpossible production process via (p,n)-reaction with 207Pb

then 208Bi should be produced as well and could be an explanation for the counts around 2615keV

picture of GeMPI II cryostat by Marty Keillor

83.01064

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82.0214 =BiR (errors ~15%)

prelim

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s!

12/02/07 23Mark Heisel – MPI für Kernphysik, Heidelberg

upcoming activities

take a background spectrum with good statistics and a nitrogen flushed chamber to get a clear picture of the contamination

create MC model of detector and perform simulations of possible origins of the contamination

once identified: open shielding and get rid of the contamination

make GeMPI III run smooth and clean

12/02/07 24Mark Heisel – MPI für Kernphysik, Heidelberg

Matthias Laubenstein Herbert Strecker Theo Apfel Mark Heisel Michael Reisfelder