status of cobra 6 th snolab workshop, 22.8.2007 picture courtesy [email protected]
TRANSCRIPT
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COBRA
Use large amount of CdZnTe Semiconductor Detectors
Array of 1cm3
CdZnTe detectors
K. Zuber, Phys. Lett. B 519,1 (2001)
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Isotopes
Zn70 0.62 1001 ß-ß- Cd114 28.7 534 ß-ß- Cd116 7.5 2809 ß-ß- Te128 31.7 868 ß-ß- Te130 33.8 2529 ß-ß- Zn64 48.6 1096 ß+/EC Cd106 1.21 2771 ß+ß+ Cd108 0.9 231 EC/EC Te120 0.1 1722 ß+/EC
nat. ab. (%) Q (keV) Decay mode
COBRA: CdZnTe semiconductors
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V.K.B. Kota, priv. comm.
116Cd comes of best...
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Advantages
• Source = detector
• Semiconductor (Good energy resolution, clean)
• Room temperature
• Tracking („Solid state TPC“)
• Modular design (Coincidences)
• Industrial development of CdTe detectors
• Two isotopes at once
• 116Cd above 2.614 MeV
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COBRA collaboration
University of Surrey (UK), University of Hamburg (Germany),Technical University Prague (Tschech Rep.), Jagellonian University (Poland),Louisianna State University (USA)
University of Dortmund
University of Sussex
Laboratori Nazionali del Gran Sasso
University of Warwick
University of Birmingham
University of Liverpool
University of York
Rutherford Appleton Laboratory
University of Bratislava
Washington University at St. Louis
Material Research Centre Freiburg
More welcome
University of Jyvaskyla
University of La Plata
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COBRA at LNGS
COBRASince april 20072004-march 2007
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worldbest
First COBRADouble beta results
T. Bloxham et al., arXiv:0707.2756,,Phys. Rev. C 76, 025501 (2007)
PertinaxCopper CZTWax
Based on 4 detectors, total of 4.34 kg x days
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Redesigned prototype
Delrin holder and kapton foilScalable design for larger masses
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The 64 array - the next step4x4x4 detector array = 0.42 kg CdZnTe semiconductors
Zur Anzeige wird der QuickTime™ Dekompressor „Cinepak“
benötigt.
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The first layer
Installed at LNGS in april 2006, world wide largest array of this type of detector, remaining 48 will be installed autumn 2007
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The first layer - some spectraCd-113 beta decaywith half-life of about 1016 yrs
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The first layer - Coincidences
Just starting to analyse/understand the power of that..
Preliminary
Coincidences around Det 7
Example:3-coincidence
Powerful tool!!!
Coincidences
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Example: 130Te 1st excited state
1. 1 Detector with 2530 keV2. 1 Detector with 1994 keV3. 2 Detectors (One with
1994 keV, one with 536 keV))4. 2 Detectors (One with
1994 keV, two sum up to 536 keV)
€
130Te→130Xe∗+ 2e− + γ (536keV )
Have performed a search for mode 3 in 4.2 kg x days and foundno event !
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New passivation (4 detectors)
Sample measurements at ICP-MS @ LNGSsuggest improvement of about 3 orders of magnitude
Monte Carloexpectation
Paint contribution at 2.8 MeV: about 0.2 counts/keV/kg/yr
Major background so far: Red paint on detector surface
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New passivation
Very preliminary: At least a factor 10 better, lot of construction workaround COBRA at LNGS, no coincidences, no nitrogen flushing...
Around 10 counts/keV/kg/yr
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Sensitivity
50 meV
€
T1/ 2 ∝ M × t /ΔE × B
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Energy Resolution
• Only electron signal read out (CPG technology)• Possible improvements: cooling, new grids• Better detectors are available
E = 1.9% @ 2.8MeV
=2.9% @ 662keV
Resolution of =0.8% at 2.8 MeV
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2 - decay
€
F =8Q(ΔE /Q)6
me= 3.7*10−10
S. Elliott, P. Vogel, Ann. Rev. Nucl. Part. Sci. 2002
Energy resolution (FWHM) important semiconductor
Fraction of 2 in 0 peak:
Signal/Background:
4331
02/1
22/1 ==
TT
FBS
yrsT 1922/1 102.3 ×=
yrsT 2602/1 102×=
2 is ultimate, irreducible background
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The solid state TPCEnergy resolution Tracking
Pixelated CdZnTe detectors
• Massive backgroundreduction• Positive signal information
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Pixelisation - I• Massive BG reduction by particle ID , 200m pixels (example simulations):
• eg. Could achieve nearly 100% identification of 214Bi events (214Bi 214Po 210Pb).
00
1-1.5mm1-1.5mm
~15~15mm
3 MeV 3 MeV
7.7MeV life-time = 164.3s
Beta withendpoint 3.3MeV
= 1 pixel, and = several connected pixel, = some disconnected p.
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Rejection power of pixels
First look on rejection power
Suggests a background reduction of 1000!
T. Bloxham, M. Freer,Nucl. Inst. Meth. A 572, 722 (2007)
Likelihood using:
-Number of pixels
- spatial separation
- energy loss (dE/dx)
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Pixelisation - II Running 256 pixel det with ASIC, 1.6mm pixel size
crystal
ASIC readout
122 keV
136 keV
Single pixel 57Co spectrum
Additional 16 pixel detectorwith conventional readout running
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Pixel detectors - next step
64 pixel detectors 2x2x0.5 cm3
Pixel electrodes will be replaced by 200 m pixels, mask in hand
By end 2007 we‘ll have two high resolution pixel detectors
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Pixellated detectors
2D - Pixelisation on both electrodes
Solid state TPC
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COBRA for solar neutrinos - King COBRA
116Cd
116In
116Sn
A real time low-energy solar neutrino experiment?
Threshold energy: 464 keV
7Be contribution g.s. alone: 227 SNU
= 14s
K. Zuber, Phys. Lett. B 571,148 (2003)
e
ee
Current idea: 40x40x40 CdZnTe detectors = 420 kg, enriched in 116Cd
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Summary
• COBRA is a new approach to double beta decay using CdZnTe semiconductors
• Follows two lines: Background identification and reduction (LNGS) and development of high resolution pixel-CZT
• Two major items for 2007:Finish the 64 array at LNGS in new locationTwo high resolution pixel detectors
• Revived interest in neutrinoless double EC• Possible interest to come to SNOLAB early 201x• Progress is fast....
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