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Title: The%20COBRA%20Experiment


1
The COBRA Experiment
  • Jeanne Wilson
  • University of Sussex, UK
  • On behalf of the COBRA Collaboration
  • TAUP 2007, Sendai, Japan

2
Contents
  • Concept
  • Experimental requirements
  • Energy Resolution
  • Backgrounds
  • Experimental status
  • Published limits
  • New results
  • Coincidences
  • Future work
  • Shielding
  • Pixellisation

3
COBRA the Concept
  • Cadmium Telluride 0-neutrino Beta Decay Research
    Apparatus
  • Build up a large array of CdZnTe semiconductor
    detectors
  • K. Zuber, Phys. Lett. B 519,1 (2001)

1 cm
4
0??? Candidate Isotopes
  • CdZnTe contains 9 ?? Isotopes
  • 116Cd, 130Te, 114Cd, 70Zn, 128Te (?-?-),
  • 64Zn, 106Cd, 108Cd, 120Te (?? ,?EC, EC/EC)
  • Main 0??? candidate 116Cd
  • Endpoint 2805 keV
  • Enrichment to 90
  • Favourable G0?M0?2 ? T1/2 1026 years for 50meV
    ?
  • Also interesting 106Cd
  • Endpoint 2771 keV
  • EC/EC, ?/EC and ?? modes
  • ?/EC - enhanced sensitivity to RH weak currents

M. Hirsch et al., Z. Phys. A 347,151 (1994)
5
Experimental Requirements
  • 64,000 1cm3 crystals 418 kg
  • 90 enriched in 116Cd
  • Backgrounds lt 0.001 count keV-1kg-1year-1
  • Energy Resolution lt 2

6
Energy Resolution
  • 2??? decays
  • T1/2(116Cd)2.71019 y
  • For ?E 2, fraction of 2??? events in 0???
    window 3 10-9
  • 10-5 events/kg/year

S. Elliott, P. Vogel, Ann. Rev. Nucl. Part. Sci.
2002
7
Energy Resolution
?E 1.9 _at_ 2.8MeV 2.9 _at_ 662keV
  • Only electron signal read out (CPG technology)
  • Possible improvements cooling, new grids
  • Better detectors are available

8
Backgrounds
  • Muons, neutrons
  • a, b, g sources
  • Intrinsic and surface contaminants
  • Cosmogenics

Crystals 238U, 232Th decay chains 40K 137Cs 210Po
210Pb on surface Cosmogenic isotopes
Gas 222Rn gas
Delrin Holder 238U,232Th decay chain 40K 137Cs
Chamber walls 210Pb on surface
9
Simulations
  • VENOM - detailed, Geant4 based Monte Carlo
    package used to simulate all aspects of
    background contributions.
  • Optimise shielding design
  • (D. Stewart et al. NIM A571 2007, 651-662)
  • Determine material purity requirements

10
Experimental Status
  • Low-background experiments in LNGS (3500 mwe)
  • 22 proto-type limits published
  • 44 proto-type installed new results
  • New laboratory space, clean room conditions,
    fully automated DAQ and environmental
    control/monitoring.
  • To be upgraded to 444 (64-Array) next month

11
Measured Backgrounds
  • Passivation paint forms dominant background.
  • Many steps being taken to reduce backgrounds
  • New passivation coatings being tested
  • New crystal production at Freiburg materials
    institute (towards enriched 116Cd crystals)
  • New contacting methods, cabling to reduce
    cross-talk and pick-up
  • Materials testing and sourcing
  • Shielding development
  • Pulse shape analysis
  • Coincidences
  • Pixellisation

12
Physics Results - published
  • 4.34 kg.days of 22 proto-type data
  • Measurement of 4-fold forbidden 113Cd ? decay
  • C. Gößling et al. Phys. Rev. C,
  • 2005, 72, 064328
  • T1/2 (8.2 0.2 (stat.) 1.0 (sys))1015 yrs
  • Likelihood analysis for double-beta decay
    signatures
  • T. Bloxham et al. Phys. Rev. C 76,
  • 025501, 2007 (arXiv0707.2756)

13
Physics Results - published
130Te?g.s.
116Cd?g.s.
T. Bloxham et al. Phys. Rev. C 76, 025501, 2007
(arXiv0707.2756)
14
Physics Results - published
T. Bloxham et al. Phys. Rev. C 76, 025501, 2007
(arXiv0707.2756)
15
Physics Results - published
T. Bloxham et al. Phys. Rev. C 76, 025501, 2007
(arXiv0707.2756)
New limits - A. Barabash et al.
(arXivnucl-ex/0703020)
16
Physics Results - New
  • 7.85 kg-days of data
  • 12 detectors operating simultaneously
  • Different backgrounds, thresholds, livetimes,
    efficiencies, resolutions etc. for each
    detector, all folded into likelihood function.

PRELIMINARY
17
New Results
  • PRELIMINARY PRELIMINARY PRELIMINARY

18
New Results
  • PRELIMINARY PRELIMINARY PRELIMINARY
  • Some new world-best limits

19
Coincidence Searches
  • Some rare decays can give distinctive coincidence
    signatures.
  • eg.130Te ? 130Xe 2e-
  • ? 130Xe 536keV

Q 536 1993keV, most likely to stay in same
crystal
Strong chance of escaping to be detected in
nearby crystal
Simulated events, calibrated resolution functions
applied
20
Coincidence Searches
  • Searching for 1993keV (?E) and 536keV (?E)
    coincident energy deposits in data
  • 2 events found ? lt5.32 events (Poissonian 90
    limit)
  • Efficiency from simulation
  • 0.652
  • Leads to a half-life limit of
  • Thalf gt 2.6 x 1019 years (90 C.L.)
  • cf 2.5 x 1020 years from single peak search
  • Efficiencies will increase significantly for
    larger array.
  • 64 array (2 resolution), efficiency 3.2

21
Coincidences
  • ßß (to g.s.) is normally single crystal event
  • Intrinsic 238U and 232Th could be major
    backgrounds, but more likely to trigger multiple
    crystals.
  • Select only single site events for 0?ßß peak
    search
  • For 64K array this reduces 232Th chain events
    from crystals by gt50

Simulated 238U chain events inside detectors No
Energy smearing
22
Timing Coincidences
  • The major contribution to 238U spectrum at 2-3MeV
    is the fast b-a decay
  • 214Bi ? 214Po ? 210Pb
  • gt40 efficiency for tagging 214Bi events
    originating inside the crystals

23
Observation of 214Bi events
  • Surface coating ? self calibrating device!
  • small dead volume
  • Measure of paint activity

T1/2 162 19?s
24
Pixellisation - I
  • Extra information on events with signal energy.
  • 200?m pixels (example simulations)
  • eg. Could achieve nearly 100 identification of
    214Bi events.
  • Bloxham and Freer, NIM A, v572, issue 2, p722-728
    (2007)

?
0???
15?m
1-1.5mm
25
Pixellisation - II
  • Tests of 1616 1.6mm pixel detectors
  • Working on photolithography for 200µm pixel
    detectors.

26
Ssssummary
27
Join the party!
  • Learnt a lot from small proto-type experiments,
    including some interesting physics results.
  • Required energy resolutions can be achieved.
  • Lots of work in progress to reduce backgrounds.

28
  • Ssspare Ssslidesss

29
Shielding and Veto
  • Optimise shielding design for neutrons
  • Size 18.4 m3, Mass 64964 kg
  • Active scintillator component for inner layer
  • Veto any residual external background components
  • Veto ?s from internal backgrounds
  • Enhance sensitivity to ?? decays with high energy
    ?s

detectors
30
?? Modes
p
n
e
e
n
p
  • (A,Z) ? (A,Z-2) 2 e (2?e) ??

Q-4mec2
Q-2mec2
  • e- (A,Z) ? (A,Z-2) e (2?e ) ?/EC

Q
  • 2 e- (A,Z) ? (A,Z-2) (2?e) EC/EC

Enhanced sensitivity to right handed weak
currents (VA)
31
Measured Backgrounds
32
Physics Results - New
PRELIMINARY
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