Polaris 3-D CdZnTe (CZT) Gamma-Ray Imaging Spectrometers

Transcription

1 Polaris 3-D CdZnTe (CZT) Gamma-Ray Imaging Spectrometers Zhong He ISOE-ALARA Symposium, January 12, 2015 Acknowledgements: DOD, DOE and DHS

2 John M. Palms Outstanding Innovation Began in early 1960s Thank you!

3 20 Ph.Ds Graduated Inc.

4 Current Orion group members Zhong He Yuefeng Zhu Jim Berry Josh Mann Steven Brown Will Koehler Michael Streicher Sean O Neal Jiyang Chu David Goodman Bennett Williams Jiawei Xia

5 Why CdZnTe? (1) Superior energy resolution Limit of semi. (CdZnTe) % Theoretical limit of scintillators Meas. uncertainty Resolution = Signal amplitude NaI Semiconductors Scintillators 0 2% 2.5-3% 7% 0.2% (High Purity Ge) (LaCl 3 ) (2) Higher sensitivity per unit volume (higher Z and density) compactness CdZnTe( , 6.0), High-purity Ge(32, 5.32) (3) Room-temperature operation (no cryogenic cooling) Wide band-gap Technical challenges (1) Severe hole trapping & electron trapping cause signal deficit (2) Crystal yield (cost) and non-uniformity

6 Before kev X-ray Measured 137 Cs Energy spectrum using conventional (cathode-anode) readout Detector #4E-1 Cathode Anode Baseline offset 137 Cs CdZnTe e- 15mm 662 kev cut-off Signal amplitude = gain (n e 0 ) (normalized electron drift length z) Energy z

7 Improvement Using 3-D Readout Technology 4 ASIC: 40 MHz Full readout on Detector 4E kev Cts (10 4 ) 2 FWHM = 0.41% 2.7 kev 0 Energy (kev) June 2013

8 All-events (no selection) kev Cts (10 5 ) 1 FWHM = 0.58% (3.8 kev) Peak-to-Compton = Energy (kev) June 2013

9 Polaris Systems Eighteen cm 3 CdZnTe detectors (108 cm 3, 648 grams = 1.43 lb) E mc 2 1 e cosθ = 1 ( E1+ E2 ) E2 Performance Goals E/E 1% FWHM (at 662 kev) Real-time γ Imaging + isotope I.D. Number of photons:

10 Polaris 1.1 (GMI ASIC) August 2010

11 Comparing to Other γ Spectrometers Source: Eu D CZT (#4E-1) single-pixel events Resolution = 0.7% FWHM High resolution High isotope selectivity/id & low background

12 Gamma Imaging Capability Polar Angle ( ) Intensity of: 22 Na 60 Co 137 Cs Azimuthal Angle ( ) 1 minute data SBP meas. EIID

13 Energy Range of Compton Imaging Normalized Probability Gamma Energy (KeV) Polaris-H performs Compton imaging for γ-rays with E 250 kev

14 Coded Aperture Imaging at E 250 kev Principle: Recognize unique mask shadows from different incident gamma-ray angles

15 Real-Time Combined Coded Aperture and Compton Imaging 22 Na 122 kev 137 Cs 57 Co 662 kev 511 kev 1275 kev

16 Advanced Capabilities Example 1 Directional spectroscopy

17 Weiyi Wang Yuefeng Zu 60 Co He Willy Kaye 22 Na Chris Wahl 137 Cs 137 Cs Polar Angle Target specific γ-spec. 23 min. data EIID Azimuthal Angle

18 Advanced Capabilities Example 2 Detect and Characterize moving sources

19 Tracking Moving Targets

20 Advanced Capabilities Example 3 3-Dimensional Imaging

21 3D Imaging with a Moving Detector Experiment Lab Bench Desk x y Wall Lab Bench Desk Cs-137 (30 μci) Na-22 (30 μci) How to locate sources in 3D? Detector Array 24

22 MLEM Imaging with a moving detector Energy Window: Cs

23 MLEM Imaging with a moving detector Energy Window: Na-22 26

24 Advanced Capabilities Example 4 Detection of Source Shielding

25 Detection of shielded source 137 Cs behind 3.7-cm steel Source Detector Cs-137 no shielding Shielded sources have unique signatures Also identified a 60 Co source behind 2.7-cm Pb

26 Today and Tomorrow

27 Univ. of Michigan Polaris Technology H3D, Inc. Licensed to

28 Fiestaware Compiled by Dr. Chris Wahl of H3D Inc. Distance: ~ 6 (15 cm) One CdZnTe ( cm 3 ) ~ 14 (36 cm)

29 6 hours (367 counts, imaging 766 and 1000 kev lines)

30 12 hours (786 counts, imaging 766 and 1000 kev lines) Shape of fiestaware start to appear what you can see from an overnight measurement

31 Residual Heat Remover (RHR) Pump Room 10.2 minutes 2.3 x 10 6 counts ~0.4 mrem/hr

32 RHR Pump Room 58 Co Area source found on pump. 2.1 x 10 4 counts in ROI (23% of those imageable)

33 RHR Pump Room 60 Co 60 Co and 58 Co are in different regions of pump. 3.7 x 10 3 counts in ROI (34% of those imageable)

34 RHR Pump Room 137 Cs See contamination on floor from prior flood. Nearer areas appear hotter. 4.0 x 10 4 counts in ROI (29% of those imageable)

35 RHR Pump Room 137 Cs Also see contamination on wall directly behind. 4.0 x 10 4 counts in ROI (29% of those imageable)

36 Shielding Verification Co-60; 30 s; shield removed Co-60; 1 minute; shield in place Can verify that shield reduces dose from one source to below that from another source. Co-60; 30 s; looking over shield 40

37 Locating Isotopes in Shipping Containers Co-60; 17 min.

38 Applications National security, homeland security and international nuclear non-proliferation Nuclear power (dose reduction, clean-up and inspection) Medical imaging (proton cancer therapy) Planetary sciences & astrophysics (NASA) Safeguard (IAEA) Fundamental Physics Environmental monitoring

39 How does an optical camera work? Object Lens Film Forming images 2-dimensional position-sensing spectrometer

40 Principle of a low-energy gamma camera (< 250 kev) Object Pin-hole Lens Film No spectroscopy No isotope ID Forming images 2-dimensional position-sensing Spectrometer? Note: Identity of isotopes are determined by γ-ray spectroscopy

41 Principle of Polaris technology for higher energy (> 250 kev, 137 Cs, 58 Co, 60 Co) γ-rays Object Computer Advanced Algorithm Lens Film Forming 3-dimensional images position-sensing 2-dimensional spectrometer position-sensing spectrometer