Organic-scintillator compton gamma ray telescope

• US 8,785,864 B2
• Filed: 09/22/2010
• Issued: 07/22/2014
• Est. Priority Date: 09/22/2009
• Status: Active Grant

• Current Assignee: Boss Physical Sciences LLC
• Original Assignee: Boss Physical Sciences LLC
• Inventors: Ricci, Kenneth N., Norris, Wayne B., Paden, Brad
• Primary Examiner(s): Hannaher, Constantine
• Application Number:
  US13/497,739
• Publication Number:
  US 20120217386A1
• Time in Patent Office: 1,399 Days
• Field of Search: 250/367
• US Class Current: 250/367
• CPC Class Codes: G01T 1/20 with scintillation detectors
• CPC Class Codes: G01V 5/20 Detecting prohibited goods, e.g. weapons, explosives, hazardous substances, contraband or smuggled objects
• CPC Class Codes: G01V 5/234 Measuring induced radiation, e.g. thermal neutron activation analysis
• CPC Class Codes: H01L 27/14663 Indirect radiation imagers, e.g. using luminescent members
• CPC Class Codes: H01L 31/0203 Containers; Encapsulations , e.g. encapsulation of photodiodesfor photovoltaic devices H01L31/048; for organic photosensitive devices H10K30/80

Abstract

Apparatus and methods for imaging sources of gamma rays with a large area, comparatively low-cost Compton telescope (20). The Compton telescope (20) uses multiple layers (24) of low-cost organic solid plastic or liquid scintillator, arranged in large arrays of identical scintillator pixels (28). Photodiodes, avalanche photodiodes (30), or solid-state photomultipliers are used to read out the fluorescent pulses from scintillator pixels (28). Multiple scintillator pixels (28) are multiplexed into a few fast digitizers (80) and a few fast FPGA programmable digital microprocessors (78). Selection rule methods are presented for processing multiple near-simultaneous gamma ray collisions within the Compton telescope (28) to identify trackable events that yield gamma ray image data of interest. A calibration method achieves improved energy resolution along with (x,y) position information in pixels (28) made of organic scintillator materials with multiple photodetectors (30). Synchronization trigger signals are used from a pulsed neutron source (58) to maximize the signal-to-background ratio for prompt gamma neutron activation analysis (PGNAA) of objects at greater than 2 meters range, where such trigger signals are based on the estimated range to PGNAA sources and neutron time-of-flight.

Claims

1. A Compton telescope-type gamma-ray imaging apparatus (20) including a plurality of scintillators (28), said device comprising:

a chassis, said chassis including at least three discrete layers (24) spaced-apart from one another and supported in an aligned, generally parallel orientation;

at least one gamma ray detector operatively disposed in each said layer (24);

each said gamma ray detector comprising a plurality of scintillator pixels (28);

said gamma ray detectors on at least two of said layers (24) including organic scintillator pixels (28), said organic scintillator pixels (28) each including a unitary volume of scintillator material having at least three semiconductor-based high-gain photodetectors (30) mounted thereon and configured to determine the (x,y) position and total energy deposited by a gamma ray collision inside the respective said organic scintillator pixel (28).

2. The apparatus (20) of claim 1, wherein said organic scintillator pixels (28) are fabricated from at least one of solid plastic scintillator and liquid scintillator material compositions.

3. The apparatus (20) of claim 2, wherein said organic scintillator pixels (28) contain up to 20% heavy metals by weight in the form of organometallic compounds.

4. The apparatus (20) of claim 1, wherein said scintillator pixels (28) are substantially identical to one another over the entirety of at least one said gamma ray detector.

5. The apparatus (20) of claim 1, wherein said at least three photodetectors (30) are selected from a group consisting essentially of low-noise photodiodes, avalanche photodiodes and solid state photomultipliers.

6. The apparatus (20) of claim 1, wherein said at least three photodetectors (30) are disposed in an array on each said scintillator pixel (28) such that the sums of and the differences between signals produced by adjacent said photodetectors (30) will yield a definable function of the position and total energy deposited by a gamma ray in that region of said scintillator pixel (28).

7. The apparatus (20) of claim 1, wherein each said scintillator pixel (28) has a plurality of sides, and wherein said at least three photodetectors (30) are located along different sides of said scintillator pixel (28).

8. The apparatus (20) of claim 1, wherein each said scintillator pixel (28) has an associated printed circuit board (32) including at least one photodetector power supply trace, photodetector preamplifier (64), and an electronic connector, and wherein said printed circuit board (32) further includes at least one analog sum amplifier (66) for summing the signals from a plurality of said photodetectors (30).

9. The apparatus (20) of claim 8, wherein said printed circuit board (32) further includes at least one analog differential amplifier (68) for subtracting the signals of adjacent said photodetectors (30).

10. The apparatus (20) of claim 8, wherein said printed circuit board (32) further includes at least one analog signal threshold detector (70) for generating a trigger signal when a pre-set trigger threshold is exceeded.

11. The apparatus (20) of claim 8, wherein said at least three photodetectors (30) are affixed to said scintillator pixel (28) with an index-matching optical adhesive.

12. The apparatus (20) of claim 1, further including housing walls (26) operatively associated with said chassis, said housing walls (26) including at least one of neutron shielding, gamma ray shielding, and coincidence/anti-coincidence detectors for improving signal/background ratio.

13. The apparatus (20) of claim 1, further including at least one fast programmable microprocessor for performing digital signal processing on groups of events.

14. The apparatus (20) of claim 1, further including a data analysis and imaging system for generating an image of the gamma ray field of view of said apparatus (20) based on an accumulation of multiple gamma events of interest in said gamma ray detectors.

15. The apparatus of claim 1, further including a non-transitory computer readable medium coded with instructions and executed by a processor to individually calibrate at least one organic scintillator pixel.

16. The apparatus of claim 15, wherein said computer readable medium coded with instructions and executed by a processor accesses at least one predetermined lookup table.

17. A method of operating a Compton telescope-type gamma-ray imaging apparatus (20) including plural scintillators (28), said method comprising the steps of:

supporting at least three discrete layers (24) of gamma ray detectors in spaced-apart generally parallel alignment;

each said gamma ray detector including a plurality of substantially identical scintillator pixels (28);

forming a plurality of the scintillator pixels (28) in at least two of the layers (24) from an organic scintillator material composition; and

individually calibrating at least one organic scintillator pixel (28) to improve its (x,y) position and energy resolution characteristics, said calibrating step including correcting the energy measurement from at least one organic scintillator pixel (28).

18. The method of claim 17, wherein said calibrating step includes using a selected subset of one or more scintillator pixels (28) to represent the response of a plurality of scintillator pixels (28) for at least one of the gamma ray detectors.

19. The method of claim 17, wherein each said scintillator pixel (28) includes at least three semiconductor-based high-gain photodetectors (30) mounted thereon and configured to determine the (x,y) position and total energy deposited by a gamma ray collision inside the scintillator pixel (28), further including the step of deriving the (x,y) position of said gamma ray collision inside at least one scintillator pixel (28) using the difference signal between adjacent photodetectors (30) divided by the sum signal from adjacent photodetectors (30).

20. The method of claim 17, further including the step of identifying gamma ray tracks that interact in multiple layers (24) of gamma ray detectors by selecting event clusters that generate groups of trigger signals coincident within a predetermined time window.

21. The method of claim 17, further including the step of rejecting energetic particle events that do not contribute to the gamma ray image of interest on the basis that the energy depositions in all gamma ray detector layers (24) for that event do not produce a sum in the range of about 9.3 to 11.3 MeV.

22. The method of claim 17, further including the step of rejecting energetic particle events that do not contribute to the gamma ray image of interest on the basis that the energy depositions in all gamma ray detector layers (24) for that event do not produce a sum approximately equal to a predetermined gamma ray energy of interest.

23. The method of claim 17, further including the step of rejecting energetic particle events that do not contribute to the gamma ray image of interest on the basis that the event clusters do not generate pixel (28) triggers in at least two distinct gamma ray detector layers (24).

24. The method of claim 17, further including the step of pulsing a neutron beam, and disregarding undesirable background events contained within the scintillator pixel (28) responses as a function of neutron time-of-flight after each neutron pulse.

25. The method of claim 17, further including the step of disregarding undesirable background events contained within the scintillator pixel (28) responses as a function of conformity with the Compton scatter law and the field of view and angular acceptance of the Compton telescope apparatus (20).