US20070057194A1

US20070057194A1 - Neutron and gamma-ray detection system

Info

Publication number: US20070057194A1
Application number: US11/513,944
Authority: US
Inventors: James Ryan; John Macri; Mark McConnell; Ulisse Bravar
Original assignee: NEW HAMPSHIR, University of
Current assignee: NEW HAMPSHIR, University of
Priority date: 2005-08-31
Filing date: 2006-08-31
Publication date: 2007-03-15
Also published as: US20090250620A1; US8829443B2

Abstract

The present invention is a radially symmetric imaging detector that measures an incident neutron's or gamma-ray's energy and identifies its source on an event-by-event basis.

Description

CROSS-REFERENCE TO RELATED APPLICATIONS

The present application claims the benefit of provisional patent application Ser. No. 60/713,104 filed Aug. 31, 2005, which is incorporated herein by reference.

GOVERNMENT SPONSORSHIP

The development of the present invention was funded in part by the DoE of the United States Government under Contract No. DE-FG52-04NA25687 and by the NASA of the United States Government under Contract No. NAG5-13519.

TECHNICAL FIELD

The present invention relates to a system for neutron and gamma-ray detection. More specifically, it relates to a radially symmetric imaging detector that directly measures the incident radiation.

BACKGROUND INFORMATION

Because they are electrically neutral, neutrons and gamma-rays have been traditionally detected using indirect means. However, typical indirect techniques of the prior art, for neutrons, for example, while able to measure count rate, provide little, if any, information on the neutron's energy or the location of the neutron's source. This lack of information limits the usefulness of prior art detectors in a number of applications, including the detection of special nuclear material (SNM). These materials—specifically uranium and transuranics—emit neutrons via spontaneous or induced fission, which neutron emissions are unique to fissionable material.
While position sensitive neutron detectors have been described in the prior art, such as the COMPTEL as described in J. Ryan, et al., “COMPTEL as a Solar Gamma-Ray and Neutron Detector,” presented at Data Analysis in Astronomy; 1992, the active areas of these prior art detectors were typically a flat surface, with a limited field of view. The radial symmetry of the detection of the present invention is a desirable feature in several applications. In space-based solar observations, the detector is typically installed on a spacecraft spinning around an axis orthogonal to the direction to the Sun. Therefore, a flat-surface detector has a time-dependent sensitivity to solar events, which is undesirable when detecting time-varying neutron or gamma-ray fluxes, such as the ones from solar flares. In another important application, the search for SNM emitting neutrons, a radially symmetric detector placed in any area (e.g. a storage warehouse or loading dock) provides a complete 360° wide scan with no need to change its orientation.
A cylindrically symmetric imaging neutron detector described in the prior art is described in U.S. Pat. No. 5,345,084. However, the detector therein is based on count rate rather than measurement of individual neutrons and, as a result, provides no information on neutron energy and no means to identify gamma-rays. With respect to the coordinate system in FIG. 1, the detector of the prior art can determine the azimuthal angle φ of the neutron source (with relatively poor accuracy, Δφ˜30°−45°), but is unable to measure the zenith angle θ, making it impossible to locate point sources.

SUMMARY OF THE INVENTION

The present invention is a system comprising a radially symmetric imaging detector that directly measures an incident neutron's or gamma-ray's energy and identifies the point source of the neutron or gamma-ray on an event-by-event basis through an event circle analysis.

BRIEF DESCRIPTION OF THE DRAWINGS

These and other features and advantages of the present invention will be better understood by reading the following detailed description, taken together with the drawings wherein:
FIG. 1 is a schematic diagram of one preferred embodiment of the present invention;
FIG. 2 is a side view of one of the plastic scintillator bars used in the preferred embodiment of the present invention shown in FIG. 1;
FIG. 3 is an end view of one preferred embodiment of the present invention;
FIG. 4 is a side view of the preferred embodiment of the present invention shown in FIG. 3;
FIG. 5 is a top view of one preferred embodiment of the present invention;
FIG. 6 is a side view of the preferred embodiment of the present invention shown in FIG. 5; and
FIG. 7 is a schematic diagram of a double n-p scatter events detected by a preferred embodiment of the present invention.

DETAILED DESCRIPTION OF THE INVENTION

The present invention relates to a radially symmetric imaging detection system for neutrons or gamma-rays.
With respect to neutrons, the present invention measures the energy of an incident neutron, and through scattering kinematics determines the point or extended sources of the neutron. This technique is based on a known detection mechanism—fast neutron scattering off ambient hydrogen (n-p scattering). Such a detection system is configured to locate n-p scatter sites within its volume using the scintillation light generated by recoil protons, highly ionizing particles. For the neutrons that undergo at least two successive n-p scatters, an image revealing the location of a source can be constructed.
FIG. 1 shows one preferred embodiment of the imaging detection system 2 of the present invention. The design consists of a radially symmetric array 4 of multiple (in this embodiment 13) parallel scintillator bars 6. The scintillator bars 6 are preferably organic scintillator bars, either plastic or liquid, selected for their relative abundance of protons. The dimensions of each scintillator bar 6 used in a particular embodiment may vary, from case to case, depending on the desired application. For example, as shown in FIG. 2, typical values for a plastic scintillator bar 20, are 30.0 cm length 22 and 1.5 cm diameter 24. The total number of the scintillator bars and the requisite cylindrical symmetric array of the bars may also vary, from embodiment to embodiment, depending on the desired application, as is discussed in more detail below. For example, as shown in FIG. 3, the detection system 30 comprises a cylindrical symmetric array 34 of 19 scintillator bars 36 in which each scintillator bar has a diameter of 1.5 cm and a length of 30 cm. As shown in FIG. 4, this detection system 30 has resulting overall dimensions of 11.5 cm diameter 38 and 51.0 cm length 40.
It is to be understood that the term “scintillator bar,” as used herein, includes optically separated chambers, filled with scintillation material, in a unitary housing. Thus, FIGS. 5 and 6 show a preferred embodiment of the imaging detection system 52 present invention in which the design consists of a radially symmetric array 54 of multiple (in this case 37) scintillator bars, or chambers 56, in a liquid scintillator tank 58 divided by baffles into optically separated chambers 56.
Referring again to the preferred embodiment of FIG. 1, a photomultiplier tube (PMT) 8, or other light sensing device, known to those skilled in the art, is connected to the first and the second end of each scintillator bar 6. Each PMT 8 is, in turn, connected 10 to signal processing electronics 12, to which it sends light-sensing signals, consisting of pulse processing electronics known to those skilled in the art. Fast discriminators and coincidence circuits are employed to initiate the measurement of the required parameters for each incident particle registering two or more interactions. The required parameters, interaction locations, energies, relative times and pulse shapes are digitized and registered as a series of detector IDs, pulse heights, and times of flight for each detected particle. A data acquisition system records these parameters for each detected particle for subsequent imaging and energy analysis.
Referring still to FIG. 1, the technique for detecting a neutron 11 impinging the detection system 2 is based on the measurement of the energies, positions, sequence and relative times of interaction of recoil protons resulting from multiple, successive, neutron-proton)(n-p) scatters 13 and on the kinematics of n-p scattering for reconstruction of the incident neutron energy and direction. In the case of gamma-rays, the same technique applies, but Compton-scatter electrons are used instead of protons. With respect to neutrons, scintillator bar 6 material and diameter are chosen to maximize the probability of single n-p scatters occurring within one scintillator bar 6, with the scattered charged particle being fully contained within the boundaries of the scintillator bar 6. At the same time, the scintillator bars 6 should be sufficiently thin for a scattered neutron to exit the bar after the first n-p scatter 13 and to produce successive n-p scatters 13 in other scintillator bars 6.
Energy information on a recoil proton, or Compton electron in the case of gamma-rays, resulting from an elastic n-p scatter in a given scintillator bar 6, is obtained from the amplitude of the signals measured by the PMTs 8 at the first and second ends of the scintillator bar 6. Position information on the proton in the x-y plane is determined from the position in the x-y plane of the scintillator bar 6 in which the interaction occurs. Position information on the proton along the z-axis is measured by analyzing the arrival time differences and/or the amplitude differences of signals measure by PMTs 8 at the ends of the scintillator 6 in which the interaction occurs. The signals measured by the PMTs at the ends of the scintillator bars 6 in which successive n-p scatters occur also provide a measure of the relative times of the successive scatters.
Referring to FIG. 7, a neutron 71, whose incident direction is unknown, undergoes at least two n-p scatters 72, 73. By measuring the coordinates of the two interactions, the relative times of the two interactions and the energy of the recoil proton of the first interaction, one can determine the energy and direction (i.e. vector velocity) of this particle. The neutron scatter angle, shown as θ _n, 74 is given by: $\sin^{2} {\hat{θ}}_{n} = \frac{E_{p 1}}{E_{n}}$
where E_p1and E_nare the energies of the first recoil proton and the incident neutron, respectively. Once E_p1and E_nare known, one can determine θ_n.
However, measurement of the sequence, energies and positions of the protons resulting from two successive n-p scatters of an incident neutron is not sufficient to localize an unknown source of neutrons. One more piece of information is needed, the energy of the incident neutron, En. In the present invention, the energy of the incident neutron is determined by measuring the time difference between the two successive n-p scatters 72, 73. This time difference provides the velocity and thus the energy of the neutron scattered after the first recoil. The incident neutron energy, E_n, is the sum of this scattered neutron's energy and the energy of the first scattered proton, E_p1. In addition, this time difference allows for the separation of 1-100 MeV neutrons from gamma-rays.
FIG. 5 shows a schematic diagram of the basic kinematics of event reconstruction for two successive n-p scatter events 72, 73 caused by a neutron 71. Again, θ_n 74 the neutron scatter angle is given by $\sin^{2} θ_{n} = \frac{E_{p 1}}{E_{n}}$
where E_p1and E_nare the energy of the first recoil proton and the incident neutron, respectively. Hard-sphere scattering implies that the scattered neutron and proton momenta will lie at right angles to one another and that the incident neutron direction must lie on a cone 75 about the recoil neutron velocity vector. The projection of this cone on the image plane or the celestial sphere is an event circle 76. The superposition of event circles from many incident neutrons provides the statistical information necessary to locate an unknown source of neutrons, event circles from a point source intersect, but unrelated, for example background event circles, do not. This procedure has been demonstrated successfully on the COMPTEL experiment by imaging MeV gamma-ray and neutron sources.
If certain liquid scintillator materials are used instead of plastic scintillator materials, pulse shape discrimination (PSD) techniques can be employed to further discriminate neutron form gamma-ray interactions.
Finally, by preferably augmenting the structure of the detection system of the present invention with an anticoincidence shield, unrelated charged particles can be excluded.
While the principles of the invention have been described herein, it is to be understood by those skilled in the art that this description is made only by way of example and not as a limitation as to the scope of the invention. Other embodiments are contemplated within the scope of the present invention in addition to the exemplary embodiments shown and described herein. Modifications and substitutions by one of ordinary skill in the art are considered to be within the scope of the present invention, which is not to be limited except by the following claims.

Claims

1. A neutron detector to determine the direction and energy of each incident neutron comprising multiple substantially parallel scintillator bars, said bars being positioned such that the bars are radially symmetric.

2. The neutron detector of claim 1 wherein said bars contain organic scintillating material.

3. A neutron detector to determine the direction and energy of each incident neutron comprising multiple substantially parallel scintillator bars, said bars each having a first end and a second end and said bars being positioned such that the bars are radially symmetric.

4. The neutron detector of claim 3 further comprising a light sensing means, attached at the first end and second end of each of said bars, for detecting n-p scatter events in each of said bars.

5. The neutron detector of claim 4 further comprising electronic signal processing means to process the light-sensing signals and measure the sequence, positions, energies, relative times and pulse shapes of each coincident n-p interaction.

6. A method of detecting neutrons by determining the direction and energy of each incident neutron comprising

positioning multiple scintillator bars so that said bars are substantially parallel;

further positioning said bars so that the bars are radially symmetric;

attaching a light sensing means to the ends of each of said bars;

detecting successive n-p scatters in different bars caused by an incident neutron;

determining the relative times of the successive n-p scatters; and

determining the sequence, positions, relative times and energies of a recoil proton and a scattered neutron resulting from each successive scatters.

7. A neutron detector to determine the direction and energy of each incident neutron comprising multiple substantially parallel scintillator bars, said bars being positioned such that the bars are radially symmetric providing a 360° wide scan without changing the detector's orientation.

8. A gamma-ray detector to determine the direction and energy of each incident gamma-ray comprising multiple substantially parallel scintillator bars, said bars being positioned such that the bars are radially symmetric.

9. The gamma-ray detector of claim 8 wherein said bars contain organic scintillating material.

10. A gamma-ray detector to determine the direction and energy of each incident gamma-ray comprising multiple substantially parallel scintillator bars, said bars each having a first end and a second end and said bars being positioned such that the bars are radially symmetric.

11. The gamma-ray detector of claim 10 further comprising a light sensing means attached at the first end and second end of each of said bars, for detecting Compton interactions in each of said bars.

12. The gamma-ray detector of claim 11 further comprising electronic signal processing means to process the light-sensing signals and measure the sequence, positions, energies, relative times and pulse shapes of each coincident Compton interaction.

13. a method of detecting gamma-rays by determining the direction and energy of each incident gamma-ray comprising.

further positioning said bars so that the bars are radially symmetric;

attaching a light sensing means to the ends of each of said bars;

detecting successive Compton interactions in different bars caused by an incident gamma-ray;

determining the relative times of the successive Compton interactions; and

determining the sequence, positions, relative times and energies of a recoil electron and a scattered gamma-ray resulting from each successive interaction.

14. A gamma-ray detector to determine the direction and energy of each incident gamma-ray comprising multiple substantially parallel scintillator bars, said bars being positioned such that the bars are radially symmetric providing a 360° wide scan without changing the detector's orientation.