I. INTRODUCTION
Research on explosives detection has gotten more attention around the world in terrorist activities in recent years. The traditional neutron activation analysis (NAA) [1] method has difficultly distinguished explosive and non-explosive organic materials because of the same components of C, H, N, and O. The pulsed fast/thermal neutron analysis (PFTNA) [2] technique can combine the prompt inelastic scattering gamma-ray spectrum of fast neutrons with the delayed radiative capture gamma-ray spectrum of thermal neutrons. Both spectra contain the characteristic gamma-ray spectrum of the four elements. When utilizing different characteristics of the gamma-ray spectrum, it is possible to identify the contents of these elements and distinguish explosive or non-explosive species. The PFTNA technique has been widely used in industrial production due to its high sensitivity and accuracy, such as analyzing coal composition [3, 4]. Also, the PFTNA technique can be used to analyze the content and ratio of H, C, O and N in the detection of mines and other explosives, especially non-metallic mines. However, the explosives have different structures in complicated environmental conditions. At present, the PFTNA technique is mainly focused on the theoretical and experimental exploration. Some actual probes are carried out in a few countries and regions [5-7].
When the gamma-ray spectra of mines and explosives are measured by the PFTNA method, many complex signals should be generated, including gamma signals from the target, and the background by neutrons and gamma signals, the experimental apparatus and the environment. However, in an experiment the detector cannot distinguish the type and source of all signals. The composition of the spectrum, the contribution of experimental apparatus to the background can be obtained by GEANT4.
In the present work, the characteristic gamma-ray spectra of TNT in the soil induced by DT neutrons are measured by the PFTNA demining system. The GEANT4 toolkit is used to simulate the whole experimental procedure, and the simulated are compared with and experimental those, to obtain background sources such as neutrons and gamma. The contribution of experimental apparatus to the background, such as the shielding, detector sleeve, and moderator, is analyzed.
II. INTRODUCTION OF EXPERIMENTAL PLATFORM
The experiment was completed in the Institute of Nuclear Physics and Chemistry, China Academy of Engineering Physics. The 14 MeV fast neutrons were produced by a pulsed D-T neutron generator at pulse width of 80 μs and pulse interval of 50 μs, and used to irradiate TNT. The pulsed neutron generator was a cylinder with 9.8 cm diameter, can reach about 107–108 /s yield, and the target was centrally away from 20 cm at its front. Neutrons launch from the target in the direction of 4π. Outside of the neutron generator, there is a layer of a polyethylene moderator [8]. TNT (2 kg) was located in the center of soil sizes of 5 m×5 m× 1m at a depth of 2 cm. A LaBr3(Ce) detector with the size of ϕ7.5 cm× 7.5 cm is used to obtain prompt inelastic scattering gamma-ray spectrum of fast neutrons and the delayed radiative capture gamma-ray spectrum of thermal neutrons. There was a sleeve with a size of ϕ150 mm×135mm outside of the detector, and its outer layer was 1 mm iron, and the inner layer is 5 mm lead. On the bottom of the sleeve, there was cadmium sheet with 2 mm thickness. To reduce its radiation damage due to neutrons A 60 mm-thick lead block was alternated with 200 mm-thick polyethylene and a 80 mm-thick lead block was used to shield the detector. The experimental arrangement is shown in Fig. 1.
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III. SIMULATED RESEARCH METHOD
The GEANT4 toolkit [9, 10] was used to simulate the whole experimental procedure based on the structure and size of the experimental apparatus. Fig. 2 shows that the apparatus contours given by GEANT4 is fundamentally consistent with the experimental apparatus. After 14 MeV neutrons hitting the TNT, the energy deposition measured by the LaBr3(Ce) detector was simulated. By recording the global time and physical process for each energy deposition, the simulated fast neutron and thermal neutron induced spectra were compared with experimental those.
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Each energy deposition produced particles was simulated, and the deposited energy, the area and the primary radiation were recorded by the detector, thus obtaining the share of the background sources, such as neutrons and gamma. Further, the contribution of shielding, the detector sleeve and the moderator to background can be obtained. The background can be reduced by improving the experimental apparatus.
IV. RESULTS AND DISCUSSION
A. Comparison between simulated and experimental results
Figure 3(a) shows the experimental and simulated fast neutron induced spectrum (fast spectrum) of the TNT. Fig. 3(b) shows the experimental and simulated thermal neutron induced spectrum (thermal spectrum). Comparatively, the experimental spectra are folded with an energy resolution due to the statistical fluctuation of the number of carriers, the noise of the detector, and electronic system. The simulated spectra are consistent with the experimental those except Gaussian broadening, the broadening coefficients are obtained by fitting the experimental data. Also, Fig. 3 shows that experimental spectra are consistent with simulated in the low-energy region of the fast spectrum, the peaks of the simulated spectra, however, are more obvious in the high-energy region. The main reason is that the TNT is buried in the soil in the experiment, and it is difficult for its complex composition to be analyzed quantitatively. Differently, the simulated soil contains only 62% SiO2, 25%Al2O3, 3%Fe2O3, 10%H2O. Each channel of the high-energy region (8–12 MeV) in the simulated spectra has only a few counts. In Fig. 3, the Y-axis counts normalized to each neutron would cause large statistical fluctuation. When doing Gaussian broadening, false peaks are formed in this energy interval, meaning that counts are not reliable in this region of the simulated spectra. In Fig. 3(a), we can clearly see the 16O(n, n’γ)16O(Eγ =6.13 MeV), 12C(n, n’ γ)12C(Eγ=4.44 MeV), and 28Si(n, n’ γ)28Si (Eγ =1.78 MeV) gamma-ray full-energy peaks and parts of their escape peaks, and the 1H(n, γ)2D(Eγ =2.23 MeV) gamma-ray full-energy peak in Fig. 3(b). Because the cross section of the radiative capture reaction between thermal neutrons and the N element is small and the share of thermal neutrons is small, the 14N(n, γ)15N(Eγ=10.83 MeV) gamma-ray full-energy peak is nearly absent in Fig. 3(b).
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B. Analysis of simulated spectrum
Based on the simulation method described above, the full spectrum of the TNT is analyzed, as shown in Fig. 4. The left figure shows that the four spectra are produced by all particles (Total), neutrons (Neutron), gamma photons from the soil and TNT (Gamma-soil and TNT), and gamma photons outside of the soil and TNT (Gamma-other), including the sleeve outside of the LaBr3 detector, shielding devices, and the moderator outside of the neutron generator, and others. On the right figure, the "Total" spectrum is produced by all particles; and the "Soil and TNT" spectrum, by particles from the soil and TNT.
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Analyzing the full spectrum signal shows that its background is too large, because the gamma signal from the soil and TNT is only 29%, the background signal from neutrons is 31%, and the background signal from the gamma photons outside of the soil and TNT is 37%. Therefore, the background needs to be reduced by improving the experimental apparatus.
C. Improvement of experimental apparatus
After studying the background sources, it was found that a significant contribution of the cadmium sheet on the bottom of the sleeve outside of LaBr3 detector to the background. In addition, the shielding placed between the detector and the DT neutron source has a limited effect on stopping neutrons, thus meaning that a larger portion of neutrons can traverse the detector through the shielding. Table 1 shows the contribution of each part of experimental apparatus to background.
Parts of experimental apparatus | Cadmium of detector sleeve | Fe and Pb of detector sleeve | Shielding | Moderator | Others |
---|---|---|---|---|---|
Contribution to background | 44.79% | 8.21% | 21.40% | 4.01% | 21.58% |
From Table 1, the contribution of cadmium of the detector sleeve and the shielding to background is more than 65%. So, improving the design of the cadmium sheet and shielding should increase the signal-to-noise ratio.
1. Improvement of cadmium sheet
Source neutrons can be scattered into the LaBr3 detector by the environment and absorbed by the cadmium sheet on the bottom of the sleeve, thus reducing the background signal from neutrons. However, gamma-rays will be produced when absorbing neutrons, and lead to an increase of the background signal. The ratio of the effective gamma signal counts (from soil and TNT) to total counts (Nefg/Nt) and background signal counts from neutrons to total counts (Nn/Nt) are considered as the targets. By gradually reducing the size of the cadmium sheet, the relationship of Nefg/Nt and Nn/Nt vs. the size of the cadmium are obtained, as shown in Fig. 5, to find the optimum size of the cadmium sheet.
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From Fig. 5(a) and 5(b), Nefg/Nt gradually increased from 29% to 34% with reducing the thickness of the cadmium sheet from 2 mm to 0.1 mm. Nn/Nt first decreased, then increased, and is minimal at 0.2 mm, generating the smallest background signal, and accounting for 28% of the full spectrum signal.
From Fig. 5(a), the share of the effective gamma signal increased only 4% up to the thickness of 0.2 mm cadmium, this is due to that the background gamma signals will be produced while the cadmium absorbs neutrons. Therefore, we considered that the 0.2 mm cadmium replaced with 0.2 mmlithium becasue 6Li does not produce gamma rays and has a high the cross section of reaction. The simulated result is shown in Table 2.
Material | 2 mm cadmium | 2 mm lithium |
---|---|---|
Nefg/Nt | 29% | 42% |
From Table 2, the share of the effective gamma signal improved from 29% to 42% at the 2 mmlithium. Then, because the GEANT4 simulated result shows that the effective gamma signal increased very slowly with the thickness of lithium, 2 mm lithium is replaced with 2 mm cadmium on the bottom of the detector sleeve.
2. Improvement of shielding
The alternating structure of polyethylene layer and lead layer is used to shielding. The lead in first layer can reduce the energy of fast neutrons by inelastic scattering, and the polyethylene moderate them to the thermal neutrons due to being slowed down and absorbed. The lead in second layer is used to absorb gamma rays during the process of moderation and absorption. In this experiment, neutrons must get through a layer of moderator, to generate less background signal in the first lead layer. The simulated result shows that the background signal is mainly produced in the polyethylene and the second lead layer. Therefore, the Nefg/Nt increases with thicknesses of polyethylene and the second lead layer, as shown in Fig. 6, thus obtaining their optimum sizes.
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From Fig. 6(a), keeping the thickness of the first lead layer of (60 mm) and the second lead layer (80 mm), Nefg/Nt increased from 29% to 31% with the thickness of polyethylene from 200 mm to 250 mm. The Nefg/Nt increased more slowly with the thickness of polyethylene. Actually, the optimum thickness of polyethylene is 250 mm. From Fig. 6(b), keeping the thickness of the first layer of lead (60 mm) and the polyethylene thickness of 200 mm, Nefg/Nt increased from 29% to 31% with the thickness of the second lead layer from 80 mm to 130 mm. The Nefg/Nt does not significantly change with the thickness of the second lead layer. Therefore, the optimum thickness of the second lead layer is 130 mm.
D. Analysis of spectrum after improving experimental apparatus
Also, the TNT spectrum is simulated and analyzed by improving the experimental apparatus. Fig. 7 shows the ratio of the effective gamma signal counts (from soil and TNT) to total counts (Nefg/Nt) changes with gamma energy before and after improving the experimental apparatus, This is only figure of low- to mid-energies because the less counts from the high-energy end of the spectrum creates large statistical error fluctuations. From Fig. 7, Nefg/Nt increased after improving the experimental apparatus. The characteristic peaks of H 2.23 MeV, C 4.44 MeV, and O 6.13 MeV have been strengthened and their signal levels have also been improved. In the full spectra, the share of gamma photons from the soil and TNT is up to 47%, increasing by 18% after improving the apparatus, and the background signal from neutrons and gamma photons reduced by 18%.
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The characteristic signal of the full spectrum should be improved because the background accounts for more than 50%. Further, shielding structures reducing the neutrons and gamma photons simultaneously should be studied.
V. CONCLUSION
A mixed gamma-ray spectrum is formed by DT neutrons hitting TNT in the soil and simulated by the GEANT4 toolkit. The contribution of different types of particles and their sources to the spectra are studied. The effective gamma signal (from soil and TNT) only accounts for 29%; and the background signal, more than 68%. The cadmium sheet on the bottom of the detector sleeve and the shielding device contribute significantly to background. After replacing cadmium with lithium and improving the size of the shielding, the characteristic peaks are strengthened. The share of the effective gamma signal increased to 47% while the background signal fell to 18%. The contribution and source of the background was performed by using the GEANT4 toolkit, to optimize a reliable experimental device of neutrons.
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