Frank Laboratory of Neutron Physics Joint Institute for Nuclear Research Author: Constantin Hramco, engeneer.

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Presentation transcript:

Frank Laboratory of Neutron Physics Joint Institute for Nuclear Research Author: Constantin Hramco, engeneer.

1. Introduction 2. Experimental work 3. Results and discussion 4. Conclusions 2

1. Introduction Medicine Mining Construction Jewelry Agriculture Synthesis 3

Our dashingly developing society needs more and bigger quantities of different materials for self-evolving. This type of requirements displays a lot of sectors of human activities, starting with food processing and ending with our brain evolution. Among these branches is placed the mining industry. The neutron physics has large achievements in the elemental content determination area. An excellent example is the neutron activation analysis. The activation with thermal neutrons is too slow method for mining. That is why the solution is to use fast neutrons for prompt gamma neutron activation analysis (PGNAA). 4

2. Experimental work Three types of ore samples for analysis: 1.Concentrate – sample with highest concentration of P 2 O 5 – 38.95% 2.Tail – sample with lowest concentration of P 2 O 5 – 0.9% 3.Mixture – sample with concentration of P 2 O 5 being between the values for first and second samples. Controlled elementApatite concentrate, mass %Tails, mass % P2O5P2O Al 2 O CaO SiO Fe 2 O K2OK2O H2OH2O TiO Na 2 O Table 1. Content of different controlled elements in phosphate ore. 5

The sample is PET sac containing 10 kg of phosphate ore. Phosphorite – Ca 5 (PO 4 ) 3 + ω(Ca)= 41.29% ω(CaO)= 57.77% ω(P)= 19.15% ω(P 2 O 5 )= 43.87% 6

For experimental setup source of neutrons was chose 239 Pu-Be mixture with average neutron energy around 4.5 MeV. To detect gamma rays that are coming from interaction of neutrons with nuclei was set a Ortec high-purity germanium detector (HPGe) with the features presented in the table below: CertifiedMeasured Resolution (FWHM) at 1.33 MeV, 60 Co1.90 keV Relative Efficiency at 1.33 MeV, 60 Co30%36% Table 2. Main characteristics of Ortec HPGe gamma-detector. 7

8 Used reaction Inelastic scattering (n, n’ γ)

In order to perform the objective, first step is to evaluate the accuracy of HPGe in detecting of gamma-radiation from different elements. This task was reached by assembling the construction that is shown in Figures below: Figure 1. The scheme of assembly for determining the elemental content of phosphate ores. Figure 2. 3D-model of assembly for determining the elemental content of phosphate ores. 9 m/solutions/3d-design- software

Figure 3. HPGe Channel-Energy calibration curve. Important step in work with any gamma-spectroscopy instrument is to have well done channel-energy calibration. In our case the calibration was performed by two methods: by standard point sources ( 60 Co & 137 Cs) and by irradiation of metal samples (Cd & Pb). 60 Co : and KeV 137 Cs : KeV 10

3. Results and discussions The data acquisition was done by COCOS (COmbined COrrelation System) program developed at JINR FLNP, data processing was performed by Canberra’s Genie™ 2000 program. As an example, in the figure below is shown the comparison between gamma-spectra from three irradiated samples (concentrate – black, tails – red, mixture – purple) and background (blue): Figure 4. Part of gamma-ray energy spectrum ( MeV) mistry_lab/genie-2000-software.asp

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In Figure 5 is shown the comparison between the measurements made with different types of detectors: HPGe (with high resolution) and BGO (with high efficiency). Although BGO has a higher efficiency of gamma-ray detection, it has a moderate energy resolution. For example: if we compare Figure 4 with Figure 5, especially the interval between 2.20 and 2.25 MeV, in case of HPGe we can see that there are three lines from different sources ( 27 Al, background and 31 P). In case of BGO (Figure 5, green and dark-blue lines) these gamma-lines, either from concentrate or from tails samples, can not be divided. Figure 4. Part of gamma-ray energy spectrum ( MeV). Figure 5. Comparison of the energy resolutions of HPGe and BGO detectors. 14

γ-line energy, keV Attachment (Concentrate/Tails) IsotopeTable energy, keV 751ConcentrateSE 31 P1266,13 766Concentrate 44 Ca761,12 843Mixture 27 Al 56 Fe 843,76 846,76 983Tails 48 Ti983, Tails 27 Al1014, Concentrate 44 Ca1157, Mixture, Tails 56 Fe1238, Concentrate 31 P1266, Mixture 56 Fe 39 K 1360, , Tails 23 Na1635, Mixture, Tails 56 Fe1810, Concentrate 31 P2148, Tails 27 Al2212, Concentrate 31 P 2233, , Mixture, Tails 56 Fe 23 Na 2273, , , Mixture 56 Fe 39 K 2523, , Tails 28 Si 27 Al 48 Ti 39 K 2838, , , , Concentrate 31 P3134, ConcentrateSE 40 Ca3736, Concentrate 40 Ca 48 Ti 3736, , Mixture, Tails 48 Ti7585,00 In table 3 (on the right) is presented a part of detected elements. Although the work was done using different software there is no big shifting between acquired and table data. Nevertheless our assembly allowed to detect all elements presented in Table 1. Table 3. Some of the identified gamma-lines in the acquired spectra.

4. Conclusions 1.An experimental setup for determining the elemental composition of materials by prompt gamma-ray neutron activation analysis (PGNAA) was commissioned and tested. 2.The better accuracy of HPGe in detecting of elemental composition was confirmed. 3.The acquired spectra was processed and decoded successful. 4.Some preliminary results are reported and further actions proposed. 16

Acknowledgement D. N. Grozdanov Yu. N. Kopach V. M. Bystritsky S. B. Borzakov F. A. Aliyev N. A. Gundorin I. N. Ruskov V. R. Skoy 17