1. Introduction
Rare earth elements (REEs) play an increasingly important role in the transition to a low-carbon economy. In addition, they possess a high quantum efficiency in the visible region [1]. Recovering REEs from secondary sources is remarkably rare due to the scarcity of RE-bearing minerals, which results in a limited supply of REEs on the global market [2]. As a result, waste phosphors have become an urban mining resource from which REEs, such as yttrium (Y), europium (Eu), dysprosium (Dy), terbium (Tb), and cerium (Ce), can be extracted [3]. There are many high-tech applications of REEs. For example, europium-doped barium magnesium aluminate (BaMgAl10O17:Eu2+, BAM) is used in various high-resolution devices, including mercury free lamps, field emission displays (FEDs), light emitting diodes (LEDs), and plasma display panels (PDPs). BAM, an attractive blue phosphor, offers excellent chromaticity, chemical stability, and high luminance efficiency under both ultraviolet (UV) and vacuum ultraviolet (VUV) excitations [4–6]. Terbium-doped cerium magnesium aluminate (CeMgAl11O19:Tb, CMAT) has been widely used as the green-emitting component in three-band lamps and has been studied for use in some PDPs [7,8]. In particular, it is used in long-life and high-loading fluorescent lamps due to its high durability under intense UV radiation [9]. Sodium–yttrium–fluoride (NaYF4), among all RE-doped fluoride host nano-crystals, is preferred for use in medical and biological fields due to the noninvasive deep-tissue penetration of its radiation [10], its low-toxicity [11], and its biocompatibility [12]. Finally, the incorporation of rare-earth ions, i.e., Eu2+, Dy3+, etc., into the lattice structure of afterglow phosphors both confers upon it the afterglow effect and introduces defects in crystal lattices [13].
Further, gamma radiation shielding features of REEs make them desirable for use in Pb (lead)-free radiation protection aprons due to health, environmental, and economic benefits of using substances that are less toxic than Pb for radiation protection. Moreover, a study of the radiation-shielding features of REEs may aid in the design of new radiation protection materials made of non-toxic and green products. Recently, there has been an increasing demands for non-Pb (or non-toxic) materials that provide radiation protection. Some research has been performed on the high-energy attenuation performance of green and non-toxic materials [14–16]. Basic parameters, such as linear and mass attenuation coefficients, effective atomic number, and effective electron density yield important information about the radiation attenuation properties of these materials when matter and photons interact.
To the best of our knowledge, there are no studies in the literature on the radiation shielding performance of the green materials NaY0.77Yb0.20Er0.03F4, Ba0.86Eu0.14MgAl10O17, Sr3.84Eu0.06Dy0.10Al14O25, Ce0.63Tb0.37MgAl11O19, and Sr0.95Eu0.02Dy0.03Al2O4. The primary aim of this work was to experimentally evaluate the radiation shielding characteristics of these environmentally friendly products at different energies, i.e., between 81-1333 keV, and compare our results to the theoretical ones obtained using the WinXCOM software.
2. Material and Method
2.1 Experimental Details
The spectroscopic pure materials were in the form of a powder and supplied by Sigma Aldrich (St. Louis, MO, USA). All the materials had a purity of ≥ 99%. The particle size was 37 mm after being sieved to minimize the effects of the powder particle size on the results. To evaluate the gamma radiation shielding effectiveness, pellets with a diameter of 10 mm and thickness varying from 0.08 to 0.128 cm were produced by pressing the powder under a pressure of 10 ton cm-2 utilizing a manual hydraulic press after precisely determining the mass of the powder using a digital balance with an accuracy of 0.001g. The evaluated samples consisted primarily of O, F, Na, Mg, Al, Sr, Y, Ba, Ce, Eu, Tb, Dy, Er, and Yb. The amounts of these elements in the samples were associated with the coding of NaY0.77Yb0.20Er0.03F4, Ba0.86Eu0.14MgAl10O17, Sr3.84Eu0.06Dy0.10Al14O25, Ce0.63Tb0.37MgAl11O19, and Sr0.95Eu0.02Dy0.03Al2O4, with densities of 3.46, 2.33, 2.61, 2.15, and 1.96 g/cm3, respectively.
A high purity germanium (HPGe) gamma-ray spectrometric system was used to measure the intensities of high-energy photons from several radioactive point sources: 133Ba (81, 276, 303, 356 and 384 keV), 57Co (121 and 136 keV), 137Cs (662 keV), 60Co (1173 and 1333 keV), 54Mn (835 keV), and 22Na (1275 keV). The diameter and thickness of the HPGe detector were 70 and 25 mm, respectively. The resolutions were 0.380, 0.585, and 1.8 keV at full width and 5.9, 122, and 1330 keV at full width half maximum (FWHM). During the measurements, the detector was kept at a temperature of -196 oC by liquid nitrogen (N2). The system’s energy calibration was performed using the calibration sources 22Na, 54Mn, 57,60Co, 137Cs, 133Ba, 203Hg, and 241Am. A schematic of the experimental setup used in this study is given in Fig. 1. An absorbent material was placed between the radioactive point source and the detector. The data were analyzed with an Ortec Maestro software package program [17,18]. Using the Origin 7.5 program (demo), the net area counts were determined via the least-squares fitting method. Furthermore, the experimental uncertainties in the measurements were calculated according to the following equation [19, 20]:
-201907/1001-8042-30-07-008/alternativeImage/1001-8042-30-07-008-F001.jpg)
where ρ and x represent the density and thickness of the samples, respectively, Δρx represents the uncertainty in mass per unit area, ΔI0 and ΔI denote the uncertainties for I0 and I, respectively.
2.2 Theoretical background
The linear attenuation (μ) of the materials to be tested followed the well-known exponential attenuation law:
where I and I0 denote the transmitted and original intensities, respectively, and x is the thickness (cm).
Using the density of any compound or mixture and μ, the mass attenuation coefficient (
where wi denotes the weight fraction for the individual element in any material. The
It is derived many parameters, such as total molecular (
where NA is the Avogadro constant, Ai and ni denote the atomic weight and the element number of the ith element in the material, respectively. It is expressed in cm2/molecule.
σa is expressed in cm2/atom.
where
The effective atomic number (Zeff), a dimensionless quantity, was calculated from σa and σe [29]:
The radiation protection efficiency (RPE) of any material was determined as follows [30]:
where, 100 is the coefficient of percent efficiency (%).
3. Results and Discussion
The experimental values of µ/ρ for NaY0.77Yb0.20Er0.03F4, Ba0.86Eu0.14MgAl10O17, Sr3.84Eu0.06Dy0.10Al14O25, Ce0.63Tb0.37MgAl11O19, and Sr0.95Eu0.02Dy0.03Al2O4 at several photon energies (ranging from 81-1333 keV) using several radioactive point sources were measured and are listed in Table 1. The experimental µ/ρ value was compared with the theoretical one calculated using the WinXCOM computer software [22] to confirm the accuracy of the experimental results of this study. The experimental and theoretical results were plotted and the graphs are shown in Fig. 2. We see from Table 1 and Fig. 2 that the experimental and theoretical µ/ρ values decrease as the photon energy increases. The trend of µ/ρ with energy can be understood photon interaction mechanisms, namely, the photoelectric effect (PE), Compton scattering (CS), and pair production (PP), as discussed in previous studies [26, 30, 31]. At lower energies, the changes in the attenuation coefficients are due changes in the PE as the energy varies, whereas at medium-energies, they are dependent on changes in the CS effect. Furthermore, NaY0.77Yb0.20Er0.03F4, which includes two elements with a high Z value (Yb, Z=70 and Eu, Z=68), has the highest µ/ρ value among all of the studied materials. However, NaY0.77Yb0.20Er0.03F4 is twice as expensive as any of the other materials. Although the mass attenuation coefficient of Sr3.84Eu0.06Dy0.10Al14O25 is lower than those of the other samples, it is the least expensive among the samples. It is seen in Table 1 and Fig. 2 that the experimental and theoretical µ/ρ values are in good agreement. However, the small differences between the experimental and theoretical data are due to uncertainties in the system, thickness of the sample, original intensity (I0), and attenuated photon intensity (I) [25]. The uncertainties in attenuation coefficient values are less than ± 3.97%.
Energy (keV) | NaY0.77Yb0.20Er0.03F4 | Ba0.86Eu0.14MgAl10O17 | Sr3.84Eu0.06Dy0.10Al14O25 | Ce0.63Tb0.37MgAl11O19 | Sr0.95Eu0.02Dy0.03Al2O4 | |||||
---|---|---|---|---|---|---|---|---|---|---|
Exp. | WinX. | Exp. | WinX. | Exp. | WinX. | Exp. | WinX. | Exp. | WinX. | |
81 | 0.5767±0.0062 | 0.5924 | 0.3173±0.0034 | 0.3126 | 0.3043±0.0033 | 0.3110 | 0.3283±0.0035 | 0.3230 | 0.3984±0.0043 | 0.3871 |
122 | 0.2799±0.0040 | 0.2771 | 0.1979±0.0029 | 0.1904 | 0.1815±0.0026 | 0.1877 | 0.1848±0.0027 | 0.1944 | 0.2203±0.0032 | 0.2110 |
136 | 0.2447±0.0097 | 0.2350 | 0.1808±0.0066 | 0.1727 | 0.1620±0.0058 | 0.1703 | 0.1823±0.0066 | 0.1757 | 0.1796±0.0065 | 0.1870 |
161 | 0.1954±0.0054 | 0.1908 | 0.1479±0.0031 | 0.1529 | 0.1528±0.0037 | 0.1510 | 0.1601±0.0036 | 0.1550 | 0.1596±0.0037 | 0.1613 |
276 | 0.1210±0.0044 | 0.1184 | 0.1149±0.0041 | 0.1133 | 0.1179±0.0043 | 0.1123 | 0.1119±0.0040 | 0.1139 | 0.1182±0.0042 | 0.1142 |
303 | 0.1169±0.0026 | 0.1117 | 0.1060±0.0024 | 0.1086 | 0.1118±0.0025 | 0.1077 | 0.1103±0.0024 | 0.1091 | 0.1062±0.0024 | 0.1091 |
356 | 0.0978±0.0011 | 0.1016 | 0.0962±0.0011 | 0.1009 | 0.1021±0.0012 | 0.1002 | 0.0974±0.0011 | 0.1013 | 0.0967±0.0011 | 0.1009 |
384 | 0.0952±0.0028 | 0.0975 | 0.0948±0.0027 | 0.0976 | 0.0944±0.0028 | 0.0969 | 0.1005±0.0028 | 0.0979 | 0.1008±0.0028 | 0.0974 |
511 | 0.0810±0.0010 | 0.0841 | 0.0883±0.0011 | 0.0859 | 0.0839±0.0010 | 0.0854 | 0.0834±0.0010 | 0.0861 | 0.0822±0.0010 | 0.0854 |
662 | 0.0754±0.0009 | 0.0740 | 0.0739±0.0009 | 0.0764 | 0.0734±0.0009 | 0.0760 | 0.0742±0.0009 | 0.0765 | 0.0771±0.0009 | 0.0758 |
835 | 0.0692±0.0018 | 0.0660 | 0.0712±0.0020 | 0.0685 | 0.0715±0.0020 | 0.0681 | 0.0697±0.0020 | 0.0686 | 0.0700±0.0020 | 0.0679 |
1173 | 0.0551±0.0007 | 0.0556 | 0.0555±0.0007 | 0.0579 | 0.0550±0.0007 | 0.0576 | 0.0599±0.0007 | 0.0580 | 0.0596±0.0007 | 0.0574 |
1275 | 0.0556±0.0006 | 0.0532 | 0.0571±0.0007 | 0.0555 | 0.0574±0.0007 | 0.0552 | 0.0579±0.0007 | 0.0555 | 0.0537±0.0006 | 0.0550 |
1333 | 0.0514±0.0006 | 0.0520 | 0.0528±0.0006 | 0.0542 | 0.0555±0.0006 | 0.0539 | 0.0521±0.0006 | 0.0543 | 0.0562±0.0006 | 0.0537 |
-201907/1001-8042-30-07-008/alternativeImage/1001-8042-30-07-008-F002.jpg)
Table 2 presents the mass attenuation coefficient values for Al, Fe, and ordinary concrete [32] calculated by WinXCOM for comparison with the experimental values. From Table 1 and Table 2, it can be seen that the µ/ρ values for all studied samples are higher than that of Al in the energy range of 81-511 keV. Moreover, Fe has a higher µ/ρ value than all the experimental samples in the energy range of 81–303 keV. We note that all the samples have higher µ/ρ values than ordinary concrete at low energies (E<356 keV), while the µ/ρ value of ordinary concrete is higher than those of the samples at high energies (E> 384 keV).
Energy (keV) | Al | Fe | Ordinary concrete |
---|---|---|---|
81 | 0.1996 | 0.5787 | 0.2022 |
122 | 0.1520 | 0.2623 | 0.1567 |
136 | 0.1441 | 0.2233 | 0.1490 |
161 | 0.1337 | 0.1808 | 0.1386 |
276 | 0.1077 | 0.1156 | 0.1122 |
303 | 0.1038 | 0.1092 | 0.1082 |
356 | 0.0973 | 0.0999 | 0.1015 |
384 | 0.0943 | 0.0960 | 0.0984 |
511 | 0.0837 | 0.0833 | 0.0873 |
662 | 0.0747 | 0.0735 | 0.0779 |
835 | 0.0670 | 0.0656 | 0.0700 |
1173 | 0.0568 | 0.0553 | 0.0593 |
1275 | 0.0544 | 0.0530 | 0.0568 |
1333 | 0.0532 | 0.0518 | 0.0555 |
To test the effectiveness of any absorber in the attenuation of gamma photons, the RPE (%) was calculated using the measured original (I0) and attenuated photon intensities (I); our experimental values are listed in Table 3. The graph of RPE versus energy is as shown in Fig. 3. As seen in Table 3 and Fig. 3, the RPE values decrease with increasing photon energy. The RPE values of NaY0.77Yb0.20Er0.03F4, Ba0.86Eu0.14MgAl10O17, and Sr3.84Eu0.06Dy0.10Al14O25 are quite close to each other at high energies (E>200 keV), while NaY0.77Yb0.20Er0.03F4 has maximum RPE values of 14.75%, 7.45%, 6.55%, and 5.27% at energies of 81, 122, 136, and 161 keV, respectively.
Energy (keV) | NaY0.77Yb0.20Er0.03F4 | Ba0.86Eu0.14MgAl10O17 | Sr3.84Eu0.06Dy0.10Al14O25 | Ce0.63Tb0.37MgAl11O19 | Sr0.95Eu0.02Dy0.03Al2O4 |
---|---|---|---|---|---|
81 | 14.75±0.05 | 10.50±0.04 | 9.66±0.04 | 6.15±0.02 | 8.08±0.03 |
122 | 7.45±0.08 | 6.69±0.07 | 5.88±0.06 | 3.51±0.04 | 4.55±0.05 |
136 | 6.55±0.25 | 6.13±0.22 | 5.27±0.18 | 3.47±0.12 | 3.73±0.13 |
161 | 5.27±0.13 | 5.04±0.09 | 4.97±0.11 | 3.05±0.06 | 3.32±0.07 |
276 | 3.29±0.11 | 3.94±0.13 | 3.86±0.13 | 2.14±0.07 | 2.47±0.09 |
303 | 3.19±0.06 | 3.64±0.07 | 3.66±0.07 | 2.11±0.04 | 2.22±0.04 |
356 | 2.67±0.02 | 3.31±0.02 | 3.35±0.02 | 1.87±0.01 | 2.03±0.01 |
384 | 2.60±0.07 | 3.26±0.09 | 3.10±0.09 | 1.93±0.05 | 2.11±0.06 |
511 | 2.22±0.01 | 3.04±0.02 | 2.76±0.02 | 1.60±0.01 | 1.72±0.01 |
662 | 2.07±0.01 | 2.55±0.02 | 2.42±0.02 | 1.43±0.01 | 1.62±0.01 |
835 | 1.90±0.05 | 2.46±0.07 | 2.36±0.06 | 1.34±0.04 | 1.47±0.04 |
1173 | 1.51±0.01 | 1.92±0.01 | 1.82±0.01 | 1.15±0.01 | 1.25±0.01 |
1275 | 1.53±0.01 | 1.98±0.01 | 1.90±0.01 | 1.11±0.01 | 1.13±0.01 |
1333 | 1.41±0.01 | 1.83±0.01 | 1.84±0.01 | 1.00±0.01 | 1.18±0.01 |
-201907/1001-8042-30-07-008/alternativeImage/1001-8042-30-07-008-F003.jpg)
Fig. 4 contains a plot of the Zeff of the five samples versus photon energy in the photon energy range of 0.015-10 MeV, obtained using the Auto-Zeff program [33]. The size of Zeff values plotted in the figure can be explained by considering the three types of photon scattering in matter. In the lower energy region, the values of Zeff for all samples are highest, primarily due to the photoelectric interaction mechanism, as seen in Fig. 4, and the effective cross-section for this process depends directly upon the atomic number as Z4 and the photon energy as E−3.5 for any absorber. Apparently, Zeff reduces exponentially with increasing photon energy up to about 800 keV, and then Zeff values are almost constant. This is because the cross section for Compton scattering is related to the atomic number and the energy as Z and E−1, respectively. In this high energy region, Compton scattering is the most important interaction process. From Fig. 4, we see that the Zeff of NaY0.77Yb0.20Er0.03F4 > Zeff of Sr3.84Eu0.06Dy0.10Al14O25 > Zeff of Ce0.63Tb0.37MgAl11O19 > Zeff of Ba0.86Eu0.14MgAl10O17 > Zeff of Sr0.95Eu0.02Dy0.03Al2O4. The high Zeff values of NaY0.77Yb0.20Er0.03F4 are due to the presence of elements with high atomic number. We note that the graphs of Zeff values for all samples have discontinuities due to photoelectric absorption near the K-, L- and M-absorption edges of some elements at low energies (see Table 4). These results are in good agreement with the results for various glass systems obtained by El-Mallawany et al. [34], Kaur et al. [35], and Chanthima and Kaewkhao [36] and with the results for several smart polymer materials reported by Sayyed [37].
Element | Z | K | L1 | L2 | L3 | M1 | M2 | M3 | M4 | M5 |
---|---|---|---|---|---|---|---|---|---|---|
Na | 11 | 1.072 | - | - | - | - | - | - | - | - |
Mg | 12 | 1.305 | - | - | - | - | - | - | - | - |
Al | 13 | 1.559 | - | - | - | - | - | - | - | - |
Sr | 38 | 16.105 | 2.216 | 2.007 | 1.940 | - | - | - | - | - |
Y | 39 | 17.038 | 2.373 | 2.156 | 2.080 | - | - | - | - | - |
Ba | 56 | 37.440 | 5.989 | 5.624 | 5.247 | 1.293 | 1.137 | 1.062 | - | - |
Ce | 58 | 40.443 | 6.549 | 6.164 | 5.723 | 1.435 | 1.273 | 1.185 | - | - |
Eu | 63 | 48.519 | 8.052 | 7.617 | 6.977 | 1.800 | 1.614 | 1.481 | 1.161 | 1.131 |
Tb | 65 | 51.996 | 8.708 | 8.252 | 7.514 | 1.968 | 1.768 | 1.611 | 1.275 | 1.241 |
Dy | 66 | 53.789 | 9.046 | 8.581 | 7.790 | 2.047 | 1.842 | 1.676 | 1.322 | 1.295 |
Er | 68 | 57.486 | 9.751 | 9.264 | 8.357 | 2.207 | 2.006 | 1.812 | 1.453 | 1.409 |
Yb | 70 | 61.332 | 10.486 | 9.978 | 9.944 | 2.398 | 2.173 | 1.950 | 1.576 | 1.528 |
-201907/1001-8042-30-07-008/alternativeImage/1001-8042-30-07-008-F004.jpg)
4. Conclusion
The shielding performances of five compounds containing REEs, namely NaY0.77Yb0.20Er0.03F4, Ba0.86Eu0.14MgAl10O17, Sr3.84Eu0.06Dy0.10Al14O25, Ce0.63Tb0.37MgAl11O19, and Sr0.95Eu0.02Dy0.03Al2O4, were studied at photon energies between 81-1333 keV. The values of µ/ρ, RPE, and Zeff were experimentally and theoretically evaluated. The obtained values indicate that Zeff is dependent on gamma ray energy intensity as well as the interaction mechanism. The Zeff values peak when the photon energy values are low because the photoelectric effect around the K-, L-, and M- absorption edges of the samples dominates. Results for RPE and Zeff also revealed that, among the five materials studied, NaY0.77Yb0.20Er0.03F4 offers the best gamma ray radiation protection. The obtained data may be helpful in various radiation shielding applications.
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