Soil is a widely available material on Earth and is recognized as a cost-effective and accessible natural resource for radiation shielding purposes (Akman et al., Reference Akman, Turan, Sayyed, Akdemir, Kaçal, Durak and Zaid2019). There are several effective shielding materials, several of which are costly and potentially hazardous, such as heavy metals (AbuAlRoos et al., Reference AbuAlRoos, Amin and Zainon2019). When a soil is used as a shielding material, the clay fraction can prove particularly advantageous due to the reactive nature of its particles, facilitating the formation of cohesive structures (aggregates; Schaefer et al., Reference Schaefer, Fabris and Ker2008). Soil horizons exhibit variability in their physical and chemical properties influenced by the texture, chemical and mineralogical composition and type of the parent rock, among other factors (Hartemink et al., Reference Hartemink, Zhang, Bockheim, Curi, Silva and Grauer-Gray2020). Thus, from an environmental perspective, determining the shielding capacity of distinct soil horizons against radiation is crucial.
Numerous studies have confirmed the feasibility of depositing radioactive waste in natural sites, highlighting the importance of investigating the efficacy of various soil layers (horizons) for attenuating radiation (Delage et al., Reference Delage, Cui and Tang2010; Tsang et al., Reference Tsang, Neretnieks and Tsang2015; Eke, Reference Eke2022). It has been demonstrated that several dozen centimetres of natural materials, such as soil and clays, can efficiently attenuate gamma ray photons of various energies (Mann et al., Reference Mann, Brar, Mann and Mudahar2016; Mamikhin et al., Reference Mamikhin, Manakhov, Shcheglov and Tsvetnov2017).
Several parameters are used to evaluate the shielding ability of various materials. The linear (κ) and mass (μ) attenuation coefficients are essential parameters that enable the determination of the probability that a photon will be attenuated (Hubbell & Seltzer, Reference Hubbell and Seltzer1995). Another highly influential parameter is the mean free path (MFP), which indicates the average distance a photon can travel in a specific material before experiencing a collision (Alabsy & Elzaher, Reference Alabsy and Elzaher2023). Overall, the MFP offers an objective measure of the probability that a given interaction between photons and matter will occur. In addition, two commonly employed parameters are the half-value layer (HVL) and the tenth-value layer (TVL), which represent the thickness of material required to reduce the radiation intensity by a factor of one-half and one-tenth, respectively, of the initial intensity (Alabsy & Elzaher, Reference Alabsy and Elzaher2023). The effective atomic number (Z eff) is another parameter commonly used in radiation physics due to its importance in calculating the absorbed dose of radiation (Alabsy & Elzaher, Reference Alabsy and Elzaher2023). This parameter is used when materials composed of many chemical elements are analysed, such as the clay fraction of the soil.
Different techniques can be used in radiation shielding, which can be based on experimental measurements and computer simulation. These techniques allow numerous parameters to be obtained, the most common being attenuation coefficient data, cross-sections (σ), Z eff, electronic density (N eff), energy absorption and exposure build-up factors (EABF, EBF), effective conductivity (C eff), MFP, HVL, TVL and fast neutron removal cross-section (FNRCS; Şakar et al., Reference Şakar, Özpolat, Alım, Sayyed and Kurudirek2020). The attenuation coefficients, MFP, HVL, TVL and Z eff are commonly found in the literature (Abdul & Rashid, Reference Abdul and Rashid2021; Eke, Reference Eke2021; Marquez-Mata et al., Reference Marquez-Mata, Chavez, Campillo-Rivera, Vazquez-Bañuelos, Garcia-Duran and Vega-Carrillo2021; Gili, Reference Gili2023). Thus, our study used the radiation shielding parameters most commonly employed in the scientific literature. For a detailed description of radiation shielding techniques and the advantages and limitations of each method, we recommend the review article by Shultis & Faw (Reference Shultis and Faw2005).
Previous studies have examined soil and clays as potential radiation shielding materials (Kucuk et al., Reference Kucuk, Tumsavas and Cakir2013; Mann et al., Reference Mann, Kaur, Sidhu and Kumar2013; Akman et al., Reference Akman, Turan, Sayyed, Akdemir, Kaçal, Durak and Zaid2019; Isfahani et al., Reference Isfahani, Abtahi, Roshanzamir, Shirani and Hejazi2019a; Hila et al., Reference Hila, Javier-Hila, Sayyed, Asuncion-Astronomo, Dicen and Jecong2021). However, these studies usually analyse one unique layer and the soil as a whole rather than its fractions, such as the highly reactive clay fraction (Medhat et al., Reference Medhat, Demir, Akar Tarim and Gurler2014a; Singh et al., Reference Singh, Badiger and Kucuk2014; Mamikhin et al., Reference Mamikhin, Manakhov, Shcheglov and Tsvetnov2017). As the various soil horizons may differ in the chemical compositions of their clay fractions, thus affecting radiation attenuation (Gedik & Baytaş, Reference Gedik and Baytaş2015; Pires, Reference Pires2022), collecting soil samples along the soil profile is necessary to assess how each layer influences radiation shielding.
This study is based on the hypothesis that the various horizons, with slight differences between their mineral compositions and soil bulk densities, show variations in shielding parameters in terms of the various photon energies based on analysis of their soil clay fractions. The study aimed to characterize the chemical composition of the clay fractions in various horizons of an Arenosol and evaluate the efficiency of these horizons for shielding radiation. Additionally, the study aimed to observe the variations of the shielding parameters depending on the photon energy. A schematic illustration of the research steps is presented in Fig. S1.
The main advance of this study regarding the area of radiation shielding is the analysis of the clay fractions of various soil horizons. This type of investigation can provide information on the efficiency of each soil layer for attenuating radiation. The study also evaluates the clay fraction obtained through physical fractionation of the soil rather than clays composed of single minerals. In general, studies on radiation shielding in the scientific literature focus on pure clays. Using the clay fraction obtained directly from the soil could be an alternative for producing low-cost materials for radiation shielding.
Materials and methods
Soil sampling and soil preparation
The studied soil was collected from the profile located at coordinates 16°30'27" S and 52°22'29" W, with a local average elevation of 565 m, in the municipality of Baliza in the state of Goiás, Brazil (Fig. 1). This soil was identified as an Arenosol according to the IUSS Working Group WRB (2022) classification system. The soil comprises five horizons (Table 1).
Figure 1. (a,b) Location of the studied experimental site (Baliza, state of Goiás, Brazil) (adapted from the Brazilian Institute of Geography and Statistics (IBGE)). (c) Aerial view of the area (accessed from Google Earth on 10 February 2024). (d) Photograph of the experimental area. (e) Photograph of the Arenosol soil profile (horizons A, AC, CA, C1 and C2).
Table 1. Description of the soil horizons and the soil bulk densities (ρb) of the studied Arenosol.
The samples were air-dried at 40°C and passed through a 2 mm mesh sieve to obtain air-dried fine earth (ADFE). The silt and clay fractions of the ADFE were separated using NaOH (1 mol L–1), with the sand fraction (2 mm to 53 μm) separated by sieving. The silt and clay fractions were physically fractionated according to Stokes’ law (Gee & Bauder, Reference Gee, Bauder and Klute1986). The particle density of the ADFE was determined using a He gas pycnometer, ranging from 2.60 to 2.62 g cm–3.
The clay fraction was separated from the water with the addition of CaCl2 (1 mol L–1). Once obtained, the clay fraction was dried at 40°C, ground with a pestle and mortar and sieved through a 45 μm sieve. The soil texture (Fig. 2) was determined using the pipette method according to the procedure outlined in Tech et al. (Reference Tech, Pires, Brinatti, Saab, Correchel and Momoli2022).
Figure 2. Percentages of sand, silt and clay in the studied Arenosol for the various horizons: (a) A, (b) AC, (c) CA, (d) C1 and (e) C2.
X-ray diffraction and X-ray fluorescence analysis
X-ray diffraction (XRD) measurements of the clay fraction were obtained from one sample from each portion. The samples were placed in the sample holder and gently pressed with a glass slide to fix them in place. The XRD analysis was carried out using an Ultima IV diffractometer from Rigaku, Cu-Kα radiation, 40 kV, 30 mA, in the range 3–100°2θ, with a 0.02°2θ scanning step and a time of 5 s per step. The slit settings used were as follows: 10 mm horizontal divergence slit, 1° scatter slit and 0.15 mm receiving slit. The XRD traces were compared with the standard mineral patterns of the Mineralogy Database (https://www.webmineral.com/) and the American Mineralogist Crystal Structure Database (http://rruff.geo.arizona.edu/AMS/amcsd.php). This comparison was carried out by considering at least the three most intense diffraction peaks of each mineral, the corresponding interlayer spacing and the peak position for Cu-Kα radiation (Prandel et al., Reference Prandel, Saab, Brinatti, Giarola, Leite and Cassaro2014).
The chemical composition of the clay fractions in each horizon was determined semi-quantitatively using energy-dispersive X-ray fluorescence (EDXRF). Na to Sc were determined at 5 kV and Ti to U were determined at 50 kV, using ~1 g of powder samples. The samples were dried at 40°C, ground with a pestle and mortar, sieved through a 45 μm sieve and placed into sample holders. The measurements were carried out using a benchtop XRF spectrometer (EDX-720, Shimadzu) with a Si(Li) semiconductor system detector cooled with liquid N at –196°C (Ferreira et al., Reference Ferreira, Pires, Brinatti and Auler2018).
Calculation of shielding parameters
The XCOM (Hubbell & Berger, Reference Hubbell and Berger1987) and Phy-X/PSD (Şakar et al., Reference Şakar, Özpolat, Alım, Sayyed and Kurudirek2020) programs were used to calculate the mass attenuation coefficient. These programs can analyse both pure and compound elements, such as soil clay fractions composed of several chemical elements. For this study, the photon energy range selected was 15 keV to 10 MeV. This range was chosen to verify the attenuation efficiency of the clay fraction for low (15 and 50 keV), intermediate (100 keV to 1 MeV) and high (>1 MeV) energy levels. The mass attenuation coefficient of a compound or a mixture can be obtained using the formula given in Equation 1 (Hubbell & Berger, Reference Hubbell and Berger1987):
where μi is the mass attenuation coefficient of the ith term and Wi is the weight fraction.
Based on the soil bulk density (ρb) results, the linear attenuation coefficient of the clay fraction was calculated. Soil bulk density was determined using sieved soil samples placed in volumetric flasks with a volume of ~17.7 cm3. The flasks were carefully filled with a funnel using small vibrations. The filling procedure followed is similar to that used in κ measurements according to the gamma-ray attenuation method (Costa et al., Reference Costa, Borges, Pires, Arthur and Bacchi2014). The ρb values obtained for the various horizons are listed in Table 1. Multiplying μ by ρb enabled calculation of κ, which is related to the probability of a photon being attenuated or absorbed per unit length.
The MFP, which measures the average distance travelled by a particle before it collides with another particle, was calculated using the relationship given in Equation 2 (Şakar et al., Reference Şakar, Özpolat, Alım, Sayyed and Kurudirek2020):
where x represents the thickness of the absorber material.
The HVL and TVL were calculated according to Equations 3 & 4 (Şakar et al., Reference Şakar, Özpolat, Alım, Sayyed and Kurudirek2020):
The effective atomic number was calculated from the ratio between the atomic (σa) and electronic (σe) cross-sections as per Equation 5 (Şakar et al., Reference Şakar, Özpolat, Alım, Sayyed and Kurudirek2020):
The atomic cross-section was obtained from division of the molecular cross-section (σm) by the total number of formula units as per Equation 6 (Medhat et al., Reference Medhat, Pires and Arthur2014b):
where $\mathop \sum \limits_i n_i$
is the total number of formula units of the compound. The molecular cross-section was calculated as per Equation 7 (Medhat et al., Reference Medhat, Pires and Arthur2014b):
where $M = \mathop \sum \limits_i n_iA_i$
is the molecular weight of the compound, NA is the Avogadro number, Ai is the atomic weight of the ith element and ni is the number of formula units in the molecule. The total electronic cross-section was obtained using Equation 8 (Medhat et al., Reference Medhat, Pires and Arthur2014b):
where $f_i = {{n_i} \over {\mathop \sum \nolimits_j n_j}}$
and Z i are the fractional abundance and the atomic number of the ith constituent element, respectively, n j is the number of atoms of the constituent element and $\mathop \sum \limits_j n_j$
is the total number of atoms present in the molecular formula.
Statistical analysis
Analysis of variance (ANOVA) was used to compare the results among the various soil horizons regarding their chemical compositions and mass attenuation coefficients. The normality and equal variance assumptions were checked using the Shapiro–Wilk and Bartlett tests, respectively. Once these assumptions were confirmed, the F-test was employed. When significant interactions were found, Tukey's test was used for post-hoc comparisons. Furthermore, Pearson's linear correlation analysis was conducted to assess possible correlations among the measured parameters. The MFP, HVL, TVL and Z eff parameters were analysed based on the average values and standard deviation. The statistical data processing was performed using the Past program (version 3.20), as described by Hammer et al. (Reference Hammer, Harper and Ryan2001).
Results
Mineralogical and chemical analysis
The XRD traces of the clay fractions of the soil samples are shown in Fig. 3. The clay fractions of all horizons were similar in terms of mineralogical composition, indicating a predominance of kaolinite (Kln; Bish & Von Dreele, Reference Bish and Von Dreele1989) and gibbsite (Gbs; Balan et al., Reference Balan, Lazzeri, Morin and Mauri2006). Other minerals present are calcite (Cal; Graf, Reference Graf1961), quartz (Qz; Wei, Reference Wei1935), anatase (An; Howard et al., Reference Howard, Sabine and Dickson1991) and magnetite (Mag; Wechsler et al., Reference Wechsler, Lindsley and Prewitt1984), with the latter two minerals being the main hosts of the Ti and Fe detected in the clay fractions.
Figure 3. XRD traces of the clay fractions of the Arenosol for the various soil horizons (A, AC, CA, C1 and C2); d-spacings are in Ångstroms (Å). An = anatase; Cal = calcite; cps = counts per second; Gbs = gibbsite; Kln = kaolinite; Mag = magnetite; Qz = quartz.
No significant differences (p > 0.05) were found for the contents of Al2O3, SiO2, Fe2O3 and SO3 (Table 2). The first three oxides accounted for ~95% of the chemical composition of the clay fraction in the studied horizons. The variation in Al2O3, SiO2 and Fe2O3 between horizons ranged between ~3.8% (AC and C1), ~4.4% (A and C1) and ~9.9% (A and C1). CaO, K2O and TiO2 displayed significant differences (p ≤ 0.05) between specific horizons (Table 2). However, their contribution (CaO + K2O + TiO2) to the composition of the clay fraction was relatively low, ranging from ~4.8% (A) to ~5.8% (AC). Only those oxides with concentrations near or exceeding 1% are presented in Table 2. The full chemical composition of the soil clay fraction is listed in Table S1.
Table 2. Average values of the chemical compositions of the clay fractions of the soil horizons (A, AC, CA, C1 and C2) of the studied Arenosol.
Notes: Only the oxides with the highest concentrations are shown. The values in parentheses represent the standard deviation of the average (n = 3). (–) indicates a standard deviation much smaller than the last significant figure of the average value. The superscript letters indicate significant differences between the soil horizons in terms of the oxide in question (p < 0.05).
Radiation shielding parameters
No significant differences (p > 0.05) were observed in the mass attenuation coefficients between the different photon energy ranges analysed and among the soil horizons (Table 3). The most considerable variations were observed at lower energies (15 and 50 keV), between AC and C1, by ~3%. When analysing the partial effects of radiation attenuation (namely, photoelectric absorption, coherent scattering, incoherent scattering and pair production), it became evident that photoelectric absorption is responsible for the majority of photon attenuation at lower energies, accounting for ~95% of the total attenuation (Fig. 4). As photon energy increased to intermediate levels, incoherent scattering became the predominant contributor to photon attenuation, responsible for ~82% at 100 keV and virtually 100% at 1 MeV. However, at higher energies, nuclear field pair production was more significant, accounting for ~32% of the radiation attenuation (Fig. 4f). However, as observed for the μ values (Table 3), there were no differences in the contributions of the partial attenuation effects between the horizons of the clay fraction studied.
Table 3. Average values of the mass attenuation coefficients for the various soil horizons (A, AC, CA, C1 and C2) and photon energies (E).
Notes: The values in parentheses represent the standard deviation of the average (n = 3). (–) indicates a standard deviation much smaller than the last significant figure of the average value. Superscript letters indicate significant differences between soil horizons in terms of the photon energy in question (p < 0.05). The statistical test was not applied for energies greater than 100 keV due to the lack of variability between the mass attenuation coefficient results among horizons.
Figure 4. Contributions of partial effects (photoelectric absorption (PA), coherent scattering (CS), incoherent scattering (IS) and pair production (PP)) to the total attenuation coefficients (μ) for photon energies of (a) 15 keV, (b) 50 keV, (c) 100 keV, (d) 500 keV, (e) 1 MeV and (f) 10 MeV. A, AC, CA, C1 and C2 represent the various Arenosol horizons. PPn = pair production in a nuclear field; PPe = pair production in an electron field.
Given the deviations (error bars) from the average values, the MFP differences were less noticeable for the lowest photon energies (15 and 50 keV; Fig. 5a,b). However, as photon energy increased (>50 keV), the differences between the soil horizons became more apparent (Fig. 5c–f). The intermediate horizon (CA) displayed the greatest average MFP value, while the surface horizon (A) displayed the lowest average MFP value. The range of MFP values between the horizons (A and CA) varied by ~5.4% (15 keV to 10 MeV). When accounting for the different photon energies, the MFP (average values considering all of the horizons) ranged from ~0.091 cm (15 keV) to 30.51 cm (10 MeV).
Figure 5. Variation in the MFP values for the various horizons (A, AC, CA, C1, C2) of the Arenosol studied for the photon energies of (a) 15 keV, (b) 50 keV, (c) 100 keV, (d) 500 keV, (e) 1 MeV and (f) 10 MeV.
Similarly to MFP, lower photon energies (15 and 50 keV) exhibited more subtle differences in the HVL (Fig. 6a,b) and TVL (Fig. 7a,b). Nonetheless, as photon energy increased (>50 keV), both HVL (Fig. 6c–f) and TVL (Fig. 7c–f) exhibited more pronounced differences (based on error bars) among the studied horizons. The surface horizon (A) demonstrated the lowest average values of both parameters, while the CA horizon exhibited the highest values. In accordance with MFP, the difference between the highest and lowest HVL and TVL average values for the horizons (A and CA) was ~5.4% (50 keV to 10 MeV). Considering the different photon energies, the HVL and TVL (average values considering all of the horizons) ranged from ~0.063 cm (15 keV) to 21.14 cm (10 MeV) and from 0.21 cm (15 keV) to 70.24 cm (10 MeV), respectively.
Figure 6. Variation in the HVL values for the various horizons (A, AC, CA, C1, C2) of the Arenosol studied for the photon energies of (a) 15 keV, (b) 50 keV, (c) 100 keV, (d) 500 keV, (e) 1 MeV and (f) 10 MeV.
Figure 7. Variation in the TVL values for the various horizons (A, AC, CA, C1, C2) of the Arenosol studied for the photon energies of (a) 15 keV, (b) 50 keV, (c) 100 keV, (d) 500 keV, (e) 1 MeV and (f) 10 MeV.
The effective atomic number showed slight differences among the soil horizons considering the average values and their deviations (error bars) for the various photon energies examined (Fig. 8). Generally, the Z eff average values were similar across horizons for the various energies, with the AC horizon having the greatest Z eff value. Among the photon energies, the lowest one (15 keV) had the greatest Z eff values, averaging ~14.5 (Fig. 8a). The Z eff value demonstrated a noticeable decrease with energy increasing up to 1 MeV, averaging ~10.3. It then showed a slight increase up to 10 MeV, averaging ~10.6 (Fig. 8e,f). The most significant decrease in Z eff was recorded between the energies of 50 keV (Fig. 8b) and 100 keV (Fig. 8c), where it decreased up to ~14.4%.
Figure 8. Variation in the effective atomic number (Z eff) for the various horizons (A, AC, CA, C1, C2) of the Arenosol studied for the photon energies of (a) 15 keV, (b) 50 keV, (c) 100 keV, (d) 500 keV, (e) 1 MeV and (f) 10 MeV.
Discussion
This study aimed to verify the efficiency of the clay fractions from various horizons (with slight differences in their mineralogical compositions) to shield photons of various energies. The clay fraction used was selected as it is possible to be mixed with other materials (e.g. concrete and metal) to produce radiation shielding materials (Akbulut et al., Reference Akbulut, Sehhatigdiri, Eroglu and Çelik2015; Isfahani et al., Reference Isfahani, Abtahi, Roshanzamir, Shirani and Hejazi2019a). Clay also has a high capacity to form soil aggregates; hence, it might be used as a shielding material due to its ability to produce soil aggregates that are relatively stable and have a strong structure (Hillel, Reference Hillel2014; Mann et al., Reference Mann, Brar, Mann and Mudahar2016).
The soil texture results (Fig. 2) show that the clay fraction varied from 9% (A horizon) to 14% (C2 horizon). The soil studied mainly consists of sand, ranging from 80% (A) to 70% (C2). The soil composition aligns with the Arenosols found in Brazil (Oliveira et al., Reference Oliveira, Nearing, Hawkins, Stone, Rodrigues, Panachuki and Wendland2016; Silva et al., Reference Silva, Montanari, Lima, da Silva, Freitas and Pinotti2017), with the texture classified as loamy sand in the most superficial horizon (A) and sandy loam in the remaining horizons. The clay fraction is mainly composed of Al2O3 and SiO2 (Table 2), the most abundant Arenosol oxides (Ngole-Jeme & Ekosse, Reference Ngole-Jeme and Ekosse2015). The mineralogical composition of the clay fraction is in agreement with other Arenosols (Mareschal et al., Reference Mareschal, Nzila, Turpault, Thongo M'Bou, Mazoumbou and Bouillet2011; Bortoluzzi et al., Reference Bortoluzzi, dos Santos, Santanna and Caner2013; dos Santos et al., Reference dos Santos, Le Pera, Souza Júnior, Corrêa and Azevedo2017; Lima et al., Reference Lima, Inda, Zinn, Silva and Nascimento2022; Zacháry et al., Reference Zacháry, Filep, Jakab, Ringer, Balázs, Németh and Szalai2023).
Due to the slight variations in the contents of the major oxides (Al2O3, SiO2 and Fe2O3) present in the clay fractions, no differences were observed in the mass attenuation coefficients (Table 3) for the various photon energies between the various horizons. The μ values are comparable to previous studies on soils, clays or sands (Medhat et al., 2014a; Eke, Reference Eke2021; Pires, Reference Pires2022; Gili, Reference Gili2023). As photon energy increases, μ values decrease, similar to that which has been observed in previous work (Singh et al., 2014; Gurler et al., 2021; Gili, Reference Gili2023). Analysing the partial attenuation effects, it can be observed that photoelectric absorption is prevalent at lower energies (Fig. 4a,b), as it depends on Z 5 (Camargo et al., 2021). However, with increasing energy levels, photoelectric absorption becomes less critical due to its inverse dependence on photon energy (E 7/2; Kaplan, Reference Kaplan1963). For intermediate energy levels (Fig. 4c–e), incoherent scattering is the predominant process affecting photon attenuation. This effect is directly proportional to Z (Camargo et al., 2021). For higher energies (Fig. 4f), pair production (i.e. when an electron–positron pair is formed after a photon with an energy of 1.022 MeV or more interacts with an atom's nuclear force field) contributes more significantly to the photon attenuation, which is related to the dependence of this effect on Z 2 (Camargo et al., Reference Camargo, Kodum and Pires2021). Overall, the similarities in the contribution of partial effects (i.e. photoelectric absorption, coherent scattering, incoherent scattering and pair production) to the total mass attenuation coefficient can be explained by slight variations in the chemical compositions of the clay fractions between horizons, particularly for the heavier chemical elements (Camargo et al., Reference Camargo, Kodum and Pires2021; Pires, Reference Pires2022).
The parameters for MFP (Fig. 5), HVL (Fig. 6) and TVL (Fig. 7) showed slight variations among the horizons for the lowest photon energies (15 and 50 keV) considering the deviations (error bars) of the average values. The horizons with the highest bulk densities (A and C2) had the lowest MFP, HVL and TVL values, even at the lowest energies (except for 50 keV). Nevertheless, as the photon energy increased (>50 keV), the differences in MFP (Fig. 5c–f), HVL (Fig. 6c–f) and TVL (Fig. 7c–f) between the various horizons became more pronounced. This result does not indicate that the proportional differences between these parameters’ highest and lowest values across the horizons have changed considering the various photon energies. These differences remain practically the same (~5.4%), but the average values’ deviations (error bars) become negligible for the higher energies. One possible explanation for these findings is that MFP, HVL and TVL values converge at greater photon energies due to the weaker attenuation caused by the absorber, resulting in reduced variability (Table 3). Inasmuch as the horizons have comparable chemical compositions, the differences in MFP, HVL and TVL were mainly influenced by the bulk density values of the absorber. Horizon (A), with the greatest bulk density, displayed the lowest MFP, TVL and HVL values, whereas horizon (CA), with the lowest bulk density, exhibited the highest MFP, TVL and HVL values. Eke (Reference Eke2022) also observed more significant variation in MFP, HVL and TVL between various soil layers (horizons) at the greatest photon energies for soils composed mainly of Ca and O, similar to the findings observed in our study.
The linear attenuation coefficient is affected by the soil bulk density, as previously stated. Thus, an increase in ρb leads to an increase in κ, assuming that the chemical composition of the material and the photon energy remain constant (Ferraz & Mansell, Reference Ferraz and Mansell1979). The parameters MFP, HVL and TVL are inversely related to κ (Equations 2–4). In general, samples with higher ρb exhibited lower MFP (Fig. 5), HVL (Fig. 6) and TVL values (Fig. 7). In this study, κ, obtained by multiplying μ by ρb, and μ, which varied depending on the chemical composition of the soil, influenced the MFP, HVL and TVL parameters.
The MFP, HVL and TVL values observed were consistent with those reported in the literature (i.e. they increased with increasing photon energy; Gülbiçim et al., Reference Gülbiçim, Tufan and Türkan2017; Isfahani et al., Reference Isfahani, Abtahi, Roshanzamir, Shirani and Hejazi2019a; Eke, Reference Eke2022). The MFP values were comparable to those observed by Eke (Reference Eke2021), although Eke reported slightly lower values than those in the current study due to the greater density of the analysed sands. However, in another study conducted with soils, Eke (Reference Eke2022) reported MFP values similar to those observed in our study. Our HVL values are consistent with those of Singh et al. (Reference Singh, Badiger and Kucuk2014), who worked with various soils with densities similar to ours; Gurler et al. (Reference Gurler, Tumsavas and Akar Tarim2020), who analysed soils with similar amounts of Fe2O3 to those observed in our study; and Gülbiçim et al. (Reference Gülbiçim, Tufan and Türkan2017), who investigated the efficiency of vermiculite in radiation shielding. Regarding the study by Gülbiçim et al. (Reference Gülbiçim, Tufan and Türkan2017), their MFP and HVL values were lower than those observed in the current study as they only used a single type of clay. The TVL values obtained were consistent with those obtained in similar studies that used clays and soils of comparable chemical composition (i.e. consisting mainly of SiO2, Al2O3 and Fe2O3; Isfahani et al., Reference Isfahani, Abtahi, Roshanzamir, Shirani and Hejazi2019b; Gurler et al., Reference Gurler, Tumsavas and Akar Tarim2020; Pires, Reference Pires2022).
The optimum values for horizon (A), with the best shielding results for MFP, can be defined as a function of photon energy as 0.088 cm (15 keV), 1.74 cm (50 keV), 3.82 cm (100 keV), 7.77 cm (500 keV), 10.68 cm (1 MeV) and 29.59 cm (10 MeV). The same horizon exhibited the greatest shielding capacity according to the HVL and TVL results. The HVL values obtained were 0.061 cm (15 keV), 1.21 cm (50 keV), 2.65 cm (100 keV), 5.39 cm (500 keV), 7.40 cm (1 MeV) and 20.51 cm (10 MeV), whereas for TVL the values recorded were 0.202 cm (15 keV), 4.02 cm (50 keV), 8.79 cm (100 keV), 17.90 cm (500 keV), 24.59 cm (1 MeV) and 68.14 cm (10 MeV).
The effective atomic number showed slight differences between the horizons and the various photon energies in terms of average values and the corresponding standard deviations (error bars; Fig. 8). The results of this study are consistent with those in the literature for soil and clay samples (Akman et al., Reference Akman, Turan, Sayyed, Akdemir, Kaçal, Durak and Zaid2019; Marquez-Mata et al., Reference Marquez-Mata, Chavez, Campillo-Rivera, Vazquez-Bañuelos, Garcia-Duran and Vega-Carrillo2021, Gili, Reference Gili2023). The fluctuations observed in Z eff values with energy were also reported for zeolites (Gili, Reference Gili2023), soils of various textures (Kucuk et al., Reference Kucuk, Tumsavas and Cakir2013) and various types of natural quartz (Marquez-Mata et al., Reference Marquez-Mata, Chavez, Campillo-Rivera, Vazquez-Bañuelos, Garcia-Duran and Vega-Carrillo2021). Thus, although natural materials such as clays and quartz have distinct chemical compositions, they are mainly composed of light elements (low Z), so the Z eff values are similar to those in the current study.
Horizon (AC) exhibited the greatest Z eff values for all of the analysed photon energies. One possible explanation for this is the greater concentration of CaO and Fe2O3 (7.4% in total) encountered in this layer (Al-Masri et al., Reference Al-Masri, Hasan, Al-Hamwi, Amin and Doubal2013; Taqi & Khalil, Reference Taqi and Khalil2017; Camargo et al., Reference Camargo, Kodum and Pires2022). The importance of Fe and Ca oxides to attenuating radiation in soils, especially for lower photon energies, has been well demonstrated (Mudahar et al., Reference Mudahar, Modi and Makhan1991; Al-Masri et al., Reference Al-Masri, Hasan, Al-Hamwi, Amin and Doubal2013; Tarim et al., Reference Tarim, Gurler, Ozmutlu and Yalcin2013; Taqi & Khalil, Reference Taqi and Khalil2017; Camargo et al., Reference Camargo, Kodum and Pires2021). In addition, soils with greater Ca contents had higher Z eff values (Eke, Reference Eke2022), which is in accord with the findings from the current study. The remaining horizons have comparable CaO and Fe2O3 contents; hence, the differences in the abundances of the remaining elements across photon energies may explain the differences between these horizons. In addition, the minor differences in the Fe2O3 contents observed between horizons may explain the similar Z eff values (Table 3).
Azreen et al. (Reference Azreen, Rashid, Haniza, Voo and Amran2018) analysed two types of concrete made from silica sand and lead glass and reported μ, HVL and TVL values of 0.065 cm2 g–1, 2.56 cm and 4.17 cm, respectively, for the silica sand concrete and 0.071 cm2 g–1, 2.44 cm and 4.05 cm, respectively, for the lead glass. Gili (Reference Gili2023) analysed natural zeolite and reported a μ value of 0.077 cm2 g–1 and a HVL value of 8.05 cm. Isfahani et al. (Reference Isfahani, Abtahi, Roshanzamir, Shirani and Hejazi2019b) recorded HVL and TVL values ranging from 3.53 to 4.96 cm (HVL) and from 11.74 to 16.47 cm (TVL) for clays modified with barite powder. Working with clay fly ash bricks, Mann et al. (Reference Mann, Brar, Mann and Mudahar2016) found μ values ranging from 0.0757 to 0.0789 cm2 g–1. The Z eff reported in the aforementioned works ranged from 10.73 to 11.85. Mirji & Lobo (Reference Mirji and Lobo2017) reported μ, HVL and TVL values ranging from 0.079 to 0.088 cm2 g–1, from 3.78 to 8.37 cm and from 12.54 to 27.76 cm, respectively, for polymeric materials of various compositions. The shielding parameters of all of these studies were obtained for the 137Cs radioactive source. For comparison, in the current study, which also simulated the results for the photon energy of a 137Cs source, μ was 0.076 cm2 g–1 (all soil horizons), HVL ranged from 6.10 cm (horizon (A)) to 6.44 cm (C2), TVL varied from 20.25 (A) to 21.40 cm (C2) and Z eff varied from 10.27 (C1) to 10.31 (C2)
The clay fraction of the studied soil has the potential to be used for radiation shielding. Previous studies suggested that natural materials can be as effective for radiation shielding as conventional materials such as concrete and are therefore promising for shielding due to their low cost, abundance and ease of extraction (Mann et al., Reference Mann, Kaur, Sidhu and Kumar2013; Gülbiçim et al., Reference Gülbiçim, Tufan and Türkan2017). For lower photon energies, blocks containing clay or clay mixtures may provide a viable alternative for radiation shielding (Mann et al., Reference Mann, Brar, Mann and Mudahar2016).
Conclusions
This study of a Brazilian Arenosol as a radiation shielding material yielded the following conclusions. The major oxides (Al2O3, SiO2 and Fe2O3) and the mineralogical composition do not differ significantly between the soil horizons. The mass attenuation coefficient and the effective atomic number of the horizons across the radiation energies did not differ significantly between the soil horizons. The proposed hypothesis was partially confirmed, as evidenced by the differences between the horizons, mainly for photon energies greater than 100 keV for MFP, HVL and TVL. The horizons with the greatest bulk densities exhibited the best shielding efficiencies. Overall, the surface horizon (A) demonstrated the most effective shielding results. This finding is evidenced by its lower MFP, HVL and TVL values compared with the other horizons. The effective atomic number was not a sensitive parameter for demonstrating differences between the horizons due to the slight variations in soil chemical compositions and mass attenuation coefficients. However, upon comparison of the results of this study with the previous scientific literature, it is evident that the clay fraction of the studied Arenosol is effective for shielding radiation. The presence of Fe and Al oxides in the clay fraction is fundamental to forming cohesive structures due to the clay minerals’ ability to form aggregates. This factor makes the clay fraction interesting as a material for attenuating radiation as denser clay structures are more efficient as radiation shielding materials. Another advantage of using clays is that extraction of a soil fraction can produce more affordable materials with the potential for use in radiation attenuation.
Acknowledgements
The authors thank the institutional laboratories FASCA/UEPG, GPMFE/UEPG, C-LABMU/UEPG, Coordination for the Improvement of Higher Education Personnel (Capes), Araucaria Foundation for Supporting Scientific and Technological Development of the State of Paraná (FA) and Brazilian National Council for Scientific and Technological Development (CNPq). LFP thanks CNPq for the research grant (304925/2019-5).
Financial support
This research was partially funded by the Coordination for the Improvement of Higher Education Personnel (CAPES – Coordenação de Aperfeiçoamento de Pessoal de Nível Superior; Grant 88882.450143/2019-01 and Finance Code 001) and Araucaria Foundation for Supporting Scientific and Technological Development of the State of Paraná (FA – Fundação Araucária de Apoio ao Desenvolvimento Científico e Tecnológico do Estado do Paraná; Grant 88882.168500/2018-01).
Conflicts of interest
The authors certify that they have no affiliations with or involvement in any organization or entity with any financial interest or non-financial interest in the subject matter or materials discussed in this manuscript.
Data availability
The datasets generated and/or analysed during the current study are available from the authors upon reasonable request.
Author contributions
Luiz F. Pires: Conceptualization, Formal analysis, Writing – original draft, Writing – review and editing. Victor A. Yanaguisawa: Formal analysis, Conceptualization, Investigation, Funding acquisition, Project administration, Resources, Writing – original draft. André M. Brinatti: Methodology, Formal analysis, Funding acquisition, Investigation, Project administration, Resources, Writing – original draft. Sérgio C. Saab: Project administration, Resources, Writing – original draft. Vladia Correchel: Project administration, Resources, Writing – original draft. All authors have read and agreed to the published version of the manuscript.
