Composite materials such as metal glasses or alloys combine the useful properties and compensate for the shortcomings of the constituent materials. Therefore, a composite material has improved attributes relative to its individual constituents and therefore, more functionalities. This makes alloys very attractive for radiation shielding in many extreme radiation environments. In this report, different gamma-photon interaction parameters of four SnX alloys (where, X = As, Bi, P, and Sb) were evaluated and analyzed at 0.2, 0.662, and 1.25 MeV. The mass attenuation coefficients (μ⁄ρ) of the materials were calculated using the XCOM. Furthermore, other parameters such as the effective atomic number (Zeff), electron density (Neff), mass energy absorption, the specific gamma constant, absorbed gamma dose rate, and buildup factors were also estimated. The values of μρ decreased with energy from 0.2844 cm2/g to 0.0518 cm2/g for SnP, 0.2664 cm2/g to 0.0510 cm2/g for SnAs, 0.3321 cm2/g to 0.0509 cm2/g for SnSb, and 0.7771 cm2/g to 0.0664 cm2/g for SnBi. Also, (Zeff)SnX and (Neff)SnX decreased with photon energy within the ranges of 33.01–41.25 and 2.66–3.32 1023 electrons/g for SnP; 41.68–44.30 and 2.59–2.76 1023 electrons/g for SnAs; 56.50–56.51 and 2.329–2.53 1023 electrons/g for SnSb; and 68.26–75.43 and 2.51–2.77 1023 electrons/g for SnBi, respectively. The exposure buildup factor of SnP, SnAs, SnSb, and SnBi at a depth of 40 mfp for 1,25 MeV photons were 27, 30, 17, and 16, respectively. Based on the computed quantities, it is clear that SnBi interact more with photons compared to the other three SnX materials. Moreover, the SnX materials can perform better than some commercial and well-known glass shields, especially at low photon energies. Being Pb-free, the SnX shields are preferable to commercial glass shields containing Pb for radiation protection purposes.
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