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基于钨和铋的重合金:制造、晶体结构、形态及对伽马辐射的屏蔽效率

Heavy alloy based on tungsten and bismuth: fabrication, crystal structure, morphology, and shielding efficiency against gamma-radiation.

作者信息

Tishkevich Daria I, Rotkovich Anastasia A, German Stepan A, Zhaludkevich Aliaksandr L, Vershinina Tatiana N, Bondaruk Anastasia A, Razanau Ihar U, Dong Mengge, Sayyed M I, Leonchik Sergey V, Zubar Tatiana, Silibin Maxim V, Trukhanov Sergei V, Trukhanov Alex V

机构信息

SSPA "Scientific-Practical Materials Research Centre of NAS of Belarus" 220072 Minsk Belarus

Belarusian National Technical University 220013 Minsk Belarus.

出版信息

RSC Adv. 2023 Aug 15;13(35):24491-24498. doi: 10.1039/d3ra04509a. eCollection 2023 Aug 11.

DOI:10.1039/d3ra04509a
PMID:37588974
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC10426328/
Abstract

W-BiO composites were fabricated using the hot isostatic pressing technique for the first time. The duration of the samples sintering was 3 minutes under conditions of high pressure and temperature. The study of microstructural features and chemical composition of sintered samples was carried out using scanning electron microscopy and energy-dispersive X-ray spectroscopy, respectively. The effect of temperature on the quality of the obtained W-BiO composites is determined. The densest samples were obtained at a pressure of 5 GPa and temperatures of 25 °C and 500 °C, the densities of which were 18.10 and 17.85 g cm, respectively. It is presented that high temperature exposure during sintering adversely affects both the composite density and microstructure due to the redox reaction accompanied by the reduction of Bi and the oxidation of W. The results of the W-BiO structure study using X-ray diffraction analysis showed that all samples included the main bulk-centered cubic W phase. The presence of the WO phase is noted only when the sintering temperature is increased up to 850 °C, which is confirmed by the appearance of diffraction peaks that correspond to 111 and 22-2 crystallographic planes. The shielding efficiency of the W-BiO composite against gamma radiation using the Phy-X/PSD software was evaluated. A Co isotope with an energy of 0.826-2.506 MeV was used as a source of gamma radiation. The calculation results were compared with those for Pb and Bi. Key shielding parameters such as the linear attenuation coefficient, half-value layer, tenth-value layer, mean free path, and effective atomic number are determined. The calculation results revealed that the W-BiO composite surpasses Pb and Bi in its shielding properties, which makes it promising for use as a prospective material for radiation shielding applications.

摘要

首次采用热等静压技术制备了W-BiO复合材料。在高压和高温条件下,样品烧结持续时间为3分钟。分别使用扫描电子显微镜和能量色散X射线光谱对烧结样品的微观结构特征和化学成分进行了研究。确定了温度对所得W-BiO复合材料质量的影响。在5 GPa压力以及25℃和500℃温度下获得了密度最大的样品,其密度分别为18.10和17.85 g/cm³。结果表明,烧结过程中的高温暴露由于伴随Bi还原和W氧化的氧化还原反应而对复合材料的密度和微观结构产生不利影响。使用X射线衍射分析对W-BiO结构的研究结果表明,所有样品均包含主要的体心立方W相。仅当烧结温度提高到850℃时才注意到WO相的存在,这通过对应于111和22 - 2晶面的衍射峰的出现得到证实。使用Phy-X/PSD软件评估了W-BiO复合材料对伽马辐射的屏蔽效率。使用能量为0.826 - 2.506 MeV的钴同位素作为伽马辐射源。将计算结果与铅和铋的计算结果进行了比较。确定了诸如线性衰减系数、半价层、十分之一价层、平均自由程和有效原子序数等关键屏蔽参数。计算结果表明,W-BiO复合材料在屏蔽性能方面超过了铅和铋,这使其有望用作辐射屏蔽应用的潜在材料。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ffa0/10426328/885f7f7bc26e/d3ra04509a-f6.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ffa0/10426328/66c0daf7a989/d3ra04509a-f1.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ffa0/10426328/f9dd24cd6712/d3ra04509a-f2.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ffa0/10426328/0ba98d8df3e0/d3ra04509a-f3.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ffa0/10426328/fafdf53578d6/d3ra04509a-f4.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ffa0/10426328/de5ed123cb84/d3ra04509a-f5.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ffa0/10426328/885f7f7bc26e/d3ra04509a-f6.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ffa0/10426328/66c0daf7a989/d3ra04509a-f1.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ffa0/10426328/f9dd24cd6712/d3ra04509a-f2.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ffa0/10426328/0ba98d8df3e0/d3ra04509a-f3.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ffa0/10426328/fafdf53578d6/d3ra04509a-f4.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ffa0/10426328/de5ed123cb84/d3ra04509a-f5.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/ffa0/10426328/885f7f7bc26e/d3ra04509a-f6.jpg

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