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Calculations of Cross-Sections and Astrophysical S-factors for the (alpha,n) Reactions of Some Structural Fusion Materials

机译:某些结构融合材料(α,n)反应的截面和天体S因子的计算

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Structural material selection in design of fusion reactors is very crucial. These structural materials should satisfy the hard conditions such as high thermo-mechanical stresses, high heat loads and severe radiation damage without compromising on safety considerations. The materials such as titanium, vanadium and chromium are used in the construction of fusion reactors. Therefore, it is important to examine these materials. Obtained results from the nuclear reactions using structural materials can be used for developing of these structural materials. For this reason, in this study cross sections of the Ti-46(alpha,n) Cr-49, Cr-50(alpha,n) Fe-53 and V-51(alpha,n) Mn-54 reactions have been calculated at 2-20 MeV energy range. In these theoretical calculations, the TALYS 1.8 and NON-SMOKER codes were used. Also, the astrophysical S-factors which describe the possibility of reaction in low energies were calculated. Results of our calculations were checked to the experimental data obtained from EXFOR database.
机译:在聚变反应堆设计中结构材料的选择非常关键。这些结构材料应满足诸如高热机械应力,高热负荷和严重的辐射损坏之类的苛刻条件,而不会影响安全性。诸如钛,钒和铬的材料用于聚变反应堆的构造。因此,检查这些材料很重要。使用结构材料的核反应获得的结果可用于开发这些结构材料。因此,在这项研究中,已计算出Ti-46(α,n)Cr-49,Cr-50(α,n)Fe-53和V-51(α,n)Mn-54反应的截面在2-20 MeV的能量范围内在这些理论计算中,使用了TALYS 1.8和NON-SMOKER代码。此外,还计算了描述低能量反应可能性的天体S因子。我们的计算结果与从EXFOR数据库获得的实验数据进行了核对。

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