112,114,116,118,120,122,124Sn同位素在10-80 MeV入射能量范围内的模拟激发函数

H. Büyükuslu
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引用次数: 0

摘要

截面数据不仅在核物理的应用领域得到了广泛的应用,而且对于理解核反应机理、开发和检验现有核反应模型的有效性都是必不可少的。可靠的实验数据是与理论核模型计算比较检验预测能力的重要依据。在实验数据失效的情况下,理论模型填补了这一空缺,以提供计算数据。由于这些原因,实验研究和理论研究都是相互需要的。长期以来,人们对质子总反应截面的计算进行了理论研究。在这些研究的最后,作者提出了几个解析方程。对所提方程的比较和不同参数值的重新排列对于成功地得到结果是非常重要的。本研究利用M.A. Alvi提出的质子-核相互作用分析方程,计算了Sn同位素112,114,116,118,120,122,124的质子总反应截面。同时,用TALYS程序对相同的反应进行了光学模型计算。用收集到的质子入射能量高达80 MeV的实验数据绘制了激发函数。通过确定的激励函数曲线进行了系数比较。用激发函数图对所得结果进行了讨论,并与已有的实验数据进行了比较。计算数据与实测数据之间的一致性令人满意。通过对这些锡同位素和这些能量范围的所得结果,对所用理论模型进行了验证和测试。
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Modelled Excitation Functions of 112,114,116,118,120,122,124Sn Isotopes for an Incident Energy Range of 10-80 MeV
The data of the cross–section is required for understanding nuclear reaction mechanism, developing and testing validity of available nuclear reaction models as much as it has been used in the applied fields of nuclear physics. Reliable experimental data is importance of comparison with theoretical nuclear model calculations for testing predictive ability. In the event that experimental data failure appearance, theoretical models are filling this gab for supplying with calculated data. Because of these reasons, both of experimental and theoretical studies need of each other. For a long time, theoretically studies have been carried out for proton total reaction cross section calculation. At the end of these studies, several analytical equations have been proposed by their authors.  Comparison of the suggested equations and rearrangement for different value of parameters are enormously important for reaching successfully results. In this study, proton total reaction cross sections have been calculated for 112,114,116,118,120,122,124 Sn isotopes using proton-nucleus interaction analytic equation that was proposed by M.A. Alvi. Also, optical model calculations carried out for same reactions by TALYS code. Excitation functions have been plotted with collected experimental data up to 80 MeV proton incident energy. Coefficient comparisons have been made via determined excitation function curves. The obtained results have been discussed by way of the excitation function graphics and compared with the available experimental data. Satisfactory agreements have been seen between calculated data and its measured equivalents. A validation of used theoretical model has been confirmed and tested via obtained results for these Sn isotopes and these energy ranges.
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