(,) ve (,) Reaksiyonları için İstatistiksel Model Bileşenlerinin Optimum Değerlerinin İncelenmesi

Halim Büyükuslu
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Abstract

In order to further develop nuclear models/functions, it is important to test various models and functions included in cross-section calculations based on different reaction types, energy ranges, and masses. In this study, the dependence of nuclear ingredients such as level density, -nucleus optical model and γ-ray strength function on the cross-section were illustrated by making systematic calculations in the statistical model window. Reaction cross-section calculations were systematically performed for (α,γ) and (γ,α) reactions, which hold significant importance in astrophysics, on various target nuclei. Theoretical model calculations were compared with experimental data. For each set of experimental and calculated cross sections, the average deviation factor values were determined. The best-fit models and functions for all incoming alpha and gamma energies and for all target nuclei were identified.
调查 (,) 和 (,) 反应的统计模型成分的最佳值
为了进一步发展核模型/函数,必须根据不同的反应类型、能量范围和质量来测试横截面计算中包含的各种模型和函数。在本研究中,通过在统计模型窗口中进行系统计算,说明了核成分(如水平密度、-核光学模型和γ射线强度函数)对截面的依赖性。系统地计算了各种靶核上的(α,γ)和(γ,α)反应的反应截面,这些反应在天体物理学中具有重要意义。理论模型计算结果与实验数据进行了比较。针对每一组实验和计算截面,确定了平均偏差因子值。确定了所有α和γ入射能量以及所有靶核的最佳拟合模型和函数。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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