A Dispersive Optical Model Analysis of the Alpha Particles Scattering by Titanium Element Nucleus and Its Natural Isotopes

Haiddar Al-Mustafa, A. Belal
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Abstract

A dispersive optical model analysis of the alpha particles scattering by titanium element nucleus and its natural isotopes has been applied for a new scattering potential within the energy range (1-100) MeV which has contained the range of the Coulomb barrier, and for constant input values of the parameters of this potential. This potential is extent of the mean field potential and is called by (coulomb-nuclear) interference potential, that contains (spin-orbit) coulomb term. The results according to DOMACNIP program that has been designed for that purpose would contain: continuous energy variation of the depths of the real and imaginary parts of the mean field, which are connected by dispersion relations have been compared with these resulting from global parameterizations of the alpha particles scattering potential. In addition to continuous energy variation of the real radius parameter of the Wood-Saxon approximation to the mean field potential with its Hatree-Fock approximation of the nonlocal potential. Consequently, our results for the continuous energy variations of the predicted total reaction cross section within the energy range (1-100) MeV, and with calculation step of the pervious range whose magnitude (1 MeV), differential cross sections, Ratio of the differential elastic scattering cross section to Rutherford cross section and polarization resulted only from the Coulomb spin-orbit term that has been appeared characteristically for selected energy and for selected center-of-mass scattering angle within the energy range (1-100) MeV, showed the excellent agreement with available experimental data and better than these resulted from global parameterizations of the alpha particles scattering potential.
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α粒子被钛元素核及其天然同位素散射的色散光学模型分析
应用色散光学模型分析了α粒子被钛元素核及其天然同位素散射的过程,得到了包含库仑势垒范围的(1-100)MeV的新散射势,且该势的参数输入值恒定。该势是平均场势的范围,称为(库仑-核)干涉势,其中包含(自旋轨道)库仑项。根据为此设计的DOMACNIP程序得到的结果包括:通过色散关系连接的平均场实部和虚部深度的连续能量变化,并与α粒子散射势全局参数化的结果进行了比较。除了平均场势的Wood-Saxon近似和非局部势的Hatree-Fock近似的实半径参数的能量连续变化外。因此,我们对预测总反应截面在(1-100)MeV能量范围内的连续能量变化的结果,以及随着前一个量级(1 MeV)的计算步长,微分截面,微分弹性散射截面与卢瑟福散射截面的比值以及仅由库仑自旋轨道项所得到的极化值与现有实验数据的一致性较好,且优于α粒子散射势的全局参数化所得到的结果。
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