在 sdgh 专业的壳模型计算为中子缺乏的 <SUP>106</SUP>,<SUP>107</SUP>,<SUP>108</SUP>,<SUP>109</SUP 轰炸 > Sn 同位素被使用 CD 波恩和 Nijmegen1 执行了二身体的有效核子核子相...在 sdgh 专业的壳模型计算为中子缺乏的 <SUP>106</SUP>,<SUP>107</SUP>,<SUP>108</SUP>,<SUP>109</SUP 轰炸 > Sn 同位素被使用 CD 波恩和 Nijmegen1 执行了二身体的有效核子核子相互作用。单个壳的状态和为描述 Sn 同位素需要的相应矩阵元素被重建由减少计算要求计算部分 parantage 的系数。这重建允许我们在很合理的时间做中子的壳模型计算缺乏的 Sn 同位素。结果与最近的高分辨率的试验性的数据相比并且发现在对实验的好同意。展开更多
The full and reduced shell model calculations have been carried out for the light odd-even ^105Sb and ^107Sb isotopes. The model space has been chosen as 1d5/2, 0g7/2, 1d3/2, 2s1/2, and 0h11/2 for the full calculation...The full and reduced shell model calculations have been carried out for the light odd-even ^105Sb and ^107Sb isotopes. The model space has been chosen as 1d5/2, 0g7/2, 1d3/2, 2s1/2, and 0h11/2 for the full calculations and excluded 0h11/2 for the reduced calculations. The reduced shell model calculations of ^105Sb and ^107Sb isotopes are presented for the first time. We obtain the energy spectra for the ^105Sb and ^107Sb isotopes in the full and reduced model space by using CD-Bonn two-body effective nucleon-nucleon interaction. The resulting energy spectra are compared to the experimental results to understand the effect of the 0h11/2 level on the shell model calculations. We draw conclusions about the right model space in the shell model calculations for the isotopes around the N =Z= 50 region of the periodic table.展开更多
We have performed two kinds of non-linear fitting procedures to the single-particle energies in the sdgh major shell to obtain better shell model results. The low-lying energy eigenvalues of the light Sn isotopes with...We have performed two kinds of non-linear fitting procedures to the single-particle energies in the sdgh major shell to obtain better shell model results. The low-lying energy eigenvalues of the light Sn isotopes with A = 103- 110 in the sdgh-shell are calculated in the framework of the nuclear shell model by using CD-Bonn two-body effective nucleonnucleon interaction. The obtained energy eigenvalues are fitted to the corresponding experimental values by using two different non-linear fitting procedures, i.e., downhill simplex method and clonal selection method. The unknown single-particle energies of the states 2s1/2, 1d3/2, and 0h11/2are used in the fitting methods to obtain better spectra of the104,106,108,110 Sn isotopes. We compare the energy spectra of the104,106,108,110 Sn and103,105,107,109 Sn isotopes with/without a nonlinear fit to the experimental results.展开更多
基金supported in part by the Scientific and Technological Council of Turkey under Grant No.TUBITAK 105T092Süleyman Demirel University under Grant No.SDUBAP 1075-m-05
文摘在 sdgh 专业的壳模型计算为中子缺乏的 <SUP>106</SUP>,<SUP>107</SUP>,<SUP>108</SUP>,<SUP>109</SUP 轰炸 > Sn 同位素被使用 CD 波恩和 Nijmegen1 执行了二身体的有效核子核子相互作用。单个壳的状态和为描述 Sn 同位素需要的相应矩阵元素被重建由减少计算要求计算部分 parantage 的系数。这重建允许我们在很合理的时间做中子的壳模型计算缺乏的 Sn 同位素。结果与最近的高分辨率的试验性的数据相比并且发现在对实验的好同意。
文摘The full and reduced shell model calculations have been carried out for the light odd-even ^105Sb and ^107Sb isotopes. The model space has been chosen as 1d5/2, 0g7/2, 1d3/2, 2s1/2, and 0h11/2 for the full calculations and excluded 0h11/2 for the reduced calculations. The reduced shell model calculations of ^105Sb and ^107Sb isotopes are presented for the first time. We obtain the energy spectra for the ^105Sb and ^107Sb isotopes in the full and reduced model space by using CD-Bonn two-body effective nucleon-nucleon interaction. The resulting energy spectra are compared to the experimental results to understand the effect of the 0h11/2 level on the shell model calculations. We draw conclusions about the right model space in the shell model calculations for the isotopes around the N =Z= 50 region of the periodic table.
基金Supported in part by Sleyman Demirel University under Grant No.SDUBAP 1822-YL-09the Scientific and Technological Council of Turkey under Grant No.TUBITAK 105T092
文摘We have performed two kinds of non-linear fitting procedures to the single-particle energies in the sdgh major shell to obtain better shell model results. The low-lying energy eigenvalues of the light Sn isotopes with A = 103- 110 in the sdgh-shell are calculated in the framework of the nuclear shell model by using CD-Bonn two-body effective nucleonnucleon interaction. The obtained energy eigenvalues are fitted to the corresponding experimental values by using two different non-linear fitting procedures, i.e., downhill simplex method and clonal selection method. The unknown single-particle energies of the states 2s1/2, 1d3/2, and 0h11/2are used in the fitting methods to obtain better spectra of the104,106,108,110 Sn isotopes. We compare the energy spectra of the104,106,108,110 Sn and103,105,107,109 Sn isotopes with/without a nonlinear fit to the experimental results.