共查询到19条相似文献,搜索用时 187 毫秒
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用形变约束的相对论平均场理论系统研究了超重核294118及其α衰变链的基态性质, 给出了这些原子核的每核子结合能和α衰变能以及基态形变, 并与实验结果进行了比较, 发现理论计算和实验结果符合得很好, 表明相对论平均场理论对超重核基态性质的描述是合理有效的. 相似文献
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用宏观-微观模型系统计算了Z=95—113奇-偶超重核的基态性质. 理论计算的结合能、α衰变能与已知的实验数据符合较好, 也与相对论平均场的计算结果符合很好, 这进一步肯定了宏观-微观模型对超重核研究的可靠性. 理论计算表明形变对超重核的性质起重要作用. 同时, 对一些未知核素基态性质的预言可为将来的实验研究提供理论参考. 相似文献
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偶-偶超重核基态性质的理论研究 总被引:2,自引:0,他引:2
在形变的相对论平均场模型下采用NL Z2,TMA两套参数对一些偶 偶核基态性质进行了系统的计算,并将理论计算的结合能、α衰变能与已知的实验数据进行了对比分析.结果发现两方面的数据能够比较好地吻合,从而验证了相对论平均场模型对超重核研究是可行的.同时在计算中给出了未知核素基态性质的计算结果,可供以后在理论或实验上研究超重核时参考. The ground state properties of the even even nuclei with proton number Z=94-104 have been systematically calculated in the deformed relativistic mean field (RMF) theory with two sets of force parameters, TMA and NL Z2. Comparing the calculated binding energies and alpha decay energys with the experimental ones, it is found that theoretical results are in good agreement with experimental data. The reliability of the RMF model for even even superheavy nuclei has been tested by this comparison... 相似文献
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用宏观--微观模型系统计算了Z=94—112偶偶超重核的基态性质. 其中宏观部分基于液滴模型, 微观部分采用改进的谐振子势. 理论计算的结合能、α衰变能
与已知的实验数据符合, 理论计算结果也与Moller的计算结果符合很好.这肯定了宏观--微观模型对超重核性质研究的可靠性和稳定性. 对一些未知核素基态性
质的预言可为将来的实验研究提供理论参考. 相似文献
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在相对论平均场理论框架下, 用NL-3和NL-Z两组相互作用参数研究了4个同位素链28Ni,54Xe,78Pt,94Pu的基态性质. 发现,在Hatree近似下奇A核结合能理论计算值与实验值的相对误差反而普遍比偶偶核小. 这说明用相对论平均场理论,即使不考虑矢量介子的空间分量,仍可以比较可靠地计算奇A核结合能. 相似文献
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用自洽的相对论平均场模型研究了核271110及其α衰变链核的结构.理论的α衰变能与实验数据符合.理论的核寿命也与实验数据比较接近.预言了未知核素275112的性质,并讨论了质子数Z=108附近的形变壳效应. 相似文献
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The relativistic mean field (RMF) model with a small number of adjusted parameters has been used successfully in the last thirty years for predictions of various ground-state nuclear properties of nuclei. In this model, Dirac and Klein–Gordon like equations obtained from application of variation principle on phenomenological Lagrangian density are solved iteratively for calculations of nuclear properties of nuclei. For this purpose, parameters such as masses of considered mesons, nucleon–meson coupling constants, and self-couplings of mesons are needed and they are fitted from experimental data. Some parameter sets for RMF model introduced to correct predictions of nuclear properties of nuclei cover nuclidic chart. Besides Artificial Neural Network (ANN) method is used successfully in many field of science as in nuclear physics. ANN is known as a very powerful tool that are used when standard techniques fail to estimate the correlation between the variables. In the present study, ANN method has been employed to check its understanding capability of relations between RMF model parameters and their predictions on the ground-state binding energies of some spherical nuclei. Understanding capability of ANN method for these relations of considered nuclei has been found well. Based on this success, new non-linear parameter set for RMF model called DEFNE by us have been produced by using ANN method. Furthermore, predictions of RMF model with DEFNE parameter set for ground-state binding energies and charge radii of nuclei cover nuclidic chart have been found as in agreement with the available experimental data. 相似文献
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WANG Cheng-Bin DONG Tie-Kuang REN Zhong-Zhou ZHU Zhi-Yuan 《理论物理通讯》2009,51(5):895-898
The relativistic mean-field (RMF) theory is used to calculate the properties of A =7-9 drip-line nuclei ^7Li, ^7;9Be, ^8;9B, and ^9C. Systematic deviations between experimental and theoretical binding energies are found. Possible reasons of these systematic deviations are discussed in terms of pairing energy. The root-mean-square (rms) radii of matter distributions for these nuclei agree with the experimental data quite well. The one-proton halo structure in ^8B is reproduced well, and the two-proton halo in ^9C is predicted. The calculations show that the RMF theory is valid in studying the properties of light drip-line nuclei. 相似文献
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We systematically calculate the ground state properties of superheavy even-even nuclei with proton number Z=94–118. The calculations are based on the liquid drop macroscopic model and the microscopic model with the modified single-particle
oscillator potential. The calculated binding energies and α-decay energies agree well with the experimental data. The reliability of the macroscopic-microscopic(MM)model for superheavy
nuclei is confirmed by the good agreement between calculated results and experimental ones. Detailed comparisons between our
calculations and M?ller’s are made. It is found that the calculated results also agree with M?ller’s results and that the
MM model is insensitive to the microscopic single-particle potential. Calculated results are also compared with results from
relativistic mean-field (RMF) model and from Skyrme-Hatree-Fock(SHF) model. In addition, half-lives, deformations and shape
coexistence are also investigated. The properties of some unknown nuclei are predicted and they will be useful for future
experimental researches of superheavy nuclei. 相似文献
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The nuclei around magic number N = 126 are investigated in the deformed relativistic mean field (RMF) model with effective interactions TMA. We focus investigations on the N = 126 isotonic chain. The N = 126 shell evolution is studied by analyzing the variations of two-neutron (proton) separation energies, quadruple deformations, single particle levels etc. The good agreement of two-neutron separation energies between experimental data and calculated values is reached. The RMF theory predicts that the sizes of N = 126 shell become smaller and smaller with the increasing of proton number Z. However, the N = 126 shell exists in our calculated region all along. According to the calculated two-proton separation energies, the RMF theory suggests 220Pu is a two-proton drip-line nucleus in the N = 126 isotonic chain. 相似文献
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The ground state properties of superheavy nuclei are systematically
calculated by the macroscopic-microscopic (MM) model with the
Nilsson potential. The calculations well produced the ground state
binding energies, α-decay energies, and half lives of superheavy nuclei. The calculated results are systematically compared with available experimental data. The calculated results are also compared with theoretical results from other MM models and from relativistic mean-field model. The calculations and comparisons
show that the MM model is reliable in superheavy region and that the
MM model results are not very sensitive to the choice of microscopic
single-particle potential. 相似文献
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R. Goswami B. Sethi M. S. Sarkar S. Sen 《Zeitschrift für Physik A Hadrons and Nuclei》1995,352(4):391-395
The band structures of121, 123I nuclei have been studied using a version of the particle-rotor-model in which the experimental excitation energies of the neighbouring (A-1) cores can be fed directly as input parameters. The calculations have been carried out with axially symmetric Nilsson potential with both prolate and oblate deformations. The parameters of the model have been chosen from earlier theoretical work and experimental odd-even mass differences. Only the Coriolis attenuation factor has been treated as adjustable parameter. The theoretical band structures are in very good agreement with the available experimental data. 相似文献