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Odd-Even Effects of the Survival Probability for Superheavy Compound Nuclei 总被引:1,自引:0,他引:1 下载免费PDF全文
The survival probability of the superheavy compound nuclei with Z=114 is studied with the statistical model. It is found that the survival probability shows drastic odd-even effects. The odd-A compound nuclei have higher survival probability by evaporating three neutrons as compared with their neigbouring even-A compound nuclei. 相似文献
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In the framework of the relativistic mean field theory, the effects of the 6 meson on protoneutron star matter with hyperons at finite temperature are investigated. In thermal protoneutron star matter, the 6 field potential increases with density first and then decreases. Fixing the density, the increase of the temperature suppresses the 6 field potential. With the inclusion of the 6 meson, the threshold densities for hyperons become lower and the abundance of trapped neutrinos decreases. The most important effect of the 6 meson is to increase the abundance of hyperons in the inner core range of protoneutron stars. With the rise of the temperature, the density range where the 6 meson plays an important role is narrowed and the effects of the 6 meson are suppressed. Moreover, the protoneutron star mass and radius are nearly not affected by the 6 meson. 相似文献
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利用连续介质模型并基于Nilsson模型考虑微观修正, 研究了重核区原子核( Z≥82)基态性质, 得到了较好的结果。 通过拟合 Z≥82原子核的结合能实验数据, 得到了两组连续介质模型的新参数。 利用这两组参数计算的重核结合能与实验值的均方根偏差约为0.8 MeV, 电荷半径的均方根偏差约为0.07 fm。 The continuous medium model with shell correction from Nilsson model is used to study the ground state properties of heavy nuclei (Z≥82). New parameters are obtained for the continuous medium model by fitting the experimental binding energies. The theoretical calculations for the masses and radii are in good agreements with experimental values, and the root mean square deviations are about 0.8 MeV for the masses, and about 0.07 fm for the radii. 相似文献
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We investigate the equation of state of asymmetric nuclear matter and its isospin dependence in various spin-isospin ST channels within the framework of the Brueckner-Hartree-Fock approach extended to include a microscopic three-body force(TBF) . It is shown that the potential energy per nucleon in the isospinsinglet T = 0 channel is mainly determined by the contribution from the tensor SD coupled channel. At high densities,the TBF effect on the isospin-triplet T = 1 channel contribution turns out to be much larger than that on the T =0 channel contribution. At low densities around and below the normal nuclear matter density,the isospin dependence is found to come essentially from the isospin-singlet SD channel and the isospin-triplet T = 1 component is almost independent of isospin asymmetry. As the density increases,the T = 1 channel contribution becomes sensitive to the isospin asymmetry and at high enough densities its isospin dependence may even become more pronounced than that of the T = 0 contribution. The present results may provide some microscopic constraints for improving effective nucleon-nucleon interactions in a nuclear medium and for constructing new functionals of effective nucleon-nucleon interaction based on microscopic many-body theories. 相似文献
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