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Probing The Gateway To Superheavy Nuclei In Cranked Relativistic Hartree-Bogoliubov Theory

机译:在相对论的Hartree-Bogoliubov理论中探索通往超重核的途径

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摘要

The cranked relativistic Hartree+Bogoliubov theory has been applied for a systematic study of the nuclei around ~(254)No, the heaviest nuclei for which detailed spectroscopic data are available. The deformation, rotational response, pairing correlations, quasi-particle and other properties of these nuclei have been studied with different relativistic mean field (RMF) parametrizations. For the first time, the quasi-particle spectra of odd deformed nuclei have been calculated in a fully self-consistent way within the framework of the RMF theory. The energies of the spherical subshells, from which active deformed states of these nuclei emerge, are described with an accuracy better than 0.5 MeV for most of the subshells with the NL1 and NL3 parametrizations. However, for a few subshells the discrepancy reach 0.7-1.0 MeV. The implications of these results for the study of superheavy nuclei are discussed.
机译:相对论性的Hartree + Bogoliubov摇动理论已被用于对〜(254)No附近核的系统研究,这是最重的核,可提供详细的光谱数据。这些核的形变,旋转响应,配对相关性,准粒子和其他特性已通过不同的相对论平均场(RMF)参数进行了研究。在RMF理论的框架内,首次以完全自洽的方式计算了奇形变核的准粒子光谱。对于大多数具有NL1和NL3参数化的子壳,描述了球形子壳的能量,从这些子壳中出现了这些原子核的活跃变形状态,其准确度优于0.5 MeV。但是,对于一些子壳而言,差异达到0.7-1.0 MeV。讨论了这些结果对超重核研究的意义。

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