Atomic structure calculations of superheavy noble element oganesson (Z=118)

被引：26

作者：

Lackenby, B. G. C. ^{[1
]}

Dzuba, V. A. ^{[1
]}

Flambaum, V. V. ^{[1
,2
]}

机构：

[1] Univ New South Wales, Sch Phys, Sydney, NSW 2052, Australia

[2] Johannes Gutenberg Univ Mainz, D-55099 Mainz, Germany

来源：

PHYSICAL REVIEW A | 2018年 / 98卷 / 04期

基金：

澳大利亚研究理事会;

关键词：

RARE-GAS; ELECTRONIC-STRUCTURE; ABSORPTION-LINES;

D O I：

10.1103/PhysRevA.98.042512

中图分类号：

O43 [光学];

学科分类号：

070207 ; 0803 ;

摘要：

We calculate the spectrum and allowed E1 transitions of the superheavy element Og (Z = 118). A combination of configuration interaction and perturbation theory is used [Dzuba et al., Phys. Rev. A 95, 012503 (2017)]. The spectrum of lighter analog Rn I is also calculated and compared to experiment with good agreement.

引用

页数：5

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