ENERGY AND FINE-STRUCTURE OF 1S(2)ND AND 1S(2)NF STATES FOR THE LITHIUM ISOELECTRONIC SEQUENCE

被引:55
作者
WANG, ZW
ZHU, XW
CHUNG, KT
机构
[1] JILIN UNIV,INST ATOM & MOLEC PHYS,CHANGCHUN,PEOPLES R CHINA
[2] TONG JI UNIV,DEPT PHYS,SHANGHAI,PEOPLES R CHINA
关键词
D O I
10.1088/0953-4075/25/19/006
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
The non-relativistic energies of 1s2 nd (n = 3, 4 and 5) and 1s2 nf (n = 4 and 5) states for the lithium isoelectronic sequence from Li I to Ne VIII are calculated with a full-core plus correlation method using multiconfiguration interaction wavefunctions. Relativistic and mass-polarization effects on the energy are evaluated perturbatively as the first-order corrections. The fine structure is calculated by using spin-orbit and spin-other-orbit interaction operators. Our results are in excellent agreement with experimental data in the literature. Possible misidentifications in the observed optical spectra are pointed out. They show that this full-core plus correlation method is useful for excited atomic systems with a 1s2 core.
引用
收藏
页码:3915 / 3927
页数:13
相关论文
共 30 条
[11]  
EDLEN B, 1934, NOVA ACTA REG SOC, V6, P153
[12]   THE SPECTRUM OF 6 TIMES IONIZED FLUORINE [J].
ENGSTROM, L .
PHYSICA SCRIPTA, 1984, 29 (02) :113-118
[13]   SPECTRAL LINE CLASSIFICATION IN PERIOD BETWEEN FLUORINE AND SILICON, OF TRANSITIONS BETWEEN LEVELS OF PRINCIPAL QUANTUM NUMBERS 3 AND 4 [J].
FAWCETT, BC .
JOURNAL OF PHYSICS PART B ATOMIC AND MOLECULAR PHYSICS, 1971, 4 (08) :1115-&
[14]   VARIATIONAL PREDICTIONS OF TRANSITION ENERGIES AND ELECTRON-AFFINITIES - HE AND LI GROUND-STATES AND LI, BE, AND MG CORE-EXCITED STATES [J].
FISCHER, CF .
PHYSICAL REVIEW A, 1990, 41 (07) :3481-3488
[15]  
HALLIN R, 1966, ARK FYS, V31, P511
[16]  
JOHANSSON I, 1959, ARK FYS, V15, P169
[17]  
JOHANSSON L, 1961, ARK FYS, V20, P489
[18]   2ND-ORDER ENERGIES AND 3RD-ORDER MATRIX-ELEMENTS OF ALKALI-METAL ATOMS [J].
JOHNSON, WR ;
IDREES, M ;
SAPIRSTEIN, J .
PHYSICAL REVIEW A, 1987, 35 (08) :3218-3226
[19]  
KELLY RL, 1987, J PHYS CHEM REF D S1, V16
[20]  
KNIGH RE, 1980, PHYS REV A, V22, P3161