SPECTROSCOPIC CONSTANTS AND POTENTIAL-ENERGY CURVES FOR OSH

被引:11
作者
BENAVIDESGARCIA, M
BALASUBRAMANIAN, K
机构
[1] Department of Chemistry, Arizona State University, Tempe
关键词
D O I
10.1016/0022-2852(91)90210-2
中图分类号
O64 [物理化学(理论化学)、化学物理学]; O56 [分子物理学、原子物理学];
学科分类号
070203 ; 070304 ; 081704 ; 1406 ;
摘要
Complete active space (CASSCF) followed by first-order configuration interaction (FOCI) and second-order CI (SOCI) are carried out on 21 low-lying electronic states of OsH. Spin-orbit effects are investigated using the relativistic CI (RCI) methodology. The ground state of OsH is found to be 4Π symmetry with Re = 1.606 A ̊, ωe = 2138 cm-1, De = 2.317 eV, and μe = -1.651 D in the absence of spin-orbit interactions, while the ground state is found to be a strong mixture of 4Π( 5 2) and 4Δ( 5 2) including spin-orbit coupling. Potential energy surfaces for 21 low-lying electronic states are reported. Allowed electronic transitions from the ground X4Π and some other low-lying states are predicted. The nature and bonding of the low-lying electronic states are analyzed through Mulliken populations. © 1991.
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页码:271 / 279
页数:9
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