首页> 外文期刊>The Journal of Chemical Physics >Two-component calculations for the molecules containing superheavy elements: Spin-orbit effects for (117)H, (113)H, and (113)F
【24h】

Two-component calculations for the molecules containing superheavy elements: Spin-orbit effects for (117)H, (113)H, and (113)F

机译:包含超重元素的分子的两组分计算:(117)H,(113)H和(113)F的自旋轨道效应

获取原文
获取原文并翻译 | 示例
           

摘要

We have calculated bond lengths, harmonic vibrational frequencies, and dissociation energies for (117)H, (113)H, and (113)F using relativistic effective core potentials (RECPs) with one-electron spin-orbit operators at the two-component coupled-cluster levels of theory. It is shown that any reasonable theoretical descriptions of the electronic structures of molecules containing superheavy elements require consideration of relativistic interactions and electron correlations. Comparisons with available all-electron Dirac-Fock (DF) based results indicate that our two-component approaches are very promising tools in the calculations for the molecules containing superheavy elements. The spin-orbit effects calculated from one- and two-component RECPs are in good agreement with those from all-electron Douglas-Kroll and DF results, implying that the potential average scheme is useful for obtaining one-component RECPs even for superheavy elements. Spin-orbit and electron correlation effects are not additive for molecular properties of (117)H, (113)H, and (113)F, but spin-orbit effects are qualitatively similar at all levels of theory considered. Spin-orbit effects contract R_e and increase #omega#_e for (113)H and (113)F, whereas they expand R_e and decrease #omega#_e for (117)H. Spin-orbit effects decrease D_e for all molecules considered, but the amount of decrease for (113)H and (117)H is substantially smaller than that estimated from the atomic splittings. For (117)H, our best calculations yield 1.983 A(R_e), 1403 cm~(-1)(#omega#_e), and 1.60 eV(D_e).
机译:我们已经使用相对论有效核心电位(RECP)和两分量的单电子自旋轨道算符来计算(117)H,(113)H和(113)F的键长,谐波振动频率和解离能耦合集群理论水平。结果表明,对包含超重元素的分子的电子结构的任何合理的理论描述都需要考虑相对论相互作用和电子相关性。与基于全电子狄拉克-福克(DF)的结果进行的比较表明,在计算包含超重元素的分子时,我们的两组分方法是非常有前途的工具。由一组分和二组分RECP计算得到的自旋轨道效应与全电子道格拉斯-克罗尔和DF结果所得出的自旋轨道效应非常吻合,这意味着势均方案对于获得一组分RECP甚至对于超重元素都是有用的。自旋轨道和电子相关效应对(117)H,(113)H和(113)F的分子性质没有加和作用,但是自旋轨道效应在所考虑的所有理论水平上在质量上都相似。自旋轨道效应使R_e收缩并使(113)H和(113)F的#omega#_e增大,而它们使R_e扩展并使(117)H的#omega#_e减小。自旋轨道效应降低了所考虑的所有分子的D_e,但是(113)H和(117)H的降低量明显小于从原子分裂估计的量。对于(117)H,我们的最佳计算得出1.983 A(R_e),1403 cm〜(-1)(#omega#_e)和1.60 eV(D_e)。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号