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后d族13 - 17族元素的变分与扩散蒙特卡罗研究

Variational and diffusion Monte Carlo study of post-d group 13-17 elements.

作者信息

Al-Saidi W A

机构信息

Laboratory of Atomic and Solid State Physics, Cornell University, Ithaca, New York 14853, USA.

出版信息

J Chem Phys. 2008 Aug 14;129(6):064316. doi: 10.1063/1.2969098.

Abstract

We present ab initio calculations of atomic and molecular systems containing the first-, second-, and third-row post-d elements (Ga-Br, In-I, and Tl-At) using several methods including variational and diffusion Monte Carlo. In the quantum Monte Carlo calculations, we used the recent scalar-relativistic energy-consistent Hartree-Fock pseudopotentials [M. Burkatzki et al., J. Chem. Phys. 126, 234105 (2007)], which are nonsingular at the origin. For the first- and second-row elements, the calculated ionization energies and electron affinities are in excellent agreement with those obtained using CCSD(T) with large basis sets and with experiment after correcting approximately for spin-orbit effects. For the third-row elements, where relativistic effects cannot be adequately included by a simple j-averaging, the results are in excellent agreement with CCSD(T) energies obtained with a large (5-zeta) basis set. Benchmark calculations of the dissociation energies, vibration frequencies, and equilibrium bond lengths of several diatomic molecules including As(2), Br(2), Sb(2), and I(2) as well as the hydrides XH (X = Ga, Br, In, I, and At) are presented.

摘要

我们使用包括变分蒙特卡罗和扩散蒙特卡罗在内的多种方法,对包含第一、第二和第三周期后d元素(Ga - Br、In - I和Tl - At)的原子和分子体系进行了从头计算。在量子蒙特卡罗计算中,我们使用了最近的标量相对论能量一致哈特里 - 福克赝势[M. Burkatzki等人,《化学物理杂志》126, 234105 (2007)],其在原点处无奇异性。对于第一和第二周期元素,计算得到的电离能和电子亲和能与使用大基组的CCSD(T)方法得到的结果以及在大致校正自旋 - 轨道效应后与实验值都非常吻合。对于第三周期元素,由于简单的j平均不能充分包含相对论效应,计算结果与使用大(5 - ζ)基组得到的CCSD(T)能量非常吻合。本文还给出了包括As₂、Br₂、Sb₂和I₂以及氢化物XH(X = Ga、Br、In、I和At)在内的几种双原子分子的解离能、振动频率和平衡键长的基准计算结果。

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