在固体乙,乙烯和乙的结合能量的贡献超出了直接随机相近似值
Khanh Ngoc Pham1, Marcin Modrzejewski2, Jiří Klimeš1
1Department of Chemical Physics and Optics, Faculty of Mathematics and Physics, Charles University, Ke Karlovu 3, CZ-12116 Prague 2, Czech Republic.
The Journal of chemical physics
|June 10, 2024
概括
随机相近似 (RPA) 为分子晶体结合能提供了一种高效的初始方法. 超越RPA的校正,如四级缩放交换,显著提高了对具有挑战性的分子集群的准确性.
科学领域:
- 计算化学是一种计算化学.
- 量子化学是一种量子化学.
- 材料科学是一种材料科学.
背景情况:
- 随机相近似 (RPA) 是一个初始的电子结构方法.
- RPA有效地捕捉了更高阶的相关性能量贡献.
- 实际的RPA应用程序面临的挑战是紧的集群和参考状态依赖.
研究的目的:
- 在RPA中研究分子晶体结合能量的问题.
- 评估RPA之外的纠正的影响.
- 改进非极性分子团的描述.
主要方法:
- 晶体结合能量的多体扩张.
- 将RPA与RPA之外的纠正进行比较.
- 使用自相一致的哈特里-福克轨道与科恩-沙姆状态.
主要成果:
- 四次缩放交换和非环合集群双重校正显示出有利的影响.
- 自相一致的Hartree-Fock轨道改善了三元体相互作用,但低估了二元体能量.
- 与重新规范化的单体相比,可以实现与RPA相比的大幅改善.
结论:
- 超越RPA的校正提供了一条可行的途径来提高准确性.
- 轨道选择显著影响相互作用能量计算.
- 为了进行可靠的电子结构计算,需要对RPA纠正进行进一步的研究.
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