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首页> 外文期刊>The Journal of Chemical Physics >Automatically generated Coulomb fitting basis sets: Design and accuracy for systems containing H to Kr
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Automatically generated Coulomb fitting basis sets: Design and accuracy for systems containing H to Kr

机译:自动生成的库仑拟合基础集:包含H到Kr的系统的设计和精度

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For intermediate sized chemical systems the use of an auxiliary basis set (ABS) to fit the charge density provides a useful means of accelerating the performance of various quantum chemical methods. As a consequence much effort has been devoted to the design of various ABSs. This paper explores a fundamentally new approach where the ABS is created dynamically based on the specific orbital basis set (OBS) being used. The new approach includes a parameter that is used to coalesce candidate fitting functions together but which can also be used to provide some coarse grain control over the number of functions in the ABS. The accuracy of the new automatically generated ABS (auto-ABS) is systemically studied for a variety of small systems containing the elements H-Kr. Errors in the Coulomb energy computed using auto-ABS and with a variety of OBSs are shown to be small compared to errors in the Hartree-Fock energy due to incompleteness in the OBS. In contrast to fixed size ABSs, the use of auto-ABS is shown to lead to smaller errors as the size (quality) of the OBS is expanded. The performance of auto-ABS is also compared with the use of the recently proposed universal fitting sets [Weigend, Phys. Chem. Chem. Phys. 8, 1057 (2006)] for 180 compounds containing atoms from H to Kr. (c) 2007 American Institute of Physics.
机译:对于中等规模的化学系统,使用辅助基本集(ABS)来适应电荷密度提供了一种有用的手段,可以加快各种量子化学方法的性能。结果,已经在各种ABS的设计上进行了很多努力。本文探索了一种根本性的新方法,其中基于所使用的特定轨道基础集(OBS)动态创建ABS。新方法包括一个参数,该参数用于将候选拟合函数合并在一起,但也可以用于对ABS中的函数数量进行一些粗粒度控制。对于包含元素H-Kr的各种小型系统,系统地研究了新的自动生成的ABS(auto-ABS)的准确性。与由于OBS的不完整性而导致的Hartree-Fock能量的误差相比,使用自动ABS和各种OBS计算的库仑能量的误差显示出很小的误差。与固定大小的ABS相比,随着OBS的大小(质量)的扩展,使用自动ABS会导致较小的错误。还将自动ABS的性能与最近提出的通用配件套件的使用进行了比较[Weigend,Phys。化学化学物理8,1057(2006)]中发现180种含有H至Kr原子的化合物。 (c)2007年美国物理研究所。

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