Importance profiles. Visualization of atomic basis set requirements

Fuente: arXiv
Saved in:
Bibliographic Details
Main Author: Lehtola, Susi
Format: Preprint
Published: 2023
Subjects:
Online Access:
Tags: Add Tag
No Tags, Be the first to tag this record!
_version_ 1866917914157776896
author Lehtola, Susi
author_facet Lehtola, Susi
contents Recent developments in fully numerical methods promise interesting opportunities for new, compact atomic orbital (AO) basis sets that maximize the overlap to fully numerical reference wave functions, following the pioneering work of Richardson and coworkers from the early 1960s. Motivated by this technique, we suggest a way to visualize the importance of AO basis functions employing fully numerical wave functions computed at the complete basis set (CBS) limit: the importance of a normalized AO basis function $|α\rangle$ centered on some nucleus can be visualized by projecting $|α\rangle$ on the set of numerically represented occupied orbitals $|ψ_{i}\rangle$ as $I_{0}(α)=\sum_{i}\langleα|ψ_{i}\rangle\langleψ_{i}|α\rangle$. Choosing $α$ to be a continuous parameter describing the orbital basis, such as the exponent of a Gaussian-type orbital (GTO) or Slater-type orbital (STO) basis function, one is then able to visualize the importance of various functions. The proposed visualization $I_{0}(α)$ has the important property $0\leq I_{0}(α)\leq1$ which allows unambiguous interpretation. We also propose a straightforward generalization of the importance profile for polyatomic appliations $I(α)$, in which the importance of a test function $|α\rangle$ is measured as the increase in projection from the atomic minimal basis. We exemplify the methods with importance profiles computed for atoms from the first three rows, and for a set of chemically diverse diatomic molecules. We find that the importance profile offers a way to visualize the atomic basis set requirements for a given system in an a priori manner, provided that a fully numerical reference wave function is available.
format Preprint
id arxiv_https___arxiv_org_abs_2309_14844
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Importance profiles. Visualization of atomic basis set requirements
Lehtola, Susi
Chemical Physics
Computational Physics
Recent developments in fully numerical methods promise interesting opportunities for new, compact atomic orbital (AO) basis sets that maximize the overlap to fully numerical reference wave functions, following the pioneering work of Richardson and coworkers from the early 1960s. Motivated by this technique, we suggest a way to visualize the importance of AO basis functions employing fully numerical wave functions computed at the complete basis set (CBS) limit: the importance of a normalized AO basis function $|α\rangle$ centered on some nucleus can be visualized by projecting $|α\rangle$ on the set of numerically represented occupied orbitals $|ψ_{i}\rangle$ as $I_{0}(α)=\sum_{i}\langleα|ψ_{i}\rangle\langleψ_{i}|α\rangle$. Choosing $α$ to be a continuous parameter describing the orbital basis, such as the exponent of a Gaussian-type orbital (GTO) or Slater-type orbital (STO) basis function, one is then able to visualize the importance of various functions. The proposed visualization $I_{0}(α)$ has the important property $0\leq I_{0}(α)\leq1$ which allows unambiguous interpretation. We also propose a straightforward generalization of the importance profile for polyatomic appliations $I(α)$, in which the importance of a test function $|α\rangle$ is measured as the increase in projection from the atomic minimal basis. We exemplify the methods with importance profiles computed for atoms from the first three rows, and for a set of chemically diverse diatomic molecules. We find that the importance profile offers a way to visualize the atomic basis set requirements for a given system in an a priori manner, provided that a fully numerical reference wave function is available.
title Importance profiles. Visualization of atomic basis set requirements
topic Chemical Physics
Computational Physics
url https://arxiv.org/abs/2309.14844