STO-nG basis sets
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STO-nG basis sets are minimal basis sets used in computational chemistry, more specifically in ab initio quantum chemistry methods, to calculate the molecular orbitals of chemical systems within Hartree-Fock theory or density functional theory. The basis functions are linear combinations of n {\displaystyle n} primitive Gaussian-type orbitals (GTOs) that are fitted to single Slater-type orbitals (STOs). They were first proposed by John Pople and n {\displaystyle n} originally took the values 2 – 6. A minimal basis set is where only sufficient orbitals are used to contain all the electrons in the neutral atom. Thus, for the hydrogen atom, only a single 1s orbital is needed, while for a carbon atom, 1s, 2s and three 2p orbitals are needed.
General definition
STO-n {\displaystyle n}G basis sets consist of one STO for each orbital in the neutral atom (with suitable parameter ζ {\displaystyle \zeta }) for each atom in the system to be described (e.g. molecule). The STOs assigned to a particular atom are centered around its nucleus. Therefore, the number of basis functions for each atom depends on its type. The STO-n {\displaystyle n}G basis sets are available for all atoms from hydrogen up to xenon.
| element | number of STOs | STOs |
|---|---|---|
| H, He | 1 | 1s |
| Li, Be | 2 | 1s, 2s |
| B, C, N, O, F, Ne | 5 | 1s, 2s, 2p |
| Na, Mg | 6 | 1s, 2s, 2p, 3s |
| Al, Si, P, S, Cl, Ar | 9 | 1s, 2s, 2p, 3s, 3p |
| K, Ca | 10 | 1s, 2s, 2p, 3s, 3p, 4s |
| Sc-Zn | 15 | 1s, 2s, 2p, 3s, 3p, 4s, 3d |
| Ga-Kr | 18 | 1s, 2s, 2p, 3s, 3p, 4s, 3d, 4p |
| Rb, Sr | 19 | 1s, 2s, 2p, 3s, 3p, 4s, 3d, 4p, 5s |
| Y-Cd | 24 | 1s, 2s, 2p, 3s, 3p, 4s, 3d, 4p, 5s, 4d |
| In-Xe | 27 | 1s, 2s, 2p, 3s, 3p, 4s, 3d, 4p, 5s, 4d, 5p |
Each STO (both core and valence orbitals) ψ m l {\displaystyle \psi _{ml}}, where m {\displaystyle m} is the principal quantum number and l {\displaystyle l} is the angular momentum quantum number, is approximated by a linear combination of n {\displaystyle n} primitive GTOs ϕ l α m j {\displaystyle \phi _{l\alpha _{mj}}} with exponents α m j {\displaystyle \alpha _{mj}}:
ψ m l STO − n G = ∑ j = 1 n c m l j ϕ l α j . {\displaystyle \psi _{ml}^{{\text{STO}}-n{\text{G}}}=\sum _{j=1}^{n}c_{mlj}\phi _{l\alpha _{j}}.}
The expansion coefficients c m l j {\displaystyle c_{mlj}} and exponents α m j {\displaystyle \alpha _{mj}} are fitted with the least squares method (this differs from the more common procedure, where they are chosen to give the lowest energy) to all STOs within the same shell m {\displaystyle m} simultaneously. Note that all ψ m l STO − n G {\displaystyle \psi _{ml}^{{\text{STO}}-n{\text{G}}}} within the same shell m {\displaystyle m} (e.g. 2s and 2p) share the same exponents, i.e. they do not depend on the angular momentum, which is a special feature of this basis set and allows more efficient computation.
The fit between the GTOs and the STOs is often reasonable, except near to the nucleus: STOs have a cusp at the nucleus, while GTOs are flat in that region. Extensive tables of parameters have been calculated for STO-1G through STO-6G for s orbitals through g orbitals and can be downloaded from the Basis Set Exchange.
STO-2G basis set
The STO-2G basis set is a linear combination of 2 primitive Gaussian functions. The original coefficients and exponents for first-row and second-row atoms are given as follows (for ζ = 1 {\displaystyle \zeta =1}).
| STO-2G | α1 | c1 | α2 | c2 |
| 1s | 0.151623 | 0.678914 | 0.851819 | 0.430129 |
| 2s | 0.0974545 | 0.963782 | 0.384244 | 0.0494718 |
| 2p | 0.0974545 | 0.61282 | 0.384244 | 0.511541 |
For general values of ζ {\displaystyle \zeta }, one can use the scaling law ψ m l ζ ( r ) = ζ 3 / 2 ψ m l 1 ( ζ r ) {\displaystyle \psi _{ml}^{\zeta }(\mathbf {r} )=\zeta ^{3/2}\psi _{ml}^{1}(\zeta \mathbf {r} )} to approximate general STOs with ζ ≠ 1 {\displaystyle \zeta \neq 1}.
STO-3G basis set
The STO-3G basis set is the most commonly used among the STO-n {\displaystyle n}G basis sets and is a linear combination of 3 primitive Gaussian functions. The coefficients and exponents for first-row and second-row atoms are given as follows (for ζ = 1 {\displaystyle \zeta =1}).
| STO-3G | α1 | c1 | α2 | c2 | α3 | c3 |
| 1s | 2.22766 | 0.154329 | 0.405771 | 0.535328 | 0.109818 | 0.444635 |
| 2s | 0.994203 | -0.0999672 | 0.231031 | 0.399515 | 0.0751386 | 0.700115 |
| 2p | 0.994203 | 0.155916 | 0.231031 | 0.607684 | 0.0751386 | 0.391957 |
Accuracy
The exact energy of the 1s electron of H atom is −0.5 hartree, given by a single Slater-type orbital with exponent 1.0. The following table illustrates the increase in accuracy as the number of primitive Gaussian functions increases from 3 to 6 in the basis set.
| Basis set | Energy [hartree] |
| STO-3G | −0.49491 |
| STO-4G | −0.49848 |
| STO-5G | −0.49951 |
| STO-6G | −0.49983 |
Use of STO- n G basis sets
The most widely used basis set of this group is STO-3G, which is used for large systems and for preliminary geometry determinations. However, they are not suited for accurate ab-initio calculations due to their lack of flexibility in radial direction. For such tasks, larger basis sets are needed, such as the Pople basis sets.