STO-3G has exponent parameters which can be found in a reference book. Can these parameters be calculated using, for instance, a Hartree–Fock equation for one atom? Or using another way?
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1$\begingroup$ Related prior questions: mattermodeling.stackexchange.com/q/6559/7, mattermodeling.stackexchange.com/q/3728/7 $\endgroup$– Tyberius ♦May 16, 2022 at 12:57
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$\begingroup$ Related question as well: chemistry.stackexchange.com/questions/63560/… $\endgroup$– SFriendlyApr 30 at 5:24
1 Answer
You are right that the STO-nG basis sets are optimized separately for each individual element (as an isolated atom, rather than as an ion or an atom within a bigger molecule). The exponents are obtained by by a least squares fit of the Gaussian orbitals to a single Slater-type orbital (STO).
For other basis sets (not named STO-nG but named something else, like cc-pCVDZ), the exponents are calculated by doing Hartree-Fock and CISD calculations, for example.
If you want to know more about how Gaussian basis sets are optimized, you might find the following thread interesting: Optimization of Gaussian basis sets within the Hartree-Fock Method.
There's also been some discussion about STO-3G specifically and why different sources have different exponent values for STO-3G: Difference between original STO-3G and BSE STO-3G