Abstract
The ground states of the three‐ and four‐electron systems He2+, He2, and linear symmetric H3, H4+, and H4 are investigated using the linear combinations of Gaussian‐type orbitals (LCGTO) self‐consistent‐field molecular‐orbital (SCF MO) approach. The basis functions are 1s GTO's, not necessarily located at nuclear positions. Optimized, near‐Hartree–Fock (HF) wavefunctions are presented for the isoelectronic H3 and He2+ systems, for which such results were not previously available. They are found to have similar correlation energies. With simpler wavefunctions, E‐vs‐R plots for H3 and He2+ give good bond lengths and shapes of the energy curve. It is found that previous SCF MO studies have not closely approximated the true HF function for He2. The H4+ calculations are the first SCF MO results available for the species, and indicate its instability with respect to H3+ + H, in agreement with recent experimental data. The GTO studies for H4 are the only rigorously executed ab initio calculations yet done for the system. E‐vs‐R data derived for H4 refute the best previous studies, which used integral approximations. The interaction potential of two H2 molecules (end to end) is derived from these H4 energies.

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