The spin-flip method
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addresses problems due to small HOMO-LUMO gaps, associated with a single-determinant
description of the wave function. Both closed- and open-shell singlet states are
described within a single reference as spin-flipping, (e.g., ) excitations from the triplet reference state, for which both dynamical
and non-dynamical correlation effects are smaller than for the corresponding
singlet state. This is because the exchange hole, which arises from the Pauli
exclusion between same-spin electrons, partially compensates for the poor
description of the coulomb hole by the mean-field Hartree–Fock model.
Furthermore, because two electrons cannot form a bond, no bond
breaking occurs as the internuclear distance is stretched, and the triplet wave
function remains essentially single-reference in character. The spin-flip
approach has also proved useful in the description of di- and tri-radicals as
well as some problematic doublet states.
The spin-flip method is available for the CIS, CIS(D), CC2, CISD, CISDT, OD, CCSD, EOM-(2,3), and CCSDT levels of theory and the spin complete SF-XCIS (see Section 7.2.3.2). An non-iterative triples corrections are also available—e.g., (dT) and (fT). For the OD and CCSD models, the following non-relaxed properties are also available: dipoles, transition dipoles, SOCs, eigenvalues of the spin-squared operator (), and densities. Analytic gradients are also for SF-CIS and EOM-SF-CCSD methods. Construction of effective Hamiltonians in Heisenberg and Hubbard spaces from EOM-SF wave functions is described in the Section 13.6. To invoke a spin-flip calculation the SF_STATES $rem should be used, along with the associated $rem settings for the chosen level of correlation by using METHOD (recommended) or using older keywords (CORRELATION, and, optionally, EOM_CORR). Note that the high multiplicity triplet or quartet reference states should be used.