Quantify the sources of large ZFS errors for Sc, Y, and La
Determine and quantify the sources of the large errors observed when predicting the zero-field splitting in the 2D ground term of Sc, Y, and La using the BP2-QDNEVPT2 and DKH2-QDNEVPT2 methods, explicitly assessing the contributions of high-order dynamic correlation effects (such as triple and higher excitations outside the active space) and their interplay with spin–orbit coupling, as suggested by the performance of variational X2C-MRCISD for Sc and La.
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Although we cannot quantify the source of these errors, the poor performance of variational X2C-MRCISD method for Sc and La suggests that they are at least in part due to high-order dynamic correlation effects, such as triple (and higher) excitations in non-active orbitals, and their interplay with spin--orbit coupling.