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We propose a computational method that drastically simplifies the inclusion of the spin–orbit interaction in density functional theory when implemented over localized basis sets. Our method is based on a well-known procedure for obtaining pseudopotentials from atomic relativistic ab initio calculations and on an on-site approximation for the spin–orbit matrix elements. We have implemented the technique in the SIESTA (Soler J M et al 2002 J. Phys.: Condens. Matter 14 2745–79) code, and show that it provides accurate results for the overall band-structure and splittings of group IV and III–IV semiconductors as well as for 5d metals.
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Fernández-Seivane et al. (2006) studied this question.
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