1997
DOI: 10.1007/s002140050181
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Spin–orbit corrections to the indirect nuclear spin–spin coupling constants in XH

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Cited by 20 publications
(43 citation statements)
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“…In contrast, no such limitation is present for any of the shielding corrections 10,11,19 or the third-order coupling corrections. 12 For couplings between light ligand nuclei in the presence of heavy elements, the second-order coupling corrections are also expected to be well-behaved.…”
Section: So-ii K Lmentioning
confidence: 93%
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“…In contrast, no such limitation is present for any of the shielding corrections 10,11,19 or the third-order coupling corrections. 12 For couplings between light ligand nuclei in the presence of heavy elements, the second-order coupling corrections are also expected to be well-behaved.…”
Section: So-ii K Lmentioning
confidence: 93%
“…The third-order contributions arising from the field-free SO Hamiltonian are, neglecting terms involving three simultaneous triplet perturbations as rationalized by Kirpekar et al 12 :…”
Section: Third-order So Correctionsmentioning
confidence: 98%
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“…13,14 The relativistic effects can be interpreted by applying perturbation theory; 15 for example, the effects caused by the interplay between the Fermi-contact (FC) interaction of nucleus K with the spinorbit (SO) interaction generated by the magnetic moment of nucleus L can be analyzed. [16][17][18] On the other hand, to include most of the relevant one-and two-electron relativistic corrections into the calculation of indirect spin-spin coupling constants in a more systematic way, it is convenient to start from two-component [19][20][21] or four-component [22][23][24][25] relativistic Hamiltonians. In this way, both scalar and spin-orbit relativistic corrections are included into the wave function variationally and thus relativistic effects to arbitrary order are accounted for.…”
Section: Introductionmentioning
confidence: 99%