2005
DOI: 10.1021/jp055884t
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Electronic Structure and Molecular Properties of the Heptacyanorhenate [Re(CN)7]3- and [Re(CN)7]4- Complexes

Abstract: We report scalar relativistic and Dirac scattered wave (DSW) calculations on the heptacyanorhenate [Re(CN)7](3-) and Re(CN)7(4-) complexes. Both the ground and lowest excited states of each complex split by spin-orbit interaction by about 0.3 eV. The calculated molecular electronegativities chi indicate that the open-shell complex is less reactive than the closed-shell complex, in agreement with experimental observations. The calculations indicate that the ground state spin density is highly anisotropic and th… Show more

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Cited by 10 publications
(7 citation statements)
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“…26 For the Re IV homologue, g ⊥ = 1.759 and g ‖ = 3.66 have been found. 27,28 Somewhat less anisotropic g was observed for a PBP W III derivative with mixed carbonyl/cyanide ligand set, cis -[W(CN) 5 (CO) 2 ] 2− , but EPR was recorded in solution. 29…”
Section: Transition Metal Ions With a Pentagonal Bipyramidal Coordina...mentioning
confidence: 99%
“…26 For the Re IV homologue, g ⊥ = 1.759 and g ‖ = 3.66 have been found. 27,28 Somewhat less anisotropic g was observed for a PBP W III derivative with mixed carbonyl/cyanide ligand set, cis -[W(CN) 5 (CO) 2 ] 2− , but EPR was recorded in solution. 29…”
Section: Transition Metal Ions With a Pentagonal Bipyramidal Coordina...mentioning
confidence: 99%
“…Due to a very strong ligand field, all orbitally degenerate 4d and 5d complexes have a low spin of S = 1 / 2 with no ZFS effect, requiring S > 1 / 2 . Examples are given by [Mo III (CN) 7 ] 4– and [Re IV (CN) 7 ] 3– pentagonal-bipyramidal complexes, [Ru III (CN) 6 ] 3– and [Os III (CN) 6 ] 3– octahedral complexes, and some trigonal-pyramidal Mo and W complexes . It is important to note that isolated complexes of this type cannot exhibit single-ion magnet behavior due to the absence of the ZFS anisotropy for the S = 1 / 2 spin.…”
Section: Introductionmentioning
confidence: 99%
“…Also, spin‐orbit effects are responsible for the magnetic anisotropy of the [Re(CN) 7 ] 3− complex. Consequently, the incorporation of relativistic corrections are essential for a good description of optical electronic transitions …”
Section: Theoretical Backgroundmentioning
confidence: 99%