S. Otto, A. Roodt / Inorganica Chimica Acta 357 (2004) 1–10
9
At first though it might seem like the m(CORh) values
Acknowledgements
for both the As and the Sb complexes suggest that the
Rh metal centre should be more electron rich (lower
m(CORh) values). However, it is clear that the Rh–Cl
bond distance for these complexes significantly shortens,
Financial assistance from the South African NRF
and the research funds of the University of the Free
State, the Rand Afrikaans University, SIDA (Swedish
International Cooperation Development Agency) is
gratefully acknowledged. Lund University and the
University of the Witwatersrand are acknowledged for
the use of their diffractometers.
ꢀ
see Table 5 (2.382(1), 2.354(2) and 2.315(3) A) for the
PPh3, AsPh3 and SbPh3 complexes, respectively. Thus it
seems as if the electron density on the Rh metal centre
decreases significantly from PPh3 to AsPh3 to SbPh3.
However, it cannot be excluded that this observation
might be due to steric effects.
It is thus suggested that the decrease in electron
density on the metal centres is a combined result of the
longer Rh–L bond distances and the corresponding
smaller steric demands of the SbPh3 versus AsPh3 versus
PPh3 ligands, which is in fact manifested by stronger M–
Cl bonds. The increased apparent higher electron den-
sity of the complexes, based on the m(CORh) values, is
thus in the order PPh3 > AsPh3 > SbPh3. The impor-
tance of the smaller steric demand is further manifested
in the fact that five-coordinate complexes for the Sb
system form with relative ease [23]. As in all experi-
mental measurements it has to be remembered that, as
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A clear trend was illustrated between the stretching
frequencies of the Rh and Ni complexes. The rhodium
Vaska-type complexes were then used in a similar fashion
as the [NiL(CO)3] complexes to establish the electronic
parameters of various ligands, as an example the elec-
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