C O M M U N I C A T I O N S
To understand the lack of CO addition to (cymene)Ru[η3-
HC(PPh2NPh)2]+ versus the facile reaction with the uncharged Cp*
analogue, we have optimized the structures of the cationic cymene
reactant and product. Comparison of the Cp* and cymene species,
(ring)Ru[η3-HC(PPh2NPh)2], shows no dramatic geometric differ-
ences (i.e., flaws) in the cymene species, although metal-ligand
bond lengths are about 0.08 Å shorter than those in the cymene
complex. However, while the reaction energy for the Cp* case is
-29.8 kcal/mol, it is only -8.8 kcal/mol for the cymene case. Since
the T*∆S term is about +8 kcal/mol at 298 K, together with a +4
kcal/mol term for the low [CO], CO addition is calculated to be
unfavorable for the cymene case, in agreement with observation.
The difference is thus thermodynamic in origin and must be
attributed to the weaker π basicity of the cationic species toward
the arriving CO ligand. Support for this hypothesis comes from
the calculated C/O stretching frequency for the Cp* adduct (1898
cm-1) versus the that for the (unobserved) cymene analogue (1967
cm-1).
Figure 2. DFT-optimized geometry of (a) doubly N-bound ligand isomer
and (b) the isomeric structure with one N and C(sp3), together with C(ortho)
and C(ipso) of one phenyl, bonded to Ru. In general, only the ipso phenyl
carbons are illustrated, except for one phenyl on P in b.
minimum only 9.3 kcal/mol higher than the ground state (Figure
2b). The implied weakness of one N-Ru bond in the ground state
was traced to structural features of the pendant PPh2NPh arm of
the ligand; it rotated during geometry optimization from being
nonbonding to Ru to a position where one phenyl ring from
phosphorus donates to the metal,13-16 thus compensating partly for
the N f Ru bond dissociation energy cost, and thereby stabilizing
this transient isomer. The C(ipso)-C(ortho) part of one phenyl
π-system donates to Ru (Ru-C(ipso) ) 2.48 Å, Ru-C(ortho) )
2.46 Å), compared to Ru-C(C5Me5) distances of 2.22 Å. Other
Ru-C distances to this phenyl are >3 Å. As a result, this C-C
distance is 0.03 Å longer than the other five C-C distances in that
phenyl ring. This phenyl donation occurs by deforming one HC-
(sp3)-P-C(ipso) angle 3° smaller than the other one on that P.
We suggest that this less stable isomer17 is thermally accessible
and thus of potential kinetic significance as the key to understanding
the facile CO addition to an 18-electron species (Figure 1).
Subsequent displacement of the aryl f Ru interaction in Figure
2b by CO is clearly favorable based on relative π acidity of phenyl
versus CO, disruption of aromaticity in the reactant, and relief of
steric congestion. Note particularly that the proposed intermediacy
of this isomer naturally accounts for the stereoselectivity of the
product, which has Cp* trans to the pendant PPh2NPh, provided
CO attacks on the side of the phenyl syn to Ru.
The broader implication of this result is that the many large
substituents in HC(PPh2NPh)2 not only create a crowded molecule,
but these phenyls can provide transient stabilization to “quasi-
unsaturated” intermediates,18 and thus play an active role in the
electronic structure of such intermediates: electronic factors
supplement steric factors. This ligand class is thus susceptible to
special substituent effects, as has already been demonstrated19 for
HC(PPh2NSiMe3)2-1. Moreover, in contrast to the usual concept
of the chelate effect keeping a ligand attached to a metal, here it
is the low energy (i.e., accessibility) of arm-off or alternative binding
modes that is the strength of this ligand class for promoting facile
ligand addition.
Acknowledgment. This work was supported by the Department
of Energy. We thank the Russian Academy of Sciences Joint
Supercomputer Center for computing time.
Supporting Information Available: CIF files and bond lengths
and angles for two X-ray structures, together with full details, and
Cartesian coordinates, and drawings of the DFT-optimized structures.
This material is available free of charge via the Internet at http://
pubs.acs.org.
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