A R T I C L E S
Fulton et al.
nylrhodium (I) dimer (Strem), dichloro(pentamethylcylcopentadi-
enyl)rhodium (III) dimer (Strem), hexarhodium hexadecacarbonyl
(Strem), and tetrarhodium dodecacarbonyl (Strem) were used as
received. Di-isopropylamine borane (DiPAB), cyclohexylamine borane
(CAB), and dicyclohexylamine borane (DCAB) were synthesized by
addition of the appropriate amine to an equimolar amount of a THF
solution of BH3-THF complex.18 The purity of all amine boranes used
in this study was greater than 99% as determined by 1H and 11B NMR.
Toluene and THF (Aldrich) were distilled from sodium and degassed
prior to use. All reactions were carried out under an inert atmosphere
unless otherwise stated.
The concentration of the precatalyst was varied between 3.5 and 35
mM, and that of the substrate, between 0.02 and 2 M. In a typical
procedure a solution of 20 mg of chloro-(1,5-cyclooctadiene)rhodium
(I) dimer ([Rh(1,5-COD)Cl]2) dissolved in 2 mL of toluene was added
to a solution containing 200 mg of DMAB in 2 mL of toluene under
an atmosphere of 4% H2 in He. The mixed solution inside of a 1.5 cm
diameter × 6 cm long sealed glass vial was taken from the glovebox
and placed in the X-ray beam. A new vial was used for each reaction.
Each vial was placed in a horizontal position to provide a 6 cm path
length for the X-ray beam. The glass sidewall of each vial was pierced
with a 1 mm diameter hole to allow for escape of the H2. To prevent
the ingress of air into the reaction vial the side hole was covered with
a 1 cm2 piece of Kapton film. The first XAFS spectrum was collected
within 3 min of mixing.
amplitude-reduction factor and is usually treated empirically. The fitted
parameters include Ni, the coordination number of the shell for each
type of neighboring atom, Ri, the shell distance, and σ2, the Debye-
i
Waller factor which represents the mean-square variation in Ri due to
both static and thermal disorder. The fitting of the FEFF8 theoretical
standards to the experimental data was accomplished using an analysis
program (FEFFIT).23
In addition to the structural parameters, a single
nonstructural parameter, ∆E0, is varied to correct for the simple estimate
of E0 made by FEFF8.
Various rhodium-containing standard compounds were used to
establish the value of the core-hole factor, S20, and to also better
understand the sensitivity of the XAFS method to the detection of longer
range rhodium atoms. In evaluating these compounds the ø(k) data were
fit to the FEFF8 theoretical standard using the atom positions that were
generated from the published crystallographic data for dichloro-
(pentamethylcylcopentadienyl)rhodium (III) dimer,24 bis(1,5-cyclooc-
tadiene)rhodium (I) trifluoromethanesulfonate, chlorodicarbonylrhodium
(I) dimer,25 Rh4(CO)12,26 Rh6(CO)16,27 chloro(1,5-cyclooctadiene)-
rhodium (I) dimer,28 and for rhodium metal.29 (Schematics of these
structures are given in the insets of Figures 9 and 10.) The complete
fits to these standards are provided in the Supporting Information. When
evaluating the new rhodium cluster, we used a core-hole factor of S02
) 0.89, i.e., the average from the five different solid standards. S20 has
an associated uncertainty of about 15%, and according to eq 2, we see
that this results in an approximate 15% uncertainty in the reported
coordination number.
2.2. XAFS Methods. The rhodium K-edge (23222 eV) XAFS spectra
were collected in transmission mode on the bending magnet beamline
(XOR/PNC, Sector 20) at the Advanced Photon Source, Argonne
National Laboratory. The bending magnet beamline was chosen over
the much higher flux insertion device line to minimize the potential
for beam damage to the rhodium complexes. No evidence of beam
damage was observed during exposure of the rhodium complexes to
the X-rays. Energy calibration was accomplished using the edge energy
of a Rh(0) foil (23222 eV). As a further measure, this rhodium foil
was placed far beyond the sample with an additional transmission
detector (I2) providing internal energy calibration for each sample
spectrum. We collected time series of X-ray absorption near edge
(XANES) spectra while the active catalyst was forming to study their
kinetics. Full extended X-ray absorption fine structure (EXAFS) spectra
were collected when the kinetics were slow or the conversion was
complete in order to capture the most molecular structural information
on the rhodium catalyst. Series of XANES spectra were normalized to
a common edge height.
The EXAFS ø(k) data were weighted by k2 and windowed in the
range 2.0 < k < 17.0 Å-1 using a Hanning window with dk ) 1.0
Å-1. The fits were to both the real and imaginary parts of ø˜(R) in the
region 0.8 < R < 5.0 Å. The quality of fits was evaluated using the
criteria defined in FEFFIT, the automated software for fitting the
structural parameters.
The structure of several Rh4 clusters have been characterized by
single-crystal XRD.26,30 One cluster of particular relevance for this study
is Rh4(CO)12 since the Rh coordination number is very close to that
measured for the rhodium catalyst in this study. Rh4(CO)12 has C3
symmetry with three equivalent rhodium atoms each binding two
terminal CO’s and sharing two bridging CO’s. The fourth apical
rhodium binds to only three terminal CO’s. The rhodium-rhodium
bond distances are only slightly different with rhodium bonds to the
apical rhodium of about 2.675 Å and slightly longer bonds between
the three equivalent rhodium atoms of 2.725 Å.26 The structure is highly
fluxional in solution, which makes it difficult to characterize by NMR.31
In the FEFF8 calculations used in this study, Rh4(CO)12 was used as
the base structure and modified by substituting B and N atoms at the
same terminal and bridging sites modified by realistic Rh-B and Rh-N
distances. Even with this more accurate representation of the rhodium
cluster much simpler FEFF8 structures generated from a single rhodium
atom coordinated with various B, N, or Rh ligands gave nearly identical
fit results showing the invariance of the fitted results with respect to
the starting model.
We used standard methods for the analysis of EXAFS data19 using por-
tions of the UWXAFS program.20 The EXAFS relationship is given by
Fi(k) S20Ni
2
2
i
ø(k) )
e-2k σi e-2R /λ(k) sin(2kRi + δi(k))
(2)
∑
kR2i
i
The EXAFS oscillations, ø(k), were extracted from the experimen-
tally measured absorption coefficient using an automated background
subtraction method (AUTOBK) developed by Newville et al.21 The
In several instances principal component analysis was used to fully
evaluate the reaction rate and to determine the number of chemical
states of the Rh species. In some systems, where only a limited number
wavenumber of the ejected photoelectron is given by
k )
2m (E - E )/p2 with E0 being the absorption edge energy. In eq 2,
x
e
0
(22) Zabinsky, S. I.; Rehr, J. J.; Ankudinov, A.; Albers, R. C.; Eller, M. J. Phys.
ReV. B 1995, 52, 2995.
(23) Newville, M.; Ravel, R.; Haskel, D.; Rehr, J. J.; Stern, E. A.; Yacoby, Y.
Physica B 1995, 208/209, 154.
(24) Chuchill, M. R.; Julis, S. A.; Rotella, F. J. Inorg. Chem. 1977, 16, 1137.
(25) Walz, L.; Scheer, P. Acta Crystallogr., Sect. C 1991, 47, 640.
(26) Farrugia, L. J. J. Cluster Sci. 2000, 11, 39.
(27) Farrar, D. H.; Grachova, E. V.; Lough, A.; Patirana, C.; Poe, A. J.; Tunik,
S. P. J. Chem. Soc., Dalton Trans. 2001, 2015.
(28) Deridder, D. J. A.; Imhoff, P. Acta Crystallogr., Sect. C 1994, 50, 1569.
(29) Singh, H. P. Acta Crystallogr. 1968, A24, 469.
(30) Ricci, J. S.; Koetzle, T. F.; Goodfellow, R. J.; Espinet, P.; Maitlis, P. M.
Inorg. Chem. 1984, 23, 1828.
(31) Cotton, F. A.; Kruczyns, L.; Shapiro, B. L. J. Am. Chem. Soc. 1972, 94,
6191.
Fi(k), δi(k), and λ(k) are the amplitude, phase, and mean-free-path factor,
respectively, that are derived from theoretical standards calculated by
FEFF8.22 The S20 term in the above equation is the core-hole or
(18) Brown, H. C.; Zaidlewicz, M.; Dalvi, P. V.; Narasimhan, S.; Mukho-
padhyay, A. Organometallics 1999, 18, 1305.
(19) Koningsberger, D. C.; Prins, R. X-ray Absorption: Principles, Applications,
Techniques of EXAFS, SEXAFS and XANES; John Wiley & Sons: New
York, 1988.
(20) Stern, E. A.; Newville, M.; Ravel, B.; Yacoby, Y.; Haskel, D. Physica B
1995, 208/209, 117.
(21) Newville, M.; Livins, P.; Yacoby, Y.; Rehr, J. J.; Stern, E. A. Phys. ReV.
B 1993, 47, 14126.
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11938 J. AM. CHEM. SOC. VOL. 129, NO. 39, 2007