Diphosphine Ligands in Tungsten Carbonyl Complexes
Organometallics, Vol. 23, No. 22, 2004 5221
1
100.54, and 161.82 MHz, respectively. H chemical shifts are
XP S Sp ectr a . The samples for XPS were prepared by the
spin-coating technique as described elsewhere:13 a few drops
of a solution of the desired complex in CH2Cl2 (0.085 mmol/L)
were placed on the carefully polished surface of a gold foil
(roughness e0.1 µm; 0.5 µm diamond suspension as polishing
medium), and the spin coater was started for 5 min, at a
spinning rate of 3000 rpm, until complete evaporation of the
solvent. The spin coater used was a Model P6708 from
Specialty Coating System Inc. The dependence of the overall
spectrum on several parameters during the sample prepara-
tion (spin speed rate, solution concentration, gold foil rough-
ness) and the necessary characteristics of the support have
already been reported in a previous paper.13 The deposition
of the complexes by this technique was shown to be homoge-
neous enough to minimize the differential charging, leading
to no drifting peaks upon changing of photon flux. The
thickness of the layer was estimated to be around a few
monolayers, but the Au 4f signal from the underlying gold foil
was always detectable and was even more intense than the
W 4f signal. Each sample was introduced into the experimental
chamber through a load-lock chamber; during all measure-
ments, the experimental chamber pressure was not higher
than 2.0 × 10-10 mbar. No evaporation of the complexes from
all the solid-state samples has been observed at room tem-
perature in UHV.
reported relative to tetramethylsilane, 13C chemical shifts are
reported relative to the solvent peak (δ 77.0 for CDCl3), and
31P chemical shifts are reported relative to 85% H3PO4 as
external standard, with downfield shifts taken as positive.
Infrared spectra were recorded in Nujol mulls on a FT-IR
Perkin-Elmer System 2000 spectrometer.
Syn th esis of th e Com plexes. (a) P r epar ation of W(CO)4-
(d p p m ). Tungsten hexacarbonyl (0.52 g, 1.4 mmol) and dppm
(0.54 g, 1.4 mmol) were added into a Schlenk tube containing
5 mL of diglyme. The reaction mixture was heated at reflux
for 75 min, during which time the hexacarbonyl that sublimed
on the Schlenk walls was periodically returned to the solution
by vigorous shaking. The yellow-brown solution obtained was
cooled to room temperature; addition of 5 mL of methanol
caused precipitation of yellow crystals, which were filtered,
washed with methanol, and dried in vacuo. Yield: 71%. 1H
NMR (CDCl3, 25 °C): δ 7.5-7.2 (m, 20H, Ar), 4.89 (t, 2H, CH2,
J HP ) 9.1 Hz); 31P NMR (CDCl3, 25 °C): δ -23.3 (s, J PW 202.2
Hz). 13C NMR (CDCl3, 25 °C): δ 210.3 (m, CO trans P), 202.8
(t, CO trans CO, J CP 7.3 Hz), 136-128 (Ar), 52.2 (t, CH2, J CP
) 14.0 Hz).
(b) P r ep a r a tion of W(CO)4(d p p p ). In a Schlenk tube
containing 5 mL of diglyme, 0.52 g of tungsten hexacarbonyl
(1.4 mmol) and 0.61 g of dppp (1.4 mmol) were added. The
reaction mixture was heated at reflux for 30 min, and then
the resulting yellow-green solution was cooled to room tem-
perature. After addition of 5 mL of methanol a pale yellow
solid was obtained, which was filtered, washed with methanol,
and dried in vacuo. Yield: 77%. 1H NMR (CDCl3, 25 °C): δ
7.5-7.3 (m, 20H, Ar), 2.56 (m, 4H, PCH2), 2.00 (m, 2H, CH2).
31P NMR (CDCl3, 25 °C): δ +0.4 (s, J PW ) 223.0 Hz). 13C NMR
(CDCl3, 25 °C): δ 205.7 (m, CO trans P), 203.1 (t, CO trans
CO, J CP ) 7.4 Hz), 138-128 (Ar), 31.1 (m, PCH2), 20.2 (s, CH2).
The XPS spectra were recorded by the angle-integrated
Omicron EA 125 HR energy analyzer mounted in the experi-
mental chamber of the VUV-photoemission beam line15 at the
Elettra Synchrotron Facility (Trieste-I). The synchrotron
radiation beam was normal incident with respect to the
surface; photoelectrons were collected with the analyzer axis
at 45° to the substrate surface normal. The photon energy was
fixed for all core level spectra at 201.31 eV, which was the
best compromise in order to maximize the photoionization
cross sections for both W 4f and P 2p core levels.16 To ensure
high-energy resolution and to minimize sample decomposition,
the spectra were acquired with a pass energy of 5 eV, and both
beam-line slits were closed at 10 µm each, thus decreasing the
photon flux on the sample. The instrumental resolution was
estimated by a Fermi edge spectrum acquired with the same
setting of the core level spectra. The resulting resolution was
never worse than 0.10 eV, with an estimated photon energy
contribution of ≈45 meV, and the remaining uncertainty was
attributed to the analyzer.
(c) P r ep a r a tion of W(CO)4(d p p b). Tungsten hexacarbo-
nyl (0.52 g, 1.4 mmol) and dppb (0.64 g, 1.4 mmol) were added
into a Schlenk tube containing 5 mL of diglyme. The reaction
mixture was heated at reflux for 35 min, the yellow-brown
solution obtained was cooled to room temperature, and addi-
tion of 5 mL of methanol caused precipitation of light yellow
crystals, which were filtered, washed with methanol, and dried
1
in vacuo. Yield: 81%. H NMR (CDCl3, 25 °C): δ 7.5-7.3 (m,
20H, Ar), 2.6 (bm, 4H, PCH2), 2.0-1.7 (m, 4H, CH2). 31P NMR
(CDCl3, 25 °C): δ 11.3 (s, J PW 230.9 Hz). 13C NMR (CDCl3, 25
°C): δ 205.4 (m, CO trans P), 202.9 (t, CO trans CO, J CP ) 7.4
Hz), 138-128 (Ar), 31.2 (m, PCH2), 23.5 (s, CH2).
XP S Da ta An a lysis. The sum of several (8 ÷ 16) quick,
single-scan spectra (∼85 s/scan), each recorded on a fresh
sample area (∼0.1 mm2), gave a final spectrum with higher
signal/noise ratio and, at the same time, a careful control of
the homogeneity of the compound distribution on the sample.
Spectra were fit with a Gaussian-Lorentzian line shape using
a nonlinear least-squares procedure, modified to allow the
variation of both Gaussian and Lorentzian components for
each doublet of peaks present in the spectrum. For each
sample, the BEs from W 4f and P 2p final spectra were
referenced to the Au 4f7/2 peak at 84.00 eV acquired before
and after the series of single scans, thus eliminating any error
due to fluctuation of photon energy or electron kinetic energy.
The BEs obtained by the fit calculation are given in the present
work with a 95% interval confidence shown in parentheses.
Such interval confidence provides an evaluation only of the
precision of the fit calculation on the basis of its standard
deviation; on the other hand, the reproducibility of the BEs
could be obtained by the comparison of several (not less than
five) samples of different batches of the same compound,
measured during different beam times, and it was within (30
meV.
(d ) P r ep a r a tion of W(CO)4(d m p e). In a Schlenk tube
containing 5 mL of diglyme were added 0.74 g of tungsten
hexacarbonyl (2.0 mmol) and 0.30 g of dmpe (2.0 mmol). The
reaction mixture was heated at 130 °C for 5 h, and then the
resulting yellow solution was cooled to room temperature. Pale
yellow crystals were obtained; precipitation was completed by
addition of pentane. The product was filtered, washed with
methanol, and dried in vacuo. Yield: 46%. 1H NMR (CDCl3,
25 °C): δ 3.64-3.50 (m, 4H, CH2), 1.60 (d, 12H, CH3, J HP
6.5 Hz). 31P NMR (CDCl3, 25 °C): δ 9.0 (s, J PW ) 222.0 Hz).
13C NMR (CDCl3, 25 °C): δ 209.1 (dd, CO trans P, J CPtrans
22.1, J CPcis ) 5.5 Hz), 201.6 (t, CO trans CO, J CP ) 7.4 Hz),
31.8 (m, CH2), 19.1 (d, CH3, J CP ) 25.8 Hz).
(e) P r ep a r a tion of W(CO)4(F -d p p e). Tungsten hexacar-
bonyl (0.35 g, 1.0 mmol) and F-dppe (0.76 g, 1.0 mmol) were
added into a Schlenk tube containing 8 mL of diglyme. The
reaction mixture was heated at reflux for 90 min, the yellow-
brown solution obtained was cooled to room temperature, and
addition of 5 mL of methanol caused precipitation of a light
gray solid, which was filtered, washed with methanol and with
)
)
DF T Ca lcu la tion s. The calculations of core electron BEs
have been performed in terms of the so-called ∆SCF approach,
1
methylene chloride, and dried in vacuo. Yield: 38%. H NMR
(CDCl3, 25 °C): δ 2.94 (m, 4H, CH2). 31P NMR (CDCl3, 25 °C):
δ +17.3 (s, J PW ) 264.4 Hz). 13C NMR data were not obtained
due to low solubility.
(16) Yeh, J . J .; Lindau, I. At. Data Nucl. Data Tables 1985, 32, 1.