M.H. Herbst, G.H.M. Dias / Journal of Physics and Chemistry of Solids 64 (2003) 2423–2428
2425
severe in comparison with their high platinum content
analogues.
the fullerene molecule, until here treated as a mere support,
a further experiment was carried out. The infrared spectra of
the samples exposed to CO were measured in the range from
Analysis of the solid residues after heating at 600 8C of
all four compounds by X-ray powder diffraction showed that
only metallic platinum was formed. It is worth of mention
that the conditions employed in the TGA experiments (air
flow 10 ml/min, heating rate 5 8C/min) afford data that are
unable to ascribe to different contents of CO, and that
fullerene solids deposited onto cool parts of the thermo-
balance were not detected.
2
1
2500 to 400 cm . It was noted after CO exposure that the
spectra of the platinum-fullerene compounds displayed in
addition to the usual strong carbonyl bands a weak
2
1
absorption at 476 cm
assigned to a Pt–CO vibration
mode [12]. Other four sharp and intense absorption bands,
2
1
observed at 526, 577, 1182 and 1428 cm , are character-
istic of the uncoordinated fullerene molecule. All these new
bands are superimposed on the spectra of the platinum-
fullerene compounds, suggesting that the fullerene mol-
ecules were partially displaced from the platinum coordi-
nation. The spectra of the platinum-fullerene compounds
and of the carbonylated products are shown in Fig. 1.
It should be mentioned that the same behavior was
observed in the presence of solvent. When a suspension of
Complementary studies were carried out to investigate
the stability and the reversibility of the interactions of these
novel platinum-fullerene compounds with carbon monox-
ide. Although the compounds have been maintained under
reduced pressure for 15 h, no noticeable change was
observed in the infrared spectra. This result also confirms
the carbon monoxide chemisorption over ½Pt C ; with the
n
60
formation of relatively stable carbonyl species, instead of a
mere physical adsorption. Nevertheless, the products were
heated at 373 K under vacuum for about 5 h in another
experiment with the loss of bridging carbonyls and an
absorption band shift of the remaining terminal carbonyl
½
Pt C in toluene is treated with a gentle carbon monoxide
n
60
stream, a magenta solution is formed in a few minutes. After
solvent removal under vacuum at low temperature, a
brownish solid is recovered. The infrared spectra of this
solid either in KBr pellet or in CH Cl solution show
2
2
1
2
from 2064 to 2059 cm . The small shift of the latter band
when compared to the non-treated sample can be attributed
to a decrease in the concentration of chemisorbed terminal
CO molecules, in terms of a lower dipolar interaction among
chemisorbed adjacent CO molecules. The reversibility of
the CO chemisorption was also tested by submitting the
heated pellets to 1 bar of carbon monoxide pressure for 1 h,
absorption bands in the CO stretching region, at 2058, 2016
21
and 1978 cm . However, the solid decomposes rapidly
under normal conditions, and the infrared absorption bands
are no longer observed.
As mentioned earlier, platinum-fullerene compounds
under ordinary CO pressures behave distinctively with the
platinum content. In order to verify this behavior, high-
pressure experiments were performed by submitting the
compounds to carbon monoxide pressures from 3 to 25 bar.
Whereas a nominal pressure of 3 bar increased only the
intensities of the absorption bands, the pressure of 25 bar
2
1
but only the 2059 cm band was observed without
significant changes in intensity.
It is interesting to note that similar results were reported
in the literature, particularly in investigations on oxide-
supported platinum [9]. Moreover, it was also observed that
the nature of the support has strong influence on the
stretching frequency of metallic carbonyls. Generally, the
higher the acidity of the support, the higher the stretching
frequencies of the chemisorbed carbon monoxide [10]. This
effect is commonly explained by the electronic density
donation from the metal to the support. In terms of HOMO
and LUMO frontier orbitals in the MO approach, the
electronic states of the surfaces near the Fermi level in solid
materials are equivalent to the HOMO. The synergistic
effects of CO chemisorption manifest themselves in a
lowering of the CO bonding stretching frequency, due to the
favoring of the p back-donation from the filled metal d
2
1
induced new bands at 2013 and 1989 cm in the infrared
spectra. A substantial increase in the intensity of the whole
spectrum was also noted, as shown in Fig. 2.
The absorption bands related to the infrared spectrum of
pure C60 shown in Fig. 2 have their intensities enhanced
with an increase in the carbon monoxide pressure,
suggesting that the pressure promotes the removal of
fullerene molecules from the platinum coordination. One
can argue that under these conditions there is formation of
½
ðCOÞ Pt species mixed with ½Pt C compounds,
x
m
n2m 60
where n is the original platinum fullerene ratio, m is the
amount of platinum excluded from fullerene coordination
and x denotes the nuclearity of the carbonyl species.
p
orbitals to the empty 2p molecular orbitals of carbon
monoxide.
Concerning the stability of the carbonyl species formed
under high-pressure conditions, a desorption test was
conducted by maintaining the samples overnight under
vacuum. Since no noticeable change was observed in the
infrared spectra, the result reinforced the previous con-
clusion about a relative high stability for the carbonyl
species. However, there was a shift of the band assigned to
the terminal carbonyl species formed at a pressure of 25 bar
Concerning the influence of the nature of the support in
the stretching frequency of the CO vibration, fullerenes
behave like an electron deficient polyolefin with p-acid
characteristics [11]. Therefore, some competition is
expected between C60 and CO for the electronic density at
the platinum atom, as was indeed suggested by the strong
shift in the CO stretching frequency from the free CO and
the chemisorbed species. In order to investigate the role of
2
1
from 2064 to 2052 cm , and the absence of the bands at