L. Marchese et al., Structure-functionality relationships of grafted Ti-MCM41 silicas. Spectroscopic and catalytic studies, PCCP PHYS C, 1(4), 1999, pp. 585-592
Detailed spectroscopic measurements have been used to elucidate the nature
of Ti(IV)-centred active sites that were anchored to a mesoporous silica su
rface (MCM41) by two distinct routes from titanocene precursors. The cataly
st prepared in dry argon (Ti-MCM41 [Ar]) is more active than that prepared
in air (in the presence of water vapour) in its activity in the epoxidation
of cyclohexene with tert-butylhydroperoxide (TBHP). The degree of loading
of the titanium onto the silica support also influences the precise nature
of the active sites. In Ti-MCM41 [Ar] samples containing less that 2 wt.% o
f Ti, the most abundant species are tetrahedrally bonded Ti(IV) active site
s which absorb at 210-230 nm in diffuse reflectance (DR) W-Vis spectra and
exhibit an emission at 430 and 490 nm when excited with a 250 nm light. Sam
ples of catalyst with greater than 4 wt.% loading are shown to contain TiO2
-like microclusters. These species absorb at lambda greater than or equal t
o 250 nm in the DR UV-Vis and emit very weakly in the 500-600 nm region. In
the case of Ti-MCM41 [air] catalysts, which were prepared in the presence
of atmospheric water at the MCM41 surface, even at the lowest Ti loading (e
.g. less than or equal to 0.5%) an incipient formation of oligomers occurs.
It is proposed that dimers or very small oligomers which absorb at around
250 nm in the DR spectra are responsible for a very strong emission at arou
nd 500 nm in the photoluminescence spectra. The abundant presence of these
species might well explain the lower catalytic performance of Ti-MCM41 [air
] in comparison with that of Ti-MCM41 [Ar]. The anchoring of the Ti species
at the surface silanol groups of MCM41 was in all cases followed by FTIR s
pectroscopy.