Francesco Geobaldo, Giuseppe Spoto, Silvia Bordiga, Carlo Lamberti and Adriano Zecchina
The oligomerization of propene on H-mordenite is the predominant
process proceeding very rapidly already at room temperature. This
process can be conveniently studied by fast FTIR spectroscopy. However
due to the rapid blockage of the pore entrances caused by the growing
chains, it is not possible to obtain a full sequence of spectra
documenting the steps of the oligomerization process involving not
only the catalytic centres at the pore entrances but also those
located in inner positions. In this paper we demonstrate that, by
changing the experimental conditions, i.e. by using
a temperature-programmed FTIR spectroscopy experiment, operating in
the temperature range 100–300 K, the formation of the
hydrogen-bonded precursor (at low temperature) and the successive
oligomerization involving all the protonic centres can be followed
without difficulty. It is demonstrated that under these conditions and
as found in the H-ZSM-5/propene system, the oligomerization proceeds
through three steeps: (i) formation of a short-lived hydrogen-bonded
precursor by interaction of the alkene with both the external and
internal acidic Brønsted sites; (ii) protonation of the
hydrogen-bonded precursor and (iii) propagation of the chain
via insertion of monomers. Although a comparison between
H-ZSM5 and H-mordenite Brønsted acidity (made on the basis of
the downward shifts of ν(OH) and ν(CC) stretching
frequencies in the hydrogen-bonded precursor) shows virtually
identical acidity, the protonation of propene proceeds faster on
H-mordenite. A plausible explanation for this effect is discussed.
While the main oligomerization process discussed so far leads to
saturated chains, the parallel formation of minor amounts of
unsaturated species can elude IR detection. It is demonstrated that
UV–VIS spectroscopy is a very sensitive tool for the detection
of unsaturated cationic species formed via a side reaction
involving hydrogen transfer.