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Z. Wang et al. / Journal of Catalysis 340 (2016) 95–106
of Cu deposition on the TiO2 surface mainly occurs at pH lower
than the PZC of TiO2 (ꢀ6). It starts at the very beginning of the
DPu, since a small amount of copper is already deposited on TiO2
at pH < 3.8 (Fig. 3), i.e., at a pH at which the TiO2 surface is not sup-
posed to interact with cationic complexes such as Cu(H2O)26+ or Cu
(NH3)26+ (Fig. 1). Cationic CuII complexes interaction with titania at
low pH has been already reported by Bourikas et al. in a recent
review on titania [50]. They mentioned that although literature
related to the studies of the deposition of CuII complexes on TiO2
is not very abundant and not recent, there are several papers
reporting the adsorption of CuII aqua complexes on TiO2 surface
at pH of 2 or 4, i.e., below the PZC of titania (ꢀ6) [51,52].
itation in solution (pH 5.2 in the absence of TiO2), and it corre-
sponds to the inflection point of the pH curves in Fig. 4. This
result is consistent with the principle of the method of deposi
tion–precipitation [1–5], in particular, the precipitation of
Cu2(OH)3NO3 onto the titania support, also attested by the fact that
the particles of the copper hydroxynitrate precipitate are much
larger than those formed in the presence of titania. One can
therefore propose that the Cu2+ species already adsorbed on TiO2
at low pH act as nucleation sites for the growth of the precipitate
onto the support rather than into solution, lowering the pH
of precipitation, i.e., lowering the pH of the supersolubility of
Cu2(OH)3NO3aq, and preventing its precipitation into solution.
As the pH of the solution increases during DPu at 80 °C, instead
of reacting with the dissolved support as for silica and forming
copper silicate [56] since TiO2 is not known to dissolve in the 3–
8 pH range, Cu2(OH)3NO3 gradually transforms into CuO; this is
accompanied by a change of the suspension color from green to
gray. The evolution of the nature of the Cu compound on TiO2 is
also attested by the different colors taken by the as-prepared sam-
ples as a function of the Cu loading (Fig. 2) and the DPu duration
(Table 2). The green color of the samples with less than 1.6 wt%
Cu is due to the presence of stable Cu2(OH)3NO3 and the more
grayish color observed for the higher Cu loadings is related to the
additional presence of CuO. The formation of CuO is attested by
XRD (Fig. 5) and by the presence of the broadband at 450–
800 nm in the UV–visible spectra (Fig. 6a). However, Cu2(OH)3NO3
is more stable on titania than in the absence of support since the
Cu/TiO2 suspension (<3 wt% Cu) remains green after 5 h of DPu
whereas it turns blackish without support (Table 1). The grayish
color taken by the sample during DPu when more Cu is deposited
(4.24 wt% Cu) (Table 1) or when DPu duration increases (Fig. 2 and
Table 2), which is due to the presence of large particles of CuO, can
be explained as follows. It probably initially results from a phe-
nomenon of Ostwald ripening of the Cu2(OH)3NO3 particles during
DPu as the particle size of metallic Cu increases with DPu time
(Fig. 5b). In addition, very small Cu0 particles were also observed
by TEM (Fig. 8). These results may therefore indicate that Ostwald
ripening has occurred during sample preparation by DPu, produc-
ing a bimodal size distribution. Moreover, as the Cu2(OH)3NO3 par-
ticles increase in size, they become instable and transform into
CuO that continue to grow. It is interesting to note that at variance
with the silica and alumina supports (see Section 1), no mixed
compound, i.e., no copper titanate formation was detected. Sankar
et al. [57] showed that in the case of a parent system, Ni/TiO2,
NiTiO3 was detected by EXAFS after calcination but at temperature
higher than 600 °C and only when the samples were prepared by
impregnation (not by cation adsorption).
The titania P25 used in this study contains two phases, anatase,
the main one, and rutile. In these two different crystal structures,
each Ti4+ ion is surrounded by six oxygen forming octahedral enti-
ties (TiO6), and each oxygen is bonded to three Ti4+ ions (Ti3–O) by
two short Ti–O bonds (1.946 Å in rutile, and 1.937 Å in anatase)
and one longer (1.984 Å in rutile and 1.964 Å in anatase) [53]. Sur-
face Ti4+ ions have lower coordination than in the bulk, and the
surface of TiO2 possesses in principle three types of surface oxy-
gens, namely singly coordinated surface oxygen (TiO), doubly coor-
dinated one (Ti2O) and triply coordinated one (Ti3O). On the basis
of different surface ionization models for these surface sites, Bour-
ikas et al. [54] proposed a derived model of protonation reactions
for TiO and Ti2O that they consider more realistic than those in
the former models:
K1
TiOꢂ0:35 þ Hþ () TiOHþ0:65 logK1 ¼ 7:8
ð4Þ
ð5Þ
K2
Ti2Oꢂ0:57 þ Hþ () Ti2OHþ0:43 logK2 ¼ 4:6
Note that the oxygen of Ti3O is not protonated (logK3 = ꢂ3.96)
[55] and that the TiO sites are negatively charged (TiOꢂ0.35
,
Eq. (4)) even at pH lower than 3, based on experimental results
of Bourikas et al. [54].
We can therefore propose that at the very beginning of the DPu
preparation, i.e., at pH < 4 before precipitation starts (Fig. 3), part of
the Cu2+ complexes in solution can interact electrostatically with
the TiOꢂ0.35 sites of TiO2 surface and then could form Ti–O–Cu spe-
cies according to [52]. The formation of inner sphere complexes is
attested by the presence of the band at 420 nm in the UV–visible
spectra of the wet Cu/TiO2 samples (Fig. 6b). At the stage of the
present study, it is not possible to discard another hypothesis as
the one proposed by Petala et al. [41], which is a direct surface
reaction between Cu2+ complexes and surface OHs of titania that
would also lead to the formation of inner sphere complexes. It is
interesting to mention that titania behaves differently from silica
support. In a former study of one of us [28], dealing with adsorp-
tion of [Cu(NH3)4(H2O)2]2+ complexes on silica, the formation of
Si–O–Cu bonding was observed only after the sample has been
dried at RT and not when it was still wet. In any case, one can pro-
pose that once CuII complexes have interacted with the negatively
charged sites of TiO2 or some surface OHs or when pH has reached
4, the remaining of the Cu complexes in solution start precipitating
on titania. The nature of the Cu precipitate is probably the same as
the one obtained in the absence of support (Experiment B2 in Sec-
tion 3.1.2), i.e., copper hydroxynitrate (Cu2(OH)3NO3) and not cop-
per hydroxide. In spite of the fact that the diffractogram of as-
prepared Cu/TiO2 (Fig. 5a) does not show the corresponding
diffraction peaks, this hypothesis is consistent with the fact that
the samples have the same green color in the presence or in the
absence of TiO2, that their UV–visible and IR spectra are similar
(Figs. 6 and S1) and that Cu2(OH)3NO3 has been identified previ-
ously in Cu/SiO2 samples prepared by DPu [56]. Moreover, the
pH ꢀ 4 of Cu precipitation in the presence of TiO2, associated with
the color change of the suspension is lower than the pH of precip-
From this discussion, one can now propose an interpretation for
the TPR profiles (Fig. 7). The first TPR peak can be attributed to the
reduction of small NPs of Cu2(OH)3NO3 while the second one at
higher temperature can be attributed to the reduction of large
NPs of CuO; this peak becomes predominant as the Cu loading
increases.
The number of Cu nucleation sites is limited; thus, when the Cu
loading increases, the particles of Cu2(OH)3NO3 grow on these
sites, and increase in size. When the Cu concentration is high
enough (>1.6 wt%), Cu2(OH)3NO3 becomes instable and transforms
into CuO that also increases in size. These results are consistent
with the different metal particle sizes obtained after reduction at
350 °C, i.e., a progressive increase of the particle size and broaden-
ing size distribution with the Cu loading (Fig. 8). One can conclude
that the various particle size ranges observed by TEM are caused by
the different Cu loadings and Cu species present on TiO2 in the as-
prepared samples and also to Ostwald ripening.
The catalytic results can now be discussed in the light of these
characterization results. Fig. 10 shows that the sample containing