-
附
录
UV Raman
Spectroscopic Study on TiO
2
.
I. Phase Transformation at the
Surface
and in the Bulk
Jing Zhang,
Meijun Li, Zhaochi Feng, Jun Chen, and Can
Li*
State
Key
Laboratory
of
Catalysis,
Dalian
Institute
of
Chemical
Physics,
Chinese
Academy of
Sciences,
P
. O.
Box 110, Dalian 116023, China
Recei
V
ed:
September 16, 2005; In Final Form:
No
V
ember 4, 2005
Phase
transformation
of
TiO
2
from
anatase
to
rutile
is
studied
by
UV
Raman
spectroscopy excited by 325and 244 nm
lasers, visible Raman spectroscopy excited by
532 nm laser,
X
-
ray diffraction (XRD),
andtransmission electron microscopy (TEM).
UV Raman spectroscopy is found to be
more sensitive to the surfaceregion of TiO2
than visible Raman spectroscopy and XRD
because TiO
2
strongly
absorbs UV light.
Theanatase phase is
detected by UV Raman spectroscopy for the sample
calcined at
higher temperatures
thanwhen it is detected by visible Raman
spectroscopy and XRD.
The
inconsistency
in
the
results
from
the
abovethree
techniques
suggests
that
the
anatase
phase of TiO
2
at the surface
region can remain at relatively highercalcination
temperatures than that in the bulk
during the phase transformation. The TEM results
show
thatsmall
particles
agglomerate
into
big
particles
when
the
TiO
2
sample
is
calcined at elevated temperatures
andthe agglomeration of the TiO
2
particles is along
with the
phase transformation from anatase to rutile. It is
suggested that the rutile phase
starts
to form at the interfaces between the anatase
particles in the agglomerated
TiO
2
particles;
namely,
the
anatase
phase
in
the
inner
region
of
the
agglomerated
TiO
2
particles turns out to
change into the rutile phase more
easily than that in the outer
surface
region of the agglomerated
TiO
2
the anatase particles
of TiO
2
are
covered with highly dispersed
La
2
O
3
,
the phase transformation in both the bulk and
surface regions is significantly
retarded, owing to avoiding direct contact of the
anatase
particles and occupying the
surface defect sites of the anatase particles by L
a
2
O
3
.<
/p>
1. Introduction
Titania (TiO
2
)
has been widely studied because of its
uniqueoptical and chemical
properties
in catalysis,
[1]
photocatalys
is,
[2]
sensitivity to
humidity and gas,
[3,4]
nonlinear
optics,
[5]
photoluminescence,
[6]
an
d
so
on.
The
two
main
kinds
of
crystalline
TiO
2,
anatase
and
rutile,
exhibit
different
physical
and
chemicalproperties.
It
is
well
-
known
that
the
anatase
phase
is
suitablefor
catalysts
and
supports,
[7]
while
the
rutile
phase is used for
optical and
electronic purposes because of its high dielectric
constant and high refractive
index.
[8]
It has been well
demonstrated
that the crystalline
phase
of
TiO
2
plays
a
significant
role
in
catalytic
reactions,
especially
photocatalysis.
[9
-
11]
Some studies
have
claimed that the anatase phase was more active
than the rutile phase in
photocatalysis.
[9,10]
Although
at
ambient
pressure
and
temperature
the
rutile
phase
is
more
thermodynamically stable than the
anatase phase,
[12]
anatase is
the common phase rather
than rutile
because anatase is kinetically stable in
nanocrystalline TiO
2
at
relatively low
temperatures.
[13]
It is believed that the anatase phase transforms
to the rutile phase over
a
wide
range
of
temperatures.
[14]
The
refore,
understanding
and
controlling
of
the
crystalline phase and
the process of phase transformation of
TiO
2
are important, though
they are difficult.
Many
studies
[13
p>
-
31]
have
been
done
to
understand
the
process
of
the
phase
transformation
of
TiO
2
.
Zhang
et
al.
[15]
proposed
that
the
mechanism
of
the
anatase
-
rutile
phase
transformation
was
temperature
-<
/p>
dependent
according
to
the
kinetic
data from X
-
ray diffraction
(XRD). On the basis of transmission and scanning
electron
microscopies,
Gouma
et
al.
[16]
suggested
that
rutile
nuclei
formed
on
the
surface of coarser anatase particles
and the newly transformed rutile
particles grew at
the expense of
neighboring anatase particles. Penn et
al.
[17]
suggested that the
formation
of rutile nuclei at twin
interfaces of anatase particles heated
hydrothermally.
Catalytic performance of
TiO
2
largely depends on the
surface properties, especially
the
surface phase, because catalytic
reaction takes place on the surface.
The surface
phase of TiO
2
should be responsible for its
photocatalytic activity because not
only the photoinduced reactions take
place on the surface
[32]
but
also the photoexcited
electrons and
holes might migrate through
the surface
region. Therefore, the surface
phase
of
TiO
2
,
which
is
exposed
to
the
light
source,
should
play
a
crucial
role
in
photocatalysis.
However,
the
surface
phase
of
TiO
2
,
particularly
during
the
phase
transformation, has not been
investigated. The challenging questions still
remain: is the
phase in the surface
region the same as that in the bulk region, or how
does the phase in
the surface region of
TiO
2
particle change during
the phase transformation of its bulk?
The difficulty in answering
the above questions
was
mainly due to lacking suitable
techniques that can sensitively detect
the surface phase of
TiO
2
.
UV Raman
spectroscopy is found to be more sensitive to
the surface phase of a
solid
sample when the sample absorbs
UV
light.
[33]
We studied the
phase transition of
zirconia
(ZrO
2
) from tetragonal phase
to monoclinic phase by UV Raman spectroscopy,
visible
Raman
spectroscopy,
and
XRD.
[33]
These
results
clearly
indicated
that
the
surface
phase of ZrO
2
is usually
different from the bulk phase of
ZrO
2
and the phase
transforma
-
tion
of ZrO
2
starts from its
surface region and then gradually develops into
its bulk when the
ZrO
2
with tetragonal phase
is calcined at elevated temperatures.
These findings lead us to further
investigate the phase transformation in the
surface
region of
TiO
2
by UV Raman
spectroscopy as TiO
2
also
strongly absorbs UV light. In
this
study, we compared the Raman spectra of
TiO
2
calcined at different
temperatures
with excitation lines in
the UV and visible
regions. XRD and
transmission electron
microscopy
(TEM)
were
also
recorded
to
understand
the
process
of
phase
transformation of
TiO
2
. It was found that the
results of UV Raman
spectra
are
different
from
those
of
visible
Raman
spectra
and
XRD
patterns.
The
anatase phase of
TiO
2
at the surface region
can remain at relatively higher temperatures
than that in the bulk at elevated
calcination temperatures; namely, the anatase
phase in
the inner region of the
agglomerated TiO
2
particles
turns out to change into the rutile
phase
more
easily
than
that
in
the
outer
surface
region
of
the
agglomerated
TiO
2
particles.
The
literature
[15,17,19]
proposed the mechanism that phase
transformation of
TiO
2
might start
at the interfaces of contacting
anatase
particles. If the anatase particles of
TiO
2
are
separated,
the phase transformation of
TiO
2
from anatase to rutile
couldbe
retarded or prohibited. Jing et
al.
[34]
showed that
La
3+
did not enter the
crystal lattices of
TiO
2
and was
uniformly dispersed onto
TiO
2
in the form of lanthana
(La
2
O
3
) particles
with small
size.
To verify the above assumption, this study also
prepared
the anatase
phase
of
TiO
2
sample
covered
with
La
2
O
3
and
characterized
the
above
sample
by
visible Raman
spectroscopy and UV Raman spectroscopy. The
results of the two types
of
Raman spectra are in agreement with
each other and show that
the TiO2
particle
covered with
La
2
O
3
can
retain its anatase phase
both in the
bulk and in the surface
region even
after calcination at 900 °C.
2. Experimental Section
2.1. Catalyst Preparation.
2.1.1. Preparation of
TiO
2
.
TiO
2
was prepared
by precipitation method. To 100 mL
of
anhydrous
ethanol was added 20 mL of
titanium(IV)
n
-
butoxide
(Ti(OBu)
4
). This
solution was added to a mixture
solution of deionized water and 100 mL of
anhydrous
ethanol.
The
molar
ratio
of
the
water/Ti(OBu)
4
was
75.
After
the
formed
white
precipitate was stirred continuously
for 24 h, it was filtered and
washed
twice with
deionized water and
anhydrous ethanol.
Finally, the sample
was dried at 100 °C and
calcined in air
at
temperatures from 200 to 800 °C for
4 h, and then cooled to
room
temperature.
2.1.2.
Preparation of La
2
O
3
-
Co
V
ered TiO
2
(La
2
p>
O
3
/TiO
2<
/p>
).
The
above
TiO
2
powder
calcined at 500 °C was used as a
support. The critical
La
2
O
3
loading corresponding to
monolayer coverage
of
La
2
O
3
on the grain surface of
TiO
2
is 0.27 g/100
m
2
.
[35,36]
On
the
basis
of
the
BET
surface
area
of
the
TiO
2
support
(54.3
m
2
/g),
the
monolayer
dispersion capacity can also be
expressed
as 15 wt %
La
2
O
3
of the weight of TiO2.
La
2
p>
O
3
/TiO
2<
/p>
samples, containing different amounts
of La
2
O
3
(0.5
-
6 wt %) were prepared
by a wet impregnation method. The
support was impregnated with aqueous solution of
various concentrations of lanthanum
nitrate (La(NO
3
)
3
·
6H
2
O) and
subsequently stirred
in a hot water
bath until it was dried. After the sample
was
kept at 110 °C
overnight, it was calcined at 900 °C in air for 4
h. A TiO
2
sample
was
prepared by calcining the
TiO
2
support
at
900 °C for 4 h (denoted as
TiO
2
-
900) for
comparison
with
the
La
2
O
3
/TiO
2
sample.
Pure
La
p>
2
O
3
was
obtained
by
calcining
La(NO
3<
/p>
)
3·
6H
2<
/p>
O at 550 °C for 4 h.
2.2. Characterization.
2.2.1.
UV
Raman
Spectroscopy.
UV
Raman
spectra
were
measured
at
room
temperature
with
a
Jobin
-
Yvon
T64000
triple
-
stage
spectrograph
with
spectral
resolution of 2
cm
-
1
. The laser
line at 325 nm of a He
-
Cd
laser was used as an exciting
source
with an output of 25 mW. The power of laser at the
sample was about 3.0 mW.
The 244 nm
line from a Coherent Innova 300 Fred laser was
used as another
excitation
source. The power of the 244 nm line at sample was
below 1.0 mW.
2.2.2. Visible
Raman Spectroscopy.
Visible Raman
spectra were recorded at room
temperature on a
Jobin
-
Yvon U1000 scanning
double monochromator with the spectral
resolution
of
4
cm
-
1
.
The
line
at
532
nm
from
a
DPSS
532
Model
200
532
nm
single
-
frequency
laser was used as the excitation
source.
2.2.3.
X
-
ray
Powder
Diffraction
(XRD),
TEM,
and <
/p>
Ultra
V
iolet
-
Visible
Diffuse
Reflectance
Spectroscopy.
XRD
patterns
were
obtained
on
a
Rigaku
MiniFlex
diffractometer with a Cu KR radiation
source. Diffraction patterns were collected from
20°
to 80°
at a
speed of 5°/min. TEM was taken on a
JEM
-
2011
TEM for
estimating
particle size and
morphology. UV
-
vis
diffuse reflectance spectra were
recorded on a
JASCO
V
-
550
UV
-
vis
spectrophotometer.
2.2.4. Br
unauer
-
Emmett
-
Teller (BET) Specific Surface Area.
The BET surface area of
the
TiO
2
support was measured
by nitrogen adsorption at 77 K using a
Micromeritics
ASAP 2000 adsorption
analyzer.
3.
Results
3.1. Spectral
Characteristics of Anatase and Rutile
TiO
2
.
The anatase
and rutile
phases
of
TiO
2
can
be
sensitively
identified
by
Raman
spectroscopy
based
on
their
Raman spectra.
The anatase
phase shows major Raman bands at 144, 197, 399,
515,
519
(superimposed
with
the
515
cm
-
1
band),
and
639
p>
cm
-
1
.
[37]
These
bands
can
be
attributed to the six
Raman
-
active
modes of anatase phase with the
symmetries of Eg,
Eg, B1g,
A1g, B1g, and Eg,
respectively.
[37]
The
typical Raman bands due
to rutile
phase appear at 143 (superimposed with
the 144 cm
-
1 band due to
anatase phase), 235,
447, and 612
cm
-
1
, which
can be ascribed to the B1g,
two
-
phonon scattering, Eg,
and
A1g
modes of rutile
phase, respectively.
38
Additionally, the band at
144
cm
-
1
is the
strongest one for the anatase phase and
the band at 143
cm
-
1
is the
weakest one for the
rutile phase. Parts
A and B, respectively, of Figure 1display the
Raman spectra of TiO
2
calcined at 500 and 800 °C with
excitation lines at 532,
325, and 244
nm. Obviously,
both visible Raman
spectra and UV Raman spectra show that the
TiO
2
sample is in the
anatase phase (Figure 1A) and rutile
phase (Figure 1B).
Figure 2
shows UV
-
vis diffuse
reflectance spectra of the
TiO
2
sample calcined at
500 and 800 °C (the
TiO
2
sample is in the
anatase phase and rutile phase, respectively).
For the anatase
phase, the
maximum absorption and the absorption band edge
can be
estimated to be
around 324 and 400 nm, respectively. The maximum
absorption and the
absorption band edge
shift to a little longer wavelength for the rutile
phase.
[39]
By
comparing
the
Raman
spectra
of
the
anatase
(Figure
1A)
or
rutile
phase
(Figure
1B)
excited
by
532,
325,
and
244
nm
lines,
it
is
found
that
the
relative
intensities of characteristic
bands due to anatase or rutile phase in
the high
-
frequency
region
are different. For
the anatase phase (Figure 1A), the band at
638
cm
-
1
is the
strongest one in the Raman spectrum
with the
excitation line at 325 or 532
nm, while
the band at 395
cm
-
1
is the
strongest one in the Raman spectrum with the
excitation
line at 244
nm.
For the rutile
phase (Figure 1B), the intensities of the bands at
445 and 612 cm
-
1
are comparable in the visible Raman
spectrum. The intensity of the band at 612
cm
-
1
is
stronger
than that of the
band at 445 cm
-
1
in the Raman spectrum with
the
excitation
line at 325 nm, and the
reverse is true for the Raman spectrum with the
excitation line at
244 nm. In addition,
for the rutile phase, a band at
approximately 826
cm
-
1
appears in
the UV Raman spectra. Some
investigations show that the rutile phase of TiO2
exhibits
a weak band at 826
cm
-
1 assigned to the
B
2g
mode.
[38,40]
The
fact that the relative intensities of the Raman
bands of anatase phase or rutile
phase
are different for UV Raman
spectroscopy
and visible Raman spectroscopy are
mainly due
to the UV
resonance Raman effect because the laser lines at
325 and 244
nm are in the
electronic absorption region of
TiO
2
(Figure 2).
There is no resonance
Raman effect
observed for
the
TiO
2
sample excited by
visible laser line, because the
line
at 532 nm is outside the absorption
region of TiO
2
(Figure 2).
Therefore, for the
anatase
or rutile phase, the Raman spectroscopic
characteristics in the visible Raman
spectrum are different from those in
the UV Raman spectrum. When the UV laser line
with different wavelengths is used as
the excitation source, the resonance enhancement
effect on the Raman bands of
anatase or rutile phase is different.
For example, for the
rutile
phase (Figure 1B), the band at 612
cm
-
1
is easily
resonance
enhanced when the
excitation wavelength is 325 nm. Among
all the characteristic bands of the rutile phase,
the extent of resonance enhancement of
445 cm
-
1
is the
strongest when the 244 nm laser
is used
as the excitation source (Figure 1B).
3.2.
Semiquantitative
Analysis
of
the
Phase
Composition
of
TiO
2
by
XRD
and
Raman Spectroscopy.
The
weight fraction of the rutile phase in the
TiO
2
sample,
W
R,
can be
estimated from the XRD peak intensities using the
following formula:
[41]
WR
?
1
[
1
?
0
.8
84
(
A
ana
A
rut
)
]
where
A
ana
and
A
rut represent the
X
-
ray integrated intensities
of
anatase (101) and
rutile
(110) diffraction peaks, respectively.
To estimate the weight fraction of the
rutile phase in the TiO
2
sample by Raman
spectroscopy, pure anatase phase and
pure rutile phase of the
TiO
2
sample, which have
been prepared by calcination of
TiO
2
powder at 500 and 800
°C for 4 h, were
mechanically mixed at given weight
ratio and ground carefully to mix
sufficiently.
Figure 3A
displays the visible Raman spectra of the
mechanical mixture with 1:1,
1:5, 1:10,
1:15, 5:1, and 10:1 ratios of
anatase
phase to rutile phase. The relationship
between the area ratios of the visible
Raman band at 395 cm
-
1 for
anatase phase to the
band
at
445
cm
-
1
for
rutile
phase
(
A
395
cm
-
1
/
A
445
cm
-
1
)
and
the
weight
ratios
of
anatase
phase to rutile phase (
W
A
/
W
R
) is
plotted in Figure 3B. It can be seen that a linear
relationship between the band area
ratios and the weight ratios of anatase phase to
rutile
phase in the mixture is
obtained. The rutile content in the Degussa P25,
which usually
consists of roughly
about 80% anatase and 20% rutile
phase,
42
was estimated by
this
plot. Our Raman result
indicates that the rutile content in
the Degussa P25 is about
18.7%, which is close to the known
result. Thus, the above linear relationship based
on
visible Raman spectroscopy can be
used to estimate the rutile content in
TiO
2
.
Figure 4A presents the UV Raman spectra
of the mechanical
mixture with 1:1,
1:2, 1:4, 1:6, 1:10, and 1:15 ratios of
anatase
phase to rutile phase with the
excitation
line at 325 nm. Figure 4B
shows the plot of the area ratios of the UV Raman
band at
612
cm
-
1 for rutile phase to the
band at 638 cm
-
1 for anatase
phase (
A
612 cm
-
1
/
A
638
cm
-
1
)
versus the weight ratios of rutile phase to
anatase phase (
W
R/
W
A). There is also a
linear
relationship between the band area ratios and the
weight ratios of rutile phase to
anatase phase.
3.3. Phase Transformation of
TiO
2
at Elevated Calcination
Temperatures.
3.3.1.
XRD
Patterns
and
Visible
Raman
Spectra
of
TiO
2
Calcined
at
Different
Temperatures.
Figure
5
shows
the
XRD
patterns
of
TiO
2
calcined
at
different
temperatures.
The
“A”
and
“R”
in
the
figure
denote
the
anatase
and
rutile
phases,
respectively. For the sample before
calcination, diffraction peaks due to the
crystalline
phase
are
not
observed,
suggesting
that
the
sample
is
still
in
the
amorphous
phase.
When the sample was calcined at 200 °C,
weak and broad peaks at
2
?
=
25.5°, 37.9°,
48.2°,
53.8°,
and
55.0°
were
observed.
These
peaks
represent
the
indices
of
(101),
(004), (200), (105),
and (211) planes of anatase phase,
respectively.
[43]
These
results
suggest that some
portions of the amorphous phase transform
into the anatase phase.
The
diffraction peaks due to anatase phase develop
with increasing the temperature of
calcination. When the calcination
temperature was increased to 500 °C, the
diffraction
peaks due to anatase phase
became narrow and intense in intensity. This
indicates that
the crystallinity of the
anatase phase is further
improved.
[44]
When the sample was calcined at 550 °C,
weak peaks were observed at
2
?
=27.6°,
36.1°,
41.2°, and 54.3°, which correspond to the indices
of (110), (101), (111), and (211)
planes
of rutile phase.
[43]
This indicates that the
anatase phase starts to
transform into
the rutile phase at 550 °C. The
diffraction peaks of anatase phase gradually
diminish in
intensity
and
the
diffraction
patterns
of
rutile
phase
become
predominant
with
the
calcination temperatures from 580 to
700 °C. These results clearly show that the phase
transformation
from
anatase
to
rutile
progressively
proceeds
at
the
elevated
temperatures.
The
diffraction
peaks
assigned
to
anatase
phase
disappear
at
750
°C,
indicating
that
the
anatase
phase
completely
changes
into
the
rutile
phase.
The
diffraction peaks of rutile phase
became quite
strong and sharp after the
sample was
calcined at 800 °C, owing to
the high crystallinity of the rutile
phase.
Figure
6
displays
the
visible
Raman
spectra
of
TiO
2
calcined
at
different
temperatures. For
the sample before calcination, two broad bands at
about 430 and 605
cm
-
1
are observed, indicating
that the
sample is
in the amorphous
phase.
[19]
For the
sample
calcined
at
200
°C,
a
Raman
band
at
143
cm
-
1
is
observed
and
the
high
-
frequency
region
shows interference from the
fluorescence
background, which
might
come
from
organic
species.
After
calcination
at
300
°C,
other
characteristic
bands of anatase phase appear at 195,
395, 515, and 638
cm
-
1
, but some
portions of the
sample may exist in the
amorphous phase because there is still a broad
background in
Figure 6.
It
was
found
that,
when
the
sample
was
calcined
at
400
°C,
the
fluorescence
disappeared,
possibly because the organic residues were removed
by the oxidation. The
bands of anatase
phase increased in intensity and
decreased in line width when
the
sample was calcined at 500 °C. This
result suggests that the crystallinity of the
anatase
phase is greatly
improved,
[18]
which
is confirmed by XRD (Figure 5). The
enlarged
section of Figure
6
shows the Raman spectrum of the
high
-
frequency region of
the
sample calcined at 500
°C. Besides the bands at 395, 515, and 638
cm
-
1
, two very
weak
bands
at
320
and
796
cm
-
1
are
observed.
These
two
bands
can
be
assigned
to
a
two
-
phonon
scattering band and a first overtone of B1g at 396
cm
-
1
,
respectively.
[37]
It
is noteworthy that a very weak band
appears
at 445
cm
-
1
due to
rutile phase for the
sample calcined at
550°C. This indicates that the anatase phase
starts to change into the
rutile phase
at
550
°C.
This
result is
in
good agreement
with
that of XRD patterns
(Figure
5).
The
weight
percentage
of
the
rutile
phase
in
the
samples
calcined
at
different temperatures was estimated by
visible Raman spectroscopy and XRD (shown
in Figure 7). As seen from Figure 7,
the rutile content
estimated from
visible Raman
spectrum
and
XRD
pattern
of
the
sample
calcined
at
550
°C
is
4.2%
and
5.7%,
respectively.
It
can
be
seen
that
the
rutile
contents
estimated
by
visible
Raman
spectroscopy and XRD are also in
accordance with each other.
When the sample
was calcined
at
580
°C,
other two
characteristic
bands were
observed at 235 and 612
cm
-
1 due to
Raman
-
active
modes of rutile phase. Figure 7
shows
the rutile content is 13.6% and 10.9% based on the
visible Raman spectrum and
XRD pattern
of the sample calcined at 580 °C.
The
intensities of the bands of rutile
phase (235, 445, and 612
cm
-
1
)
increased steadily while those of the bands of
anatase
phase (195, 395, 515, and 638
cm
-
1
) decreased
when the calcination temperatures were
elevated from 600 to 680 °C
(Figure 6). These results suggest that
the TiO2 sample
undergoes the phase
transformation from anatase to rutile gradually.
The rutile content
was estimated for
the samples calcined from 600 to 680 °C based on
the visible Raman
spectra. The results
show that the content of the rutile phase is
increased from 33.1% to
91.2%
respectively for the samples calcined at 600 and
680 °C
(Figure 7). The XRD
results
corresponding
to
the
above
two
samples
indicate
that
the
rutile
content
is
changed from 32.9%
to 90.7%
(Figure 7). These results clearly show that the
rutile
content in the sample estimated
by visible Raman spectroscopy is agreement with
that
estimated by XRD.
The
Raman
spectrum
of
the
sample
calcined
at
700
°C
shows
mainly
the
characteristic bands of rutile phase,
but the very weak
bands of anatase
phase are still
observed (Figure 6).
When the
sample was calcined at 750 °C,
the bands of anatase
phase disappeared
and only the bands due to rutile phase (143, 235,
445, and 612
cm
-
1
)
were observed. These results indicate
that the anatase phase completely transforms into
the rutile phase
and are
consistent with the results from XRD (Figure 5).
When
the
temperature
was
increased
to
800
°C,
the
characteristic
bands
due
to
rutile
phase
increased in intensity
further.
Both the results of XRD and visible
Raman spectra (Figures 5 and 6) show that
the anatase phase appears at around 200
°C
and perfect anatase phase is formed
after
calcination at temperatures
of 400
-
500 °C.
The rutile phase starts to form at 550
°C,
and the anatase phase
completely transforms into the rutile phase at 750
°C. The signals
of visible Raman
spectra come
mainly from the bulk
region of TiO
2
because the
TiO
2
sample
is
transparent
in
the
visible
region
(Figure
2).
[33]
XRD
is
known
as
a
bulk
-
sensitive
method. Therefore, it is essentially in
agreement between the results of
visible Raman spectra and XRD
patterns.
3.3.2. UV Raman
Spectra of TiO
2
Calcined at
Different
Temperatures.
UV
-
vis diffuse
reflectance spectra (Figure 2) clearly
show that TiO
2
has strong
electronic absorption in
the
UV region. Thus, the UV Raman spectra
excited by a UV laser
line contain more
signal from the surface skin region
than the bulk of the TiO
2
sample because the signal
from the bulk
is attenuated sharply due to the strong
absorption.
[33]
Therefore,
if
a UV laser line in the
absorption region of TiO
2
is
used as the
excitation source of
Raman spectroscopy, the information
from
UV Raman spectra is often
different from
that of visible Raman
spectra.
The laser line
at 325 nm was selected as the excitation source
of the UV Raman
spectra. The
UV Raman spectra and the content of the rutile
phase of the TiO
2
sample
calcined at different temperatures are
shown in parts A and B, respectively, of Figure 8.
When the sample was calcined at 200 or
300 °C,
the Raman band at 143
cm
-
1
with a
shoulder
band
at
195
cm
-
1
and
three
broad
bands
at
395,
515,
and
638
cm
-
1
were
observed, indicating
that the anatase phase is formed in the sample.
However, the low
intensity
and
the
broad
band
indicate
that
the
amorphous
phase
still
remains
in
the
sample. It can be seen
that the fluorescence in the
high
-
frequency region can be
avoided
when
the
UV
laser
line
is
used
as
the
excitation
line.
However,
the
corresponding
visible Raman spectra (Figure 6) show
interference from the fluorescence.
All bands assigned to anatase phase
become sharp and strong
after
calcination at
500 °C (Figure 8A).
These results are in
agreement with
those of XRD and visible
Raman
spectra
(Figures
5
and
6).
The
UV
Raman
spectra
of
the
sample
with
the
calcination temperatures from 550 to
680 °C are essentially
the same as
those of the
sample calcined at 500 °C
(Figure 8A).
However, according to the
XRD patterns and
visible Raman spectra
(Figures 5 and 6), the anatase phase starts to
transform into the
rutile phase at only
550 °C and the anatase phase gradually changes
into the rutile phase
in the
temperature range of 550
-
680
°C.
After
calcination at 700 °C, a new band at 612
cm
-
1 and two weak bands at
235
and 445 cm
-
1
due to rutile phase appear
while the
intensities of the bands of anatase
phase begin to decrease (Figure 8A). On
the basis of the UV Raman spectrum and XRD
pattern of the sample calcined at 700
°C, the rutile content in the sample is 56.1% and
97.0%, respectively (Figure
8B). It is found that the rutile
content estimated by UV
Raman
spectroscopy is far less than that estimated by
XRD.
When the sample
was calcined at 750 °C, the intensities of the
bands due to rutile
phase increased,
but the intensities of the bands due to anatase
phase were still strong in
the UV Raman
spectra (Figure 8A). The UV Raman spectrum of the
sample calcined at
750 °C indicates
that the rutile content is
84.3%
(Figure 8B). However, the results of
XRD and visible
Raman
spectrum (Figures 5 and 6) suggest that the
anatase phase
totally transformed into
the rutile phase after the sample was
calcined at 750 °C. The
characteristic bands due to anatase
phase disappear and the sample is in the rutile
phase
after calcination at 800 °C
(Figure 8A). Obviously, there are distinct
differences
between
the
results
from
the
UV
Raman
spectra,
visible
Raman
spectra,
and
XRD
patterns.
It seems that the anatase phase remains at
relatively higher temperatures when
detected by UV Raman spectroscopy than
by XRD and visible Raman spectroscopy.
Another UV laser line at
244 nm was also selected as the excitation source
of UV
Raman spectroscopy in order to
get
further insights into the phase
transformation of
TiO
2
. The results
of the UV Raman spectra of
TiO
2
calcined at different
temperatures
with the
excitation line at 244 nm are presented
in Figure 9. When the sample was
calcined at 200 °C, four broad
bands were observed at 143, 395, 515,
and 638 cm
-
1,
which clearly indicate that the anatase
phase exists in the sample. The intensities of the
Raman bands due to anatase phase (143,
395, 515, and 638
cm
-
1
) become
strong after
calcination at 500 °C. The
UV Raman spectra hardly change for the sample
calcined at
different temperatures even
up to 680 °C. The characteristic bands (445 and
612 cm
-
1
)
of
rutile
phase
appear
only
when
the
calcination
temperature
exceeds
700
°C.
This
result
is
in
good
agreement
with
that
from
the
UV
Raman
spectrum
of
the
sample
calcined at 700 °C
with 325 nm excitation (Figure 8A). The
intensities of the bands due
to anatase
phase (395, 515,
and 638
cm
-
1
) decrease
while those of bands assigned to
rutile
phase (445 and 612
cm
-
1
) increase
after calcination at 750 °C
(Figure 9).
When
the sample was calcined at 800 °C,
the Raman
bands due to
anatase phase disappeared, while the bands of
rutile phase developed. This
result
indicates that the sample calcined at 800 °C is in
the rutile phase. It is interesting
to
note that the results of the UV Raman spectra with
the excitation lines at
325
and 244 nm are in agreement with each other but
are different from those of XRD
patterns and visible Raman
spectra.
3.3.3.
TEM
of
the
TiO
2
Sample
Calcined
at
Different
Temperatures.
TEM
was
used to characterize the
microstructure
of the
TiO
2
sample calcined at 500,
600, and
800 °C (shown in
Figure 10). Most particles in the
sample calcined at 500 °C
exhibit
diameters in a range between 10 and 30
nm (Figure 10a). On the other hand, remarkable
agglomeration is observed
for the TiO
2
sample calcined at 500 °C. The particle
size
increases after calcination at 600
°C (Figure 10b). According to the results of XRD
and
visible
Raman
spectra
(Figures
5
and
6),
the
sample
undergoes
the
phase
transformation from
anatase to rutile gradually in the temperature
range of 550
-
680 °C. These
results imply that the phase transformation and
growth of the particle
size
are interrelated. Many researchers
[45
p>
-
49]
reported
similar phenomena. Kumar et al.
45
attributed
this
particle
size
growth
to
the
higher
atomic
mobility
because
of
bond
breakage
during
the
phase
transformation.
When
the
calcination
temperature
was
increased to 800 °C,
TiO
2
particles further grew
and the particle size could be as large
as about 200 nm (Figure
10c).
3.4.
Visible
Raman
Spectra
and
UV
Raman
Spectra
of
La
2
O
3<
/p>
/TiO
2
with
Increasing
La
2
O
3
Loading.
The
lite
rature
[15,17,29]
proposed
the
mechanism
that
the
phase
transformation
of
TiO
2
might
start
at
the
interfaces
of
contacting
anatase
particles.
If
direct
contact
between
anatase
particles
of
TiO
2
is
avoided,
the
phase
transformation
of
TiO
2
from
anatase
to
rutile
could
be
retarded
or
prohibited.
This
assumption may be verified by covering
the surface of anatase TiO
2
with an additive. In
this work, we used
La
2
O
3
dispersed on anatase TiO
2
to
prevent
the anatase particles
from contacting directly because it was
reported that
La
2
O
3
could be highly dispersed
on anatase Ti
O
2
.
[34
-
36]
Figure
11A
displays
the
visible
Raman
spectra
of
La
2
O
3
/TiO
2
with
increasing
La
2
O
3
loading.
TiO
2
support is in the
anatase
phase because only
characteristic bands
(143, 195, 395,
515, and 638
cm
-
1
) due to
anatase phase are observed. When the
TiO
2
support was
calcined at 900 °C
(TiO
2
-
900), the
Raman spectrum gave the characteristic
bands of rutile phase, indicating that
the TiO
2
-
900
sample was in the rutile phase. When
the sample with 0.5 wt %
La
2
O
3
loading was calcined at 900 °C, the Raman spectrum
drastically changed, as compared to the
TiO
2
-
900 sample.
Only characteristic bands of
anatase
phase were observed, suggesting that the
TiO
2
sample retains its
anatase phase
when
La
2
O
3
loading is 0.5 wt % while the
TiO
2
-
900 sample
is in the rutile phase. The
spectra of
the samples
with
La
2
O
3
loadings from 1 to 6 wt % are almost the same as
those
for
the
sample
with
0.5
wt
%
La
2
O
3
loading,
except
for
a
small
decrease
in
intensity.
Figure 11B shows the UV Raman spectra
of La2O3/TiO
2
with
increasing
La
2
O
3
loading. The Raman spectrum of the
TiO
2
support and
the TiO
2
-
900
sample gives the
characteristic
bands
of
anatase
phase
and
rutile
phase,
respectively.
When
La
2
O
3
loading is
varied from 0.5 to 6 wt %, the results of the UV
Raman spectra show that all
the samples
are in
the anatase
phase.
These results are in
accordance with
those of
visible Raman spectra (Figure
11A). The results from XRD patterns (the XRD
patterns
for the above samples are not
shown) agree
well with those of visible
Raman spectra
and UV Raman spectra.
For both visible Raman spectra and UV
Raman spectra, no
bands due to
crystalline phase of
La
2
O
3
are observed for all the
La
2
O
3
/TiO
2
samples,
showing that
La
2
O
3
is highly dispersed
on the surface of
the anatase phase of TiO
2
particles.
[35]
4. Discussion
It
has been clearly shown that the results of visible
Raman
spectra (Figure 6) are in
good agreement with the results from
XRD patterns (Figure 5) but are
different from
those
of
UV
Raman
spectra
(Figures
8A
and
9)
for
TiO
2
calcined
at
elevated
temperatures.
The
inconsistency
in
the
results
from
the
three
techniques
can
be
explained by the fact that UV Raman
spectroscopy provides the information
mainly
from
the
surface
region
while
visible
Raman
spectroscopy
and
XRD
provide
information from the bulk of
TiO
2
. The discrepant results
of UV Raman spectra, visible
Raman
spectra, and XRD patterns are attributed to their
different detectable depths for
TiO
2
particles.
[33]
The
disagreements
of
UV
Raman
spectra,
visible
Raman
spectra,
and
XRD
patterns suggest that the crystal phase
in the surface region is different from that in
the
bulk during the phase
transformation of TiO
2
.
Busca et al.
[20]
characterized the Degussa
P25
using
Fourier
transform
Raman
spectroscopy
and
XRD
technology.
They
estimated the rutile
-
to
-
anata
se ratio by Raman
spectroscopy and XRD,
and found that
the ratio estimated by
Raman spectroscopy for the Degussa P25 was smaller
than that
evaluated by XRD. Therefore,
they assumed that the rutile phase
in
the Degussa P25
was more concentrated
in the bulk because
Raman spectroscopy
excited by a near
-
IR
laser
line
should
be
more
surface
-
sensitive
than
XRD.
Different
from
their
investigations,
our experimental results give direct UV
Raman
evidence to show that
the phases in the surface region are
generally different from that in the
bulk region of
TiO
2
,
particularly when TiO
2
is in
the transition stage of the phase
transformation.
As
presented
above,
the
anatase
phase
can
remain
at
relatively
higher
temperatures
as
observed
by
UV
Raman
spectroscopy
than
by
visible
Raman
spectroscopy
and
XRD.
These
facts
lead
us
to
the
conclusion
that
the
phase
transformation of
TiO
2
takes place from its
bulk region and then extends to its surface
region.
To
further understand the process of the phase
transformation of TiO
2
, we
used the
TEM
technique
to
observe
the
microstructure
of
the
sample
calcined
at
different
temperatures
(Figure
10).
TEM
results
show
that
the
samples
are
composed
of
aggregated particles after the
calcination. According to TEM measurements, Penn
et al.
[17]
suggested
that
structural
elements
with
rutilelike
character
can
be
produced
at
a
subset of
anatase interfaces, and these might serve as
rutile nucleation sites. Lee et al.
[29]
investigated the growth and
transformation in nanometersize
TiO
2
powders by
in situ
TEM. The nucleation of rutile
was found to occur at the amorphous interface of
anatase
particles
where
there
are
strain
and
disorder.
On
the
basis
of
the
experimental
observations
and
combined
with
the
results
from
the
literature,
we
suggest
that
the
phase transformation of
TiO
2
starts from the
interfaces among the anatase particles
of
the agglomerated
TiO
2
particles. On the basis
of kinetic data from XRD, Zhang et
al.
15
Also
proposed
that
interface
nucleation
dominated
the
transformation
for
nanocrystalline anatase samples
with denser particle packing below 620
°C, or in the
temperature range of
620
-
680 °C.
If the direct contact between anatase
particles is avoided, the phase transformation
could be retarded or prohibited because
the rutile phase nucleates at the
interfaces of
contacting
anatase
particles.
We
prepared
the
anatase
particles
covered
with
highly
dispersed
La
2
O
3
,
and the results of visible Raman spectra and UV
Raman spectra of the
La
2
O
3
/TiO
2
samples (Figure 11) indicate that the
samples are stabilized at their anatase
phase both in bulk and in the surface
region even after the calcination at 900
°C.
It is interesting to note
that the impregnation of only 0.5 wt%
La
2
O
3
can inhibit the
phase transformation.
The explanation of this interesting result could
be as follows: the
defect sites on the
surface of the anatase particles are assumed to
play an important role
in the phase
transformation of TiO
2
. When
the defect sites of the anatase particle react
with
a
neighboring
anatase
particle
with
or
without
defect
sites,
the
rutile
phase
formation may start at
these sites.
La
2
O
3
easily reacts with the defect sites of the anatase
particles, and only 0.5 wt %
La
2
O
3
can occupy or deactivate all the defect
sites of the
anatase particles because
usually the surface defect sites concentration is
relatively low.
The easy migration of
surface atoms of anatase and the nucleation of
rutile phase most
possibly take place
at
the surface defect
sites.
Therefore, only 0.5 wt %
La
2
O
3
can
effectively inhibit the phase
transformation of anatase.
In addition to occupying the defect
sites, the highly dispersed
La
2
O
3
on the surface
of the anatase particles
effectively prevents
direct contact of
the anatase particles for
the sample
with high
La
2
O
3
loadings. Therefore, the La
p>
2
O
3
/TiO<
/p>
2
sample can retain its
anatase phase even when the calcination
temperature is up
to 900 °C, owing to
the
above two roles played by
La
2
O
3
.
A
proposed
scheme
for
the
phase
transformation
of
TiO
2
with
increasing
calcination
temperature
is
illustrated
in
Figure
12.
The
TiO
2
particles
with
anatase
phase intimately contact each
other. Thus, the surface and the bulk
region of the TiO
2
sample
actually refer to
respectively the outer surface region and the
inner region of
agglomerated
TiO
2
particles. The
interfaces of
contacting anatase
particles, which are
only present in
the inner region of agglomerated particles,
provide the nucleation sites
of the
rutile phase.
Therefore, the rutile
phase is
first
detected
by
XRD
and
visible
Raman spectroscopy for the
sample calcined at 550
-
680
°C. Once phase transformation
takes
place, the particle size increases rapidly. The
agglomeration of the TiO
2
particles
is along with the phase
transformation from anatase
to rutile.
The rutile phase needs a
fairly
high
temperature
to
progressively
develop
into
the
whole
conglomeration
composed
of
the
coalescence
of
some
neighboring
particles
because
the
phase
transformation
is
a
diffusing
process.
Thus,
the
outer
surface
region
of
the
agglomerated particles without directly
interacting with other particles maintains in the
anatase phase
when the
calcination temperature is
below 680
°C.
Accordingly,
UV
Raman spectroscopy detects only the
anatase phase in the outer region of agglomerated
particles in the temperature range of
550
-
680 °C.
When the calcination
temperature is higher than 700 °C, the anatase
phase in the
outer surface region of
agglomerated
particles begins to change
into the rutile phase.
Therefore, the
mixed phases of anatase and rutile are observed by
UV Raman
spectroscopy but
the inner region of agglomerated particles is
nearly in the rutile phase.
Both
XRD
and
visible
Raman
spectra
show
that
the
inner
region
of
agglomerated
particles is in
the
rutile phase when the sample is
calcined at 750 °C. However,
the
phase transformation is not yet
complete because the outer surface region is still
in the
mixed phases of anatase and
rutile. After calcination at 800 °C, the anatase
phase in the
outer surface region
completely transforms to the rutile phase; the
whole agglomerated
particles are in the
rutile phase.
Following the
above reasoning, for the agglomerated particles
of TiO
2
, the
rutile
phase nucleates at
the interfaces
of contacting
anatase particles. However, from
the
point view of a single
anatase crystal particle, the rutile phase starts
to form still at the
surface
of
TiO
2
,
where
it
contacts
other
particles.
It
is
reasonably
assumed
that
the
phase transformation of single
particles might start from the surface, where
there is no
direct
interaction with
other
particles, but
it needs
a
high temperature.
Zhang
et
al.
[15]
indicated
that thermal fluctuation of Ti and O atoms in
anatase is not strong enough
to
generate rutile nuclei on the surfaces or in the
bulk of the anatase particles at lower
temperatures.
When
the
small
anatase
particles
agglomerate
into
large
particles,
interface
nucleation is
easier, as compared to nucleation at the surface,
where there is no contact
with
other
particles.
Zhang
et
al.
[15]
indicated
that
the
activation
energy
for
surface
nucleation is expected to be higher
than that for interface
nucleation.
Therefore, we
observed
the
phenomenon
that
the
crystalline
phase
in
the
outer
surface
region
of
agglomerated
TiO
2
particles is different from that in the
inner region of
agglomerated
TiO
2
particles.
5.
Conclusions
UV
Raman
spectroscopy
is
found
to
be
more
surface
-
sensitive
than
visible
Raman
spectroscopy and XRD
for TiO
2
because of strong
absorption of TiO
2
in the UV
region.
According to
the
visible Raman spectra and XRD patterns, the phase
transformation
from anatase
to rutile takes place at 550 °C and the anatase
phase completely transfers
to the
rutile phase when
the sample is
calcined at temperatures up to 750 °C. On the
basis of the UV Raman spectra, the
rutile phase is observed only when the calcination
temperature exceeds 700 °C, and the
anatase phase can still be detected at 750 °C. The
disagreements of UV Raman spectra,
visible Raman spectra, and XRD patterns suggest
that the crystalline phase in the
surface region is usually different from that in
the bulk
during the phase
transformation of TiO
2
.
Furthermore, the anatase phase in the surface
region
can remain at
relatively higher temperatures than it can in the
bulk region of
TiO
2
. The results
of TEM show that the agglomeration of the
TiO
2
particles and growth
of particle size
are along
with the phase transformation. The anatase phase
of
TiO
2
sample covered with highly dispersed
La
2
O
3
can retain
its anatase phase both in
bulk
and in surface region
even after
calcination at
900 °C because the direct contact of
anatase particles of
TiO
2
is avoided and the
surface defect sites of anatase particles are
occupied by
La
2
O
3
.
It is proposed that the phase transformation of
TiO
2
starts from the
interfaces between the anatase
particles in the agglomerated
TiO
2
particles.
Acknowledgment.
This work
was financially supported by
the
National Natural
Science Foundation of
China (NSFC, Grants 20273069, 90210036), the
National Basic
Research
Program
of
China
(Grant
2003CB615806),
and
the
National
Key
Basic
Research and Development Program (Grant
2003CB214500).
p>
《物理学》
、
《化学》
2006
年
,110,927<
/p>
-
935 B
二氧化钛的紫外拉曼光谱研究
一、相变和在地球表面散装
作者:张京、李梅君、冯召池、陈军、和李勘
研究院:国家重点催化实验室、大连化学物理研究所、中国科学院
地址:中国大连市
116023
邮政信箱号
110
成稿日期
:
2005
年
11
月
4
日
截止
:2005
年
9
月
< br>16
日
;
p>
对从锐钛矿型到金红石型的二氧化钛进行了研究
,
< br>利用紫外拉曼光谱激光器
325nm
和
< br>244nm
激发、可见拉曼光谱
532nm
激光、
x
射线衍射仪
(XR
D)
、透射
电镜
(TEM)
。研究发现紫外拉曼光谱比可见拉曼光谱、
x
射线
衍射等对二氧化钛
表面的吸收更加敏感,
这是由于二氧化钛能够
强烈地吸收紫外线的缘故。
锐钛矿
阶段检测的样品用紫外拉曼光
谱相比可见拉曼光谱、
x
射线衍射等方法需要在较
高的煅烧温度条件下进行。
上述三种技术的不同结果表明
,
二氧化钛表面的锐钛
矿阶段比在相变部分更需要维持相
对较高的煅烧温度。
在透射电镜
(TEM)
实验结
果表明
,
当二氧化钛样品
在高温下煅烧时小颗粒凝聚成大颗粒,
并且二氧化钛粒
子的凝聚
力是从锐钛矿转向金红石时伴随着相变。
它表明在二氧化钛粒子结晶中
< br>金红石阶段形成于界面上的锐钛矿粒子与粒子之间
,
即锐
钛矿阶段结晶二氧化钛
颗粒的中心区域比外表面区域转换成金红石相更容易。
当二氧化钛颗粒的锐钛矿
晶型被高度分散的
La<
/p>
2
O
3
覆盖着时
,
在相变的大部分区域和表面部分都被明显的
< br>弱化,这是因为避免了锐钛矿粒子的直接接触和锐钛矿粒子表面缺陷部位被
La<
/p>
2
O
3
占据的原
因。
1.
介绍
提
泰妮娅
(
二氧化钛
)
< br>被广泛研究是由于其在催化作用中独特的光学和化学性质
[1]
< br>、
光催化
[2]
、对湿度和气体
灵敏度
[3,4]
、非线性光学
[5]
、光激发光
[6]
等等。这两种主
p>
要的二氧化钛晶型:
锐钛矿和金红石,
分别
展现出了不同的物理和化学性质。
众
所周知
,
因其高介电常数和高折射指数
[8]
< br>,在锐钛矿相是适用于催化剂的研究
[7]
,
而金红石相是以研究光学和电子为目的,
这已很好的论证了二氧化钛的结晶
阶段
在催化反应中扮演着一个重要的角色,尤其是光催化作用
[
9
-
11]
。一些研究已经声
称
,
这锐钛矿阶段比金红石相的光催化
[9,10]
更加活跃。
尽管在外界压力和温度下,金红石相比锐钛矿阶段更加热稳定
,
锐钛矿是最
常见的阶段
,
而不是金
红石,
[12]
因为在相对较低温度下的二氧化钛纳米晶中锐钛
矿是极其稳定。
[13]
可以这样认为
锐钛矿向金红石相位变换时在很宽的温度范围
内。
[14]
p>
因此
,
结晶阶段的了解和控制阶段和二氧
化钛的相变过程是很重要的
,
虽
然他们
是困难的。
很多研究
[13
-
31]
已经熟悉了二氧化钛的相变过程。
p>
张等
15
提出锐钛矿向金红石
相变阶段的机制是根据
x
-
射线衍射
(XRD)
动力学数据随温度变化而变化的。在
p>
传输和微电子扫描的基础上,格玛等
[16]
提出金红石核形成于较粗的锐钛矿粒子
的表面上,
并且新转化
的金红石颗粒增长速度以牺牲邻近的锐钛矿的粒子为代价。
宾等
17
提出金红石的原子核形成于
{112}
被热液加热的锐钛矿粒子双接口上。
二氧化钛催化性能很
大程度上取决于表面特性
,
特别是表面阶段
,
因为催化反
应发生在表面上。二氧化钛表面阶段应负责其
光催化活性
,
因为不仅光诱导反应
发生
在表面
[32]
而且光激的电子和孔也可能迁徙到表面区域。<
/p>
因此
,
暴露在光源下
< br>的二氧化钛表面阶段
,
应在光催化中发挥至关重要的作用
。
然而
,
二氧化钛表面阶
段
,
特别是相变阶段还未被研究。这具有挑战性的
问题依然存在
:
表面区域和大部
分区域
的阶段相同处
,
或者如何计算二氧化钛粒子的表面区域阶段在相
变期间它
的体积变化了多少?回答上述问题的困难主要在于缺乏合适的技术可以迅速检<
/p>
测出表面阶段的二氧化钛。
经发现,<
/p>
当样品吸收紫外线时,
紫外拉曼光谱对于固体样品的表面阶段具有
更加敏感性,我们利用紫外拉曼光谱、可见光谱、
XRD
研究了氧化锆
(
氧化锆
)
[33]
从四方相阶段到单相阶段的相变阶段。
这些结果清楚地表明
,
当四方相阶段的
二氧化锆在高温下煅烧时,
氧化锆的表面阶段通常是不同于氧化锆的大部
分阶段
并且氧化锆的相变阶段始于表面区域
,
< br>然后逐渐发展到它的大部分。
这些发现使我们能够利用
紫外拉曼光谱更进一步的研究二氧化钛表面区域
的相变阶段,同时二氧化钛也能强烈吸收
紫外线。在这项研究中
,
我们比较了在
紫外和可见地区二氧化钛的拉曼光谱使用激发线在不同温度下的煅制品。用
x
射线衍射、透射电镜
(TEM)
记录理解二氧化钛
相变阶段的过程。它的结果发现紫
外拉曼光谱是不同于那些可见的拉曼光谱和
x
射线衍射模式。
二氧化钛表面区域
的锐钛矿阶段相比高温煅烧的大部分区域要维持在较高的温度
,
这就是说在二氧
化
钛颗粒结块中心区域比在外表面二
氧化钛颗粒结块的区域的锐钛矿阶段转变成
金红石相更加容易。
有著作
[15,17,29]
提出一种
原理是二氧化钛的相变可能开始在锐钛矿颗粒相互
接触的界面,如果二氧化钛的锐钛矿颗
粒被分离
,
那么二氧化钛的相变从锐钛矿
转变为金红石的过程中将被弱化或禁止。京等
[34]
人研究
表明
La
3+
不能进入二氧
化钛的晶格并且以小粒径的氧化镧粒子的形式均匀分散在二氧化钛。
为了验
证上
述假设
,
该研究也精制了被
La
2
O
3
覆盖着的二氧化钛样品的锐钛矿阶段,并且利
用可见拉曼光谱和紫外拉曼
光谱分析了上述样品的特征。
拉曼光谱的两种不同类
型的分析结
果是相互一致的,
并且表明被
La
2<
/p>
O
3
覆盖着的二氧化钛粒子在大部分
p>
区域和表面区域甚至在
900
°C
煅烧后都能维持它的锐钛矿阶段。
2
.实验部分
2.1
.催化剂反应。
2.1.1
.
二氧化钛的制备。
二氧化钛通过沉降方法制备。
向
100
毫升的无水乙
醇中加入
20
毫升的
钛
(4)n
-
butoxide
合成技术
(Ti(IV))
,将这种溶液添加
到去离子
水的混合溶液和
100
毫升的
无水乙醇中,水与
Ti(OBu)
4
的
摩尔比是
75
,连续搅
拌
24
小时形成白色沉淀后,过滤并用去离子水和无水乙醇冲洗两次,最后
p>
,
在
100°C
下干燥样品并在空气中从
200
到
80
0°C
下煅烧
4
小时,然后冷却到室温
。
2.1.2
.附着有
La
2
O
3
的二氧化钛的制备
. (La
2
O
3
/TiO
2
)
。上述二氧化钛粉末在
500°C
煅烧被使用。临界
La
2
O
3
载荷对应于二氧化钛粒子表面上的
La
2
O
3
的单层
覆盖率是
0.27
g/100
m
2
,
[3
5,36]
在此基础上支撑二氧化钛的表面区域
(54.3
m
2
/g),
当二氧化钛的质量为
15%
的
La<
/p>
2
O
3
时单层分
散能力也可以被表达。
La
2
O
3
/TiO
2
样
p>
品,
使用浸湿法制备出包含有不同数量的
L
a
2
O
3
(0.5
-
6 wt %)
,
这种物质用含有不
同浓度的硝酸镧水溶液浸渍,随后在热水浴中搅拌直到
它吹干。将样品保持在
110°C
一夜后,
在空气
900°C
下煅烧
4
小时。
比较在
900°C
下煅烧
4
小时制备出
的二氧化钛样
品与
La
2
O
3
/TiO
2
样品。
< br>在
550°C
下煅烧
La(N
O
3
)
3
·6
H
2
O 4
小时得到
< br>纯的
La
2
O
< br>3
。
2.2
.表征。
2.2.1
.
紫外拉曼光谱。
紫外
拉曼光谱在室温下
使用
Jobin<
/p>
-
Yvon
T64000
三倍
2 cm
-
1
的光谱分辨率的光谱仪进行测量。
这个
He
-
Cd
激光器的
325 nm
激光线常
被作为输出
p>
25
兆瓦的激光源,在样品中激光的能量大约
3.0
亿瓦,将
Coherent
Innova
300
弗雷德的
244
纳米线通常作为另一
振源。样品中
244
纳米线的能量
低于
1.0
兆瓦
。
2.2.2
.
可见拉曼光谱。
可见拉曼光谱在室温下使用
Jobin
-
Yvon
U1000
双光栅
4 cm
-
1
光谱分辨率的扫描单色仪进行记录,
将离散<
/p>
532
模型
200 532 nm
的
532
纳
米线通常
作为单纵模激光振源。
2.2.3.
粉末
x
-
射线衍射
(XRD)
、透射
电镜
(TEM)
、紫外可见扩散反射光谱技
术。在
Rigaku
MiniFlex
< br>衍射仪上使用铜基米
-
雷克南辐射源得到
XRD
模式,以
p>
5°/min
的速度从
20°
到
80°
收集衍射模式,透射电镜法采取的
JEM
-
2011
透
射电
镜法估算粒度大小和形态。紫外可见扩散光谱记录在
JAS
CO
V
-
550
紫外可见分
光光度计。
2.2.4.
Brunauer
-<
/p>
Emmett
-
Teller(BET)
特定的表面区域。二氧化钛的
BET
表
面
积被测量在
77K
下氮气吸附钾微速
2000
吸附分析仪。
3.
结果
3
.1.
二氧化钛锐钛矿和金红石的光谱特性。基于它们的拉曼光谱,通过拉曼
-
-
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-
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-
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