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二氧化钛的紫外拉曼光谱研究外文翻译

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2021-02-27 17:03
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2021年2月27日发(作者:生态环境材料)







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


-

< p>
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


-


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


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


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


2


O


3



was


obtained


by


calcining


La(NO


3< /p>


)



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


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]


< p>
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

< p>
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


-


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


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).

























《物理学》



《化学》


2006



,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


< p>
地址:中国大连市


116023


邮政信箱号


110



成稿日期


: 2005



11


4




截止


:2005



9


< br>16



;







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


< 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)

< p>
。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。

< p>
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


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。



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]


,

< p>
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



,


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]


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


,



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。


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


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

< p>


,


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。

< p>
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

< p>
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

< p>
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



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

< p>
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


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。



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



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


,



100°C


下干燥样品并在空气中从


200



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%



La< /p>


2


O


3


时单层分 散能力也可以被表达。


La


2


O


3


/TiO


2



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


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



532



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








5°/min


的速度从


20°



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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