Metal–metal charge transfer and interfacial charge transfer mechanism for the visible light...
Transcript of Metal–metal charge transfer and interfacial charge transfer mechanism for the visible light...
ORIGINAL PAPER
Metal–metal charge transfer and interfacial charge transfermechanism for the visible light photocatalytic activity of ceriumand nitrogen co-doped TiO2
Rajashekhar K. Eraiah • Giridhar Madras
Received: 21 December 2013 / Accepted: 7 April 2014
� Springer Science+Business Media New York 2014
Abstract Nanosized cerium and nitrogen co-doped TiO2
(Ce–TiO2-xNx) was synthesized by sol gel method and
characterized by powder X-ray diffraction (PXRD), X-ray
photoelectron spectroscopy (XPS), FESEM, Fourier trans-
form infrared, N2 adsorption and desorption methods,
photoluminescence and ultraviolet–visible (UV–vis) DRS
techniques. PXRD analysis shows the dopant decreases the
crystallite sizes and slows the crystallization of the titania
matrix. XPS confirm the existence of cerium ion in ?3 or
?4 state, and nitrogen in -3 state in Ce–TiO2-xNx. The
modified surface of TiO2 provides highly active sites for
the dyes at the periphery of the Ce–O–Ti interface and also
inhibits Ce particles from sintering. UV–visible DRS
studies show that the metal–metal charge transfer (MMCT)
of Ti/Ce assembly (Ti4?/Ce3? ? Ti3?/Ce4?) is responsi-
ble for the visible light photocatalytic activity. Photolu-
minescence was used to determine the effect of cerium ion
on the electron–hole pair separation between the two
interfaces Ce–TiO2-xNx and Ce2O3. This separation
increases with the increase of cerium and nitrogen ion
concentrations of doped samples. The degradation kinetics
of methylene blue and methyl violet dyes in the presence of
sol gel TiO2, Ce–TiO2-xNx and commercial Degussa P25
was determined. The higher visible light activity of Ce–
TiO2-xNx was due to the participation of MMCT and
interfacial charge transfer mechanism.
Keywords Co-doped TiO2 � Metal–metal charge
transfer � Interface charge transfer � Visible light active
1 Introduction
Though titania is used for environmental remediation [1], it
is active primarily under ultraviolet radiation. Therefore,
investigators have tried to make titania more active under
visible light by doping the materials with either transition
metal or non-metal ions. The incorporation of several non
metal ions such as nitrogen [2, 3], carbon [4, 5] and fluorine
[6, 7] in the TiO2 lattice has been accomplished. Though
the modification of TiO2 by co-doping with metal ion and
non metal ion has been extensively studied [8–13], the
influence of lanthanide oxides on electron–hole pair sepa-
ration under visible light irradiation has not been widely
investigated.
Among the lanthanide oxides, ceria is a potentially good
catalyst because of its ability to shift between CeO2 and
Ce2O3 under oxidizing and reducing conditions as well as
the ease of formation of labile oxygen vacancies. The use
of metal-to-metal charge transfer (MMCT) of hetero-
bimetallic assemblies as a new class of visible-light
absorbing material has been recently demonstrated [14].
The anchored Zr (IV)–O–Cu(I) assembly on the pore of
mesoporous silica showed the photochemical splitting of
CO2 to CO by photoexcitation of the Zr(IV)/Cu(I) MMCT
band at 355 nm [15]. Similarly, MMCT has been reported
[16] for the combination of Ti4? and Ce3? ions as consti-
tuting elements [E0(Ce4?/Ce3?) = 1.72 V, E0(TiO2/
Ti3?) = -0.67 V] for the photocatalytic oxidative
decomposition of organics under visible light irradiation.
Ce has been employed as a catalyst in both stable Ce3?
(4f15d0) and Ce4? (4f05d0) oxide states due to its redox
property and oxygen storage capacity [17, 18]. There are a
few reports on cerium and nonmetal co-doped TiO2 [19,
20]. Cao et al. [19] prepared C, N and Ce co-doped TiO2
for the visible light activity of the catalyst. Xu et al. [20]
R. K. Eraiah � G. Madras (&)
Department of Chemical Engineering, Indian Institute of
Science, Bangalore 560012, India
e-mail: [email protected]
123
J Sol-Gel Sci Technol
DOI 10.1007/s10971-014-3350-4
studied the Ce and C co-doped TiO2 for the degradation of
dye Reactive Red X-38 under visible light.
In this investigation, cerium and nitrogen co-doped TiO2
(Ce–TiO2-xNx) with higher concentration (more than
1 at.%) of ceria was investigated for the visible light
degradation of dye. The surface area, crystallite size, sur-
face basicity, metal–metal charge transfer and interfacial
charge transfer mechanism was investigated. Significant
photocatalytic activity was observed for the degradation of
dyes like methylene blue (MB) and methyl violet (MV)
using this catalyst.
2 Experimental section
2.1 Materials
Analytical reagent (AR) grade chemicals were used in the
synthesis. Titanium isopropoxide (Lancaster Chemicals,
UK), Cerium Ammonium Nitrate (CAN), hexamethylene
tetraamine, Cationic dyes methylene blue (MB), methyl
violet (MV) dyes were obtained from SD Fine Chemicals,
India. Water was double distilled and filtered through a
Millipore membrane filter prior to use.
2.2 Catalyst preparation
Nanosized Ce–TiO2-xNx was prepared via the modified sol
gel method, using CAN as Ce and N precursor. 0.007 mol/l
of CAN was dissolved in 50 ml of distilled water and
cooled in ice cold bath to 4 �C. The pH of the solution was
adjusted to 8 using hexamethylene triamine. 5 ml titanium
isopropoxide (0.3 mol/l) was added drop wise to the ice
cooled solution to obtain a pale yellow colored precipitate.
The precipitate was stirred for 3 h at room temperature
using magnetic stirrer and washed repeatedly for 5 times
using distilled water. The obtained precipitate was filtered
using a vacuum filtration pump and dried for 12 h. The
powder was manually grinded for 1 h and calcined at
350 �C for 3 h to obtain 6 at.% cerium doped TiO2
(CTN06).
Similarly, 3 and 9 at.% cerium doped TiO2 (CTN03) and
(CTN09) samples were prepared by adding 0.0035 and
0.0106 mol/l solution of CAN to the 5 ml solution of
0.3 mol/l titanium isopropoxide separately. The pure ana-
tase TiO2 (ST) was prepared using same method without
adding ceria precursors.
2.3 Catalyst characterization
Powder X-ray diffraction (PXRD) patterns of catalysts
were recorded in a Phillips X’ Pert diffractometer using Cu
Ka radiation with a scan rate of 0.5�/min. The surface area
of the catalyst was determined with a standard Brunauer–
Emmett–Teller (BET) apparatus (model NOVA-1000,
Quantachrome). X-ray photoelectron spectroscopy (XPS)
using a Thermo Scientific Multilab 2000 instrument with
Al Ka source. Fourier transform infrared (FTIR) studies
were performed in the transmission mode in the frequency
range of 400–4,000 cm-1 (Perkin-Elmer, FTIR Spectrum-
1000). The photoluminescence measurements were per-
formed on a luminescence spectrometer (Perkin-Elmer LS
55) at room temperature under the excitation light of
285 nm. The ultraviolet–visible (UV–vis) absorption
spectra of TiO2 powders were obtained for the dry-pressed
disk samples using a UV–vis spectrophotometer (UV-1700
pharmaspec) with a wavelength range of 270–800 nm.
2.4 Photocatalytic experiments and sample analysis
Photocatalytic measurements were carried out in a cylin-
drical jacketed borosilicate glass container tube of 3.4 cm
inner diameter, 4 cm outer diameter and at the height of
21 cm where in the dye was degraded. The radiation was
provided by a 150 W metal halide lamp (with a cutoff
wavelength of 400 nm), which was placed inside a jacketed
quartz tube. The intensity was determined by o-nitro-
benzaldehyde actinometry and was found to be 1 W m-2
[21]. The quartz tube was dipped into the solution that was
stirred continuously and the temperature was maintained at
35 �C by cold water circulation. 100 mL of 50 ppm dye
solution and 25 mg of catalyst were stirred for 1 h in the
absence of light to check the initial surface adsorption. The
solution was then exposed to light and samples were col-
lected at regular intervals, which were then centrifuged to
remove the catalyst. These samples were then analyzed by
an UV-spectrophotometer (Shimadzu UV 1700 Pharma
Spec). The maximum absorption wavelengths (kmax) for
MB and MV were at 665 and 585 nm, respectively. The
change in the dye concentration with respect to time was
quantified based on the calibration of each dye by spec-
trophotometry. All experiments were repeated three times
and the error in concentration during degradation was less
than ±1 ppm. The stability of the catalyst was also
examined by conducting experiments with the spent cata-
lyst for at least seven cycles and no decrease in the rate of
degradation was observed.
3 Results and discussion
3.1 PXRD and BET studies
Figure 1a shows the typical PXRD patterns of ST, CTN-
03, CTN-06 and CTN-09 samples. The diffraction peaks at
2h = 25.3�, 37.9�, 48.4�, 53.9�, 62.7�, 69.0�, 70.2� are
J Sol-Gel Sci Technol
123
related to the anatase phase of TiO2 [22]. In addition, peaks
appear at 2h = 28.4� for the samples CTN-06 and CTN-09
due to the cubic cerium oxide (Ce2O3) [23] that is absent in
CTN-03 due to lower concentration of Ce2O3. The average
crystalline sizes were found to be 64, 62, 61 and 60 nm for
the samples ST, CTN-03, CTN-06 and CTN-09. This
indicates that an increase in % doping of Ce marginally
influences the crystallite size.
The ionic radii of Ce3? (1.11 A) Ce4? (1.01 A) and N3-
(1.71 A) are bigger than that of Ti4? (0.68 A) and O2-
(1.40 A), for Ce3?/Ce4? to replace Ti4? and N3- to replace
O2- in the crystal leading to change in the lattice param-
eters are as shown in Table 1 [24, 25]. This change is due
to the strain caused by the dopants in the lattice, Hence,
Ce3?/Ce4? and N3- can substitute in the TiO2 lattice,
without distorting the phase structure of TiO2.
On the basis of this, it can be inferred that Ce3?/Ce4? ions
has been substituted in the crystal lattice of the titania or cerium
oxide or exists as a highly dispersed polymorph over the titania
surface. N3- can substitute O2- and Ce3?/Ce4? can substitute
Ti4? in the TiO2 lattice. Therefore, some of the Ce3?/Ce4? ions
were incorporated into the TiO2 network while some were well
dispersed in the bulk and surface as Ce2O3. The average
crystallite sizes (D) were calculated using the Scherrer’s for-
mula D = kk/b cos h, where k is the wavelength of Cu Kaused, b is the full width at half maximum (fwhm) of the dif-
fraction angle under consideration, K is a shape factor (0.94)
and h is the angle of diffraction using a slow scanned spectra
(1/2�/min) of 101 plane of the samples are given in the Fig. 1b
and same is used to calculating the crystallite size.
The width of the (101) peak is broadened and its
intensity significantly decreased with an increase in the
10 20 30 40 50 60 70 80
Inte
nsit
y (a
.u)
CTN-09
CTN-03
CTN-06
ST
a
*
*
22 24 26 28 30
2θ scale (Degrees)2θ scale (Degrees)
*
Inte
nsit
y (a
.u)
CTN-09
CTN-06
CTN-03
ST
*b
Fig. 1 a PXRD patterns and
b enlarged spectra of 101 plane
of synthesized samples ST,
CTN-03, CTN-06, CTN-09 and
asterisk indicate Ce2O3
Table 1 Summary of data obtained by PXRD, UV–vis DRS absorption and BET measurements
Photo catalysts D (nm) (A´
) (A´
)3 kmax (nm) Eg (eV) Sarea (m2/g) Ti:Ce
ST 64 a = b = 3.7251
c = 9.2898
128.9014 380 3.3 63 1:0
CTN-03 62 a = b = 3.7165
c = 9.3854
129.5997 406 3.05 71 1:0.031
CTN-06 61 a = b = 3.7438
c = 9.3979
131.7213 409 3.03 84 1:0.062
CTN-09 60 a = b = 3.7117
c = 9.4072
129.6003 412 3.01 86 1:0.093
D: crystallite size in nm, A: lattice parameters, (A)3: unit cell volume, k max: absorption maxima in nm, Eg: band gap energies in eV, Sarea: surface
area obtained by N2 adsorption in m2/g, Ti:Ce ratio obtained from EDX data
J Sol-Gel Sci Technol
123
dopant concentration, as shown in Fig. 1b. This decrease
shows that the doping of the cerium ion inhibited the phase
transfer of titania from amorphous to anatase because the
addition of dopant suppresses the crystal growth. This also
indicates that Ce3?–TiO2 had higher thermal stability than
pure TiO2. Although the nitrogen content was increased up
to 4 at.%, no other crystalline phase like TiN could be
detected. Therefore, nitrogen ions can be assumed to be
incorporated in TiO2 [26]. The oxygen atom is replaced by
the nitrogen atom in the TiO2 lattice [27] and the marginal
shift may be due to the nitrogen incorporation in the TiO2
matrix [28].
This indicates a modification occurs in the electronic
states due to the replacement of oxygen by nitrogen on
doping [28, 29]. This leads to a substantial shift towards
the visible region in the optical absorption. The lattice of
the cell in doped samples expands in the c direction
because a small amount of Ce and nitrogen may enter
the TiO2 lattice. The interaction between Ce species and
Ti4? is because Ce2O3 has a strong basic property. Thus
partially cationic (e.g. Ce4?/Ti3?) exchanges between
Ce2O3 and TiO2 phases occur. This results in lattice
defects that enhance interaction between Ce2O3 and
TiO2.
860 870 880 890 900 910 920150000
155000
160000
165000
170000Ce 3da
Ce 3d5/2
Ce 3d3/2
Inte
nsit
y (c
ps)
Binding Energy (eV)
450 455 460 465 4700
2000
4000
6000
8000
10000
461.86 eV
456.12 eV
b
Ti 2p 1/2
Ti 2p 3/2
Ti 2p
Binding Energy (eV)524 528 532 536
2000
4000
6000
8000
10000
12000
14000 c
529.4 eV
527.4 eVO 1s
Inte
nsit
y (c
ps)
Inte
nsit
y (c
ps)
Inte
nsit
y (c
ps)
Inte
nsit
y (c
ps)
Binding Energy (eV)
375 380 385 390 395 400 405 410 415 420
21000
22000
23000
24000
25000
26000
27000
28000
29000d
396 eVN 1s
Binding Energy (eV)
1200 1000 800 600 400 200 00
50000
100000
150000
200000
250000
300000
350000
400000e
Ti 2s
Ti 3sTi 3p
Ti 2p
Ce 3d
O 1s
C 1s
N 1s
Binding Energy (eV)
Fig. 2 XPS spectra of a Ce 3d,
b Ti 2p, c O 1, d N 1s and
e CTN-06
J Sol-Gel Sci Technol
123
The BET surface area was measured for the synthesized
doped TiO2 samples. The values of the BET surface area
for the sample obtained for the samples are shown in
Table 1. It can be found that the co-doping of Ce3?/Ce4?
and nitrogen increase the surface area.
3.2 XPS analysis
Several studies have been devoted to Ce 3d XPS inter-
pretation for the two sets of spin–orbital multiplets corre-
sponding to the 3d3/2 and 3d5/2 by different researchers
[30–36]. The Ce 3d XPS CT-06 catalyst is shown in
Fig. 2a. The peaks at 881 and 885.2 eV represent Ce3?
while the peaks at 882.4, 887, and 895.2 eV represents
Ce4? in the Ce 3d5/2 spin–orbit split doublet. Corre-
spondingly, peaks at 899.6, 905.3, and 913.7 eV represent
Ce4?, while the peaks at 903.1 and 897.4 eV represent
Ce3? in the Ce 3d3/2 spin–orbit split doublet [31].
The Ti 2p3/2 peak was well fitted into the peaks of Ti4?.
From Fig. 2b, it can be seen that the Ti 2p3/2 spectra of
CTN-06 had an significant peak at 456.12 eV representing
Ti4?. The peaks at 461.86 eV represented Ti 2p1/2 peak.
Figure 2c shows the O 1s XPS spectra of the CTN-06
catalysts. Generally, the surface oxygen can be classified as
two types: the lattice oxygen (OI) and the chemisorbed
oxygen (OII) [31, 37, 38], which plays an important role in
the catalytic reaction. Furthermore, the oxygen in the gas or
that absorbed on the catalysts could easily exchange with
the chemisorbed oxygen. As shown in Fig. 2c, two peaks at
527.4 and 529.4 eV were observed on the CTN-06 catalyst,
which could be attributed to the OI type (527.4 eV) and OII
type (529.4 eV) oxygen on catalyst surface [31, 37, 38].
XPS reveals that the coexistence of Ce3?/Ce4? and N3-
results in charge imbalance leading to oxygen vacancies
and unsaturated chemical bonds that result in chemisorbed
oxygen on the catalyst surface. It could be seen from
Fig. 2d that the broad N 1s peak was found at 396–400 eV,
indicating nitrogen incorporation in the TiO2 lattice. The
broad XPS peak observed at 396–400 eV for the CTN-06
particles can be attributed to the substitutional O–Ti–N
sites in the TiO2 lattice [39–41]. The complete XPS spec-
trum of CTN-06 is shown in Fig. 2e.
3.3 UV–visible diffused reflectance spectral studies
for metal–metal charge transformation
The optical absorbance spectra of ST, CTN-03, CTN-06
and CTN-09 were measured in the UV–vis region and
shown in Fig. 3a. It shows that ST sample absorbs mostly
UV light, while all the prepared CTN-03, CTN-06 and
CTN-09 show absorbance in the region of 400–450 nm, the
absorbance increases with dopant concentration. The band
gap of the samples was determined from the bang edge [42]
as well as based on the Tauc plot. The respective calculated
band gap values are summarized in the Table 1. The co-
doping with nitrogen and cerium induces the narrowing of
the band gap of TiO2. In the metal ion-substituted TiO2, the
overlap of the conduction band due to Ti (d orbital) of TiO2
and the cerium (f orbital) orbital of the implanted cerium
ions could decrease the band gap of TiO2 to absorb visible
light (as shown in Scheme 1) [43].
Furthermore, nitrogen doping can form new states that
lie just above the valence band for the substitutional
nitrogen. This decreases the band gap of TiO2 and absorbs
200 300 400 500 600 700 800
1.6
1.4
1.2
1.0
0.8
0.4
0.2
Abs
orba
nce
(a.u
)
a
CTN-09
CTN-06
CTN-03
ST
Wavelength (nm)
0.6
750 1500 2250 3000 3750
b
Tra
nsm
itta
nce
(%)
Wavenumber (cm-1)
CTN-09
CTN-06
CTN-03
ST
1120
1424
16302853
29243438
Fig. 3 a UV–visible DRS absorption spectra and b FTIR spectra of
ST, CTN-03, CTN-06, CTN-09 samples
J Sol-Gel Sci Technol
123
the visible light (as shown in Scheme 1). Therefore,
nitrogen and cerium ion doping induces the formation of
new states close to the valence band and conduction band,
respectively. The interaction of the nitrogen and cerium ion
leads to the narrowing of the band gap and enhances the
photocatalytic activity in the visible light region. The shift
of the absorption edge in Ce3?/Ce4? and N3- doped titania
is due to the charge-transfer between the cerium ion
4f electrons and the TiO2 conduction or valence band
(tracks 1–6 in Scheme 1) [44, 45].
The absorbance of CTN-09 sample in the visible light
region is highest among these samples because the Ce3?
ion possesses an optically-active electron in the 4f orbital,
which have excited states of 4f7/2 and 4f5/2. The light
absorption in visible region cannot be due to 4f–4f transi-
tions because these 4f–4f transitions should be observed in
the infrared spectral region [46]. Thus the red shift of the
doped samples is attributed to the electron that can be
excited from the (1) valence band of Ce–TiO2-xNx into the
Ce 4f level (track 4 in Scheme 1) (2) ground state of CeO2
into the Ce 4f level (track 5 in Scheme 1) [47].
The UV–vis diffused reflectance spectrum of Ce–
TiO2-xNx exhibits the absorption that extends from the UV
to visible region (Fig. 3a). Since neither Ce3? nor the Ti4?
ion possess the 4f ? 5d transition in the spectral region,
the visible region absorption is due to the MMCT of Ti/Ce
assemblies i.e., Ti4?/Ce3? ? Ti3?/Ce4? [16, 47]. The
bimetallic Ti/Ce assembly shows intense MMCT absorp-
tion that can activate the catalyst (track 9 and 10 in
Scheme 1) [16].
The availability of charge is the sum of the detrapped
electrons and the conduction band electrons [48]. The
electrons in the Ce–TiO2-xNx increased indicating
increased electron injection from the Ce–TiO2-xNx con-
duction band. The charge density in the Ce–TiO2-xNx is
much smaller than the pure ST. Thus the charge transport
resistance of Ce–TiO2-xNx is higher due to the strong
recombination in Ti4?/Ce3? ? Ti3?/Ce4?. The increase of
the capacitance of Ce–TiO2-xNx indicates the enhance-
ment of the capability to accept or release electrons due to
the enhanced electron injection from the Ce4?. Ce4? trap
states grab the injected electrons from Ti3? and block the
interface recombination (track 6, 7, 8, 9 and 10). Ti3? trap
states in TiO2 determine the electron transport and result in
the suppression of interface recombination. The catalytic
activity is determined not only by the oxygen storage
capability but also the rate of the redox activity (MMCT
and interfacial charge transfer). Poor dispersion of ceria on
the surface of TiO2 as well as the transformation of Ce3?
and Ce4? lead directly to the disappearance of oxygen
vacancies in ceria particles. This slows down the reduction
rate of ceria and decreases its rate of degradation (oxida-
tion/reduction) in case of Ce–TiO2-xNx.
3.4 FTIR, SEM and EDX analysis
FT-IR of the ST, CTN-03, CTN-06 and CTN-09 were
analyzed and are shown in the Fig. 3b. All samples show a
relatively strong band at 1,630 cm-1, attributed to the O–H
bending vibration of chemisorbed/physisorbed H2O mole-
cule on the catalyst surface [49]. The peaks at
*3,600 cm-1 are attributed to the Ti–OH bond [31, 49].
The new peak at 1,120, 1,424 cm-1 was clearly observed
for cerium and nitrogen doped samples. This is due to the
bending vibration mode of the N–H bond [50] and this is
apparent because the intensity of the N–Ti absorption peak
increases with the increase in nitrogen concentration. The
peaks at 1,450 cm-1 correspond to N–Ti–N stretching and
N–Ti bending vibrations and are observed in all the doped
samples. FTIR shows that the N–Ti stretching and bending
Scheme 1 Schematic
illustration of interfacial charge
transfer between Ce3?–
TiO2-xNx and Ce2O3 and
Metal–metal charge transfer
between Ti3? and Ce4?
mechanism (highlighted) in
valence band structure of Ce3?–
TiO2-xNx and Ce2O3, the
mechanisms of photoresponse
under visible light and
photogenerated electron transfer
J Sol-Gel Sci Technol
123
vibration peaks were prominent and confirm the incorpo-
ration of nitrogen in the TiO2. The broad peak around
600 cm-1 was ascribed to the absorption bands of Ti–O/
Ce–O and O–Ti–O/O–Ce–O with no indication of Ce–O
bond vibration [51]. The increase in concentration of cer-
ium oxide species is due to expected competition between
the Ce and N with the hydroxyl group and accounts for the
difference in electronegativity of the supports. A sub
Fig. 4 SEM images of a ST, b CTN-03, c CTN-06, d CTN-09, and e EDX spectra of CTN-06
J Sol-Gel Sci Technol
123
monolayer of oxide is formed at similar electronegativity
values but a multilayer is formed when the latter values are
between Ti and Ce.
FESEM images of ST, CTN-03, CTN-06 and CTN-09
samples are shown in Fig. 4a–d. The morphology of the
sample prepared with water is made of many agglomera-
tions of smaller crystallites. The smaller crystallite sizes
are due to cerium ion, which are less reactive than the
titania precursor species. This retards the condensation and
crystallization and is consistent with the values obtained in
PXRD. The images clearly indicate that the particle was
homogeneous with agglomerates and agglomeration was
reduced in ST. The diameter of the particles was about
40–100 nm. These smaller crystallites are closely packed
in each particle, which reduces the porosity within each
agglomerated assembly. Figure 4e shows the EDX spectra
of CTN-06 samples, which confirm the doping of ceria and
nitrogen in the samples. The Ti:Ce ratio of the samples are
given in Table 1.
3.5 Mechanism for interfacial charge transformation
for the photocatalytic degradation
The projected contribution to the energy levels from O
(2s22p4), Ti (3s23p63d24s2), Ce (4f15d16s2) and N (2s22p3)
are given in Scheme 1. It is found that the valence band is
mainly composed of O 2p electric states strongly hybrid-
ized with Ti 3d and Ce 4f. The conduction band (CB) is
determined by the Ti 3d and Ce 4f. The CB is determined
by the Ti 3d electronic states strongly hybridized with O
2p. The energy level of introduced Ce is mainly composed
of Ce 4f and Ce 5d electronic states, hybridized with O
2p corresponding to Ce2O3. Other hybridized states are
valence band (VB) composed of N 2p electronic states
hybridized with Ti 3d and Ce 4f. The CB originates from Ti
3d cubic states hybridized with N 2p. The DRS (Sect. 3.3)
results demonstrated that while ST had no absorption in the
visible region ([400 nm), CTN had significant absorption
between 400 and 500 nm, which increased with increase of
cerium ion content. The absorption in the visible region has
been observed for Ce3?-doped Y2O3, Lu2O3, ZrO2 or
La2O3 wherein the onset of the absorption of Ce3? was
around 460 nm [51, 52]. CeO2 is an n-type semiconductor
with a band gap of about 3.2 eV [53, 54] and the absorption
at 400–500 nm by the CTN catalysts is not due to CeO2 but
because of Ce2O3 (as shown in Scheme 1).
Ce3? ion possesses a single optically active electron
with the ground state configuration in the 4f1 orbital. There
are only two electronic levels, an excited state of 2F7/2 and
a ground state of 2F5/2, in this configuration. The 4f–
4f transitions attributed to Ce3? can be observed only in the
infrared spectral region. However, Ce3? has the first state
configuration 5d1 that is rather close in energy. The
electronic dipole transitions 4f1$ 5d1 may occur in either
UV or visible region (track 1 and 2 in the Scheme 1).
Based on the valence band of Ce3?–TiO2-xNx from
XPS, electron–hole pairs could be generated in both types
of catalysts: Ce3?–TiO2-xNx and Ce2O3 in three ways
(Scheme 1). An electron can be excited from the (a)
valence band of Ce3?–TiO2-xNx into Ti3? defect level
(track 3 in Scheme 1), (b) valence band of Ce3?–TiO2-xNx
into Ce 4f level (track 4 in the Scheme 1) and (c) ground
state of Ce2O3 into Ce 4f level (track 5 in the Scheme 1).
Therefore, the red shift of absorption edge for Ce3?–
TiO2-xNx was expressed in the following Eqs. (1) and (2).
The Ce 4f levels play an important role in generating
electron–hole pairs.
Ce3þ�TiO2�xNx þ hv! e� þ hþ ð1Þ
Ce2O3�!hv
e� þ hþ ð2Þ
The charge transfer (metal-to-metal and interfacial) is the
rate determining step for photocatalytic reaction [55].
In this investigation, the PL emission spectra of catalysts
were investigated to determine the separation efficiency of
charge carriers. To enhance the photocatalytic activity, it is
critical to separate the photo generated electrons and holes
efficiently. The PL emission spectra of all samples were
examined in the range of 400–700 nm, and shown in
Fig. 5. It can be seen that the PL intensity of ST was sig-
nificantly higher than that of CTN samples. The lower PL
intensity of modified ST may be attributed to the efficient
capture of charge carriers by the energy levels of surface
states related to N–O species. The lower intensity for the
modified indicated a lower recombination rate. Hence, the
PL results imply the co-modified of Ce and N can effi-
ciently accelerate the separation of charge carriers.
For CTN, the Ce 4f level plays an important role in
interfacial charge transfer and elimination of electron–hole
Inte
nsit
y (a
.u)
CNT-09
CNT-06
CNT-03
ST
700650600550500450400
Wavelength in nm
Fig. 5 Photoluminescence spectra of ST and Ce–TiO2-xNX samples
J Sol-Gel Sci Technol
123
recombination. Cerium ions are superior to the oxygen
molecule in their ability to trap CB electrons of TiO2 (track
7 and 8 in the Scheme 1) [56, 57]. The electrons trapped in
Ce4?/Ce3? site are then transferred to the surrounding
adsorbed O2. Therefore, presence of Ce4? on TiO2 surface
may promote the processes indicated by Eqs. (3) and (4).
Equation (5) indicates the formation of OH�.
For CTN, the formation of labile oxygen vacancies and
particularly the relatively high mobility of bulk oxygen
species have been reported [57]. Below the conduction
band edge of TiO2 as defect levels of Ti3? (Scheme 1),
ceria had a high oxygen transport and storage capacity [58]
and thus the excited electrons can be easily transferred to
O2 on the surface of CTN catalysts.
Ce4þ þ TiO2ðe�Þ ! Ce3þ þ TiO2 ð3Þ
Ce3þ þ O2 ! Ce4þ þ O�2 ð4Þ
2Hþ þ�� O2 ! 2HO � ð5Þ
Ti3? can also form a defect level and act as hole-traps to
promote charge transfer (track 6 in Scheme 1). These
defects on the surface of titania can suppress the recombi-
nation of electron–hole pairs. The mechanism of interfacial
charge transfer [59, 60] can be expressed in Eqs. (6) and (7).
Ti4þ � O�Hþ e� ! Ti3þ � O�H ð6Þ
Ti3þ � O�Hþ hþ ! Ti4þ � �O�H ð7Þ
However, to certain degree, the higher content of Ti3? on
the CTN-03 and CTN-06 surface compared to that of TiO2
results in better interfacial charge transfer and superior
photocatalytic activity.
The photocatalytic activity of Ce–TiO2-xNx and P25
(used as a comparison) was evaluated (Fig. 6a, b) by
degradation of MB and MV as a model compound under
visible light. The photocatalytic properties of all the sam-
ples was in the following order; CTN-06 [ CTN-
03 [ CTN-09 [ ST [ P25. The photocatalytic degrada-
tion of MB and MV were fitted with first order kinetics
(log(C/C0) = kt), C is the concentration in the solution
after irradiation for time t and C0 is the initial concentra-
tion. The kinetics of degradation of MB and MV can be
expressed by Langmuir–Hinshelwood model. The kinetic
rate coefficient (k) values of CTN-06, CTN-03, CTN-09,
ST, P25 were calculated to be 0.0174, 0.0161, 0.0095,
0.0082, 0.0017 and 0.0454, 0.0278, 0.0242, 0.0183,
0.0005 min-1 for the MB and MV dyes respectively.
CTN-06 exhibits highest photocatalytic activity than pure
ST and P25, which is due to the narrow band gap [61] higher
surface area, interfacial charge transfer and MMCT. The
sample with higher concentration of Ce and N shows a lower
degradation rate of the dyes. This is due to defects on the
surface of Ce–TiO2-xNx that act as excess recombination
centers of photo induced electron–hole pairs [61]. As a result,
it leads to the decrease of photocatalytic activity.
Ce3? is incorporated to the system and this is considered
more effective than other lanthanides due to the 4f–
5d transition. Its Fermi energy level is very close to the
conduction band edge of TiO2. This contributes to the
accelerating the flow of electrons in the phenomenon of
interface charge transfer and MMCT within the Ce–
TiO2-xNx. For CTN-06, we can clearly observe that the
photocatalytic activity improved and the degradation effi-
ciency was 70 and 90 % for MB and MV dyes, respec-
tively. Therefore, the higher degradation rates of the dyes
in the presence of CTN-06 compared to other modified
materials is likely due to the synergistic effect of Ce and N
in addition to the interfacial charge transfer and MMCT.
4 Conclusions
The existence of cerium ion in ?3 or ?4 state, and nitrogen
in -3 state support the Ce–TiO2-xNx particles and provide
-40 -20 0 20 40 600.0
0.2
0.4
0.6
0.8
1.0
C/C
0C
/C0
Time (min)
WC DP25 ST CTN-03 CTN-06 CTN-09
a
-10 0 10 20 30 40 50 60 700.0
0.2
0.4
0.6
0.8
1.0
Time (min)
WC DP25 ST CTN-03 CTN-06 CTN-09
b
Fig. 6 Variation of normalized concentration with time for the
photocatalytic degradation of a MB and b MV by CTN-03, CTN-06,
CTN-09, DP25 and ST photocatalysts in the presence of visible light
J Sol-Gel Sci Technol
123
highly active sites for the degradation of dyes at the
periphery of the Ce–O–Ti interface. UV–visible DRS
studies shows that the MMCT of Ti4?/Ce3? ? Ti3?/Ce4?
and electron–hole pair separation between two interfaces of
Ce–TiO2-xNx and Ce2O3 are responsible for the visible
light activity. The degradation kinetics of two dyes, MB
and MV, in the presence of Ce–TiO2-xNx exhibited sig-
nificantly high visible light activity compared to commer-
cial Degussa P25.
Acknowledgments Authors thank to University Grants Commis-
sion (UGC), RKE thanks UGC for awarding Dr. D. S. Kothari Post
Doctoral Fellowship.
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