nitrogen-containing tio2 photocatalysts

8
Nitrogen-containing TiO 2 photocatalysts Part 1. Synthesis and solid characterization C. Belver a , R. Bellod a , A. Fuerte b , M. Ferna ´ndez-Garcı ´a a, * a Instituto de Cata ´lisis y Petroleoquı ´mica, CSIC, Campus Cantoblanco, 28049 Madrid, Spain b Departamento de Energı ´a, CIEMAT, Av. Complutense, 28040 Madrid, Spain Available online 11 April 2006 Abstract A series of N-substituted Ti isopropoxide precursors were synthesized by using three different amine-type ligands. The resulting Ti-complexes were characterized by nuclear magnetic resonance (NMR) and used to obtain solid precipitates by a reverse microemulsion method. These N-rich solid precipitates were subjected to three calcination treatments differing in the gas atmosphere allowed to contact the solid, yielding nanosized materials. A thermogravimetric analysis of the solid precipitates, combined with a mass spectrometry/infrared study of the evolving gaseous products, were able to show the influence of preparation parameters, e.g. Ti-precursor nature and treatment conditions, in the decomposition process of the solid precursors and the formation of the final nanoparticulated solid catalysts. Both parameters affect the interaction between solid oxygen species (O 2 ; OH ) and N,C-containing fragments present in the solid precursors. The chemical (e.g. nitrogen content), structural (phase, cell parameters and volume, and defect structure) and morphological (BET area and primary particle size) properties of the catalytic final solids were studied as a function of the preparation conditions. # 2006 Elsevier B.V. All rights reserved. Keywords: Photocatalysis; Microemulsion method; NMR; TG-MS; DRIFTS; TiO 2 anatase materials; N-doping and impurity; Visible light absorption; Pollutant mineralization and degradation 1. Introduction Photocatalytic destruction of organic pollutants in the presence of TiO 2 appears as a viable decontamination process of widespread application, no matter the state (gas or liquid) or chemical nature of the process target [1,2]. However, its technological application seems limited by several factors, among which the most restrictive one is the need of using an ultraviolet (UV) excitation source. The efficient use of solar light or, in other words, of the visible region of the spectrum, may then appear as an appealing challenge for developing the future generation of photocatalytic materials [3,4]. One new approach to produce visible light activated TiO 2 photocatalysts is by doping with anions, such as N 3 ,C 4 ,S 4 or halides (F , Cl , Br ,I ) [5]. It was first suggested that these species substitute the oxygen lattice on TiO 2 and lead to a band gap narrowing, resulting in high visible absorption. Many works described the enhanced photocatalytic properties of titania by nitrogen doping [6–9], although special care must be taken with the synthesis method [10–12]. The nitrogen substitutional doping of TiO 2 is through to be a method for narrowing the band gap by changing the valence band structure without a change in the position of conduction band. Nevertheless, an open question in this way is to know how the absorption shift towards the visible part occurs. Quantum chemical calculations suggest that the narrowing of the band gap is due to a mixing of the N 2p and O 2p states [13,14], being identified the dominant transitions at the absorption edge those from N 2p P to Ti d xy , instead of from O 2p P as occurred in TiO 2 [15]. Nevertheless, Irie et al. [16] suggest that the N 2p levels are separated (not mixed) from the valence band (formed by O 2p states), forming an isolated narrow band responsible for the visible light sensitivity of the oxynitride powders. By other side, some authors point out that the N-doping of TiO 2 is rather similar in properties to impurity sensitization, inducing the formation of localized states in the band gap [17,18]. In this sense, the doped nitrogen may exist as NO-related species www.elsevier.com/locate/apcatb Applied Catalysis B: Environmental 65 (2006) 301–308 DOI of related article: 10.1016/j.apcatb.2006.02.016. * Corresponding author. Tel.: +34 91 5854939; fax: +34 91 5854760. E-mail address: [email protected] (M. Ferna ´ndez-Garcı ´a). 0926-3373/$ – see front matter # 2006 Elsevier B.V. All rights reserved. doi:10.1016/j.apcatb.2006.02.007

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Nitrogen-containing TiO2 photocatalysts

Part 1. Synthesis and solid characterization

C. Belver a, R. Bellod a, A. Fuerte b, M. Fernandez-Garcıa a,*a Instituto de Catalisis y Petroleoquımica, CSIC, Campus Cantoblanco, 28049 Madrid, Spain

b Departamento de Energıa, CIEMAT, Av. Complutense, 28040 Madrid, Spain

Available online 11 April 2006

Abstract

A series of N-substituted Ti isopropoxide precursors were synthesized by using three different amine-type ligands. The resulting Ti-complexes

were characterized by nuclear magnetic resonance (NMR) and used to obtain solid precipitates by a reverse microemulsion method. These N-rich

solid precipitates were subjected to three calcination treatments differing in the gas atmosphere allowed to contact the solid, yielding nanosized

materials. A thermogravimetric analysis of the solid precipitates, combined with a mass spectrometry/infrared study of the evolving gaseous

products, were able to show the influence of preparation parameters, e.g. Ti-precursor nature and treatment conditions, in the decomposition

process of the solid precursors and the formation of the final nanoparticulated solid catalysts. Both parameters affect the interaction between solid

oxygen species (O2�; OH�) and N,C-containing fragments present in the solid precursors. The chemical (e.g. nitrogen content), structural (phase,

cell parameters and volume, and defect structure) and morphological (BET area and primary particle size) properties of the catalytic final solids

were studied as a function of the preparation conditions.

# 2006 Elsevier B.V. All rights reserved.

Keywords: Photocatalysis; Microemulsion method; NMR; TG-MS; DRIFTS; TiO2 anatase materials; N-doping and impurity; Visible light absorption; Pollutant

mineralization and degradation

www.elsevier.com/locate/apcatb

Applied Catalysis B: Environmental 65 (2006) 301–308

1. Introduction

Photocatalytic destruction of organic pollutants in the

presence of TiO2 appears as a viable decontamination process

of widespread application, no matter the state (gas or liquid) or

chemical nature of the process target [1,2]. However, its

technological application seems limited by several factors,

among which the most restrictive one is the need of using an

ultraviolet (UV) excitation source. The efficient use of solar

light or, in other words, of the visible region of the spectrum,

may then appear as an appealing challenge for developing the

future generation of photocatalytic materials [3,4].

One new approach to produce visible light activated TiO2

photocatalysts is by doping with anions, such as N3�, C4�, S4�

or halides (F�, Cl�, Br�, I�) [5]. It was first suggested that these

species substitute the oxygen lattice on TiO2 and lead to a band

DOI of related article: 10.1016/j.apcatb.2006.02.016.

* Corresponding author. Tel.: +34 91 5854939; fax: +34 91 5854760.

E-mail address: [email protected] (M. Fernandez-Garcıa).

0926-3373/$ – see front matter # 2006 Elsevier B.V. All rights reserved.

doi:10.1016/j.apcatb.2006.02.007

gap narrowing, resulting in high visible absorption. Many

works described the enhanced photocatalytic properties of

titania by nitrogen doping [6–9], although special care must be

taken with the synthesis method [10–12]. The nitrogen

substitutional doping of TiO2 is through to be a method for

narrowing the band gap by changing the valence band structure

without a change in the position of conduction band.

Nevertheless, an open question in this way is to know how

the absorption shift towards the visible part occurs. Quantum

chemical calculations suggest that the narrowing of the band

gap is due to a mixing of the N 2p and O 2p states [13,14], being

identified the dominant transitions at the absorption edge those

from N 2pP to Ti dxy, instead of from O 2pP as occurred in TiO2

[15]. Nevertheless, Irie et al. [16] suggest that the N 2p levels

are separated (not mixed) from the valence band (formed by O

2p states), forming an isolated narrow band responsible for the

visible light sensitivity of the oxynitride powders. By other

side, some authors point out that the N-doping of TiO2 is rather

similar in properties to impurity sensitization, inducing the

formation of localized states in the band gap [17,18]. In this

sense, the doped nitrogen may exist as NO-related species

C. Belver et al. / Applied Catalysis B: Environmental 65 (2006) 301–308302

Table 1

Main synthesis details of Ti–N samples and T references

Sample/reference Ti:ligand

molecular ratio

Treatment

M1 1:1 Ar/O2 20–450 8CM2 1:1 Ar 20–200 8C; Ar/O2 200–450 8CM3 1:1 Ar 20–450 8C; Ar/O2 450 8C2M1 1:2 Ar/O2 20–450 8C2M2 1:2 Ar 20–200 8C; Ar/O2 200–450 8C2M3 1:2 Ar 20–450 8C; Ar/O2 450 8CN3 1:1 Ar 20–450 8C; Ar/O2 450 8CPh3 1:1 Ar 20–450 8C; Ar/O2 450 8CT1 – Ar/O2 20–450 8CT3 – Ar 20–450 8C; Ar/O2 450 8CTaq3 1:3 Ar 20–450 8C; Ar/O2 450 8C

which may be present alone or together with Ti–N bondings,

the former (NO-type) created by a N–O interaction where N

is close to tetrahedral-like interstitial positions and the latter

(Ti–N bond) formed by substitutional replacement of O anions

by N anions. By other side, doping with nitrogen not only

modifies the electronic properties of titania, but also can induce

the formation of oxygen-defect sites having critical influence in

catalytic activity [18,19]. Therefore, at least two types of

species could exist on Ti–N catalysts. N-doping of TiO2-based

materials affect the photocatalytic activity of TiO2-based

systems because can act as charge trapping or recombination

centers depending on their presence at the surface/bulk and

other structural/electronic details.

Here, we will describe the synthesis of N-containing TiO2-

based materials by modifying a titanium(IV) isopropoxide

precursor with a series of N-containing molecules. Three

different molecules will serve as ligands; the first one 2-

methoxyethylamine, the second N,N,N0,N0-tetramethylethyle-

nediamine and the third one 1,2-phenylenediamine. They are

able to substitute one or several propoxide ligands forming

different Ti precursors which would be utilized to obtain TiO2-

based photocatalysts by using a reverse micelle microemulsion

method. There are, to our knowledge, two recent reports using a

N-containing Ti precursor from TiCl4 to obtain Ti–N catalysts

after calcination [9,11]. However, the use of a titanium(IV)

isopropoxide may be able to eliminate a potential interference

from Cl� ions. This synthetic approach could have, on the other

hand, several advantages over those already described in the

literature and mostly based on the post-treatment of TiO2

materials with NH3 or other (like triethylamine) molecules and/

on N ion implantation [6–10,12]. These beneficial effects are

essentially related to the simultaneous potential control of the

chemical, e.g. nitrogen and associated vacancy species content,

and morphological, e.g. particle size, properties of the final

solid, allowing correct comparisons between different speci-

mens. In this paper, we will describe the synthesis method and

the resulting catalytic solids, while in the following paper (part

2), we will analyze the catalytic properties of these systems.

Apart from using three different N-containing ligands, we will

study the influence of the calcination treatment temperature and

atmosphere, as these variables have been shown to be important

in obtaining adequate photocatalytic materials (see [18] and

references cited therein).

2. Experimental

Titanium(IV) isopropoxide (Aldrich) was first subjected

to a reaction with different N-containing amine-type ligands:

2-methoxyethylamine (called M, hereafter), CH3OCH2CH2

NH2 (Aldrich); N,N,N0,N0-tetramethylethylenediamine (N),

(CH3)2NCH2CH CHCH2N(CH3)2 (Aldrich); and 1,2-pheny-

lenediamine (Ph), C6H4(NH2)2 (Aldrich). In a typical expe-

riment, the corresponding N-containing ligand was added to

a 0.05 M solution of Ti(iPrO)4 in dry isopropanol, in a Slenchk

type flask under nitrogen atmosphere. After stirring at room

temperature for 1.5 h, the solvent was evaporated, under

reduced pressure, until obtaining a concentrated solution of

the N-containing Ti precursor in isopropanol (1.9 M approxi-

mately). This solution was added dropwise to an inverse

microemulsion containing an aqueous solution dispersed in

n-heptane (10/85, v/v), using Triton X-100 (Aldrich) as

surfactant and hexanol (Aldrich) as cosurfactant [20]. The

resulting mixture was stirred for 24 h, centrifuged, rinsed with

methanol and calcined using three different treatments always

consisting on a ramp at 1 8C min�1 with 2 h plateaus at 200 and

450 8C, being the latter the final temperature of treatment.

Treatments differ in the specific point/temperature where O2

(20 vol.%) is added to the Ar, being incorporated from the

beginning (treatment called ‘‘1’’), at the onset of the first (‘‘2’’)

and second plateau (‘‘3’’). Reference samples (called T,

hereafter) were produced by using the Ti isopropoxide as

precursor. An additional reference was obtained by a post-

treatment with the N ligand of a TiO2 nanoparticle (Taq) in

order to have a comparison with samples already studied in

the literature. Table 1 summarizes the names of the samples

and references and main synthesis parameters.1H and 13C NMR spectra of N-containing Ti precursors were

taken on a Varian XR300; chemical shifts are given in ppm with

tetramethylsilane used as internal standard. Bidimensional

homonuclear (COSY) and heteronuclear (HMQC) chemical

shift correlation experiments were carried out in a Varian

INOVA-500 spectrometer. On account of the very poor

solubility of these titanium complexes in the deuterated

solvents, their 1H NMR spectra were not of sufficient quality,

and only in the case of the 2-methoxyethylamine ligand, a

reasonable signal was obtained (see below).

Chemical composition was analyzed by using inductively

coupled plasma and atomic absorption (ICP–AAS). The BET

surface areas were measured by nitrogen adsorption–desorption

isotherms at 77 K with a Micromeritics TriStar 3000 equip-

ment. XRD profiles were obtained with a Seifert diffractometer

using Ni-filtered Cu Ka radiation. Particle sizes were cal-

culated from XRD patterns using the Willianson–Hall method

which takes into account, the strain and particle size contribu-

tions to the XRD peak broadening [21]. Lattice parameters

were calculated by fitting and refining the anatase unit cell with

the help of the PLV program [22].

Thermogravimetric measurements were performed by using

a thermogravimetric-mass spectrometer (TG-MS) system

C. Belver et al. / Applied Catalysis B: Environmental 65 (2006) 301–308 303

from Perkin-Elmer TG-7. Samples were treated in He at room

temperature (RT) before subjected to a heating ramp of

10 8C min�1 from 25 to 600 8C under He or 20% O2/He

mixture. The evolving gaseous products were detected by mass

spectrometry, scanning the m/z values of 15, 16, 17, 18, 27, 28,

29, 30, 32, 39, 40, 41, 44, and 46.

The infrared analyses were carried out during the calcination

treatments described before by using a Perkin-Elmer 1725X

FTIR spectrometer, with a multiple reflection transmission cell

(Infrared Analysis Inc.), directly connected to the gaseous

effluents from the calcination reactor.

3. Results and discussion

The synthesis of the N-containing Ti precursor was

followed by NMR in the case of a Ti:M 1:1 precursor. For

comparison purposes, spectroscopic data (1H NMR and 13C

NMR) of the reactants [titanium(IV) isopropoxide and 2-

methoxyethylamine] and the Ti:M 1:1 precursor are sum-

marised in Table 2. Homonuclear (COSY) and heteronuclear

(HMQC) bidimensional NMR experiments were required to

unequivocally assign the signals to the corresponding atoms.

The differences between the chemical shift of the titanium

complex (Ti:M 1:1) and free ligand (e.g. coordination shift,

Dd = dcomplex � dligand) are also included in this Table 2. It can

be observed that all proton signals experience a low-field shift

(Dd = 0.02–0.64 ppm), being this more dramatic for protons

that are closer to the titanium atom (DdNH2>Dda >Ddb >Ddc).

This de-shielding effect is induced for the coordination of

the new ligand (methoxyethylamine) to the titanium atom.

Additionally, signals corresponding to protons in positions

Table 21H and 13C RMN data for the Ti:M 1:1 precursor

1H, d (ppm) CH2 [a] CH2 [b] CH3 [c]

Methoxyethylamine 2.85 {t, 2H, J = 6.8} 3.39 {t, 2H, J = 6.8} 3.36 {s,

Ti(iPrO)4 – – –

Ti:M 1:1 3.36 {t, 2H, J = 6.1} 3.64 {t, 2H, J = 6.1} 3.38 {s,

Dd 0.51 0.25 0.02

13C, d (ppm) CH2 [a] CH2 [b] CH

Methoxyethylamine 41.8 74.9 58

Ti(iPrO)4 – – –

Ti:M 1:1 51.3 73.0 59

Dd 9.51 �1.94 0

Deuterated solvent: CDCl3; {multiplicity, number of protons, coupling constant (J

e and d also display a small shift; the introduction of the

N-containing ligand in the structure of the titanium complex

implies that isopropoxide groups are no longer equivalent by

symmetry. The integration of signals appearing in the 1H NMR

spectrum confirms that only one isopropoxide group has been

substituted by a M group (integration; a:b:c:d:e = 2:2:3:3:18).

Similar behavior is observed in the 13C NMR spectrum, where

the coordination shifts (Dd) for different carbon atoms vary

between 0.2 and 13.2 ppm. All these facts proof that the Ti:M

1:1 titanium complex is successfully formed under our

synthesis conditions.

Although we were not able to characterize by NMR

spectroscopy the precursor state when using the N and Ph

molecules as N-containing ligands due to problems with

solubility of these compounds in the deuterared solvents,

convincing evidence of the Ti:N and Ti:Ph precursor formation

can be obtained from the TG-MS study. Fig. 1 displays the

weight loss and derivative thermograma of solid precursors/

precipitates (obtained from the corresponding microemulsions)

under He. Solid and dotted lines correspond, respectively, to

materials treated with O2/Ar at RT or at 200 8C and dried,

respectively, at RT or at 200 8C under He for treatment 2

previously to the recording stage. Samples pre-treated at higher

temperatures (450 8C) do not show appreciable mass losses.

Samples Ti:M and Ti:N show a similar behavior, displaying

peaks at 86, 233, 300, 330 and 438 8C in the derivative plot

while Ti:Ph only shows a weak contribution around 86 8C,

mostly ascribable to water/CO2 evolution according to MS (see

below). Precursor Ti:M is affected by the pre-treatment at

200 8C, losing the peaks evolving at temperature below or near

200 8C with respect to its counterpart pre-treated at RT. This

CH [d] CH3 [e] NH2

3H} – – 1.38 {s, 2H}

4.47 {septet, 4H, J = 6.1} 1.23 {d, 24H, J = 6.1} –

3H} 4.92–4.50 {m, 3H} 1.58–1.12 {m, 18H} 2.02 {s, 2H}

�0.24 �0.12 0.64

3 [c] CH [d] CH3 [e] NH2

.7 – – –

64.0 25.3 –

.0 78.3–76.3 25.6–24.4 –

.28 �13.2 ��0.2

, Hz)}.

C. Belver et al. / Applied Catalysis B: Environmental 65 (2006) 301–308304

Fig. 1. Thermogravimetric analyses for indicated precursors: (A) percentage of weight loss; (B) derivative thermograma. Solid and dotted lines correspond,

respectively, to materials treated in O2/Ar at RT or at 200 8C and dried for 2 h under He previously to the recording stage. See text for details.

accounts for ca. 5% of its initial weight. Surprisingly, an almost

complete absence of contributions with a main peak at ca. 86 8Ccan be observed for Ti:N after pre-treatment at 200 8C. The

Ti:Ph precursors display a behavior only weakly dependent on

the pre-treatment, with weak contributions at 86 and 330 8C.

The proof that the N-containing Ti precursors are formed

can be extracted from the strong similarities detected in the

evolving gaseous products detected by MS for solid precursors

treated at RT. In Fig. 2A, we depicted the 30 and 46 m/z signals

which due to its parallel behavior for each material are mostly

associated to NO and NO2 desorption (the m/z 30 secondary

contribution has been eliminated from the plot). The thermal

evolution of these species displays strong similarities among

our three precursors, with the sharing of peaks at ca. 220, 250,

300 and 350 8C. Owing that the Ti:M 1:1 complex is known to

be formed by NMR, this would indicate that the N-containing

Ti precursor is obtained to a certain extent in all cases. The

NO + NO2 signal intensity roughly shows the expected ratio for

the Ti:M and Ti:N precursors, indicating the similar 1:1

Ti:ligand molecular ratio reached in both cases and that Ti–M,

Ti–N bonds are not hydrolyzed in the microemulsion media

during the preparation procedure. We could thus speculate that

the Ti precursor has four ligands with presence of one N-

containing molecule in both cases, being tetra-coordinated in

the M case (NMR result) but five-coordinated in the N case. For

Ti:Ph we found, however, rather weak contributions, indicating

the failing of the precursor synthesis and/or a significant

hydrolysis of Ti–Ph bonds at the microemulsion media. Still

some residual Ti–N bonds are present in the Ti precursor.

The decomposition route of the solid precursors can be

analyzed by using the MS spectra showed in Fig. 2. In addition

to the NO/NO2 contributions (Fig. 2A), in Fig. 2B, C and D, we

plotted the evolution of the 16 (B), 28, 44 (C), and 40 (D) m/z

signals. Fig. 2B profile is assigned to ammonia fragment

evolution and again indicate the strong similarities displayed in

the decomposition of solid precursors coming from Ti:M and

Ti:N precursors. Ammonia is desorbed from the sample in

essentially the same range of NO-containing molecules,

indicating a common intermediate in the process. This will

be further discussed below by using IR data. Main products of

the treatments are H2O and CO-containing molecules. Fig. 2C

displays a strong similarity between the 28 and 44 m/z signals

indicating that CO and CO2 are the main desorption products

associated (the m/z 28 secondary contribution has been

eliminated from the plot). An alternative assignment to a N2/

N2O couple seems less likely as the N-coupling reactions

demands for the presence of atomic nitrogen, hardly created in

the temperature ramp treatment. Differences between the Ti:M

and Ti:N solid precursors concern the significantly lower CO2

quantity desorbed in the former case, leading to a higher

CO:CO2 ratio. Apart from that, 39, 40 and 41 m/z values give

evidence of the evolution of C3 (C3H8, C3H6, C3H4) and C2

(CH2CN) hydrocarbon (HC) chains. Presence of relatively

weak signals at 27 and 29 m/z values favors the assignment to

propine or C2 products, giving rise to the main signal at m/z 40

(Fig. 2D). However, a number of C3 and C2 HC compounds

seems to be formed in variable quantities in both cases, the Ti:M

and Ti:N solid precursors. Concerning the Ti:Ph decomposi-

tion, apart from the overall lower magnitude, we found practical

absence of ammonia and HC chains in the desorption products.

With these data, it can be envisaged a similar pathway for the M

and N thermal breaking which releases C2/C3 and ammonia/

NO fragments, suggesting the breaking of the molecules by

both C–C and C–N bonds. C–N bond seems to break at lower

temperature than C–C ones (Fig. 2A and D). In any case, this

may leave different C,N fragments at the solid after

calcinations, as will be shown in part 2. Assuming that the

CO:CO2 ratio differences are mainly associated with the

burning of the N-containing ligand, we may also suggest a

significantly higher involvement of O anions coming from the

Ti-oxo-hydroxide solid precursor through the treatment and a

higher number of (anion) vacancies for catalysts (final solid)

C. Belver et al. / Applied Catalysis B: Environmental 65 (2006) 301–308 305

Fig. 2. MS signals detected in the evolving gaseous products for Ti:M, Ti:N and Ti:Ph solid precursors pre-treated at RT: (A) 30, 46 m/z signals; (B) 16 m/z signal; (C)

28, 44 m/z signals; and (D) 40 m/z signal. Vertical lines are plotted to facilitate comparison among samples.

obtained from the Ti:N precursor. Finally, the Ti:Ph precursor

seems too voluminous to be present in significant quantities at

the solid precursor, although, as mentioned, we found evidence

of N-containing fragments during the TG-MS experiment.

The treatment in O2/Ar at 200 8C gives precursors having

similar decomposition behaviors as those illustrated in Fig. 2

expect for the smaller amount of CO2 detected as product for all

precursors. An obvious difference with corresponding N-

containing Ti precursors pre-treated at RT is visible in Fig. 1;

the Ti:N precursor is more sensitive to the pre-treatment than

Ti:M and Ti:Ph precursors, being the latter rather insensitive. It

thus appears that the N-containing ligand already evolves under

the treatment in the former case, a fact which may be predicted

by the strong NO and CO2 signals displayed at low temperature

by this sample with respect to the others in Fig. 2. So, although

the N and M precursors may evolve similarly under continuous

thermal treatments, it appears that a plateau at 200 8C may

enhance differences between final solids.

The decomposition process was also studied by infrared

spectroscopy (Fig. 3) comparing the different calcination

processes (described in Table 1) for the Ti:M solid precursor.

Data on treatment ‘‘3’’ (RT—450 8C Ar; 450 8C 2 h Ar/O2; see

Table 1) do not give additional insights concerning the

precursor decomposition described above by using TG-MS,

nevertheless complementary information was obtained from

the other two treatments (Fig. 3A and B). At the beginning of

calcinations, only a small contribution of water is detected by

infrared analysis, with absorbance in the region 1800–

1400 cm�1. When the temperature increased above 200 8C,

new bands appear in the spectra. The most significant are

centered at 3700, 3050–2950, 1390 and 1100–1000 cm�1.

Comparing their positions with different infrared databases, we

can attribute these bands to bonded O–H stretching, C–H

stretching (from CH3 or CH2 groups), CH3 or CH2 deformation

and C–O stretching frequencies, respectively [23]. The

presence of these vibrations suggests the formation of R–OH

species, mainly associated with the presence of gaseous

CH3OH (although CH3CH2OH can also contribute) [24,25].

The vibrations related to C–H bonds are also common for

alkanes, as C3H8, which presence in large quantities is,

however, not likely on the basis of the thermal analysis results.

Two narrow bands, centered at 932 and 968 cm�1, associated

with the formation of NH3 can be observed above 220 8C. In

some spectra is also possible to see the N–H stretching and NH2

C. Belver et al. / Applied Catalysis B: Environmental 65 (2006) 301–308306

Fig. 3. Infrared spectra of gaseous effluents from treatments 1 (A) and 2 (B) of the Ti:M 1:1 solid precursor. See text for details.

bending vibrations at 3336 and 1628 cm�1, respectively

(Fig. 3A) [26]. At higher temperatures, we detected CO2

(668 and 2350 cm�1) and CO (2142 cm�1) molecules [26],

which appearance suggests again the relevance of oxygen (O2�;

OH�) anions from the Ti-oxo-hydroxide in the calcination

process. The detection of these species at higher temperature

indicates that the decomposition of the Ti:M precursor begins

with the breaking of the C–N and RO–C bonds, corroborating/

completing the results obtained by thermal analysis.

The infrared spectra suffer small changes when the

temperature reaches 300 8C. A new band appears centered at

1745 cm�1 which can be related to a C O stretching frequency.

Comparing the location of this band with different carbonyl

compounds, we can suggest the detection of saturated esters,

which C O spectral region are centered at 1750–1735 cm�1. A

detailed analysis of the bands observed in the spectra indicates

the detection of methyl acetate (CH3COOCH3) with small

bands at 2960 (nas CH3), 1440 (ns CH3), 1366 (d CH3), 1240

(CO–O stretching) and 1040 cm�1 (O–CH2) [23]. This

molecule should give dominant mass signals at 31 and 28 m/

z values but the significant number of entities contributing to

both disallow its unambiguous detection by the MS technique.

The detection of ester compounds from 300 8C by IR

corroborates again the higher resistance of C–C bonds

compared with C–N bonds and indicates that the fragments

like those formed during the first steps of the calcination (as R–

OH) can react between them to form more complex species.

This fact also explain the small bands at 3087 and 887 cm�1

observed from 320 to 450 8C that can be due to the presence of

C3H6 (marked as (*) in Fig. 3), which detection implies the

C. Belver et al. / Applied Catalysis B: Environmental 65 (2006) 301–308 307

Fig. 4. XRD diffractograms for the Ti–N samples and T references indicated.

Table 4

XRD-derived anatase-type lattice parameters (a, c) and volume (V) and primary

particle size (t) of Ti–N samples and T references

Sample/reference a (A) c (A) V (A3) t (nm)a

M1 3.781 � 0.009 9.43 � 0.03 134.9 � 0.7 13.5

M2 3.78 � 0.04 9.46 � 0.01 135.8 � 0.3 10.1

M3 3.792 � 0.007 9.48 � 0.03 136.4 � 0.5 10.0

2M1 3.80 � 0.01 9.50 � 0.04 137.2 � 0.7 13.1

2M2 3.788 � 0.008 9.47 � 0.02 135.9 � 0.4 13.7

2M3 3.793 � 0.03 9.48 � 0.01 136.4 � 0.6 8.3

N3 3.78 � 0.02 9.48 � 0.06 135.7 � 0.1 30.3

Ph3 3.786 � 0.004 9.48 � 0.02 136.0 � 0.3 12.8

T1 3.793 � 0.001 9.486 � 0.005 136.49 � 0.09 13.3

T3 3.791 � 0.004 9.471 � 0.004 136.2 � 0.3 10.9

Taq3 3.79 � 0.09 9.45 � 0.03 136.1 � 0.6 19.8

a Standard error 30%.

formation of C3 hydrocarbons with C C bonds. By other side,

the infrared study only identifies ammonia as nitrogen

compound formed during the amine decomposition, without

evidence of the formation of NO (1883 cm�1), NO2 (1618,

1318, 750 cm�1) or N2O (2224, 1286, 589 cm�1) [25]. This and

the existence of a common intermediate for ammonia and NO-

type species suggested by the TG-MS study would indicate that

ammonia is first formed in the degradation process and that

NO-type species are secondary products. Differences between

TG and IR results may be grounded on a different contact time

(rate of the temperature ramp) which would mainly affect

production and/or evolution of secondary products.

In brief, ‘‘1’’ and ‘‘2’’ thermal treatments studied by

infrared spectroscopy yields rather similar gaseous products

(Fig. 3A and B). The main differences between them are

related to the temperature at which the species were observed;

as an example, during the treatment 1 (Ar/O2 20–450 8C)

ammonia appears at 200 8C while for treatment 2 (Ar/O2

200–450 8C) was detected at 250 8C. Other important diffe-

rence resides in the ester compounds because the treatment

2 produces lower amount of them (the C O stretching band

only has some intensity at 300–350 8C). The increase of

Table 3

Main characterization results of Ti–N samples and T references

Sample BET area (m2 g�1)a %Nb

M1 107.8 0.05

M2 104.2 0.06

M3 61.2 0.07

2M1 106.5 0.53

2M2 100.2 0.14

2M3 68.2 0.04

N3 46.5 0.07

Ph3 63.1 0.03

T1 107.3 –

T3 74.9 –

Taq3 69.7 0.005

a Standard error � 0.5 m2 g�1.b Standard error � 0.2%.

temperatures detected in absence of O2 gas indicates a different

degree of O2�/OH� involvement in the chemical reactions

occurring during calcinations treatments. This fact suggests

again that the calcination process suffered by the solid

precursor can leave different N,C fragments and oxygen

vacancies in the final solid.

The final solids formed under the three treatments display

the exclusive presence of anatase-type phases as detected by

using XRD (Fig. 4) and Raman spectroscopy (data not shown).

The BET area and N content of the solids are summarized in

Table 3 while cell parameters and unit cell volume and primary

particle size are included in Table 4. Crystallinity of the

samples is somewhat poor except for the N3 sample and T1

reference; the latter is rather crystalline as it does not contain

N,C impurities and is calcined in oxygen from the beginning

while the former suffers a strong sintering process during

calcination, leading to the higher primary particle size observed

(Table 4). The pre-treatment influence seems to affect

morphological properties, decreasing surface area when

oxygen is not included in the treatment gas mixture, probably

due to the lost of surface OH species as could be observed in

their correspondence DRIFTS spectra (not shown), but less

affecting primary particle size. Differences in secondary

particle size and porosity are therefore evident between

treatments 1/2 and 3. The ligand nature, on the other hand,

seems to have significant influence on primary particle size,

giving increasing size in the N > Ph > M order. Main structural

properties as cell volume and parameters seem only weakly

varying in our set of samples. The N content of the samples was

rather small in all cases, independently of the precursor nature

of even the Ti:ligand molecular ratio, which is exemplified for

the M case in Table 3. The comparison with the T reference

systems would indicate that except for primary particle size,

morphological properties (BET area), main structural proper-

ties and chemical composition (N content) are not strongly

sensitive to the N-containing ligand nature or Ti:ligand

molecular ratio variables. As will be shown, strong differences

are, however, encountered in the photocatalytic properties

under sunlight excitation in terms of the N-containing Ti-ligand

precursor nature and Ti:ligand molecular ratio which can be

rationalized on the basis of the defect nature and distribution of

C. Belver et al. / Applied Catalysis B: Environmental 65 (2006) 301–308308

the different solids formed during the ‘‘calcination’’ treatments

of the solid precipitates/precursors.

4. Conclusions

Several N-containing Ti isopropoxide precursors have been

synthesized and used to obtain solid precipitates by a reverse

microemulsion method. The M and N ligands seem to allow the

production of N-rich solid precursors by maintaining Ti-ligand

bonds after hydrolysis of the isopropoxide groups in the

microemulsion media, while the failure of the synthesis method

is detected in the Ph case.

The thermal evolution of the solid precursor phases was

followed by TG, while the corresponding gas phase evolution

was analyzed by MS and IR. Overall, we detected the breaking of

C–N bonds before C–C ones for the M, N (and Ph) derived

fragments present in the solid precipitates/precursors. The

presence of oxygen in the calcinations gas mixture seems to

mainly facilitate the solid transformation, lowering the

temperatures of N (ammonia; NOx) and C (CO, CO2, HCs

and esters) containing gaseous products. So, the different

temperature (RT, 200, and 450 8C) where O2 is allowed to contact

the solid precursors modifies the interaction between solid

oxygen (O2�; OH�) species and N,C-containing fragments. The

latter is also affected by the N-containing ligand nature as

indicated by the differences encountered in the CO:CO2 ratio

detected by MS between N and M samples pre-treated in equal

conditions. Both preparation parameters (Ti precursor and

treatment conditions) will leave different C,N fragments and

oxygen vacancies in the final, catalytic solids.

The resulting solids display exclusive presence of an

anatase-type phase according to XRD/Raman results. Main

structural characteristics as cell parameters and volume are not

sensitive to both the treatment (1–3) and the N-containing

ligand nature. The treatment characteristics (1–3) seem to affect

morphological properties, decreasing surface area when

oxygen is not present in the calcinations gas mixture and

weakly affecting primary particle size, which is 10 � 2.5 nm

throughout the M/2M series of samples. The ligand nature has a

strong influence in the primary particle size, leading to an

increasing size in the N > Ph > M order. Main synthetic

variables (Ti precursor and the thermal treatment) permit

therefore to control the chemical, structural and morphological

properties of the final solids, being possible to synthesized

optimum visible response photocatalysts. Their promising

photocatalytic properties could be related to the presence of

differences in the N,C fragments and/or oxygen vacancies

formed during the synthesis process. This is the subject of part 2

of the study.

Acknowledgements

We appreciate financial support by CYCIT project

CTQ2004-03409. C.B. thanks the Spanish Ministry of

Education for a ‘‘Juan de la Cierva’’ post-doctoral grant.

References

[1] N. Serpone, E. Pelizzetti (Eds.), Photocatalysis Fundamental and Appli-

cations, Wiley, New York, 1989.

[2] M.R. Hoffmann, S.T. Martin, W. Choi, D.W. Bahnemann, Chem. Rev. 95

(1995) 69–96.

[3] C. Belver, G. Colon, M. Fernandez-Garcıa, in: M. Fernandez-Garcıa, J.A.

Rodrıguez (Eds.), Synthesis, Properties and Application of Oxide Nano-

particles, Wiley, USA (Chapter 17), 2006, in press.

[4] H. Thu, M. Karkmaz, E. Puzenat, C. Guillard, J.M. Herrmann, Res. Chem.

Intermed. 31 (2005) 449–461.

[5] J. Zhao, C. Chen, W. Ma, Top. Catal. 35 (2005) 267–278.

[6] S. Sato, Chem. Phys. Lett. 123 (1986) 126–128.

[7] J.L. Gole, J.D. Stout, C. Burda, Y. Lou, X. Chen, J. Phys. Chem. B 108

(2004) 1230–1240.

[8] Y. Sakatani, J. Nunoshige, H. Ando, K. Okusako, H. Koike, T. Takata, J.N.

Kondo, M. Hara, K. Domen, Chem. Lett. 32 (2003) 1156–1157.

[9] D. Li, H. Haneda, S. Hishita, N. Ohashi, Mater. Sci. Eng. B 117 (2005) 67–

75.

[10] C. Burda, Y. Lou, X. Chen, A.C.S. Samia, J. Stout, J.L. Gole, Nano Lett. 3

(2003) 1049–1051.

[11] T. Sano, N. Negishi, K. Koike, K. Takeuchi, S. Matsuzawa, J. Mater.

Chem. 14 (2004) 380–384.

[12] Y. Kuroda, T. Mori, K. Yagi, N. Makihata, Y. Kawahara, M. Nagao, S.

Kittaka, Langmuir 21 (2005) 8026–8034.

[13] R. Asahi, T. Morikawa, T. Ohwaki, K. Aoki, Y. Ega, Science 293 (2001)

269–271.

[14] T. Morikawa, R. Asahi, T. Ohwaki, A. Aoki, Y. Taga, Jpn. J. Appl. Phys. 40

(2001) L561–L563.

[15] R. Asahi, Y. Taga, W. Mannstadt, A.J. Freeman, Phys. Rev. 61 (2000)

7459–7465.

[16] H. Irie, Y. Watanabe, K. Hashimoto, J. Phys. Chem. B 107 (2003) 5483–

5486.

[17] S. Sato, R. Nakamura, S. Abe, Appl. Catal. A 284 (2005) 131–137.

[18] C. Di Valentin, G. Pacchioni, A. Selloni, S. Livraghi, E. Giamello, J. Phys.

Chem. B 109 (2005) 11414–11419.

[19] T. Ihara, M. Miyoshi, Y. Iriyama, O. Matsumoto, S. Sugihara, Appl. Catal.

B 42 (2003) 403–409.

[20] V. Uskokovic, M. Drofenik, Surf. Rev. Lett. 12 (2005) 239–277.

[21] G.K. Williamson, W.H. Hall, Acta Metall. 1 (1953) 22–31.

[22] J.D. Martın Ramos, PLV Program, Dep. L. M.11719, Granada, Spain,

1990.

[23] N.B. Colthup, Introduction to Infrared and Raman Spectroscopy, Aca-

demic Press, San Diego, 1990.

[24] H.L. Fang, D.M. Meister, R.L. Swofford, J. Phys. Chem. 88 (1984) 405–

409.

[25] R.H. Pierson, A.N. Fletcher, E.C. Gantz, Anal. Chem. 28 (1956) 1218–

1239.

[26] K. Nakamoto, Infrared Spectra of Inorganic and Coordination

Compounds, Wiley, New York, 1970.