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CHAPTER 1 INTRODUCTION 1.1 Literature review Titanium is the world’s fourth most abundant metal and ninth most abundant element. It was discovered in 1791 in England by Reverend William Gregor, who recognised the presence of a new element in ilmenite [1]. It was then rediscovered in rutile ore several years later by a German chemist, Heinrich Klaporth who named it after Titans, mythological first sons of the goddess Ge (earth in Greek mythology). Titanium has the symbol Ti, with atomic number 22, and atomic weight 47.90. It is placed in the fourth group of the periodic table, and its chemistry shows similarities to that of silicon and zirconium. The outer electronic arrangement is 3d24s2, and the principal valence state is IV; III, II states are also known, but are less stable. The element burns in air when heated to give the oxide, TiO2. Titanium is not found in its elemental state, it occurs mainly in minerals like rutile, ilmenite, leucoxene, anatase, brookite, perovskite and spene. It is also found in titanates and many iron ores. The metal has been detected in meteorites and stars. In fact, samples brought back from the moon by Apollo 17 contained 12.1 % TiO2. The primary source and the most stable form of titanium dioxide is rutile ore. It was discovered in Spain by Werner in 1803. Its name is derived from the Latin rutilus, red because of the deep colour observed in some specimens when the transmitted light is viewed. Rutile is one of three main polymorphs of titanium dioxide (TiO2), the other polymorphs being; anatase and brookite [2, 3]. Brookite was discovered in 1825 by A. Levy and was named after an English mineralogist, H. J. Brooke. In 1801 anatase was named by R. J. Hauy from the Greek word ‘anatasis’ meaning extension, due to its longer vertical axis compared to that of rutile. In all three forms, titanium (Ti4+) atoms are co-ordinated to six oxygen (O2-) atoms, forming TiO6 octahedra [4]. All three forms differ only in the arrangement of these octahedra. The anatase structure, is made up of corner (vertices) sharing octahedral (figure 1.1a) resulting in a tetragonal structure. In rutile the octahedra share edges to give a tetragonal structure (figure 1.1b) and in brookite both edges and corners are shared to give an orthorhombic structure (figure 1.1c)[5]. 1 (a) Anatase (b) Rutile (c)-Brookite Figure 1.1 Crystalline structures of titanium dioxide (a)-rutile, (b)-anatase, (c)brookite [6] Figure 1.2 more clearly shows the unit cell structures of the rutile and anatase TiO2 [7]. Both these structures can be described in terms of chains of TiO6 octahedra. The two crystal structures differ in the distortion of each octahedron and by the assembly pattern of the octahedra chains. In rutile, the octahedron shows a slight orthorhombic distortion; in anatase, the octahedron is significantly distorted so that its symmetry is lower than orthorhombic. The Ti-Ti distances in anatase are larger, whereas the Ti-O distances are 2 shorter than those in rutile. In the rutile structure, each octahedron is in contact with 10 neighbour octahedrons (two sharing edge oxygen pairs and eight sharing corner oxygen atoms), while, in the anatase structure, each octahedron is in contact with eight neighbours (four sharing an edge and four sharing a corner). These differences in lattice structures cause different mass densities and electronic band structures between the two forms of TiO2. Figure 1.2 Lattice structures of rutile and anatase TiO2 Titanium dioxide is an n-type semiconductor [8] that has a band gap of 3.2 eV for anatase,[9-12] 3.0 eV for rutile [13], and ~3.2 eV for brookite[14]. Titanium dioxide (TiO2) is the most widely investigated photocatalyst due to its strong oxidative properties, low cost, non-toxicity, chemical and thermal stability [15]. Anatase and rutile are the most researched polymorphs. Their properties are summarised in Table.1 and Table 1.2. In the past few decades there have been several exciting breakthroughs with respect to titanium dioxide. The first major breakthrough was in 1972 when Fujishima and Honda reported the photoelectrochemical splitting of water (2H2O → 2H2 + O2) using a TiO2 anode and a Pt counter electrode. Titanium dioxide first showed promise for the remediation of environmental pollutants in 1977 when Frank and Bard investigated the 3 reduction of CN- in water [16]. This led into an increasingly well researched area of TiO2 because of the potential implications for environmental water and air purification utilising solar energy [17]. In 1997 Wang et al reported TiO2 surfaces with excellent anti-fogging and self-cleaning abilities which were attributed to the super hydrophilic attributes of the TiO2 surfaces [18]. Table 1.1 Physical and structural properties of anatase and rutile Property Anatase Molecular weight ( g/mol) 79.88 Rutile 79.88 Melting point (°C) 1825 Boiling Point (°C) 2500 ~ 3000 2500 ~ 3000 Specific gravity 3.9 4.0 Light absorption (nm) < 390 < 415 Mohr’s Hardness 5.5 6.5-7.0 Refractive index 2.55 2.75 Dielectric constant 31 114 Crystal structure Tetragonal Tetragonal Lattice constants (Å) a = 3.78 a = 4.59 c = 9.52 c = 2.96 Density (g/cm ) 3.79 4.13 Ti–O bond length (Å) 1.94 (4) 1.95 (4) 1.98 (2) 1.98 (2) 3 Nano sized titanium dioxide was employed to excellent use in an efficient solar cell, the dye sensitised solar cell (DSSC) as reported by Graetzel and O’Regan in 1991[19]. 1.2 Anatase to rutile transformation The anatase to rutile phase transformation in TiO2 is the most studied area of scientific and technological interest [20]. The anatase to rutile transformation (ART) is kinetically defined and the reaction rate is determined by parameters such as particle shape/size 4 [21], purity [22], source effects [23], atmosphere [24] and reaction conditions [25]. It is agreed that the mechanism for phase transformation of titania is one of nucleation and growth [26]. Anatase nanocrystals coarsen, grow and then transform to rutile only when a critical size is reached [27]. Therefore, phase transformation is dominated by effects such as defect concentration [28], grain boundary concentration [29], and particle packing [30]. Table 1.2 X-Ray Data on TiO2 modifications (Clark, 1968: 268) Titania Space group Z Phase Cell parameters A a Anatase C4h= C4/ amc 8 3.784 Brookite D2h= Pbca 8 9.51 Rutile D4h= P42/mnm 2 4.593 b 5.44 Ti-O c ( A)b 9.515 1.934 (4), 1.98 (2) 4.593 1.84-2.03 2.959 1.94(4), 1.98(2) Rutile is the thermodynamically most stable phase, while anatase and brookite are both metastable, transferring to rutile under heat treatment at temperatures typically ranging from 873 to 973 K [2]. Anatase is widely regarded as the most photocatalytically active of the three crystalline structures [31-33]. The generally accepted theory of phase transformation is that two Ti–O bonds break in the anatase structure, allowing rearrangement of the Ti–O octahedra, which leads to a smaller volume, forming a dense rutile phase [34]. The removal of oxygen ions, which generate lattice vacancies, accelerates the transformation. The transition follows first order kinetics; with activation energy of ~ 418 k J mol-1[22]. The breaking of these bonds can be affected by a number of factors, including the addition of dopants, synthesis method and thermal treatment. 1.3 Electronic Structure of a Semiconductor When molecular orbitals are formed from two atoms, each type of atomic orbital gives rise to two molecular orbitals. When N atoms are used, N molecular orbitals are formed. In solids, N is very large, resulting in a large number of orbitals [35]. The overlap of a large number of orbitals leads to molecular orbitals that are closely spaced in energy and so form a virtually continuous band (figure 1.3) [36]. The overlap of the lowest 5 unoccupied molecular orbitals (LUMO) results in the formation of a conduction band and a valence band is formed from overlapping the highest occupied molecular orbitals (HOMO). The band separation is known as the band gap (Eg), a region devoid of energy levels. From the illustration shown in figure 1.3, the reduction in the band gap size with the formation of bands can clearly be seen. Figure 1.3 Change in the electronic structure of a semiconductor compound with increasing number of monomer units [37] If a band is formed from the molecular overlap of s orbitals it is called an s band and likewise, an overlap of p orbitals, forms a p band and an overlap of d orbitals will give a d band. Typically, p orbitals have higher energy than s orbitals, resulting in a band gap. However, if the s and p bands are of similar energy, then the two bands overlap [38]. In titanium dioxide, the valence band consists of oxygen 2 p orbitals and the conduction band is made up from the titanium 3 d orbitals [12]. The band gap of TiO2 anatase is 3.2 eV and rutile is 3.0 eV corresponding to an absorbance threshold, λ = 388 and 415 nm respectively. Figure 1.4 shows the various band positions of different semiconductors. For a semiconductor to be capable of producing hydroxyl radicals, the potential of the valence band must be greater than the potential of OH•. From figure 1.4 it can be seen that ZnO, TiO2, WO3 and SnO2 have the potential to produce hydroxyl radicals. 6 Figure 1.4 Band positions of various semiconductors and relevant redox couples Titanium dioxide is regarded as an n-type semiconductor due to the presence of oxygen vacancies in the lattice. These vacancies are formed upon the release of two electrons and molecular oxygen leaving a positive (+2) oxide ion vacancy [2]. When electrons of energy lower than the conduction band are present, the result is an n-type semiconductor (figure 1.5a). Alternatively if a material is added with fewer electrons than the host, positive holes are added above the valence band resulting in a p-type semiconductor (figure 1.5b). (a) (b) Figure 1.5 Semiconductors, n-type (a), p-type (b) 7 1.4 A brief study of TiO2 as photo catalyst Photo catalytic degradation of organic compounds on semiconductor surfaces is an important area of current research with respect to both fundamental understanding [39] and potential practical applications [40]. Several simple oxide and sulfide semiconductors have band-gap energies sufficient for promoting or catalysing a wide range of chemical reactions of environmental interest. The primary criterion for good semiconductor photocatalysts for organic compound degradation is that the redox potential of the H2O/·OH (OH- = ·OH + e-; Eº= -2.8 V) couple lies within the band gap domain of the material (photocatalysts) and that the material is stable over prolonged periods of time. Among the semiconductors TiO2 (Eg = 3.2 eV), WO3 (Eg = 2.8 eV), SrTiO3 (Eg= 3.2 eV), a-Fe2O3 (Eg = 3.1 eV), ZnO (Eg = 3.2 eV), and ZnS (Eg = 3.6 eV) [41], TiO2 is the most promising, low-cost, robust photocatalyst and extensively investigated material. Semiconductor photocatalysis with a primary focus on TiO2 as a durable photocatalyst has been applied to a variety of problems of environmental interest in addition to water and air purification, for the destruction of microorganisms [42], for the inactivation of cancer ce11s [43], for the photo splitting of water to produce hydrogen gas [44], and for the clean-up of oil spills [45]. In the light of solid-state physics, semiconductors (and insulators) are defined as solids in which at 0 K (and without excitations) the uppermost band of occupied electron energy states is completely filled up with electrons. It is well-known from solid-state physics that electrical conduction in solids occurs only via electrons in partially-filled bands, so conduction in pure semiconductors occurs only when electrons have been excited--thermally, optically, etc.--into higher unfilled bands. At room temperature, a proportion (generally very small, but not negligible) of electrons in a semiconductor have been thermally excited from the "valence band," the band filled at 0 K, to the "conduction band," the next higher band. The ease with which electrons can be excited from the valence band to the conduction band depends on the energy gap between the bands, and it is the size of this energy band gap that serves as an arbitrary dividing line between semiconductors and insulators. Generally, semiconductors are defined as materials with band gap less than 4 eV at room temperature. Semiconductor electronic structures are characterized by a filled valence band (VB), and an empty conduction band (CB). When a photon with energy of hv 8 matches or exceeds the band gap energy (Eg) of the semiconductor, an electron (ecb-), is promoted from the valence band, into the conduction band, leaving a hole (hvb+) behind. Excited state conduction-band electrons and valence-band holes can react with electron donors and electron acceptors adsorbed on the semiconductor surface or within the surrounding electrical double layer of the charged particles or recombine and dissipate the input energy as heat; get trapped in metastable surface states. The above process in the photocatalysis is illustrated in Figure 1.6. Figure 1.6 Schematic photo excitation in a solid followed by de-excitation events [7] Once excitation occurs across the band gap there should be a sufficient lifetime (in the nanosecond regime) for the created electron-hole pair to undergo charge transfer to adsorbed species on the semiconductor surface from solution or gas phase contact. If the semiconductor remains intact and the charge transfer to the adsorbed species is continuous and exothermic the process is termed heterogeneous photocatalysis [46]. The initial process for heterogeneous photocatalysis of organic and inorganic compounds by semiconductors is the generation of electron-hole pairs in the semiconductor particles. Upon excitation, the fate of the separated electron and hole can follow several pathways. Recombination of the separated electron and hole can occur at the surface (pathway A) in the volume of the semiconductor particle (pathway B) or with the release of heat. The photo induced electron/hole can migrate to the semiconductor surface. At the surface the semiconductor can donate electrons to reduce an electron acceptor (usually oxygen in an aerated solution) (pathway C); in turn, a hole can 9 migrate to the surface where an electron from a donor species can combine with the surface hole oxidizing the donor species (pathway D). The electron transfer process is more efficient if the species are spreadsorbed on the surface [47]. The probability and rate of the charge transfer processes for electrons and holes depends upon the respective positions of the band edges for the conduction and valence bands and the redox potential levels of the adsorb ate species. 1.5 TiO2 nanostructured materials as semiconductor photocatalysts Titanium (Ti) is a light, strong, lustrous, and corrosion-resistant metal. Titanium dioxide (TiO2) is the most commonly used compound of titanium. Since its commercial production in the early twentieth century, TiO2 has been widely used as a pigment in sunscreens, paints, ointments, and toothpaste. It is also used in cements, gemstones, as an optical opacifier in paper, and a strengthening agent in graphite composite fishing rods and golf clubs. TiO2 powder is chemically inert, stable under sunlight, and is very opaque. This allows it to impart a pure and brilliant white colour to the brown or gray chemicals that form the majority of household plastics. However, in 1972, Fujishima and Honda discovered the phenomenon of photocatalytic splitting of water on a TiO2 electrode under ultraviolet (UV) light. Since then, enormous efforts have been devoted to the research of TiO2, which has led to many promising applications such as photocatalysis, photovoltaic, photoelectrochromics and sensors. Some potential applications of TiO2 are mentioned below. 1.6 Photocatalytic Applications As has been pointed out by Heller, the development of semiconductor photo electrochemistry during the 1970 and 1980s has greatly assisted the development of photocatalysis [47, 48]. In particular, it turned out that TiO2 is excellent for photocatalytically breaking down organic compounds. For example, if one puts catalytically active TiO2 powder into a shallow pool of polluted water and allows it to be illuminated with sunlight, the water will gradually become purified. Ever since 1977, when Frank and Bard first examined the possibilities of using TiO2 to decompose cyanide in water [16], there has been increasing interest in environmental applications. These authors quite correctly pointed out the implications of their result for the field of 10 environmental purification. Their prediction has indeed been borne out, as evidenced by the extensive global efforts in this area [49]. One of the most important aspects of environmental photocatalysis is the availability of a material such as titanium dioxide, which is close to being an ideal photocatalyst in several respects. For example, it is relatively inexpensive, highly stable chemically, and the photogenerated holes are highly oxidizing. In addition, photogenerated electrons are reducing enough to produce superoxide from dioxygen. The commonly studied principle of the photocatalysis reaction mechanisms is given in Figure 1.7. SEMICONDUCTOR TiO2 Figure 1.7 The principle of TiO2 photocatalysis [50] When photons with energies larger than the band gap of TiO2 are absorbed, electrons are excited from the valence band to the conduction band, creating electron-hole pairs [50]. These photogenerated charge carriers can undergo recombination, become trapped in metastable states, or can migrate to the surface of the TiO2, where they can react with adsorbed molecules. In an aqueous environment saturated with air, the photogenerated electrons and holes participate in reacting with dissolved molecular oxygen, surface hydroxyl groups, and adsorbed water molecules to form hydroxyl and superoxide radicals. The energy band diagram for TiO2 in pH 7 solution is shown in Fig. 1.8. 11 Figure 1.8 The energy band diagram for TiO2 As shown, the redox potential for photo generated holes is + 2.53V [41] versus the standard hydrogen electrode (SHE). After reaction with water, these holes can produce hydroxyl radicals (OH), whose redox potential is only slightly decreased. Both are more positive than that for ozone. The redox potential for conduction band electrons is −0.52V, which is in principle negative enough to evolve hydrogen from water, but the electrons can become trapped and lose some of their reducing power, as shown. However, even after trapping, a significant number are still able to reduce dioxygen to superoxide O2−., or to hydrogen peroxide H2O2. Depending upon the exact conditions, the holes, OH radicals, O2−., H2O2 and O2, all can play important role in the photocatalytic reaction mechanisms. Although the detailed mechanism of TiO2 photocatalysis reactions differs from one pollutant to another, it has been widely recognized that superoxide and, specifically, •OH hydroxyl radicals act as active reagents in the degradation of organic compounds. These radicals are formed by scavenging of the electron–hole pair by molecular oxygen and water, through the following sequences [51]: TiO2 + hν → e− + h+ O2 + e− →O2 − • H2O + h+ → •OH + H+ 12 •OH + •OH → H2O2 H2O2 + O2−•→ •OH + OH− +O2 Following a similar mechanism, the TiO2 photocatalyst can reduce CO2 to CH3OH or produce H2 in a controlled environment (inert or oxygen free). However, the photocatalytic activity of a semiconductor widely depends on its: (i) light absorption properties, (ii) surface reduction and oxidation rates by the electron and hole, and (iii) electron-hole recombination rates. On the other hand, the following three factors pertaining to the band structure of semiconductors have the greatest effect on the photocatalytic reactions: (i) band gap energy, (ii) position of the lowest point in the conduction band, and (iii) position of the highest point in the valence band. In photocatalytic reactions, the band gap energy principally determines which light wavelength is the most effective, and the position of the highest point in the valence band is the main determinant of the oxidative decomposition power of the photocatalyst. Naturally occurring TiO2 has three polymorphs, i.e. anatase, brookite, and rutile. Although all three types of polymorphs are expressed using the same chemical formula (TiO2), their structures are different. Rutile is thermodynamically the most stable phase, although the anatase phase forms at lower temperatures. Despite the fact that the band gap values are 3.0 eV for the rutile and 3.2 eV for the anatase phases, both absorb only UV rays. Hence both of these phases show photocatalytic activity whereas the brookite phase does not. Characteristics of the rutile phase seem more suitable for use as a photocatalyst because the rutile phase can absorb light of a wider range. But, the anatase phase exhibits higher photocatalytic activity [52]. The most prominent reasons are attributed to the difference in the energy structure between the two phase types and the surface area. In both phases, the position of the valence band is deep, and the resulting positive holes show sufficient oxidative power. However, the conduction band in the anatase phase is closer to the negative position than in the rutile phase. Therefore, the reducing power of the anatase phase is stronger than that of the rutile phase. Usually, the anatase crystal phase formed at lower temperatures, show higher surface areas compared to the rutile phase. A larger surface area with a constant surface density of adsorbents leads to faster surface photocatalytic reaction rates. In this sense, the higher the specific surface area, the higher the photocatalytic activity that one can expect. Therefore, the anatase phase exhibits higher overall photocatalytic activity compared to 13 the rutile phase. However, Hermann et al. [53] hypothesized that the anatase and rutile mixed phases showed better photocatalytic activity because any kind of solid–solid interface is a key structural feature that facilitates the charge separation to hinder recombination. The interface also acts as an active site to initiate the catalytic activity and enhance photocatalytic efficiency [54]. In addition, TiO2 nanomaterials with high crystallinity show superior photocatalytic activity. High temperature treatment usually improves the crystallinity of TiO2 nanomaterials, which can induce the aggregation of small nanoparticles and decrease the surface area [55]. Therefore, it is very difficult to predict the photocatalytic activities from the physical properties of TiO2 nanomaterials. Optimal conditions are sought by taking into account all these considerations, which may vary from case to case. 1.7 Other Potential Applications In addition to the photocatalysis and photovoltaic applications, TiO2 nanomaterials can also be used in biomedical applications [56], functionalized hybrid materials [57], and in sensors and nanocomposites [58, 59]. The one dimensional TiO2 nanotubes are promising for reinforcement due to their unique physical properties, i.e. large surface to volume ratio, low cost and better biocompatibility compared with carbon nanotubes [60]. These materials can be used as fillers for many applications such as a radio pacifier in bone cement, a solid plasticizer of poly (ethylene oxide) for lithium batteries, a dye in a conjugated polymer for photoelectrochemical photoconductive agents, and as a photocatalyst in a photodegradable TiO2-polystyrene nanocomposite film [61, 62]. Moreover, TiO2 nanocrystalline films have been widely studied as sensors for various gases. For instance, Varghese et al. observed that TiO2 nanotubes were excellent roomtemperature hydrogen sensors not only with a high sensitivity but also with ability for self-cleaning after environmental contamination [63]. TiO2 nanomaterials also have been widely explored as electro chromic devices, such as electro chromic windows and displays. Electrochromism can be defined as the ability of a material to undergo colour change upon oxidation or reduction. Electro chromic devices are able to vary their throughput of visible light and solar radiation upon electrical charging and discharging using a low voltage. 14 1.8 Water splitting using semiconductor photocatalysis The importance of hydrogen energy has recently been recognized again, especially for use in fuel cells with due concern for environmental issues. However, industrially hydrogen is produced by steam reforming of hydrocarbons such as methane. Dihydrogen has to be produced from water using natural energy if one is concerned about environmental issues. Therefore, water splitting using a photocatalyst is a challenging reaction because it is one of the most important reactions for solving energy and environmental problems. Water splitting using photocatalysts is not new. Water splitting has been studied in the fields of catalysis, electrochemistry, photochemistry, organic and inorganic chemistry, etc., for about 30 years since the Honda–Fujishima effect was reported using a TiO2 semiconductor electrode. However, the number of reported photocatalysts that are able to decompose water into H2 and O2 in a stoichiometric amount with a reasonable activity has been limited. The only active photocatalysts at present are oxide materials. Many people believe that water splitting is impossible at a practical level. Against such a background, various types of new photocatalysts for water splitting have been developed and this research field is taking a new turn. H2O cannot be photo decomposed on clean TiO2 surfaces, even though TiO2 can be effectively photo excited under band-gap irradiation. Figure 1.9 illustrates the band edge positions of TiO2 relative to the electrochemical potentials of the H2/H2O and O2/H2O couple [64]. Figure 1.9 Potential energy diagram for the H2/H2O and O2/H2O redox couples relative to the band-edge positions for TiO2. 15 According to this electron energy diagram, water photolysis is energetically favourable. However, due to the presence of a large over potential for the evolution of H2 and O2 on the TiO2 surface, TiO2 alone becomes inactive. Sustained photodecomposition of water has been achieved under conditions where photogenerated electrons and holes are separated for maximum photoreaction yield. 1.9 Limitation of TiO2 as an efficient photocatalyst and the modification of TiO2 There are some important drawbacks that severely limit the application of titanium dioxide photocatalyst as a general tool either to degrade organic pollutants in the gas or liquid phase or to perform useful transformations of organic compounds [65, 66]. One of the most important limitations is the lack of TiO2 photocatalytic activity with visible light [67, 68]. Figure 1.10 Solar spectrum at sea level with the sun at zenith with the absorption region of TiO2 The reason for this is that the anatase form of TiO2 is a wide band gap semiconductor with a band gap of 3.2 eV in most media, corresponding to an onset of the optical absorption band at light photocatalytic activity, since approximately 5% of the solar 16 light energy (figure 1.10) can be absorbed by TiO2. The above comments explain the continued interest in improving the photocatalytic efficiency of TiO2. 1. 10 Modified Titania systems for improved photocatalytic activity Two general strategies have been developed to increase the photocatalytic activity of TiO2, namely the use of an organic dye as photosensitizer or doping TiO2 with metallic and non-metallic elements [69-71]. The first route (using an organic dye that absorbs visible light) has worked very well under conditions where oxygen/air is excluded and the degradation of the dye is minimized by the efficient quenching of the dye oxidation state with an appropriate electrolyte [72, 73]. Otherwise, particularly the dye becomes rapidly mineralized and the photocatalytic system loses its response towards visible light in the presence of oxygen. The mechanism of TiO2 dye sensitization has been determined using time resolved sub nanosecond laser flash photolysis techniques [74]. In dye sensitization, the most relevant points are the absorption spectrum of the dye in the visible region and the energy of the electron in the excited electronic state of the dye, which has to be high enough to be transferred to the semiconductor conduction band. A second chemical route to promote titania photoresponse into the visible spectra is the doping of TiO2 material either with metallic or non-metallic elements [75]. In this case, doping introduces occupied or unoccupied orbitals in the band gap region leading to negative or positive doping, respectively. A summary of some novel preparations of UV and visible light responsive titania photocatalysts developed over the last few years has been recently compiled [76].The limitations of titania semiconductor as a photocatalyst for a particular use can be surmounted by modifying the surface of the semiconductor in the following ways: 1.10.1 Metal semiconductor modification Among the metal doped titania, Pt doping has recently attracted a great deal of attention due to promising improvement in photo oxidation rate especially in gas phase. It has been found that Pt–TiO2 improves the photo oxidation rate of ethanol, acetaldehyde and acetone in the gaseous phase [77]. Li et al [78] reported a further development of mesoporous titania as photocatalyst. These authors have prepared a photocatalyst constituted by mesoporous titania embedding gold nanoparticles (Au/TiO2) whose preparation requires P-123 as structure directing agent, a mixture of TiCl4 and Ti(OBu)4 17 and AuCl3 as the source of gold using ethanol as solvent. The gel is cast on a Petri dish to form a thin layer that is subsequently aged at 373 K to form a homogeneous mesostructured nanocomposite. Calcinations at 350°C in air remove the template while inducing crystallization of TiO2 and formation of gold nanoparticles. TiO2 has also been doped with other metals, including V, Cr, Mn, Fe and Ni. The presence of the dopant was found to cause large shift in the absorption band of titanium dioxide towards the visible region. However, there are contradictory reports, particularly in the case of metal doping, describing either an increase or a decrease of the photocatalytic activity [79]. This controversy arises in part from the difficulty to establish valid comparisons between the photocatalytic activity of various solids testing different probe molecules and employing inconsistent parameters. Also, the doping procedure and the nature of the resulting material are very often not well defined and, most probably, controversial results can be obtained depending on the way in which the metal has been introduced. It also depends on the final concentration of the dopant. Thus, it has often been reported that there is an optimum doping level to achieve the maximum efficiency and beyond this point a decrease in photocatalytic activity is again observed [80]. Nevertheless, a generalised consensus has been reached with regards to the inappropriateness of metal doping as valid solution to enhance the photocatalytic activity of TiO2. 1.10.2 Composite semiconductors Figure 1.11 Photoexcitation in composite semiconductor photocatalyst. The efficiency of a photocatalytic process can be increased by coupled semiconductor photocatalysts which provide an interesting way to increase the charge separation, and extending the energy range of photoexcitation for the system. Figure 1.11 illustrates 18 geometrically and energetically the photoexcitation process for the composite (coupled) semiconductor photocatalyst CdS-TiO2. The energy of the excitation light is too small to directly excite the TiO2 portion of the photocatalyst, but it is large enough to excite an electron from the valence band across the band gap of CdS (Eg = 2.5 eV) to the conduction band. The hole produced in the CdS valence band from the excitation process remains in the CdS particle while the electron transfers to the conduction band of the TiO2 particle. The electron transfer from CdS to TiO2 increases the charge separation and efficiency of the photocatalytic process. The separated electron and hole are then free to undergo electron transfer with adsorbates on the surface. The quantum yield for the reduction of methylviologen drastically increased and approached an optimum value of 1 when the concentration of TiO2 was increased in a CdS-TiO2 system [81]. The coupling of semiconductors with the appropriate energy levels can produce a more efficient photocatalyst via better charge separation. 1.10.3 Surface sensitization Figure 1.12 Excitation steps using dye molecule sensitizer. The efficiency of the excitation process of wide band-gap semiconductor photocatalyst (TiO2) can also be increased by surface sensitization of a chemisorbed or physisorbed dyes. The photosensitization process can also expand the wavelength range of excitation for the photocatalyst through excitation of the sensitizer followed by charge transfer to the semiconductor. Erythrosin B, 3 thionine, and analogs of Ru (bpy) 3 2+ are some of the common dyes which are used as sensitizers. Figure 1.12 illustrates the excitation and charge injection steps involved for the regenerative dye sensitizer surface process. Excitation of an electron in the dye molecule occurs to either the singlet or triplet excited state of the molecule. If the oxidative energy level of the excited state of the dye 19 molecule with respect to the conduction band energy level of the semiconductor is favourable (i.e. more negative), then the dye molecule can transfer the electron to the conduction band of the semiconductor. The surface acts as a quencher accepting an electron from the excited dye molecule. The electron in turn can be transferred to reduce an organic acceptor molecule adsorbed on the surface. 1.10.4 Transition metal doping An interesting area of semiconductor modification is the study of the influence of dissolved transition metal impurity ions on the photocatalytic properties of TiO2. The advantage of transition metal doping species is the improved trapping of electrons to inhibit electron-hole recombination during light illumination. Different metals have been employed to tune the electronic structure of TiO2-based material either by the ion implantation method or by a wet chemical method [82]. The photocatalytic reactivity of metal-doped TiO2 depends on many factors, including the dopant concentration, the energy level pattern of the dopants within the TiO2 lattice, their d-electronic configuration, and the distribution of the dopants. Enhanced photocatalytic activity has been reported for Fe (III), Mo (V), Ru (III), Re (V), V (IV), and Rh (III) metals doped TiO2 at 0.5% atomic ratio. It has been reported that the metal ions physically implanted have produce significant changes in the TiO2 material. However, metal doping can result in thermal instability and increased carrier trapping. 1.10.5 Non-metal doped TiO2 for photocatalysis The elements used as the dopants in TiO2 cover almost the whole periodic table and is summarized in Figure 1.13. Recent theoretical and experimental studies have shown that the desired band gap narrowing of TiO2 can also be achieved by using a nonmetal, although there is controversy regarding the origin of the resulting band gap narrowing. Asahi and co-workers calculated the electronic band structures of anatase TiO2 with different substitutional dopants, including C, N, F, P, or S and found that the substitutional doping of N was the most effective for band gap narrowing. This is because the p states of N mix with the 2p states of O, while the molecularly existing species, e.g., NO and N2 dopants, give rise to the bonding states below the O 2p valence 20 bands, while the antibonding states deep within the band gap hardly interact with the band states of TiO2 [83]. Figure 1.13 The elements used as the dopants in TiO2 Di Valentin et al. reported that the N 2p orbital formed a localized state just above the top of the O 2p valence band, both for the anatase and rutile phases. However, these two crystal systems showed the opposite photoresponce. In anatase, these dopant states caused a red shift of the absorption band edge toward the visible region, while in rutile, an overall “blue shift” was observed. This experimental evidence confirmed that Ndoped TiO2 formed N induced midgap levels slightly above the oxygen 2p valence band [84]. Nakano et al. reported that in N-doped TiO2, deep levels located at approximately 1.18 and 2.48 eV below the conduction band were attributed to the O vacancy state and a band gap narrowing was achieved by mixing with the O 2p valence band, respectively [85]. N-doped TiO2 normally has a colour from white to yellow or even light gray, and the onset of the absorption spectra red shifts to longer wavelengths. Table 1.3 shows different methods used to prepare N-doped and S-doped titania. In N-doped TiO2 nonmaterial, the band gap absorption onset shifted 600 nm from 380 nm for the undoped TiO2, extending the absorption up to 600 nm. The optical absorption of Ndoped TiO2 in the visible light region was primarily located between 400 and 500 nm, while that for oxygen deficient TiO2 was mainly above 500 nm. N-F-co-doped TiO2 prepared by spray pyrolysis was shown to absorb light up to 550 nm in the visible spectrum [102, 103]. Livraghi et al. recently found that N-doped TiO2 contained single atom nitrogen impurity centres, localized in the band gap of the oxide, which were responsible for the visible light absorption with promotion of electrons from the band gap localized states to the conduction band [104]. 21 Table 1.3 Various methods of preparation of N and S doped titania N-Doped titania Reference By hydrolysis of TTIP in a water/amine mixture and the post 86, 87 treatment of the TiO2 sol with amines Directly from a Ti-bipyridine complex 88 By ball milling of TiO2 in a NH3 water solution 89 By heating TiO2 under NH3 flux at 500-600 °C 90, 91 By calcination of the hydrolysis product ofTi(SO4)2 92 with ammonia as precipitation By decomposition of gas-phase TiCl4 with 93 an atmosphere microwave plasma torch By sputtering/ion-implanting techniques with 94, 95 nitrogen or N2+ gas flux. S-Doped Titania Reference By mixing TTIP with ethanol containing thiourea 96, 97 By heating sulfide powder 98, 99 10. By using sputtering or ion-implanting 100, 101 techniques with S+ ion flux 1.11 Synthetic Methods for TiO2 Nanostructures: Various synthetic methods used for the preparation of TiO2 Nanostructures are as follows1.11.1 Sol-gel methods: The sol-gel method is a versatile process which is widely used for synthesizing various oxide materials [105-107]. This synthetic method generally allows control of the texture, the chemical, and the morphological properties of the solid. This method also has several advantages over other methods, such as allowing impregnation or co precipitation, which can be used to introduce dopants. The major advantages of the solgel technique includes molecular scale mixing, high purity of the precursors, and homogeneity of the sol-gel products with a high purity of physical, morphological, and chemical properties. In a typical sol-gel process, a colloidal suspension, or a sol, is 22 formed from the hydrolysis and polymerization reactions of the precursors, which are usually inorganic metal salts or metal organic compounds such as metal alkoxides. When a metal precursor alkoxide/salt reacts with water, nucleophilic substitution occurs as shown in Figure 1.14 For the coordinative saturated metals such as the metal alkoxides, hydrolysis and condensation both occur by nucleophilic substitution (SN) mechanisms, in which coordination and proton transfer are involved and followed by removal of either alcohol or water. Complete polymerization and loss of solvent leads to the liquid sol transforming into a solid gel phase. Figure 1.14 Hydrolysis and condensation pathways of metal alkoxides Thin films can be produced on a piece of substrate by spin-coating or dip-coating. A wet gel will form when the sol is cast into a mold, and the wet gel is converted into a dense ceramic upon further drying and heat treatment. A highly porous and extremely low-density material, called an aerogel, is obtained if the solvent in a wet gel is removed under supercritical conditions. Figure 1.15 shows the conventional scheme to produce aerogels. This method involves hydrolysis of the metal alkoxide with water and a catalyst, i.e. an acid or a base, condensation into macromolecules, forming a colloidal sol and subsequently three-dimensional network, solvent exchange to remove water by alcohol, and then drying the wet gel using a supercritical fluid to produce the aerogel. Aerogels can be used for advanced applications including electrochemical devices, thin coatings, composite biomaterials, catalysts, ceramics, and heat and electric insulation 23 devices due to the aerogels having unique morphological and chemical properties. Ceramic fibbers can be drawn from the sol when the viscosity is adjusted into the proper range. Since the precursors react with water quickly and tend to precipitate, many methods have been used to control the reaction rate in order to obtain desired nanostructures. However, in binary metal systems, the main difficulty is to control the hydrolysis rate of the precursors. Modifying the precursors with a suitable complexing agent is one way to alter the hydrolysis rate, while generating in-situ water (instead of externally added water) is another possible way to control the hydrolysis rate. In practice, acetic acid is often used to modify the reactivity of metal alkoxides by replacing the alkoxy groups bonded to the metal by acetate groups, forming M-OAc complexes and alcohols. Metal alkoxide Water+ acid (or base) +alcohol Hydrolysis Aging Calcinatio Figure 1.15- Conventional scheme to produce aerogels Moreover, acetic acid (HO-Ac) can react with the alcoholic solvent and intermediates, (produced by modification reaction) to form water via an esterification reaction [108] However, the properties of the sol-gel products depend on the precursors, processing temperature, catalyst, solvents, and solvent removal process [109] 1.11.1.1 Mechanism of Sol-Gel Synthesis The sol-gel process involves hydrolysis and condensation of the metal alkoxide followed by heat treatment at elevated temperatures which induce polymerisation, 24 producing a metal oxide network [110]. In general, transition metals have low electronegativity’s and their oxidation state is frequently lower than their coordination number in an oxide network. Therefore, coordination expansion occurs spontaneously upon reaction with water or other nucleophilic reagents to achieve their preferred coordination [111]. Metal alkoxides are in general very reactive due to the presence of highly electronegative OR groups (hard-π donors) that stabilise the metal in its highest oxidation state and render it very susceptible to nucleophilic attack. The lower electronegativity of transition metals causes them to be more electrophilic and thus less stable toward hydrolysis, condensation and other nucleophilic reactions. Controlling the conditions can be difficult but successful control of the reaction conditions has the potential to produce materials of consistent size, shape and structure [112-114]. 1.11.1.2 Mechanism of hydrolysis As stated previously the sol-gel reaction involves hydrolysis of the metal alkoxide followed by condensation. Hydrolysis of titanium alkoxides occurs through a nucleophilic substitution (SN) reaction. When a nucleophile, such as water is introduced to titanium alkoxide a rapid exothermic reaction proceeds. The nucleophilic addition (AN) of water involves a proton from the attacking nucleophile (water) being transferred to the alkoxide group. The protonated species is then removed as either alcohol or water (scheme 1.) [107, 115]. HOH+ RO M → HO M + ROH Scheme 1- Hydrolysis reaction The nucleophilic substitution reaction that occurs during hydrolysis can be described as follows [115]: 1. Nucleophilic addition of the H2O onto the positively charged metal atom. 2. Proton transfer, within the transition state from the entering molecule to the leaving alkoxy group. 1.11.1.3 Mechanism of condensation Condensation reactions complete the sol-gel process. Condensation can proceed through either alcoxolation or through oxolation. In both processes an oxo bridge is formed 25 between the metals (M–O–M) but the leaving group differs. During alcoxolation, two partially hydrolysed metal alkoxide molecules combine and an oxo bridge is formed between the two metals with alcohol departing as the leaving group (scheme 2) [109, 115]. Scheme 2 Alcoxolation reaction In oxolation (scheme 3) two partially hydrolysed metal alkides combine to form an oxo bridge between the metal centres but water is the leaving group. Scheme 3 Oxolation reaction Condensation reactions ultimately polymerised to form large chains of molecules. Solvent used also influence the reaction kinetics of sol-gel reactions. Because if a suitable solvent is chosen; it may be preferentially hydrolysed over the alkoxide ligands. This allows for greater control over the reaction kinetics through the correct use of solvent [116]. Hydrolysis and condensation kinetics are also affected by the organic ligand. The hydrolysis rate of titanium alkoxides decreases with increasing alkyl chain length [117, 118]. This is mainly due to the steric effect which is expected for an associative SN reaction mechanism 1.11.1.4 Role of the catalyst Acid and base catalysts can have a strong influence over hydrolysis and condensation rates as well as the structural properties of the final product. The addition of an acid will 26 result in the preferential protonation of the negatively charged alkoxide group (scheme 4). Protonation of the alkoxide group produces good leaving groups which enhance the reaction kinetics, eliminating any proton transfer that occurs in the transition state and thus allowing hydrolysis to go to completion upon the addition of water. H M + OR + H → + M O R Scheme 4- Acid catalyst reaction In alkaline conditions, hydroxo ligands are deprotonated, producing strong nucelophiles: L–OH +: B → L–O- + BH+ where L = M or H and B = OH- or NH3. The hydrolysis rate of Ti (OBu) 4 was less in basic conditions than in acidic or neutral conditions. It was postulated that the nucleophilic addition of OH- may reduce the partial charge of the titanium metal centre (δ (Ti)), making the hydrolysis reaction less favourable [109, 119]. While hydrolysis kinetics is retarded in basic conditions, the condensation kinetics of metal alkoxides is enhanced. 1.11.2 Hydrothermal Method The hydrothermal method is widely used for the production of small particles in the ceramics industry. Usually, this process is conducted in steel pressure vessels called autoclaves under controlled temperature and/or pressure with the reactions occurring in aqueous solution. The temperature can be elevated above the boiling point of water, reaching the pressure of vapour saturation. The temperature and the amount of solution added to the autoclave largely determine the internal pressure produced. The hydrothermal method has been widely used to prepare TiO2 nanotubes after the pioneering work by Kasuga et al. in 1998 [120]. Generally, several grams of TiO2 powders are added to concentrated NaOH solution and held at 20-110oC for 20 h in an autoclave. TiO2 nanotubes were obtained after the products were washed with a dilute HCl aqueous solution and distilled water. When the raw TiO2 material was treated with 27 NaOH aqueous solution, some of the Ti-O-Ti bonds were broken and new Ti-O-Na and Ti-OH bonds were formed. New Ti-O-Ti bonds were formed after the Ti-O-Na and TiOH bonds reacted with acid and water. The bond distance from one Ti atom to the next Ti atom on the surface was found to decrease. This resulted in the folding of the sheets and connection between the ends of the sheets, resulting in the formation of a tube structure. In this mechanism, the TiO2 nanotubes were formed in the stage of the acid treatment following the alkali treatment. The hydrothermal method is also currently being used to produce many new hybrid materials with new morphologies and improved crystallinity. 1.11. 3 Micelle and Inverse Micelle Methods Micelles and inverse micelles are commonly employed to synthesize TiO2 nanomaterials. A statistical experimental design method was conducted by Kim et al. to optimize experimental conditions for the preparation of TiO2 nanoparticles [121]. The values of H2O/surfactant, H2O/titanium precursor, ammonia concentration, feed rate, and reaction temperature were significant parameters in controlling TiO2 nanoparticle size and size distribution. 1.11.4 Sol Method: The sol method here refers to the nonhydrolytic sol-gel processes andusually involves the reaction of titanium chloride with a variety of different oxygen donor molecules, e.g., a metal alkoxide or organic ether [122-125] 1.11.5 Solvothermal Method: The solvothermal method is almost identical to the hydrothermal method except that the solvent used here is nonaqueous. 1.11.6 Direct Oxidation Method: TiO2 nanomaterials can be obtained by oxidation of titanium metal using oxidants or under anodization. 1.11.7 Chemical Vapour Deposition: Vapour deposition refers to any process in which materials in a vapour state are condensed to form a solid-phase material. Thick crystalline TiO2 films with grain sizes below 30 nm as well as TiO2 nanoparticles with 28 sizes below 10 nm can be prepared by pyrolysis of TTIP in a mixed helium/oxygen atmosphere, using liquid precursor delivery [126]. 1.12 Characterization Methods for TiO2 Nanostructures 1.12.1 XRD: XRD gives the following information: i) The nature of materials such as amorphous or crystalline ii) Types of structure and phases iii) Degree of crystallinity and thermal stability iv) In case of metal doping in a particular structure it can tell us whether the metal atom has been incorporated into the framework by measuring the unit cell volume. The powdered diffraction pattern of titania semiconductors are generally recorded between 2θ values of 10-90 0. XRD patterns of nano-TiO2 and microTiO2 in rutile and anatase phases are shown in Figure 1.16 and Figure 1.17, respectively [127]. In Figure 1.16, XRD patterns exhibited strong diffraction peaks at 27°, 36° and 55° indicating TiO2 in the rutile phase. On the other hand, in Figure 1.17, XRD patterns exhibited strong diffraction peaks at 25° and 48° indicating TiO2 in the anatase phase. All peaks are in good agreement with the standard spectrum (JCPDS no.: 88-1175 and 84-1286). Figure 1.16 X-ray diffraction of rutile TiO2 (a) micropowders and (b) nanopowders. 29 Figure 1.17 X-ray diffraction of anatase TiO2 (a) micropowders and (b) nanopowders. These results suggested that the nano-TiO2 powder is composed of irregular polycrystalline. Amorphous revealed a broad pattern with low intensity; however, the effect of the amorphous materials on the broadening of the XRD patterns of nanosized TiO2 is negligible. The low-angle X-ray diffraction patterns of the mesostructured titanium dioxide thin films before and after calcinations (573 or 673 K for 4 h) are shown in Figure 1.18 [128]. Figure 1.18 Low-angle X-ray diffraction patterns of a mesostructured titanium dioxide thin film before (––) and after (- - - -) calcination (573 K for 4 h). The insets show expanded views of the (110) and (200) regions for each. 30 Table 1.4 2 Theta values and hkl planes of anatase, rutile and brookite phase of titania. PHASE 2-THETA ANATASE 25.30 (101) 0 37.8 (004) 540 (105) 25.40 (120) 30.80 (121) 40.20 (022) 0 (110) 0 (101) 0 (211) BROOKITE RUTILE hkl PLANE 27.3 35.9 54.1 JCPDS 84-1286 29-1360 86-1175 The XRD of the as-synthesised films display 3 peaks in the low-angle range with d (interatomic plane) spacing corresponding to 9.59 nm, 5.66 nm and 4.93 nm. 1.12.2 Raman Spectroscopy Raman spectroscopy is used in condensed matter physics and chemistry to study vibrational, rotational, and other low-frequency modes in a system. It relies on inelastic scattering, or Raman scattering of monochromatic light, usually from a laser. The laser light interacts with phonons or other excitations in the system, resulting in the energy of the laser photons being shifted up or down. The shift in energy gives information about the phonon modes in the system. Infrared spectroscopy yields similar, but complementary information. 31 Figure 1.19 Raman spectra of anatase, rutile and brookite phases of titania The three crystalline phases of titania; anatase, rutile and brookite, exhibit wellseparated and distinct Raman activities (figure 1.19) following 1064 nm excitation which allows unambiguous identification of phase composition [129]. Knowledge of the Raman scattering cross-sections allows analysis of both crystallite size and phase compositions by comparing the relative intensities of isolated bands such as those appearing at 320 cm-1 (brookite), 608 cm-1 (rutile) and 519 cm-1 (anatase)[130, 131]. 1.12.3 I.R.Study The Diffuse Reflectance Fourier-Transform Infrared (DRFT-IR) spectroscopy helps to identify characteristic bands of the mesoporous framework. For example let us consider the FT-IR spectra of the F-doped TiO2 sol particles shown in Fig. 1.20 [132]. The TiO2 sol particles showed the main bands at 400–700 cm–1, which were attributed to Ti-O stretching and Ti-O-Ti bridging stretching modes. The small peak at 889.0 cm–1 was attributed to Ti-F vibration [133]. The peak at 1384.0 cm–1 was produced by NO3–1. The stronger peak at 1626.0 cm–1 was attributed to bending vibrations of O-H and N-H. The IR spectra of the sol sample dried at 383 K revealed that Ti-O, Ti-F, N-H, Ti-OH, H-OH groups existed in the as-prepared sample by sol-gel-hydrothermal method. 32 Figure 1.20 FT-IR spectra of the F-doped TiO2 sol particles The forming of Ti-F indicated that F atoms were incorporated into the TiO2 crystal lattice. 1.12.4 UV-Vis Spectroscopy Many molecules absorb ultraviolet (UV) or visible light. The absorption of UV or visible radiation is caused by the excitation of outer electrons, from their ground state to an excited state. This technique is based on the reflection of light in the ultra violet, visible and near infrared region by a powdered sample. The DRS study (Fig. 1.21) gives valuable information on the coordination of the transition metal such as Ti. Titania samples have in common an intense UV absorption band with a maximum in the range 220–320 nm due to charge transfer from oxygen to titanium (IV) [134]. The position of this band is affected by the coordination geometry around the titanium atom and by the presence of adsorbents. More precisely, the bands in the region 210– 240 nm are attributed to oxygen to tetrahedral Ti (IV) [135], whereas the bands at higher wavelength (λ>240 nm) are due to octahedral Ti (IV) sites [136]. For TiO2 in the form of anatase the transition occurs in 315 nm region. Hence Diffuse Reflectance UVVisible Spectroscopy is a widely available technique and is a very useful tool for characterization TiO2 structure. 33 Figure 1.21 DRS of F-doped titania The absorption spectra of pure undoped TiO2, pure F-doped TiO2 and F- doped TiO2 sol prepared by the sol-gel-hydrothermal method and dried in a rotatory evaporator and dried in vacuum at 333 K was shown in Fig.1.21A [132]. It was found that sample FTiO2 could cause a new absorption band in the visible range of 400–600 nm apart from the fundamental absorption edge of TiO2, which was located in the UV region at about 385 nm (shown in Fig. 1.21C); whereas, pure F-TiO2 did not lead to any significant shift in optical absorption of TiO2 (shown in Fig. 1.21B). 1.12.5 X-ray Photoelectron Spectroscopy (XPS) XPS is a quantitative spectroscopic technique that measures the elemental composition, empirical formula, and the chemical state and electronic states of the elements that exist within a material. XPS spectra are obtained by irradiating a material with a beam of aluminium or magnesium X-rays while simultaneously measuring the kinetic energy (KE) and number of electrons that escape from the top 1 to 10 nm of the material being analysed. Because the energy of a particular X-ray wavelength equals a known quantity, we can determine the electron binding energy (BE) of each of the emitted electrons by using an equation that is based on the work of Ernest Rutherford (1914): Ebinding = Ephoton - Ekinetic – Φ; where E binding is the energy of the electron emitted from one electron configuration within the atom, E photon is the energy of the 34 X-ray photons being used, E kinetic is the kinetic energy of the emitted electron as measured by the instrument, and Φ is the work function of the spectrometer. Fig. 1.22 XPS survey spectra of the 4%Fe doped TiO2 films grown on LAO substrate. [137]. Fig. 1.23 XPS spectra of (a) N-doped mesoporous titania (1:1), (b) N-doped mesoporous titania (1:2) and (c) N-doped mesoporous titania (1:3) [138]. Figure 1.22 and 1.23 gives the XPS spectra of Fe-doped and N-doped titania. 35 1.12.6 Thermal Analysis Thermal analysis is an important technique for the characterization of solid materials, as it provides information on the physical and chemical changes involving endothermic and exothermic processes, temperatures for phase transitions, melting points and crystallization, and the weight loss when the temperature is increased. TGA can determine: (1) moisture/liquid content and the presence of volatile species, (2) decomposition temperatures, and (3) the rate of degradation. Figure 1.24 gives the TGA data of Er-doped luminescent TiO2 nanoparticles [139]. The results indicate there were about 4% weight loss from room temperature to 773 K and little weight loss after that. The weight loss from room temperature to 373 K is almost certainly from removal of water, while it is suspected that the weight loss above 373 K is due to removal of water, and perhaps hydroxyl groups. Figure 1.24: TGA data obtained from 3% Er-doped TiO2 Full decomposition of hydroxyl groups requires a heat treatment around 1273 K; however, it is seen that little weight loss between 773 K and 1073 K, indicating that only trace structural water is present at 773 K since most would likely be removed by 1073 K. 1.12.7 N2 Physisorption The textural characterization, such as surface area, pore volume and the pore size distribution of the titania samples can be obtained by N2 physisorption studies. Prior to N2 physisorption, the samples have to be degassed at 473 K under vacuum for 2 hours. From the N2 adsorption isotherms, the specific surface area can be calculated. The 36 mesopore volume (VBJH), the average pore diameters (Dpore), and the pore size distributions can be estimated by the Barret–Joyner– Halenda (BJH) method applied to the desorption branch of the isotherm. BET Surface Area When a highly dispersed solid is exposed in a closed space to a gas or vapour at some definite pressure, the solid begins to adsorb the gas. Adsorption on porous materials proceeds via monolayer adsorption followed by multilayer adsorption and capillary condensation. At a low relative pressure, a monolayer of adsorbent is absorbed on the surface like non porous materials. The amount of adsorbent is used to calculate the surface area. Using the Brunauer, Emmett and Teller (BET) theory, one can calculate the specific surface area of a solid sample from the number of monolayer gas molecules required to cover the solid surface, and the cross-sectional area of the gas molecule being adsorbed. BJH Pore-Size Distribution and Pore Volume According to the IUPAC definitions, microporous, mesoporous and macroporous materials exhibit pore diameters of less than 2 nm, in the range of 2-50 nm and above 50 nm, respectively [140]. During a physisorption process, beyond a monolayer formation, the amount of adsorbed gas gradually increases as the relative pressure increases, and then at higher pressures, the amount of gas adsorbed increases steeply due to capillary condensation in the mesopores. Once these pores are filled, the adsorption isotherm is complete. The capillary condensation is believed to be proportional to the equilibrium gas pressure and the size of the pores inside the solid. The Barrett, Joyner and Halenda (BJH) computational method allows the determination of pore sizes from the equilibrium gas pressures. Hysteresis Loops After an adsorption isotherm, desorption isotherm can be generated by withdrawing the adsorbed gas by reducing the pressure. However, capillary condensation and capillary evaporations do not take place at the same pressure, resulting in hysteresis loops. The resulting hysteresis loops can be mechanistically related to particular pore shapes. 37 Figure 1.25 shows the classification of hysteresis loops denoted as H1, H2, H3 and H4 by IUPAC. Type H1 and H2 loops were obtained from agglomerated spherical particles and corpuscular systems, respectively, while type H3 and H4 were obtained from slitshaped pores or plate-like particles. Figure 1.25 Hysteresis loops Figure 1.26 BET surface area of Phosphated titania [141] Figure 1.26 gives the BET surface area of phosphate titania which demonstrates that the structure of pure titanium dioxide collapses after calcination at 973 K. In contrast, hysteresis observed in the case of phosphated titanium dioxide samples is indicative of porous structure. The specific surface area (as BET) increases with increasing phosphate content at a given calcination temperature 38 1.12.8 Scanning electron microscopy (SEM) Manfred von Ardenne pioneered the scanning electron microscope (SEM) and built his universal electron microscope in the 1930s. In the SEM, a very fine beam of electrons with energies up to several tens keV is focused on the surface of a specimen, and is scanned across it in a parallel pattern. The intensity of emission of secondary and backscattered electrons is very sensitive to the angle at which the electron beam strikes the surface of the sample. The emitted electron current is collected and amplified. The magnification produced by the SEM is the ratio between the dimension of the final image display and the field scanning on the specimen. Usually, the magnification range of the SEM is between 10 to 222,000 times, and the resolution is between 4-10 nm (figure 1.27). Figure 1.27: SEM images of Ni-doped TiO2 spheres: (a) side and (b) top views. SEM images of Co-doped TiO2 spheres: (c) side and (d) top views [142]. Generally, the TEM resolution is about an order of magnitude greater than the SEM resolution, however, because the SEM image relies on surface processes rather than transmission, it is able to image bulk samples and has a much greater depth of view, and so can produce images that are a good representation of the overall 3D structure of the sample. SEM images of the Fe-doped TiO2 agglomerates are presented in Fig. 1.27. 39 1.12.9 Transmission Electron Microscopy (TEM) In 1931, Knoll and Ruska built the first electron microscope prototype. In 1938, Eli Franklin Burton built the first practical electron microscope and in 1939, Siemens produced the first commercial TEM. However, the TEM was not used for material studies until 40 years ago, when the thin-foil preparation technique was developed. More improvements of the TEM technique in the 1990s provided 0.1 nm of resolution, which made TEM an indispensable analysis technique for studying materials in the micron or nano size region. TEM bright field images of TiO2 nanopowders in anatase phases are shown in Figure (1.28a), respectively [127]. Figure 1.26: Images of anatase phase. (a) TEM image of micro-TiO2 powder; (b) TEM image of nano-TiO2 powder; (c) SAED pattern of nano-TiO2 powder and (d) HRTEM image of nano-TiO2 powder. 40 It can be estimated that the particle size of powders in Figure (1.28 b) are nanoscale with the grain size less than 10 nm. The corresponding selected area electron diffraction (SAED) patterns of nano- TiO2 powder anatase phases are shown in Figure (1.28c), respectively. SAED patterns of nano-TiO2 powders in anatase phase (Figure (1.28c) shows that the brightness and intensity of polymorphic ring is weak, so they are poorly crystallized and partly amorphous. The crystallinity of nano-TiO2 powders can also be observed by phase-contrast images or Moire patterns. Figure (1.28) show crystal lattice planes of nano-TiO2 in rutile and anatase phases, respectively. It is seen that, anatase give many crystal lattice planes with d-spacing of 0.313 nm for the plane (101). 1.12.10 Photoluminescence: Photoluminescence (PL) emission spectra have been widely used to investigate the efficiency of charge carrier trapping, migration, and transfer in order to understand the fate of electron/hole pairs in semiconductor particles, since PL emission results from the recombination of free carriers. Figure 1.29a [143] shows the room-temperature PL spectra for C-doped and undoped TiO2 using the excitation light of 280 nm UV light. It can also be seen that the PL intensity of the undoped TiO2 is much higher than that in the spectra of C-doped samples, indicating that carbon doping can effectively inhibit excited electron and hole recombination. The effective inhibition of excited electron and hole recombination due to carbon doping can be explained by the following two pathways. First, the surface hydroxyl groups can be trapped by the holes to form hydroxyl radicals which can suppress electron-hole recombination, thus the PL intensity. Second, theoretical and experimental investigation indicated that carbon doping favours the formation of oxygen vacancies. The electron is trapped by the oxygen vacancy, while the hole is trapped by the doped carbon, which can decrease the PL intensity. However, no PL signal is observed for undoped TiO2, while a strong PL peak is excited for C-doped TiO2 under the excitation of 514.5 nm visible light (Figure 1.29b). The energy of the excitation visible light used is not sufficient enough to promote electronic transitions from the VB to conduction band (CB) for undoped TiO2 according to the UV-vis DRS and VB XPS. As a result, no electron/hole pairs can be generated to give PL signals for undoped TiO2 under 514.5 nm light irradiation. As for C-doped TiO2, electron/hole pairs can be generated and recombine radiatively to give 41 broad and strong PL signals. This can be ascribed to the carbon doping which reduces the band gap and increases visible light absorption. Figure 1.29: PL spectra of undoped TiO2 and C-doped TiO2 under UV-280 nm (a) and visible light-514.5 nm (b). 1.12.11 EPR Study This technique provides the information of oxidation state of the metal atom in the mesopores and the position of the metal ion in the framework 1.12.12 Photocatalysis of dyes with titania: The effluents, gaseous or liquid produced by some of our industries are harmful to the health and general well-being of man. When undesirable substances are present in liquid effluents, it can be disastrous as their presence pose severe threat to the immediate recipients. Wastewaters from various industries, factories, laboratories, etc. are serious problems to the environment. The discharged wastes containing dyes are toxic to microorganisms, aquatic life and human beings [144]. These deleterious effects of chemicals on the earth ecosystems are a cause for serious concern. Several of these chemicals such as azo dyes, herbicides, and pesticides are actually present in rivers and lakes, and are in part suspected of being endocrine-disrupting chemicals (EDCs) [145, 146]. Konstantinou and Albanis [147] reported that textile dyes and other industrial dyestuffs constitute one of the largest groups of organic compounds that represent an increasing environmental danger. About 1–20% of the total world production of dyes is 42 lost during the dying process and is released in the textile effluents [148]. Photocatalysis may be termed as a photoinduced reaction which is accelerated by the presence of a catalyst [37]. These types of reactions are activated by absorption of a photon with sufficient energy (equals or higher than the band-gap energy (Eg) of the catalyst). The absorption leads to a charge separation due to promotion of an electron (e−) from the valence band of the semiconductor catalyst to the conduction band, thus generating a hole (h+) in the valence band. The recombination of the electron and the hole must be prevented as much as possible if a photocatalyzed reaction must be favoured. The ultimate goal of the process is to have a reaction between the activated electrons with an oxidant to produce a reduced product, and also a reaction between the generated holes with a reductant to produce an oxidized product. The photogenerated electrons could reduce the dye or react with electron acceptors such as O2 adsorbed on the Ti (III)surface or dissolved in water, reducing it to superoxide radical anion O2−• . The photogenerated holes can oxidize the organic molecule to form R+, or react with OH− or H2O oxidizing them into OH• radicals. Together with other highly oxidant species (peroxide radicals) they are reported to be responsible for the heterogeneous TiO2 photodecomposition of organic substrates as dyes. The resulting •OH radical, being a very strong oxidizing agent (standard redox potential +2.8 V) can oxidize most azo dyes to the mineral end-products. According to this, the relevant reactions at the semiconductor surface causing the degradation of dyes can be expressed as follows [149]: TiO2 +hv (UV) → TiO2 (eCB− +hVB+) (1) TiO2 (hVB+) + H2O → TiO2 +H+ +OH• (2) TiO2 (hVB+) + OH−→ TiO2 +OH• (3) − TiO2 (eCB ) + O2→ TiO2 +O2 −• −• (4) • (5) Dye + OH → degradation products (6) Dye + hVB+→ oxidation products (7) Dye + eCB−→ reduction products (8) O2 + H+→ HO2 • where hv is photon energy required to excite the semiconductor electron from the valence band (VB) region to conduction band (CB) region. 43 Table 1.5 Photocatalysis of different dyes with titania: Dye degraded Type of Reference Catalyst no Methylene Violet(MV), cationic red (X-GRL) Ag–TiO2 150 Acid orange 7 (AO7) Ag–TiO2 151 Sirius Gelb GC (SG-GC) Ag–TiO2 152 0 Rhodamine B (RB) Ag –TiO2 153 nanosol Acid red B (ARB), reactive red (K-2G), cationic red (X- Ag–AgBr– GRL reactive brilliant red (X-3B ) TiO2 Methylene blue (MB) Au–TiO2 155 Fast Green FCF, Patent Blue VF TiO2 156 Orange G Sn-TiO2 157 BRL K-TiO2 158 Methyl orange Pt-TiO2 159 Acid Red B Ce-TiO2 160 Orange II Zn-TiO2 161 Bromocresol purple TiO2 162 methyl orange (MO), thymol blue (TB), and bromocresol M-TiO2 , (M = green (BG) 154 163 Ni, Cu, Zn) 1.13. Specific aims of this dissertation Since the discovery of photoinduced splitting of water on single crystal TiO2 electrodes, the technology of semiconductor-based photocatalysis has shown potential application in various areas such as sewage disposal, air purification, antibiosis and detoxification, glass antifogging and self-cleaning, reclamation of precious metal ions, and development of solar energy. TiO2 is a chemically stable, nontoxic, biocompatible, inexpensive material with very high dielectric constant and interesting photocatalytic activities. It is a wide-gap semiconductor, and depending on its chemical composition, it shows a large range of electrical conductivity. However, the performance of TiO2 44 nanomaterials strongly relies on their crystallinity, crystallite size, crystal structure, specific surface area, thermal stability and quantum efficiency. Bulk modifications such as cation or anion doping have been found very effective to improve the properties of TiO2 to enhance their performance. Several different processing techniques have been used for the preparation of TiO2-based nanostructures, such as template techniques, hydrothermal processes, and soft chemical processes. However, each of these methods has limitations. The main objective of this project was to develop a synthesis route to produce superior quality TiO2 based nanomaterials by introducing Zr, Fe, Co, N, S, and P as doping materials. The following have been identified as the specific objectives of this project: I. Synthesis of the following nanomaterials using sol-gel technique and hydrothermal technique. A. Non-metal doped titania (i) S-doped TiO2 (ii) P- doped TiO2 (iii) N- doped TiO2 B. Metal doped titania (i) Fe- doped TiO2 (ii) Zr- doped TiO2 (iii) Co- doped TiO2 II. 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