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Surface photochemical reactions

Besides these features, the formation of a layer due to an interaction of a stratified fluid with light is itself noteworthy. Analogs to this phenomenon can be found in other media. Examples include photochemical reactions in the atmosphere near the Earth s surface, photochemical reactions in the surface water of the ocean and biological activity near the ocean surface. [Pg.138]

Chen, C. J. and Osgood, R. M. (1983). Direct observation of the local-field-enhanced surface photochemical reactions. Phys. Rev. Lett. 50 1705-1708. [Pg.275]

Nevertheless, detailed information on nudear wavepacket dynamics of surface adsorbates is important both from fundamental and from practical points of view. As is evidenced from the huge success of catalysis, solid surfaces sustain various kinds of reactions [8]. In order to understand the elementary steps of these reactions, the electronic and vibrational dynamics of surface adsorbates should be investigated in depth. Photochemistry at surfaces involves the photoinduced nuclear dynamics of adsorbates, which needs to be elucidated by ultrafast spectroscopy. Furthermore, combining with recently developed pulse shaping technologies [9], elucidation of the wavepacket dynamics will open up a novel laser control scheme of surface photochemical reactions. [Pg.55]

Figure 5.37 Theoretical dependencies of the quantum yield of a surface photochemical reaction involving electrons (for the case of strong light absorption) on the absorption coefficient at different surface potentials t/s. Note that the scale in 0 is arbitrary—important is the trend in 0 with increase in a. Reprinted with permission from Emeline et al. (2003). Copyright (2003) American Chemical Society. Figure 5.37 Theoretical dependencies of the quantum yield of a surface photochemical reaction involving electrons (for the case of strong light absorption) on the absorption coefficient at different surface potentials t/s. Note that the scale in 0 is arbitrary—important is the trend in 0 with increase in a. Reprinted with permission from Emeline et al. (2003). Copyright (2003) American Chemical Society.
According to the simple model of surface photochemical reactions illustrated earlier (eqs. 5.114-5.117), if reductive and oxidative processes, Le. interaction of reagent molecules with electrons and holes, respectively, take place only on the photocatalyst surface then the selectivity toward product formation by the reductive pathway can be expressed by eq. 5.136, and for product formation through the oxidative pathway by expression 5.137 (Emeline et al, 2003). [Pg.366]

Zirconia also displays high activity in more complex surface photochemical reactions, for instance in the photolysis of water (Sayama and Arakawa, 1996) and the photoreaction between CO2 and H2 (Kohno et al, 2000). Although these and several other surface reactions on metal oxides (and metal halides) in heterogeneous photocatalysis have been claimed to be photocatalytic, no experimental evidence in support of their photocatalytic nature has ever been demonstrated. [Pg.375]

A non-photocatalytic reaction occurring on the surface of an irradiated wide bandgap metal oxide such as ZrOa can also affect the process of photoinduced formation of Zr F- and V-type colour centres. The effect of such reactions is seen as the influence of photostimulated adsorption on the photocolouration of the metal-oxide specimen. Photoadsorption of electron donor molecules leads to an increase of electron colour centres, whereas photoadsorption of electron acceptor molecules leads to an increase of hole colour centres. Monitoring the photocolouration of a metal-oxide specimen by DRS spectroscopy during surface photochemical reactions can provide a further opportunity to evaluate whether the reactions are photocatalytic. [Pg.380]

Photochemical reactions (chapter A3.13) and heterogeneous reactions on surfaces (chapter A3.10) are discussed in separate chapters. [Pg.759]

For the mechanistic studies made, this protocol is able to give information about how dynamical properties affect the evolution of a photochemical reaction, but is not accurate enough for quantitative results. The information obtained relates to aspects of the surface such as the relative steepness of regions on the lower slopes of the conical intersection, and the relative width of alternative channels. [Pg.302]

Conical intersections, introduced over 60 years ago as possible efficient funnels connecting different elecbonically excited states [1], are now generally believed to be involved in many photochemical reactions. Direct laboratory observation of these subsurfaces on the potential surfaces of polyatomic molecules is difficult, since they are not stationary points . The system is expected to pass through them veiy rapidly, as the transition from one electronic state to another at the conical intersection is very rapid. Their presence is sunnised from the following data [2-5] ... [Pg.328]

The first is a pyrolytic approach in which the heat dehvered by the laser breaks chemical bonds in vapor-phase reactants above the surface, allowing deposition of the reaction products only in the small heated area. The second is a direct photolytic breakup of a vapor-phase reactant. This approach requires a laser with proper wavelength to initiate the photochemical reaction. Often ultraviolet excimer lasers have been used. One example is the breakup of trimethyl aluminum [75-24-1] gas using an ultraviolet laser to produce free aluminum [7429-90-5], which deposits on the surface. Again, the deposition is only on the localized area which the beam strikes. [Pg.19]

TBT exists in solution as a large univalent cation and forms a neutral complex with CH or OH . It is extremely surface active and so is readily adsorbed onto suspended particulate material. Such adsorption and deposition to the sediments limits its lifetime in the water column. Degradation, via photochemical reactions... [Pg.87]

Fig. 13.11. A schematic drawing of the potential energy surfaces for the photochemical reactions of stilbene. Approximate branching ratios and quantum yields for the important processes are indicated. In this figure, the ground- and excited-state barrier heights are drawn to scale representing the best available values, as are the relative energies of the ground states of Z- and E -stilbene 4a,4b-dihydrophenanthrene (DHP). [Reproduced from R. J. Sension, S. T. Repinec, A. Z. Szarka, and R. M. Hochstrasser, J. Chem. Phys. 98 6291 (1993) by permission of the American Institute of Physics.]... Fig. 13.11. A schematic drawing of the potential energy surfaces for the photochemical reactions of stilbene. Approximate branching ratios and quantum yields for the important processes are indicated. In this figure, the ground- and excited-state barrier heights are drawn to scale representing the best available values, as are the relative energies of the ground states of Z- and E -stilbene 4a,4b-dihydrophenanthrene (DHP). [Reproduced from R. J. Sension, S. T. Repinec, A. Z. Szarka, and R. M. Hochstrasser, J. Chem. Phys. 98 6291 (1993) by permission of the American Institute of Physics.]...
The electronic wave function has now been removed from the first two terms while the curly bracket contains tenns which couple different electronic states. The first two of these are the first- and second-order non-adiabatic coupling elements, respectively, vhile the last is the mass polarization. The non-adiabatic coupling elements are important for systems involving more than one electronic surface, such as photochemical reactions. [Pg.55]

About 51 percent of solar energy incident at the top of the atmosphere reaches Earth s surface. Energetic solar ultraviolet radiation affects the chemistry of the atmosphere, especially the stratosphere where, through a series of photochemical reactions, it is responsible for the creation of ozone (O,). Ozone in the stratosphere absorbs most of the short-wave solar ultraviolet (UV) radiation, and some long-wave infrared radiation. Water vapor and carbon dioxide in the troposphere also absorb infrared radiation. [Pg.86]

We cover each of these types of examples in separate chapters of this book, but there is a clear connection as well. In all of these examples, the main factor that maintains thermodynamic disequilibrium is the living biosphere. Without the biosphere, some abiotic photochemical reactions would proceed, as would reactions associated with volcanism. But without the continuous production of oxygen in photosynthesis, various oxidation processes (e.g., with reduced organic matter at the Earth s surface, reduced sulfur or iron compounds in rocks and sediments) would consume free O2 and move the atmosphere towards thermodynamic equilibrium. The present-day chemical functioning of the planet is thus intimately tied to the biosphere. [Pg.7]


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