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Fractional quenching model

Quantitative data are available by fitting the data to the fractional quenching model (15). The Stern-Volmer model is modified by assuming that only a fraction f of the fluorophores can be quenched. The remaining (1-f ) are protected ... [Pg.14]

The block of inter-linked columns offers robust simulation of a combination of complex distillation columns, as heat-integrated columns, air separation system, absorber/stripper devices, extractive distillation with solvent recycle, fractionator/quench tower, etc. Because sequential solution of inter-linked columns could arise convergence problems, a more robust solution is obtained by the simultaneous solution of the assembly of modelling equations of different columns. [Pg.73]

One of the most challenging aspects of modeling turbulent combustion is the accurate prediction of finite-rate chemistry effects. In highly turbulent flames, the local transport rates for the removal of combustion radicals and heat may be comparable to or larger than the production rates of radicals and heat from combustion reactions. As a result, the chemistry cannot keep up with the transport and the flame is quenched. To illustrate these finite-rate chemistry effects, we compare temperature measurements in two piloted, partially premixed CH4/air (1/3 by vol.) jet flames with different turbulence levels. Figure 7.2.4 shows scatter plots of temperature as a function of mixture fraction for a fully burning flame (Flame C) and a flame with significant local extinction (Flame F) at a downstream location of xld = 15 [16]. These scatter plots provide a qualitative indication of the probability of local extinction, which is characterized... [Pg.156]

The reversibility of QM adducts also creates numerous challenges. For example, measuring the full burden of DNA alkylation by a QM can be obscured by the loss of its labile products during or before chemical identification can be completed. Results from a deoxynucleotide model system indicated that only a small fraction of the possible adducts could be measured after the interval required for analysis of DNA. Perhaps the kinetic products of QMs also contribute to the cellular activity of these intermediates although this has yet to be explored. QM equivalents can be envisioned to migrate from one reversible nucleophile such as the N1 of adenine in such cofactors as ATP to another until quenched by a compound such as glutathione that is present in cells as a defense against undesirable electrophiles. [Pg.322]

Thus, at small rj, kb viscosity dependence. At very large viscosities, on the other hand, one may get back a stronger viscosity dependence. An equation like (327) has already been proposed by Sumi and coworkers [167] for isomerization in viscous liquids, although from an entirely different model. The analysis presented here seems to provide an understanding of the eventual quenching of the isomerization rate at very high viscosities. [Pg.192]

At 2000 K and 1 atm, Hollander s state-specific rate constant becomes k. = 1.46 x 1010 exp(-AE/kT) s-1, where AE is the energy required for ionization. For each n-manifold state the fraction ionized by collisions is determined, as well as the fraction transferred to nearby n-manifold states in steps of An = 1. Then the fractions ionized from these nearby n-manifold states are calculated. In this way a total overall ionization rate is evaluated for each photo-excited d state. The total ionization rate always exceeds the state-specific rate, since some of the Na atoms transferred by collisions to the nearby n-manifold states are subsequently ionized. Table I summarizes the values used for the state-specific cross sections and the derived overall ionization and quenching rate constants for each n-manifold state. The required optical transition, ionization, and quenching rates can now be incorporated in the rate equation model. Figure 2 compares the results of the model calculation with the experimental values. [Pg.180]

In Figure 7, we have plotted the response of the fraction active material to quench promoting assembly and (partial) disassembly. The model seems... [Pg.59]

Figure 7 The fraction polymerized material fas a function of the dimensionless time Ty according the kinetic Landau model discussed in the main text, with h the nucleation rate. Shown are results valid in the limit where the nucleation reaction is rate limiting, for a quench to X/Xp = 2 where in equilibrium f— 0.5. Depolymerization is much faster than polymerization. Figure 7 The fraction polymerized material fas a function of the dimensionless time Ty according the kinetic Landau model discussed in the main text, with h the nucleation rate. Shown are results valid in the limit where the nucleation reaction is rate limiting, for a quench to X/Xp = 2 where in equilibrium f— 0.5. Depolymerization is much faster than polymerization.
Figure 19.5 Schematic diagram showing decomposition of total phosphorescence enhancement of PtOEP on silver films into absorption enhancement E X. ) and emissive rate enhancement E (%.2) based on the photophysical model described in the text and data from steady state and transient spectroscopy of PtOEP films with various thicknesses and excitation wavelengths as labeled. The lines represent the possible combinations that could explain the experimentally observed changes in photoluminescence where each position on the line represents a different choice of fQ, the fraction of the excited states that are quenched nonradiatively by interactions between the molecule and the metallic surface. The blue shaded region on the vertical axis is the range of possibilities allowed by constraints from extinction and excitation spectra as explained in the text. The dotted oval is what we believe to be the most likely decomposition for the 6 nm films characterized in Figure 19.4 as discussed in the text. Reprinted from reference 45 with permission of the American Chemical Society. Figure 19.5 Schematic diagram showing decomposition of total phosphorescence enhancement of PtOEP on silver films into absorption enhancement E X. ) and emissive rate enhancement E (%.2) based on the photophysical model described in the text and data from steady state and transient spectroscopy of PtOEP films with various thicknesses and excitation wavelengths as labeled. The lines represent the possible combinations that could explain the experimentally observed changes in photoluminescence where each position on the line represents a different choice of fQ, the fraction of the excited states that are quenched nonradiatively by interactions between the molecule and the metallic surface. The blue shaded region on the vertical axis is the range of possibilities allowed by constraints from extinction and excitation spectra as explained in the text. The dotted oval is what we believe to be the most likely decomposition for the 6 nm films characterized in Figure 19.4 as discussed in the text. Reprinted from reference 45 with permission of the American Chemical Society.
Fig. 2. Polymer fraction vs. irradiation time for a 4-BCMU film, 1300 A thick. Data points are experimental, full curves are obtained for the energy transfer model for various quenching parameters k, = k To (from Ref. >)... Fig. 2. Polymer fraction vs. irradiation time for a 4-BCMU film, 1300 A thick. Data points are experimental, full curves are obtained for the energy transfer model for various quenching parameters k, = k To (from Ref. >)...
Non-Forster fluorescence quenching of trans-etiochlorin by magnesium oc-taethylporphine in phosphatidylcholine vesicles gives evidence for a statistical pair energy trap. Energy transfer also occurs in the excited singlet manifold of chlorophyll. " The photophysics of bis(chlorophyll)-cyclophanes, models of photosynthetic reaction centres, have been explored for use in artificial photosynthesis.Picosecond time-resolved energy transfer in phycobilosomes have also been studied with a tunable laser. The effect of pH on photoreaction cycles of bacteriorhodopsin, " the fluorescence polarization spectra of cells, chromatophores, and chromatophore fractions of Rhodospirillum rubrum, and a brief review of the mechanism and application of artifical photosynthesis are all relevant to the subject of this Chapter. [Pg.37]

The chemical fractionations observed among chondrites and the compositions of many chondritic components are best understood in terms of quenched equilibrium between phases in a nebula of solar composition (Palme, 2001 Chapters 1.03 and 1.15). The equilibrium model assumes that minerals condensed from, or equilibrated with, a homogeneous solar nebula at diverse temperatures. Isotopic variations among chondrites and their components show that this assumption is not correct and detailed petrologic studies have identified relatively few chondritic components that resemble equilibrium nebular products. Nevertheless, the equilibrium model is invaluable for understanding the chemical composition of chondrites and their components as the solar nebular signature is etched deeply into the chemistry and mineralogy. [Pg.150]

Fig. 1. Schematic of model generation. Quench molecular dynamics simulations of a binary mixture (top) produce a series of networked stmcturcs which are processed into adsorbent models (bottom, shown in cutaway view.) The longer the quench is allowed to proceed, the greater the resulting pore size. The porosity of the model materials is detennined by the mole fraction of the quenched mixture. Fig. 1. Schematic of model generation. Quench molecular dynamics simulations of a binary mixture (top) produce a series of networked stmcturcs which are processed into adsorbent models (bottom, shown in cutaway view.) The longer the quench is allowed to proceed, the greater the resulting pore size. The porosity of the model materials is detennined by the mole fraction of the quenched mixture.

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