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Transition-state theory Conventional

Three possibilities were considered to account for the curved Arrhenius plots and unusual KIEs (a) the 1,2-H shift might feature a variational transition state due to the low activation energy (4.9 kcal/mol60) and quite negative activation entropy (b) MeCCl could react by two or more competing pathways, each with a different activation energy (e.g., 1,2-H shift and azine formation by reaction with the diazirine precursor) (c) QMT could occur.60 The first possibility was discounted because calculations by Storer and Houk indicated that the 1,2-H shift was adequately described by conventional transition state theory.63 Option (b) was excluded because the Arrhenius curvature persisted after correction of the 1,2-H shift rate constants for the formation of minor side products (azine).60... [Pg.73]

The simplest generalization of free-energy-of-solvation concepts to dynamics in solution is provided by transition state theory. In conventional transition state theory, the rate constant of a chemical reaction at temperature T is given by... [Pg.61]

If only the solvation of the gas-phase stationary points are studied, we are working within the frame of the Conventional Transition State Theory, whose problems when used along with the solvent equilibrium hypothesis have already been explained above. Thus, the set of Monte Carlo solvent configurations generated around the gas-phase transition state structure does not probably contain the real saddle point of the whole system, this way not being a correct representation of the conventional transition state of the chemical reaction in solution. However, in spite of that this elemental treatment... [Pg.138]

Free energy is the key quantity that is required to determine the rate of a chemical reaction. Within the Conventional Transition State Theory, the rate constant depends on the free energy barrier imposed by the conventional transition state. On the other hand, in the frame of the Variational Transition State Theory, the free energy is the magnitude that allows the location of the variational transition state. Then, it is clear that the evaluation of the free energy is a cornerstone (and an important challenge) in the simulation of the chemical reactions in solution... [Pg.139]

In both solvents, the variational transition state (associated with the free energy maximum) corresponds, within the numerical errors, to the dividing surface located at rc = 0. It has to be underlined that this fact is not a previous hypothesis (which would rather correspond to the Conventional Transition State Theory), but it arises, in this particular case, from the Umbrella Sampling calculations. However, there is no information about which is the location of the actual transition state structure in solution. Anyway, the definition of this saddle point has no relevance at all, because the Monte Carlo simulation provides directly the free energy barrier, the determination of the transition state structure requiring additional work and being unnecessary and unuseful. [Pg.146]

Vibrational frequencies for various normal modes must be estimated and active as well as inactive energies should be decided. Numerical methods may be used to calculate rate constant k at various concentrations obtained by RRKM theory. The rate constant has been found to be same as given by conventional transition state theory, i.e. [Pg.108]

The top of the profile is maximum (saddle point) and is referred as the transition state in the conventional transition state theory. It is called a saddle point because it is maximum along the orthogonal direction (MEP) while it is minimum along diagonal direction of Fig. 9.12. The minimum energy path can be located by starting at the saddle point and mapping out the path of the deepest descent towards the reactants and products. This is called the reaction path or intrinsic reaction coordinate. [Pg.218]

In conventional transition state theory (TST) (see Chapter 4) the first approximation for the thermal rate constant k is given ... [Pg.181]

The Basics of Variational Transition State Theory and How It Differs from Conventional Transition State Theory... [Pg.182]

TST = conventional Transition State Theory, ICVT = Improved Canonical Variational Transition state theory, ICVT/SCT = ICVT/Small Curvature Tunneling, ICVT/p,OMT = ICVT/Microcanonical Optimized Multidimensional Tunneling. [Pg.200]

The rate constant ka(E) of Equation 14.3 is the rate constant which is calculated by transition state theory. Analogously to the discussion in Chapter 4 of conventional transition state theory, where chemical equilibrium is between reactants and transition state, it will be assumed here that an equilibrium exists between A (excited A molecules with vibrational energy E, equal to or larger than Eo, the minimum... [Pg.431]

As in the conventional transition state theory Equation 14.27 does not contain any reference to the mass of the reaction coordinate motion or to the length l of the transition state. While some aspects of the derivation have been skipped, it is hoped that the reader understands that the expression in the numerator for the sum of the vibrational energy levels in the transition state arises from Equation 14.25 which applies to the transition state but not to the excited molecule A. ... [Pg.435]

The formidable problems that are associated with the interpretation of LP kinetic data for nonstatistical IM reactions can be entirely avoided if the reactions can be studied in the HPL of kinetic behavior. In the HPL, the energy content of the initially formed species, X and Y, in reaction (2) would be very rapidly changed by collisions with the buffer gas so that the altered species, X and Y, would have normal Boltzmann distributions of energy. Furthermore, those Boltzmann energy distributions would be continuously refreshed as the most energetic X and Y within the distributions move forwards or backwards along the reaction coordinate. The interpretation of rate constants measured in the HPL is expected to be relatively straightforward because conventional transition-state theory can then be applied. [Pg.225]

Kramers [67], Northrup and Hynes [103], and also Grote and Hynes [467] have considered the less extreme case of reaction in the liquid phase once the reactants are in collision where such energy diffusion is not rate-limiting. Let us suppose we could evaluate the (transition state) rate coefficient for the reaction in the gas phase. The conventional transition state theory needs to be modified to include the effect of the solvent motion on the motion of the reactants as they approach the top of the activation barrier. Kramers [67] used a simple model of the... [Pg.231]

Transition-state theory is one of the earliest attempts to explain chemical reaction rates from first principles. It was initially developed by Eyring [124] and Evans and Polayni [122,123], The conventional transition-state theory (CTST) discussed here provides a relatively straightforward method to estimate reaction rate constants, particularly the preexponential factor in an Arrhenius expression. This theory is sometimes also known as activated complex theory. More advanced versions of transition-state theory have also been developed over the years [401],... [Pg.415]

Further simplification gives the well-known expression for the conventional transition-state theory rate constant ... [Pg.418]

This result is equivalent to Eq. (5.53), the classical version of what is known as conventional transition-state theory, to be discussed in detail in subsequent chapters. [Pg.129]

In conventional transition-state theory, we place the dividing surface between reactants and products at the saddle point, perpendicular to the minimum-energy path, and focus our attention on the activated complex. That is, we write the reaction... [Pg.141]

In this section, we present a derivation of the conventional transition-state theory expression for the rate constant, Eq. (6.8), that avoids the artificial constructs of the... [Pg.145]

The rate constant predicted by conventional transition-state theory can turn out to be too small, compared to experimental data, when quantum tunneling plays a role. We would like to correct for this deviation, in a simple fashion. That is, to keep the basic theoretical framework of conventional transition-state theory, and only modify the assumption concerning the motion in the reaction coordinate. A key assumption in conventional transition-state theory is that motion in the reaction coordinate can be described by classical mechanics, and that a point of no return exists along the reaction path. [Pg.146]

The basic expressions for the rate constant within a fully classical version of conventional transition-state theory were derived in Chapter 5. According to Eq. (5.53), we may write... [Pg.241]

In Kramers theory that is based on the Langevin equation with a constant time-independent friction constant, it is found that the rate constant may be written as a product of the result from conventional transition-state theory and a transmission factor. This factor depends on the ratio of the solvent friction (proportional to the solvent viscosity) and the curvature of the potential surface at the transition state. In the high friction limit the transmission factor goes toward zero, and in the low friction limit the transmission factor goes toward one. [Pg.262]

It should be emphasized that these dynamical effects can lead to significant corrections to conventional transition-state theory where recrossings are neglected. However,... [Pg.263]

The application of isotope effects studies of reaction mechanism includes comparison of experimental values of isotope effects and predicted isotope effects computed for alternative reaction pathways. On the basis of such analysis some of the pathways may be excluded. Theoretical KIEs are calculated using the method of Bigeleisen and Mayer.1 55 KIEs are a function of transition state and substrate vibrational frequencies. Equilibrium isotope effects are calculated from substrate and product data. Different functionals and data sets are used in these calculations. Implementation of a one-dimensional tunnelling correction into conventional transition-state theory significantly improved the prediction of heavy-atom isotope effects.56 Uncertainty of predicted isotope effect can be assessed from the relationship between KIEs and the distances of formed or broken bonds in the transition states, calculated for different optimized structures.57 Calculations of isotope effects from sets of frequencies for optimized structures of reactants and transition states are facilitated by adequate software QUIVER58 and ISOEFF.59... [Pg.159]

Thus, based on NHIMs with saddles with index 1, we can construct a theory that is a rigorous reformulation of the conventional Transition State Theory [9,10]. Moreover, the use of the Lie perturbation brings the system locally into the Birkhoff normal form with one inverse harmonic potential [2]. This form is nothing but the Fenichel normal form. [Pg.339]

The principal focus of the present article is on the "mass-independent isotope fractional effect" (MIF) found in atmospheric and laboratory produced ozone. When this MIF occurs, a plot of the positive or negative "enrichment" in samples versus that of in those same samples has a slope of approximately unity, rather than its typical value of about 0.52. The 0.52 is the value expected using conventional transition state theory when nuclear tunneling effects are absent. For an isotope Q, 5Q is defined in per mil as 1000 [(Q/0)/(Q/0)std - 1]/ where Q/O is the ratio of Q to in the sample and std refers to its value in some standard sample, standard mean ocean water. An example of a three-isotope plot showing a slope of 0.52 is given in Figure 2.1. [Pg.9]

Chemical kinetic rate methods including conventional transition state theory (TST), canonical variational transition state theory (CVTST) and Rice-Ramsper-ger-Kassel-Marcus in conjunction with master equation (RRKM/ME) and separate statistical ensemble (SSE) have been successfully applied to the hydrocarbon oxidation. Transition state theory has been developed and employed in many disciplines of chemistry [41 4]. In the atmospheric chemistry field, conventional transition state theory is employed to calculate the high-pressure-limit unimole-cular or bimolecular rate constants if a well-defined transition state (i.e., a tight... [Pg.179]


See other pages where Transition-state theory Conventional is mentioned: [Pg.74]    [Pg.126]    [Pg.127]    [Pg.148]    [Pg.151]    [Pg.232]    [Pg.184]    [Pg.186]    [Pg.188]    [Pg.382]    [Pg.382]    [Pg.435]    [Pg.439]    [Pg.25]    [Pg.256]    [Pg.121]    [Pg.148]    [Pg.149]    [Pg.211]    [Pg.343]    [Pg.338]   
See also in sourсe #XX -- [ Pg.305 ]

See also in sourсe #XX -- [ Pg.415 ]




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