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Height, energy barrier

In prineiple, nothing more is neeessary to understand the infiuenee of the solvent on the TST rate eonstant than the modifieation of the PMF, and the resulting ehanges in the free energy barrier height should be viewed as the dominant effeet on the rate sinee tliese ehanges appear in an exponential fonn. As an example, an error... [Pg.888]

Figure 2.3. Tunnelling of a wave with kinetic energy E through a rectangular potential energy barrier, height V. The narrower the barrier, the smaller the mass of the particle and the smaller the difference between V and E, the greater the tunnelling probability. If the amplitude of the wave has not reached zero at the far side of the barrier, it will stop decaying and resume the oscillation it had on entering the barrier (but with smaller amplitude). Figure 2.3. Tunnelling of a wave with kinetic energy E through a rectangular potential energy barrier, height V. The narrower the barrier, the smaller the mass of the particle and the smaller the difference between V and E, the greater the tunnelling probability. If the amplitude of the wave has not reached zero at the far side of the barrier, it will stop decaying and resume the oscillation it had on entering the barrier (but with smaller amplitude).
Fig. 14. Potential energy barrier heights as calculated using ab initio theory for insertion of transition metal atoms into a C-H or C-C bond of (a) ethane and (b) cyclopropane. Values taken from Ref. 22. Fig. 14. Potential energy barrier heights as calculated using ab initio theory for insertion of transition metal atoms into a C-H or C-C bond of (a) ethane and (b) cyclopropane. Values taken from Ref. 22.
DFT method combined with a cluster model approach was compared regarding its suitability for describing both structures and energy profiles. This study shows that the relative stability and geometry depend on the cluster sizes in agreement with previous studies [15] but shows that the energy barrier heights of the reaction processes are not affected. [Pg.372]

If, as above, the potential-energy barrier height is E, statistical mechanical considerations indicate that the atom will have sufficient thermal energy to pass over the barrier a fraction exp(— E/k T) of the time. If/is a characteristic atomic vibrational frequency, the probability p that during unit time the atom will pass the potential-energy barrier is given by... [Pg.310]

In Equation 21, T is the absolute temperature, h is Planck s constant, is Boltzmann constant, and AG is the free energy barrier height relative to infinitely-separated reactants. The temperature-dependent factor r(7) represents quantum mechanical tunneling and the Wigner approximation to tunneling through an inverted parabolic barrier ... [Pg.90]

These two examples clearly demonstrate that Ea is not equal to Eq- The temperature dependence of Ea will, however, often be negligible since typically kbT -C Eo-Thus, we have a rough identification of Ea with Eo- It should be remembered that this is not the potential energy barrier height, Ec, but the difference in zero-point energies between the activated complex and the reactants. [Pg.218]

The energy barrier height of reversal is estimated as 1.0 x 10"10 erg. The energy corresponds to the switching volume comparable with the volume of... [Pg.282]

In order to overcome the reaction barrier within current restrictions of computer time, the hydrogen coordination number of the hydroxylic oxygen was forced to decrease from unity to zero by applying a suitable constraint [47, 88, 89], By thermodynamic integration it is possible to determine the free energy barrier height for this process [19]. [Pg.280]

Figure 7. Calculated two-dimensional energy surfaces for heterogeneous non-Franck-Condon transition of the three-dimensional 6-oscillator trikisoctahedral Inner Shells of 3+ and 2+ ions at (A) equal potential energies after ground state energy correction (B) at equal ground state free energies. Barrier height in B +22.9kT at 298 K (+56.9 kJ/mole, +0.59 eV, experimentally +0.59 eV177). Figure 7. Calculated two-dimensional energy surfaces for heterogeneous non-Franck-Condon transition of the three-dimensional 6-oscillator trikisoctahedral Inner Shells of 3+ and 2+ ions at (A) equal potential energies after ground state energy correction (B) at equal ground state free energies. Barrier height in B +22.9kT at 298 K (+56.9 kJ/mole, +0.59 eV, experimentally +0.59 eV177).
These six isoenergetic configurations are not necessarily the energetically lowest ones. However, they may be assumed to be for our purposes, and if the energy barrier height between the minima are sufficiently low then inter-conversion movements can occur. The Hamiltonian operator corresponding to such a movement may be transcribed if we take into account ... [Pg.38]

Although all theoretical approaches discussed in previous sections do refer to a particular molecular model, rather they represent attempts to rationalize experimental kinetic data in terms of mean values of electrical field or ion distribution, energy barrier height, energy change, ion mobility and viscosity of medium, which are all supposed to be closely related to the molecular properties of the ions and solvent molecules involved. However, no direct link to molecular properties has been established within the framework of the models discussed above. [Pg.327]

Eb supermoment reversal energy barrier height or barrier function of 0... [Pg.219]


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See also in sourсe #XX -- [ Pg.220 ]




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