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Activation energy with excited species

The overall requirement is 1.0—2.0 s for low energy waste compared to typical design standards of 2.0 s for RCRA ha2ardous waste units. The most important, ie, rate limiting steps are droplet evaporation and chemical reaction. The calculated time requirements for these steps are only approximations and subject to error. For example, formation of a skin on the evaporating droplet may inhibit evaporation compared to the theory, whereas secondary atomization may accelerate it. Errors in estimates of the activation energy can significantly alter the chemical reaction rate constant, and the pre-exponential factor from equation 36 is only approximate. Also, interactions with free-radical species may accelerate the rate of chemical reaction over that estimated solely as a result of thermal excitation therefore, measurements of the time requirements are desirable. [Pg.56]

This contrasts to the situation for the oxirane radical cation, for which the nature of the species observed experimentally in frozen matrices was long disputed [63], Tomasi and his group [64] first reported calculations on the fate of the oxirane radical cation produced by vertical excitation. Later calculations [65-67] all agree that the C- C ring-opened product 15 is formed from the oxirane radical cation with a low activation energy and that this is the structure observed in frozen matrices. Remarkably, the prototype W.-H. electrocyclic... [Pg.14]

In complete equilibrium, the ratio of the population of an atomic or molecular species in an excited electronic state to the population in the groun d state is given by Boltzmann factor e — and the statistical weight term. Under these equilibrium conditions the process of electronic excitation by absorption of radiation will be in balance with electronic deactivation by emission of radiation, and collision activation will be balanced by collision deactivation excitation by chemical reaction will be balanced by the reverse reaction in which the electronically excited species supplies the excitation energy. However, this perfect equilibrium is attained only in a constant-temperature inclosure such as the ideal black-body furnace, and the radiation must then give -a continuous spectrum with unit emissivity. In practice we are more familiar with hot gases emitting dis-... [Pg.527]

It might be thought that photoisomerization and photoaquation could be competitive towards a common precursor excited state, but this explanation fails on quantitative testing. Briefly, the quantum yield for photoaquation is too high to accommodate its negative apparent activation energy. Photoaquation must then be competitive with some other process such as deactivation, or return to the original cis species. [Pg.243]

The threshold energy or activation energy for the reaction of atomic fluorine with hydrocarbons (79, 80) or hydrogen (81) is near zero, and these reactions, in fact, produce a similar set of HF molecules in excited vibrational states. In a variety of studies by various techniques, the reactions of F and F2 with such species are generally reported to have activation energies of... [Pg.203]

Non thermally Activated Unimolecular Reactions. Consider the steady-state system in which an excited species, M, is formed with an energy distribution/(e). The situation is represented by eq. (18), where D and S are the experimentally measured decomposition and stabilization products, respectively,... [Pg.35]


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See also in sourсe #XX -- [ Pg.240 , Pg.242 ]




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Activated species

Activation energy species

Active species

Active specy

Excitation energy

Excited species

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