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Critical energy barrier

Investigations on various salts in these solvents show that competition between ion-ion and ion-solvent interactions with increasing salt concentration leads to comparable states of the different solutions at their respective maximum conductance i.e. the maximum specific conductance for every solution is obtained when the conductance-determining effects have established a critical energy barrier which depends almost exclusively on solvent and temperature and not on the solute. As an important consequence, in spite of large ion-ion association constants, the maximum specific conductance can be found at unexpectedly high K a,(-values in solvents of low permittivity This feature can be used advantageously for technical... [Pg.62]

Fig. 3. Curve ihustrating the activation energy (barrier) to nucleate a crystalline phase. The critical number of atoms needed to surmount the activation barrier of energy AG is n and takes time equal to the iacubation time. One atom beyond n and the crystahite is ia the growth regime. Fig. 3. Curve ihustrating the activation energy (barrier) to nucleate a crystalline phase. The critical number of atoms needed to surmount the activation barrier of energy AG is n and takes time equal to the iacubation time. One atom beyond n and the crystahite is ia the growth regime.
Below a critical size the particle becomes superparamagnetic in other words the thermal activation energy kTexceeds the particle anisotropy energy barrier. A typical length of such a particle is smaller than 10 nm and is of course strongly dependent on the material and its shape. The reversal of the magnetization in this type of particle is the result of thermal motion. [Pg.176]

Studies based on the Frenkel-Kontorova model reveal that static friction depends on the strength of interactions and structural commensurability between the surfaces in contact. For surfaces in incommensurate contact, there is a critical strength, b, below which the depinning force becomes zero and static friction disappears, i.e., the chain starts to slide if an infinitely small force F is applied (cf. Section 3). This is understandable from the energetic point of view that the interfacial atoms in an incommensurate system can hardly settle in any potential minimum, or the energy barrier, which prevents the object from moving, can be almost zero. [Pg.181]

There are also voices critical of the rTCA cycle Davis S. Ross has studied kinetic and thermodynamic data and concludes that the reductive, enzyme-free Krebs cycle (in this case the sequence acetate-pyruvate-oxalacetate-malate) was not suitable as an important, basic reaction in the life evolution process. Data on the Pt-catalysed reduction of carbonyl groups by phosphinate show that the rate of the reaction from pyruvate to malate is much too low to be of importance for the rTCA cycle. In addition, the energy barrier for the formation of pyruvate from acetate is much too high (Ross, 2007). [Pg.198]

Polymer crystallization is usually initiated by nucleation. The rate of primary nucleation depends exponentially on the free-energy barrier for the formation of a critical crystal nucleus [ 110]. If we assume that a polymer crystallite is a cylinder with a thickness l and a radius R, then the free-energy cost associated with the formation of such a crystallite in the liquid phase can be expressed as... [Pg.19]

The natural questions that arise are what constitutes the stems, how the stems (if they exist) get attached at the growth front, what the free-energy barriers are, etc. The molecular modeling has provided vivid details for these questions, and has shown that the assumptions of the LH model are not valid in any universal way. The simulation results have clearly underscored the need for new theories of polymer crystallization by providing credence to the criticisms of the LH theory. [Pg.240]

The nucleation time r, i. e.. the time needed to form a critical droplet of deconfined quark matter, can be calculated for different values of the stellar central pressure Pc which enters in the expression of the energy barrier in Eq. (5). The nucleation time can be plotted as a function of the gravitational mass... [Pg.362]

Nucleation. The energy barrier and the nucleation rate depend critically on the supersaturation. [Pg.215]


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