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Equilibrium differences

An adsorbent can be visualized as a porous soHd having certain characteristics. When the soHd is immersed in a Hquid mixture, the pores fill with Hquid, which at equilibrium differs in composition from that of the Hquid surrounding the particles. These compositions can then be related to each other by enrichment factors that are analogous to relative volatiHty in distillation. The adsorbent is selective for the component that is more concentrated in the pores than in the surrounding Hquid. [Pg.291]

The state of equilibrium differs from the equilibrium between water and pure water vapor in that, in a gas phase, there is also inert gas (dry air) present. This means that the water pressure is equal to the total gas pressure, p -- p, + ph, not to the water vapor pressure p, . [Pg.69]

Other modes of LC operation include liquid-liquid partition chromatography (LLC) and bonded phase chromatography. In the former, a stationary liquid phase which is immiscible with the mobile phase is coated on a porous support, with separation based on partition equilibrium differences of components between the two liquid phases. This mode offers an alternative to ion exchange in the fractionation of polar, water soluble substances. While quite useful, the danger exists in LLC that the stationary phase can be stripped from the column, if proper precautions are not taken. Hence, it is typical to pre-equil-ibrate carefully the mobile and stationary phases and to use a forecolimn, heavily loaded with stationary phase 9). [Pg.227]

Ion partition equilibria at ITIES were first studied by Walther Nemst in 1892. Nemst derived the fundamental relationship linking the equilibrium difference of the inner (or Galvani) potentials, to the ratio of ion concentrations in... [Pg.608]

It is further interesting to observe that the behavior of a system approaching a thermodynamic equilibrium differs little from one approaching a steady state. According to the kinetic interpretation of equilibrium, as discussed in Chapter 16, a mineral is saturated in a fluid when it precipitates and dissolves at equal rates. At a steady state, similarly, the net rate at which a component is consumed by the precipitation reactions of two or more minerals balances with the net rate at which it is produced by the minerals dissolution reactions. Thermodynamic equilibrium viewed from the perspective of kinetic theory, therefore, is a special case of the steady state. [Pg.392]

A 0.5-gram mass of either the organo-treated or inorganic cation exchanged zeolite and 50 mL of 10 mM/L arsenate or chromate aqueous solutions were placed into Erlenmeyer flasks and mechanically shaken in reciprocating mode to attain equilibrium. Different equilibrium periods for individual zeolite modifications and both aqueous oxyanions species have been established. The adsorption isotherm experiments were conducted using above mass/ volume ratio of samples with an initial metal concentrations ranged from 0.5 to 100 mM/L at laboratory temperature. The... [Pg.11]

Abstract Hybrid stars with extremely high central energy density in their core are natural laboratories to investigate the appearance and the properties of compactihed extra dimensions with small compactification radius - if these extra dimensions exist at all. We introduce the necessary formahsm to describe quantitatively these objects and the properties of the formed hydrostatic equilibrium. Different scenarios of the extra dimensions are discussed and the characteristic features of these hybrid stars are calculated. [Pg.297]

No particular relationship between solvent polarity and the observed change is apparent. Rader notes that the experimental conditions are such that no appreciable intramolecular hydrogen-bonding occurs between methanol molecules, presumably ruling out the possibility that the change arises from solvent induced variation of the self-association equilibrium. Differences in solvent-solute association are still a possible interaction mechanism. [Pg.183]

One of these, electron transfer, actually occurs in the ideal definitional sense. It applies to the few overworked redox reactions where there is no adsorbed intermediate. The ion in a cathodic transfer is located in the interfacial region and receives an electron (ferric becomes ferrous) without the nucleus of the ion moving. Later (perhaps as much as 10-9 s later), a rearrangement of the hydration sheath completes itself because that for the newly produced ferrous ion in equilibrium differs (in equilibrium) substantially from that for the ferric. Now (even in the electron transfer case) the ion moves, but the definition remains intact because it moves after electron transfer. The amounts of such small movements (changes in the ion-solvent distance for Fe2+ and Fe3+ ions in equilibrium) are now known from EXAFS measurements. [Pg.780]

The Prisoner s Dilemma equilibrium differs from all the other equilibria mentioned so far, in that it is made up of aaions each of which is the best response to anything others could do, not just to their equilibrium behavior. Equilibrium then does not require a person to have correct expectations about what others will do, since he will take the same action whatever he expects them to do. (An action of this type is called a dominant strategy. 1 If he expects wrongly, he will be surprised, perhaps unpleasantly so, but he will not regret what he did. In such cases there can be unintended consequences in equilibrium. Usually, however, surprise and regret go together. [Pg.113]

Differences in steric hindrance due to overcrowding, in conjugation of the substituents, and in solvation play a subtle role in determining the kinetic and equilibrium differences between 6 and 9. [Pg.341]

Macrosyneresis, in which the network polymer is contained only in one phase is not the only possibility for phase equilibria in networks. Under favorable conditions two polymer phases can coexist in a network with a diluent phase (50). The two polymer phases in equilibrium differ in the conformations of the network chains. The transition resembles the condensation of a real gas or, in macromolecules, an intramolecular transition due to long-range net attraction between segments in a poor solvent (coil-globule type transition [139)). [Pg.55]

The electrochemical interface is the site where electrode reactions take place. At equilibrium, differences of chemical potential in the electrode and electrolyte bring about differences in electrical potential across the interface. The structure and models of such an electrochemical interface will be discussed in Sect. 2.3. [Pg.4]

These three different T parameters are related to each other and to the total number of RNA charges, Z (see T relationships in Fig. 21.IB). First, the number of KC1 pairs lost from the left hand side during the approach to equilibrium is the same as the equilibrium difference in the number of Cl-ions between the two chambers, TKci = r. Electroneutrality also requires that T+ = F + Z, that is, the left side excess of cations (relative to the right side solution) must be balanced by an equivalent number of negative charges (note that T < 0). [Pg.438]

This simple calculation indicates that if H+ were passively distributed across the plasma membrane, and for a mean membrane potential of-60 mV, intracellular pH values (pHi) would be expected to be 1 pH unit lower than the external pH values (pHo). Numerous experiments performed on a large variety of cells indicate, however, that pHi values are usually close to pHo values, or slightly below (Roos and Boron, 1981). This implies that H+ ions are not passively distributed across the plasma membrane and that H+ pumps drive H+ out of equilibrium. Different H+ pumps have been identified in eukaryotic cells an ubiquitous Na+/H+ exchanger, and pumps that have a more restricted cellular distribution. These are (H+)ATPases,... [Pg.152]

Now consider the kinetics of the flow of spins between spin states. For each pair of spin states, we calculate the difference in population and compare it to the equilibrium difference. If these two are not the same, there will be a flow of spins from the overpopulated state to the underpopulated state at a rate that is proportional to the rate constant for that transition and to the amount by which the transition is out of equilibrium. The rate constants, or relaxation rates, for each transition are determined by... [Pg.410]

Consider first the single-quantum transition between the afi and pp states (Ha(2) transition, Fig. 10.1). This is an Ha transition with relaxation rate W. The equilibrium difference in population for this transition is Pap — Ppp = 28. If this equality does not hold, then the overpopulation of the pp state is given by Ppp — Pap + 28, and the rate of spins dropping down from the pp state to the ap state is Wf(Ppp — Pap + 28). If this were the only transition available (i.e., if there were no double-quantum or zero-quantum pathways), we could write down the rate of change of population as... [Pg.411]

Note that the equilibrium difference across the DQ transition (Paa - Ppp) is 45 because the energy separation is twice that of an SQ transition. Combining all three terms,... [Pg.412]

Figure 2.2 Concentration equilibrium. Difference in height corresponds to osmotic pressure of the solution. Figure 2.2 Concentration equilibrium. Difference in height corresponds to osmotic pressure of the solution.
Under the condition of electroneutrality, Eq. (10.1) describes the Donnan equilibrium across a membrane, which separates solutions containing nonpermeating ions. With the Donnan equilibrium, differences of pressure and electric potential will appear. If the nonpermeating components are electrically neutral, only the pressure difference occurs. [Pg.506]

The equilibrium difference between the Gibbs free energies of interaction of an SWNT with its surroundings, in the solid phase and in the cluster volume or on... [Pg.113]

Yet different isotopes have, also by definition, different masses, and because of this their chemical properties are not identical the same reactions can occur but at somewhat c[ifferent rates (or, for reversible reactions, with different positions of equilibrium)/ difference in rate (or position of equilibrium) due to a difference in the isotope present in the reaction system is called an isotope effect. ... [Pg.353]

It may seem strange that the droplet growth law is so different in form from the transpon-limited law. After all. the gas-phase species mu.st be transponed to the droplets. Actually, both laws are obeyed. The explanation is that the reactive species are nearly in equilibrium in the gas and droplet phases. Their small displacement from equilibrium differs, however. depending on droplet xfee. but not sufficiently to affect the rate of reaction in solution. [Pg.287]

Melting equilibrium. Different ice-water mixtures are produced, stirred for some time, and measured with the thermometer (see E6.1) the temperatures are always 0°C. The following melting equilibrium exists ... [Pg.156]

The apparent discrepancy between the results of Saegusa497) and of Penczek191) reflects the effect of the concentration of ionic species upon the equilibrium. Different concentrations of initiator were used by these workers and the higher its concentration, the higher the concentration of oxonium ions in the system. This, in turn, reduces the activity coefficient of the ether leading to higher [THF]e. [Pg.20]


See other pages where Equilibrium differences is mentioned: [Pg.135]    [Pg.187]    [Pg.4]    [Pg.311]    [Pg.294]    [Pg.84]    [Pg.357]    [Pg.188]    [Pg.191]    [Pg.259]    [Pg.260]    [Pg.628]    [Pg.41]    [Pg.1879]    [Pg.113]    [Pg.662]    [Pg.396]    [Pg.44]    [Pg.651]    [Pg.118]    [Pg.6382]   
See also in sourсe #XX -- [ Pg.137 ]




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Energy difference, equilibrium

Energy difference, equilibrium position and

Equilibria Between Complexes with Different Coordination Numbers

Equilibrium between different phases

Equilibrium between different phases in ideal solutions

Equilibrium constant different forms

Equilibrium electrode potential difference

Equilibrium population difference

Equilibrium potential difference

Equilibrium-dispersive model finite difference methods

Estimations based on experimental values of equilibrium constants at different ionic strength

Evaluation of Equilibrium Constants at Different Temperatures

Interfacial potential difference partition equilibrium

Organic reaction mechanisms energy difference, equilibrium constant

Results for Different Chemical Equilibrium Constants

Shapes of different equilibrium adsorption isotherms

Thermal equilibrium, between different spin

Thermal equilibrium, between different spin states

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