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The equilibrium state

Aqueous geochemists work daily with equations that describe the equilibrium points of chemical reactions among dissolved species, minerals, and gases. To study an individual reaction, a geochemist writes the familiar expression, known as the mass action equation, relating species activities to the reaction s equilibrium constant. In this chapter we carry this type of analysis a step farther by developing expressions that describe the conditions under which not just one but all of the possible reactions in a geochemical system are at equilibrium. [Pg.29]

How can we express the equilibrium state of such a system A direct approach would be to write each reaction that could occur among the system s species, minerals, and gases. To solve for the equilibrium state, we would determine a set of concentrations that simultaneously satisfy the mass action equation corresponding to each possible reaction. The concentrations would also have to add up, together with the mole numbers of any minerals in the system, to give the system s bulk composition. In other words, the concentrations would also need to satisfy a set of mass balance equations. [Pg.29]

Such an approach, however, is unnecessarily difficult to carry out. Dissolving even a few elements in water produces many tens of species that need to be considered, and complex solutions contain many hundreds of species. Each species represents an independent variable, namely its concentration, in our scheme. For [Pg.29]

Fortunately, few of these variables are truly independent. Geochemists have developed a variety of numerical schemes to solve for equilibrium in multicomponent systems, each of which features a reduction in the number of independent variables carried through the calculation. The schemes are alike in that each solves sets of mass action and mass balance equations. They vary, however, in their choices of thermodynamic components and independent variables, and how effectively the number of independent variables has been reduced. [Pg.30]

In this chapter we develop a description of the equilibrium state of a geochemical system in terms of the fewest possible variables and show how the resulting equations can be applied to calculate the equilibrium states of natural waters. We reserve for the next two chapters discussion of how these equations can be solved by using numerical techniques. [Pg.30]

The statistical interpretation of the trend towards equilibrium has been discussed in 1 17 and 1 18, and the significant points will be briefiy summarized. Consider any closed macroscopic system of chosen energy and volume. In general, the statement of the values of these variables is sufficient to fix neither the thermodynamic state of the system nor the value of Cl. Thus we need to know in addition whether the volume is divided internally by means of impermeable or non-conducting partitions, and also what catalysts are present. In brief, we need to know what quantum states are accessible to the system. [Pg.338]

The removal of a partition or the introduction of a catalyst is the lifting of a restraint. They may result in either of the two possibilities either the system stays as it was, with the same value of or it undergoes an internal change, such as the fiow of energy or of matter, or a chemical reaction. This is equivalent to an increase in 11, the number of quantum states which the system can take up, each of [Pg.338]

It may be remarked, once again, that the need for the basic postu-late arises because it cannot be predicted which one of the Cl states the system will actually be in, at any given moment. Failing the possibility of prediction the next best thing is to assume that the system is as likely to be in any one of the quantum states as any other. [Pg.339]

So much for the effect of lifting a restraint. In the converse case, where a partition is inserted, or a catalyst is removed, the value of Cl, or at any rate the value of In 1, is not significantly affected. Intuitively this is fairly plausible, and we shall not seek to prove it in detail if a gas is uniformly distributed throughout a vessel, the replacement of a partition between the two halves of the vessel does not cause any significant decrease in the logarithm of the number of accessible quantum states. [Pg.339]


In considering isotherm models for chemisorption, it is important to remember the types of systems that are involved. As pointed out, conditions are generally such that physical adsorption is not important, nor is multilayer adsorption, in determining the equilibrium state, although the former especially can play a role in the kinetics of chemisorption. [Pg.698]

The populations, /Q, appear on the diagonal as expected, but note that there are no off-diagonal elements—no coherences this is reasonable since we expect the equilibrium state to be time-independent, and we have associated the coherences with time. [Pg.233]

The equilibrium state for a gas of monoatomic particles is described by a spatially unifonn, time independent distribution fiinction whose velocity dependence has the fomi of the Maxwell-Boltzmaim distribution, obtained from equilibrium statistical mechanics. That is,/(r,v,t) has the fomi/" (v) given by... [Pg.666]

Radiation probes such as neutrons, x-rays and visible light are used to see the structure of physical systems tlirough elastic scattering experunents. Inelastic scattering experiments measure both the structural and dynamical correlations that exist in a physical system. For a system which is in thennodynamic equilibrium, the molecular dynamics create spatio-temporal correlations which are the manifestation of themial fluctuations around the equilibrium state. For a condensed phase system, dynamical correlations are intimately linked to its structure. For systems in equilibrium, linear response tiieory is an appropriate framework to use to inquire on the spatio-temporal correlations resulting from thennodynamic fluctuations. Appropriate response and correlation functions emerge naturally in this framework, and the role of theory is to understand these correlation fiinctions from first principles. This is the subject of section A3.3.2. [Pg.716]

Here L is the Onsager coefficient and the minus sign (-) indicates that the concentration flow occurs from regions of high p to low p in order that the system irreversibly flows towards the equilibrium state of a... [Pg.720]

The exponential fiinction of the matrix can be evaluated tln-ough the power series expansion of exp(). c is the coliinm vector whose elements are the concentrations c.. The matrix elements of the rate coefficient matrix K are the first-order rate constants W.. The system is called closed if all reactions and back reactions are included. Then K is of rank N- 1 with positive eigenvalues, of which exactly one is zero. It corresponds to the equilibrium state, witii concentrations r detennined by the principle of microscopic reversibility ... [Pg.790]

Relationships from thennodynamics provide other views of pressure as a macroscopic state variable. Pressure, temperature, volume and/or composition often are the controllable independent variables used to constrain equilibrium states of chemical or physical systems. For fluids that do not support shears, the pressure, P, at any point in the system is the same in all directions and, when gravity or other accelerations can be neglected, is constant tliroughout the system. That is, the equilibrium state of the system is subject to a hydrostatic pressure. The fiindamental differential equations of thennodynamics ... [Pg.1956]

A simple, non-selective pulse starts the experiment. This rotates the equilibrium z magnetization onto the v axis. Note that neither the equilibrium state nor the effect of the pulse depend on the dynamics or the details of the spin Hamiltonian (chemical shifts and coupling constants). The equilibrium density matrix is proportional to F. After the pulse the density matrix is therefore given by and it will evolve as in equation (B2.4.27). If (B2.4.28) is substituted into (B2.4.30), the NMR signal as a fimction of time t, is given by (B2.4.32). In this equation there is a distinction between the sum of the operators weighted by the equilibrium populations, F, from the unweighted sum, 7. The detector sees each spin (but not each coherence ) equally well. [Pg.2100]

Naturally, the study of non-cquilibriti m properties in vo Ives different criteria alth ough the equilibrium stale and cvoltilion towards the equilibrium state may be important. [Pg.316]

In Ihc canonical, microcanonical and isothermal-isobaric ensembles the number of particles is constant but in a grand canonical simulation the composition can change (i.e. the number of particles can increase or decrease). The equilibrium states of each of these ensembles are cha racterised as follows ... [Pg.321]

Our aim is to analyze the solution properties of the variational inequality describing the equilibrium state of the elastic plate. The plate is assumed to have a vertical crack and, simultaneously, to contact with a rigid punch. [Pg.107]

The inequahty apphes to all incremental changes toward the equilibrium state, whereas the equahty holds at the equilibrium state where any change is reversible. [Pg.534]

Since the phase rule treats only the intensive state of a system, it apphes to both closed and open systems. Duhem s theorem, on the other hand, is a nJe relating to closed systems only For any closed system formed initially from given masses of preseribed ehemieal speeies, the equilibrium state is completely determined by any two propeities of the system, provided only that the two propeities are independently variable at the equilibrium state The meaning of eom-pletely determined is that both the intensive and extensive states of the system are fixed not only are T, P, and the phase compositions established, but so also are the masses of the phases. [Pg.535]

The activities in Eq. (4-342) provide the connection between the equilibrium states of interest and the standard states of the constituent species, for which data are presumed available. The standard states are alwavs at the equihbrium temperature. Although the standard state need not be the same for all species, or Sipaliicular species it must be the state represented by both Gf and thej ° upon which the activity dj is based. [Pg.542]

The partial pressure of water vapor in air cannot be higher than the vapor pressure of saturated water ft (T) corresponding to air temperature T. If it were higher, condensation of water vapor would occur until the equilibrium state corresponding to the saturated vapor pressure was achieved. [Pg.71]

The plate buckling equations inherently cannot be derived from the equilibrium of a differential element. Instead, the buckling problem represents the departure from the equilibrium state when that state becomes unstable because the in-plane load is too high. The departure from the equilibrium state is accompanied by waves or buckles in the surface of the plate. That is, the plate cannot remain flat when the... [Pg.505]

The irreversible step is irrelevant to the following argument, which is based on the equilibrium state. Proceeding to define equilibrium constants as Ki = k,/k i = [IH]/[ImH][L] and so on, we obtain the identity... [Pg.127]

It is known that polymers may exist in various stationary states, which are defined by the amount and distribution of intermolecular bonds in the sample at definite network structure. The latter is defined by the conditions of storage, exploitation, and production of the network. That is why T values may be different. The highest value is observed in the equilibrium state of the system. In this case it is necessary to point out, that the ph value becomes close to the ph one at n,. [Pg.366]

The most important result of this work is that despite two different SRO patterns, we have found concentration independent EPI. The evolution of the diffuse intensity with composition is thus mainly due to the sensitivity of the equilibrium state (i.e. the correlation function) to the concentration. [Pg.36]

Consider the equilibrium state of the system assuming that m grams of n-heptane are dissolved in the benzene phase. Then the mass fraction of n-heptanc in this phase is to. 2 = m/(400 + m). [Pg.351]

Most traditional models focus on looking for equilibrium solutions among some set of (pre-defined) aggregate variables. The LEs are effectively mean-field equations, in which certain variables (i.e. attrition rate) are assumed to represent an entire force, the equilibrium state is explicitly solved for and declared the battle outcome. In contrast, ABMs focus on understanding the kinds of emergent patterns that might arise while the overall system is out of (or far from) equilibrium. [Pg.601]

Consideration of the dissolving of iodine in an alcohol-water mixture on the molecular level reveals the dynamic nature of the equilibrium state. The same type of argument is applicable to vapor pressure. [Pg.145]

By direct visual observation we can watch the contents of these two bulbs approach the constancy of macroscopic properties (in this case,, color) that indicates equilibrium. In bulb A equilibrium was approached by the dissociation of > N2Qi, reaction (4) in bulb B it was approached by the opposite reaction, reaction (5). Here it is clear why the color of each bulb stopped changing at the particular hue characteristic of the equilibrium state at 25°C. The reaction between N02 and N204 can proceed in both directions ... [Pg.146]


See other pages where The equilibrium state is mentioned: [Pg.208]    [Pg.514]    [Pg.1099]    [Pg.2101]    [Pg.328]    [Pg.597]    [Pg.368]    [Pg.4]    [Pg.534]    [Pg.394]    [Pg.409]    [Pg.273]    [Pg.288]    [Pg.357]    [Pg.506]    [Pg.469]    [Pg.865]    [Pg.435]    [Pg.367]    [Pg.87]    [Pg.435]    [Pg.956]    [Pg.75]    [Pg.472]    [Pg.1285]    [Pg.84]    [Pg.147]   


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