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Subsystems, equilibrium

In the subsystem resolution one also considers the constrained (intra-subsystem) equilibrium states [4,5,7,9,12,83], when all subsystems are mutually closed, which is symbolized by the vertical solid lines in the symbolic representation of a collection of AIM in Mc = (a fi y. ..). In order to probe the open subsystem characteristics in Mc, when each AIM is characterized by the intra-subsystem equalized, generally different levels of the AIM chemical potentials,... [Pg.145]

The assumption (frequently unstated) underlying equations (A2.1.19) and equation (A2.1.20) for the measurement of irreversible work and heat is this in the surroundings, which will be called subsystem p, internal equilibrium (unifomi T, p and //f diroughout the subsystem i.e. no temperature, pressure or concentration gradients) is maintained tliroughout the period of time in which the irreversible changes are... [Pg.340]

Two subsystems a. and p, in each of which the potentials T,p, and all the p-s are unifonn, are pennitted to interact and come to equilibrium. At equilibrium all infinitesimal processes are reversible, so for the overall system (a + P), which may be regarded as isolated, the quantities conserved include not only energy, volume and numbers of moles, but also entropy, i.e. there is no entropy creation in a system at equilibrium. One now... [Pg.343]

If there are more than two subsystems in equilibrium in the large isolated system, the transfers of S, V and n. between any pair can be chosen arbitrarily so it follows that at equilibrium all the subsystems must have the same temperature, pressure and chemical potentials. The subsystems can be chosen as very small volume elements, so it is evident that the criterion of internal equilibrium within a system (asserted earlier, but without proof) is unifonnity of temperature, pressure and chemical potentials tlu-oughout. It has now been... [Pg.343]

Given a size N lattice (thought of now as a heat-bath), consider some subsystem of size n. An interesting question is whether the energy distribution of the subsystem, Pn E), is equal to the canonical distribution of a thermodynamic system in equilibrium. That is, we are interested in comparing the actual energy distribution... [Pg.385]

The prediction and understanding of a state of equilibrium constitutes one of the most important applications of thermodynamics. If we wait long enough, a system consisting of subsystems that are not at equilibrium will change until equilibrium is established. Heat will flow until all parts of the system are at the same temperature. Thus = = 7, is a criterion for equilibrium. [Pg.225]

To derive the condition for thermodynamic equilibrium, we start with an isolated system consisting of two subsystems as shown in Figure 5.6. Subsystem A is the one of primary interest in that it is the one in which the chemical process is occurring. Subsystem B is a reservoir in contact with subsystem A in such a way that energy in the form of heat or work can flow between the two subsystems. If left alone, the system will come to equilibrium. Energy will be transferred between the subsystems so that the temperature and pressure will be... [Pg.226]

Figure 5.6 An isolated system composed of subsystem A (the one we will eventually designate as the system) and subsystem B (the surroundings containing a heat reservoir). Heat and work will be exchanged until TA = 7b, pA = p%, and equilibrium is established. Figure 5.6 An isolated system composed of subsystem A (the one we will eventually designate as the system) and subsystem B (the surroundings containing a heat reservoir). Heat and work will be exchanged until TA = 7b, pA = p%, and equilibrium is established.
Equation (5.47) gives the criterion for reversibility or spontaneity within subsystem A of an isolated system. The inequality applies to the spontaneous process, while the equality holds for the reversible process. Only when equilibrium is present can a change in an isolated system be conceived to occur reversibly. Therefore, the criterion for reversibility is a criterion for equilibrium, and equation (5.47) applies to the spontaneous or the equilibrium process, depending upon whether the inequality or equality is used. [Pg.228]

Now the previously isolated subsystem is allowed to exchange x with an external reservoir that applies a thermodynamic force Xr. Following the linear analysis (Section II F), denote the subsystem thermodynamic force by Xs(x) (this was denoted simply X(x) for the earlier isolated system). At equilibrium... [Pg.36]

The generic case is a subsystem with phase function x(T) that can be exchanged with a reservoir that imposes a thermodynamic force Xr. (The circumflex denoting a function of phase space will usually be dropped, since the argument T distinguishes the function from the macrostate label x.) This case includes the standard equilibrium systems as well as nonequilibrium systems in steady flux. The probability of a state T is the exponential of the associated entropy, which is the total entropy. However, as usual it is assumed (it can be shown) [9] that the... [Pg.39]

Equation (9) was obtained using the assumption that the vibrational subsystem is in the state of thermal equilibrium corresponding to the initial electron state. The expression for the effective frequency a>eff has the form5... [Pg.101]

The physical mechanism of entirely nonadiabatic and partially adiabatic transitions is as follows. Due to the fluctuation of the medium polarization, the matching of the zeroth-order energies of the quantum subsystem (electrons and proton) of the initial and final states occurs. In this transitional configuration, q, the subbarrier transition of the proton from the initial potential well to the final one takes place followed by the relaxation of the polarization to the final equilibrium configuration. [Pg.129]

For entirely nonadiabatic transitions, the transition probabilities are so small that the reaction does not disturb the equilibrium distribution in the nuclear subsystems (q9 Q, s), and the calculation of the mean transition probability is reduced to averaging the corresponding local transition probability over the equilibrium distribution of the coordinates q, Q, s ... [Pg.161]

The carrier-phonon interaction decreases with the lowering of temperature, since the emission and absorption of phonons by carriers is proportional to the number of final states available to carriers and phonons. At sufficiently low temperatures, the interaction between the two subsystems can be so weak that there is no thermal equilibrium between them, and the energy is distributed among electrons more rapidly than it is distributed to the lattice, resulting in a different temperature for electron and phonon subsystems, giving rise to the so-called electron-phonon decoupling . [Pg.327]

Tunnel relaxation of orientational states in the phonon field of a substrate is considered in Appendix 2). When a molecule has a single equilibrium orientation (p = 1) the deformation potential is also characterized by a well-defined barrier AU which separates the equivalent minima. That is why, the subsystem Hamiltonian (4.2.12) used in the exchange dephasing model147,148 with... [Pg.97]

The quantities introduced have a number of properties necessary for thermodynamic equilibrium to establish between the subsystem and the reservoir at / - oo. First of all, we note that by virtue of the definition (4.2.30) the summation of the matrix elements Wqq over the first index gives zero. Therefore, summation over q of both sides of Eq. (4.2.31) makes the product Cqv vanish. From... [Pg.100]

The first term in expression (4.2.38) for T has a simple physical meaning it sums the perturbed leaving rates from each level of the subsystem taking into account the equilibrium probabilities for their occupation. On the other hand, the second term depends on the unperturbed rates for transitions between states of the subsystem and is inversely proportional to them by virtue of the definition of... [Pg.101]

The equilization of pressure between the two subsystems in equilibrium agrees with the dictates of mechanics, identifying P as a mechanical pressure. [Pg.415]

The surface BCDE represents a segment of the surface defined by the fundamental equation characteristic of a composite system with coordinate axes corresponding to the extensive parameters of all the subsystems. The plane Uo is a plane of constant internal energy that intersects the fundamental surface to produce a curve with extremum at A, corresponding to maximum entropy. Likewise So is a plane of constant entropy that produces a curve with extremum A that corresponds to minimum energy at equilibrium for the system of constant entropy. This relationship between maximum entropy... [Pg.417]

By way of illustration consider a binary composite system characterized by extensive parameters Xk and Xf in the two subsystems and the closure condition Xk + X k — Xk. The equilibrium values of Xk and X k are determined by the vanishing of quantities defined in the sense of equation (3) as... [Pg.422]

Continuum models remove the difficulties associated with the statistical sampling of phase space, but they do so at the cost of losing molecular-level detail. In most continuum models, dynamical properties associated with the solvent and with solute-solvent interactions are replaced by equilibrium averages. Furthermore, the choice of where the primary subsystem ends and the dielectric continuum begins , i.e., the boundary and the shape of the cavity containing the primary subsystem, is ambiguous (since such a boundary is intrinsically nonphysical). Typically this boundary is placed on some sort of van der Waals envelope of either the solute or the solute plus a few key solvent molecules. [Pg.3]

Here, the relaxed softness matrix Srel groups the equilibrium, fully relaxed responses in the subsystem numbers of electrons, following the displacements in the chemical potentials of their (separate) electron reservoirs, the relaxed geometric softness matrix... [Pg.473]

Equilibrium data for the NH3-H2S-H2O subsystem have been reported by van Krevelen et al. at 20°, 40°, and 60°C(7 ), by Miles and Wilson at 80° and 120°C(46), and by Ginzburg et al. at temperatures from 57° to 87°C (obtained at constant total pressure rather than at constant temperature) (60,61) We correlated data having ionic strengths above 0.2 molal in terms of an equilibrium coefficient K4 ... [Pg.131]

The non-linear theory of steady-steady (quasi-steady-state/pseudo-steady-state) kinetics of complex catalytic reactions is developed. It is illustrated in detail by the example of the single-route reversible catalytic reaction. The theoretical framework is based on the concept of the kinetic polynomial which has been proposed by authors in 1980-1990s and recent results of the algebraic theory, i.e. an approach of hypergeometric functions introduced by Gel fand, Kapranov and Zelevinsky (1994) and more developed recently by Sturnfels (2000) and Passare and Tsikh (2004). The concept of ensemble of equilibrium subsystems introduced in our earlier papers (see in detail Lazman and Yablonskii, 1991) was used as a physico-chemical and mathematical tool, which generalizes the well-known concept of equilibrium step . In each equilibrium subsystem, (n—1) steps are considered to be under equilibrium conditions and one step is limiting n is a number of steps of the complex reaction). It was shown that all solutions of these equilibrium subsystems define coefficients of the kinetic polynomial. [Pg.48]


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See also in sourсe #XX -- [ Pg.13 , Pg.14 ]




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