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Maxwells constraint

We assume the gas density = pb to be fixed the density of coexisting liquid and the coexistence temperature are unknown. Therefore, we must solve Eqs. (4.43) and (D.ll) simultaneously for Tob and p, . We solve the equations by the following procedure  [Pg.419]

The procedure is halted when [/ (7 ) [ 10 . At the end it is sensible to check whether p (T ) = pb, as specified at the outset, and that / (T ,p ) = P(T , Pb) for the coexisting phases, so that Tob (pb) = Tn- Convergence is achieved after five or six iterations. The resulting bulk coexistence curve is plotted in Fig. 4.5. To illustrate the effect of confinement, we eilso plot in that same figure the pore coexistence curve for s = 50 determined by the procedure detailed above using, however, the corresponding equation of state for the pore fluid given in Eq. (4.28). [Pg.419]


We argued earlier that some of the Maxwell constraints can be removed by the action of symmetry, and this allows for the possibility of a structure having some RUM flexibility. This, however, is not the whole story. A network glass, such as silica, has no internal symmetry, and might therefore be thought incapable of supporting RUMs. Recent calculations of the RUM density of states of silica glass have shown that this is not the case. [Pg.29]

These constraints must be satisfied in the solution of the Stefan-Maxwell equations. At a point within a chemically reacting flow simulation, the usual situation is that the diffusion velocities must be evaluated in terms of the diffusion coefficients and the local concentration, temperature, and pressure fields. One straightforward approach is to solve only K — 1 of Eqs. 3.105, with the X4h equation being replaced with a statement of the constraint. For... [Pg.91]

Property 1. In a theory based on the pair of fields (, 0) with action integral equal to (118), submitted to the duality constraint (119), both tensors Fap and Fap obey the Maxwell equations in empty space. As the duality constraint is naturally conserved in time, the same result is obtained if it is imposed just at t = 0. [Pg.231]

Let us now identify the Cauchy data. As the Maxwell equations are of second order in the scalars, the initial data should be the two functions (time derivatives 0o[Pg.232]

It can be shown [8] that Hadamard instabilities are possible for admissible motions if a is in the interval (—1,1), e.g., in extensional flows. On the other hand, restrictions on the eigenvalues of r prevent Hadamard instabilities for a = 1. This is immediately seen from the integral forms qf (4)-(5) for the upper- and lower-convected Maxwell models, which imply constraints on the eigenvalues of the Cauchy-Green tensors. (See, for instance, [12].)... [Pg.202]

Summons R. E., Thomas J., Maxwell J. R., and Boreham C. J. (1992) Secular and environmental constraints on the occurrence of dinosterane in sediments. Geochim. Cosmochim. Acta 56, 2437-2444. [Pg.3981]

This leads us to conclude that A 0, in addition to the constraint (Eq. 2.3.21) for the positive definiteness of the Maxwell-Stefan diffusion coefficients at infinite dilution )°y. [Pg.269]

The n-1 equations given by eq. (8.2-34) and the physical constraint of the form (8.2-43) will form the necessary n equations for solving for the fluxes N. What we shall show in this section that the Stefan-Maxwell equations can be inverted to obtain the useful flux expression written in terms of concentration gradients, instead of concentration gradient in terms of fluxes. [Pg.426]

ConsidCT a solution of two species (1 and 2) that respond to the magnetic field and a solvent that does not The Stefan-Maxwell equation (Equation 8.63), with the constraint that there is no convection, leads to... [Pg.489]

The last case study deserves a special comment as it deals with the attenuation provoked by spatial constraints and not by a conduction process as was the case for all previous case studies in this chapter (and as usually done for this case). The Maxwell equations need to be modified to take into account this peculiarity, thus allowing demonstration of the Lambert-Beer-Bouguer law of light absorption in materials that can be electrically nonconducting and noncharged (which is the most frequently encountered situation). [Pg.518]

Maxwell-Faraday equation for taking into account the reduced capacitance creating the spatial constraint. [Pg.559]

An example of a completely classical approach can be found in Feynman et al. (2006) and Jackson (1998). Their approach can be summarized as follows. It relies on the electric polarization of the medium, which absorbs part of the energy owing to the separation of charges induced by the electric field acting on the charged material. To take into account this effect, called dielectric loss, the free space (vacuum) permittivity Eq is replaced by a material permittivity e equal to the free space permittivity multiplied by the relative permittivity e,. The Maxwell equations are written with this material permittivity e but without spatial constraint or conduction current. In doing so, the wave pulsation co and the wave-vector k are unchanged, equal to the natural variables of the oscillator cOq. and kq. The wave velocity u is therefore equal to the natural velocity Uq which directly depends on the material permittivity e, thus (continued)... [Pg.559]

Formal Graph approach. The Formal Graph approach has been used voluntarily in a limited but essential aspect, which is the justification of the incorporation of a spatial constraint into the Maxwell-Faraday equation. The reason... [Pg.560]

To find the Maxwell relation for any quantity, first identify what independent variables are implied. In this case the independent variables are (T, p,N) because these are the quantities that are either given as constraints in the subscript, or are in the denominator of the partial derivative. Second, find the natural function of these variables (see Table 8.1, page 141). For (T,p,N), the natural function is G(T, p,N). Third, express the total differential of the natural function ... [Pg.156]

Note that this Four-Parameter Fluid model is composed of a Kelvin element (subscripts 1) and a Maxwell element (subscripts 0). Thus, the constitutive laws (differential equations) for the Kelvin and Maxwell elements need to be used in conjunction with the kinematic and equilibrium constraints of the system to provide the governing differential equation. Again, treating the time derivatives as differential operators will allow the simplest derivation of Eq. 5.12. The derivation is left as an exercise for the reader as well as the determination of the relations between the pi and q, coefficients and the spring moduli and damper viscosities (see problem 5.1). [Pg.164]

Since the Maxwell elements are connected in parallel, if strain e(t) is given, one can either solve the pair of linear first order E s. (5.15) or the single second order equation (5.16b) to find the solution for a(t). As an example, consider the case of stress relaxation in which a constant strain history is applied, e(t) = oH(t). Due to the kinematic constraint, each Maxwell element sees the same global strain history and the solution for ai(t) and 02(1) from Eqs. 5.15 are as given earlier in Eq. 3.17. [Pg.169]

A differential equation for either of the series of Kelvin elements can be found using the same procedure described in developing the differential equation for a series of Maxwell elements. The equilibrium constraint, kinematic constraint and constitutive equations are given by... [Pg.173]

Fig. 11.1 An atomic structure of SnSc2 obtained from First-Principles Molecular Dynamics [10]. The resulting structure can be viewed in terms of atomic positions but can be also be viewed as a bar (bonds) and node (atoms) network that can be analyzed using Maxwell-Lagrange constraints... Fig. 11.1 An atomic structure of SnSc2 obtained from First-Principles Molecular Dynamics [10]. The resulting structure can be viewed in terms of atomic positions but can be also be viewed as a bar (bonds) and node (atoms) network that can be analyzed using Maxwell-Lagrange constraints...

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