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Local Helmholtz Energy

Furthermore, the concept of susceptibility can be extended to inhomogeneous systems where the thermodynamic properties are functions of the coordinate vector Let (p, x) be a generalized density, and let h,( ) be the field con- [Pg.176]

For an isotropic fluid, the susceptibility must be invariant under rotations and translations. These conditions imply that the susceptibility should only be a function of the distance x x. As the distance x-x between two fluctuations increases, the random thermal motion increasingly degrades the correlations. This implies lim x x l ( Pi x) 9 /(x )) = 0. For a distance much larger than the distance between the neighboring molecules, the spatial correlation function is given by the Ornstein-Zernike exponential decay  [Pg.177]

The simplest way to connect the mesoscopic susceptibility with other thermodynamic properties and introduce smooth heterogeneities into mesoscopic thermodynamics is to consider a local (coordinate-dependent) thermodynamic [Pg.177]

In particular, near the vapour-liquid critical point the reduced function /= flpJc-sTa is represented by a Landau expansion.  [Pg.178]


As a result of the long-range critical fluctuations, the local density will actually be a function of the position r. In the classical theory of fluctuations such a spatial dependence is accounted for by the presence of a gradient term (Vp) in the local Helmholtz-energy density which has an expansion of the form [11]... [Pg.95]

In this chapter, we have discussed only a few examples of mesoscale phenomena in fluids, for which the methods of meso-thermodynamics appeared to be applicable. However, since coarse-grained models of meso-thermodynamics, such as the Landau-Ginzburg local Helmholtz energy, demonstrate a high degree of universality, associated with the meso-scale structure, an extension of this approach to a broader variety of phenomena is very promising. [Pg.210]

The potential I speak of is usually called the potential of average force. Insofar as it is to be identified to a thermodynamic potential it is a local Helmholtz free energy as a function of the coordinate positions of all the atoms (or radicals) that must change relative positions in the reaction it may be defined by... [Pg.102]

To follow to actually carry out a TSA simulation a three-dimensional grid, with grid interval of about 0.2 A (5 -106 equispaced points in (132)) is built and the Helmholtz energies at all grid points are computed. Before this can be done in practice, a value for (A2) must be found. Then, local minima and the crest surfaces must be found, using the procedures given in (130,132,165). To study the dynamics of the penetrant molecules on the network of sites a Monte-Carlo procedure is employed, which is presented is some detail in (97). [Pg.149]

Van der Waals consciously omitted contributions of the profile shape to the inter-facial excess entropy. In other words, at each position in the transition layer the local entropy is only determined by the local density, p z) On the other hand, the total Helmholtz energy is considered to depend both on P lz) and on the profile p (z) over the entire transition range, see later in this subsection. All of this is in line with the assumptions made in mean field theories for low-molecular mass molecules. ... [Pg.145]

Over a long period of time experimental results on amphiphilic monolayers were limited to surface pressure-area ( r-A) isotherms only. As described in sections 3.3 and 4, from tc[A) Isotherms, measured under various conditions, it is possible to obtain 2D-compressibilities, dilation moduli, thermal expansivities, and several thermodynamic characteristics, like the Gibbs and Helmholtz energy, the energy cmd entropy per unit area. In addition, from breaks in the r(A) curves phase transitions can in principle be localized. All this information has a phenomenological nature. For Instance, notions as common as liquid-expanded or liquid-condensed cannot be given a molecular Interpretation. To penetrate further into understanding monolayers at the molecular level a variety of additional experimental techniques is now available. We will discuss these in this section. [Pg.336]

Here p(z) is the local density of the adsorbed fluid at a distance z from one of the walls of the pore, f(z) is the intrinsic molecular Helmholtz energy of the adsorbate phase, p is the chemical potential. The free energy f(z) comprises tire ideal, mean-field attractive terms, and the excess fine energy (repulsive) term as a function of so-called smoothed weighted average density. [Pg.150]

The advantage of this approach over kinematically extended continua is twofold first, the additional parameter is abstract and does not require special assumptions of the local kinematics as it is necessary in micropolar continua, for example. As a consequence, the corresponding boundary conditions can be formulated more flexibly. Second, the coupling between the macroscopic balance of momentum and the additional balance of equilibrated forces is obtained consti-tutively, via the free Helmholtz energy function and not via the free energy function in combination with measures of deformation assumed a priori. Therefore, such an approach allows for size effects in both ways - either smaller is stiffer" or smaller is weaker depending on the boundary conditions. [Pg.321]

For simplicity, we assume that the sites L and H are localized and that the adsorption of s on a site does not change the internal degrees of freedom of the site. Calculate the Helmholtz energy of solvation, the entropy and enthalpy of solvation of s in this system. Compare the results with Exercise E.3.10. [Pg.375]

The local Helmholtz free energy density corresponding to Equation 1.41 in such a film is... [Pg.91]

Fig. I. The distribution functions for the frequencies y, of the normal mode vibrations of a solute molecule in local maxima of p(r) (i.e., local minima of the Helmholtz energy of residence of the solute molecule). Data were collected from S x 10 sites for He and from 1x10 sites for Ar fircmi two micro-structures of PC. The vertical line indicates the threshold 3-kT/h, significantly bdow whidi all the frequencies must lie if the quasi-dassical approximation is ai rc riate... Fig. I. The distribution functions for the frequencies y, of the normal mode vibrations of a solute molecule in local maxima of p(r) (i.e., local minima of the Helmholtz energy of residence of the solute molecule). Data were collected from S x 10 sites for He and from 1x10 sites for Ar fircmi two micro-structures of PC. The vertical line indicates the threshold 3-kT/h, significantly bdow whidi all the frequencies must lie if the quasi-dassical approximation is ai rc riate...
Allowing for variable density, the expression for the local Helmholtz free energy per molecule f[p x)] derived under the above assumptions reads... [Pg.2]

Equation 2.101 can be used now with the understanding that P (z) is the pressure given by the EoS model for given temperature and number densities (local density and composition). Alternatively, Equation 2.102 can be used, but, now, the EoS model will be used to provide with the local Helmholtz free-energy density To(z) for given temperature, local density, and composition. [Pg.175]

Figure 2.35 compares local defect-type and collective proton transitions. Transitions are completed within 140 and 45 ps for local and collective pathways, respectively. Reconstructed Helmholtz energy profiles, as a function of the CV, are shown together with snapshots of configurations during transitions. Activation and reaction Helmholtz energies of the defect-type transition are AFa = 0.6 eV and AFr = 0.5 eV. The final state of this transition is metastable. For the collective transition, activation, and reaction Helmholtz energies are AFa = 0.3 eV and AFr = 0 eV. [Pg.139]

In contrast to previous treatments [12,13], Eq. (13) emphasizes the effect of the degree of coverage on the overall resistance by a separate factor 1 - 9.) For a rigid object (such as, c.g., a colloidal particle), U z) can simply be taken to be the (Helmholtz) energy of interaction at separation z. However, a polymer is flexible and can adjust its shape to the local field. We should, therefore, average over all allowed conformations of a polymer molecule that has an arbitrary segment at the distance of closest approach z. In other words, one has to evaluate the partition function Q(z) of a chain at a distance z fi-om the surface, in the imposed field of the surface ... [Pg.162]

The Group Contribution Equation of State (GC-EoS) has two eonlributions to the residual Helmholtz energy of the system a repulsive hard sphere Camahan-Starling type term and an attractive term, which combines the group contribution approach wifli the local-composition mixing rules. A complete explanation of the model is given by Skjold-Jorgensen. ... [Pg.779]


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