Big Chemical Encyclopedia

Chemical substances, components, reactions, process design ...

Articles Figures Tables About

Simple square well

Plot the Leimard-Jones potentials for each of the gases studied. Obtain ft from Eqs. (16)-(18) by numerioal integration and compare the values from this two-parameter potential with those from the van der Waals and Beattie-Bridgeman equations of state. Optional A simple square-well potential model can also be used to eradely represent the interaction of two molecules. In place of Eq. (18), use the square-well potential and parameters of Ref. 6 to ealeulate /t. Contrast with the results from the Lennard-Jones potential and comment on the sensitivity of the calculations to the form of the potential.]... [Pg.105]

The properties of electrons in a periodic potential are demonstrated with the use of a simple square well potential, the Kronig-Penney model. The potential is zero for 0 < x < a and Vq for —b < x < 0, i.e. it has a period (a + b). The Schrodinger equations for the two regions follow directly and lead on substitution of a Bloch function to ... [Pg.118]

The properties of the above system at modest particle concentrations are relatively simple to model, because the grafted octadecyl layer is thin compared to the particle radius and because the particle-particle interactions are weak enough that the properties of the dispersion are not sensitive to the detailed shape of the particle-particle interaction potential. These considerations have motivated the use of a simple square-well potential as a model of the particle-particle interactions (Woutersen and de Kruif 1991) (see Fig. 7-3). This potential consists of an infinite repulsion at particle-particle contact (where D — 0), bounded by an attractive well of width A and depth e. There are no interactions at particle-particle gaps greater than A. Near the theta point, the well depth s depends on temperature as follows (Hory and Krigbaum 1950) ... [Pg.333]

Sensitivity to the shape of W D) differentiates weakly from strongly interacting particles. For the former, the precise shape of the potential is not important we saw in Section 7.2.4 that even a simple square-well potential is an adequate approximation. But insensitivity to the shape of the potential can only be expected when the particles are only weakly bound by that potential, so that rapid, thermally driven changes in particle-particle separation average out the details of the shape of the potential. For strongly flocculated gels, the particle-particle separations remain trapped near the minimum in the potential well, and the shape of the well near this minimum matters much more. [Pg.350]

There is a simpler way to decide that the symmetric solution has lower energy. As the barrier height becomes lower and lower, the two solutions become more and more separated in energy, but they always remain symmetric or antisymmetric with respect to reflection since the hamiltonian always has reflection symmetry. In the limit when the barrier completely disappears we have a simple square well again (but larger), the lowest solution of which is symmetric. (See Fig. 2-13b.) This lowest symmetric solution must... [Pg.45]

Here distance Edihedrai represent the violation energies based on the distance and dihedral angle restraints, respectively. These functions can take several forms, although a simple square well potential is commonly used. The expressions also include a summation over both upper and lower distance violations for example, Edistance = When considering upper distance re-... [Pg.339]

In order to model experimental systems with short-range attractions, different models have been used. Spherically symmetric interaction potentials, such as the simple square well (SW) [22], or the Asakura Oosawa (AO) depletion potential [23], model the colloid-polymer mixture considering that the polymers are ideal [24]. However, due to the short range of these simple potentials, crystallization and fluid-fluid phase separations occur in the same region where gelation is expected, what makes more difficult the interpretation of the data. Therefore, strategies to avoid this equilibrium phase separation have been devised. [Pg.140]

Turning to molecular attractions, the molecular dynamics results of Alder et al (1972) indicate that, even the simple square-well interaction potential, leads to a much more complex expression for the attractive term, than those used in the van der Waals and Redlich-Kwong EoS. [Pg.636]

Alder and Wainwright gave MD treatments of particles whose pair potential was very simple, typically the square well potential and the hard sphere potential. Rahman (1964) simulated liquid argon in 1964, and the subject has shown exponential growth since then. The 1970s saw a transition from atomic systems... [Pg.65]

Some simple models for V(r) are shown in Fig. 2.1. Two crude approximations, the infinite square well (ISW) and the 3-dimensional harmonic oscillator (3DHO), have the advantage of leading to analytical solutions of the Schrodinger equation which lead to the following energy levels ... [Pg.18]

MC simulations can reflect the nonclassical critical fluctuations if the simulation box is sufficiently large or if special techniques are applied to analyze the fluctuations. Simulations for simple nonionic models such as the square-well fluid (SCF) [52] show that there is indeed a good chance to study details of criticality. As noted, MC simulations have also been profitably exploited... [Pg.50]

The solution to the Schrodinger equation for a particle confined within a simple harmonic potential well is a set of discrete allowed energy levels with equal intervals of energy between them. It is related to the familiar simple solution for a particle in an infinite square well, with the exception that in the case of the simple harmonic potential, the particle has a non-zero potential energy within the well. The restoring force in a simple harmonic potential well is fcsc, and thus the potential energy V(x) is x/2 kx2 at... [Pg.44]

Although Eq. (16.12) is based on an intemiolecular potential function that is in detail unrealistic, it nevertheless often provides an excellent fit of second-virial-coefficieiitdata. An example is provided by argon, for which reliable data for B are available over a wide temperature range, from about 85 to 1000 K. The correlation of these data by Eq. (16.12) as shown in Fig. 16.3 results from the parametervaluese/k = 95.2 K,/ = 1.69,andJ = 3.07 x 10 cm. This empirical success depends at least in part on the availability of three adjustable parameters, and is no more tlian a limited validation of the square-well potential. Use of tins potential does illustrate by a very simple calculation how the second virial coefficient (and hence tire vohnne of a gas) may be related to molecular parameters. [Pg.610]

Here we consider a lattice model of a simple pure confined fluid, that is, a fluid composed of molecules having only translational degrees of freedom. The positions of theses molecules are restricted to M n Uyn sites of a simple cubic lattice of lattice constant f. Each site on the lattice can be occupied by one molecule at most which accounts for the infinitely repulsive hard core of each molecule. In addition to repulsion, pair-wise additive attractive interactions between the molecules exist. They are modeled according to square-well potentials where ff is the depth of the attractive well whose width equals t. [Pg.115]

For pedagogic reasons it seems sensible to eon.sider a fluid confined to a slit-pore with chemically heterogeneous substrates to make contact with the parallel mean-field calculations described in Section 4.3. As in that section we employ a simple cubic lattice of M sites. In accord with our previous notation, represents a configuration of fluid molecules where the (doublevalued, discrete) elements of the A/ -dimensional vector are represented by Eq. (4.51). Molecules of the (pure) lattiee fluid intoraet with each other via a square-well potential where the width of the attractive well is equal to the lattice constant... [Pg.293]

However, for such well-known reactions 45> as positional isomerization and bimolecular substitution in simple square planar coordination compounds, very recently promissing attempts have been reported to derive selection rules on the basis of the orbital symmetry conservation principle 189> and state correlation diagrams 521> e.g. the cis-trans isomerization of square planar complexes has been predicted as a thermally forbidden and photochemically allowed process, in accordance with experiments 28,31,370) [see aiso section FI]. [Pg.196]

The scheme just described (2.14), (2.15) for generating an effective sampling distribution % has some attractive features. For one, an improved n(rN) corresponds merely to improved estimates of /L4 , a quantity that is to be estimated in any case thus no extra computations are required while refining . And the fact that one knows that j3Aa is (very nearly) proportional to N means that there is no need to start from scratch when seeking n for a larger or smaller system size N. The scheme has proved simple and effective in practice, and was used unmodified to study Lennard-Jonesium [10] and the square-well fluid [11] by TDSMC. [Pg.383]

Escobedo and de Pablo have proposed some of the most interesting extensions of the method. They have pointed out [49] that the simulation of polymeric systems is often more troubled by the requirements of pressure equilibration than by chemical potential equilibration—that volume changes are more problematic than particle insertions if configurational-bias or expanded-ensemble methods are applied to the latter. Consequently, they turned the GDI method around and conducted constant-volume phase-coexistence simulations in the temperature-chemical potential plane, with the pressure equality satisfied by construction of an appropriate Cla-peyron equation [i.e., they take the pressure as 0 of Eq. (3.3)]. They demonstrated the method [49] for vapor-liquid coexistence of square-well octamers, and have recently shown that the extension permits coexistence for lattice models to be examined in a very simple manner [71]. [Pg.433]

Aqueous solutions can be modeled by writing a virial equation such as (17.37) in which osmotic pressure replaces pressure. Friedman (1962) describes applications of cluster expansion theory, which include long-range Coulombic potentials as well as short-range square-well potentials that operate when unlike ions approach within the diameter of a water molecule. These models are mathematically quite cumbersome and are not easily used for routine calculations. They do predict the non-ideal behavior of simple electrolytes such as NaCl quite admirably at moderate concentrations however, they use the square-well potential as an adjustable parameter and so retain some of the properties of the D-H equation with an added adjustable term. For this reason these are not truly a priori models. [Pg.447]

In order to get more experience with the newly proposed index ( ) we will consider the leading eigenvalue X of D/D matrices for several well-defined mathematical curves. We should emphasize that this approach is neither restricted to curves (chains) embedded on regular lattices, nor restricted to lattices on a plane. However, the examples that we will consider correspond to mathematical curves embedded on the simple square lattice associated with the Cartesian coordinates system in the plane, or a trigonal lattice. The selected curves show visibly distinct spatial properties. Some of the curves considered apparently are more and more folded as they grow. They illustrate the self-similarity that characterizes fractals. " A small portion of such curve has the appearance of the same curve in an earlier stage of the evolution. For illustration, we selected the Koch curve, the Hubert curve, the Sierpinski curve and a portion of another Sierpinski curve, and the Dragon curve. These are compared to a spiral, a double spiral, and a worm-curve. [Pg.188]

For some simple mathematical forms of the potential energy U(r) it is possible to find analytical solutions to the integral in (11.41). The simplest form of U r), a square well nuclear potential according to Figure 11.12, yields the following expression after integration and some algebra ... [Pg.328]

The temperature dependence of the second virial coefficient can be fitted by two-constant equations, e.g. that of Lennard-Jones, but these have not a simple algebraic form. It can be fitted by several alternative three-constant equations. The form here used is the simplest derivable from a well defined model, namely a square-well potential (see Guggenheim, Australian Rev. Pure and App. Chem. 1953, 3,1). [Pg.168]


See other pages where Simple square well is mentioned: [Pg.429]    [Pg.282]    [Pg.202]    [Pg.332]    [Pg.341]    [Pg.429]    [Pg.282]    [Pg.202]    [Pg.332]    [Pg.341]    [Pg.296]    [Pg.306]    [Pg.112]    [Pg.44]    [Pg.160]    [Pg.163]    [Pg.191]    [Pg.99]    [Pg.5950]    [Pg.76]    [Pg.36]    [Pg.99]    [Pg.258]    [Pg.54]    [Pg.294]    [Pg.320]    [Pg.165]    [Pg.158]    [Pg.321]    [Pg.871]    [Pg.5949]   
See also in sourсe #XX -- [ Pg.140 ]




SEARCH



Square well

© 2024 chempedia.info