Extraction of Dunham Coefficients from Murrell-Sorbie Parameters

2008 ◽  
Vol 63 (1-2) ◽  
pp. 1-6 ◽  
Author(s):  
Teik-Cheng Lim

A set of relationships between parameters of the Dunham and Murrell-Sorbie potential energy function is developed. By employing Taylor series expansion and comparison of terms arranged in increasing order of bond length, a set of Dunham coefficients is obtained as functions of Murrell- Sorbie parameters. The conversion functions reveal the importance of factorials in extracting Dunham coefficients from Murrell-Sorbie parameters. Plots of both functions, based on parameters of the latter, reveal good correlation near the equilibrium bond length for a group of diatomic molecules. Potential function relations, such as that shown in this paper, are useful when the preferred/reliable data is based on a potential function different from that adopted in available computational software.

1970 ◽  
Vol 25 (12) ◽  
pp. 1932-1936
Author(s):  
Walter Yeranos

Abstract Taking into account the universal correlation of the force constants of halide bonds with their respective dissociation energies (excluding the fluorides), an internuclear potential energy function of the type V(r) = De (1-e-α(r-re))2 + β (1-δF,X) (r - re)2e-γ(r-re) has been proposed for the diatomic halides. α und β, in the latter are constants for a specific series, γ is determined from the rotational-vibrational constant αe, and the function reduces to the ordinary Morse potential function in the case of the fluorides. It, moreover, performs as well as the Hulburt-Hirschfelder 5-parameter function, and, unlike the latter, utilizes the anharmoni-city constant ωeXe as an internal check.


A polyatomic molecule may be considered as a system of heavy nuclei, the relative motions of which are strictly limited by a particular potential energy function. To a higher order of approximation the motion consists of a series of harmonic vibrations, whose amplitudes are small in comparison with the dimensions of the system. Certain of the spectroscopic frequencies (infra-red and Raman) may be identified with the normal frequencies of vibration, which frequencies may be readily be computed, provided the geometric form of the molecule and its potential energy function are known.Unfortunately it is very difficult to derive the potential energy function from purely theoretical considerations although some progress has been made in this direction, notably for H 2 O. It would appear that the converse problem of determining the potential energy from the experimentally known normal frequencies would be comparatively simple. This, however, is not usually the case, since in general the potential function contains more parameters than there are frequencies. Thus the molecule YX 2 has three normal modes of vibration, but its potential function depends on four constants; the molecule YX 3 has four frequencies, which are functions of six constants and so on.


2004 ◽  
Vol 59 (3) ◽  
pp. 116-118 ◽  
Author(s):  
Teik-Cheng Lim

The two-body interactions in the Biswas-Hamann (BH) and Murrell-Mottram (MM) potential functions are analytically related in this paper by equating the zeroth to second differentials at equilibrium bond length. By invoking the Maclaurin series expansion for the exponential term, the MM potential function could be expressed in a manner that enables comparison of repulsive and attractive terms. Approximate and refined sets of scaling factors were obtained upon comparing the indices and coefficients, respectively. Finally, the suitability for each set of scaling functions is discussed in terms of the “softness” of the bonds.


Author(s):  
Lionel Raff ◽  
Ranga Komanduri ◽  
Martin Hagan ◽  
Satish Bukkapatnam

In this chapter, we describe results obtained by five methods that have been employed to fit ab initio potential-energy. These methods are (i) moving or modified Shepard interpolation (MSI), (ii) interpolative moving least squares (IMLS), (iii) invariant polynomials (IP), (iv) reproducing kernel Hilbert space (RKHS), and (v) a hybrid method that combines MSI and IMLS methods. The MSI and IMLS methods are described in some detail in the following. The IP and RKHS procedures are significantly more complex, and the reader is referred to the original papers for a more complete discussion of the details by which these methods are executed. The moving or modified Shepard interpolation (MSI) method was developed primarily by Collins and co-workers. The method employs electronic structure calculations to obtain the molecular potential energy at configuration points generated by an automated procedure. These data are then employed in a Shepard interpolation procedure to obtain the potential energies of the system at points other than those in the database. This procedure involves expressing the local potential about each configuration point in a Taylor series expansion. The term “moving” in the title derives from the fact that the set of internal coordinates employed in the interpolation varies from point-to-point in the database. Like all fitting methods, the MSI procedure requires the potential energy at a set of configuration points in the (3N-6) dimensional internal space of the system under investigation. These energies are generally obtained using ab initio electronic structure methods at some level of accuracy. In addition to the potential energies at each configuration point, the method also requires at least the first and second derivatives of the potential with respect to the coordinates being employed at each configuration point. These derivatives are needed to allow the local potential about a given configuration point in the database to be expressed in terms of a Taylor series expansion about that point. In principle, the MSI method may be extended to include third or fourth derivatives, but in most applications, the expansions are truncated after the quadratic terms.


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