Wavefunction diabatic

The state mixing term, the first in the r.h.s., usually dominates, at least in the presence of avoided crossings. Its determination reduces to a simple problem of interpolation of the Hu matrix elements, according to eq.(16). The second term corresponds, for large R, to the electron translation factor (see for instance [38]). This term depends on the choice of the reference frame that is, for baricentric frames, it depends on the isotopic masses. It contains the Gn matrix, which may be determined by numerical differentiation of the quasi-diabatic wavefunctions [16] this calculation is more demanding, especially in the case of many internal coordinates. It is therefore interesting to adopt the approximation ... 

Figure 4. Calculated HAB values as a function of Fe -Fe separation, based on the structural model given in Figure 1 and the diabatic wavefunctions I/a and f/B. Curves 1 and 2 are based on separate models in which the inner-shell ligands are represented, respectively, by a point charge crystal field model [Fe(H20)62 -Fe(HsO)63 ] and by explicit quantum mechanical inclusion of their valence electrons [Fe(HgO)s2 -Fe(H20)s3+] (as defined by the dashed rectangle in Figure 1). The corresponding values of Kei, the electronic transmission factor, are displayed for various Fe-Fe separations of interest.

Fig. 3. Interacting fragment configurations (IFC) for reactant and product diabatic wavefunctions for a 2 + 2 addition, la—Id are no-bond reactant-like configurations while II is a triplet-triplet Heitler-London configuration.

To summarize, in the preceding discussion we have presented two formalisms for the computation of diabatic wavefunctions using an effective Hamiltonian. In the Van VIeck method the diabatic wavefunctions are orthogonal In the non-orthogonal transformation method the diabatic wavefunctions are non-orthogonal. In practice, perturbation theory is normally used to solve the equation system (20) the review of Spiegelmann and... 

So far, we have mentioned methods that produce all-electron diabatic wavefunctions and corresponding Hamiltonian matrix elements. There are two other classes of methods which simplify the quantum problem by focusing on the wavefunction of the transferred charge such as methods making use of the frozen core approximation Fragment Orbital methods (FO), and methods that assume the charge to be localized on single atomic orbitals [50]. In this work, we will also treat these computationally low-cost methods. 

More generally, the integral may also equal a multiple of tt in view of the trigonometric functions in Eq. (9), and the diabatic wavefunctions (10) still be well defined. A value of tt is expected when encircling a conical intersection between potential energy surfaces in order to compensate for the singularity of the adiabatic wavefunctions (see also Chapters 1 and 7 in this book). In the ideal case, Eq. (22) is generalized as ... 

Several methods to determine quasi-diabatic states are based on the assumption that single determinants or configurations are quasi-diabatic wavefunctions in other words, their physical content should not change too much with the nuclear geometry and the matrix elements of d/dQa in this basis should be small. When this is true, the main source of variation of the adiabatic wavefunctions, and the dominant contribution to is the change of the Cl coefficients as functions of the nuclear coordinates keeping the Cl coefficients as constant as... 

The other method, due to Persico and Cimiraglia et al., is based on a rotation of the adiabatic basis to obtain the quasi-diabatic one, as in equation (14). The rotation matrix U is determined so that the multi-configurational quasi-diabatic wavefunctions have the maximum overlap with the reference states ... 

In the diabatic picture, the transition is caused by a coupling term 12(2, r), and hence the time-dependent Schrodinger equation (TDSE) which has to be solved involves two diabatic wavefunctions... 

The ultimate approach to simulate non-adiabatic effects is tln-ough the use of a fiill Scln-ddinger wavefunction for both the nuclei and the electrons, using the adiabatic-diabatic transfomiation methods discussed above. The whole machinery of approaches to solving the Scln-ddinger wavefiinction for adiabatic problems can be used, except that the size of the wavefiinction is now essentially doubled (for problems involving two-electronic states, to account for both states). The first application of these methods for molecular dynamical problems was for the charge-transfer system... 

This reactivity pattern can be rationalized in terms of a diabatic model which is based upon the principle of spin re-coupling in valence (VB) bond theory [86]. In this analysis the total wavefunction is represented as a combination of two electronic configurations arising from the reactant (reaction coordinate. At the outset of the reaction, is lower in energy than [Pg.141]

The treatment developed here is based on the density matrix of quantum mechanics and extends previous work using wavefunctions.(42 5) The density matrix approach treats all energetically accessible electronic states in the same fashion, and naturally leads to average effective potentials which have been shown to give accurate results for electronically diabatic collisions. 19) The approach is taken here for systems where the dynamics can be described by a Hamiltonian operator, as it is possible for isolated molecules or in models where environmental effects can be represented by terms in an effective Hamiltonian. 

The aim of this work is to obtain the four lowest E curves and wavefunctions of BH at the same level of accuracy and to bring out the interplay of ionic, Rydberg and valence states at energies and internuclear distances which were not previously investigated. We have therefore made use of a method, already put forward by us [16,17] to determine at once quasi-diabatic and adiabatic states, potential energy cnrves and approximate nonadiabatic couplings. We have analogously determined the first three E+ states, of which only the lowest had been theoretically studied... 

Charge Localized vs. Delocalized Wavefunctions. In the spirit of the Condon approximation discussed above, we do not include the full dependence of the purely electronic matrix elements on q n, but rather evaluate them where the diabatic curves... 

This is referred as BO ansatz. This ansatz is taken as a variational trial function. Terms beyond the leading order in m/M are neglected m is the electronic and M is nuclear mass, respectively). The problem with expansion (4) is that functions /(r, R) contain except bound states also continuum function since it includes the centre of mass (COM) motion. Variation principle does not apply to continuum states. To avoid this problem we can separate COM motion. The remaining Hamiltonian for the relative motion of nuclei and electrons has then bound state solution. But there is a problem, because this separation mixes electronic with nuclear coordinates and also there is a question how to define molecule-fixed coordinate system. This is in detail discussed by Sutcliffe [5]. In the recent paper by Kutzelnigg [8] this problem is also discussed and it is shown how to derive adiabatic corrections using, as he called it, the Bom-Handy ansatz. There are few important steps to arrive at formula for a diabatic corrections. Firstly, one separates off COM motion. Secondly, (very important step) one does not specify the relative coordinates (which are to some extent arbitrary). In this way one arrives at relative Hamiltonian Hrd [8] with trial wavefunction If we make BO ansatz... 

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