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Rayleigh-Schrodinger equations

In the second order, however, the EOM-CC and CCLR formulations differ due to the appearance of quadratic terms in Eq. (18). Starting from the CCLR second-order Rayleigh-Schrodinger equation projected onto the zeroth-order left-hand wave function, we obtain... [Pg.229]

The Rayleigh-Schrodinger Perturbation Theory (see [2]) leads then to the following system of linear equations for the determination of cj (j=l,. ..M) ... [Pg.41]

The mathematical procedure that we present here for solving equation (9.15) is known as Rayleigh-Schrodinger perturbation theory. There are other procedures, but they are seldom used. In the Rayleigh-Schrodinger method, the eigenfunctions tpn and the eigenvalues E are expanded as power series in A... [Pg.240]

Angyan, J. G. Rayleigh-Schrodinger perturbation theory of non-linear Schrodinger equations with linear perturbation, IntJ.Quantum Chem., 47 (1993), 469-483... [Pg.352]

At the same time, Meissner, Kucharski and others [56,57] developed the quadratic MR CCSD method in a spin-orbital form which does not exploit the BCH formula. The unknown cluster amplitudes are calculated from the so-called generalized Bloch equation [45-47,49,64,65] (or in our language the Bloch equation in the Rayleigh-Schrodinger form)... [Pg.84]

It should be apparent that the expressions for the wave functions after interaction [equations (3.38) and (3.39)] are equivalent to the Rayleigh-Schrodinger perturbation theory (RSPT) result for the perturbed wave function correct to first order [equation (A.109)]. Similarly, the parallel between the MO energies [equations (3.33) and (3.34)] and the RSPT energy correct to second order [equation (A. 110)] is obvious. The missing first-order correction emphasizes the correspondence of the first-order corrected wave function and the second-order corrected energy. Note that equations (3.33), (3.34), (3.38), and (3.39) are valid under the same conditions required for the application of perturbation theory, namely that the perturbation be weak compared to energy differences. [Pg.45]

If the solutions (energies and wave functions P ) of the Schrodinger equation for the unperturbed system Tf(°) P = F,1,01 4/jl°l are known, and the operator form of the perturbation, Hp, can be specified, the Rayleigh-Schrodinger perturbation theory will provide a description of the perturbed system in terms of the unperturbed system. Thus, for the perturbed system, the SE is... [Pg.241]

In the above formula, Q is the nuclear coordinate, p, and I/r are the ground state and excited electronic terms. Here Kv is provided through the traditional Rayleigh-Schrodinger perturbation formula and K0 have an electrostatic meaning. This expression will be called traditional approach, which has, in principle, quantum correctness, but requires some amendments when different particular approaches of electronic structure calculation are employed (see the Bersuker s work in this volume). In the traditional formalism the vibronic constants P0 dH/dQ Pr) can be tackled with the electric field integrals at nuclei, while the K0 is ultimately related with electric field gradients. Computationally, these are easy to evaluate but the literally use of equations (1) and (2) definitions does not recover the total curvature computed by the ab initio method at hand. [Pg.371]

Hence E(p1 and denote the polarization energy and wave function of /th-order in VAB, y Ih-ordcr in VBC, and th-order in VCA. The energy and wave function perturbation corrections are solutions of triple Rayleigh-Schrodinger (RS) perturbation equations88,309 see Ref. (302) for the explicit form of these equations. [Pg.75]

In 1997, Pakiari and Mohammadi used the FSGO basis set for a perturbation variation Rayleigh Ritz (PV = RR) calculation. We used a matrix representation Schrodinger equation for the configuration interaction calculation. [Pg.303]

Up to this point we are still dealing with undetermined quantities, energy and wave function corrections at each order. The first-order equation is one equation with two ImEnowns. Since the solutions to the unperturbed Schrodinger equation generates a complete set of functions, the unknown first-order correction to the wave function can be expanded in these functions. This is known as Rayleigh-Schrodinger perturbation theory, and the equation in (4.32) becomes... [Pg.125]

In quantum calculations, the Rayleigh-Ritz variational method is widely used to approximate the solution of the Schrodinger equation [86], To obtain exact results, one should expand the exact wave function in a complete basis set... [Pg.23]

When VQ — VT —, i.e., when no symmetry is enforced, the Taylor expansion of Eqs. (5) and (6) defines the Rayleigh-Schrodinger perturbation equations,... [Pg.174]

We start the presentation of our results with the Rayleigh-Schrodinger perturbation theory. The results presented in Table 1 show that for small interatomic distances the RS perturbation expansion converges to the energy of the mathematical ground state of the dimer. This state is a Pauli forbidden solution of the Schrodinger equation, completely symmetric un-... [Pg.179]

HMO theory gives particularly simple and intuitively appealing results upon application of Rayleigh Schrodinger perturbation theory and we shall take advantage of this to interpret trends and make predictions (see, in particular, Section 4.6).d The equations for first- and second-order perturbation given below are derived in the Appendix (Section 4.11). [Pg.144]

In order to obtain the Rayleigh Ratio it is necessary to introduce the concept of an effective wave-equation for each electron (specifically, for each jr-electron since, for the moment, these are all we are discussing). If there really were only one electron which we had to deal with there would be no problem since the Schrodinger Equation for a single electron is well known and can immediately be written down. There is a very convenient shorthand-symbolism for this and, for one electron—which of course is not a very realistic situation in organic chemistry—the wave equation can be written in the form... [Pg.112]

The Hilbert space multireference CC (see e.g. Refs. [36-40]), based on the Jeziorski-Monkhorst ansatz for the wave operator [36]. This ansatz can be either combined with the standard (Rayleigh-Schrodinger) Bloch equation, or with the Brillouin-Wigner Bloch equation (cf. Section 18.4), or with a linear combination of both... [Pg.469]

The state-specific Rayleigh-Schrodinger permrbation theory based on the unperturbed eigenvalue equation... [Pg.510]

The Rayleigh-Schrodinger perturbation series is obtaining by applying Go (is) from the left to equation (15) after re-writing it in the form... [Pg.373]


See other pages where Rayleigh-Schrodinger equations is mentioned: [Pg.8]    [Pg.77]    [Pg.168]    [Pg.216]    [Pg.204]    [Pg.115]    [Pg.259]    [Pg.14]    [Pg.16]    [Pg.27]    [Pg.112]    [Pg.309]    [Pg.6]    [Pg.668]    [Pg.84]    [Pg.98]    [Pg.150]    [Pg.65]    [Pg.92]    [Pg.107]    [Pg.467]    [Pg.341]    [Pg.475]    [Pg.1052]   


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First-order Rayleigh-Schrodinger equation

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Rayleigh-Schrodinger equations calculations

Second-order Rayleigh-Schrodinger equation

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