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Perturbation waves

As discussed in detail in [10], equivalent results are not obtained with these three unitary transformations. A principal difference between the U, V, and B results is the phase of the wave function after being h ansported around a closed loop C, centered on the z axis parallel to but not in the (x, y) plane. The pertm bative wave functions obtained from U(9, <])) or B(0, <()) are, as seen from Eq. (26a) or (26c), single-valued when transported around C that is ( 3 )(r Ro) 3< (r R )) = 1, where Ro = Rn denote the beginning and end of this loop. This is a necessary condition for Berry s geometric phase theorem [22] to hold. On the other hand, the perturbative wave functions obtained from V(0, <])) in Eq. (26b) are not single valued when transported around C. [Pg.463]

The expansion coefficients determine the first-order correction to the perturbed wave function (eq. (4.35)), and they can be calculated for the known unperturbed wave functions and energies. The coefficient in front of 4>o for 4 i cannot be determined from the above formula, but the assumption of intermediate normalization (eq. (4.30)) makes Co = 0. [Pg.125]

On application of the ordinary methods of perturbation theory, it is seen that the first-order perturbed wave function for a normal hydrogen atom with perturbation function f r)T, tesseral harmonic, has the form ] ioo(r)-HKr)r(i>, tesseral harmonic as the perturbation function. The statements in the text can be verified by an extension of this argument. [Pg.740]

The foundation of our approach is the analytic calculations of the perturbed wave-functions for a hydrogenic atom in the presence of a constant and uniform electric field. The resolution into parabolic coordinates is derived from the early quantum calculation of the Stark effect (29). Let us recall that for an atom, in a given Stark eigenstate, we have ... [Pg.272]

We propose to construct the polarization functions from these perturbed wave functions. The genuine basis set u has to be enriched by ... [Pg.272]

Figure 5. Schematic arrangement for hologram formation with an electron biprism. A plane wave illuminates the specimen placed off-axis. After the object lens a wire is placed between two earthed plates. The wire is the electron optical analog of a Fresnel biprism and causes the unperturbed and perturbed waves forming the electron hologram to interfere. The object phase-shift causes a displacement in the hologram fringes, and is thus observable. Figure 5. Schematic arrangement for hologram formation with an electron biprism. A plane wave illuminates the specimen placed off-axis. After the object lens a wire is placed between two earthed plates. The wire is the electron optical analog of a Fresnel biprism and causes the unperturbed and perturbed waves forming the electron hologram to interfere. The object phase-shift causes a displacement in the hologram fringes, and is thus observable.
The first (and still the foremost) quantum theory of stopping, attributed to Bethe [19,20], considers the observables energy and momentum transfers as fundamental in the interaction of fast charged particles with atomic electrons. Taking the simplest case of a heavy, fast, yet nonrelativistic incident projectile, the excitation cross-section is developed in the first Born approximation that is, the incident particle is represented as a plane wave and the scattered particle as a slightly perturbed wave. Representing the Coulombic interaction as a Fourier integral over momentum transfer, Bethe derives the differential Born cross-section for excitation to the nth quantum state of the atom as follows. [Pg.13]

Here both the perturbed wave function (f) > and static ground state wave function 0 > are Slater determinants Qk r) and generalized co-... [Pg.131]

It is natural to equate the dynamical variations of the basic operators 6Xk and 5Yk, obtained with the scaling (7) and Thouless (25) perturbed wave functions. This provides the additional relation between the amplitudes and deformations Qk and pk and finally result in the system of equations for the unknowns pk and p. ... [Pg.134]

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]

The parameter is introduced to keep track of the order of the perturbation series, as will become clear. Indeed, one can perform a Taylor series expansion of the perturbed wave functions and perturbed energies using X to keep track of the order of the expansions. Since the set of eigenfunctions of the unperturbed SE form a complete and orthonormal set, the perturbed wave functions can be expanded in terms of them. Thus,... [Pg.242]

Let the first-order correction to the perturbed wave function be expanded as a linear combination of unperturbed wave functions, that is,... [Pg.243]

The method of treatment of the shallow traps by expanding the perturbed wave functions in a series of the delocalized pure-crystal wave functions r [Eq. (10)] is also convenient for intensity calculations. Since 0 is the only spectrally active function its... [Pg.40]

An instability analysis of a multiphase flow is usually based on the continuum assumption and the equations of motion of the phases. Two different approaches are common. One approach is to study the wave propagation speed from the equations of motion using an analogy to the surface wave situation. The other approach is to study the growth rate of the perturbation wave when a small perturbation wave is introduced to the system. The criterion for stability can then be derived. A perturbation wave can be expressed by... [Pg.270]

The corresponding first-order perturbed wave function reads... [Pg.164]

A weakness of these methods lies in the limited number of zeroth-order states that are used for an expansion of the first-order perturbed wave function. In particular, it has been demonstrated that probabilities of spin-forbidden radiative transitions converge slowly with the length of the perturbation expansion.92... [Pg.166]

In terms of the first-order perturbed wave functions, the matrix element for an electric dipole transition moment is given by... [Pg.181]

Conversely, a purely capacitive response is completely out of phase with the perturbation wave. The capacitive impedance response varies continuously and inversely with frequency and has no real component. In the complex plane, an ideal capacitance (C) appears as a vertical line that does not intercept the real axis. [Pg.220]

In order to evaluate 5s/ISv from Eq. (282), we further need the functional derivatives dqfjjdvs and ScpflSv. The stationary OPM eigenfunctions (< /r), = 1,..., oo) form a complete orthonormal t, and so do the time-evolved states unperturbed states, remembering that at t = ti the orbitals are held fixed with respect to variations in the total potential. We therefore start from t = ti, subject the system to an additional small perturbation (5i)s(r, t) and let it evolve backward in time. The corresponding perturbed wave functions [Pg.135]

The mininnim time needed to make a measurement at any frequency is the inverse of the frequency i.e., the period) of the perturbing wave. [Pg.535]

Hussain, A. K. M. F., and Reynolds, W. C., The Mechanics of Perturbation Wave in Turbulent Shear Flow, Rep. FM-6. Mech. Eng. Dept., Stanford University, Stanford, California. See, also, J. Fluid Mech. 41, 241 (1970). [Pg.245]

The expansion coefficients determine the first-order correction to the perturbed wave... [Pg.70]

In two previous papers [8,9] we have calculated the static polarizabilities and hyperpolarizabilities for ls3p Pj (J = 0, 2)-states of helium. The method was based on degenerate perturbation-theory expressions for these quantities. The necessary dipole matrix elements were found by using the high-precision wave function on framework of the configuration-interaction (Cl) method [10]. The perturbed wave functions are also expanded in a basis of accurate variational eigenstates [11]. These basis sets of the wave functions explicitly take account of electron correlation. To control the result we have also carried out similar calculations with Fues model potential method. [Pg.754]


See other pages where Perturbation waves is mentioned: [Pg.124]    [Pg.740]    [Pg.740]    [Pg.134]    [Pg.434]    [Pg.134]    [Pg.141]    [Pg.23]    [Pg.144]    [Pg.270]    [Pg.302]    [Pg.99]    [Pg.148]    [Pg.385]    [Pg.163]    [Pg.179]    [Pg.98]    [Pg.250]    [Pg.58]    [Pg.135]    [Pg.70]   
See also in sourсe #XX -- [ Pg.45 , Pg.112 , Pg.130 , Pg.164 ]




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