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Ellinger Y., Defranceschi M. (eds.) Strategies and applications in quantum chemistry (Kluwer, 200

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206

G. P. ARRIGHINI AND C. GUIDOTTI

matrix element of the QMP

in determining the electronic

density. Considering that the QMP knowledge allows one, in principle, to solve the problem of the time-evolution of any arbitrary initial quantum state, the obtainment of

is to be regarded in general as a true piece of skill. It is a fact that we have at

disposal only very few exact QMP expressions in analytical closed form [29], despite tremendous advances in quantum dynamics, particularly during the past fifteen years [31]. Much progress in the QMP evaluation has been realized following mainly the idea that the propagator for an arbitrary time t can be rigorously expressed in terms of shorttime propagators, for which simple approximations are available [31]. The latter procedure has actually been developed in some of the papers quoted [10-15,25], which

should therefore be regarded as more rigorous contributions to the problem of representing the electronic density according to eq. (2.5), even though it is right to say that the implementation of the formalism to explicit calculations has not kept the pace with theory.

Our more rudimentary approach is basically founded on an ansatz choice for the quantity

of higher quality with respect to the short-time approximation which neglects all quantum effects arising from the

noncommutativity of the operators

and . In order to appreciate the nature of the

approximation, let us consider the case where the energy potential

with

constant quantities. Although the QMP for a particle subjected to a constant

force is one of the few cases explicitly known [32], for our convenience we adopt the following exact alternative representation of the propagator for a particle moving in a linear potential [see Appendix A, eq. (A.8)]

The ansatz for the diagonal matrix element of the QMP appearing in eq. (2.5) corresponds to assume the validity of eq. (2.6) also for potentials other than the

linear one. Taking, moreover, into account that a homogeneous and static electric field

is associated with a potential energy the propagator ansatz for the system subjected simultaneously to the action of an electric field generalizes in a straightforward way from eq. (2.6) to yield

Eq. (2.7) is the starting point of the procedure we are going to develop. The neglect of the

exponentials involving and leads to the same result obtainable according to the Trotter formula [30]; as easily verified, such short-time approximation is the basis for recovering from eq. (2.5) the same result predicted by the Thomas-Fermi theory.

Thanks to eq. (2.7), the electronic density expression given by eq. (2.5) can be cast into the (obviously approximate) form

ELECTRONIC CHARGE DENSITY OF QUANTUM SYSTEMS

207

with

A series of manipulations [see Appendix B, eq. (B.4)] allows the function

to be

expressed as follows

where we have set

and Ai[x] denotes the Airy function of argument x [33].

The replacement of the result for

eq. (2.10), into eq. (2.8) yields for the

electronic density

where

The expression for

can be elaborated rather simply,[see Appendix C, eq. (C.4)]

Indefinite integrals involving products of Airy functions and/or their derivatives can be evaluated without many difficulties [34]. Thus,

208

G. P. ARRIGHINI AND C. GUIDOTTI

and successively

After carrying out the integrations involved in eq. (2.15) [34], we finally obtain the result

which allows one to calculate the numerical electronic density in terms of both the

potential characterizing the one-electron model assumed and the electric field polarizing the electron distribution itself. It should be evident from the derivation that the

effect of the field has not been taken into account according to a perturbative treatment; eq. (2.16) is an approximate result for the electron density that includes at infinite order the polarization distortion caused by the external field.

Eq. (2.16) is not an entirely new result. After this work had been concluded and we were looking around in search of bibliographical material, we came upon a paper by Englert and Schwinger [24] dealing with the introduction of quantum corrections to the ThomasFermi statistical atom. These authors attain the same result expressed by eq. (2.16) (for

the case

by resorting to a somewhat more general assumption about the adopted

QMP

as compared to our choice.

 

For a quantum system with a single degree of freedom (dimensionality

a procedure

parallel to that sketched above leads to the following result

 

where

The Fermi level energy

appearing in eq. (2.16) [or eq. (2.17)] through the argument b

of the Airy function and its derivative is fixed by the normalization requirement

[or the analogous one-dimensional stemming from eq. (2.17)]. Obviously

depends on

the external field

amplitude.

 

Unperturbed electron densities descend naturally from the above formalism by letting

vanish.

ELECTRONIC CHARGE DENSITY OF QUANTUM SYSTEMS

209

3. An elementary application of the formalism

As a very simple application of the approach presented in sect. 2, we confine our attention to a model system consisting of independent charged particles

("electrons"), moving in a one-dimensional harmonic effective potential

while simultaneously acted by a static, homogeneous electric field E. An exact treatment of this standard problem is sketchily reviewed in Appendix D for reasons of completeness.

The approximate numeral density n(x;E) is that obtained from eqs. (2.17), (2.18) with

Typical properties of the charge distribution are summarized by its various electric multipole moments. The electric dipole moment induced in the system by the external field is obviously

For further progress, it is convenient to change integration variable from x to F, eq. (3.1), so that

with

After noting that

we are simply left with

Use of the normalization condition finally leads to

a result coincident with the exact prediction [see Appendix D, eq. (D.6)].

The static electric dipole polarizability of the model system investigated is therefore

while higher-order polarizabilities (hyperpolarizabilities) vanish rigorously.

In view of the result just found, it is interesting to contrast exact and approximate behaviour of the density n(x;E) [eqs. (D.5) and (2.17), respectively]. Some insight into the nature of the approximations contained in our treatment is gained through the inspection of Table 1, which collects Fermi-level energy values calculated for several electron occupation numbers and two different electric field amplitudes. The entries have

210

G. P. ARRIGHINI AND C. GUIDOTTI

been obtained by an easily feasible trial-and-trial procedure until satisfying the normalization requirement [eq. (2.19)] evaluated by numerical quadrature. The field-free

values

are seen to be spaced nearly uniformly by

according to the

Table

1. Fermi-level energy

predicted for the harmonic-well model

 

for different

electron numbers

and

different electric

field amplitudes E (a.u.).

well known behaviour of the quantum harmonic oscillator spectrum. The lowest energy

value (corresponding

to

and consequently all the others, however, are shifted

upward about

thus suggesting the picture of a ladder spectrum of discrete energy

values dephased with respect to the exact one. Some progressive deterioration seems to creep slowly into such harmonic picture as the electron number increases more and more. For a given number of electrons, moreover, the dependence of the Fermi-level energy

shift

on the electric field E is in perfect agreement with the exact

prediction,

Figs. 1-4 allow one to gain some further feeling about the quality of the approximation upon which our derivation of eq. (2.17) for n(x;E) has been founded. Figs. 1 and 2 represent the electron density as a function of the coordinate x, in the absence of external

electric field, for

 

respectively. Excellent overall agreement between

exact and approximate profiles

of

is immediately recognized. In particular,

there is a perfect reproduction

of the

electron distribution in the outer region, while for

the central core the approximation leads to a "simulation" of the exact behaviour, able to represent only in some average manner the typical spatial oscillations of the quantum density. Such "simulation" becomes seemingly more adequate as the electron number increases from the two cases actually display a similar behaviour, the drawing in Fig. 2 being unable to put in evidence details because of the too coarse-grain scale employed. Fig. 3 refers to the same situation illustrated in Fig. 2, the only change

corresponding to the presence of an external electric field

a.u. It should be manifest

ELECTRONIC CHARGE DENSITY OF QUANTUM SYSTEMS

211

that the effect of switching on the external field is simply to translate uniformly the whole electron distribution toward more negative x values, the shift amounting to

in accordance with the exact prediction [eq. (D.5)].

The behaviour of the approximate density n(x;E = 0) at both large and small x values

can

be

understood

considering the

analytical

properties

of the

function

 

 

 

, eq. (2.17)

[24,33].

As

,

in

fact,

 

and

 

exponentially, since asymptotically

 

 

 

 

as

.

On the other hand, from the asymptotic behaviour

 

 

valid for

 

,

as

,

according

to

,

so

that

we deduce

 

 

, a divergent result. The density at x=0, however, is finite, its value

from

eq.

(2.17) being

 

 

Very

rapid

small

oscillations

which characterize both Ai(z) and Ai'(z) at large negative values of their arguments become concentrated in the region of small x values around x=0. Such unphysical oscillations, which arise from the approximate nature of the QMP utilized in our approach, do not result evident in the figures because of scale reasons, but can be

partially perceived. Exact and approximate physical oscillations exhibited by n(x; E) are compared on a magnified scale in Fig. 4 for the case and E=1. a.u.

212

G. P. ARRIGHINI AND C. GUIDOTTI

ELECTRONIC CHARGE DENSITY OF QUANTUM SYSTEMS

213

Appendix A

The time-evolution operator

for a single electron moving in a 3D-linear potential

can be expressed in the form

where

A useful manipulation of the operator can be carried out by setting

being an unknown operator, with A differential equation for is easily obtained by deriving with respect to t both sides of eq. (A.3):

Noting that

214

G. P. ARRIGHINI AND C. GUIDOTTI

and therefore

Taking into account that operators associated with different labels j commute between each other, form eqs. (A.1), (A.3), (A.6) we get

The diagonal matrix element

of the QMP can therefore be written in the form

The evaluation of the simple integral contained in eq. (A.8) would lead, of course, to the known expression for the QMP of the system under study [32].

Appendix B

The function

of eq. (2.9) is conveniently expressed as follows

with

The Fourier representation of the Dirac delta function leads then to the result

and therefore,

The cubic form in t appearing in the exponential of eq. (B.1) is expressible as

ELECTRONIC CHARGE DENSITY OF QUANTUM SYSTEMS

215

where we have set

Thus the integration in the time variable involved in eq. (B.1) yields

where we have utilized the definition of the Airy function [33]

From the latter result, eq. (B.1) is finally cast into the form

Appendix C

Eq. (2.14) in the text can be derived in a straightforward way after choosing the z-axis along the direction of the vector , so that . Then , eq. (2.13), can be written down in the form

By a simple variable change the integration in

is expressible in terms of the Airy

function of proper argument [see eq. (B.3)], so that

 

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