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HAL Id: jpa-00208868

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Submitted on 1 Jan 1978

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Frequency dependent multipole polarizabilities of atomic systems

S.I. Easa, G.C. Shukla

To cite this version:

S.I. Easa, G.C. Shukla. Frequency dependent multipole polarizabilities of atomic systems. Journal de

Physique, 1978, 39 (12), pp.1259-1262. �10.1051/jphys:0197800390120125900�. �jpa-00208868�

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FREQUENCY DEPENDENT MULTIPOLE POLARIZABILITIES

OF ATOMIC SYSTEMS

S. I. EASA and G. C. SHUKLA

Department of Physics, Basrah University, Basrah, Iraq (Reçu le 8 mai 1978, accepté le 4 septembre 1978)

Résumé.

2014

On calcule les dépendances en fréquence des polarisabilités multipolaires de systemes atomiques en utilisant une méthode variationnelle qui rejoint, à fréquence nulle, le formalisme du

cas statique. Ce développement a été appliqué au calcul de l’énergie de dispersion entre paires d’hydro- gène et d’helium.

Abstract.

2014

A variational calculation for frequency dependent multipole polarizabilities of atomic systems is proposed ; for zero frequency it reduces to our previous formalism of the static case.

This present scheme has been applied to obtain the dispersion energy between interacting hydrogen

and helium pairs. Our results are in harmony with others.

Classification Physics Abstracts

31.10

The calculation of multipole polarizabilities was

initiated by the use of single [1] and double [2] per- turbation theory. Recently Rivail and Rinaldi [3] have proposed an alternative single perturbation theory applicable to static multipole polarizabilities of atomic

systems. We have already generalized [4] this scheme.

In this procedure the total energy of the atomic system is expressed in terms of expansions involving induced multipole moments so that the static multipole pola-

rizabilities are obtained as second order derivatives of the total energy w.r.t. p,m, Pt being the associated Legendre polynomial. Furthermore, Rivail and Rinaldi’s work was based on the variational cal- culation with one variational constant in the perturbed

wave function while we took an appropriate number

of variational constants till convergence was achieved in static multipole polarizabilities.

The schemes [3, 4] are parallel to the method of single perturbation [1] or double perturbation [2], if not

identical. In the present communication we extend such [4] a scheme to incorporate the frequency- dependent multipole polarizabilities of atomic systems.

We propose the following expansion for the total

energy, the applied electric field being harmonic in

time with angular frequency w,

in the notation of earlier references [3, 4], al(w) being

the frequency dependent multipole polarizability and

Note that for w = 0, the expression (1) reduces to the

static expression [3, 4]. We outline the procedure to

work out aI(w) by taking the perturbed wave function

as

for one variational constant. Note that the variational

constant Àl depends on frequency.

Rewrite 03C8(±) as

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:0197800390120125900

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1260

Now, E(± w) as defined below is minimized w.r.t.

variational constant 03BBl(± w), subject to normalization

We obtain

Substituting for Âl(± w) in (7) we have

at(w) has the following expression

which for w = 0 reduces to the static case as obtained

by Rivail and Rinaldi [3].

al(w) may be written as

For two variational constants,

the minimization of E( ± w) w. r. t. Âl(± w) and bl(± w)

as given by eq. (6) with x1( ± ) given by (12) yields

where C1(:t w) and C2( ± w) a’re solutions of the

following matrix equation,

Using equations (12) to (14) in (6) we get

which simplifies to

Note that oei(0) are static multipole polarizabilities ; they have the same expression as in our earlier commu-

nication [4]. We write down values of oei(0) and other expressions in (17) as

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Considering n variational constants in the perturbed wave function implies the following choice for X,(±) :

where there are n constants Âl(± w), bl( ± w), ôi(+ w),

...

Minimizing eq. (6) w.r.t. n constants Ài( + w), bl(± w), ... and using xi( + ) as given by (18),

we get

which is the [N, N - 1] Padé approximant for al(w) [5].

Note that, now, SnL and PnL have cumbersome

expressions unlike those for n = 1 and 2 as given

above by eqs. (11) and (17) respectively.

We work out ocl(w) for atomic hydrogen and He (our model for He is the same as in an earlier commu-

nication [4]) by using eq. (19) and varying the varia-

tional constants from 1 to 5. In table 1 we list the

TABLE 1

Dipole resonance frequency of atomic system (in a.u.)

with varying number of variational constant n

resonance frequencies for H and He (dipole case)

while table Il contains the numerical values of the

dipole polarizability of the He atom at imaginary frequency. We compare our results with earlier works.

Our values of lJ.1(iw) for the He atom (dipole case)

are in harmony with those of Broussard and Kestner [2]

because our model for a1(w) for the He atom is equi-

valent to a calculation using the uncoupled Hartree-

Fock approximation, as in reference [2]. Our values for

TABLE Il

Dipole polarizability of He at imaginary frequencies

dipole resonance frequencies with 5 variational cons-

tants are in harmony with earlier works, both for H and He atom [6-9].

An important application of frequency-dependent multipole polarizability is to obtain the dispersion

force coefficient for the long range interaction between two (or more) interacting neutral systems by utilizing

the generalized Casimir-Polder integral formulas [5]

where

lJ.,(iy) refers to frequency dependent multipole pola-

rizabilities at an imaginary axis w = iy, the second order dispersion energy between two interacting

systems is given by [10],

The following expression for the second-order

dispersion energy for interacting hydrogen and He

pairs results using eqs. (19) to (22)

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1262

The corresponding expressions in earlier work are

The present work is concluded with the remark that

our values for E2(H-H) are in harmony with those of Dalgarno and Bartolotti et al. Note that we have worked out ai(w) by taking only 5 variational cons-

tants. However, the slight discrepancy in our values

for E2(H-H) and those of Dalgarno and Bartolotti

et al. should be reduced by increasing the number of

variational constants for al(w),- our values for

E2(He-He) are comparable with those of Broussard and Kestner [2] as both works use the uncoupled

Hartree-Fock approximation. We are extending our

scheme for the lJ.1(W) H atom [4] equivalent to the coupled Hartree-Fock approximation.

The authors are grateful to Dr. R. Al Rashid for his encouragement throughout the present investigation.

References

[1] LANGHOFF, P. W. and HURST, R. P., Phys. Rev. 139A (1965)

1415.

[2] BROUSSARD, J. T. and KESTNER, N. R., J. Chem. Phys. 53 (1970) 1507.

[3] RIVAIL, J. L. and RINALDI, D., C. R. Hebd. Séan. Acad. Sci.

Paris 283B (1976) 111.

[4] SHUKLA, G. C. and EASA. S. I., Solid State Commun. 26 (1978) 873.

[5] LANGHOFF, P. W. and KARPLUS, M., J. Chem. Phys. 53 (1970) 233.

[6] YOUSIF, F. N. and SHUKLA, G. C., Phys. Rev. A 17 (1978) 1269.

[7] DALGARNO, A. and VICTOR, G. A., Proc. Phys. Soc. (London) 90 (1967) 605.

[8] LUYCKU, R., COULIN, Ph. and LEKKERKERKER, H. N. W., Chem. Phys. Lett. 48 (1977) 187.

[9] Atomic Energy Table (NBS), Circular No.

[10] DALGARNO, A., Adv. Chem. Phys. 12 (1967) 143.

[11] BARTOLOTTI, L. J. and TYRELL, J., Chem. Phys. Lett., 39

(1976) 19.

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