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3Pe states of two-electron atoms. Feshbach-Rubinow approach

I. K. Dmitrieva (*) and G. I. Plindov (**)

(*) A. V. Luikov Heat and Mass Transfer Institute Byelorussian Academy of Sciences, Minsk 220728, U.S.S.R.

(**) Nuclear Power Engineering Institute, Byelorussian Academy of Sciences, Minsk, U.S.S.R.

(Reçu le 19 dgcembre 1985, accepti le 18 avril 1986)

Résumé.

2014

Les expressions analytiques de la fonction d’onde et de l’énergie de l’état 3Pe d’un atome à deux élec- trons sont obtenues dans le cadre de l’approximation de Feshbach-Rubinow. Les valeurs numériques de l’énergie

ainsi obtenues sont

en

bon accord

avec

les valeurs exactes. On montre que l’approximation FR donne les valeurs

exactes des deux premiers coefficients du développement de l’énergie

en

Z-1 et

une

bonne estimation du troisième coefficient.

Abstract

2014

The Feshbach-Rubinow approach is applied to obtain analytical expressions for the energy and

wave

function of the lower 3Pe state for helium-like atoms. The numerical results provide good estimates of the exact

eigenvalues. The FR approach is shown to give the exact values of the two first coefficients of the Z-1 expansion

for energies and

a

good estimate of the third coefficient.

Classification Physics Abstracts

31.90

The problem of bound states of two-electron atoms has a long history and attracts continuing interest

The variational method of solving this problem is

well known. In order to obtain accurate results, an appropriate trial function is chosen and a large number

of variational parameters is introduced. The number of parameters may be reduced provided that the approach used takes account of physical features of

the problem. One of the most advantageous is the

Feshbach-Rubinow approach [1] that allows one to reduce a three-body problem to a two-body one.

The modified FR approach when applied to the ground

state of a two-electron atom [2, 3] provided rather

accurate analytical energy and wave function expres- sions with the aid of but one or two variational parameters.

We shall show here that this approach is also of

success when applied to excited states. We shall analytically estimate the wave function and the energy of the lowest 3pe state for helium-like atoms with the

help of a single parameter.

Let us write down the Schr6dinger equation for

two electrons in the field of an infinitely heavy nucleus

with a charge Z :

Here ri , r2, V2 1 and V2 2 are the radius-vector and the

Laplacian of the first and second electrons; r12

=

r2 + ri - 2 rl-r2 cos 0 the distance between them.

Atomic units will be used in the paper.

It has been shown recently [4] that for the states with

a certain total angular momentum J and parity

1t

the six-dimensional equation (1) might be reduced to

a system of three-dimensional ones. For -3P’ states,

as well as for S-states, this system reduces to one

equation [4, 5]. The form of the wave function of the 3pe state

shows that in (1) the external variables, Euler angles a,

P and y are completely separated and (1) becomes

where

- - -1 - -

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:019860047080131500

(2)

It can be easily seen that in (4) the variables are not

separated, thus hindering an exact solution. We shall

use the FR approach [1, 3] in order to approximately

estimate the eigenvalues and eigenfunctions in equa- tion (3). The approach implies that in searching for

the variation of the function

the trial function f,(rl, r2, r12) is chosen as the function of a single-non-negative variable f = f (R) where

R

=

R(rl, r2, rl2). Then, so far It is a function of the variable R alone, integration over two other variables

may be performed in (5). This approach describes well the ground state of atomic and nuclear systems [1, 3].

Direct application of the FR approach to the doubly-excited pe state would cause divergent inte- grals. This is not surprising since the singularities of

Hamiltonian (4) are omitted. If the singularities are

taken account ot the trial function may be written as

Having in mind that the 3Pe state is symmetric relative

to the permutation ’1

-+

r2, it is convenient to choose the simplest form of R(rl, r2, r12) as

where a is the variational parameter. As R > 0, the

condition a > - 1 must hold

Performing the variation in (5), provided the integral f,(rl, r2, r12) f (ri, r2, r12) > is finite, yields

and integrating over r2 and r12, we arrive at

The main steps in derivation of (8) and the values of the coefficients A(a), B(a), C(a) and F(a) are cited in

Appendix.

By writting T(R)

=

R III 11 (R), we get the Schr6dinger-like equation to obtain the wave function and the energy of the 3Pe state of a two-electron atom

This is the wave equation of

a

particle in the Coulomb field with an effective charge

and an effective orbital momentum lee

=

7/2.

Note, that the use of the FR approach for the ground state of helium-like systems results in a similar equation

with an effective orbital momentum lee

=

3/2 [2, 3].

Solutions of (9) are well-known. Using one of them,

we

find now the energy and wave function of the lowest

lpe state in an analytical form as functions of a :

(3)

Before minimizing (10) over a, we shall consider (10) at a

=

0. As it follows from R estimation, a

=

0 cor- responds to an effective one-particle problem. Equation (10) implies that at a

=

0 the FR approach yields the

energy of the 3pe state of a two-electron atom

that coincides with the value obtained within the screened Coulomb approximation.

Minimizing E(a) over

a

for a given Z, we obtain

Table I.

-

Energies of the lowest ’P’ states for He-like atoms.

Having found the roots of (13) in a physically per- missible region - 1 a , 0, we obtain the energies

of He-like atoms presented in table I. The comparison

with the results of precision calculations shows that

(10) finely reproduces the energy of the 3pe state of

two-electron atoms beginning from He. These data

resulting from the application of a single variational parameter are more accurate than the results of calculations based on the truncated diagonalization

method with hydrogen basis with thirty variational parameters [6].

High accuracy in describing the binding energy

is due to a good quality of the wave function on the

average. It seems of interest to study the behaviour of the wave function in the vicinity of the points of

double electron-nucleus and electron-electron colli- sions. Equation (11) yields the expression at ri

-+

0,

r2

-+

0 or ri2

-+

0

Here is the root of (13).

Comparison with the expansion of the exact wave function, 4PO, of the 3pe state [4] ,

shows that the trial function f,(rl, r2, r12) well des-

cribes the domain in the vicinity of the electron- nucleus collision point (ri -+ 0 or r2

-

0), being

Table II.

-

Expansion coefficientsof3pe wave function

at ri(r2) 0 and rl2 -+ 0’

satisfactory in the vicinity of the electron-electron collision point (Table II). The description accuracy

for double collisions increases, in general, with increasing Z. However, for electron-electron collision,

in contrast to electron-nucleus one, the ultimate value

(at Z -+ oo) of the coefficient 1/9 Zef(am).am accounts only for about 54 % the exact value of 1/4.

The analytical function E(a, Z) and f,(a, Z) allows

one to present the energy and wave functions of the 3pe state of helium-like ions in the form of a Z-’

expansion. Indeed, the solution of (13) for large Z

may be given as

Two terms of (16) ensure am estimation with an error less than 1 % even for Z

=

1. Substituting (16) into (10)

and expanding (10) over Z-1 gives

(4)

The zeroth and first terms of (17) coincide with exact values [7], while the second-order term, due to the variational character of the estimate, gives an upper limit for the value of 82 constituting 94.5 % of the

exact value - 3.939

x

10-2 [7]. It is worth noting

that the first three expansion terms (17) yield more

accurate values of the energy of the 3pe state than total variational estimate (10) (Table I). This is explain-

ed by the positive coefficient ~3 in the Z - ’ expansion.

We shall show now that the FR approach may

provide a reliable estimate for the leading correla-

tional contribution to the energy.

The Z-1 expansion similar to (17) may also be obtained for the energy Eo of the ground state of the

He-like ions. Using the analytical function Eo(a, Z)

obtained within the FR approach [2]

and repeating the procedure similar to derivation of

(17) we arrive at

As for the 3Pe state, the first two terms of (19) coincide

with the exact values [7], the third one yields 92.7 %

the exact value of 82. The first three terms in (19) once

more yield better energy values than the direct varia- tional estimate (Table III). An approximate estimate

of the leading correlation contribution, AE,., to

the ground state energy within the FR approach is equal to the difference of 8R(a".) and 8’(a

=

0) values

obtained for the effective one-particle consideration

(at

a =

0) :

Table III.

-

Energies of the ground state of He-like

atoms.

This value is very close to the exact one

In (21), e2 is the exact value of the perturbation theory

second-order coefficient of Z - 1 obtained by very tedious variation-perturbation calculation [7]. t!1F is

the second coefficient value calculated within the Hartree-Fock method [8]. It is seen that the error in åEcor estimation within the FR approach is of the

same order as in 4t.

For the ’P’ state, we fail to find the value of t!1F in

the literature. By comparing (17) with the energy estimate in the framework of effective one-particle

consideration (12), we find an approximate value of the leading correlation contribution to the energy of the 3Pe state

We hope, that (22) gives the value of ð-Ecor, as it is the

case in (20).

So, the FR approach provides not only a fair estimate for the energy of doubly excited state of helium-like

ions, but also reliable values of the first three coeffi- cients of the Z-1 expansion.

Appendix.

Now, substitute the variables

As f is the function of the variable R, we may integrate over r2

= u

and r,2

= v

in (7). Because ft(R) is symme-

trical in r1 and r2, the range ri > r2 is only integrated The normalization integral for a half-volume

(5)

where

In a similar way we find

where

References

[1] FESHBACH, H. and RUBINOW, S. I., Phys. Rev. 98 (1955)

188.

[2] BHADURI, R. K. and NOGAMI, Y., Phys. Rev. A 13 (1976) 1986.

[3] SRIVASTAVA, M. K., BHADURI, R. K. and DUTTA, A. K., Phys. Rev. A 14 (1976) 1961.

[4] DMITRIEVA, I. K. and PLINDOV, G. I., in : 9th All-Union Conf. Theory of Atoms and Atomic Spectra,

Uzhgorod, 1985 ; J. Physique, in press.

[5] KOMAROV, L. I. and SOLODUKHIN, A. M., Izv. AN BSSR

N 2 (1985) 86.

[6] LIPSKY, L., ANANIA, R. and CONNEELY, M. J., Atom.

Data Nucl. Data Tables 20 (1977) 127.

[7] MIDTDAL, J., Phys. Rev. 138 (1965) A 1010.

[8] FROESE, Ch., Astrophys. J. 141 (1965) 1206.

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