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Hyperfine structure evolution in an electric field and determination of tensor polarizabilities in He (4 and 5 1D)

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Hyperfine structure evolution in an electric field and determination of tensor polarizabilities in He (4 and 5 1D)

A. Denis, Y. Ouerdane, G. Docao and J. Désesquelles

Laboratoire de Spectrométrie Ionique et Moléculaire, associé

au

CNRS,

Université de Lyon I, Campus de la Doua, 69622 Villeurbanne Cedex, France

(Reçu le 5 août 1986, accept6 le 8 octobre 1986)

Résumé. 2014 On étudie la variation de la structure hyperfine des niveaux

n

1D de 3He dans

un

champ électrique statique. Par

une

méthode de battement quantique

sur un

faisceau d’hélium excité par

une

feuille de carbone, on suit l’évolution temporelle du taux d’alignement des niveaux 4 et 51D pour

une

série de champs électriques. On

en

déduit

les valeurs de la polarisabilité tensorielle de

ces

niveaux.

Abstract.

2014

Variations of hyperfine structure in 3He (n 1D)

are

calculated

as

a function of an applied electric

field. Using

a

quantum beat method

on a

fast helium beam excited and aligned by

a

thin carbon foil,

we

observe the time evolution of the alignment for

a

set of static electric fields. Tensor polarizabilities of levels

are

deduced.

Classification

Physics Abstracts

32.60

-

34.50F

-

35.10D

1. Introduction.

Beam-foil spectroscopy is now well known for its efficient measurement of fine and hyperfine structures

in many neutral and ionised atoms. Zero field quantum

beat experiments on 3He by Brooks et al. [1] are in fair

agreement, within 2 % error bars, with the best avail-

able theoretical and experimental values [1-4] for the

low lying levels 4 1D and 5 1D.

Rather less common is the extension of this technique

to optical polarization measurements of structures when combined with applied electric fields. The study

of electric field induced quantum beats seems to have

been reduced to hydrogenic species, namely hydrogen [5, 6], charged helium [7] and doubly ionized lithium

[8]. The case of non-hydrogenic species has not, as far

as we know, been studied using this method.

We report here the observation of intensity fluctu-

ation in the emission of Stark-perturbed 2p ’P - 4d ’D

and 2p ’P - 5d ’D radiations from helium atoms formed

by the passage of helium ions through a carbon foil.

Comparison of measured frequencies with theoretical calculations using a tensor operator formalism leads to the determination of the tensor polarizability of these

levels.

2. Theory.

To treat the problem of 3He atom in an electric field we

begin with a Hamiltonian which includes electrostatic interactions (electron-electron and electron-nucleus)

and magnetic interactions (spin-orbit, spin-other orbit, spin-spin and nuclear moment-angular moment). In 3He the hyperfine coupling energy is not negligible compared to the singlet-triplet splitting and the mixing

of these two multiplets has to be taken into account in

the case of the ’D levels. As a consequence, a small fraction of the hyperfine structure of the triplet state is

transferred to the singlet in which it can be observed.

The field-independent terms of the matrices have been calculated and are given in tables I and II. These matrix

elements are similar to those of Brooks et al. [1]

deduced from the work of Lurio et al. [9]. The Fermi

contact term A (1s, 3He+) and the singlet-triplet mixing parameter a [10, 11] are taken equal to

-

4 332.8 MHz [12] and 17 527.3 MHz/n3 [1,10] re-

spectively. The magnetic dipole interaction parameter

a is equal to - 0.68 for n

=

4 and - 0.35 for n

=

5. D is

the singlet-triplet separation ; dlg d2 and d3 are the fine

structure splitting of the triplet states.

When an electric field perturbation is added, we obtain a Stark Hamiltonian [13] which splits into two parts : HStark

=

Hr, + Ht. The scalar contribution HS produces an overall shift of the levels and the tensor

contribution Ht splits the different Mf magnetic

sublevels.

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01987004802022700

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Table I.

-

Matrix elements of the total system hamiltonian for Mf I

=

1/2. Lx., and ati are related to singlet states

and (IS3 and (It3 are related to triplet states. The matrix has to be completed by symmetry.

i) For a singlet :

E

is the electric field strength. as (J) and a t ( J ) are the scalar and tensor polarizabilities of the J level and are

defined as follows :

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Table II.

-

Matrix elements of the total system Hamiltonian for I Me I

=

3/2, with the same notations as in table 1 for scalar and tensor polarizabilities. The matrix has to be completed by symmetry.

The sum is over all J’ levels which lie near the J level. wo is the energy of the J level and w’ the energy of a close J’. (Jllp, 11 V’) is the electric dipole matrix element.

ii) For a triplet,

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It can be seen from these expressions that the scalar polarizability plays a role only in diagonal elements and

that the tensor polarizability contributes to M

=

M’

transitions because of

«

3 j coefficient » rules.

The addition of Stark perturbation allows us to

determine the entire matrices displayed in tables I and II.

Diagonalisation of these matrices gives the energy of all the levels together with their evolution as a function of the electric field.

In figure 1 we illustrate the evolution of singlet states

alone. Because only the 41 I Mf = 0 terms are coupled,

just two frequencies appear :

and

These two frequencies were the subject of our exper- imental work.

Fig. 1.

-

Variations of hyperfine magnetic sublevel energies

as a

function of squared electric field in 3He (4 ’D).

3. Experiment.

To measure the energy differences between n ’D sub- levels of 3He and their evolution as a function of an

electric field, the quantum beat technique has been

used on fast-foil excited beam.

The ion source of a 350 keV Danphysik accelerator is filled with a mixture of helium-3 and helium-4, the

L’ L L Z/J 000 - ClJ’

latter being used for precise calibration of the atom

velocity. After acceleration up to about 100 keV, the 3He’ beam is sent through a thin (10 ug/cm2) self-

supporting carbon foil and through an electric field parallel to the helium beam. The field is produced by a

set of two circular metallic plates biased at potential

+ V and 0 respectively. The carbon foil is placed on the

first electrode (Fig. 2).

Fig. 2.

-

Experimental arrangement. The plates used to apply the electric field

are

140

mm

in diameter, are separated by

a

distance of 3

cm

and have a circular aperture 4

mm

in diameter d : diaphragm, 1: focus lenses, p : linear polarizer,

if : interference filter,

s :

slit, P.M. : EMI 9635Q Peltier cooled photomultiplier, F.C. : Faraday cup.

The light emitted at 90° to the beam passes through

an optical system that includes a lens, a linear polarizer

and an interference filter. A second lens focusses the transmitted light on a slit placed in front of the detector

(P.M. EMI 9635 Q). The decays of 4 1D and 5 1D levels

are observed at 4 922 A and 4 388 A respectively. At

the energy we chose to use, both amplitude and the

total light are more intense than at higher energies [14].

Moreover, the range of studied frequencies (80-

250 MHz) does not require a long displacement of the target for exploration of several periods of modulation.

On the other hand, the lifetime of the target is short at

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such a low velocity and we are obliged to use very weak beam intensities ( ~ 100 nA).

The main experiment necessitates the measurement of the light intensity at the exit of the polarizer turned alternately parallel (III) and perpendicular (I..L.) to

the helium beam, repeating the measurements many times for each foil position. The same operation is repeated for about twenty foil positions separated by a regular interval. From a series of recordings, the

7,, -11

variation of

A’ = I II + 2 ; ..L. can be deduced as a

function of the distance to the target (Fig. 3b), the

electric fied being fixed at a given value. We use this parameter A’ to free ourselves of all absolute intensity

variations when the distance to the foil changes (expo-

nential damping of oscillation amplitude) or as a

function of time (target ageing).

Fig. 3.

-

Modulation of the polarization ratio of the

41D 3He level as

a

function of distance to the target when

a

627 V/cm field is applied (3b). Quantum beat pattern for the 4He line at 3 888 A recorded before (3a) and after (3c) the 3He

curve

(3b). From these curves 3a and 3c the evolution of the velocity from va

=

1.987 to Vc

=

1.938 mm/ns is deduced and consequently vb =1.962 mm/ns. The

curve

3b is an

example of measurement obtained when the applied electric

field is such as the frequencies 5/2, 3/21 - 3/2, 13/21 and 5/2, 1/2 ( - 3/2, 1/2) are too close to be resolved.

A least square analysis of the sinusoid gives the wavelength of the beat corresponding to the difference of energy between two sub-levels for a given electric

field strength. In the present case, because four levels selectively coupled two by two by the field are involved,

the recording includes two sinusoids rather than just

one. However, the modulation corresponding to the

difference in energy between the 5/2, 11/21 and 3/2, 1/2 sub-levels only reaches a significant amplitude for

field strenghts above 1 kV/cm. At lower field strengths, only the beats due to the 5/2, 13/21

-+

3/2, 13/21 transi-

tion are observed.

In order to deduce these frequencies we need to

know a precise value of the emergent beam velocity.

Therefore, we recorded the modulation curve of the

4He line at 3 888 A whose frequency is known to be

658.55 MHz [15], without changing the accelerator volt- age. The curves given in figures 3a and 3c correspond

to the modulated curve recorded before and after the main experiment (curve 3b). They show a systematic

decrease in velocity (typically of the order of 3 % during a whole sequence) due to thickening of the foil, which is also responsible for the growing of intensity in

curves 3a and 3c (the cross section increases when the

energy decreases). The adopted velocity is the mean

value of the two extreme velocities. An additional shift of velocity is due to the fact that the energy loss is not the same for helium-3 and helium-4 ions submitted to the same accelerating voltage. Using the curves of

energy loss of Ziegler [16], correction of velocity can be

made : it is of the order of 1 % for a 10 ug/cm2 target thickness and an incident energy of 100 keV

Another interesting result obtained from these re-

cordings is the target position which coincides with the

zero phase of beat. The reproductibility of measure-

ments allows us to fix the foil position with a precision

of 50 tim.

4. Analysis and results.

For each electric field, the experimental data are fitted

to a sinusoid or a sum of sinusoids with the help of a

least square programme.

Fig. 4.

-

Evolution of the two frequencies 5/2, 332 1 - 3/2, 3/2) and 5/2, 1/2 - 3/2, 1/2

as a

function of squared

electric field strength Solid lines are theoretical curves calcu-

lated from matrices of tables I and II with best value of

at.

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The error on each frequency is estimated to be of the order of 5 MHz when uncertainties in the beam vel-

ocity, target position and statistics are taken into account. Figure 4 illustrates the frequency measure-

ments made for electric fields ranging from 0 to

1.3 kV/cm.

For 4 1D level we compare the experimental data

with theoretical curves obtained with different values of the tensor polarizability. This is done for both trans-

itions. The best X2 value is obtained with:

for the

for the

and with:

for both transitions simultaneously.

For the 5 1D level with similar curves the result is :

In table III our present results are compared with

theoretical and other experimental values. Previous

beam-foil data were obtained in 4He using different geometries [17,18]. The level-crossing data of Szostak et al. [19] are also available for comparison. The pre- cision of the measurements is about 1 %. Agreement is

also found with calculations using the Coulomb approxi-

mation of Bates and Damgaard [20] for the dipole

matrix elements and the table of Martin [21] for the

level energies.

Table III.

-

Tensor polarizabilities (kHz/(V/cm)2) of 4 and 51D levels in helium.

References

[1] BROOKS, R. L., STREIF, V. F. and BERRY, H. G., Nucl. Instrum. Meth. 202 (1982) 113.

[2] BESSIS, N., LEFEBVRE-BRION, H. and MOSER ; C. M., Phys. Rev. A 135 (1964) 957.

[3] DESCOUBES, J. P., Thèse d’Etat, Paris (1967) ; DESCOUBES, J. P., in Physics of

one-

and two-

electron atoms (Elsevier : North-Holland, Amsterdam) 1969.

[4] LIAO, P. F., FREEMAN, R. R., PANOCK, R. and HUMPHREY, L. M., Opt. Commun. 34 (1980)

195.

[5] ANDRÄ, H. J.,, Nucl. Instrum. Meth. 90 (1970) 343.

[6] ALGUARD, M. J. and DRAKE, C. W., Nucl. Instrum.

Meth. 110 (1973) 311.

[7] BOURGEY, J., DENIS, A. and DÉSESQUELLES, J., J.

Physique 38 (1977) 1229.

[8] PINNINGTON, E. H., BERRY, H. G., DÉSESQUELLES,

J. and SUBTIL, J. L., Nucl. Instrum. Meth. 110

(1973) 315.

[9] LURIO, A., MANDEL, M. and NOVICK, R., Phys.

Rev. 126 (1962) 1758.

[10] DEROUARD, J., LOMBARDI, M. and JOST, R., J.

Physique 41 (1980) 819.

[11] MILLER, T. A. and FREUND, R. S., Adv. Mag. Res. 9 (1977) 50.

[12] SCHUESSLER, H. A., FORTSON, E. N. and DEHMELT, H. G., Phys. Rev. 187 (1969) 5.

[13] ANGEL, J. R. P. and SANDARS, P. G. H., Proc. R.

Soc. London Ser. A 305 (1968) 125.

[14] PERCIVAL, I. C. and SEATON, M. J., Philos Trans. R.

Soc. London A 251 (1958) 114.

[15] WIEDER, J. and LAMB, Jr. W. E., Phys. Rev. 107 (1957) 125.

[16] ZIEGLER, J. F., Helium stopping powers and ranges in all elements (Pergamon, New York) 1977,

Vol. 4.

[17] OUERDANE, Y., DENIS, A. and DÉSESQUELLES, J., J. Physique Lett. 44 (1983) L-871.

[18] OUERDANE, Y., DENIS, A. and DÉSESQUELLES, J. to

be published in Phys. Rev. A (1986).

[19] SZOSTAK, D., VON OPPEN, G. and PERSCHMANN,

W. D., Phys. Lett. 76A (1980) 376.

[20] BATES D. R. and DAMGAARD, A., Philos Trans. R.

Soc. London A 242 (1949) 101.

[21] MARTIN, W. C., J. Phys. Chem. Ref. Data 2 (1973)

257.

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