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HAL Id: jpa-00208745

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Submitted on 1 Jan 1978

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Optical pumping of the metastable (2p5 3s 3P0) state of 21Ne

J.-P. Lemoigne, F. Sage, D. Lecler

To cite this version:

J.-P. Lemoigne, F. Sage, D. Lecler. Optical pumping of the metastable (2p5 3s 3P0) state of 21Ne.

Journal de Physique, 1978, 39 (2), pp.125-128. �10.1051/jphys:01978003902012500�. �jpa-00208745�

(2)

OPTICAL PUMPING OF THE METASTABLE (2p5 3s 3P0)

STATE OF 21Ne

J.-P.

LEMOIGNE,

F. SAGE and D. LECLER

Laboratoire de

Spectroscopie Atomique (*),

Université de

Caen, 14032

Caen

Cedex,

France

(Reçu

le 4 octobre

1977, accepté

le 8 novembre

1977)

Résumé. 2014 Le pompage

optique

dans une

décharge

H.F. faible du niveau métastable

2p5

3s

3P0

( 1S3 en notation de Paschen) a été obtenu à l’aide d’un laser continu à colorant. On observe un signal

de résonance

magnétique

correspondant à un facteur de Landé

g(3P0) =

(3,02 ± 0,30) x 10-4

supérieur

au facteur de Landé de l’état fondamental

g(1S0) =

(2,402 75 ± 0,000 05) 10-4 et en

bon accord avec les prévisions

théoriques

(3,08 x

10-4)

tenant compte du mélange des états

3P1

et

1P1

de la configuration

2p5

3s avec l’état

3P0

sous l’effet de l’interaction hyperfine. La précision

médiocre du résultat est due au temps de relaxation relativement court de l’orientation des méta- stables dans les conditions expérimentales actuelles.

Abstract. 2014 Metastable

2p5

3s

3P0 (1S3

in Paschen notation) atoms of 21Ne are optically

pumped

in a weak

discharge

by means of a C.W.

dye

laser. The magnetic resonance is observed for a g-factor

g(3P0) = (3.02

± 0.30) x 10-4

larger

than the ground state g-factor

g(1S0) =

(2.402 75 ± 0.000 05) x 10-4

and in

the

1P1

good and

3P1

agreement levels of the with

the theory 2p5

3s configuration through (3.08 x

10-4) taking

the into

hyperfine

account interaction. The the

mixing

of the précision

3P0

withof

the result is poor because of a

relatively

short relaxation time of the orientation of the

3P0

state in the

present

experimental

conditions.

Classification

Physics Abstracts

32 . 80B

1. Introduction. - For odd

isotopes,

the J = 0

levels of atoms may have

magnetic

moments

signi- ficantly

different from the pure nuclear values. The effect is due to the

hyperfine coupling

which mixes

non zero J contributions into the wave functions

describing

J = 0 states and therefore introduces some

electronic

magnetism

into these states.

Experimental

evidence of such effects has

already been reported [1, 2].

Similar behaviour is

expected

in the J = 0 metastable

states of rare gases. On the other

hand, optical pumping

of metastable

3P2

states of rare gases has

been achieved

by

several authors

[3, 4],

the metastable states

being initially populated by

a weak H.F. dis-

charge.

The orientation of the

2p5

3s

3Po

state

of

2 ’Ne

has also been observed

[4] but,

to our know-

ledge,

we

give

below the first

report

on a

magnetic

resonance

experiment leading

to the determination of the Lande factor of the

3Po

state

of 2’Ne.

2.

Experiment.

- The

geometrical arrangement

of the set up is shown

schematically

in

figure

1.

The cubic cell

(3

cm

edge length)

is filled with a

mixture of 0.5 torr of He and 0.015 torr of Ne enriched at

50 % in 21 Ne.

A weak

capacitive discharge

at 7 MHz

is maintained in the cell. A

simplified

energy level

diagram

of the Ne levels involved in our

experiment

FIG. 1. - Optical pumping and detection.

is

given

in

figure

2. One can think of several

optical pumping

schemes to achieve the orientation of the F =

3/2, ’Po

state. With our

experimental

arrange- ment we found that the most efficient way was to tune the

dye

laser to 5 882

À (lss-2p2) (Í).

The

absorption

of the

circularly polarized light propagating

in the

magnetic

field direction Oz and the

spontaneous

(’) Pumping schemes starting from the 3Po state need the laser to

be tuned on a particular hyperfine component, which was not possible with our « broad band » and free running dye laser.

(*) Associé au C.N.R.S.

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01978003902012500

(3)

126

FIG. 2. - First excited levels of Ne.

emission at 6 164

A (ls3-2p2)

ensure the desired orientation. The laser has a

long symmetric cavity (1.5 m)

of the Z type so that the modes are

separated by only

100 MHz. The line width of the laser is about 2

GHz, slightly

smaller than the

Doppler

width. We

found that a small

detuning

of the laser to the blue from the maximum of fluorescence

gives

a better

signal, probably

because the

hyperfine

components

(F

=

5/2 -

F’ =

5/2) (F

=

5/2 -

F’ =

7/2)

of the

21Ne

5 882

À

line are

preferentially

used for

optical pumping.

The total power at 5 882

A

is

typically

30 mW

and the beam is

expanded

in the cell to have a section of about 1

cm2.

The

steady magnetic

field

Ho

is

produced by

Helmholtz coils and has been calibrated

using

proton

magnetic

resonance.

The

rotating

field for

magnetic

resonance is pro- duced

by

two

pairs

of coils whose axes are in the Ox and

w

directions

(perpendicular

to

Ho). They

are fed

with R.F.

signals

90° out of

phase

with each other

by

means of two

high

power

amplifiers.

With such a

rotating

field we can avoid

Block-Siegert

effects that could have occurred with a conventional

oscillating

field.

The detection uses the crossed beam

technique (see

e.g.

[6]).

The source is an electrodeless

discharge lamp

filled with 2 torr of natural Ne. The

light

is

circularly polarized

and we monitor the modulation of

absorption

at the R.F.

frequency

on the 6 267

A

line

(lS3-2p.).

The

signal

is detected with a lock-in

amplifier

whose

phase

is

adjusted

to get either Lorent- zian

shaped

or

dispersion shaped signals.

A

signal

averager is used to

improve

the

signal

to noise ratio

further ;

its memories are

explored synchronously

with the

magnetic

field sweep.

3. Results. - We have observed

magnetic

reso-

nuances at

43.2, 46.7

and 52.3 kHz.

Averaging

times of

about two hours are necessary to obtain curves with a

signal

to noise ratio of about 20. The

experimental

curves are fitted to a sum of Lorentzian and

dispersion shaped

curves, centred at the same location and with the same width. This

procedure

is necessary because it is difficult to set the

phase

of the lock-in

precisely.

For

example

if we set the

phase

to

get

a Lorentzian

shaped

curve,

typical experimental

curve shows a deformation

corresponding

to a mixture of 20

%

to 25

%

of dis-

persion shaped

curve.

Figure

3

represents

the mean values obtained for the

position

of the resonances

FIG. 3. - Position of the resonances versus frequency. The errors quoted in the graph takes into account the standard error of the measurements and the systematic difference of the position of

symmetric and antisymmetric curves.

FIG. 4. - Statistics of the g-factor measurements : e with anti-

symmetric dispersion shaped curves ; + with symmetric Lorentzian shaped curves.

(4)

versus

frequency.

The

slope

of the

straight

line fitted to the three

experimental points

of

figure

3

gives

a

g-factor significantly

different from the pure nuclear

one of the

ground

state

lso (dotted

line on

figure 3).

Figure

4 represents the statistics of our

g-factor

measurements. It can be seen from this

figure

that a

slightly

different mean value is obtained for the measurements made with a Lorentzian

shaped

symme- tric curve

(S)

or with a

dispersion shaped antisymmetric

curve

(AS).

In our

present experimental conditions,

the relaxation time of the orientation of the

3Po state

is

relatively

short. If we assume for the

3Po

state a

metastability exchange

cross section

equal

to the one

measured

by

M. Pinard and M. Leduc

[5]

for the

3P2

state, we calculate a relaxation time of the orientation of about 12 us

(in

our pressure

conditions)

that is to

say a full width at half

height (FWHH)

of 63 gauss ;

experimentally

our curves have a FWHH of about 70 gauss. The

magnetic

field is swept from a few gauss to about 200 gauss. With such field variation the

discharge

in the cell

depends

on

Ho,

and the

optical pumping

may also vary with it. The

resulting

effect is a

background

which can have different effects on the

position

of

symmetric

or

antisymmetric

resonance

curves

(Fig. 4). Taking

into account the

dispersion

of

the measurements and

possible systematic

errors we

obtain the

g-factor

but we

hope

to

improve

this result in a near future.

4.

Theory.

- The

mixing

of

3P1

and

iPl

states in

the

3Po

wavefunction is

responsible

for the difference between the

g-factor

of the metastable state and the pure nuclear

g-factor

of the

ground

state. Calculation of these effects have

already

been

published

in the case

of cadmium

[1]

and mercury

[2].

The relations esta-

blished for an sp

configuration

can be used for the

p’s configuration

of Neon and the

hyperfine coupling

constants for the s electron and the p hole are deduced from the

hyperfine

structures of the

1 P 1 (ls2), 3P1(ls4)

and

3p 2(lss)

levels

using

the Breit and Wills

theory [7].

In the case

of Neon,

it is not necessary to use the modi- fication of the Breit and Wills

theory

introduced

by

Lurio

[8],

and as Neon is a

light

element the relativistic parameters 0

and ç

used

by

Lurio

[8]

and several references therein can be taken

equal

to 1.

Finally,

we

need the intermediate

coupling

coefficients introduced

by expanding

the

1 PI

and

3P1

real wave functions

1 ’Pl > and 13pl >

on the basis of pure LS

coupling

functions : ,

The table

gives

the different theoretical values of the Lande factor

g(3Po)

of

21Ne

that can be

computed

using

the different

possible

sets of A values and also different values of the intermediate

coupling

cons-

tant

fi.

Theoretical values

of

the

Landé factor

The

following A

values have been used in the

computation

and

for the

ground

state

g-factor.

As can be seen from the

table,

the

theoretical g

value

does not

depend strongly

on the intermediate

coupling

coefficient

fi.

In the frame of the Breit and Wills

theory,

we use

only

two individual

hyperfine coupling

constants a3, and a2p for the s electron and the p hole

respectively.

Such a

simplified theory

does not

give

very

good agreement

between the

experimental

set of A

values and the

computed

one

[ 11 ] .

A

discrepancy

of

the same

type

is to be seen between the different columns of the table where we have used the différent

possible

sets of A values to determine a3s and a2p.

5. Conclusion. - In

spite

of the poor

precision

of

our present

experimental

determination of the

g-factor

of the

3Po(ls3)

level of odd

isotope 21Ne

the

agreement

between

experiment

and

theory

is

fairly good

and

sufficient to

distinguish clearly

the

3Po g-factor

from

the

groundstate

one. An

experiment

is in progress to obtain narrower resonance curves

especially by lowering

the Ne pressure in the cell. An atomic beam of metastable rare gases atoms is also in construction in the

laboratory

to enhance the

precision

of our

present

measurement and to allow us to extend it to J = 0 metastable states of other rare gases.

We are very

grateful

to F. Laloe and M. Leduc from

the Laboratoire de

Spectroscopie

Hertzienne

(ENS Paris)

for

helpful

discussions

throughout

this work.

(2) C. Delsart, J. C. Keller, Private communication.

(5)

128

References [1] SIGNOLLE, J. P. and LECLER, D., Opt. Comm. 13 (1975) 60.

[2] LAHAYE, B., MARGERIE, J., J. Physique 36 (1975) 943.

[3] SCHEARER, L. D., Phys. Rev. 180 (1969) 83; 188 (1969) 505;

Phys. Lett. 28A (1969) 660.

[4] LEDUC, M., LALOE, F. et BROSSEL, J., C. R. Hebd. Séan. Acad.

Sci. Paris 271B (1970) 342.

[5] PINARD, M., LEDUC, M., J. Physique 38 (1977) 609.

[6] LALOE, F., Thesis Paris (1970).

[7] BREIT, G., WILLS, M. A., Phys. Rev. 44 (1933) 470.

[8] LURIO, A., Phys. Rev. 142 (1966) 46.

[9] DELSART, C., KELLER, J. C., Opt. Comm. 16 (1976) 388.

[10] GROSOF, G. M., BUCK, P., LICHTEN, W., RABI, I. I., Phys. Rev.

Lett. 1 (1958) 214.

[11] LIBERMAN, S., Physica 69 (1973) 598.

[12] LA TOURETTE, J. T., QUINN, W. E., RAMSEY, N. F., Phys. Rev.

107 (1957) 1202.

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