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g Factors and lifetimes in the B state of molecular iodine

M. Broyer, J.-C. Lehmann, J. Vigue

To cite this version:

M. Broyer, J.-C. Lehmann, J. Vigue. g Factors and lifetimes in the B state of molecular iodine.

Journal de Physique, 1975, 36 (3), pp.235-241. �10.1051/jphys:01975003603023500�. �jpa-00208248�

(2)

g

FACTORS AND LIFETIMES IN THE

B

STATE

OF MOLECULAR IODINE

M.

BROYER,

J.-C. LEHMANN and J. VIGUE Laboratoire de

Spectroscopie

Hertzienne de l’ENS

Université de Paris

VI, 4, place Jussieu,

Tour 12-E1 75230 Paris Cedex

05,

France

(Reçu

le 31 octobre

1974)

Résumé. 2014 Nous avons mesuré les facteurs de Landé et les durées de vie des niveaux de vibration- rotation de la molécule I2 excités par les diverses raies des lasers à argon ionisé et à krypton ionisé.

Pour cela nous avons utilisé les méthodes de l’effet Hanle et des résonances en lumière modulée.

Les valeurs expérimentales obtenues pour gJ varient beaucoup avec le nombre quantique de vibra-

tion v’ de l’état B. La relation théorique que l’on peut établir entre gJ et CI la constante de structure hyperfine

magnétique

est assez bien vérifiée.

Abstract. 2014 We have measured

the g

factors and lifetimes of the vibration-rotation levels of molecular iodine excited

by

the various lines of Ar+ and Kr+ lasers. To obtain these results we have used the Hanle effect and the method of resonances in a modulated

light

beam. The

experimental

values of gJ vary very much with v’ the vibrational quantum number of the B state. A theoretical

relationship

between gJ and

CI,

the

magnetic hyperfine

constant, has been

proved

to be valid to a good

approximation.

Classification

Physics Abstracts

5.448

1. Introduction. - The first measurements of the

magnetism

of the B state of

12

were

performed

in 1914

by

Wood and Ribaud who studied the

Faraday

effect

[1].

In

1937, using

the

theory

of Serber

[2],

Thomas

Caroll

[3] interpreted

the results of Wood and Ribaud : for the level v’ = 27 J’ = 109 excited

by

the

Hg

line 5 461

Á, they

gave : gJ = 0.06. Until

recently [4, 5]

it was the

only

information about the

magnetism

of the B state.

In order to measure

the g

factors of several indi- vidual rotational-vibrational levels of the B state we

have used the Hanle effect

technique

which was

developed

a few years ago for the

study

of molecular excited states

[6].

When it was necessary to measure the g J factor

[4]

directly,

we used the method of resonances in a

modulated

light

beam introduced

by

Series

[7].

By

these

experiments

we have measured the values of g J and i for the

following

levels of the B state :

Independently

of our

work,

Paisner and Wal- lenstein

(5) (7)

have used the method of quantum beats to measure g factors and lifetimes in the B state. We shall compare their results with our own at the end of this paper.

2. Hanle effect. - 2.1 ZEEMAN SPLITTING IN THE

B STATE OF

12.

- The Hanle effect of molecular iodine is

complicated

since each rotational level J is

split

into

a great number of

hyperfine

sublevels.

The nuclear

spin

of the

12’I

nucleus

being 5/2,

each level of the

B3Ilô

u state is

split

as follows :

e For even J the state is

ortho,

the total nuclear

spin

I =

h

+

/2

takes the values

1,

3 or 5. Each rotational level is

split

into 21

hyperfine

sublevels.

e For odd J the state is para, I =

0, 2, 4,

each rotational level is

split

into 15

hyperfine

sublevels.

The

hyperfine

structure of some of these levels has been measured

by

Levenson et al.

[8].

It is

mainly

due

to the

quadrupole

moment of the two nuclei. There-

fore,

I =

h

+

12

is not a

good

quantum number and

the

eigenstates

are

given by :

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01975003603023500

(3)

236

The Zeeman hamiltonian is written :

g J is the

rotational g

factor

gl is the

nuclear g

factor of the 127 1

nucleus,

gi = 1. 12 [9].

gl, should be the

magnetic shielding

tensor. In fact if

J >

I, (i.

e. as soon as J >

10),

it may be shown

[10]

that it is sufficient to

consider g1

as a number. For

most

rnolecules g1

is

negligible

gi z

10-4 [11].

We

shall come back to this

point

at the end of this paper.

In the low field limit a Landé factor 9 tE can be defined for each

hyperfine

sublevel :

where

The

intensity

of the fluorescence is obtained

using

irreducible tensor formalism

[20].

It is

proportional

to

A(E, F, k, J’)

is the contribution of each

hyperfine

sublevel.

J’ is the rotational number of the excited state.

Tr

is the inverse of the radiative lifetime of the excited state and T, the inverse of the total relaxation time.

E is the excitation

operator, 5)

the detection

operator.

E:

and

U)k

are the components of î and 0 on the basis of irreducible tensor operators

Tq.

By

this method the H anle effect curves may be calculated. It must be noted that for a

given

rota-

tional level the

shape

of the curves

depends only

upon the relative values of gj and

(g,

+

g,),

r

being only important

for the width of the curves. Two cases

should then be considered :

almost

equal

to gj. The Hanle effect curves are then lorentzian. From the width of the

experimental

curves

at zero pressure the

product

g J z is deduced.

2) 1 gj 1 5 j (gi + gt).gü

varies very much for the

various

hyperfine

sublevels. Its

sign

may

change.

The

Hanle effect curves are very different from lorentzian

ones. The relative size and width of the

dispersion

and

absorption

Hanle effect curves are very sensitive

to the relative values of gj and

(gl

+

gl).

From the

comparison

between the

shape

of

experimental

and

theoretical curves the gi value is deduced as a

function of (g,

+

g).

Il g, « gj, one can

neglect gl

and deduce

the value of gj. Then from the width of the curves the

lifetime

is also obtained.

Both of these cases occurred in the set of rotational levels studied here.

2.2 EXPERIMENTAL sEr uP. -

Figure

1 shows the

experimental

set up. The

magnetic

field is

produced by

an

electromagnet.

The fluorescent

light

is observed in the direction of the

magnetic

field

using

a mirror

(this

mirror is not drawn on the

figure).

The

pola-

rization is detected

by

a

rotating quarter

wave

plate

followed

by

a fixed

polarizer. By changing

the

phase

of the lock-in detector

by

900 it is

possible

to record a

dispersion

or an

absorption

Hanle effect curve. The monochromator is necessary when a laser line excites

simultaneously

several rotational levels of the B state

[21].

. |

FIG. 1. - Expérimental set up for the Hanle effect experiment.

The laser beam was

expanded by

a

lens,

the power

density

of the laser

being

then about 20

mW/cm.

We have verified that in these conditions saturation effects are

negligible.

Our observations

related

to these saturation effects in

12

have been

published

elsewhere

[12] [13].

2.3 EXPERIMENTAL RESULTS. - From the observa- tion of the Hanle

dispersion

curves recorded under suitable

conditions,

the

sign

of gj can be deduced.

For all levels studied gj is found to be

negative,

that

is the same

sign

as an electron.

2. 3 .1 Case 1.

gj (g, + . -

The levels excit-

ed

by

the laser lines 5 145

A

and 5 309

A

are most

representative

of this case. For the levels excited

by

the laser line 5 682

A ;

the determination of gj

by comparison

between

experimental

and theoretical

curves was also

performed

but the

precision

was very poor. The lifetimes of these levels are deduced from the width of the Hanle curves

extrapolated

to zero

pressure. The whole set of results obtained is pre- sented in table 1.

2. 3 .1.1 Excitation at 5 145

A. - Two

rotational

levels J’ = 12 and J’ = 16 of the set v’ = 43 are

(4)

TABLE 1

The whole set

of results.

The values

of gl

with * are estimated

by

the method

explained

in 4. It must be

remarked that we measure

a (2)

the cross section

of destruction of alignment.

On the contrary, Paisner et al.

measure

0’(0)

the cross section

of destruction of

the

population.

( 1 ) On this level, we had already reported [4] g J = - 0.31 ± 0.06 and i = 2.9 ± 0.05 s. These values were obtained by assuming

g, = 0 which is evidently wrong since we have measured gl = 3.4 for the laser line 5 017 A.

excited. The Hanle effect was

simultaneously

observed

for both levels since in order to

separate

the fluores-

cence from the two levels the slits of the monochroma-

tor would need to be

20 Il

wide and would therefore

give

too low a

signal

to noise ratio for any serious measurements. To calculate the theoretical curve

shapes

we assumed that the two levels involved have the same g J factor and the same lifetime 1’. This

assumption

is in

good

agreement with the

interpre-

tation of

the g

factor

developed

in the last

paragraph

of this paper;

following

this

interpretation

gj is

independent

of the rotational number J’ and

depends only

upon the vibrational quantum number v’.

The

dispersion

and

absorption

curves are in this

case very different from each other both in their size and their width. Therefore the

precision

of the fit is rather

good :

20

%.

Furthermore the Hanle effect

curves are so narrow that

magnetic predissociation [14]

can be

neglected.

-

2.3.1.2 Excitation at 5 309

A.

- The situation is very similar. Two levels v’ = 32 J’ = 9 and v’ = 32 J’ = 14 are excited and

they

are observed simul-

taneously.

The gj factor of both levels is fitted with

a

precision

about 15

%. Again

the

magnetic predis-

sociation has no influence on the Hanle curves.

2. 3 .1. 3 Excitation at 5 682

Á.

- Each level excited

by

this line has been studied

separately, using

the monochromator with narrow slits

(60

to 100

03BC).

Furthermore, gj being

of the order

of gj,

the curves

were not

drastically

different from lorentzian. At the

end,

the width of the Hanle curves

being

in this

case about 2 000 to 5 000 gauss the

magnetic predisso-

ciation was not

negligible.

Therefore the

precision

of

the gj determination was rather poor : about 40

%

or

50 %.

The results are shown in table I. The levels v’ =

21,

J’ = 11 b and J’ = 122 have been studied

separately

but no

meaningful

difference was noticed in their gj factors.

As an illustration of our method for the determi- nation of gj,

figure

2 shows the

agreement

between the theoretical and

experimental

curves in the case

of an excitation at 5 309

Á.

The

dispersion

and

absorption

curves are recorded at the same

sensitivity.

It must be noticed that their sizes and their widths are

quite different.

FIG. 2. - Comparison between theoretical and expérimental Hanle

curves for the excitation at 5 309 A. The points are theoretical.

The 12 pressure was 3 mtorr.

2.3.2

Case 2. gj » (g,

gj ~

9r 9i) + gl). -

This case cor-

responds

to an excitation

by

the laser lines 5 017

Å

and 5 208

A.

The values of the

product

gj i obtained

by extrapolation

of the width of the Hanle curves to

zero vapour pressure are also

presented

in table I.

2.3 .2.1 Excitation at 5 017

Á.

- One rotational level J’ =

27,

v’ = 62 is

mainly

excited. The

product

(5)

238

gi i is

large.

The

extrapolation

of the line width of the curves to zero vapour pressure is very difficult since it is very sensitive

[15]

to small

quantities

of

gaseous

impurities

in our cells. This is due to the

high

value of the lifetime r.

2.3.2.2 Excitation at 5 208

À.

- One rotational level J’ =

77,

v’ = 40 is

mainly

excited. The

product

^

gj,r is much weaker and there is no

problem

for

extrapolation

to zéro vapour pressure.

Figure

3 shows the Hanle effect curves recorded for the laser line 5 208

Á.

Of course

they

are lorentzian

and one can notice that the

dispersion

and

absorption

curves have about the same

amplitude

and the same

width.

FIG. 3. - Hanle effect curves for the excitation at 5 208 Á. The

points correspond to the best fit of lorentzian curves. The 12 pressure

was 3 mtorr.

2. 3. 3 Particular case

of

the excitation at 6 328

Â.

-

The excited level is v’ = 6 J’ = 32. The

interpretation

of the Hanle effect is very difficult in this case since the various

hyperfine

sublevels are not

equally

excited

by

the

laser,

the laser line

being only

coïncident

with the

wing

of the

absorption

line of

I2.

Furthermore the

magnetic predissociation

is so

important [16]

that is

strongly

modifies the

shape

of the Hanle curves.

However

preliminary experiments

and calculations show that : - 0.04 g J 0.

The whole set of results for lifetimes shown in table 1 are in

good agreement

with those obtained

independently by

J. A. Paisner and R. Wallenstein

[17]

by

the

decay

method.

On table 1 we also

give

the values of

0’(2), the

cross section for destruction of the

alignment. 0’(2)

is

deduced from

the slope

of the curve AH=

f ( p)

FIG. 4. - dHD is the distance of the two maxima of the dispersion

Hanle curves. p is the 12 pressure. Laser line 5 145 Á.

where AH is the width of the Hanle curves

and p

the

12

pressure.

Figure

4 shows such a curve for an

excitation at 5 145

Á.

Apart

from the levels v’ = 32 J’ = 14 and 9 excited at 5 309

Á,

the

depolarisation

of the fluores-

cence as a function of the

12

pressure is

generally

very weak and

(1(2)

is not very different from

(1(0)

the cross section for destruction of the

population (quenching

cross

section).

3. Resonances in modulated

light.

- This

technique permits

us to measure

directly

the Landé factors g eF of the various

hyperfine

sublevels. The

principle

of this

experiment

is the

following :

the laser

light

is

modulated at a fixed

frequency

m and the modulation of the fluorescence

light

is detected at the same

frequency

co. If the

magnetic

field is

swept,

resonances

are observed when hm is

equal

to the

splitting

between

two Zeeman sublevels of the excited states. The exci- tation and the detection must be coherent. This condition is obtained

using

linear 6

polarisation

both

for excitation and detection. Therefore at resonance,

we induce coherence between Zeeman sublevels such

as Am = + 2.

The

experimental

set up is very

simple.

The laser

light

is modulated at 800 kHz

by

a Pockels cell or an

electro-optic

modulator. The modulation of the fluo-

rescence is monitored

by

a

photomultiplier

and

by

a brookdeal lock-in

amplifier.

This

experiment

was

performed

on the levels

excited

by

the laser lines 5 017

Á

and 5 208

À.

3.1 EXCITATION AT 5 017

A. - Figure

5 shows

the

spectrum

of resonances

corresponding

to the 15

hyperfine

sublevels of the para state v’ = 62 J’ =

27.

(6)

FIG. 5. - Resonances in modulated light for the laser line 5 017 À.

The same resonances are obtained with the direction of the

magnetic

field reversed.

The

position

of the central resonance

gives

g J = - 1.8 ± 0.2. The

dispersion (or scattering)

of

resonances

gives (gl

+

gl).

We

obtain gi

= 3.4 ± 0.5.

Figure

5 shows the theoretical

position

of the reso-

nances calculated for these values

of gl

and gj.

The agreement

is

very good.

In fact one resonance is not

explained by

this

theory.

However it is known

[19]

that the laser line 5 017

A

also

significantly (10 to

20

%)

excites another level

(v’

= 71

± 2

J = 55 ±

2)

of the B state. Most

probably

this resonance corres-

ponds

to the level v’ = 71.

Thé

value of g J deduced from the

position

of

this

resonance would be

gj _ - 5.2 ±

0.8,

in

good agreement

with the inter-

pretation of 9J developed

in the last

part

of this paper.

The lifetime of the v’ = 62 J’ = 27

level

is deduced from the,

product

gi T

given previously.

We find

1 = 14 ± 3 J.1s. This result was confirmed

by

a direct

measurement of the

exponential decay [18]

of the

fluorescence

following

a

pulsed

excitation.

These values

of g J

and i for the level v’ = 62 J’ = 27

are in

disagrqement

with those

reported by

Paisner

and Wallenstein.

They

find gj = - 2.6 andr = 8.8 J.1s.

We believe that in the present case of a very

compli-

cated

spectrum

of 15 resonances the

technique

of

of resonances in a modulated

light

beam is more

accurate than the

quantum

beats method that

they

used.

Indeed,

Paisner and Wallenstein observed an almost unresolved

quantum

beat

signal

that

they

had to fit with a theoretical curve

involving

two

parameters gl

and gj. In our

experiment

we can

observe well resolved resonances from which it is

extremely

easy to determine the values of these two

parameters and even to check the theoretical expres- sions used for the Landé factors.

Furthermore,

the lifetime is difficult to obtain with

precision

because it

is very

long

and very sensitive to gaseous

impurities

in the cells. Therefore we have confidence in our

results.

3.2 EXCITATION AT 5 208

Â.

-

Figure

6 shows

the resonances obtained in this case. The width of each resonance

being

too

large

it is not

possible

to

Fm. 6. - Resonances in modulated light for the laser line 5 208 A.

measure gl. We. can

only

deduce gj = - 0.32 ± 0.04 in

agreement

with the results of Paisner and Wallenstein who find g J = - 0.28.

4.

Interprétation

of the

experimental

results. -

4.1 SECOND ORDER PERTURBATION THEORY. - The gj factor of molecules without electronic

angular

momentum

(Q

=

0)

is

generally interpreted

in terms

of second order

perturbation theory [11].

The

perturbation

hamiltonian can be written :

where

L and S are the electronic

angular

momenta,

J = L + S. 1 =

Il

+

12

is the total nuclear

spin.

re is the

position

of the electron.

V,

is the off

diagonal

part of the rotational

hamiltonian, V2

is the Zeeman

hamiltonian, V3

is the

magnetic hyperfine

hamiltonian.

A molecular

eigen

state may be

written : 1 rQva >

where T and S2 are characteristic of the electronic state. v is the vibrational

quantum number,

a represents

(8JF MF).

For the

perturbated state 1 r’,

Q =

0, v’,

a’

>,

the

second order

perturbation

term is :

The summation over v becomes an

integral

when

the

perturbing

electronic states form a continuum.

The cross

perturbation

term

(7)

240

gives CI,

the constant of the

magnetic hyperfine

struc-

ture term

(C, I.J). CI

has been measured for several levels

by

Levenson and Schawlow

[8].

The cross term

gives

g J.

The cross term

gives gl.

These constants are

independent

of

J, they depend only

on

v’,

the vibrational quantum number of the

perturbed

level.

Suppose

that we assume that :

Then,

for each term,

expression (1)

has a factor :

and the various constants gl, g J

and CI

are propor-

tional to each other.

Indeed this

approximation

is rather

rough,

but it

is useful to comparç the measurements of gj and

CI,

and to

estimate gl

for the levels

where gl

is not mea-

sured.

For

instance,

it would

give :

The value

of gl

estimated

by

this way for the level

(27, 62)

excited

by

5 017

A

is g, = 3 in

good agreement

with our

experimental

result.

For the other

levels,

the estimated values

of gl

have been

reported

in table 1.

4.2 VARIATION

OF g J

wm v’. - This variation is very similar to that

of CI

with

v’,

observed

by

Leven-

son and Schawlow

[8].

The authors have

given

the formula :

which

they

both derived

theoretically

and verified

experimentally.

E is the energy of the studied level in the

potential

curve of the B state.

Ec is

an

adjustable

parameter.

It is

possible

to

verify experimentally

that such a

law is also valid for g J. We find :

where

Ec

and E are taken in cm-1.

Ec

= 4 360

cm-1

in

good

agreement with the value of reference

[8] Ec

= 4 340 ± 40

cm-1.

Also Paisner and Wallenstein have

reported Ec=4 391 ± 40

cm -1.

Figure

7 shows our

expérimental

values for g J

plotted against

the theoretical curve obtained from eq.

(2).

The

reported

values for

Ec

are very close to

Do

the dissociation energy of the B state. This fact seems to prove, as was

already

noticed

by Levenson,

that the

perturbing

state

(or states)

is a dissociative state with the same

asymptote

as the B state.

FIG. 7. - gj as a fonction of vibrational energy.

5. Conclusion. - In this paper we have

reported

a set for measured values

for g J,

gl and 1 in the B3

II Q

u

state of iodine.

Although

these results seem in

good agreement

with an

oversimplified

theoretical inter-

pretation, they

should be considered as

preliminary

to a more

complete analysis.

We are in the process of

measuring

a series of such

parameters

over a

great

number of vibrational and rotational levels of the B electronic state. We use for this purpose several

types

of

dye

lasers. A careful

analysis

of

these

data will then

permit

us to

give

a more detailed theoretical

interpretation. Especially interesting

will be the para-

meters measured for levels very close to the dissocia- tion limit for which the Landé factors become very

high.

Also

interesting

will be the results obtained for low vibrational levels for which the Landé factors

are very small and become sensitive to first order per- turbation terms

giving

rise to a

small,

pure rota-

tional,

Landé factor.

(8)

References [1] WOOD and RIBAUD, Phil. Mag. 27 (1914) 1009.

[2] SERBER, Phys. Rev. 41 (1932) 489.

[3] CAROLL, T., Phys. Rev. 52 (1937) 822.

[4] BROYER and LEHMANN, Phys. Lett. 40A (1972) 43.

[5] WALLENSTEIN, R., PAISNER, J. A. and SCHAWLOW, A. L., Phys. Rev. Lett. 32 (1974) 1033.

[6] MCCLINTOCK, M., DEMTRÖDER, W. and ZARE, R. N., J. Chem.

Phys. 51 (1969) 5509 ;

MARECHAL, M. A., JOURDAN, A., NEDELEC, O. and PEBAY PEYROULA, J. C., C. R. Hebd. Séan. Acad. Sci. 268 (1969)

1428.

[7] CORNEY, A. and SERIES, G. W., Proc. Phys. Soc. 83 (1964)

207.

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