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Collisionally induced optical double resonance in I2 : rotational analysis of the D'(2g) - A'(2u) laser transition

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Submitted on 1 Jan 1982

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Collisionally induced optical double resonance in I2 : rotational analysis of the D’(2g) - A’(2u) laser transition

J.B. Koffend, A.M. Sibai, R. Bacis

To cite this version:

J.B. Koffend, A.M. Sibai, R. Bacis. Collisionally induced optical double resonance in I2 : rotational analysis of the D’(2g) - A’(2u) laser transition. Journal de Physique, 1982, 43 (11), pp.1639-1651.

�10.1051/jphys:0198200430110163900�. �jpa-00209545�

(2)

Collisionally induced optical double

resonance

in I2 :

rotational analysis of the D’(2g) - A’(2u) laser transition

J. B. Koffend, A. M. Sibai and R. Bacis

Université Claude-Bernard (Lyon I), Laboratoire de Spectrométrie lonique et Moléculaire, 43, boulevard du 11 Novembre 1918, 69622 Villeurbanne, France

(Reçu le 9 juin 1982, accepté le 27 juillet 1982)

Résumé. - La transition D’(2g)-A’(2u) de la molécule I2 a été excitée par double résonance optique induite par collisions. Une analyse rotationnelle correspondant à plus de 50 niveaux vibrationnels de l’état A’(2u) a été effec-

tuée. On a étudié le comportement de l’état A’ à longue distance internucléaire. L’énergie de dissociation de cet état a été déterminée : De = 2 505,7 ± 1,9 cm-1. On a montré que l’état D’ est l’état 03B1 de King et al. (Chem.

Phys. 56 (1981)

145).

Les énergies de D’ et A’ relatives à l’état fondamental X

1~g+(03BD

= 0, J = 0) ont été déter-

minées comme étant T0 = 40 331,6 ± 1,6 cm-1 et T0 = 9 988,7 ± 1,6 cm-1 respectivement. On discute le mécanisme de la double résonance. Un transfert collisionnel de grande efficacité vers l’état D’ a été observé, ce qui permet de mieux comprendre le fonctionnement du laser à iode D’-A’ pompé optiquement.

Abstract. - The I2 D’(2g)-A’(2u) transition has been excited by collisionally induced optical double resonance.

This system has been rotationally analysed for more than 50 vibrational levels of the A’(2u) state. The long range behaviour of the A’ state has been studied. The dissociation energy of this state has been determined to be

Dc = 2 505.7 ± 1.9 cm-1.

The D’ state has been identifed with the 03B1 state of King et al. (Chem. Phys. 56 (1981) 145). The energies of the D’

and A’ states have been determined relative to X

1~g+(03BD

= 0, J = 0) to be T0 = 40 331.6 ± 1.6 cm-1 and

To = 9 988.7 ± 1.6 cm-1,

respectively. The mechanism of this double resonance is discussed. Efficient collisional transfer to the D’ state is observed and helps to shed some light on the operation of the optically pumped I2 D’-A’ laser.

Classification

Physics Abstracts

33.50 - 33.20L

1. Introduction. - The 340 nm transition in

I2

was

suggested

as a

possible interesting

U-V laser

by

McCusker and coworkers [1] ] and laser action was

originally

obtained using electron beam excitation

[2-4].

The

efficiency

of the system was found however to be rather low and interest in it

quickly

diminished.

This transition has also been

optically pumped

in

the presence of buffer gases,

using light

from

exploding

wires

[5].

The

efficiency

of this system however has also

proved

to be low. But Zuev et al.

[6], pumping

with a conventional quartz

lamp,

obtained

pulsed operation

with an output energy of 10-50 mJ per

pulse. Recently,

laser action was obtained using

optical

excitation with an ArF laser at 193 nm

[7]

with

surprising

intrinsic energy conversion

efficiency

of

approximately

30

%, equivalent

to a

photon

effi-

ciency

greater than 50

%.

Despite

a number of studies of

I2

emission in the visible and UV range

[1, 8-14],

little is known about the collisional transfer involved in this U-V laser.

A

spectroscopic study

of this transition was

performed by Tellinghuisen [ 11 ],

who attributed it to the

12 D(3 172g)>, A’(3 n 2u) (1)

system and gave an

isotopic

vibrational

analysis.

However, he could not locate the absolute

energies

of those two states. A more complete

analysis

will

be

published by Tellinghuisen [11&].

The lower level of this transition is also of interest in

regard

to the C.W. chemical atomic iodine laser

[ 15].

(1) As 12 is a case c molecule the transition will be noted

D’(2g)-A’(2u).

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:0198200430110163900

(3)

The laser action is achieved on the

lPl/2-lP3/2

tran-

sition of the iodine atom

by

energy transfer from the

1 d g

or

1 Eg

metastable states of

02

to

I2

molecules

which results in

I2

dissociation.

Among

the various transfer schemes, the A’(2u) state seems to

play

an

important

role

(see

Ref.

[16]

and references

therein).

In order to elucidate this

point

the absolute energy of this state must be determined.

In order to

study

these different

questions

we have

undertaken a rotational

analysis

of this transition.

A priori, this seems to be a difficult

’problem.

The

D’(2g)

state cannot be excited

directly

from the

ground

state or other accessible known states which

precludes

an absolute energy measurement. More- over, the

D’(2g)-A’(2u)

transition has

always

been

excited

through

collisional transfer and the

typical

pressure of inert gas

(a

few hundred

torr)

will broaden the lines and

complicate

a

high

resolution

analysis.

In this report, we present a

study

of the

I2 D’(2g)- A’(2u)

fluorescence excited

by collisionally

induced

double resonance. We have

performed

a rotational

analysis

of this system. The observation of

high

vibrational levels of the

A’(2u)

state allows the deter- mination of its dissociation energy. Since the

A’(2u)

state shares the same dissociation limit as the

X(l E 9 ’)

state, the absolute

energies

of the D’ and A’ states have been measured. This allows

important

conclu-

sions to be made with respect to the 342 nm laser action and shows that the 2u state cannot be excited

directly

from

O2(1 Ag).

2. Experiment - In the work of Shaw et al.

[7],

the

D’(2g)-A’(2u)

stimulated emission was obtained after ArF 193 nm

pulsed

excitation. The ArF laser excites the

D(O:)

state from the

X(ll:’g+) ground

state

(see Fig. 1).

The inert buffer gas causes transfer to the

D’(2g)

state which results in D’-A’ laser oscil- lation.

In order to make a rotational

analysis

of the spontaneous emission of the laser transition, the

excitation

by

a continuous wave laser is

preferable.

As the direct excitation of the D state is

impossible

with

existing

C.W. lasers, we have

attempted

to

excite the D’-A’ transition

through

double resonance.

The

E(Og )

state can be excited with two C.W. lasers via the

B(O’)

state

(Fig. 1).

We have observed that very efficient

E(O’)-D’(2g)

collisional transfer can be

obtained, which a priori should

permit

a spectros-

copic analysis

of the

D’(2g)-A’(2u)

transition.

A schematic

diagram

of the

experimental

appa-

ratus is shown in

figure

2. The beams of a

Spectra Physics

model 171 Ar + laser and a

Spectra Physics

model 171 Kr’ laser were

superimposed using

a

dichroic mirror and then focussed with an

f =10

cm

lens into an

I2

cell. The

resulting I2

fluorescence

was observed with a 0.20 meter spectrometer

(Jobin

Yvon model

H-20) equipped

with an RCA 1 P28

photomultiplier

tube.

Higher

resolution studies were

performed by focussing

the forward-scattered fluo-

rescence from the

I2

cell onto the slits of a 3.4 meter

Fig. 1. - Low-lying valence and charge transfer states of 12.

Potential energy curves for the

D(O:)

and

F(O:)

states are

estimated while others shown are RKR curves. Also shown

are the 193 nm pump and 340 nm laser transitions [7].

Atomic dissociation products and molecular states which

correlate to these limits are displayed on the right.

spectrograph

equipped with a 1 200 lines/mm

grating

blazed at 1 300 nm. Filters were

placed

in front of each laser to isolate the laser lines and eliminate any interference from

plasma

lines from the

discharge.

Appropriate

band pass filters, inserted

just

after the

I2

cell were used to isdlate

particular spectral regions.

Kodak SWR film was used for U-V spectra while Kodak Tri-X was used for visible studies.

Typical

exposure times were six hours for the observation of faint lines, but the more intense U-V lines could be

photographed

with exposure of the order of an

Fig. 2. - Schematic diagram of the experimental set-up.

(4)

hour or less. Fe lines from an iron arc were used for

wavelength

calibration. The accuracy of the measu- rements is of the order of 0.05 cm - 1. The

I2

cells

were evacuated to pressures below 10-’ torr with a

liquid N2

cooled cryopump. Reagent

grade I2,

sub-

jected

to several

freeze-pump-thaw cycles,

was intro-

duced into the cells

by

distillation onto a

liquid N2

cooled

point

in the cell.

Argon

could be added to the cells and the argon pressure was determined

using

a Pirani type gauge. In some

experiments,

to

study

the

D’(2g)

excitation mechanism, the Ar+

laser was

replaced by

a

Spectra Physics

model 380-D

ring dye

laser

operating

with Rhodamine 6-G.

3.

Experimental

results. - In

preliminary experi-

ments,

12 X(lEg )-B(Ou )

transition was excited

using

the 514.5 nm Ar + line which is known to be in reso- nance with a few lines of the B-X system

[17].

We

tried to effect the second excitation step with the U-V or violet lines of a Kr+ laser in order to excite the

E(O:)

state as

high

as

possible. Using

the 406.7 nm line, strong

E(O:)-B(O:)

fluorescence was observed

indicating

an E-B-X double resonance. It was found that upon addition of argon to the

I2

cell a new system,

peaked

at 340 nm,

appeared. Figure

3 shows

several low resolution spectra near 320-340 nm taken with different argon pressures. As

already

seen in

the spontaneous emission of the

D’(2g)-A’(2u)

tran-

sition

[7],

the increase of argon pressure

strongly

favours emission at 340 nm. We observed the same

behaviour

giving

us confidence that collisional transfer from the

E(O:)

state leads to the

preferential

popu- lation of the

D’(2g)

state as was the case with the

D(O:)

state in reference

[7].

The

peak appearing

at

325 nm

(Fig. 3)

is due to the

D(0")-X(lEg )

transi-

tion. Thus a small part of the collisional transfer from

E(O:)

results in the

population

of the

D(Ou)

state.

High

resolution spectra of

I2

with 2 torr argon

excited

by

the 514.5 nm and 406.7 nm laser lines

were recorded in the range 315-345 nm and in the

region

of

expected E(O:)-B(O:)

fluorescence (408-

435 nm). Several

E(O:)-B(O;)

transitions were assi-

gned, indicating

that the

E(O’)

state was involved.

However, even at a

reciprocal dispersion

of

0.04 nm/mm, the 330-345 nm U-V spectrum appear- ed continuous with few discrete features

barely

visible in the continuum

background.

The excita- tion of

high

vibrational levels of the

D’(2g)

state

mainly give

emission to the continuum of the A’(2u)

state. An

interesting

result from these spectra is that the E state can be

easily

excited

through

collisional double resonance excitation. An

example

is shown in

figure

4.

Argon-I2

collisions transfer

population

to

a

large

number of B states levels near the

initially

excited levels. Thus, numerous B state rovibrational levels are

populated

and since the

density

of E-B

lines is very

high (higher

than in the B-X

system)

there is a

high probability

that any discrete laser line with sufficient energy will excite some rovibra- tional level of the E state.

If the 454.5, 457.9, 465.8, 472.7 and 476.5 lines of

an Ar + laser were used for the second excitation step in

conjunction

with either the 514.5

nm Ar+,

520.8

or 530.9 nm Kr+ lines

(first step),

a discrete spectrum

was observed in the D’-A’

region

with Ar buffer gas.

That collisional

population

of many B state levels

occurs is confirmed

by

the observation of the same

D’-A’ spectra when either 514.5, 520.8, or 530.2 nm

are used as the first step.

We have also noted that if care is not taken in

preparing

the

I2

cells, D’-A’ spectra are obtained,

even in the absence of Ar. This may be due to traces of water in the

I2

which will be condensed as well onto the

liquid

nitrogen cooled

point

in the cells.

Fig. 3. - Spectra of 12 excited with 200 mW 406.7 nm and 1 500 mW 514.5 nm.

QO.3

torr 12 + 100 torr Ar;

Q)0.3

torr

12 + 12 torr Ar;

(3) 0.3

torr 12 + 1 torr Ar;

(4)0.3

torr 12.

(5)

Fig. 4. - Energy level diagram showing observed example

of

E(O+) -->

D’(2g) collisional transfer.

Thus, the cross section for E-D’ transfer may be

large

for collisions of excited

I2

with

H20. Figure

5

shows a low resolution spectrum of the

D’(2g)-A’(2u)

fluorescence obtained with 530.9 nm Kr+ line as a

first step and various Ar+ lines as a second step.

Some fluorescence lines of the D-X transition were

observed in the 320-325 nm range with 454.5 nm and 457.9 nm as seen in

figure

5. No spectra of either the D’-A’ or the D-X transitions were obtained

using

Ar + lines with

wavelengths

greater than 476.5 nm.

4. Analysis of the data. - The

spectroscopic

ana-

lysis

of the fluorescence lines was

complicated by

the

superposition

of numerous fluorescence series,

large

Franck-Condon gaps in

(V2g, V2.)

series, and

overlapping

of the D-X transition in the 320-330 nm

range. Furthermore, for the most intense series no

rotational relaxation lines were observed. Hence the series appear as groups of two lines

(P

and

R)

for every v2u level. That no Q lines were detected

eliminates a Af2 :0 0 transition

(in particular 1 g-2u).

Among

the numerous series observed about 15 of the more intense were selected for the measurements.

The observed line

positions

were least squares fitted to the

expression :

where v is the transition

frequency, G(v)

is the rota-

tionless energy for v’ or v", X =

J ( J

+

1),

and B, D, H and L are the usual rotational constants. Since few lines for each vibrational band

(v’, v")

were mea- sured, the distortion constants for the 2u state were

fixed at calculated values in the fit. Thus, an iterative

fitting procedure

was used. First, the distortion

constants were set to zero and the

resulting G(v")

and

B(v")

obtained from the fit were used to construct an RKR curve for the 2u state. Then the distortion constants were calculated from the RKR

potential using

a program

by

Hutson

[19, 20].

These values

were used in a second fit and the

procedure

was

repeated

until no

significant change

in the successive fits was observed. The results for the 2u state are

presented

in table I a. These constants result from

a

weighted

fit of 720 lines and the RMS error of the fit is 0.07 cm - 1. Table I b

displays

coefficients for the

polynomial expansions

of these constants in

- Fig. 5. - Spectra of 12 emission when excited by 530.9 nm

and 454.5, 457.9, 465.8, 472.7, or 476.5 nm laser lines. Spectra

were obtained with 0.3 torr I2. Arrows show

emission observed using 454.4 and 457.9 nm as the second step.

(6)

Table I a. - A’(2u) spectroscopic constants.

e) All constants given in cm - 1. 2 a estimates in parentheses. Constants for v = 0, 1 extrapolated from data.

(b) Calculated (see text).

(7)

Table I a

(continued).

- A’(2u) spectroscopic constants.

Table I b. -

A’(2u)

expansion parameters valid

for

v = 0-59.

(a) Expansion of the form :

G(v) = £

Yio(v +

2)‘.

t=i 1

(b) Expansion of the form :

B(v) = L

Yil (v +

i)‘.

i=O

(C) Expansion of the form : In

(F(v)) = Y

Ki(v +

t)i,

where F(v) = D(v), - H(v), or - L(v).

i=o

Table II. -

D(OU )

parameters.

(a) Values of the parameters obtained from 5 fluorescence series G(v + 4) has been obtained using B(v + 4) estimated

0.020 6 cm-1. Values given are in cm-1.

powers of v + 1/2. The J’ values

ranged

from 14-120 for v" = 2 - 12, from 36-90 for v" = 19-39, and from 36-40 for v" = 40-59.

In some cases, there was

enough

information to fit

D(v")

for some 2u levels. The fitted values of

D(v")

are

generally

in agreement with those calculated from the RKR

(see

table

II).

However, in a few cases

the agreement is

questionable.

This is

probably

due

to the fact that few lines of

high

J" were measured

for these A’ vibrational levels.

In order to understand the emission in the

region

320-330 nm a few

D(O +)-X(’Z +)

fluorescence series

were

analysed.

The results are

given

in table II for

the

D(O:)

parameters determined. The

X(E 9 ’)

vibra-

tional levels cover the range v = 53-63 for the most intense lines.

5. Near-dissociation behaviour of the A’(2u) state.

- As no

perturbations

were observed in the spectra, the

only

way of

fixing

the absolute energy of the

A’(2u)

state with respect to the

ground

state is

by extrapola-

tion of the

positions

of the

higher

vibrational levels to the dissociation limit. Le

Roy’s theory [21-22]

is

particularly

well suited for this

extrapolation.

From

the relative values of the

energies G(v")

of the

A’(2u)

vibrational levels, this

theory

allows a

precise

extra-

polation

to the dissociation limit. Since the

A’(2u)

state has the same dissociation limit as the

X( 1 E g+ )

state, its value is

precisely

known. It has been deter-

mined

directly

from Fourier Transform

Spectros-

copy measurements

[23]

to be 12 440.083 ± 0.145 cm - ’

(with

respect to

X(1 E g+)

v = 0, J =

0).

This value is in excellent agreement with the indirect determination

Do

= 12 440.086 ± 0.023

cm-1,

taken from the dissociation limit of the iodine

B(O:)

state

(20 043.063 ± 0.020

cm -1 )

[24] and the atomic

I 2 P 1 J2-

2P3/2

energy

separation

(7 602.977 ± 0.003

cm-1) [25].

(8)

An

example

of this

extrapolation procedure

can

be found in reference

[23].

The interaction

potential

of the two atoms in the

long-range region

is

approxi-

mated

by :

where

Do

is the dissociation limit, R is the inter- nuclear distance,

C,,

is a constant, and n is some

weighted

average (in

general non-integer)

of the

powers of the

locally important

terms.

The energy G(v) of the vibrational levels may then be

expressed

as [21, 22,

26]

where VD is the effective vibrational index at the disso- ciation limit and

Xo(n)

is

given by :

where T is the gamma function

and p

is the reduced

mass.

The observed values of G(v) were least squares

Fig. 6. - 12 A’(2u) long- range parameters obtained from least squares fits to equation (3). The abcissa displays the

range of vibrational levels included in the different fits.

fitted to equation (3) for the

highest v"

levels measured

to obtain the parameters n, vD,

C.,

and

G(vD). Figure

6

shows the results from several fits where the number of v" levels used is varied from v" = 42-59 to v" = 54-59.

This

procedure

allows us to fix the absolute

positions

of the

D’(2g)

and A’(2u) states relative to v = 0, J = 0 of the

X 1 Eg+

state with a

precision

of 1.6 cm -1.

At

long

range the interaction

potential

is

expected

to be of the form

Values of

and

have been calculated from iodine atom

properties

[27, 28]. When one compares the theoretical value of

CS

calculated

by

Saute and Frecon

[27]

for the

I2 B(Ou )

state, 3.59 x 105 AS

cm-1,

with the

experimental

value of

Danyluk

and

King [24], 2.89

x 105 AS

cm-1,

the theoretical value is a factor of 1.2 times

larger.

Since the atomic contribution to

CS

is identical for

all

I2

valence states, a more reasonable value for

C.

for the

A’(2u)

state is

C5 -

1.68 x 105 A5 cm-1.

The order of

magnitude

of the

respective

contribution of

C5, C6

and

C8

in the 6.5 A-7 A range for

A’(2u)

are

shown in table IV.

C8

was

roughly

estimated from

C6 using

the

C8lC6

= 15.3 A2 ratio determined in

[24].

Displayed

in table III are the constants

Cn,

n, vD, and

G(VD)

deduced from the fits to

equation

(3)

along

with

Te

and

De.

The results are a

weighted

mean of

the fits with v"

spanning

50-59, 51-59, 52-59, and 54-59.

The values obtained for n and

Cn

are in reasonable agreement with the data

presented

in table IV, i.e.

the dominant contribution to the

binding

energy is due to

C6

in the 6.5-7 A range.

To test the

previous analysis,

the values of G(v)

from the

experiment

with their correct absolute ener-

Table III. - Long-range parameters

of

the

A’(2u)

state.

Estimated errors are two standard deviations. For definition of parameters see text.

(a) Experimental data adjusted to give known value of

G(v,) (see text).

(’) Te is defined as the energy difference between the minima of the A’(2u) and

X(lEg )

potential energy curves.

The

X( 1 Eg )

(v = 0, J = 0) level lies 107.107 cm -1 above the minimum of the

X(lEg )

curve [38].

(9)

Table IV. - Contribution to binding energy

of long-range

potential parameters

for

the A’(2u) state.

(a) From references [24] and [28] (see text).

(b) From reference [28].

(C) The value of C8 is only roughly estimated from reference [24] as explained in the text. However the deduced contri-

butions are in agreement with the remaining binding energy determined from the RKR outer turning points when the cal- culated Cs and C6 contributions are subtracted.

gies

with respect to v = 0, J = 0 of the

X(ll’g+)

state

were fitted to the

expression :

where AG(v) = G(v + 1) -

G(v)

and

K 5

is a cons-

tant which

depends only

upon the value of

C5

and the

reduced mass.

Equation

(6) results from the

theory

of Le Roy [21,

22]

when the

leading

term of the inter- atomic

potential

at

long

range is n = 5, as is the case for the A’(2u) state of

I2.

The

plot

is shown in

figure

7.

The value

of Do

= 12 440.8 ± 4.0 cm-1 is in agree- ment with that

displayed

in table III. The value of

C s

Fig. 7. - Fit of experimental data to equation (6). Error

bars denote two standard deviations.

determined from this fit, (3.9 ±

1. 0) - 10’ A’ cm - ,

is too

large, probably

since in the range of R

sampled C.

is

really

closer to

C6,

because in

equation

(2) n - 6 (see Tables III and IV). However, the

experimental

vibrational

energies,

as is often the case

[39], obey

the

limiting

near-dissociation

equations

even when the

leading

term (here

CS/R 5)

is

responsible

for

only

a

fraction of the

binding

energy. We have also tested the results of table III in an

extrapolation procedure

of the A’ RKR curve which is discussed in the next section.

6. RKR curves. - The positions of the D’ and A’

states have been fixed relative to v = 0, J = 0 of the

X( 1 E g+ )

state from the

long

range

analysis

of the A’

state. Table V shows a

comparison

of constants for

the D’ state obtained

along

with the constants for the

a-state in the work of

King et

al.

[ 18].

We have decreas- ed the vibrational

numbering

of reference

[ 18] by

seven.

This has been

suggested by Tellinghuisen [llb]

and

in our case this was necessary to reach agreement between Franck-Condon factors calculated from RKR

curves and our observed

D’(2g)-A’(2u)

fluorescence intensities. The agreement between the values of G(v)

for the D’ state seen in table V is of the order of 0.3

cm -1,

which suggests that our estimated 2 a error in the

positions

of the D’ and A’ states (1.6

cm -1 )

is

probably

too

large.

We used the data of reference

[18]

with the new

vibrational

numbering

for the a-state to construct

Table V. -

D’(2g)

spectroscopic constants.

All G(v) relative to X

1 Eg (v

= 0, J = 0).

(a) This work (2 Q estimates in parentheses).

(b) Reference [18] observed.

0 Reference [18] calculated (Te + we(v +

t) -

We xe(v +

t)2).

(d) Reference [18] calculated (Be - ae(v

+’t)).

(10)

Table VI b. -

D’(2g)

state constants.

Constants determined from data of reference [18] with

v numbering decreased by seven (levels used were v = 1-14).

an RKR curve for the

D’(2g)

state. Table VIa

(2)

presents the RKR curve and table VIb

displays

the

molecular constants for the D’ state. It should be men- tioned that the

D’(2g)

RKR

potential

had to be shifted

by -

0.030 A so that calculated intensities agree with our observed 2g-2u fluorescence intensities.

This shift is

compatible

with the

poorly

defined values of B(v) in reference

[18]

(see for instance Table V).

The RKR curve for the A’(2u) state is

reported

in

table VIIa

(2). Equilibrium

constants are

presented

in table VIIb. There is excellent agreement with the RKR curve

given by Tellinghuisen [ 11 bJ

and the

observed D’-A’

intensity

distribution is

reproduced

Table VII b. - A’(2u)

equilibrium

constants.

Estimated errors are two standard deviations.

(2) Tables VIa and VIIa are too lengthy to be published here, but they may be obtained on request to Les Editions de Physique or the authors.

when Franck-Condon factors are determined. As a

second check of the consistency of our

long-range

treatment of the A’ state, the outer turning

points

were

extrapolated

using equation (5) for R > 9 A

(the C8

term is

negligible

in that

range).

The program of Hutson

[20]

was then used to calculate the molecular constants for all bound levels of the A’ state. Two

extrapolations

were

performed,

one

using

the value

of

Cs

from the work of Saute and Frecon

[27,

28]

and the other

using Cs

= 1.68 x 10S AS

cm-’,

which

we consider to be the better value. In both cases, the value of

C6

from reference

[28]

was used. Table VIII presents these results. The constants for the last two bound levels (v = 68, 69) were not found

by

Hutson’s

program and were determined

by extrapolation using

the

long-range

theory of Le Roy. The

energies

of the

levels v = 60-67 were fitted to the

expression :

Table IX. -

D’(2g)-A’(2u)

Franck-Condon

factors.

2 6 estimates in parentheses.

(") Frequencies given are for band origins.

Table VIII. - A’(2u) molecular constants at large internuclear distance.

e) This work (2 6 estimates in parentheses).

105 106 6 CM-1

(b) Calculated from RKR curve having CS = 2.09 x 105 AS cm-1 and C6 = 1.95 x 106 A6 cm-1 (see text).

(C) Calculated from RKR curve having Cs = 1.68 x 105 AS cm-’ and C6 = 1.95 x 106 A6 cm-1 (see text).

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