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The vibration-rotation bands v2 and v5 of methyl bromide

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The vibration-rotation bands v2 and v5 of methyl bromide

G. Graner, W.E. Blass

To cite this version:

G. Graner, W.E. Blass. The vibration-rotation bands v2 and v5 of methyl bromide. Journal de

Physique, 1975, 36 (9), pp.769-771. �10.1051/jphys:01975003609076900�. �jpa-00208314�

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769

THE VIBRATION-ROTATION BANDS v2 AND v5 OF METHYL BROMIDE

G. GRANER

Laboratoire

d’Infrarouge,

Laboratoire Associé au

CNRS,

Université Paris

XI,

Bâtiment

350,

91405

Orsay,

France

and W. E. BLASS

Molecular

Spectroscopy Laboratory, Department

of

Physics

and

Astronomy,

The

University

of

Tennessee, Knoxville,

Tennessee

37916,

U.S.A.

(Reçu

le

20 février 1975, accepté

le 4 avril

1975)

Résumé. 2014 Le spectre infrarouge de

CH3Br

a été analysé entre 1 200 et 1 500 cm-1 en tenant compte de la résonance de Coriolis en x- y entre les deux niveaux

fondamentaux v2

= 1 et 03C55 = 1.

Les centres de bande ont été trouvés

respectivement

à 1 305,907 et 1 442,885 cm-1 et le terme de

couplage 03B6x2,5

vaut 0,617.

Abstract. 2014 The infrared spectrum of

CH3Br

has been analyzed between 1 200 and 1 500 cm-1 taking into account the x - y Coriolis resonance between the two fundamental levels 03C52 = 1 and 03C55 = 1. The band centers were found

respectively

at 1 305.907 and 1 442.885 cm-1 and the

03B6x2,5 coupling

term was determined to be 0.617.

LE JOURNAL DE PHYSIQUE TOME 36, SEPTEMBRE 1975, 1

Classification Physics Abstracts

5.444

1. Introduction. - The infrared spectrum of

CH3Br

between 1200-1500

cm-1

has not so far been studied under a

high

resolution. In

1965,

Morino and Naka-

mura

[1] reported

a

study

of the

perpendicular

fun-

damental v-, with

only

the unresolved

Q-branch positions being

measured. In

1966, Jones, Popplewell

and

Thompson [2] reanalyzed

the same band with

a somewhat

higher

resolution and

assigned

about

one hundred ’P and RR lines.

They

also

reported

a

study

of the

parallel fundamental v2

without

being

able to resolve any of the K structure,

fitting

the

P(J)

and

R(J)

lines to a

polynomial

in m.

In

1969,

Kurlat

[3]

recorded

the V2

and vs

region

with

higher resolving

power at the Ohio State Univer-

sity, using

a

path

of one meter and pressures of one to two torr. The half-width of a

typical

recorded line

was 0.15

cm-1

and the transitions due to the

isotopes

of bromine were not resolved. The

spectra

were cali- brated

using absorption

standards after the method of Rao et al.

[4]. Preliminary assignments

were made

by

Kurlat

exploring

the use of a

generalized

molecular

prediction

model for

assignment

of

complicated

spectra

[3].

The results obtained

by

Kurlat indicated the existence of strong, non-localized resonance

between states

of v2 and v. ; using

a

Taylor expansion

of the upper state energy in terms of

J, K,

and

lt,

and

a

physical expression

for the

ground

state

[5],

he

found that 32

parameters

were

required

to

represent

the

assigned vs

transitions for K

9,

J

30,

with

a standard deviation a = 35 x

10- 3 cm-’,

and

17

parameters

were

required

to

represent v2 frequen-

cies for K

7,

J

35,

with (1 = 17 x

10-’ cm-’.

We have now decided to

reanalyze

the same

experi-

mental data with the introduction of

the x - y

Coriolis interaction.

2.

Analysis

of the spectrum. - A

complete

re-

appraisal

of Kurlat’s

assignments

was undertaken.

Weights

were

given

to each

line,

some wrong or dubious

assignments

were corrected and a few new ones were made

possible by

the

predictions.

The

R Ra

and

RPo

lines

of v.

which had been

assigned by

Kurlat but not used

by

him were reintroduced. In contrast, it was decided not to use K > 5 lines in v2 since

they

are

overlapped by

low K lines.

A

difficulty

arose due to the fact that the lines

belonging

to the two

approximately equiabundant isotopic species, CH379Br

and

CH381Br

were not

resolved. From

high-resolution

studies of

2 vs [6]

and

2 v2 [7],

we

expect

the band-center to be

slightly

lower for

81 Br

than for

79Br, by

about 0.009 cm-1

for vs

and 0.028

cm -1

for v2, but because B-values are, smaller for

81 Br by

about 0.0012

cm -’,

the

isotopic

shift should grow rather

quickly

for the

R(J)

lines

(up

to 0.100

cm-1

around J =

30)

while

it cancels and

eventually changes sign

in the P-

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01975003609076900

(3)

770

branches. We therefore used

throughout

this work

an average bromine with

ground-state

molecular

constants obtained

by averaging

the values

given

in

[8]

for the two

species :

This

procedure

will of course .limit the accuracy of our results. In the final

computational

stage, 346 transitions were

used, namely

110

for v2

and 236

for Vs.

3. Model used. - We have used the

least-squares

program described in reference

[9, 10].

The energy-

expression

includes

Maes’ qj and ’IK

terms from the

third-order Hamiltonian. We solve 3 x 3 Hamilto- nian matrices

taking

into account not

only

the x - y Coriolis interaction

[11-13J,

but also the

l(2, 2)-type

resonance. All

computations

were

performed

at

Orsay ’on

a Univac

1110 computer.

Although

17

parameters

can vary in the program,

we found that several of them are not

significantly

determined from the data. Therefore

Dj, D;’lK

and

D’

were constrained to their

ground

state values for

TABLE 1

Molecular constants

derived for

an average bromine

Ground state values fixed. Distorsion constants fixed to ground

state values. All values except Cx2., in cm-1. The errors quoted are

standard deviations given by the least squares calculation.

both vibrational levels

and q

as well as ilj were set to zero. A fit with the

remaining

9

parameiers gives

the results listed in Table 1 and a standard deviation

on residuals of 25.3 x

10-3 cm-l.

A somewhat better standard deviation was obtained with

D’

free to float but the fit

yields

an

unacceptable

value

of - 3 x

10-4 cm-l

for this

parameter.

In Table 1 we

quote

the standard deviations

given by

the

least-squares

calculation. The real uncertainties

are

probably

much

larger, especially

for

A 2 - Ao

which is not well known because we could not find K values

larger

than 5 in

the V2

band.

TABLE II

Comparison

with

previous

studies

of

v2 and v 5

(all

cm-

1)

... ,

TABLE III

Comparison

with indirect determinations

of

a2 and ce,

(all cm-1)

(4)

771

4. Discussion. - The values found in this work

can be

compared

with ones obtained

previously

from

direct studies

of v2

and v.,

by

infrared

[1, 2, 3]

or

microwave

[14] spectroscopy

which have been sum- marized in Table

II,

and also to indirect determina- tions of the same constants

by

studies of overtones

[6, 7, 15]

or combinations bands

[16],

which are collected

in Table III.

As mentioned

above,

Kurlat

[3] treated v2 and v5 independently.

His

prediction

model

required

49 para- meters to fit the observed spectra

(32 for v5

and

17 for

v2) compared

to the

only

9 free parameters and 5 fixed known

ground-state

values for the combin- ed V2

and Vs

data set used here. In an

attempt

to

extract

physically meaningful

parameters from the

severely perturbed spectra,

Kurlat then used a

physical

model for each band

limiting

the

input

data to very low J and K-values.

Fitting

the thus restricted data

required only

three and five parameters

for v2

and v.

respectively

- a result not

unexpected

in the presence of an x - y Coriolis resonance.

Morino and Hirose

[14]

recorded two micro-

wave transitions of

CH3Br (J

= 1 -

0,

K =

0)

and

(J

= 2 -

1,

K =

1)

in

the V2

= 1 and v5 = 1 vibra- tional states.

They

treated the Coriohs resonance.

explicitly, finding 2,5

values between 0.60 and

0.67,

as

compared

with

0.616s

here.

Table II shows that the band-centers are reaso-

nably

determined from any model. For

a5,

old

determinations as well as the

physical

model of

Kurlat

give surprisingly good

results. For

a2,

which

was taken as zero in reference

[2]

the

prediction

model

gives

a nonsensical

value ;

the

surprising

value

of + 23.1 x

10-3 given by

the

physical

model

[3]

is due to a clerical error in the value of

a2 - a2,

which should be - 0.021 instead of + 0.021

giving

a derived value of

a2

of - 18.9 x

10-3.

The

major

effect of the Coriolis interaction is

apparent

in the

aB values.

Previous values

of oc2 quoted

in Tablè II

are too

large by

a factor of 2 or 3. Even

though

Morino

and Hirose treated the Coriolis

interaction,

their

high

value is

probably

due to the fact that

only

low

J lines were

used,

as was

pointed

out in reference

[17].

Similarly,

it seems

likely

that the

a’

are closer to

zero than was

suggested by previous

work.

Overtone and combination bands

yield

similar

results. In reference

[1],

the

2 v2

band was treated

as if it were

unperturbed.

The same data treated in reference

[15] by taking

into account a Coriolis inter- action with

(V2

+

V.) gives a2

much closer to the present results. In reference

[16],

constants are deter-

mined for the

(v3 + vs

+

v6) (A 1

+

A2)

band which

interacts with vl, but the very

likely

Coriolis interac- tion between

(v3 + v_,

+

v6)

and

(v2

+ V3 +

v.)

could

not be taken into account; moreover the values of

as

and

as

obtained in reference

[16] rely

on the cor-

rectness of v3 and V6 - values from other works.

Finally,

the

present

results compare

reasonably

with

the values obtained in reference

[6] by

at treatment of the interaction of 2

vs(A1)

with

(v2

+

vs) although

the small values

of oej

have

conflicting signs.

These

could result from the limited resolution data used for

(v2

+

v.) [6]

or the limited data set used

for v2

in this work.

5. Conclusions. - This work does not

by

any

means conclude the

analysis of v2

and Vs. We have nevertheless shown for the first time

directly

that

x - y Coriolis resonance is

actually present

and

important.

The molecular constants

given here, although

not final are

probably

closer to the real

values than

previous

ones. We are

planning

extended

work with a

higher resolution,

at

Orsay

as well as at

Knoxville,

on these fundamentals and their overtone and combination bands.

Acknowledgments.

- The spectra used in the ana-

lysis

were taken from the doctoral dissertation of M.

Kurlat, who,

while a student at the

University

of

Tennessee,

was

permitted

to use the

spectroscopic

facilities at Ohio State

University

in 1969 with the

compliments

of Professor K. Narahari Rao of Ohio State

University.

Portions of this work were

supported by

NASA grant NGL-43-001-006.

References

[1] MORINO, Y. and NAKAMURA, J., Bull. Chem. Soc. Japan, 38 (1965) 443.

[2] JONES, E. W., POPPLEWELL, R. J. L. and THOMPSON, H. W., Spectrochim. Acta. 22 (1966) 647.

[3] KURLAT, M., Ph. D. Dissertation, University of Tennessee, Knoxville, 1969.

[4] NARAHARI RAO, K., HUMPHREYS, C. J. and RANK, D. H., Wavelength Standards in the Infrared (Academic Press, New York) 1966.

[5] BLASS, W. E., NIELSEN, A. H., in Methods of Experimental Physics, 3A, 2nd ed. D. Williams, ed. (Academic Press, New York) 1974.

[6] GRANER, G., J. Mol. Spectrosc., 51 (1974) 238.

[7] BETRENCOURT-STIRNEMANN, C. and MORILLON-CHAPEY, M.,

J. Mol. Spectrosc., 46 (1973) 171.

[8] BETRENCOURT-STIRNEMANN, C., GRANER, G. and GUELACH- VILI, G., J. Mol. Spectrosc. 51 (1974) 216.

[9] DEROCHE, J. C., GRANER, G. and ALAMICHEL, C., J. Mol.

Spectrosc., 43 (1972) 175.

[10] DEROCHE, J. C., Thèse de 3e Cycle, Paris 1971.

[11] DI LAURO, C. and MILLS, I. M., J. Mol. Spectrosc. 21 (1966) 386.

[12] DILLING, R. L. and PARKER, P. M., J. Mol. Spectrosc. 28 (1967) 178.

[13] BLASS, W. E., J. Mol. Spectrosc. 31 (1969) 196.

[14] MORINO, Y. and HIROSE, C., J. Mol. Spectrosc. 24 (1967) 204.

[15] BETRENCOURT-STIRNEMANN, C., Thèse, Orsay 1975.

[16] BETRENCOURT, M., MORILLON-CHAPEY, M., GUELACHVILI, G.

and AMIOT, C., to be published in J. Mol. Spectrosc.

[17] GRANER, G., J. Physique 31 (1970) 435.

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