Critical analysis of the series expansion of the potential energy function of CO2

Critical analysis of the series expansion of the potential energy function of CO2

JOURNAL OF MOLECULAR SPECTROSCOPY (1975) ST,464479 Analysis of the Series Expansion of the Potential Energy Function of CO, Critical I. JOBARD A...

871KB Sizes 0 Downloads 9 Views

JOURNAL OF MOLECULAR

SPECTROSCOPY

(1975)

ST,464479

Analysis of the Series Expansion of the Potential Energy Function of CO,

Critical

I. JOBARD AND A. CH~DIN Laboratoire de Physique Mol~czdaire el d’0ptiqzce AtmosplzCriq~e,~ B(itiment 221, Campus d’Orsay, 91405 Orsay, France

We present in this paper new values of the coefficients involved in the series expansion with respect to internal coordinates of the potential energy function of the COZ molecule. The relative importance of each potential coefficient and the cancellation of some potential coefficients nonsignificantly different from zero, are discussed.

I. INTRODUCTION

In 1971, Cihla and ChCdin (1) proposed an accurate determination of the potential function of the carbon dioxide molecule. This solution has recently been reiterated (2) with a view to fitting additional vibrational levels belonging to more than three isotopic species so as to obtain a more efficient “data-reduction.” By rewriting some of the programs currently used in a slightly different way, one of us (A. C.) has pointed out an error affecting the values of the Aw’s (fourth-order correction to the W’S). Correcting this error has led to smaller values for the Aw’s and a few iterations have significantly improved the fit. This paper is concerned with the presentation of this new solution and

its application

to the calculation

paper numerical

each coefficient involved respect to internal

II.

The potential

of nine isotopic species of COZ. We also present in this

trials which make it possible

to analyze

in the series expansion

the relative

of the potential

importance

energy function

of with

coordinates.

DETERMINATION

energy function

OF THE

POTENTIAL

of linear triatomic

ENERGY

FUNCTION

molecules has been determined

to a

high order of approximation by means of the method carried out by Cihla and ChCdin. Let us recall that this method (f-8) consists in solving algebraically the SchrGdinger equation2 associated

with the motion of the nuclei of the molecule under consideration.

The coefficients occurring in the expansion of the potential energy function are determined through an iterative process which leads to the minimization of the sum of the squares of the deviations between experimental and theoretical energy values of the 1A part of this work has been done Pierre et Marie Curie (Paris VI). 2 Resulting from the Born-Oppenheimer

at the Laboratoire approximation. 464

Copyright

Q 1975 by Academic

All rights of reproduction

Press. Inc.

in any form reserved.

de Spectroscopic

Mol&ulaire,

Universite

POTENTIAL

FUNCTION TABLE

Ii

COEFFICIENTS

OF CO?

I

OF THE POTENTIAL ENERGY FUNCTION WITH

RESPECT TO THE INTERNAL COORDINATES i

a

Identification of Fi

1

b

Fll

2

F22

3

F33

4

F1ll F

5 6

122

F133

7 8

F1lll Fl122

9 10

F1133

F

11

2222

R,&2

AND R3_

Value of Fi (in cm-' 7.10118486

lO+2

3.35544533

10+2

I.23097527

10+3

-4.64853340

IO+'

-2.92561323

IO+'

-2.66177899

IO+~

1 . 68642683

IO+'

8.95554064

lo-'

2.10697178

IO+'

8.31589408

10-l

-1.37333355

1o+o

7.06295807

1o+O

13

-3.14774539

lo+O

14

-4.40575542

1O-2

F2233

12

F3333

6 . 07253274

15 16

-7.71360113

17 18

F1 F

19 20

3333

111111

F111122

21

Fl11133

22 24

F223333

28

F333333

a VaIue of the index

12233

9.63040322

IO-'

?8

lO-3 lo-' Ido 10-I 10-~

7.93249999

lo-2

2.74749816

IO-'

i in the summation of Eq.(l)

‘J/he = FOP example F

10-l 10-l

-2.38249065

F222233

27

7.10695154 4.64850010

1.05571018

F222222

26

10-I IO+'

-1 * 61542514

F113333

25

1.60647895

-5.96705384

'112233

IO+' IO-'

-3.54636163

3.75013123

F112222

23

b

46.5

:

-i Fi Oi(R) i=l

is the coefficient which multiplies

the third order operator RIR$i

vibrational levels.The

theoretical values of the energies are obtained by computing the eigenvalues of the vibrational Hamiltonian transformed by means of two successive contact transformations and expanded up to the fourth order of approximation. This method makes it possible to determine accurately the 28 coefficients involved in the series expansion of the potential energy function of the CO2 molecule. This expansion is

466

JOBARD

AND

TABLE fi

COEFFICIENTS

CHEDIN

II

OF THE POTENTIAL ENERGY FUNCTION

WITH RESPECT TO THE INTERNAL COORDINATES

i

a

Identification

1

2 3 4 5 6

fl73 f122

fl122

13

15 16 17 18 19 20 21 2; 23 24 25 26 27 28

*I113

f1133 f1223 f 2222 f11111 f11113 fll122 fll133 *II223 f12222 f

Value

111111

f111113 *Ill122 f111133 *Ill223 f111333 f112222 '112233 '122223 P 222222

AND 5;

of fi (in cm-'

5.423606

fill

9 IO

14

b

f13 f 22

*Ill1

12

fi

fll

7 8

11

of

6,,&

IO5

8.511384

IO4

1.971324

lo4

-1.485150

lo6

-6.894162

IO4

-3.488122

104

2.338757

IO6

-2.017686

lo4

5.289104

IO3

-6.043205

IO4

7.609672

lo4

2.870283

lo3

-3.497619

106

-3.497362

lo7

1.725030

IO4

-1.348908

10~

-1.037847

105

-5.403060

lo3

5.768660

lo7

4.052455

10'

1.893240

lo6

7.734308

107

1.776057

IO7

7.046218

IO8

-1.136341

IO4

1.480776

lo7

4.405020

lo4

2.140762

IO4

’ Value of the index.i in the summation~of Eq.(2) : V/he = $, fi O;(c) b For example,

'1,223

is thk coefficient which multiplies

the operator

carried out with respect to the three internal coordinates3 RI, Rz, and RB [defined Ref. (I)] which are quasinormal and mass-independent. It is written as

&=2 FiOi(R), i-l

in

(1)

3 Let US call Arl and Arz the variations of the bond lengths, and AtJ the angle of the two bonds. RI, &, and & are linear combinations of the dimensionless coordinates ~~ = Arl/rl", b = ~q t1 = Ar~/rz', where rlc and TP are the equilibrium bond lengths (rIe = rye for a C&like molecule).

POTENTIAL

FUNCTION

TABLE

TO

i

a

Ai

COEFFICIENTS

THE

NORMAL

OF

THE

COORDINATES

b

:dentification of ki

EXPANSION

7

1 2C1 ho

-43.2577 75.2396 -252.a942

111 122

11

1111

13 14

1122 1133 2222

17 18

1 .5321 -11.5804 19.5438 2.6634 -28.0753 6.6889

2233 3335

19 20

11111 11122

22

11133 12222 12233 13333

5.5465 -3.2789

32 34 35 38 39 40

0.61 -0.830”

;;

111111 111122 111133 11222: 112233 113333 222222 222233

46 47

223333 333333 Value

of

D For

12233

example,

ill (q&

are

+ qE2)q;

i

in

snly

the 28

stands

(in

cm-‘)

‘4c’ 60

2

2

676.8553 318.4470 1133.8167

-5771

-39.5923 69.82’0

-43.2577 71 .2124 .239 ..3580

-234.6813 1.3615 -10.4339 17.6088

0.7181

-2.4089 0.6662

-2.4089 0.6466

5.3427 -0.993’ 5.2353 -3.0950

4.9562 -z.g909 5.2216 -3.0869

4.8107 -0.9336 4.9194 -2.9082

0.6996 5.2049 -0.9429 4.9686 -2.9373

0.6154 _‘I.8068 0.8272 0.1146 ci.6109

12.5156 -.‘.7267

0.5156 -0.7054 ‘2.7232 0.1045

0.6154 -0.7860 0.8059 0.1087

rJ. 55?3 -1 -3.0235 0.2572 -0.2683 0.2211

-1.3063 -0.0229 ‘1.2498 -3.2606

18.9875

2.5139 6.3136 -2.7920

.3764

of

:

V/he

k12,,33

,

=

czfficient

L

?>.9920 -2.7920

0.5797

.2517

-3.2934 0.2418

Eq.(3)

18.4977 2.3859 -25.1503

6.1104

-1.3329 -c.0257 0.2813

coefficients).

1.5321 -10.9606

2.4330 -25.6472

0.7451 1.1110 :. i91:

-1 -0.0247 0.2701 -1).2819 0.2322

the

RESPECT

438.058’7 321 1144.9614

-39.5923

-26.5000

summation

SPECIES

13C18,7

?

1 .5321 .2508

non-vanishing for

12~18~

WITH

1.361: -10.7495 ’ 18.1416 2.5825 -27.2225 6.4857

-11

54

FUNC’UO?,

SYMMETRIC

71 a9334 -241.7815

-1 .4582 -0.027@ 0.2946 ‘-0.3073 0.2532 index

VARIOUS

-43.2577 73.0982 -245.6966

0.8514 3.1214 0.647:

there

FOR

638.0587 331 a3063 1179.6018

-1.0526

the

species,

q3

ENERGY

676.8553 326.8799 1163.8418

-2.7920 0.7392 , .4992

23 26 57 28

POTENTIAL

13c’ 60:

2

133

a

AND

33

;;

III THE

q,~21’~~

11 22

1

OF

467

OF COn

c i=l

which

ki

@i(q)

0.2147

. (For

mi1tiplies

the

the

symetri::

#Jperator

.

where the Fi’s are numerical coefficients,4 and the Oi(R)‘s are operators which may be (m, n, and p being integers such that written under the general form RlmRPRP 2 < m + 2n + 2p < 6); they are invariant with respect to the symmetry operations belonging to the point group D-I, of the linear symmetric molecule XYZ. The expansion up to the fourth order of approximation contains 28 operators5 of that kind. III.

IMPROVED

POTENTIAL

ENERGY FUNCTION MOLECULE

OF THE

CARBON

DIOXIDE

Table I gives the set of the 28 “potential coefficients” appearing in the expansion of the potential energy function obtained at the end of the new iterative process. The set of the fi coefficients involved in the expansion

hc

i-l

4The F; coefficients will hereafter be called “potential coefficients.” 6 Let us notice that our programs are actually adapted to the point group C,, and so make it possible to deal with the general linear triatomic molecule, XYZ.

JOBARD

468

AND

CHEDIN

of the potential energy function with respect to the dimensionless internal coordinates 51, [2, and & [also defined in Ref. (I), and recalled in footnote 31, are given in Table II. In Tables III and IV we give the sets of the ki coefficients appearing in the expansion ‘I’ABLE _Iri

COEFFICIENTS

FUNCTION

WITH

zq3 i

a

OF

THE

RESPECT

TO

,FOR

VARIOUS

IV

EXPANSION THE NON

1

11 13 22

3 4

33

2 7 P

SYMMETRIC

SPECIES

11

1111 1113

::

1122

14 15 16

1133 1223

0.7454 2.6284

19 20 21 22

11111 11113 11122

23 24 25 26

11133 11223 11333 12222 12233 13333 22223 22333 33333 111111 111113 117122 111133 111223 111333 112222 112233 113333 12222 3 122333 133333 222222 2222 33 223333 333333

I‘ 1

(in

;.b

See

*

These

footnotes

they fwlrth

order.

16013c170

666.6740

324.2394

325.4845 1158.9482

0.0

-42.3001 2.7924 72.2i48 -242.6949 3.5472 -4.4471

-8.3278

1.4877 -0.2640 -11.3564 19.1611 -0.4490 0.4010

18.2433 -0.R503 0.7768

2.6435 -27.861A 6.6393

2.4793 -26.1207 6.2284

1.4879 -0.2834 -11.0297 18.6089 -0.4515 0.4182 2.4941 -26.2874 6.2644

-2.6867

-2.5880 -0.6490 0.6809

-0.3556 0.69RP

1.4499 -0.5210 -1O.P211

-2.5894 -0.6049 0.7@lj 5.1650 -0.0147 0.7313 -1.0209

0.7195 5.3374 -0.0085 -1.0361

5.0047 -0.0184 0.7618 -0.9626

5.3793 -3.1552 -0.1434 0.2533 -0.1026

5.4594 -3.2203 -0.0762 0.1352 -0.0550

5.0718 -2.9706 -0.1422 0.2543 -0.1038

-0.3312

0.3967

-2.6863

5.1811 -0.0106 0.4137 -0.9774 5.15@3 -3.0368 -0.0756 0.1358 -0.0557

0.5629 *

0.5879 *

-0.7767 C.7981 * *

-0.8023 0.8231 x *

-0.7541 c1.7752 * *

0.1159 0.6150 -1.3AOl * * *

0.1185 0.6312 -1 .4206 * * *

0.5792 -1.2989 * * *

0.5952 -1 .3395 x * *

-0.0267 0.2914

-0.0243 0.2650

-0.3037 0.2497

-0.2753 0.2247

-0.0245 0.2671 -0.2783 0.2287.

-0.0265

0.2892 0.2457

@f Tai,le are

contribute

I

-41.4453 5.1711 71.3741 -2 39.7900 6.6867

74.3522 -249.8844 3.4605 -4.2637

-0.3006

coefficients

do not

cm-‘)

657.2738 0.0

@.587i? Y

0.5627 *

-0.7792 0.7995 * *

O.lC92

0.1113

I

I

a

q,-Lq2,1q22

1154.7075

-42.2988 2.6005

19.7950 -0.8454

-27.6925 6.6020

29 30 31

335.1002 1193.1766

1.4493 -0.4856 -11.1461

2233 3333

27 28

0.0

-7.9893

1333 2222

17 IR

666.6847

6.5247

333

ENERGY

116~13~18~

l16012C170

-41.4409 4.8186 73.5128 -246.9964

133 223

9 IO

POTENTIAL

COORDINATES

657.3123 0.0 333.B910 1189.0427

111 113 122

THE

NORMAL

I~en:~~~pationbl~6012ClEo

2

OF

III. not

considered

t,> the

energy

the

program

expanded

in

~cp to

since the

Eil

Gil

E+O

E-

E-Z

E-?

E-’

-1.‘251506

-1.256150

-i .069564

-4.2920.‘9

‘4.889310

-8.840810

-4.168802

E-l

E-:

1.347

3.9<%

AU,

AW,

E-2

'.955189

Ati;

E-1

1.347743

E-2

E-i

E-2

3.1c19S84

E-l

E-?

2.69859Z

E-.

5.R745"4

6.957749

3.227750

E-2

1.458479

7.136251

Et,

E-?

-3.9244R7

-2.548829

E-i

F-?

-4.7.l4031

E-?

Et0

1.642029

6.35504f

E+1

-1.920453

E-‘

Et-0

Y.413195

E+O

E+?

2.3954725

-;.4,609*

Et2

-..7291162

-~.PRylOb

Ei4

1.353:!0’

-7.390

A3 u

12

A1

wl?2

Y3u

YZLI.

YlLC

y333

y233

y223

y222

y733

y123

y122

y113

Yl12

y111

xLI.

“33

X22 x23

?13

x12

X11

Y

Y

w.

E+O E-3 L-2 E-2 s-1 E-i E-2

-1.052780 -7.9405,4 c.obP*o, 031571 -4.290061 1.375666

* .394?47

EID

E+3

E+*

ii3

E-,

E-:

E+1

El'

E+C

E+!

E-2

E-2

E-3

E-' E-Z E-i

-1.154 1.384 4.010

1.933282

1.078493 E-2

E-1

E-!

E-1

3.156134

2.598968

E-I E-t

I.290773

! .737202 E-2 -1,.010E-2 1.119E-: 3.5’5 E-:

E-1

Eel

-2.458139

Ei'

-2.530556

E--

2.943187

E-2

2.826262

u.892474

2.474485

E-3

,.a,,341 .%.*I7779

c;.o192.35 E-2

2.982558

E-i

.23U4i6

E-i

E-? E-3

1.258390

E-2

E-2

-J.507144

-1.235768

1.282340 E-l r .666,68E-2

-3.646787

-;>.379034

i.202338.E-2

-..V,2642

-'1.8e7457

-:.lt76L*

-'.I59375

'.$20722

-'.'97,79

-',.0503:,5 ElO

-i.721237

2.3094140

...4847874

IQ

E-2

Et,

lzc

1.3145476

ii0

1.364490

E-2

2.35920,6

E+3 El.2

'.<26,268

2 1.27<,I74

‘E.

4.41&63

-3.690712

~-3

Et,

-!.244124

-4.728260

E+1

-1.238089

Is+'

-1.845113 =+o

E+O

7.6,6867

E+O

Et3

2.3780854

-5.226719

E+7

-2.718761

Et3

1.3146245 1.6778200

lZc

ljc;

ir,

E12

E+j

1.:33

7.117

-4.000

I,747882

E-’

E-2

E-2

1.4217,6

2.976968

,.521415

-6.4R6529

2.922749

c .240222

',.260209

'.731840

'.316589

-3.626153

-3.241860

..429991

1.297013

~-2

E-i

E-l

E-1

E+?

E-L

E-3

E-2

E-3

E-2

6-2

E-3

E-?

E-l

E-2

E-2

-1.'778103 -j.600551

E-2

E-J

E-l

E+i

E+1

6+i)

E+1

E+C

tro

l’io

1.137119

-4.871597

-9.97723!;

-,.17269?

-'.i05WG

i.'33554

-'.P336Pj

-',.150423

-2.799597

2.317R9t‘l

i.5096894

1.33334'0

lto

1.2761174

E-2 E-3

.'02

E-2 '.244

-8.420

1.721855

1.068291

2.877846

2.382910

-2.405647

2.722552

G.116854

5.3*5058

7.166399

I.265405

-3.366298

-4.~84027

-,.8x789

1.223004

-3.770944

-:'.604161

1.473154

-1.595523

-9.787065

-i.r50544

-'.14700h

i.501660

-1.727238

-n.886403

-1.564109

‘.2899228

: .4315428

E-2

E-l

E-l

E-l

II+,

E-e

E-3

E-2

U-j

E-2

E-2

E-3

E-2

E-l

E-2

~-2

E-2

E-3

E-I

E,l

E+i

EtL?

E+,

Et0

E+O

E+j

Et2

E+,

1.3537107

3.178

Q.980

2.390

E-l

E-3

E-2

1.594051

'.727305

2.832418

2.465502

->.452454

2.875891

5.738091

4.685648

i.050121

’ .268297

-3.578870

-,.86115?

,,.168650

1.243815

-,.066174

-7.941239

j-364055

-I.P92079

-9.516932

-1.113e30

-1.105444

".464516

-1.831650

-c.098828

-'.885406

2.2676334

- .3689398

E-L

E-7

E-'

E-l

El,

E-2

E-,

E-i

E-2

E-Z

E-L

E-3

E-2

E-l

E-l

E-2

E-2

E-l

E-l

6+1

E+l

E+O

E+i

E+O

E+O

Et,

E+L

E+3

JOBARD AND CHEDIN

470

of the potential energy function with respect to the dimensionless normal ccordinates (ql, 421,q22,43) of each one of the nine isotopic species we have studied. This expansion is written as

(3) with e(q)

We have computed,

=

qlm(q212

+

with this new solution,

q222)"q3".

the values of the spectroscopic

constants

TABLE VI COMPARISON BETWEEN EXPERIMENTAL AND CALCULATED VALUES OF SOME ENERGY LEVELS (in cm-')

W60, vibrational level

(1) -E

E exp

(1000)1 (1000),1

(11)



CFilC~

E

exP

-E

oc7

0.002

0.006

-0.001

-0.

(I)

i ribrational talc 1

level

OllU

E

exP

-E

(II) talc )

E

-E exP

-0. DC11

-0.007

I:ll'o)I

ca1c

0.020

-c.o05

-0.020

0.007

0220

0.040

0.002

0002

0.030

O.cill

0221

O.O,?O

(21’1 II

0.040

0.003

oo"l

0.001

-0.001

0.010

-0.004

-0.020

0.003

oo"3

0.06C

0.020

(21’1),, (21'1) III

I:11'0),,

’ %’ 602

o.002

16012c180 -¶-

vibrational level

0001

(11)

(1)

IEexp -Ecalc rE

i exP -Ecalc

-0.060

V'ibrational

level

-E ’ exp talc'

-0.040

-0.005

ooO2

-0.c50

O.Cl4

( IO01 1I

-0.050

-0.011

-0.070

-0.033

-0.020

0.004

-0.120

-0.011

-0.019

(10°1)11

-0.02C

-0.013

-0.06c

0.019

( loo1

(2221 111

-0.29o

0.017

01'2

(2221 JIII

-0.430

0.050

01'

(I) : value of 1971 (Ref.(l))

column (II): new value.

(II 1 E

oo"l

-0.1 YO

column

(I) -E ) exp talc

0.026

(lOOl)I

0112

E

II

3

POTENTIAL. FUNCTION OF CO,

471

TABLE VII

VALUES OF THE NORM GIVEN BY Eq.(4) FOR 9 SPECIES OF CO2

Isotopic species

Norm t0N201 (in cm-*)

'%'60*

2.3

10-4

'%'60*

I.7

10-3

16012c~80

1.2

10-3

16012c170

2.7

10~~

~2~18~ 2

8.0

IO-~

16013c180

2.6

1O-3 1

I

--I 10-l

occurring in the expression6 of the vibrational energy, referred to the minimum of the potential ; they are given in Table V for the nine species. In order to illustrate, by a few significant examples, the improvement brought by these new iterations, we compare in Table VI the new values of the discrepancies between experimental and calculated values of some representative vibrational levels for 12C1602, WsOz and 16012C1s0 molecules with the values of the discrepancies obtained in 1971 (1). The calculation, for each isotopic species respectively, of the “norm” N2, given by the expression X2 = 5 AE,2Pi/ 2 Pi i=l

i=l

(4)

(that is to say, the weighted sum of the squares of the deviations AE; between experimental and calculated energy values of a set of n observed levels), leads to the nine numerical values of Table VII. These values correspond to a mean deviation of a few hundredths of cm-‘, which is in very good agreement with the present accuracy of the experimental data. Particularly, the best levels of the principal isotopic molecule 12C1602 are reproduced within a few thousandths of cm-‘. 6 See Ref. (2). Our X’s are defined as being one-half of the X’s of Ref. (1).

472

JOBARD IV. CRITICAL

A. Relative Importance

AND

ANALYSIS

of the “Potential

CHEDIN OF THE

SOLUTION

Coejicients”

The numerical tests which were carried out with the new set of the 28 “potential coefficients” Fi (given in Table I) aimed at examining the influence of a modification of the value of one coefficient on the mean value of the deviations (or better, on the “norm”) between theory and experiment. We have represented some of the results in Figs. l-4. For each of the 28 potential coefficients, the percentage of modification of the coeffkient value is plotted along the X-axis, and the change of the “norm,” characterized by the factor multiplying the reference norm obtained with the nonmodified value of the coefficient, is plotted along the Y-axis. For example, Fig. 1 shows that a 1% increase of the value of the F33 coefficient leads to a “norm” equal to 3.10 f6 times the reference norm. We must notice that the scales on each figure are different, but most of the 28 curves reveal an important increase of the norm for a rather small change of the coefficient value, except the curves of Fig. 4, relative to the variations of the coefficients F 1~22 and FwB~~. Nevertheless, all these curves have the same shape : they are almost exactly parabolas, having as their minimum a 0% variation of the coefficient. This means that the reference solutionthat is to say, the new potential energy function-constitutes a minimum stable with respect to the modification of the value of one of the coefficients. IJ~(x% ),‘N* (0%)

-2% FIG. 1. The relative

potential

coefficient

variation value.

-1%

of the norm

0%

t1%

+2%

[see Eq. (4)] as a function

OF/F

of relative

variations

of one

POTENTIAL

FUNCTION

473

OF COz

t

-2% FIG.

potential

2. The relative variation coefficient value.

-1%

of the norm

c!%

+2%

+1%

[see Eq.

(4)] as a function

.&F/F

of relative

variations

of one

If we define the “importance” of a coefficient as being the magnitude of the increase of the norm yielded by a 1% variation of the accepted coefficient values, it is then possible to classify the 28 coefficients, for instance, in decreasing order of importance. This classification is given in Table VIII: -The column.

index giving

the order of importance

of each coefficient

is given in the first

-The coefficients appear in separate columns according to whether they belong to the terms of order 0, 1,2,3, or 4 in the series expansion of the potential energy function. --In the last column are given the values of the relative increases of the “norm.” B. Discussiot~ In this theoretical frame, let us recall that, by the expansion of the potential energy function order n - 2 to the energy.’ Thus, as Tlo, VI, Vz, ators of degrees 2, 3, 4, 5, and 6, they contribute, 7Actually, it is sometimes difficult energy of a nondiagonal operator.

to evaluate

assumption, an operator of degree n in is supposed to give a contribution of ‘v3, and V4 contain, respectively, operrespectively, to the energies of orders

the order

of magnitude

of the contribution

to the

474

JOBARD

AND CHEDIN

0, 1, 2, 3, and 4. Furthermore, when the expansion of the potential is carried out with respect to internal quasinormal coordinates and if we consider only low values of the vibrational quantum numbers, the convergence of the potential expansion is ensured by the values of the coefficients Fi. So, it is important to check that the classification of the “potential coefficients F;,” in decreasing order of their absolute values, is in agreement with these assumptions. This classification, given in Table IX, shows that it is generally verified. If we compare Table IX with Table VIII, which gives the classification of the potential we can see that they are, as a whole, coefhcients in decreasing order of “importance,” slightly different. The essential differences between the two classifications are set forth on Table IX by arrows pointing out the rows occupied by the same coefficients in Table VIII. So, we must notice the partrcular importance of the coefficients F22, F2222, F222222,and Fa3, F 3333, Fr3333, F333333.That importance can essentially be explained by experimental reasons regarding the characteristics of the set of levels whose agreement between theory and experiment is studied : (a) Among the 100 levels of the principal isotopic species which compose the set of levels we use, the vibrational levels involving the quantum number 7~2are associated with statistical weights, the sum of which is three times greater than the sum of the statistical weights associated with the levels involving or, and four times greater than

~*(x%)/‘N~(o%) ,L

4

0%

-10%

0%

+10%

+20%

AF/F

FIG. 3. The relative variation of the norm [see Eq. (411 as a function of relative variations Jotential coefficient value.

of one

POTENTIAL FUNCTION OF COP

L

I

-20%

I

I

I

I

-10%

0%

+10%

+20%

475

I

.

AF/F

FIG. 4. The relative variation of the norm [see Eq. (4)] as a function of relative variations of one potential coefficient value.

the sum of the weights associated with the levels involving vs. So, the choice of the statistical weights, which are to some extent related to the accuracy of the experimental data, favors the peculiar importance of the coefficients Fz, FXW, and FKWXW (b) The other characteristic is that the set of levels used contains highly excited levels : -First, there are levels involving high values of ~3; seven levels are such that v3 is larger or equal to 5, while vr is not involved in any level with a value greater than 4; those levels are, particularly, levels belonging to the ooOv3series* (the ~3 value going up to 9). This explains the peculiar importance of the F 3333,FLM, and F333333coefficients : effectively, the successive contact transformations to which the original Hamiltonian is submitted are such that these coefficients, for instance, strongly contribute to the spectroscopic constant ~333; for example, a variation of ~333in the energy expression of the level CNY9is multiplied by 729 (va3 = 9”) and contributes to the deviation (observed value minus calculated value) which occurs itself in the norm by its square. The fact 8 See Ref. (9).

JOBARD AND CHEDIN

476

TABLE VIII CLASSIFICATION

OF THE Fi COEFFICIENTS WITH RESPECT TO

THEIR "IMPORTANCE".

(DECREASING ORDER).

coefficients

27 28 a

_-.U_*.~~_-~__._.______ 11122 71 I_-_~~___-__^___~______I_ 112222 1.1

For exemple , 12233 stands for the coefficient F multiplies

the operator

R R2R2 123

12233 which in the potential expansion.

that there are levels involving high ~3 values explains in this way the importance of the coefficients mentioned before, and greatly contributes to their accurate determination. -Second, the set of levels also contains many levels which are strongly coupled by the Fermi resonance, and consequently involve rather large values of the “quantum

POTENTIAL

FUNCTION

01: CO2

477

number ~2” compared to the mean value of zlrfor the whole set of levels. This contributes as well to emphasizing the importance of the F22, F2222, Fzzzzzz coefficients. In conclusion, we see that the order of importance of the ‘Lpotential coefficients,” defined by reference to the criterion of their respective influences on the norm of the discrepancies between theoretical and experimental values, takes into account not only the respective values of the coefficients, but also the accuracy of experimental data, and the nature of the vibrational levels constituting the set of levels we use. TABLE IX CLASSIFICATION

OF THE

Fi COEFFICIENTS WITH RESPECT To

THEIR ASSOLUTE VALUE. (DECREASING OXDER)

Fi coefficients 0th

lSt

xder

order

1

33b

2

11

3

22'

IFiI

a

rd 3 oMer

2nd order

th 4 order

I

(in cm-I)

230.975 710.118 335.545

4

133

5 6

111 122

266.178

-+--

46.485

\

29.256

t _

-

21.070

1133

7 8

'7.063

3333

9

11133

10

13333

II

11111

12 _____ 13

_

3.148 -~-_ 1.686 113333

1.615

117733 .---_.___._

1.373 ---.... 0.963

14 -.~

6.073 __-__. _~_3.546

0.896

------_-.___ :lI;ii::

0.832 ____ 0.711 0.597 ___.. 0.465

I

0.275

I

0.161

0.106 0.077

0.044

a See footnote of Table VIII

222233

0.024

112222

0.004

JOBARD

478

AND CHEDIN TABLE X

ITERATIONS CARRIED OUT WITH LESS THAN 28 NON-ZERO

Fi COEFFICIENTS

26 COEFFICIENTS

27 COEFFICIEN

I No

of the iteration 167. 2.2 1.6

F222233

I

1 2 3

2.1 1.5

25 COEFFICIENTS

+I F

223333

C. Cancellation

11. 3.8 2.3 1.5

of the Potential

i 3 4

Coqqicients

24 COEFFICIENTS

Nonsignificantly

Dijerent

from Zero

Some of the less important coefficients (in the lower part of Table VIII) are not necessary for the accurate determination of the vibrational energies of the present set of levels. It is indeed possible to obtain a similar agreement between theory and experiment when one of these coefficients is constrained to zero during several iterative cycles. Likewise, a satisfactory norm is reached when different combinations of two, three, four, or even five unimportant coefficients are simultaneously set equal to zero. As examples, the results of some of these trials are given in Table X.g The coefficients whose values are kept equal to zero during iterations are set down in the first column; the values of the ratios (N*/N*n,r) of the norms N*, obtained at the end of each iterative cycle, to the reference norm N2nor, obtained by working with the full set of the 28 accepted potential coefficient values, are given in the second column. It appears that several solutions with 27,26,2.5, or 24 coefficients are satisfactory and, more precisely, lead to an agreement between theory and experiment, close to the agreement yielded by using the full set of 28 coefficients. This means that the values of five or six coefficients (Fww, F11122,F222233,FwB~, F12222,F223333)are not significantly different from zero. *We could not intend, for obvious reasons regarding computation time, to try all the possible combinations of coefficients to be cancelled out simultaneously; nevertheless the tests, restricted in numbers, that we carried out are conclusive.

POTENTIAL

FUNCTION

Ok’ COr

479

It seems reasonable to state that the values of these coefficients will be better defined when it is possible to work with a set of levels at the same time more numerous and more accurate, that is to say, composed of levels highly excited in wl, vz, and zrS,and systematically measured with better accuracy. ACKNOWLEDGMENT

We wish to express our gratitude to Professor G. Amat and to Dr. Z. Cihla for helpful discussions throughout the course of this work. RECEIVED :

March 31, 1975 REFERENCES

1. Z. CIHLAANDA. CH~DIN,J. Mol. Spectrosc. 40, 337 (1971). 2. I. JOBARD,Thesis, University of Paris, 1974.

3. A. C&DIN, Thesis, University of Paris, 1971. J. A. CHBDINANDZ. CIHLA,J. Mol. Spectrosc. 45, 475 (1973). 5. Z. CIHLAANDA. CH~DIN, J. Mol. Spectrosc. 47, 531 (1973). 6. A. C&DIN ANDZ. CIHLA:J. Mol. Spedrosc. 47, 542 (1973). 7. A. CH~DINANDZ. Crrry J. Mol. Spectrosc. 49, 289 (1974). 8. A. CHBDINANDZ. C~FILA,J. Mol. Spectrosc. 47, 554 (1973). 9. T. K. MCCURBIN,JR., J. PL~VA,R. PULFREY,W. TELFAIR, ANDT. TODD,J. Mol. Spectrosc. 49, 136 (1974).