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The analysis of the spark spectrum of gadolinium (Gd II)

J. Blaise, Th. A. M. van Kleef, J.F. Wyart

To cite this version:

J. Blaise, Th. A. M. van Kleef, J.F. Wyart. The analysis of the spark spectrum of gadolinium (Gd

II). Journal de Physique, 1971, 32 (8-9), pp.617-626. �10.1051/jphys:01971003208-9061700�. �jpa-

00207118�

(2)

617

THE ANALYSIS OF THE SPARK SPECTRUM OF GADOLINIUM (Gd II)

by

J.

BLAISE,

Th. A. M. van KLEEF

(*)

and J. F. WYART

Laboratoire Aimé

Cotton,

C. R. N. S.

II, Orsay,

France and

Amsterdam,

The Netherlands

(Reçu

le 29

janvier 1971)

Résumé. 2014 L’analyse du spectre d’émission de Gd II a permis de découvrir 108 niveaux impairs

et 70 niveaux pairs. Les 2 200 raies actuellement classées correspondent à 2 300 transitions entre 162 niveaux impairs et 150 niveaux pairs. Les longueurs d’onde de 18 500 raies de Gd I et Gd II ont été mesurées dans le domaine 2 468-8 752 A. On a observé la structure Zeeman de plus de

900 raies de Gd II entre 2 700 et 11400 A et le facteur de Landé de chaque niveau est maintenant

connu. Les termes impairs appartiennent à 4 f7 5 d 6 s, 4 f7 6 s2, 4 f7 5 d2 et à la nouvelle confi-

guration 4 f8 6 p ; les termes pairs sont attribués à 4 f7 6 s 6 p, 4 f7 5 d 6 p et aux nouvelles confi-

gurations 4 f8 6 s et 4 f8 5 d. On donne une interprétation paramétrique des configurations 4 f8 6 s, 4 f8 5 d et 4 f8 6 p.

Abstract. 2014 The analysis of wavelength data of the Gd II spectrum has resulted in the detection of 108 odd and 70 even levels in addition to those reported by previous investigators. The total

number of classified lines is now 2 200, belonging to 2 300 transitions between 162 odd and 150 even

levels. The wavelength list, including the Gd I lines, contains over 18 500 lines in the wavelength region 2 468-8 752 Å. The Zeeman effect has been investigated in the wavelength region 2 700-

11400 A. Of about 900 lines belonging to Gd II transitions the splitting has been observed. The

g-values of all levels could be determined. The odd terms belong to the electron configurations

4 f7 5 d 6 s, 4 f7 6 s2, 4f7 5 d2 and the newly established 4 f8 6 p ; the even terms have been associated with the configurations 4 f8 6 s and 4 f8 5 d (see 4 f8 6 p), 4 f7 6 s 6 p and 4 f7 5 d 6 p. Calculations have been carried out in the 4 f8(7F) 6 s, 5 d and 6 p subconfigurations. The values of the electro- static and spin-orbit interaction parameters give a good least-squares fit to the experimental levels.

LE JOURNAL DE PHYSIQUE TOME 32, AOUT-SEPTEMBRE 1971,

Classification Physics Abstracts :

13.20

1. Historical

Survey.

- An

analysis

of the Gado- linium II

spectrum

was

given

in 1950

by

Russell

[1].

His

analysis

was based on the temperature classi- fication of Gd lines

published

in 1943

by King [2].

Russell

only

established terms of

configurations belonging

to the 4 f’-core

(system A) :

the

expected

4

f8-configurations

remained undetected

(system B).

He classified 1 177 out of the 2 627 Gd II lines of

King’s

list.

Isotope

shift measurements of Brix

[3]

a few years

later,

confirmed Russell’s

analysis

for

the lowest levels of the

4 f’

5 d 6 s and

4 f’ 5 d 6 p configurations. Only

a few Zeeman effect measurements were available to

Russell, by

Albertson’s work

[4].

In 1965 Smith and

Wybourne [5]

made calculations in the

subconfigurations

- neglecting

the 4

f7 (8S0) 6 S2 8S7/2

level -, and

in

4 f7 (8S0) 6 s 6 p

and 4

f7 (8S0)

5 d 6 p.

Though they

made a wrong

supposition

about the

coupling

scheme in the 4

f7 (8S0)

5 d 6 s

configuration

as we

shall discuss later

(see § IV), they

gave

predicted

g-

values of all levels

belonging

to the

subconfigurations

mentioned

above,

which turned out to be useful.

Furthermore

they predicted

the

positions

of the

unknown levels of 4

f7 (8S0)

5

d2,

which viere not

detected

by

Russell. In 1967 Desmarais and

Pinning-

ton

[6] published

measurements of 120 resolved Zeeman patterns

belonging

to 86

wavelenghts

and

determined the

g-values

of 26 odd and 41 even known levels. The agreement between the observed

g-values

and the

predictions

of Smith and

Wybourne [5]

was

satisfactory

for most of the levels. In the same year Noorman made two series of spectrograms

of 158Gd

at the

Paschen-Runge mounting equipped

with the

« G5 »

grating

of the

Argonne

National

Laboratory

with an electrodeless

discharge

tube in the

region

2 468-8 752

A.

Each

plate

contained three

images

of

the

gadolinium

spectrum

exposed

for different

lengths

of

time,

and a

superposed

thorium spectrum for purposes of calibration. This series has been measu-

red

by

Slooten and Hoekstra

[7] by

means of an auto-

matic comparator « Zelacom »

[8]

built at the Zeeman

laboratory.

The second series contains Zeeman spec- trograms which we used for

deriving

the

g-values.

In 1969 an additional series was taken

by

M. Fred

in the

region

6 000-11400

A.

Our first results of the

analysis

of the Gd II spec- (*) Zeeman-Laboratorium der Universiteit van Amsterdam.

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01971003208-9061700

(3)

trum were

published

in March 1969

[9].

We gave the

positions

of the unknown levels

along

with the g- values of 4

f7 (8S0)

5

d2 levels,

the

complete 4 f8(7P) 6 s

multiplets,

over 40 levels of the 4

fl(7 F)

5

d,

many

levels of the 4

f8(7F)

6 p

subconfigurations

and many unidentified odd levels.

Independently

and at the

same

time, Spector [10]

at the San

Diego Meeting

of the

Optical Society (March 1969) presented

11 levels

of the 4

f8(7F)

6 s

multiplets (the

two levels with

J =

1/2

were not

given).

The same author

[11] ]

in

March 1970

published

a list of 966 Gd lines in the

region

7 300-12 300

A ;

he

assigned

602 of them to the Gd 1 and 309 to the Gd II spectrum. In the sche-

mes of Gd I and Gd

II,

we classified 491 of these lines as transitions between Gd 1 levels and 243 as

transitions between Gd II

levels ;

36 of the classified lines had a wrong

assigment.

In 1970

Spector [12]

gave more results : 17 even

levels of the 4

fl(7 F)

5 d

subconfiguration (all

pre-

viously published by

us in

1969)

which levels

belong

to the octets and 61 odd

levels,

31 of which he inter-

preted

as levels

belonging

to the 4

f8(8F)

6

po

suc-

configurations.

Seven levels of the group of odd

levels have incorrect

J-values,

three of these levels

were

already given

in our article

[9]

and at least four

levels,

not

belonging

to the 4

f ’(’F)

6

p° subconfigu-

ration are fortuitous

(see also § II).

Furthermore he gave 300 classified lines as transitions on the

newly

detected levels. In connection with the incorrect

interpretations

of the J-values and the fact that several levels which

Spector

ascribed to the 4

f8(7F)

6 p

subconfiguration

must be

interpreted differently (see § IV),

his calculations of the

predicted positions,

percentage

compositions

and calculated values for this

subconfiguration

is erroneous.

Recently Spector [13] ]

made a calculation in the 4

f8(7F)

5 d subcon-

figuration, using

45 of our level

values,

and a

good

fit was obtained

(see §

V and

VI).

II. The

wavelength

list and the classifications. - Our list contains over 18 500 lines in the

region

2 468-8 752

A,

with all information on a

magnetic

tape. In the table 1 we

give

the computer-output of

a part of the list. In the first column the number of the line is

given, starting

with

1, 6, 11,

etc. In the case

of a

doubly

or

trebly

classified

line,

it has 2 or 3 num-

TABLE 1

Gadolinium

wavelengths, wavenumbers,

transitions and Zeeman

effects

bers

(see

2 370 and 2

371).

In the second column is the

intensity ;

lines with an asterisk have been measu-

red in the track of the lowest exposure

[8].

The num-

bers in the third column refer to the character of the line under consideration. The code is the

following :

0 means the line is

symmetrical, 1

and 2 are used for

asymmetrical lines (1

for shaded to shorter

wavelength,

2 for shaded to

longer wavelength,

and 3 is used for lines which are

strongly perturbed ; 5, 6, 7,

and 8 have the same

meaning

as

0, 1,

2 and 3 for broadened lines. In the columns 4 and 5 the

wavelengths

and

wavenumbers have been recorded. In column 4 the

wavelength

is

given

in

A

x

10+4

and the wavenumber

in column 5 in mK

(1

K is 1

cm-1).

In the next column

we

give

the

assignment

of the classified lines to Gd 1

or Gd II. The columns

7, 8,

9 and 10 contain the level values in 0.1 K

(the

first level is

always

the odd

one)

and the J-values

(omitting

the decimal

point).

In

column

11,

Au = 6 observed-a calculated

(in mK).

Owing

to the accuracy of the measurements

only

values

of 1 Au 1

30 mK are

printed. Only

in

special

cases, for instance

doubly

classified

lines,

has a

bigger discrepancy

been

accepted.

The next 5 columns refer to the results of the Zeeman effect measurements, in columns 12 and 14 the

g-values

of the levels times

10+ 3,

mentioned in the columns 7 and

9,

in the columns 13 and 15 the J-values

(identical

with the columns 8 and

10).

When the

pattern

was

unresolved,

we calculated the

g-values

if the transition was known

(see

for instance the lines Il 326 and

11 332) (1).

In

the cases of unclassified lines

(2

399 and 2

401),

when

J1 =1= J2,

we list in column 12 the

position

of the

strongest a-component f on one side of the pattern and in column 14 the value of the width of the x-

pattern Je on the same

side ;

in column 16 the cha-

racter of the

pattern :

SO means shade-out

(1)

See note on next page.

(4)

619

SI means shade-in

(Jl > J2

and 91 >

g2).

When

J1

=

J2,

we put in column 12 the values of the center

of gravity

in the a-pattern and in column 14 the value of the strongest Tr-component on one side of the pattern ; in column 16 the

symbol

S stands for sym- metrical. In cases of the presence of Paschen-Back effect

(over

10

%

of the measured

patterns)

column

16 is needed for the abbreviation PB.

In column 17

King’s

classification is

given.

If it

is necessary to

give

more information about the

wavelength,

the Zeeman

effect,

etc., we add our

comments under that

wavelength.

It is not

possible

to

publish

the whole

wavelength

list.

People

who are

interested in it can receive a copy of the list upon request

(1).

Since we do not want to repeat ourselves in both articles about the

Gd-spectrum,

we

give

information for both

spectra.

We have classified over 2 200 lines as Gd II tran- sitions and over 5 300 lines as Gd 1 transitions. This is about

42 %

of the total number of the lines.

Nearly

400 lines have been

doubly

classified

(in

Gd 1 and Gd

II) ;

in many cases the double classifications could be deter- mined

by

Zeeman effect measurements

(see

numbers

2 370 and 2 381 in Table

I).

We measured about 2 700 Zeeman patterns, of which about 300 have not

yet been used in the

analysis.

It must be mentioned

that for a

large

number of unclassified

lines,

we have

not yet measured the Zeeman patterns.

Progress

can be

expected

in the

analysis, especially

for

detecting

levels of

high

energy which are not based

on the 4

f7 (8S0)

- and 4

f8(7F)

terms.

However,

the location of these levels will be

difficult,

because

in most cases the lines are weak. The total

intensity

of the unclassified lines is about

10 %

of the total

integrated intensity

in the spectrum. From the Gd-

lines

given

in the

NBS’monograph 32-part

1 : Tables

of

spectral-line

intensities

[14]

we classified 1 402 lines out of the total number of

1413,

that is

99 % ;

5 lines

assigned

to Gd II and 6 lines to Gd I remained un-

classified. In respect to

King’s

list

[2],

we remarked

that many of his

assigments

to Gd 1 or Gd II lines

were

incorrect,

some in the lowest

wavelength region

and many in the

highest region.

In the lowest

region

a number of lines which he

assigned

as Gd II lines

belong

to Gd 1 transitions and in the

highest region

vice versa. Out of 2 627 Gd II lines

given by him,

about 800 remained

unclassified,

most of them in

the

wavelength region

less than 3 000

Á.

This confirms

the above mentioned

proposition

that many

high expected

levels can be found.

III. The levels of Gd II. - In Table II we

give

all known odd levels of Gd II in the order

of increasing

energy and in Table III the even ones

(2).

We

give

in column 1 the term value in

cm-1,

column 2 the

J-value and in column 3 the

g-value

rounded off

at 0.005. If the level has a Paschen-Back

effect,

it is

given

in column 4. In the fifth column we

give

the

configuration

to which the level

belongs

and in the

last column the

multiplet.

Here it must be mentioned

that the level values differ somewhat from the values

given

in reference 9. The reason for this difference

has been described

by

Hoekstra and Slooten

[7],

so

we can omit a discussion here. In the same article the reader can find the method for

determining

the

level values to three decimal

places.

The J-values

are without doubt well

established,

because for all levels we determined the

g-value

at least twice.

A more accurate

listing

of the

g-values

than ± 0.005

is without

meaning

because many of the measured patterns are unresolved. In Table IV we

give

the computer output of all transitions of the odd level

TABLE IV

Transitions

of

the level 37

569.5310

J =

11/2

37

596.5310 cm-’

J =

11/2

of the 4

f8(7F)

6 p confi-

guration.

The columns have the same

meaning

as

given

in Table 1

(the

number in the list of the lines

has been

omitted)

except that in the last column

we have

accepted

a

discrepancy of Ao- 1

50

mK,

to include transitions which we had not

accepted

in

our

list ;

in many cases a line has 2

classifications,

and this is the case with the

wavelength 5 212.2104Â

(the

line is broadened

(character 5),

the

discrepancy

is

- 31 mK in this

transition,

and in the other one

it is - 6

mK). Furthermore, King’s

classification

[2]

(1) Th. A. M. van Kleef, Zeeman Laboratorium.

(2) The tables II and III are available to anyone interested at the address : Rédaction du Journal de Physique, 33, rue Croulebarbe, Paris.

(5)

and the measured Zeeman pattern indicate that the line

belongs

to Gd I. We measured two Zeeman patterns at 3 510. 5984

A ;

the first one is in agreement with the transition

given,

the second one

belongs

to

an unknown

transition, probably

a

6p 1/2 - 8G,/2

(accepting negative g-values).

A level is attributed to a

configuration only

when

we are

absolutely

convinced of its

reality.

The same

assumption

is made for the

multiplet assignment.

Of the 11 new odd levels

given by Spector [12], only

two could be confirmed

by

means of Zeeman effect

measurements and

they

are included in Table III.

We remarked that in addition to our

previous publi-

cation

[9],

we located 12 even levels of the 4

f8(7P)

5 d

subconfiguration

and 24 odd levels. The 4

f8(7 F)

5 d

configuration

is

complete.

IV.

Interprétations

of the odd levels. - The lowest

odd levels of Gd II can be derived from the

ground-

state of the

Gd3 + -ion

4

f7 (8S7/2) by adding

a combi-

nation of two

(d

+

s)-electrons.

As the lowest level in Gd IV

(8S°7/2)

is about 32 500 cm-1 below the

next

multiplet (6P° [15], [16]),

we also can expect that

in Gd II the odd levels not based on the

’S07/2

will

be about 32 500 cm-1 above the lowest

multiplet

4 f7(IISO) 5 d 6 s ’OD5/2, 0

We have also identified the

configuration

4

f8

6 p. The lowest

multiplets

in this

configuration

are based on the 4

f8(7F).

In

comparison

with other

spectra

in the lanthanides

[17], [18], [19], [20],

the transitions between

4 f8(7P)

6 s and the

4

f8(7F)

6

p-levels

must be found at about 24 500

cm-1 (4 000 A).

As the lowest state of the 4

f8(7F)

6 s

8F13/2

has been located at 7 992. 268 cm-1

(see § V)

above

the

groundstate

4

f’(8S°)

5 d 6 s

10D5/2’

the lowest

levels of the 4

fl(7 F)

6 p

subconfiguration

can be

expected

about 32 500 cm-1 above the

groundstate, independently

of the

coupling

scheme in the 4 f8 6 p

configuration.

These two facts indicate that many levels will appear at the same energy. This means that

only intensity

rules and not the

g-values give

information about the

assignment

of the

levels,

because both

configurations

contain the same multi-

plets.

In Table V we

give

the lowest

multiplets

of the

lowest odd

configurations

in Gd II. The underlined

multiplets

in the 4

f7

5 d 6 s

configuration

are

expected

TABLE V

« Low

»-expected

odd

multiplets

in Gd II

at the same

height,

as the lowest

multiplets

in

4 f8(7F)

6 p. The

multiplets

derived from the

can be

expected

3 000 cm-1

higher [15], [16].

The

subconfigurations

based on the 4

f 7 8SO)-core.

-

We have determined all levels based on 4

f7(8 S’)

5 d 6 s,

4

f7(8S0) 6 s2

and 4

f7(8S0)

5

d2

and have confirmed the

analysis

of Russell

[1].

All his levels except 1 ° J =

5/2

have been confirmed

by means

of Zeeman

effect measurements. His

20,

and 40 levels were identified as 4 f7 5

d2 8P07/2, 8P9/2

and

6F9/2

respec-

tively.

The other levels

belonging

to the 4

f7 (8S)

5 d2

subconfiguration

were

easily

found

by

us

including

the

high

level 4

f7

5

d2 8S07/2.

The one remarkable

thing

about the 4

f’(8S°)

5

d 2 subconfiguration

is the

large discrepancy

in the

g-values

of the 4 f7 5

d2 ’Do .5/2

and

8G5/2-values,

which are 1.690 and 1.720 respec-

tively.

As the theoretical

g-values

of these levels

predicted

in

LS-coupling

are 2.057 and 1.257 respec-

tively,

and since the calculation in the

coupling

scheme

mentioned elsewhere

[12] gives approximately

these

same results

(a

similar calculation was made in

1969) (see § VI)

- there must be an interaction with

higher

levels of the

multiplets

with the same

L-values,

which

have not yet been detected.

The difference in the sum between the

experimen- tally

determined

g-values

and the theoretical ones

is 0.096

(see

Table

II).

Moreover when we take the

g-sum of all levels with J =

5/2

in the

configurations

4 f’ 5 d 6 s and

4 f7 5 d2

we find

in LS-coupling experimentally

21.086 and 21.050

respectively,

the

difference

being

within our limits of error.

Only

the

fact that the levels

18.00103/2,

18

09505/2

and

18 15007/2

have P. B.

effects,

allows us to maintain the

given interpretations

in

spite

of the

g-values

which suggest the alternative identification.

The

subconfiguration

4

f8(7F)

6 p. This subconfi-

guration

contains 37

levels ;

among the levels

arising

above 32 500

cm-1,

we have ascribed 30 to this

configuration by

means of their strong transitions with the levels based on the 4

f8(7F)

6 s and

4f8(7 F)

5 d

subconfigurations.

As

already

mentioned

(§ II)

the

p-d

transitions have been located in the red and infrared

region. Many

lines in

King’s

list

[2]

which

he attributed to class

V, appeared

to be

just

these

p-d

transitions. This was confirmed

by

Zeeman effect

measurements. Our first

attempt

to

interpret

the

4

f8(7F)

6 p was in the

LS-coupling

scheme

[9],

but

in the course of this work we concluded that the

J-j coupling agreed

much better with

experimental

data.

The

remaining levels,

those not

belonging

to this

configuration,

in the

region

32 500-40 000

cm-1,

and the levels with

higher

energy, have not yet been ascribed to a definite

configuration.

(6)

621

V.

Interprétations

of the even levels. - The low

even

subconfigurations

in Gd II are

4 f8(7F) 6 sand

4

f8(7 F)

5

d,

4

f7(8So)

6 s 6 p and 4

f7(8S0)

5 d 6 p.

All levels of the last two

subconfigurations

were

previously given by

Russell

[1] ; they

were confirmed

by

us and the

experimental g-values

were in

good

agreement with the calculated values

given by

Smith

and

Wybourne [5].

The

interpretation

needs no further

discussion. The first two

subconfigurations

are new.

In the

region

above 38 000 cm-1 there are some levels which do not

belong

to the 4

f7 (8S0)

5 d 6 p

configu-

ration. One

of them,

40 888.843 J =

11/2 g

=

1.310,

has been

interpreted

as

4 f8(5D) 5 d 4G11/2;

the

position

of this level is in very

good

agreement with the calculated value.

THE SUBCONFIGURATION 4

fl(7 F)

6 s. - We have

located the 13 levels

belonging

to the

8F

and 6p

multiplets.

The lowest level

8F 13/2

is 7 992.268

cm-1

above the

groundstate

4

f7(8SO)

5 d 6

s ’ODOS/2.

The

level intervals in both

multiplets

agree

quite

well

with the Landé-interval

rule,

except for the

- and the

’F, 1/2 _ 6F9/2

intervals. In Table VI we

give

the intervals in these

multiplets

and the ratio

This ratio increases

slightly

when J increases from

1/2

to

13/2

in both

multiplets

except for the

13/2-11/2

interval in the

8p,

but

strongly

increases from

9/2

to

11/2

in both

multiplets.

TABLE VI

Levels

of

the 4

f8(7P)

6 s

8F and 6F multiplets

The

possible

reason for this

jump

may be that there is a strong

perturbation

between the levels of these

multiplets

and the levels

belonging

to the 4

f8(5D)

6 s

6,4D multiplets.

The lowest ones which have J =

9/2

and J =

7/2,

were located at 26 351. 767 cm-1 and 27 273.505 cm-1

respectively.

The

experimental g-values

of the

8,6F

levels agree very well with the theoretical

gLs-values. Only

for the levels

having

J =

11/2

in both

configurations

is

Ag (=

gobS -

9cale.) large

in

comparison

with the other

dg’s,

which indi- cates a strong

interaction,

as was confirmed later

by

calculations

(see § VI).

We should

point

out that the

Ag-values

are

negative

for all 8F levels and

positive

for the 6p ones, which is in agreement with the

theory

that when there is an interaction between two levels with the same

J-value,

the

highest g

decreases and the

lowest g

increases.

THE SUBCONFIGURATION 4

f8(7F)

5 d. - This confi-

guration

contains ten

multiplets : 8,"(HGFDP).

All

57

expected

levels are known. In our

previous publi-

cation

[9]

we have

given

a wrong

assignment

to the

levels

belonging

to the 4

f ’(’F)

5 d and 4

f8(5D)

6 s

multiplets respectively. Spector [12]

has

given

a

explanation

of this

misunderstanding.

The fact that the 4

f8(-5D)

6 d

6D9/2

level is lower than the

level

explains why

the total

splitting

of the 4

f8(7F)

6 s

6D

multiplet

is smaller than the

predicted

one

[22],

because of a strong interaction between both multi-

plets [21].

This is contrary to

Spector’s opinion [12].

In

figure

1 we

give

the Grotrian

diagram

for the

even levels of Gd II in the

region

18 000-34 000

cm-1.

It can be seen, that the 4

f 8(’F)

5 d 6D

multiplet

is

(7)

FIG. 1.

irregular

for the interval

6D9/2 - ’D7/2.

The

figure

shows the isolated

position

of the

8(G, F, D, H)

and

6F multiplets.

Most of the other

multiplets

of this

subconfiguration

appear at the same energy as the levels of the 4

f ’(’S’)

6 s 6 p and 4

f7(8S0)

5 d 6 p

configurations.

An interaction between these levels

can be

expected

and is demonstrated

by finding

com-

binations with reasonable

intensity

for transitions between the levels of these

multiplets

and the lowest

odd

multiplets

4

f7 (8S0)

5 d 6

s 10,8,8,6D°

and

The

recently

detected 6H

multiplet

is a

good example.

The

6H15/2

and -

6H13/2

levels which are isolated from the 4 f’

6 s 6 p

and

4 f’ 5 d 6 p

levels with the

same

J-values,

combine

only

with the levels derived from 4 f8 6 p in the infrared

region. They

do not

give

any transition with the levels of the low-odd multi-

plets

mentioned above. The

6H5/2

and

6H7/2

levels

were determined

only

on transitions with the levels of these low

multiplets,

while the

6H9/2

and

6Hll/2

give

weak transitions both with the levels of the low odd

multiplets

and those of the 4

f8

6 p

configuration.

VI. The calculations. - We have

recently

detected

12 levels of the 4

f ’(’F)

5 d

subconfiguration

and have

made a theoretical

study

of this

configuration together

with the 4 f8

(three SD)

6 s terms. Their interaction is very strong and one of us has

recently published [21] ]

the 4

f7(8SO) (5

d + 6

s)2 subconfiguration

in con-

junction

with the 4

f7(6pO) (5

d + 6

s)’ subconfigu-

ration. The results are

given

in Table

VII, together

with the parameters of

The parameters are

given

in the first column

(0153L(L+

1)

takes care of the effect of the operator

aL2) ;

in the

last three

columns,

the values of the radial parameters and the associated standard errors are

given.

When

a parameter has been

assigned

to a value in the last

iteration,

the standard error is

replaced by

« fixed ».

At the end of the table we

give

the mean

coupling

percentage for LS

coupling.

Here :

where

Eo

is the observed term value and

Ec

the cal- culated value of the levels. N is the number of observed levels and p is the number of free parameters used in the calculation. The main

part

of these calculations has been carried out

by

means of four programs

[23]

with the use of the computer UNIVAC 1108 of the Faculté des Sciences

d’Orsay.

(8)

623

TABLE VII

Slater parameters in the

configurations of

Gd II

LE JOURNAL DE PHYSIQUE. - T. 32, 8-9, AOUT-SEPTEMBRE 1971

(9)

TABLE VII

(suite)

In

Spector’s

treatment of the 4

f $(’F)

6 p subcon-

figuration

several levels were misidentified and some

of the J-values were wrong.

Consequently,

we made

a new calculation of this

subconfiguration

both in

LS - and

Jj-coupling.

The

parameters

are

given

in

Table VIII. The calculated values for the 4

f8(7P)

6 p levels are

given

in Table IX

along

with the

predicted positions

and percentage

compositions.

Most of the

levels are

extremely

pure in

J-j coupling,

whereas

only

22 levels have a main L-S component greater than 50

%.

In

comparison

with

Spector’s

treatment

[12]

we have

changed

8 level values out of 28. There is

now a

good

agreement between the calculated and the

experimental level

values.

TABLE VIII

Parameter values

of

the 4

f8

6 p

configuration

Acknowledgements.

- The authors are

grateful

to Dr. P. E. Noorman and Dr. M. Fred for

exposing

the

Gd-plates.

We thank Dr. R. Hoekstra and Mr. Slooten for

measuring

the

wavelengths

in zero

magnetic

field. The CDC-3 200 computer was put at the

disposal

of the Zeeman

laboratory by

the « Stich-

ting

voor Fundamenteel Onderzoek der Materie ».

(*) Spector’s

values

[12].

(10)

625

TABLE IX

Predicted

positions,

percentage

compositions

and calculated values

for

4

f8

6 p

(11)

References

[1] RussELL (H. N.), J. Opt. Soc. Amer., 1950, 40, 550.

[2] KING (A. S.), Astrophys. J., 1943, 97, 323.

[3] BRIX (P.) and LINDENBERGER (K. H.), Z. Physik., 1955,141,1.

[4] ALBERTSON (W. E.), BRUYNES (H.) and HANAU (R.), Phys. Rev., 1940, 57, 292.

[5] SMITH (G.) and WYBOURNE (B. G.), J. Opt. Soc. Amer., 1965, 55, 1278.

[6] DESMARAIS (D.) and PINNINGTON (E. H.), J. Opt.

Soc. Amer., 1967, 57, 1245.

[7] HOEKSTRA

(R.)

and SLOOTEN (R.),

Spectrochim.

Acta, 1971, 26B.

[8] HOEKSTRA (R.), Thesis, Amsterdam, 1969.

[9] BLAISE

(J.)

and VAN KLEEF (Th. A. M.), C. R. Acad.

Sci., 1969, 268, 792.

[10] SPECTOR (N.), J. Opt. Soc. Amer., 1969, 59, 488A.

[11] SPECTOR (N.) and HELD (S.), Astrophys. J., 1970, 159, 1079.

[12] SPECTOR

(N.),

J. Opt. Soc. Amer., 1970, 60, 763.

[13] SPECTOR (N.), J. Physique, 1970, 31, C4-173.

[14] MEGGERS (W.

F.),

CORLISS (Ch. H.) and SCRIBNER

(B. F.), N. B. S. Monograph 32-Part 1, 1961.

[15] CARNALL (W. T.), FIELDS (P. R.) and RAJNAK (K.),

J. Chem. Phys, 1968, 49, 4412 and 1968, 49,

4443.

[16] CASPERS (H. H.), MILLER (S. A.) and RAST (H. E.), Phys. Rev., 1969, 180, 329.

[17] ROSEN (N.), HARRISON (G. R.) and MCNALLY (J. R.), Phys. Rev., 1941, 60, 722.

[18] RUSSELL (H. N.), ALBERTSON

(W.)

and DAVIS (D. N.), Phys. Rev., 1941, 60, 641.

[19] MCNALLY (J. R.) and VAN DER SLUIS (K. L.), J. Opt.

Soc. Amer., 1959, 49, 200.

[20] BLAISE

(J.)

and CAMUS (P.), C. R. Acad. Sci., 1965, 260, 4693.

[21] WYART (J. F.), C. R. Acad. Sci., 1970, 271, 849.

[22] ELLIOTT (J. P.), JUDD (B. R.) and RUNCIMAN (W. A.),

Proc. Roy. Soc., 1957, 240, 509.

[23] BORDARIER (Y.) and CARLIER

(A.),

Programme

AGENAC de calcul de formules suivant l’algèbre

de Racah ; BORDARIER (Y.), Programme ASSAC

de regroupement des résultats d’AGENAC.

BORDARIER

(Y.),

and DAGOURY

(P.),

Programme

DIAGAC de diagonalisation et de calcul de dérivées des énergies et des g, Orsay, 1968 ;

BORDARIER (Y.), Programme GRAMAC d’opti-

misation des paramètres par moindres carrés, Brochure en préparation.

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