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HAL Id: jpa-00206761

https://hal.archives-ouvertes.fr/jpa-00206761

Submitted on 1 Jan 1969

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Coefficients of fractional parentage and LL-coupling

B.G. Wybourne

To cite this version:

B.G. Wybourne. Coefficients of fractional parentage and LL-coupling. Journal de Physique, 1969, 30

(1), pp.35-38. �10.1051/jphys:0196900300103500�. �jpa-00206761�

(2)

COEFFICIENTS

OF FRACTIONAL PARENTAGE AND LL-COUPLING

(1)

Par B. G. WYBOURNE

(2),

Laboratoire Aimé-Cotton, C.N.R.S. and Faculté des Sciences, Orsay, Essonne

and Physics Department, University of Canterbury, Christchurch, New Zealand.

(Reçu

le 1 er avril

1968.)

Résumé. 2014 Les coefficients de

parenté

fractionnelle nécessaires aux calculs en

couplage

LL

des

configurations

d’électrons

équivalents d

et f sont obtenus directement à

partir

des tables

disponibles

de coefficients de

parenté

fractionnelle en

couplage

LS. Les résultats

complets

sont tabulés pour les deux types de

configurations.

Les détails

pratiques

des calculs en

couplage

LL ont été considérés.

Abstract. 2014 The coefficients of fractional parentage

required

for

making computations

in the

LL-coupling

scheme for

equivalent

electron

configurations

of d and f electrons are

shown to be

directly

derivable from

existing

tabulations of coefficients of fractional

parentage

in the

LS-coupling

scheme.

Complete

results are tabulated for both

configurations.

Practical

details of

making

calculations in the

LL-coupling

scheme are considered.

LE J OURN AL PHYSIQUE 30, JANVIER 1969,

1. Introduction. -

Judd [1]

has

recently

shown

that atomic calculations can sometimes be substan-

tially simplified by considering

two spaces, one

(the

A

space)

in which all the

spins

are

"up"

and the

other

(the

B

space)

in which

they

all are "down".

Mathematically,

this amounts to

representing

the pro- duct

[ 1 /2] [1]

as

([J] A

+

[J]B)

where

[1] A corresponds

to the orbital functions in

"spin up space"

and

[1] B

to

the set in

"spin

down

space".

The wave functions thus span the

representation ([IJA

+

[1] B)

of the

imprimi-

tive rotation group in two sets of variables

[2].

The

plethysm appropriate

to the

n-particle configu-

ration may be

expanded

to

yield [3] :

The S-functions

[4] {I n}, {1 rx}

and

{ ln-,, I

may be taken as

labelling

the

antisymmetric representa-

tions of the

unitary

groups

L+ U2 +1

and

UB respectively

where :

(1)

Research

sponsored

in

part by

the Air Force Office of Scientific Research, Office of

Aerospace

Re- search, United States Air Force, under A.F.O.S.R.

Grant No 1275-67.

(2)

This work was done in

part

while the author was a

visiting

Professor with Laboratoire Aim6-Cotton, under

the

sponsorship

of D.G.R.S.T.

The

description

of the

n-particle

states is extended

by making

the

decompositions :

The states of the In

configurations (I 3)

may then be

uniquely

labelled

by

the sequence :

where

[1 X]

and

[1 Y]

label the irreducible representa- tions of

R’,l

and

RB+1 respectively

and if oc

1,

directly

from Newell’s

[5]

modification rules for ortho-

gonal

groups.

The

representations {1} and f ln-o, I

remain irre-

ducible upon restriction of the

unitary

group to the

orthogonal

group

and, hence,

the

symbols [1"]

and

[1 Y]

in eq.

(4) give

no additional classification of the states.

They

are,

however,

retained to make the

correspondence

with other classification schemes more

transparent.

The

opposition

of the

spins

in the two spaces, A and

B,

means that we need

only

ensure that the

Pauli exclusion

principe

is satisfied in each space

separately and, then, couple

the

antisymmetrized

orbital states of these two spaces

by

the usual

angular

momentum

coupling techniques

to be assured that the resultant

eigenfunctions

are

totally antisymmetric

with respect to both the orbital and

spin

functions.

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:0196900300103500

(3)

36

In this respect, the

problem

of

constructing antisym-

metric

eigenfunctions

in

LL-coupling

is

entirely

ana-

logous

to that of

constructing antisymmetric eigen-

functions in

J J-coupling [6].

As such we expect the

problem

of

constructing

coefficients of fractional parentage

(c.f.p.)

for

LL-coupled

states to be substan-

tially simpler

than that

required

for

LS-coupled

states

[7, 8].

In this paper, we shall first show how the

c.f.p.

may be

simply

constructed and

give

the results for dn and

f n configurations.

We shall then

briefly

discuss

their

application

to the calculation of the

off-diagonal

matrix elements of the

spin-orbit

interaction.

2. Construction of coefficients of fractional paren-

tage.

- In

LL-coupling

we need

only

construct

c.f.p.

for the states of the

subconfigurations :

The same set of

c.f.p.

may be used for calculations in the A and B spaces and hence we shall limit our

discussion to the A space

c.f.p.

In the formulas that follow the A

subscripts

will be omitted.

A

typical state I {I rx} [111] LML > may be

repre- sented as a linear combination of states formed

by coupling

the

eigenfunction

of the a-th

particle

to

those of the

(a 2013 1) LL-coupled particles by writing :

where the

symbols i

and "t’ have been introduced to serve as

auxiliary

labels for

distinguishing

states

having

the same set of

question

numbers. The coeffi- cients of this linear combination may be factored

using

a theorem due to Racah

[7]

to

give :

The first factor on the

right

in the usual Clebsch- Gordan coefficient which the second factor is the

c.f.p.

The

c.f.p.

may be further factored to

give :

Since the

c.f.p.

must form an orthonomal set we are at

liberty

to choose for the first factor the value

x-l ex-2

(- 1)

2 for rJv odd and

(- 1) s

for x even. This

somewhat bizarre choice is made to retain a close

relationship

with the

corresponding phase

choice

made

by

Racah for

LS-coupling c.f.p.

Thus,

in

LL-coupling

the

c.f.p.

may be taken as

just :

where we have

suppressed

the

symbols ( I ) [1]

asso-

However,

the

right-hand-side

of eq.

(9)

is identical

to the

corresponding

factor that arises in the

c.f.p.

for

states of maximum

multiplicity

in

LS-coupling [7, 8]

and hence the

c.f.p

for

LL-coupled

states of dn and

f n

may be deduced

directly

from known results.

3.

LL-coupling c.f.p.

for dn

configurations.

-

Applying

eq.

(9)

to the case of

equivalent

d-electrons leads

immediately

to the results :

Using

the results

given by

Racah

[7]

to obtain the

right-hand-side

of the above

equations gives directly

the results of table I.

TABLE I

(4)

4.

LL-coupling c.f.p.

for

f n configurations.

-

Applying

eq.

(9)

to the case of

equivalent f-electrons

leads to the results :

The

right-hand-side

of these

equations

may be

readily

evaluated from the known tables

of ( W U

+

f ) I wu >

and (

UL -)-

f I UL >

as

given,

for

example, by Judd [8].

The results are

presented

in table II.

5. Calculations in the

LL-coupling

scheme. -

Judd [1]

has discussed the calculation of the

diagonal

matrix elements for a number of interactions. In these cases, it is

possible

to make the calculations

entirely

in terms of the known

LS-coupling

matrix

elements for states of maximum

multiplicity

without

using

the

LL-coupling c.f.p. However,

calculations of the

off-diagonal

matrix elements of interactions that do not commute with the

angular

momentum

operators

L2, LZ,

or

SZ usually require LL-coupling c.f.p.

We shall restrict our discussion to the calcula- tion of the

off-diagonal spin-orbit

interaction matrix elements.

The

diagonal

matrix elements of the

spin-orbit

interaction involve

just

the

components Es,il,,i

of

i

the scalar

product £ (si li)

while the

off-diagonal

2

matrix elements involve the components :

where

Wil!i

and

Wlli

are

components

of the double

tensor operator W(1I) as defined

by Judd [8]. Equa-

TABLE II

(5)

38

tion

(10),

as it

stands,

is not in a suitable form for

calculating

matrix elements of the

spin-orbit

interac-

tion with

LL-coupled

states. The calculation becomes very

simple

if the

components

of the

operator

W(Il,

are

expressed

in terms of

coupled products

of the

creation and annihilation

operators a+

and

ba

defined

in Judd’s

paper

[1], leading

to the final result :

Alternatively,

the above result may be derived

using

conventional

recoupling techniques.

As a

simple example

of the

application

of the above

formula to find an

off-diagonal spin-orbit

matrix

element in the

LL-coupling

scheme we have :

Equation (11)

has the appearance of

being

substan-

tially simpler

than the

corresponding expression

for

the

spin-orbit

interaction matrix element with

LS-coupled

states..

Notably,

there is no summation

over

c.f.p., only

a

simple product.

The

advantages

of

LL-coupling

for

practical

calculations are however

largely illusory

since while the calculation of individual matrix elements is

substantially simpler

in

LL-coupling

the number of matrix elements

required

is

vastly

greater since while in

LS-coupling

the

spin-orbit

interaction commutes with J2 and

I z, allowing

us to

label the matrices with the

quantum

numbers

JMJ

in

LL-coupling

we are

only

left with

MJ

to label

the matrices.

One noticeable

computational advantage

of the

LL-coupling

scheme is the compactness of the table of

c.f.p.

For

example,

Nielson and Koster

[10]

list 211

c.f.p.

for the

LS-coupled

states of dn whereas in

LL-coupling only

9

c.£ p.

are

required.

Even more

dramatic reductions occur in

fn and configurations.

However,

the same reductions in size of the

c.f.p.

tables can be obtained in the

JJ-coupling

scheme

which has the

advantage of requiring

the construction of matrices that can be characterized

by J

and of

being

the natural scheme for the

study

of relativistic effects.

REFERENCES AND FOOTNOTES

[1] JUDD (B. R.),

Phys. Rev., 1967, 162, 28.

[2]

LITTLEWOOD

(D. E.),

Proc. Lond. Math. Soc.

(3),

1956, 6, 251.

[3]

SMITH

(P. R.)

and WYBOURNE

(B. G.), J.

Math.

Phys.,

1968, 9, 1040.

[4]

LITTLEWOOD

(D. E.),

The

Theory

of

Group

Charac- ters, 2nd Edition, 1950, Oxford

University

Press, London.

[5]

NEWELL

(M. J.),

Proc. Roy. Irish Acad., 1951, A 54, 153.

[6]

DE SHALIT

(A.)

and TALMI

(I.),

Nuclear Shell

Theory,

1963, Academic Press, Inc., New York.

[7] RACAH

(G.), Group Theory

and

Spectroscopy,

1965,

Springer-Verlag,

Berlin.

[8]

JUDD

(B. R.), Operator Techniques

in Atomic

Spectroscopy,

1963, McGraw-Hill Book Co., Inc., New York.

[9] JUDD (B. R.),

Second

Quantization

and Atomic

Spectroscopy,

1967, The

Johns Hopkins

Press, Baltimore.

[10]

NIELSON

(C. W.)

and KOSTER

(G. F.), Spectroscopic

Coefficients for the pn, dn and fn

Configurations,

1963, The M.I.T. Press, Massachusetts Institute of

Technology, Cambridge.

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