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On the use of Liouville relaxation supermatrices in Mössbauer studies

F. Hartmann-Boutron, D. Spanjaard

To cite this version:

F. Hartmann-Boutron, D. Spanjaard. On the use of Liouville relaxation supermatrices in Mössbauer

studies. Journal de Physique, 1975, 36 (4), pp.307-314. �10.1051/jphys:01975003604030700�. �jpa-

00208255�

(2)

ON THE USE OF LIOUVILLE RELAXATION

SUPERMATRICES IN MÖSSBAUER STUDIES

F. HARTMANN-BOUTRON and D. SPANJAARD

Laboratoire de

Physique

des

Solides,

Université

Paris-Sud,

91405

Orsay,

France

(Reçu

le 22 novembre

1974)

Résumé. 2014 Dans une publication antérieure

(F.

Gonzalez-Jimenez, P. Imbert et F. Hartmann- Boutron, Phys. Rev. B 9 (1974),

95),

nous avions exprimé la forme de raie Mössbauer en présence

de relaxation, en fonction d’une certaine supermatrice de relaxation R. Dans le présent article,

nous établissons une expression rigoureuse de R qui est valable quelle que soit la température, et

nous relions R à la supermatrice de relaxation S qui caractérise la relaxation de la matrice densité 03C3 de l’atome radioactif. Nous examinons ensuite le problème général des moyennes sur le réseau dans le calcul des effets de relaxation thermique, et à titre d’exemple nous établissons l’expression de

la forme de raie Mössbauer d’un émetteur.

Abstract. 2014 In a previous paper

(F.

Gonzalez-Jimenez, P. Imbert and F. Hartmann-Boutron, Phys. Rev. B 9

(1974), 95),

we have related the Mössbauer spectrum in the presence of relaxation to

a certain relaxation supermatrix R. In this paper we derive a rigourous expression of R which is

valid at arbitrary temperatures and we relate it to the relaxation supermatrix S which characterizes the relaxation of the density matrix 03C3 of the radioactive atom. We then discuss the

general problem

of lattice

averaging

in the computation of relaxation effects and as an illustration, we derive the expression for the Mössbauer lineshape of an emitter.

Classification Physics Abstracts

4.200 - 8.610 - 8.680

Introduction. - In this paper, we want to revise

slightly

one of the results of ref.

[1]

i. e : the definition

of the relaxation

supermatrix R

associated with

M,

which comes into

play

in eq.

(16)

and

(23)

of

[1] and

whose elements are defined

by

footnote

(7)

of

[1].

We will show here that the

supermatrix R

must be

the

transposed

matrix of the relaxation

supermatrix S

associated with the

density

matrix 6 of the radioactive atom.

Explicit expressions

of S and R are then derived and are

compared

with the results

of previous

theories.

Finally,

in view of future

applications

to Môssbauer

transmission and

scattering

we

give

some

general

rules for

performing

lattice averages in relaxation

problems.

1. Liouville évolution

superoperators

for an isolated

atom without relaxation. - Let us first assume that

we have an isolated atom described

by

a

complete

orthonormal set of

functions 1 a ), 1 b ), 1 c), 1 d)

and whose evolution is

govemed by

a hamiltonian

Jeo [1].

The relevant evolution operator

Uo(t)

is :

In terms of this operator the time

dependence

of the

density

matrix a of this atom in the

Schrôdinger

representation

is :

with :

where Xxo

is the Liouville superoperator

[1]

asso-

ciated with the hamiltonian

Ho.

On the other

hand,

in the

Heisenberg representation

the time

dependence

of an atomic

observable Q

is :

with :

In

explicit

form :

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01975003604030700

(3)

308

From this it follows that :

i. e. the Liouville matrix associated with

°’11o(t)

is the

complex conjugate

of the

transposed

matrix of the

Liouville matrix

corresponding

to

CU o(t).

2. Standard treatment of relaxation. - We must now consider the case where the atom is

coupled

to a quantum bath

by

a relaxation hamiltonian

H1,

the hamiltonian of the bath and its

eigenstates being

denoted

respectively by XB

and

by 1 r >, 1 r’ >.

The standard

approach

to relaxation effects

[2, 3]

consists in

calculating

the relaxation of the

density

matrix u of the atom. For

this,

one first derives the

equation

of motion of the total

density

matrix 0 of the atom

plus

the bath in the interaction

representa-

tion

[3].

Let us define :

The

equation

of evolution of 0* is :

This

equation

is

integrated by

successive

approxi-

mations

([2] chap.

VIII eq.

(32)

and

(60)) :

It is then admitted that since the heat

capacity

of the

lattice is very

large,

the

density

matrix 0 can be facto-

rized as :

where po is the Boltzmann

density

matrix of the lattice.

Further

approximations

which are discussed

by Abragam ([2] chap.

VIII p.

276) finally

lead to the

well-known master

equation :

We must now translate these results into terms for the evolution

superoperators.

3. General

properties

of the évolution superoperators in the présence of relaxation. - From the total hamil- tonian of the system atom + bath

we can construct the evolution

operator :

In order to transform to the interaction

representation

one may write

[4] :

-

Il - il 1 - 1

with :

and U’

being

the solution of the

equation :

In terms of U the evolution of the total

density

matrix 0 is :

or

alternatively

in thé interaction

representation :

This

equation

is

equivalent

to eq.

(12) (see

also

[2]

chap.

VIII eq.

(30)).

We may therefore

perform

the

factorization of 0* and then take the average over the lattice variables. We obtain :

or, after

going

back to the normal

representation :

(this equation

could also be obtained

by performing

the factorization of 0

directly

in eq.

(19)

but we find

this method less

convincing).

We shall define

’BJ(t) by :

’BJ(t)

will be the evolution superoperator of J in the presence of relaxation.

Eq. (23) gives

us an

expression

of

V(t)

in the form of a lattice average.

On the other hand in the interaction

representation,

the average value of an atomic

variable Q

is :

(4)

which,

after

using

eq.

(21)

and the invariance of the trace under circular

permutation

may be cast into the form :

In the normal

representation

we also have that :

(28)

with :

We shall define :

flL(t) being given by

eq.

(29). Using

this

equation

and eq.

(23)

in

explicit

form it is easy to show

(by rearrangement

of the lattice

indices)

that :

which is identical to the relation

(8) already

derived

in the absence of relaxation.

As is well known the

general

solution of the eq.

(14)

of evolution of the

density

matrix has the

form,

in the

normal

representation :

S

being

a relaxation matrix which will be

specified

below. It follows that :

and,

after relation

(31) :

where R is the

transposed supermatrix

of the

(real) supermatrix S :

Notice that once S or R has been

determined,

we may

compute

the

properties

of the atom as if there were

no

lattice ; simply we

must

everywhere replace ctto(t)

and

’U o(t) by flL(t)

and

’U(t) (details

of the

procedure

are

given

in

Appendix I).

In other words the

practical

effect of relaxation is to add a

dissipative

term to the atomic Liouville hamil- tonian.

It is also worthwhile

mentioning

that if 6 = UB, Boltzmann

density

matrix

corresponding

to

Jeo,

we

have the

identity :

We shall now

apply

these results to the case consi- dered in ref.

[1].

4.

Application

to relaxation effects in Môssbauer spectra

[1] [6].

- Let us consider a Môssbauer emit- ter with a Môssbauer excited state 1 and

corresponding

electronuclear

kets 1 f >

and with a Môssbauer

ground

state

Ig

and

corresponding kets 1 g ).

In the

Appendix

of

[5]

we have

computed

the

Môssbauer

intensity I(cv)

emitted

by

a

powder

source, under the

assumption

that state 1 is fed

by

a radio-

active transition from an upper nuclear state

I;.

This

was achieved

by

first

performing

a

complete

calcula-

tion of the radioactive cascade in the interaction

representation

with

respect

to the radiative

coupling

and then

going

back to the

Schrôdinger

represen- tation. The final result of the calculation is repre- sented

by

eq.

(AI)

of

[5].

The formula relative to

a

powder

source is

readily

deduced from this equa- tion

by averaging

over

02

CP2

(which

introduces

a Kronecker

symbol bM2M2 ).

Let us first consider the case where there is no

relaxation. Then

[5] :

where T is the inverse nuclear

lifetime,

M is the nuclear electric or

magnetic multipole

moment which induces the Môssbauer

transition,

and

o1n(t")

is the

density

matrix of state I

just

after

feeding by

radioactive

decay

of the upper state

I;

at time t"

(in practice

it is inde-

pendent

of

t").

Let us set : t’ = t - i’ and t" = t’ - 7:".’ Then :

or in compact form :

where we have introduced the operators :

(5)

310

Let us now write the trace in eq.

(37)

in

explicit

form

before

introducing

the Liouville evolution super- operators :

After the definition of

Vo,

eq.

(6),

the bracket is

equal

to :

Let us now introduce relaxation. In the

preceding paragraph

we have shown that in the presence of relaxation

vo

must be

replaced by v.

After substi-

tuting

eq.

(33)

into

(43), using

eq.

(31)

and

(34),

report-

ing

into

(42)

and

performing

the double time

integral

we

finally

obtain :

i. e. eq.

(9)

of ref.

[6].

In the case where the

temperature

is

high compared

to the level

spacing

in the excited Môssbauer state, its

density

matrix remains

always equal

to the unit

matrix and the second

parenthesis

may be

replaced by ôfl f3

We then obtain the

expression

for the

high

temperature spectrum :

This

expression

was

already

derived in ref.

[1]

but the

supermatrix R

as defined in footnote

(7)

of this refe-

rence was in

reality S

and not

ST

as it

ought

to be

(notice

however that at

high temperature S = ST

= R

and that this condition is fulfilled in the

practical example

worked out in ref.

[1]).

Our error arose from

the fact that we calculated

directly

the relaxation of

pM

instead of

proceeding

to a full

analysis

of the

problem.

Let us now consider the structure of the relaxation matrices S and R. Let 6 be the

density

matrix for the total set of states associated with both the excited and the

ground

nuclear states 1 and

Ig.

In terms of

projection operators Pl

and

PIs

one may write :

The evolution

operator U,

eq.

(15),

which does not contain radiative

couplings (see

the definition

of Jeo

in

[1 ])

has no matrix element8 between 1 and

Ig.

There-

fore

by

virtue of eq.

(23)

each of the matrices in the R.H.S. of eq.

(46)

is

coupled only

with itself. Conse-

quently,

the relaxation

supermatrix

S factorizes into the submatrices :

The

physical meaning

of

ull

and

(II 1 S II)

is obvious.

These are the

density

matrix of state 1 and the associated relaxation matrix. As concerns

uIlg

it is

usually

zero but it becomes

temporarily

excited

during

the émission of the y ray, since the two nuclear states 1 and

Ig

are

coupled by

the transition operator M. The relaxation matrix which characterizes the relaxation of M is

clearly :

Consequently

in the first

parenthesis

of eq.

(44)

R

reduces to the submatrix

(Ig 1 1 su 1 Ig I)

while in the

second

parenthesis, S

reduces to

(II 1 s II).

Let us now

give

the

explicit expression

for S. We

assume that JC1 has the same form and

properties

as

in ref.

[1] :

:

a 1 = L Kq

F4.

Starting

from eq.

(14)

q

one

expands

the double commutator and introduces lattice correlation functions :

where :

,

Finally

when all calculations are

completed,

it

turns out that the

equation

of evolution of a has the form of eq.

(32)

with a relaxation

supermatrix S given

by :

(6)

Notice that if we associate with

Jet

a Liouville ope- rator

(JC*)’, Sd,&-

can also be obtained from the for- mula :

1

where r,

r’,

rl, r2 represent the

degrees

of freedom of the lattice.

We have demonstrated above that the relaxation matrix R relative

to Q

is the

transposed

matrix of S.

Using

this

result,

let us calculate the relaxation

equation of Q

in the case where

Q only

has

diagonal

matrix elements :

This

equation

shows that in this case the sum of the elements of a row of R is zero.

This result is

satisfactory

in connection with a

problem

which we have been

considering recently,

that of the Môssbauer

lineshape

of an

Yb170

trivalent

ion in the presence of relaxation between two electro- nic Kramers doublets

[7].

If we assume that the

hyper-

fine structure in each doublet is

completely

anisotro-

pic,

of the type

Alz Sz

+

P(3 I’ - I(I

+

1)), (this being

an

example

of a

diagonal Q),

our

approach

to the

problem

should be

equivalent

to the old sto-

chastic

approach [8].

This means that the relaxation matrix R must reduce to a Markov matrix. But an

essential

property

of such a matrix is that the sum of the elements of one row is zero. As an

example,

when

the

system jumps

between two

frequencies

which

are not

equally probable :

This is how we discovered that one should have R =

ST..

5.

Comparison

with Hirst’s relaxation

équation

and

Môssbauer

lineshape.

- It is worth

mentioning

that

the value of R which can bè deduced from eq.

(51), (35)

is still different from that associated with the eq.

(4)

of Hirst’s

Paper [9].

Indeed

using

eq.

(30), (34), (35), (51)

of the

present

paper it is

possible

to show that the

equation

of motion

of an

operator

M in the normal

representation

is :

In our

opinion

the reason for the differences between this

equation

and Hirst’s

equation (which

are espe-

cially appearant

in the correlation functions of the first and fourth relaxation

terms)

is the

following.

As a function

of H*(t)

the evolution operator U’

in the interaction

représentation

is

given by :

The exact

expression

for the derivative of 7* in the interaction

representation

is

(see

eq.

(21)) :

where in the

expression

of

U’,

to = 0.

The master eq.

(14)

for Q* amounts to

approximat- ing

this

equation by :

where now to = - oo .

Let us use the same

approximation

to derive an

equation

of motion for

Q *(t)

from eq.

(27) :

(7)

312

Upon substituting expression (56)

of U’ in this equa- tion we arrive at

(up

to second order in

H1*) :

Notice that this

equation

differs from the relaxation eq.

(14)

for 6* both

by

the

position

of po and

by

the

order

of Je!(t - i) and Je!(t)

in the double commuta-

tor. This is due to

the’

fact that in

passing

from U’

to U’t the two time arguments t1

and t2

in the double

time

integral of eq. (56)

are inverted. It may be checked that the eq.

(60)

leads to a relaxation matrix R which is indeed

equal

to

ST.

A further check is the

following.

Let us start from

the

equation

derived from eq.

(12) by

factorisation of the

density

matrix

0,

and

drop

the term linear

in H*1

which we know would

disappear

at the end of

calculation. Then :

Let us consider

(by

definition of

Q *,

see eq.

(27) ; Q *(0)

=

Q).

After

rearrangement

of the trace this becomes :

or

altematively

after

performing

the standard

approximations :

in

complete

agreement with eq.

(60) (compare

with

ref.

[2] chap. VIII,

eq.

(44)).

On the other hand

according

to this author

[10],

Hirst’s eq.

(3)

must

be interpreted

as :

For a quantum bath eq.

(60)

and

(66)

are

clearly

different

(since [Po, Je1] =1 0)

and this is the reason

for the

discrepancy.

Notice that Hirst’s eq.

(3)

is what

is obtained

by using

the method of successive

approxi-

mations in the same way as for the

density matrix,

in order to solve an

equation

of the type :

Our results

clearly

indicate that in the case of M*

this method leads to an incorrect

handling

of the time

variables,

i. e. the past and the future are inverted.

Incidentally

this conclusion is in

agreement

with a remark formulated more than twenty years ago

by

Gell-Mann and

Goldberger ([12]

eq.

(3.13)

and

(3.14)).

As a final

remark,

let us also mention that eq.

(8)

of Hirst

[9]

for the Môssbauer

lineshape

is

only

valid

for emission from a

stationary

excited state.

Indeed,

it is

clearly

stated in the text of

[9]

that the row vec-

tor W which enters into the

expression

for

G(t)

p. 660 is time

independent,

all the evolution in the excited state

being

included in the

quantity M(t).

In

reality,

formulae like eq.

(8)

of

[9]

are well

adapted

to the

description

of slow passage

lineshapes

in NMR or of

light absorption

from an atomic

ground

state. But as

shown

by comparison

with our own results eq.

(39)

and

(44) they

cannot describe radiation emission from

a transient excited state in a

cascade,

unless Boltzmann

equilibrium

in this state is achieved before emission

(in

which case

6(1/T )

in eq.

(39)

can be

replaced by

the

Boltzmann

density

matrix of level

I).

As a further

proof,

let us recall that in

[5]

we have checked that

by integration

of eq.

(A .1 )

over 0153, we did recover the

expression

for the Nuclear Orientation

signal (eq. (A. 3))

as we

ought

to. In cascades

involving

, transient states, this N.0

signal

is a direct measure-

(8)

ment of the

quantity u(1/r),

whose value

depends

on

relaxation effects in this state. The nuclear

Korringa

relaxation time of

Ag109

in Fe at very low

temperatures

has

already

been determined

by

this method several years ago

[13].

Note added in

proof.

- Notice that while Hirst’s formulas involve

only

one

time,

Blume has derived

an

expression

for the Môssbauer

lineshape

which

contains an

integration

over two times

([14]

eq.

(4)).

We have been able to show that this last

expression

is

exactly equivalent

to our

equations (37)-(39).

We

thank Dr. Blume for

calling

our attention to his

work.

6. Conclusion. - In conclusion we feel that we have elaborated a consistent

description

of relaxation

phenomena

within the frame of the Liouville forma- lism. The main results of this paper are

represented by

eq.

(33), (34), (35).

APPENDIX 1

We have demonstrated in the main text that

(for t > 0) :

and

These results show us how to

compute

lattice averages

involving

two operators U and Ut whose

positions

relative to po are

Up.

U t

(and

circular

permutations).

Now we have

(for t

> to >

0) :

On the other

hand,

after eq.

(33) :

This

gives

us a rule for

taking

the lattice average of

products

of

operators

U and ut of the type :

and also of more

general products :

where

A, B, C,

D are atomic

operators.

As an

example :

Let us stress that this

breaking

of the lattice average is made

possible

both

by

the fact that eq.

(A. 5)

contains successive ordered time intervals which are

long compared

to the memory of the

lattice,

and

by

the

exponential

form of

V(t),

eq.

(A. 3).

Let us now

apply

these results to the

computation

of atomic observables. In the absence of

relaxation,

a

physical

atomic observable is a trace over

atomic

variables of a

product :

In the presence of

relaxation,

one must

replace Uo by U, r(0) by 0(0)

and the trace must involve both atomic and lattice variables. 0 is then factorized as

po Q,

leading

to a lattice average over a

product

like

eq. (A. 5).

The standard method for

computing

the

properties

of the atom in the presence of relaxation should therefore be the

following :

1) Ignore

relaxation and express the atomic quan-

tity

of interest as a trace over a

product of operators Uo, Uô

and u

(plus possibly

inserted atomic

operators).

2) Rearrange

the trace in such a way that all the

Uo

be on the left of 6 and all the

on the

right,

with

positive

time arguments

(corresponding

to

integration variables)

ordered in the same way as in eq.

(A. 5).

While

performing

the

rearrangement,

one may use transient

Ui

s with

negative arguments.

3)

Write the trace in

explicit form,

relate the matrix elements of the

UO, UJ

to

Liouville operators Vo.

Finally,

make the substitution

’BJo -->

9Y. This is how eq.

(43)

was derived in the main text.

(9)

314

APPENDIX II

As shown

by

this paper, one must be very careful in

deriving expressions

for the Môssbauer

lineshape, although

at first

sight

the

position

and

sign

of the time argument in the correlation function of M would seem

of little

importance,

since one looks at the real part

of a

complex

number. A

complete analysis

of the

emission process led us to the exact

expression (eq. (39)) :

Strickly speaking

this

expression

is different from eq.

(5) of [1]

and from eq.

(8) of [6]

and should

replace

these

equations.

As concems ref.

[6],

eq.

(9)

of this

paper as well as

subsequent equations

were derived

from the correct

equation (7)

and are therefore correct.

Eq. (1)

of

[6]

is also correct.

On the contrary, eq.

(15)

of ref.

[1]

differs from eq.

(45)

of the present paper in that the order

of f and g

in the Liouville kets is inverted

(this

has the effect of

changing

the

signs

of the

energies). However,

in eq.

(72)

of

[1]

there was an

interchange of f and g

in

going

from the left hand side to the

right

hand side.

It follows that all

equations following

eq.

(72)

are

entirely

correct. Notice that eq.

(45)

of the present paper agrees with eq.

(27)

of Clauser and Blume

[11].

References

[1] GONZALEZ-JIMENEZ, F., IMBERT, P., HARTMANN-BOUTRON, F., Phys. Rev. B 9 (1974) 95.

[2] ABRAGAM, A., The principles of Nuclear Magnetism (Oxford University Press) 1961, Chap. VIII.

[3] WANGSNESS, R. K., BLOCH, F., Phys. Rev. 89 (1953) 728.

[4] MESSIAH, A., Mécanique Quantique, tome I (Dunod) 1962, Chap. VIII, § 14.

[5] HARTMANN-BOUTRON, F., SPANJAARD, D., J. Physique 33 (1972) 285.

[6] HARTMANN-BOUTRON, F., Phys. Rev. B 10 (1974) 2113.

[7] CHOPIN, C., HARTMANN-BOUTRON, F., SPANJAARD, D., Communication to the International Conference on the

Applications of the Mössbauer Effect. Bendor (France)

Sept. 1974, to be published in J. Physique Colloq. 35

(1974) C 6-433.

[8] See Chap. X of ref. [2], eq. (53), p. 448.

[9] HIRST, L. L., J. Phys. & Chem. Solids 31 (1970) 655. According

to the author, in eq. (4) of the article the frequency argu- ments of the four spectral densities should be reversed.

In

addition Jq

should be replaced by J-q in the last two

terms (HIRST, L. L., private communication).

[10] HIRST, L. L., private communication.

[11] CLAUSER, M. J., BLUME, M., Phys. Rev. B 3 (1971) 583.

[12] GELL-MANN, M., GOLDBERGER, M. L., Phys. Rev. 91 (1953) 398.

[13] STONE, N. J., FOX, R. A., HARTMANN-BOUTRON, F., SPANJAARD, D., J. Physique Colloq. 32 (1971) C 1-897.

[14] BLUME, M., Hyperfine structure and nuclear radiations, Eds.

E. Matthias, D. A. Shirley (North Holland) 1968, p. 911.

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