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Study of the saturation of a multilevel spin system : Mn++ in Zns

C. Blanchard, A. Deville, B. Gaillard

To cite this version:

C. Blanchard, A. Deville, B. Gaillard. Study of the saturation of a multilevel spin system : Mn++

in Zns. Journal de Physique, 1976, 37 (12), pp.1475-1481. �10.1051/jphys:0197600370120147500�.

�jpa-00208550�

(2)

Centre de

Saint-Jérôme,

13397

Marseille,

Cedex

4,

France

(Reçu

le

29 juin 1976, accepté

le 23 aofit

1976

Résumé. 2014 Aux basses températures, les raies de structure fine et hyperfine de Mn2+ dans ZnS

sont

couplées

par diffusion. On a étudié la saturation continue d’une raie à deux températures

2014

4,2 et 39 K - encadrant la température caractéristique pour laquelle les temps de relaxation et de diffusion sont égaux (20 K). On a d’autre part observé à 1,34 K une anomalie dans la loi de saturation, qui ne peut être due à une accumulation des phonons résonnants. On a mis en évidence un raccour-

cissement de T1 avec la puissance incidente.

Abstract. 2014 At low temperature the fine and hyperfine structure lines of Mn2+ in ZnS are

coupled

by diffusion. Continuous saturation of one line was studied at two temperatures 2014 4.2 and 39 K 2014 above and below the characteristic temperature for which relaxation and diffusion times are

equal (20 K). Moreover at 1.34 K, an anomalous behaviour of the saturation law was observed which cannot be due to an accumulation of resonant phonons. A reduction of T1 with incident power has been observed.

1. Introduction. - In

previous

paper

[1, 2],

we

described

pulse

saturation

experiments

on the multi-

level system

Mn"

in cubic ZnS

(I

=

5/2, S

=

5/2).

We showed the

existence,

at low

temperatures (T

20

K),

of

spectral

diffusion with characteristic time

TD (TD

= 0.5

ms).

The width of the saturated line which has to be considered for continuous satu- ration measurements should be

quite

different

depend- ing

on whether the bath temperature is greater or lower than that for which the relaxation time

T,

is

equal

to

TD.

In section

2,

we

present

and

interpret

the measu-

rements made at 4.2 K and 39

K,

where

T1

= 0.28 s

and 8 x

10-’

s

respectively (pulse experiments [1]).

We do not make the usual but unrealistic treatment where all relaxation

probabilities

are

equal.

We show

how to relate the time deduced from continuous saturation

experiments

to that measured in

pulse experiments

when

Tl

>

TD.

In section

3,

we discuss the anomalous behaviour of the

saturating

process under strong r.f. field for low temperature

( T

= 1.34

K).

This behaviour cannot be attributed to an accumulation of resonant

phonons.

In order to know whether

T1

is r.f. power

dependent,

we have used a modified version of Look and Locker’s method

[3],

which is well suited for these measure-

ments. The results are discussed in section 4. We

finally give

some

concluding

remarks.

2. Continuous saturation

experiments.

- 2 .1 SATU-

RATION OF THE ABSORPTION LINE AT 4.2 K. - The concentration of the

crystals

was

10-4

atom g Zn per ZnS mole. We used a

superheterodyne

X band

spectrometer

( f F

= 30

MHz)

which was

frequency-

locked on an

auxiliary temperature-stabilized cavity,

and allowed us to detect the

absorption

line

directly.

Field

sweeping

effects observed for

long T,

were

thus avoided.

We measured

X"(roo, Hl),

the

peak amplitude

of

the

absorption signal (resonant frequency mo)

for

different values of the r.f. field 2

H,

cos roo t present

on the

sample.

In our

experiments Hi

= 0.6

P(G’, W),

P is the incident power on the

cavity. Figures

1 and 2

plot

the ratio a

X"(o-)O, O)IX’(coo, Hl)

versus P in the

range 30 nW P 100

JlW. They

show a linear

variation of a versus P. These results can be understood

by considering

that a diffusion process establishes a

spin

temperature for the

spin

levels. In a

population model,

we have the

following expression

for a : :

(*) E.R.A. no 375.

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:0197600370120147500

(3)

1476

FIG. 1. - Variation of a = x"(roo, 0)/x"(.wo, Hl) versus incident powerP(P 12 pW - H // [III]W - 11/2, - 1/2 > -+ I - 1/2, - 1/2 )

transition).

10

FIG. 2. - Variation of a

versus P (P

300 IlW - H // [III]W - 1/2,

- 1/2 > -+ / - 1/2, - 1/2 > transition).

Tl

is the

spin-lattice

relaxation

time, p(wo)

is the

shape

factor of the unsaturated

absorption

line :

where

f(w)

is the

signal intensity,

and the

integral

is

performed

over the whole spectrum. For the

! 1/2, - 1/2 > -+ I - 1/2, - 1/2 > transition,

Experimentally,

we find a = 2 for P = 6

Jl W.

This

leads to

Tl

= 0.33 s. which compares

favourably

to the 0.28 s obtained

by

the

pulse

method.

2.2 SATURATION OF THE DERIVATIVE OF THE ABSORP- TION LINE. - We studied the same transition as

previously

with the same orientation of the static field.

We used lock-in detection

(20 Hz) giving

the deriva- tive of the

absorption

line

dX"IdH.

In

figure 3,

we

plot

the ratio

FIG. 3. - Variation of

versus the rotating r.f. field H1

(T

= 39 K - H // [III]W 1/2,

- 1/2 ) --- I - 1/2, - 1/2 ) transition).

versus

H1; [dX"(w, Hl)/d1lJM

is the

peak amplitude

of the derivative of the

absorption

line. We still have

Hi

= 0.6

P(G2, W).

We determined

p

for r.f. powers in the 1.8

ptW-1.8

mW range. The

experimental

conditions are such that even at the

highest

r.f. power,

we do not fulfil the conditions of Redfield’s model

[4].

The characteristic results are shown below :

The

spin-lattice

relaxation times differ

by

a factor

3

000,

whereas the

corresponding

factor for the r.f.

powers is 15

only. Although

we cannot compare

directly

the values of the two incident powers, since

one involves the

absorption

line and the other its

derivative,

this cannot

explain

such a difference

in the ratios. We must consider that the satura- tion does not occur

by

means of the same process in the two

experiments.

We will show that the results for T = 39 K are consistent with the saturation of the

11/2, 1/2 > --+ 1 - 1/2, - 1/2 )

transition

only,

whereas the whole spectrum was saturated at 4.2 K.

To

interpret

the results of

figure 3,

we have

to consider a multilevel

system (MI

= -

1/2, Ms

= -

5/2, ...,

+

5/2).

The different levels are numbered from 1 to 6

by increasing

value of

Ms.

We will call Pi the

population

of level i. Levels 3 and 4 are

coupled by

the r.f. field

with transition

probability

U. The

spin-lattice

transi-

tion

probability

from i

toward j

is

Wij.

We have the

following

relations

(see

ref.

[1], [2])

between the

Wij :

v

(4)

obtained

following

the method used

by Llyod

and

Pake

[5].

The calculation

gives :

Ak4

is the cofactor of the 4th column element in the kth row in the determinant of

the pi

coefficients.

More

explicity :

where z =

a/b.

We thus get for a an

expression

similar to Bloem-

bergen’s [6],

with

k/2

to be

compared

to

TI.

When the

transition line

shape

is lorentzian

(width Aco), P

is

given by

the

following expression :

The coefficient 9 in

(6)

comes from the ratio :

The theoretical

expression (5)

cannot describe the

experimental

results. This suggests that the observed line is not

homogeneous.

We will use the

independent homogeneous spin-packets

model

[7]

and we will

consider that the distribution law

h(w - mo)

of the

spin-packets

is lorentzian with a width Am*. The

absorption

line of a

spin-packet

will be obtained from

expression (3) using

for the

shape

factor of the tran- sition

probability

U a lorentzian line with width A(o.

The

expression

for

#

is thus :

try

experimental by

the

pulse

method are consistent with our

interpretation

of continuous saturation

experiments.

The evolution of

A 34(t)

after

saturating

the 3 --+ 4 transition is :

The reduced

eigenvalues Ailb

of

equation (2) (where

U =

0),

were calculated for z

varying

between

1/16

and

16,

and classified

by increasing

values

(A,

=

0).

To

study

the

amplitudes Ai,

we must first know the values of the

populations

at the end of the satu-

rating pulse,

which in our

experiments

was

by

far

longer

than any

IlAi.

These values are obtained from

(2),

with U - oo and

using

the new variable

The

amplitudes A2, A3, A5

versus z are

plotted

in

figure 4; A4

and

A6

are

108

times weaker than

As.

For a

given

value of z,

the Ai

are obtained from the reduced

quantities Ailb,

b

being

determined from continuous saturation

through (4).

The time constants

of interest are

plotted

in

figure

5.

Experimentally,

we have observed an

exponential

return to

equilibrium,

with a 80 ps time constant.

This is consistent with the

interpretation

of continuous saturation

experiments

if z has a value between 0.5 and 2. We cannot

hope

for a better determination of z, because of the strong variation of the relaxation

probabilities

with

temperature.

We

experimentally

observe -

I/Â2

if z =

0.5, - 1/Â3

if z = 2 and

-

I/A2 - - 1/ Â3

if z = 1.

3.

Study

of the saturation law at 1.34 K. - We

see

(Fig.

1 and

2)

that

a(P)

does not follow expres- sion

(1)

for

high

r.f. power P. We have taken into account various

hypothesis

which failed to

explain

the

experimental

results. We therefore made expe-

(5)

1478

FIG. 4. - Variation of the amplitudes A2, A3 and A5 versus

Z = W65/W64-

FIG. 5. - Variation of the time constants - I/A2, - IIA3 and

- IIA5 versus z = W65/ W64. 80 ps is the time constant of the observed exponential signal (saturating pulse » relaxation time

constants, T = 39 K - H % [III]w).

riments

using

a modified version of Look and Locker’s method

[3],

which allowed easy determination of

Tl

versus the r.f. power P. We observed a

shortening

of

Tl

with

increasing

P. We will discuss these different

points successively.

3.1 DISCUSSION OF THE CONTINUOUS SATURATION EXPERIMENTS. - a was measured

using

the same

experimental

conditions as at 4.2

K,

and two

samples

of different sizes

(3 x 5 x 8

mm and 1 x 2 x 3

mm)

obtained from the same

crystal.

For low r.f.

fields,

a varies

linearly

with P. In the linear

region

a = 2

is obtained for P = 2

JlW.

This leads to

T1

= 1.0 s,

in

agreement

with the results of the

pulse

method

(7B

T = 1.18 s.

K,

T 10

K).

This shows that the model considered at 4.2 K is still valid for low r.f.

fields. For

increasing

powers, the saturation of the

absorption

line is more difficult than

expected

from

(1).

This effect is more

important

for the

large crystal :

for P = 100

Jl W,

the a value is 32 for the small

crystal

and 13 for the

large

one, instead of 51.

The observation of a size effect suggests that the

mean number of resonant

phonons

may be increased from no

(thermal equilibrium value)

to n, either

by spins (phonon-bottleneck)

or

by piezoelectric

effect.

We will discuss these two

hypothesis successively,

for a

spin 1/2.

Phonon-bottleneck has been treated

by Faughnan

and

Strandberg [8]

for

pulse

saturation

experiments,

and

by

Scott and Jeffries

[9]

for continuous saturation.

They supposed

an

exponential

return of n to no,

with time constant iph, and introduced the bottleneck factor 7. Under severe bottleneck

(0-

>

1)

and after

a

saturating pulse,

the

spins

and

phonons

come

first to

equilibrium

with time constant i" -

TphlU,

then the

spin-phonon

system reaches the bath tempe-

rature with time constant r’ =

u Tl.

If

Tl

oc

T

then ’t" oc T - 2. For continuous saturation

where p is the

population

difference between the two

spin levels,

and S’ = 2

UTi,

where lJ is the

probability

of the transition induced

by

the r.f. field. If a -

0,

u - ao = 1 + S’.

Expression (9)

shows that

a/oco

> 1 for any r.f. field. This means that saturation is easier with

phonon-bottleneck.

Our

experimental results,

inconsistent with the

preceding features,

cannot be

explained by

a

phonon-bottleneck.

Because of the strong

piezoelectricity

of

ZnS,

one may consider that the

crystal,

submitted to a

weak electric

field,

absorbs acoustical energy,

leading

to an increase of the mean number of resonant

phonons.

We can

study

this situation

using Faughnan

and

Stranberg’s

model

[8]. n and

p are

given by

a set

of

coupled equations :

In

equation ( 10b),

the

quantity

l U describes the

(6)

Locker’s method

[3]

in the

following

way. Constant

magnetic

field was set at the resonance of

the 11/2,

-

1/2 ) -t - 1/2, - 1/2 )>

transition. The

crystal

was submitted to a known r.f. power

by switching

on the fast diode

(Fig. 6) ;

at the same time the 30 E.S.R.

FIG. 6. - Block diagram of the experimental apparatus for T,

measurements by successive field-sweeps. We use two Helmoltz coils (0 25 mm, 120 turns) situated on both sides of a slotted TEo 12

cavity.

lines were swept

by

a

triangular magnetic

field

Hpp

of 450 G

peak-to-peak amplitude

and

period Tf Tl.

During

the successive sweeps the

spin

system came

progressively

to saturation. The r.f. field was then switched off for a time

long enough

to

bring

the system back to

equilibrium.

The theoretical

analysis

of this

experiment [10]

shows that the two

following

conditions must be fullfilled :

1)

The

sweeping

rate of the

magnetic

field must be

such that the variation of the resonant

frequency

in a time

T2

=

(yHL) - 1 be

much less than the time width

yHL.

This leads to

2)

The

spin

temperature must not vary

greatly during

a passage

through

the resonant line. This leads to

Under the

preceding conditions, during

the field

A

knowledge

of r and

v(aJ)/v(0)

then allows the determination of

T1

in the presence of the r.f. field.

In these

experiments Wral = nyHf/Hpp. Comparison

of the results obtained

by

this method and

by

conti-

nuous saturation

requires

some care. For

example,

for a

given

incident power P

since the absorbed r. f. energy is not the same in the two

experiments ( WSat

is weaker than W defined

in (1)).

In order to

satisfy

the

previous conditions,

we chose :

For the

large sample

we obtained :

(This

value compares

favourably

with the 880 ms time

constant obtained

by

the

pulse

saturation

method)

Since the observed spectrum was somewhat

complex,

it is difficult to make a

precise

determination of the

envelope.

This

gives

us a 20

%

error in the

T1

measu-

rement. We could not obtain similar information from the small

crystal

because of the poor

signal-to-

noise ratio.

A decrease of

Tl

with

increasing

P has

already

been observed

by Davis, Strandberg

and

Kyhl [11]

in

pulse experiments

on

Lal-xGdx(C2HsS04)39 H20 (x

= 5 x

10-3)

at 4.2 K.

They suggested

that this

decrease

came from an increase

(in

the conventional

sense)

of the lattice

temperature.

Marr and

Swarup [12], making

continuous saturation measurements on a

sample

with x =

10 - 2,

observed that the

spin

system

was difficult to saturate. Their

suggestion

of a

phonon-

bottleneck cannot be retained because this would lead to

a/ao

>

1,

whereas

they

observed

cx/cxo.

1.

Finally

the

hypothesis

of Davis et al. is at the present

(7)

1480

U)

FIG. 7. - Saturation of the absorption signal by successive field-sweeps which gives values of T1(P). (T = 1.34 K - H // [III]w).

a) P = 0.1 mW ; T1 = 600 + 120 ms. b) P = 0.9 mW ; T1 = 125 + 25 ms.

time the

only

valid

interpretation

of the

experimental

results on

gadolinium ethylsulfate.

Our continuous saturation

experiments

have been

made at 1.3 K where the relaxation takes

place through

a direct process. It is then difficult to

explain

our

results

by simple

lattice

heating.

We still consider

a

spin 1/2.

Let

T( U)

be the lattice temperature when the transition

probability

induced

by

the r.f. field is U.

In continuous saturation

experiments

we obtain the

quantity G/p,

where G is a coefficient

independent

of

U,

and of the variation of the lattice temperature from its value

To

for U = 0. For a

paramagnetic

center

following

the Curie law and

relaxing by

a

direct process,

expression ( l0a)

with n = no

gives :

where A and B are two coefficients

independent

of T

and U. It is easy to show from

expression (11) that,

for

any U,

the value a will be greater than that obtained

without lattice

heating.

This is the contrary to our observation. If one retains the

assumption

of lattice

heating,

it is therefore necessary to reach the Raman

region.

For ZnS :

Mn2 +,

this means that the lattice

temperature must be greater than 10

K,

which one can

hardly accept.

4. Conclusion. - A

difficulty

may appear in the

interpretation

of continuous saturation

experiments

made on a multilevel system when there is a tempe-

rature-independent

diffusion process. It may then be necessary to use different models

according

to the

temperature

range. This

difficulty

may be removed

by making simultaneously pulse

measurements.

For ZnS :

Mn 2+

it has been confirmed that :

- at 4.2 K the whole spectrum is saturated and behaves like a

homogeneous

line because of

spin diffusion;

- at 39 K one saturates

only

the considered transition. The

experimental

saturation law was

justified by considering

a model where the six fine- structure levels are

coupled by spin-lattice relaxation,

and

using

the

independent spin packet

formalism.

Comparing

the results obtained

by

both

methods,

it was shown that the ratio z =

W5/2-3/2/W5/2-1/2

(8)

References

[1] DEVILLE, A., BLANCHARD, C., GAILLARD, B., GAYDA, J. P.,

J. Physique 36 (1975) 1151.

[2] DEVILLE, A., BLANCHARD, C., GAILLARD, B., J. Physique 37 (1976) 1067.

[3] LOOK, D. C., LOCKER, D. R., Phys. Rev. Lett. 20 (1968) 987.

[4] REDFIELD, A. G., Phys. Rev. 98 (1955) 1787.

[5] LLOYD, J. P., PAKE, G. E., Phys. Rev. 94 (1954) 579.

[6] BLOEMBERGEN, N., PURCELL, E. M., POUND, R. V., Phys.

Rev. 73 (1948) 679.

[7] PORTIS, A. M., Phys. Rev. 91 (1966) 1092.

[8] FAUGHNAN, B. W., STRANDBERG, M. P. W., J. Phys. Chem.

Solids 19 (1961) 155.

[9] SCOTT, P. L., JEFFRIES, C. D., Phys. Rev. 127 (1962) 32.

[10] GOLDMAN, M., Spin temperature and nuclear magnetic reso-

nance in solids (The Clarendon Press, Oxford) 1970.

[11] DAVIS, C. F., STRANDBERG, M. P. W., KYHL, R. L., Phys.

Rev. 111 (1958) 1268.

[12] MARR, G. V., SWARUP, P., Can. J. Phys. 38 (1960) 495.

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