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HAL Id: jpa-00210659

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Submitted on 1 Jan 1987

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Acoustic study of low-energy activation processes in magnetic rare-earth glasses : amorphous holmium

aluminosilicates

F. Lerbet, G. Bellessa

To cite this version:

F. Lerbet, G. Bellessa. Acoustic study of low-energy activation processes in magnetic rare-earth glasses : amorphous holmium aluminosilicates. Journal de Physique, 1987, 48 (12), pp.2111-2118.

�10.1051/jphys:0198700480120211100�. �jpa-00210659�

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Acoustic study of low-energy activation processes in magnetic rare-earth glasses : amorphous holmium aluminosilicates

F. Lerbet and G. Bellessa

Laboratoire de Physique des Solides (*), Bâtiment 510, Université Paris-Sud, 91405 Orsay, France

(Requ le 17 juillet 1987, accept6 le 25 août 1987)

Résumé.

2014

Nous présentons une étude acoustique de verres d’aluminosilicates de différentes teneurs en

holmium. Les mesures sont faites jusqu’à 100 mK, dans le domaine de fréquences 10-500 MHz et dans des

champs magnétiques compris entre 0 et 60 kOe. Nous observons un pic de l’atténuation en fonction de la

température qui suit une loi d’Arrhenius et qui est sensible au champ magnétique. Nous observons aussi un

petit pic d’atténuation dont la localisation en température ne dépend ni de la fréquence acoustique ni du champ magnétique. Associée au premier pic, une variation de la vitesse du son est observée. Le pic d’activation et la variation de vitesse associée sont bien interprétés dans le contexte de la relaxation par des processus d’activation de systèmes magnétiques à deux configurations. Grâce à l’étude en fonction de la concentration,

nous établissons que ces systèmes ne sont pas les mêmes que ceux observées par d’autres auteurs dans la phase

verre de spin et sont certainement beaucoup plus légers. Nous considérons le modèle d’anisotropie aléatoire

des alliages de terres rares, pour expliquer nos effets.

Abstract.

2014

An acoustical study of aluminosilicate glasses with various holmium contents is reported. The

measurements are performed down to 100 mK, in the frequency range 10-500 MHz and in a magnetic field up to 60 kOe. An attenuation peak as a function of the temperature following an Arrhenius law and depending on

the magnetic field is reported. Another small attenuation peak depending neither on the acoustical frequency

nor on the magnetic field is also reported. Connected with the first peak, a sound velocity variation is observed. The activation peak and the connected sound velocity variation are well explained in the framework of the relaxation of two-configuration magnetic systems by activation processes. Thanks to the acoustical study

as a function of the holmium content, we show that these systems are certainly not the same as those observed

by other authors in the spin glass phase and are much lighter. The random anisotropy model of the rare-earth

alloys is considered to explain the observed effects.

Classification

Physics Abstracts

63.20M - 75.50K

-

63.50

1. Introduction.

Ultrasonic measurements in metallic spin glasses

have revealed a small dip in the sound velocity near

the freezing temperature [1, 2]. An effect of the

magnetic field on the thermal conductivity of spin glasses has been observed [3, 4]. These authors

proposed that this effect should arise from thermal activation of magnetic clusters. In insulating spin glasses we have reported an acoustical study which

revealed an activation process non-connected with the spin freezing but rather with the reversing of the magnetic ions on their anisotropy axis [5]. Sub- sequently, other acoustical measurements have been

reported [6]. They have been interpreted in terms of dipolar and quadrupolar freezing [7].

We report an acoustical study of aluminosilicate

glasses doped with holmium ions at different concen-

trations. Our preliminary measurements already published were for a concentration of 10 % at. [5].

The low-temperature magnetic study of Chappert et

al. [8] has shown that for this concentration, this insulating amorphous material exhibits a spin glass

behaviour. Hence, it is interesting to vary the

magnetic-ion concentration, mainly below 10 %

(12 % is the concentration from which nearest neigh-

bours appear in a cubic lattice and the interaction between the magnetic moments is dipolar). The

atomic holmium concentrations studied are 10.1 %,

6.7 %, 3.4 % and 1.5 %. The acoustic measurements have been performed down to 100 mK’ and in the

frequency range 10-500 MHz.

In this paper, we do not consider the effects on the acoustic wave of the tunneling states which always

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:0198700480120211100

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2112

exist in the amorphous matter [9, 10]. They give rise

in our samples to a logarithmic temperature depen-

dence of the sound velocity and to an acoustic

attenuation variation at the lowest temperatures [5].

A detailed study of these effects are reported

elsewhere [11, 12].

2. Experimental procedure.

The samples studied are aluminosilicate glasses doped with rare earth ions. The ion which interested

us was the Ho3 + magnetic ion. It is easy to obtain

good glasses for a holmium content of 10 % [8]. But,

if one tries to decrease this one, it is no longer possible to obtain a glass from the liquid phase. In

order to overcome this difficulty, we have kept

constant (and equal to 10.1 %) the rare earth ion

content and partly replace the Ho3 + ions by La3 + ions, which are not magnetic. Thus, the

different compositions studied are :

1.5 % at. Ho :

The 10.1 % Ho sample exibits a spin glass behaviour

with a freezing temperature around 0.5 K [8].

The ultrasonic study was made by sending acoustic

wave pulses of various frequencies (10 MHz-

500 MHz) through the samples. The experimental apparatus is phase sensitive and allows measure- ments on both acoustic attenuation and relative variation of sound velocity (with an accuracy better than 10-6 for a reasonnably good signal-to-noise ratio). The very good precision on the ultrasonic attenuation at 10 MHz ( = 10- 3 dB/cm) has been

obtained by studying the n-th echo, in order to lengthen the acoustic path.

The samples are parallepipeds (10 x 4 x 4 mm).

They are cooled in a dilution refrigerator which

works down to 8 mK. A superconducting magnet

can produce a field up to 60 kOe. Its homogeneity is

better than 1 x 10- 5 in the whole sample. The thermometry at low temperatures and high fields has

been achieved with a carbon resistor [13] and a capacitive sensor. At 0 kOe we use also a germanium

resistor in the temperature range 50 mK-10 K.

3. Experimental results : activation processes.

3.1 10.1 % HO GLASS IN ZERO MAGNETIC FIELD [5].

The variations of the ultrasonic attenuation in this

sample as a function of the temperature are shown in figure 1, for different frequencies. A well resolved

peak on the attenuation at 10 MHz clearly appears.

Fig. 1.

-

Attenuation variation of longitudinal acoustic

waves as a function of the temperature for various

frequencies and without magnetic field in the 10.1 % Ho

sample. 0 : f = 10 MHz ; * : f= 60 MHz ; + : f =

210 MHz ; x : f = 480 MHz. The vertical scale is arbitrary

and different for every curve.

It becomes a shoulder and its location shifts towards the high temperatures at higher frequencies (between 10 MHz and 480 MHz). Obviously, there

is superposed on these peaks another attenuation variation. The latter arises from the relaxation of the

tunnelling states which exist in our samples [5].

Using the theory [14] and the parameters of the

Fig. 2.

-

Attenuation variation of longitudinal acoustic

waves as a function of the temperature at 10 MHz and without magnetic field in the 10.1 % Ho sample. The

asterisk line is the expected attenuation variation due to

the tunnelling states (see text).

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tunnelling states in our samples [12], we have displayed in figure 2 the expected attenuation vari- ation. The attenuation peak appears clearly upon this curve (Fig. 2). Our analysis cannot be conducted

at all the frequencies because another contribution appears at higher temperatures (T > a few K) and is

more important at higher frequencies. We can despite this fact, extract a peak at all the frequencies

from the « natural » curve which is also deduced from the results at high magnetic fields (see below).

The variations of the location temperature and of

the amplitude of the peak as a function of the frequency are shown in figure 3 and figure 4, respect- ively. They are easily interpreted in the framework of the relaxation of two-configuration systems (TCS) by activation processes [14, 15]. In this model each system characterized by a barrier V and an asymme- try E interacts with the elastic wave of frequency jf2/2 7T and one calculates the attenuation and the variation of sound velocity using the equations :

where To is a characteristic time. T follows the Arrhenius law of the activation processes and r

depends on the density of states of the TCS and on

their coupling with the elastic strain. r is often called the relaxation strength. We can deduce from these

equations, neglecting the distribution g (V), the

location temperature and the amplitude of the peak :

Fig. 3.

-

Location temperature of the activated peak as a

function of the frequency for two magnetic fields. 0 : H = OkOe; +: H= 5k0e.

Fig. 4.

-

Amplitude variation of the activated peak with-

out magnetic field as a function of the frequency.

and

Our results can be interpreted in the framework of this model. Hence, we obtain :

In fact, the description with only one barrier height

is not satisfying with regard to the width of the peak

which is better (but not perfectly) fitted with a

constant distribution of barriers between 2 K and 8 K. In this case the Arrhenius law is still followed in

our frequency range 10 MHz-480 MHz. Since the basic line is not perfectly known, there is no more meaning to search for a better fit of the attenuation

peak, with unknown parameters. However, a broad distribution of relaxation times is not surprising in glasses [16-19] and does not change fundamentally

our interpretation.

According to equation (2), there is a variation of the sound velocity correlated with the attenuation

peak. However, the experimental results are more

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2114

difficult to interpret due to another source of vari-

ation for the sound velocity [5]. Nevertheless, in figure 5 which displays the variations of the sound

velocity at 110 MHz, it appears a diminution of the

velocity around the peak temperature Tp, as ex- pected from equation (2) [5]. The relaxation

strength r’ deduced from figure 5 using equation (2)

and assuming an additional logarithmic variation,

is :

It agrees very well with the one obtained from the attenuation peak.

Fig. 5.

-

Relative velocity variation of the acoustic waves as a function of the temperature at 110 MHz without

magnetic field in the 10.1 % Ho sample. The solid line is

only a guide for the eyes. Tp is the location temperature of the attenuation peak for the same frequency.

3.2 10.1 % Ho GLASS IN MAGNETIC FIELD [5].

-

We

have observed an attractive effect, which is the

displacement of the attenuation peak induced by a magnetic field. The attenuation peak (and correla- tively the characteristic variation of the sound vel-

ocity) shifts towards the high temperatures as the magnetic field increases (Fig. 6). Restricting us to

the range [0-10 kOe], where the deformation of the attenuation peak is not too large, we show this shift at 10 MHz. In figure 6, the vertical shifts of the

curves are arbitrary for a clearer display, but we can experimentally adjust them with respect to each other, since we are able to measure for the same temperature and frequency the variations of the attenuation (and of the sound velocity) as a function

of the magnetic field. Thus, can we find a right basic

line for the results without magnetic field as it is

shown in figure 7. The variations of the ultrasonic attenuation for two different magnetic fields at

110 MHz are shown without any arbitrary shift with respect to each other. Since the attenuation is the

same for the two magnetic fields above 4 K, the

Fig. 6. - Attenuation variation as a function of the temperature at 10 MHz for different magnetic fields in the 10.1 % Ho sample. The vertical shifts of the curves with respect to each other are arbitrary for clarity. 0 : H

=

0 kOe ; * : H

=

5 kOe ; x : H

=

10 kOe.

disappearance of the activation peak as the high magnetic field is set up, is obvious in figure 7 (we

shall consider later the attenuation peak which

appears at low temperature in high magnetic field).

Fig. 7. - Attenuation variation as a function of the temperature at 110 MHz for two different magnetic fields

in the 10.1 % Ho sample. Here, there is no arbitrary

vertical shift of the curves. 0 : H

=

0 kOe ; * : H

=

60 kOe.

If we restrict now our study to a single relaxation time, we can perform the same analysis as in paragraph 3.1, but for various magnetic fields be- tween 0 kOe and 10 kOe. For all the magnetic fields,

we have found that the peak follows an Arrhenius

law with the parameters :

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The first remarkable result is that To does not change

with the magnetic field (Fig. 3). This means that the

wells neither change. The shift of the attenuation

peak towards the higher temperatures (Fig. 6 and Fig. 3) has to be interpreted as an increase of the barrier height. This one increases linearly with increasing magnetic field up to 10 kOe (Fig. 8). If we

write a

=

Kgj Jg B, using the values of the Ho3 + ion

(J = 8 and gj = 1.25), we find that K - 1. This result will be examined below.

Fig. 8.

-

Activation energy of the peak as a function of

magnetic field.

3.3 Ho GLASSES AT 0 k0e AND LOWER CONCEN- TRATIONS.

-

We have extended our study with the

concentration of magnetic ions from a rather concen-

trated regime (10.1 % at. ; at this concentration there is a spin glass behaviour with a freezing temperature around 0.5 K [8]) to a more dilute one ( = 1.5 %). The other concentrations studied are :

6.7 %, 3.4 %, 1.5 %. We may believe, that with decreasing the magnetic-ion content the freezing temperature decreases strongly, since the ion interac- tion is dipolar. Thus, we can check whether the attenuation peak here reported is directly connected

with the spin glass phase or not. It is this last hypothesis we have made previously [5].

Figure 9 displays the ultrasonic attenuation in two

Fig. 9.

-

Attenuation variation as a function of the temperature at 110 MHz without magnetic field and for two Ho contents. The solid lines are only guides for the

eyes. 0 : cHo

=

0.101 ; * : cHo

=

0.067.

aluminosilicate glasses with a holmium content of

6.7 % and 10.1 % respectively, at the same frequency (110 MHz). Whereas the phenomena related to the

T9 are certainly moving towards the lower temperat-

ures for this diminution of Ho content, it appears that the peak temperature does not change and that

the peak amplitude decreases. In view of the natural basic line, the peak amplitude is :

/-1 (10.1 %) = 0.8 X /-1 (6.7 %) .

At lower concentration, the attenuation peak is no longer clearly discernible due to its decrease and also to the large increase of the effect of the tunnelling

states on the acoustic propagation which changes significantly the basic line [12]. Nevertheless, as it

can be seen in figure 10, the correlated effect on the

Fig. 10.

-

Relative variation of the sound velocity as a

function of the temperature without magnetic field and for different Ho contents. The solid lines are only guides for

the eyes. The arrow points the location temperature of the attenuation peak. V : cHo

=

0.101, f

=

110 MHz ; 0 :

cHo

=

0.067, f = 110 MHz ; * : cHo

=

0.034, f

=

60 MHz.

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2116

sound velocity (Eq. (2)) is still present in the 3.4 % Ho glass. Its temperature location does not change perceptibly and the amplitude of the effect decreases with decreasing concentration from 10.1 % to 3.4 %.

This confirms that the activation processes here

reported have energies which do not vary sensibly

between 10.1 % and 3.4 % and are not directly

connected with the spin glass phase [5].

4. Non-Arrhenius attenuation peak [5].

Another interesting experimental observation is the appearance of a second peak at a lower temperature

(T -- 370 mK) when a magnetic field is set up. One

can see it in figure 7. Its main features are :

- The location temperature of the peak does not change with the frequency, the magnetic field and

the Ho3 + content. The independence of this tem- perature with respect to the acoustical frequency

excludes Arrhenius processes.

- The peak amplitude increases with the fre- quency, the magnetic field and the Ho3 + content.

We have displayed in figure 11 this attenuation

peak at 470 MHz and 60 kOe (the experimental

Fig. 11. - Attenuation variation as a function of the temperature at 470 MHz and 60 kOe for different Ho contents. The solid lines are only guides for the eyes. x : CH.

=

0.101 ; V : CH.

=

0.067 ; 0 : CH.

=

0.034 CHo

=

0.015.

conditions which give the largest peak), for different holmium contents. It vanishes at low concentration of holmium and its location temperature does not change sensibly with varying the concentration. The correlated effects on the sound velocity, if they exist,

are hidden by the rather complicated behaviour of the sound velocity in high magnetic field [5].

Although it is obvious that this peak is due to the magnetic ions, we have presently no satisfactory explanation for it.

5. Discussion on the activation processes.

We have seen that the main attenuation peak and

the correlated effect on the sound velocity can be interpreted with activated processes involving mag- netic entities. The activation barriers are low (height

=

5 K) and increase with increasing magnetic field.

Then, the question is what are these magnetic

entities ?

The magnetic study of an aluminosilicate glass

with a 10.1 % holmium content [8] has shown that activation processes exist in such samples, with the following parameters :

The processes were supposed to involve super-

paramagnetic clusters related to the spin glass transi-

tion [8]. We can state however, and for several

reasons considered below, that our magnetic entities

are not the same as these clusters.

Firstly, the parameter values of the relaxation processes obtained from the two experiments are

different. Specially, our To is three orders of mag- nitude smaller than To. Since To characterizes the motion of the entities in each well, that proves that in both experiments the involved entities are not the

same. Moreover, we may think that the entities observed in our acoustic study are lighter than those

observed in the magnetic one, because of the much smaller value of To. This value, which is of the order of that found for atomic motions, suggests that our process might be a single-ion activated one. This is

also indirectly supported by the a value in the

paragraph 3.2 which is of the order of gJ J..tB.

Moreover, the fact that To does not change with the magnetic field means that it is always the same objects which are thermally activated.

It is possible to explain our main experimental results, assuming a single-ion activation process [5].

In the framework of the random anisotropy model of

the rare-earth alloys [20, 21], the rare-earth ions can

be described as magnetic moments in a double-well

potential. In their model Harris et al. [20] assume

that each rare-earth spin i is subjected to a local anisotropy field of random orientation zi and the lowest states are I JZi > = ±J). Fert and Campbell

have shown that a model with nonaxial field gra- dients is nearly equivalent to the preceding one,

when the rare-earth momentum J is large [21].

Hence, alloys with Ho3 + (J

=

8) are well described

with this model. Then, we may define two potential

minima corresponding to the direction of the ion

along its anisotropy axis. To reverse its direction on

this axis, the magnetic moment at each site has to

overcome an energy barrier because it is necessary

to draw out of its minimum energy orientation the

electric quadrupole. Thus, we have defined at each

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rare-earth site a phenomenological double-well po- tential [5]. Moreover these objects will be strongly coupled to the acoustic waves due to the associated modulation of the crystal field. Taking, for simp- licity, a symmetrical double-well in zero magnetic field, this one becomes asymmetrical with an asym- metry E

=

2 gf JIXB Hz (gj is the Lande factor equal

to 1.25) when a magnetic field is set up. Then, the

relaxation time of the rare-earth ion in this double well is given by [5] :

The last factor of equation (7) which is sometimes omitted cannot be neglected here. Obviously, equation (7) is identical to equation (3) in zero magnetic field. In the presence of a magnetic field H, the asymmetry e

=

10 1’ B H is equal to 7 K at

10 kOe and this value is larger than T in the temperature range of the experimental peak. Hence,

the factor sech (e/kB T) can be replaced by exp (- ê / kB T). As a result, the asymmetry disap-

pears in equation (7). This shows that it is not

possible to explain the peak displacement with the magnetic field if V is treated as field independent.

However, the experimental results agree with

equation (7) if V is replaced by the expression given

in equation (6) (To is field independent as proven

experimentally). A theoretical model of the barrier would be necessary to explain this field effect.

It must be pointed out that our phenomenological model, although it explains qualitatively our exper- imental results, leads to barrier heights which are surprisingly low. Indeed, magnetic study in our glasses would be necessary. However, in the metallic

rare-earth alloys the barrier heights are rather of the order of 100 K than of the order of 5 K [22]. If we

are looking for different light magnetic entities, we

can try to consider pairs or other little clusters. They

have been involved in Eu,,Sr, -,,S in order to explain

the magnetization results for low Eu3 + ion content

[23, 24]. Energy barriers appear during the reversing

of a pair of spins linked together by the high exchange energy. These barriers arise from the

dipolar interaction and can be quite small. However,

it is worth remembering out that the Eu3 + ion is

isotropic and has no anisotropy barrier to overcome.

This is not the case for the Ho 3, ion and any process

involving a reversing of this one will have an energy barrier equal or greater than the anisotropy energy.

In any case, the effect reported here must lead to a

remanent magnetization [5]. We know that in a

similar sample, a remanent magnetization has been already observed by Chappert et al. [8] but it is not the same as the one we are proposing. These authors

have reported a time constant of about 102 s at

0.34 K. For the process that we propose, the sample

put in a magnetic field at 0.34 K and then removed from the field, will be demagnetized with a time

constant determined by equation (3). Its value using

our parameters is found to be 4 x 10- 5 s which is too short to be observed. However, by choosing a more

suitable temperature such 0.2 K, equation (3) gives a

time constant of 3 s which is easily observable [5]. In

order to avoid the cluster effects at this temperature it is necessary to study dilute alloys. To this end, preliminary results of remanent magnetization in

one of our samples with a 3.4 % holmium content

have been obtained [25]. The experimental sequence

was : cooling of the sample in a magnetic field of

1 kOe from 1.25 K down to 0.145 K, then switching

off of the magnetic field and measurement of the

magnetization as a function of time. Indeed, a non- exponential remanent magnetization has been obser-

ved, corresponding to a broad distribution of relax- ation times. The relaxation times are distributed between 50 s and 4 000 s [25]. Using equation (3)

and our To value, this distribution leads to potential

barriers between 4.3 K and 5 K. This is quite satisfac-

tory with regard to the barrier distribution obtained in the acoustic experiments (§ 3.1). From the amplitude of this remanent magnetization, it is also

possible to estimate the number of Ho3 + ions

involved, if we interpret it as a reversing of the Ho 3, ions along their anisotropy axis. So doing, we

find that one tenth of the Ho3 + are reversing.

Taking into account all the approximations, this

result is qualitatively satisfactory. Nevertheless,

further magnetization experiments are necessary

(mainly, magnetization measurements as a function of holmium content).

6. Conclusion.

Our acoustic study of aluminosilicate glasses doped

with Ho3 + ions has given a lot of results. Some of them (the non-Arrhenius peak) have not been explained. However, the main results are well interp-

reted in the framework of the relaxation of two-

configuration systems by activation processes. It has been shown that these systems are magnetic entities

which surely are not the same ones as those of the

spin glass phase and certainly much lighter. In order

to explain the relaxation of these objects by activa-

tion processes, we have presented a single-ion activa-

tion model (a model of reversing of the rare-earth ions on their anisotropy axis) which is qualitatively satisfactory but which leads to some surprising

parameter values (very low anisotropy barrier heights). This model leads to the existence of a remanent magnetization which has been indeed observed and call for other studies, mainly magneti-

zation studies with varying Ho content and acoustic

studies with other rare earth ions.

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2118

Acknowledgments.

The authors are indebted to J. Godard who made the samples and to J. L. Tholence who performed a

magnetization experiment on one of their samples.

They thank I. A. Campbell and J. Y. Duquesne for

fruitful discussions.

References

[1] HAWKINS, G. F., THOMAS, R. L. and DE GRAAF, A.

M., J. Appl. Phys. 50 (1979) 1709.

[2] HUANG, F. S., J. Appl. Phys. 54 (1983) 5718.

[3] ARZOUMANIAN, C., DE GOER, A. M. and SALCE, B., J. Phys. Lett. 44 (1983) L-39.

[4] HERLACH, D. M., WASSERMANN, E. F. and WILLNECKER, R., Phys. Rev. Lett. 50 (1983)

529.

[5J LERBET, F. and BELLESSA, G., J. Phys. Lett. 45 (1984) 1045.

[6] DOUSSINEAU, P., LEVELUT, A., MATECKI, M., RE-

NARD, J. P., SCHön, W., Europhys. Lett. 3 (1987) 251.

[7] VOLKMANN, U. G., BÖHMER, R., LOIDL, A., KNORR, K., HÖCHLI, U. T. and HAUSSÜHL, S., Phys. Rev. Lett. 56 (1986) 1716.

[8] CHAPPERT, C., BEAUVILLAIN, P., RENARD, J. P. and KNORR, K., J. Magn. Magn. Mater. 15-18 (1980)

117.

[9] ANDERSON, P. W., HALPERIN, B. I. and VARMA, C., Philos. Mag. 25 (1972) 1.

[10] PHILLIPS, W. A., J. Low Temp. Phys. 7 (1972) 351.

[11] LERBET, F. and BELLESSA, G., J. Physique 48 (1987)

1251.

[12] LERBET, F. and BELLESSA, G., to be published.

[13] LERBET, F. and BELLESSA, G., Cryogenics 12 (1986)

694.

[14] JÄCKLE, J., PICHE, L., ARNOLD, W. and HUNK- LINGER, S., J. Non Cryst. Solids 20 (1976) 365.

[15] HERZFELD, K. F. and LITOVITZ, T. A., Absorption

and dispersion of ultrasonic waves (Academic

Press, New York, London) 1959.

[16] ANDERSON, O. L. and BÖMMEL, H. E., J. Am.

Ceram. Soc. 38 (1955) 125.

[17] HUNKLINGER, S. and ARNOLD, W., Physical Acous- tics, Eds Mason, W. P. and Thurston, R. N.

(Academic Press, New York) 1976, Vol. 12, p. 155.

[18] GILROY, K. S. and PHILLIPS, W. A., Philos. Mag.

B 43 (1981) 735.

[19] DUQUESNE, J. Y. and BELLESSA, G., J. Non Cryst.

Solids 81 (1986) 319.

[20] HARRIS, R., PLISCHKE, M. and ZUCKERMANN, M.

J., Phys. Rev. Lett. 31 (1973) 160.

[21] FERT, A. and CAMPBELL, I. A., J. Phys. F. 8 (1978)

L-57.

[22] MOORJANI, K. and COEY, J. M. D., Magnetic

Glasses (Elsevier, Amsterdam) 1984, p. 197.

[23] THOLENCE, J. L., HOLZBERG, F., GODFRIN, H., LÖHNEYSEN, H. V. and TOURNIER, R., J. Physi-

que 39 (1978) C6-928.

[24] EISELT, G., KÖTZLER, J., MALETTA, H., STAUFFER, D. and BINDER, K., Phys. Rev. B 19 (1984)

2664.

[25] THOLENCE, J. L., private communication.

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for hysteresis effects in amorphous alloys using the HPZ model is related to the results of Monte Carlo calculations for both ferro- and antiferro- magnetic coupling.. The structure

Résumé. — Les expériences de diffraction neutronique ont été de première importance pour mettre en évidence la grande variété de propriétés magnétiques des