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Submitted on 1 Jan 1982

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Anisotropy energy of spin glasses at T < Tg studied by transverse susceptibility

F. Hippert, H. Alloul

To cite this version:

F. Hippert, H. Alloul. Anisotropy energy of spin glasses at T < Tg studied by transverse susceptibility.

Journal de Physique, 1982, 43 (4), pp.691-703. �10.1051/jphys:01982004304069100�. �jpa-00209441�

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Anisotropy energy of spin glasses at

T Tg studied by transverse susceptibility

F. Hippert and H. Alloul

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

(Reçu le 18 septembre 1981, révisé le 16 dicembre, accepté le 18 dgcembre 1981)

Résumé.

2014

Nous avons étudié les propriétés d’anisotropie des verres de spin CuMn, AgMn, CuMnAux, AuFe, à

T Tg par des mesures de susceptibilité transverse (~) en présence d’un champ statique H0 // z (Ho ~1 kG) et en

champ nul. Nous démontrons que, en présence d’une aimantation rémanente 03C3 créée initialement suivant z, la

réponse du système de spins à un petit champ transverse ( z) met en jeu une rotation collective des spins qui est

entièrement caractérisée, dans la limite des faibles deviations, par la donnée d’un champ d’anisotropie macroscopi-

que HA. A une température donnée l’énergie d’anisotropie K

=

03C3HA ne dépend pas de 03C3. K décroît légèrement

avec la température dans la zone étudiée T ~ Tg/3. Pour T ~ Tg une valeur unique de K rend compte des expé-

riences de ~, RMN, et RPE (en présence de rémanence comme dans l’état obtenu après refroidissement en champ nul). Lorsqu’un renversement de 03C3 peut être induit par application d’un champ H0 négatif, l’analyse des valeurs de ~ pour les deux orientations de 03C3, ainsi que les etudes de cycles d’hystérésis, suggèrent que l’énergie d’anisotropie

totale est la somme d’une contribution uniaxiale et d’une contribution unidirectionnelle. L’énergie d’anisotropie

par atome augmente comme la concentration c en Mn dans les verres de spin CuMn et AgMn et croit linéairement

avec la concentration x en Au dans les alliages ternaires CuMnAux, en accord qualitatif avec les prévisions théo- riques.

Abstract.

2014

We have investigated the anisotropic properties of CuMn, AgMn, CuMnAux, AuFe spin glasses at

T Tg by performing transverse susceptibility (~) measurements in zero and small (~ 1 kG) static field H0 //z. We

demonstrate that, in presence of a remanent magnetization 03C3 initially developed along z, the response of the spin system to a small transverse ( z) field involves a collective rotation of the spins which is fully characterized by a macroscopic anisotropy field HA for small deviations. At a given temperature the anisotropy energy K

=

03C3HA

is found independent of 03C3. A slight decrease of K with temperature is evidenced in the investigated range T ~ Tg/3.

At T ~ Tg the same value for K is found to explain ~, NMR and ESR (both in presence of remanence and in the

zero field cooled state). In cases where 03C3 can be reversed by the application of a negative field Ho, analysis of ~

data in the states with 03C3 up and down, in addition to hysteresis cycles studies, suggests that the total anisotropy

energy might be the sum of uniaxial and unidirectional contributions. The anisotropy energy per atom is found to

scale as the Mn concentration c in CuMn and AgMn and to increase linearly with the Au concentration x in ternary alloys, in qualitative agreement with theoretical predictions.

Classification

Physics Abstracts

75.40

1. Introduction.

-

In a magnetic alloy such as

CuMn the disorder of atomic positions of Mn magne-

tic impurities, in addition to the oscillatory depen-

dence of the exchange RKKY interaction [1] with

Mn-Mn distance, prevents any kind of long range

magnetic order at T = 0. However well below a

characteristic temperature Tg(- I Ja 1/kB), the Mn spins appear to freeze in the random directions of their local fields, in the so called spin glass state, as evidenced by impurity Mossbauer spectra [2] and host NMR [3,

4]. Whether this freezing is a progressive phenomenon

or a new kind of phase transition, as suggested by the

existence of a sharp cusp in the low frequency a.c.

susceptibility at Tg [5, 6], is still an open question [7, 8].

As long as no external field has been applied no macroscopic magnetization can be detected in such a spin glass. However, when cooling the sample through Tg under a magnetic field H,, // z which is then reduced to zero, a remanent magnetization a /’ He is obtain-

ed [9], which decays roughly logarithmically with

time [10, 11]. Existence of remanence and magnetic

after effects have been commonly interpretated within

a highly inhomogeneous picture [10, 12], by analogy

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01982004304069100

(3)

with the Neel model for a collection of isolated ferro-

magnetic particles.

At T T i’ 6 is found to remain in the direction of the cooling field Hc. The corresponding anisotropy

of the system which, as the remanence properties,

does not depend upon the direction of H, with respect

to the crystalline axis [13], has been probed by study- ing the response of the spins to the r.f. field in a NMR experiment. The NMR data on the Cu nearest peigh-

bours of a Mn impurity [4] revealed that the electronic

spins respond collectively to a small external field.

The anisotropy forces are characterized by a single macroscopic field HA // z which depends strongly

upon 6. These results, as well as the detection of sharp hysteresis loops [14, 15], imply a rigid body descrip-

tion of the spin system for small applied fields, at variance with the inhomogeneous description needed

to describe the construction of a in large applied

fields [10]. The parameter measured in a NMR experi-

ment, namely the enhancement factor of the r.f. field,

is an indirect determination of the transverse (-L z) magnetization due to the collective rotation of the electronic spins. One can as well directly measure

the transverse magnetization [16] or the low frequency susceptibility (xl). We indeed checked the identity

between HA values deduced from NMR and xl

experiments [17]. This anisotropy also induces a shift of the ESR line, either in presence of remanence [18],

or in the zero field cooled (ZFC) state [19, 20].

In this paper [21] we intend to present a series of extensive xl measurements which allows :

-

the analysis of the relationship between ESR

and X, data,

-

the clarification of the properties of the aniso- tropy energy K = cHA and especially its variations

with remanence, temperature and the nature of the system,

-

an insight into the microscopic origin of the anisotropy in spin glasses.

This paper is organized along the following lines.

First, in section 2, we establish that a model based on

the assumption of strongly coupled spins perfectly explains the response of the spin system to a small

transverse field. In section 3, the dependence of K

upon Q at a given temperature is investigated by analysing Q and Xj_ data on the same CuMn sample

for identical cooling processes. We then examine the relationship between ESR and X, in section 4 and the temperature dependence of K in section 5.

The link between the small angle behaviour and the hysteresis loops is discussed in section 6 while the

scaling of K with Mn concentration, and its variation with the addition of non magnetic Au impurities, are analysed in section 7. The microscopic coupling at the origin of this anisotropy, as well as the properties of

the macroscopic anisotropy energy, are discussed in section 8.

2. Transverse susceptibility of a spin glass.

-

Let us

assume that, for T much smaller than T 91 the electronic spins in a spin glass are frozen along their randomly

distributed local fields and that, in presence of a rema-

nence a initially developed along z, they respond collectively to a small field. In this picture a single parameter, the angle 0 between a and z, is required

to fully characterize the magnetic state. Let us describe

the anisotropy forces by an uniaxial anisotropy

energy EA = (K/2) sin2 0. In presence of a transverse

(± z) field h, the total energy of the spin system is given by :

The equilibrium value of 0, in the limit of small devia-

tions, is given by 0,,q = h/HA where HA = Kla is the anisotropy field. Due to the rotation of the remanence_

a transverse magnetization uhjHA appears. Besides

this collective motion slight distortions of the distribu- tion of local fields do exist, as in an antiferroma- gnet [22]. They are responsible for the non zero iso- tropic susceptibility (/;sJ of the ZFC spin glass at

T = 0. As long as we can assume that the response of the spins in presence of remanence is the sum of the two previous contributions, i.e. x;so is not modified

by the existence of a, the total transverse susceptibility

will be given by :

This assumption is reasonable as the existence of 6, which never exceeds 5 % of the saturated high field magnetization of the alloy, is not expected to drasti- cally modify the distribution of local fields. When a

positive static field Ho is applied along z, equation (2)

is modified into :

We have performed xl measurements by a mutual

inductance technique. The cooling field H,, as well as Ho, were produced by a horizontal magnet (Hma. =

13 kG, see figure 1). The magnitude of the vertical a.c.

field h ( v 5 300 Hz) does not exceed 1 G while HA was

never found smaller than 300 G. Therefore the small

angle approximation is fully justified. In order to use

the same samples in ESR, NMR and xl experiments

we have produced foil samples about 40 pm thick.

They have been annealed, in a good vacuum at

500 °C for about one hour, in order to eliminate

stresses due to the rolling process. A well characterized

metallurgical state is then obtained, which indeed was

found to exhibit the same anisotropy properties as the original bulk sample.

In order to analyse the xl data it is necessary to

check the validity of the previous decomposition of xl

(4)

Fig. 1.

-

Geometry of the transverse susceptibility experi-

ment.

into two independent terms. Let us consider for the time being the susceptibility Xiso involved in equa- tion (3) as an unknown parameter Xo which can be

deduced, as well as HA, from an analysis of xl versus

Ho (see Fig. 2). When (XIXO) &#x3E;&#x3E; 1 the fit to equa- tion (3) is not very sensitive to the exact value of Xo.

However when Xl./ Xo 1 any error in the determi- nation of xo yields a curvature in the plot (xl - xo)-1

versus Ho. Then xo is determined with an accuracy

Fig. 2.

-

Transverse susceptibility data versus Ho. The

range of negative Ho has been limited in order to avoid a

reversal of « (see section (6)). On one hand xl data have been plotted versus H 0 and the best fit to a hyperbola has been

indicated which corresponds to HA

=

870 G and a field independent contribution xo

=

9.7 x 10- 5 emu/g identical

to the isotropic susceptibility Xis. as directly measured in the

ZFC state. On the other hand we have plotted (xl - Xir 1,

i.e. the inverse of the transverse susceptibility due to a rotation, versus Ho.

of about 10 % and is always found to agree with the

isotropic susceptibility measured in the zero field

cooled state. This is indeed coherent with the facts that :

- x;so does not depend appreciably upon the static field Ho in our experimental conditions : T Tg and I Ho I I kG [17, 5],

-

the longitudinal susceptibility in presence of

remanence is found to coincide with Xi,,. within a good

accuracy - 5 %; the initial slopes of magnetization

curves are indeed known to be identical whatever

Q [16,15].

We have therefore systematically measured Xiso in the ZFC state and plotted (åX)-1 = (xl - Xiso)-1

versus Ho. In the case of figure 2 for the CuMn 4.7 % (Tg ’" 30 K) at T = 4.2 K in presence of a saturated

remanence, the straight line fitting the data yields from equation (3) 820 G HA 950 G. We have taken

care to start the xl measurements at sufficiently long

time (one hour) after reducing H, to zero in order to

minimize the variations of r during the time of the

experiment. The validity of equation (3) is confirmed

as the inverse slope of the straight line fitting the data

in figure 2, (2.95 ± 0.22).10-1 emu/g, coincides with

a = (2.7 ± 0.1).10-1 emu/g, directly measured in the

same conditions. Therefore equation (3) with a well

defined value for HA perfectly explains the response of the spins to a small transverse field at T Tg.

All the remanence is involved in the rotation pro-

cess. At this step we cannot assert from xl data alone whether all the Mn spins are involved in the collective rotation. Some Mn spins, bearing negligible resultant magnetization, might indeed be excluded. However

analysis of the intensity of NMR signals [3, 4] revealed

that the fraction of spins which participate to the

collective rotation certainly exceeds 50 % (’).

It is well known that HA strongly depends upon the

magnetothermal history of the sample [4]. At a given temperature, larger HA values are associated with smaller remanences. The anisotropy energy K = aHA might a priori vary with remanence, cooling process and temperature. In a first step let us consider the

dependence of K upon Q at a given temperature.

3. Dependence of K upon a at a given temperature T Tg.

-

As all the remanence is involved. in the rotation process the anisotropy energy can be equi-

(1) Let us recall here the arguments developed in refe-

rences [3, 41 to reach this conclusion. The fraction of spins

involved in the NMR signal does not vary by more than a

factor 2 whatever the Q value and the temperature in the range 0 T Tg/3. As for T Tg nearly all the Mn spins

are frozen and therefore contribute to the ZFC signal, the experimental accuracy allows then to conclude that more

than 50 % of the spins are involved in the collective rotation

detected for non zero remanence.

(5)

Fig. 3.

-

Transverse susceptibility due to a rotation in zero

applied static field, A/(0), plotted versus the square of the remanent magnetization in a logarithmic scale. A x(0) and Q

are measured after identical magnetothermal history at a

time t after reduction of He to zero. The corresponding rema-

nence curves are shown in the insert. A straight line with slope unity fits the data, which demonstrates that

does not depend upon at a given temperature.

valently determined according to equation (2) as

K = A x(0) H1 or K = u2[AX(O)]-t, where

Ax(0) = xl - x;so in zero applied static field. The last formulation is the only available when HA is very large (practically HA larger than a few kG), as a direct deter- mination of HA from the variation of AX versus Ho

becomes inaccurate. In order to clarify the dependence

of the anisotropy energy upon the magnetic state we

have therefore performed systematically xl and a mea- surements on the same CuMn samples after identical

magneto-thermal histories. In both experiments, the

external fields have been applied during the same time,

decreased at the same speed, and Ax(0) and a have

been measured at the same moment of their time evo-

lution. All the magnetization measurements have been

performed by an extraction method in Grenoble, in col-

laboration with J. J. Pr6jean. The data for A x(0) and u, concerning the 4.7 % sample at 4.2 K for various

cooling processes, are summarized in figure 3. The

variations of Ax(0) versus U2 in a logarithmic scale

fit a straight line of slope unity. This demonstrates that the anisotropy energy K = U2[LBX(0)]-1 does

not depend upon a at a given temperature. This result

Fig. 4.

-

log J (filled symbols) and log [AX(O)] III (empty symbols) in arbitrary units versus log t. Origin of time is

taken when the cooling field has been decreased to zero.

Parallel straight lines can fit the time variations of both

quantities.

is strictly demonstrated only for J values larger than

one tenth of the saturated remanence. Its validity for

lower Q values cannot be checked from xl experi-

ments with our experimental set up. From the straight

line drawn in figure 3 we obtain K = 220 erg/g for the CuMn 4.7 % at T = 4.2 K.

Let us focus our attention on the two data points corresponding to the highest values on figure 3.

They have been measured at t = 5 min. and t = 45 min.

after cooling the sample under 13 kG. The complete

time evolution of both Q and Ax(0) during the first

45 min. is detailed in figure 4 where log J and log [AX(O)]’I’ are plotted versus log t. The important

feature is that parallel curves fit the time variations of both quantities. This means that ex(0) is proportional

to (J2(t), without any assumption on the exact function a(t) [23]. In other terms HA varies in time like (J-I.

Therefore time variations of xl are by no means negli- gible, especially when T is not very low compared to Tg. This has lead us to take severe precautions, all along this work, in order to ensure that J does not

vary during the measurements of xi versus Ho.

Therefore, at a given temperature T T g’ a well-

defined anisotropy energy K characterizes the aniso- tropy of the system. The transverse response of the

spins is also probed at higher frequencies (- 55 MHz)

in NMR experiments [4]. We have checked in many cases, as in reference [17] that K values deduced from xl and NMR experiments perfectly coincide. At this stage it seems rather important to clarify whether the

same values of K also explain ESR data.

4. Comparison between ESR and Xl. data.

-

Let us briefly summarize the experimental situation concern- ing ESR data. We shall in a first step distinguish

between two opposite limits. First an ESR mode has been detected in presence of a high (saturated) rema-

nence, in nearly zero applied field for a suitable choice

of the frequency of the spectrometer [18]. The reso-

(6)

nance, is then entirely associated with the remanent

magnetization. It is found to behave quite similarly

to a ferrimagnetic resonance in presence of an uniaxial

anisotropy, fitting in first approximation

In this picture the zero field resonance frequency COA

provides a determination of the anisotropy field. In an opposite limit, ESR has been observed in a ZFC

sample in fields low enough to only induce negligible

remanence [19]. Data for various concentrations yield

then a non zero resonance frequency when Ho -1- 0

and fit OJ = ayHo + m(0) for small Ho with a close to 1/2.

While the resonance in presence of remanence

is fairly easily understood by analogy with a ferri- magnet, interpretation of the ESR in the limit of

vanishing a requires a detailed analysis of equations

of motion in the spin glass state.

This has been done by Schultz et al. [19] (and by

Saslow [24, 25] using slightly different methods) in the

framework of a macroscopic model based on the following free energy :

where M is the total magnetization. n is a unit vector

which allows to characterize the rotation of the spin system and which is aligned along a in presence of

remanence. The two first terms of equation (4) repre- sent the magnetic free energy associated with the non remanent part of the magnetization when keeping

the possibility of two different values of the suscepti- bility along and perpendicular to n. We shall here-

after indeed assume, in agreement with experimental

results in CuMn (see section 2), that xo = XII = Xi,..

The third term of equation (4) is the Zeeman coupling

The last one modelises the anisotropy energy, N

being a fixed unit vector directed along the anisotropy

axis. In presence of remanence and in zero external field the minimum of the free energy is given by

n = N and M = Qn. In this case N is the direction z

of the cooling field and equation (4) is therefore

exactly the free energy implicitely used in section 2.

This can be easily seen as, writing for example

with

in presence of the static field H = Ho N + hu, where

u is a unit vector -1 N, we indeed obtain the trivial identity Mo = x;so H, and

which, in the limit of small 0 yields equation (3) [26],

that is :

Equations of motion for M and n, and then resonance

frequencies, have been derived from equation (4) by Schultz et al. [19] neglecting dissipation processes.

In the limit X" = xa = x;so their result for the two resonance modes is given by :

for arbitrary cooling conditions. Let us focus our

attention on the mode labelled + which is the one

usually observed up to now. In the limit of high rema-

nence, when the conditionv/k-/--xi7. a/xi.,. is satisfied, equation (6) yields

Table I.

-

Comparison between values of K deduced from ESR and xl data on the CuMn 4.7 % sample. In the first columns, we have indicated the parameters of the ESR experiments : cooling process, temperature, remanence, isotropic susceptibility. From the resonance frequency in zero external field, we deduced a value for K, using equa-

tion (6), which is compared with K deduced from xl data at the same temperature.

(a) The error bars on a have been slightly increased in order to include time variations, as the time at which the

resonance has been observed is not known accurately.

(7)

Assuming moreover a &#x3E;&#x3E; XHO equation (7) becomes m/y = Ho + K/Q, i.e. a ferrimagnetic like mode. On the other hand, for vanishing 0’, equation (6) is sim- plified into :

which provides an initial slope + 1/2 in the plot w/ y

versus Ho while m(0)/y = (KIX)11’. This mode pre- sents a strong analogy with the resonance in an anti- ferromagnet at T 0 0 as derived by Keffer and Kittel [27].

As long as (1 and x;so can be measured independently

in the same conditions, K is the single parameter involved in the previous theory. Comparison of xl and ESR experiments therefore provides a fundamen-

.

tal test of its validity. This has been performed on the

4.7 % CuMn sample as we could measure a and X,

on the foil sample studied in ESR by Monod and

Berthier [18]. In presence of saturated remanence at T = 4.2 K the resonance is observed in zero

applied field for v = (2 250 ± 50) Mz [28]. Using the

measured values x;so = (9.7 ± 0.8). 10-’ emu/g and

(1 = (2.45 ± 0.20). .10-1 emu/g, we deduce from equa- tion (6) K

=

(260 ± 30) erg/g, to be compared with

K = (220 ± 20) erg/g obtained from X, data of figure 3. This comparison, and similar ones, are’

summarized in table I. In the case of the saturated

remanence at T

=

1.5 K, w/y versus Ho has been

moreover determined [18]. A careful analysis reveals

that the slope is slightly reduced with respect to the paramagnetic gyromagnetic factor y. The field dependence of w/y is in perfect agreement with

equation (7). ESR in the same 4.7 % CuMn sample

has also been observed in the ZFC state at T = 2.2 K [28]. The remanence induced by the field applied to detect this resonance (H,. - 2 350 G) is

indeed negligible and the measured value of the shift of the ESR, 6H = (w/y - Ho) = (960 ± 40) G, yields

from equation (8) K = (280 ± 35) erg/g. This result

perfectly coincides with the value of K deduced from ESR and xl data in presence of remanence. So at

T Tg the same value for K can fit ESR and xl data,

whatever the cooling conditions, in the framework of

equations (3) and (6). This establishes the validity of

the previous phenomenological macroscopic descrip-

tion of the spin glass. Let us point out that it is valid at T Tg for a range of frequencies extending from a

few Hz (a.c. susceptibility) to a few GHz (ESR). How-

ever it is clear that such an approach will fail to describe

the spin glass properties in the limit of extremely low frequencies (v 1 Hz) when « internal » modifica- tions of the spin glass state do occur, as revealed for

example by the existence of magnetic after effects.

In consequence one can expect that its frequency

range of validity will be reduced at higher tempera-

tures.

5. Temperature dependence of K.

-

It is possible

to observe the ESR through Tg and it has been already

known for a long time that the shift of the resonance 6H

only vanishes above Tg [30]. Assuming the validity of equation (6) at all temperatures, including T &#x3E; Tir

Schultz et al. deduced K(T)

=

K(0) [1

-

TII.5 Tg]

(where Tg = 0.9 Tg is the temperature of the peak of

the susceptibility in 3 kG applied field), from their

data for various concentrations [20]. Let us point

out that K(T) is found to be non zero above Tg in a region where no remanence effects are evidenced from

static magnetization measurements [12, 31, 32]. It

would be particularly interesting to do comparisons of

xl and ESR experiments at all temperatures, as the

validity of the previous model checked at T Tg

becomes questionable at higher temperature.

However X, experiments, as performed here, require the existence of a finite remanence during the time of the experiment. They are therefore not appropriate

when T &#x3E; T g. Indeed when T increases towards T g

the time constants involved in the spontaneous decay

of a become shorter and shorter and finally at T - Tg

it is impossible to distinguish the paramagnetic res-

ponse from the remanence without analysing the

transients of the magnetization once the field has been switched off [33]. In our experimental set up we could

only perform experiments in the range 1.5-4.2 K.

It was therefore necessary to study a more dilute alloy than the 4.7 % sample (Tg - 30 K). We report

here results concerning the 1.35 % CuMn sample (Tg - 12 K). In figure 5, AX(O) versusu2 data are plotted at T = 4.2 K and T = 1.5 K for various

cooling processes. The anisotropy energy K, determin-

ed as the inverse slope of the straight line fitting

the data, is found to vary with temperature :

K

=

(13.2 ± 1.4) erg/g at T = 4.2 K and K =

Fig. 5.

-

Transverse susceptibility due to a rotation in

zero applied static field A x(0) plotted versus the square of the remanent magnetization for the CuMn 1.35 % at

T

=

4.2 K (filled symbols) and T

=

1.5 K (empty symbols).

Straight lines fit the data at both temperatures demonstrat-

ing that K

=

a2[LBx(O)]-1 does not depend upon a at a

given temperature but is a decreasing function of tempera-

ture. The associated IRM curves are shown in the insert.

(8)

Fig. 6.

-

Inverse of the transverse susceptibility due to a

rotation in zero applied static field plotted versus tempera-

ture in the range 1.5-4.2 K for a given constant remanence.

This is achieved by cooling the sample in zero applied

field from T

=

4.2 K to 1.5 K after having developed

the saturated remanence at T = 4.2 K. The variation of K oc [AX(O)] - 1 with temperature is clearly evidenced.

(18.6 ± 1.5) erg/g at T

=

1.5 K. A much more accurate method to study this temperature depen-

dence has been to establish a remanent magne- tization at T = 4.2 K and then to cool the sample

in zero applied field. In such a process the rema-

nence is constant as the magnetic after effects which occurred at 4.2 K are drastically slowed down when the temperature is decreased [34]. AX(O) is found to

decrease continuously when the temperature is lowered from 4.2 to 1.5 K (Fig. 6). After heating the sample back to 4.2 K we found again the initial value for AX(O), which corroborates the absence of time evo-

lution of Q during the experiment. The relative in-

crease of [A/(0)] ’ B and therefore of K = a’[AX(O)] - 1,

between 4.2 K and 1.5 K is about 50 %, in agreement with the previous results of figure 5. The temperature variation deduced from figure 6 is consistent with

K(1) = K(0) [1

-

T/Ta] with To

=

(115 ± 3) K.

This result is in rough agreement with ESR results [35].

So K(T) deduced from xl experiments seems to

coincide with K(T) deduced from analysis of ESR data

at least in the range 0 T/Tg 0.3. Further experi-

ments are planned in order to investigate tempera-

tures closer to Tg.

6. Complete study of AX versus Ho in presence of reversals of Q.

-

In AgMn and in CuMn spin glasses

a more or less sudden reversal of «can be induced at T Tg/3 in presence of a high remanence by applica-

tion of negative fields [15]. When cycling the static

field Ho, nearly square and shifted hysteresis cycles are detected, as long as Ho is small enough to develop no

isothermal remanence, i.e. I (J I is kept constant. For example in the case of figure 7, a points down when Ho is decreased below - 550 G, and remains down if

Ho is then increased up to - 450 G. In these conditions xl measurements probe small angle deviations from the reversed equilibrium position. As can be seen on

Fig. 7.

-

Inverse of the transverse susceptibility due to (J rotation, (AX)-’, plotted versus Ho for the CuMn 4.7 %

cooled at T

=

1.5 K under 3.2 kG. Ho is swept downwards from 700 G to - 1 200 G (squares) and then upwards (circles). The corresponding hysteresis cycle, as directly

measured [281 is indicated in the upper part of the figure.

As long as a is along z, xl data fit equation (3) with HA

=

(800 ± 50) G .

When Q has been reversed we find HA

=

(70 ± 50) G.

Data are found symmetrical with respect to Ho

= -

370 G.

The inverse slope of the two straight lines fitting the

data coincide with the value of Q directly measured (2.8 + 0.1 ) .10-1 emu/g.

figure 7 a straight line of slope a-’ fits (LBX)-1 data

versus Ho :

but the anisotropy field deduced from this analysis HA = (70 ± 50) G, differs from the value HA = (800 ± 50) G measured when a points upwards, data being symmetrical with respect to Ho = - 370 G and

not to Ho = 0.

These features are common to all xl or NMR

experiments as long as a can be reversed. From these

data alone one cannot infer anything on the relation- ship between the states with a up and down which

might merely have different and independent uni-

axial anisotropy energies. But on the other hand the existence of shifted hysteresis cycles has been com- monly interpreted by introducing uniaxial and unidi- rectional contributions to the anisotropy energy :

Such an equation indeed predicts sudden reversals of a

from 0 to n for Ho = - (Hax + Hd) and from n to 0

for Ho = HaX - Hd, where Hax = Kax/u and

Hd = Kd/U. For small angle behaviour one obtains :

(9)

where 8 = sign (a.z). This equation is equivalent to equations (3) and (9), with HA = Ha. + Hd and HA

=

Hax - Hd, as in a small angle approximation

one cannot distinguish between uniaxial and unidirec- tional contributions.

Experimentally the centre of symmetry of xl data

roughly coincides with the centre of the hysteresis cycle (which is directly seen in the xl experiments).

However the width of the hysteresis cycle is always

much less than 2 H ax deduced from the fit of xl data to equation (11). Therefore equation (10), where KaX and Kd are determined to fit the small deviations from 0=0 and 0 = n, does not explain the reversals of a. The reversals of a are in fact complicated proces-

ses and not simple 7c rotations. Indeed an intermediate state, where the longitudinal remanence is zero, can be

stabilized. This state, for which no transverse magne- tization could be detected, is rather divided in magne- tic domains bearing opposite remanences [14, 36].

Therefore the single domain picture of equation (10),

with KaX and Kd determined from xl measurements,

might still apply for large 0 although it does not

describe the reversals of a. Experiments, where a

true progressive rotation of a can be induced, would

check the angular dependence of EA (ESR, xl or torque measurements). At present torque experiments

Fig. 8.

-

Inverse of the transverse susceptibility due to a

rotation plotted versus Ho for a CuMn 4.7 % at T

=

4.2 K

(filled symbols) and T

=

1.5 K (empty symbols) in presence of the same remanence : the sample has been cooled under

13 kG at T

=

4.2 K and then in zero applied field from 4.2 K to 1.5 K. The field was swept downwards from 1000 G to - 1 100 G (circles) and then upwards in the same range

(squares). Identical slopes fit data at both temperature which demonstrates the invariance of (1. The centre of symmetry of xl data is multiplied by 1.7 when T is lowered from 4.2 to 1.5 K while HA only varies of - 15 %. The width of the hysteresis cycle is simultaneously reduced by a factor - 3.

were only performed in a case for which the unidirec-

tional contribution was dominant [13].

So, as long as 6 can be reversed, two parameters HaX and Hd (or HA and H’) are required to fully des-

cribe the small angle deviations of J from its two

equilibrium positions. As the independence of

K = KaX + Kd upon and its temperature variations

are well established, it is natural to wonder whether

Kax and Kd separately follow the same dependences,

and whether there is a general relationship between HaX and the width of the hysteresis cycle AH. At a given temperature alld is found to be roughly cons-

tant. This invariance could only be tested from xl data when reversals occur, i.e. for Q &#x3E; 6Sat/3, and is

far less accurate than the invariance of aHA. For example for the two states obtained by cooling the

4.7 % CuMn under 13 and 3.2 kG at T = 4.2 K the

respective ratios of y, HA, Hd values are (1.19 ± 0.03), (1.16 ± 0.12) and (1.48 ± 0.20). Similarly at a given temperature J AH is found to be roughly constant.

In order to clarify the temperature dependences- we

have performed a detailed study of Ax versus Ho at

T = 4.2 K and T = 1.5 K, for the 4.7 % CuMn, in

presence of the same remanence, as ensured by the

fact that the data can be fitted at both temperatures by straight lines with identical slopes (Fig. 8). We observe

an important change of the unidirectional anisotropy

field : Hd

=

(220 ± 20) G at T = 4.2 K and Rd

=

(380 ± 20) G at T = 1.5 K, while HA only varies of

15 %. The width of the hysteresis cycle ’is simulta- neously reduced by a factor - 3. This tendency to an

increase of the displacement field of the hysteresis cycle

and to a reduction of its width for decreasing T can also

be detected in the magnetization data of reference [15].

It could be inferred from figure 8 that the observed variation of HA between 4.2 K and 1.5 K is entirely due

to a change in the undirectional anisotropy field Hd, the

uniaxial contribution Hax remaining unchanged. We

are not able at this stage to clarify whether this is an

universal behaviour.

In conclusion the hysteresis cycle characteristics do not reflect exactly the properties of the anisotropy

energy as deduced from X, measurements in the states with a up and down. Let us point out moreover that

the hysteresis cycles can only be observed in the limit where the negative field required to inverse a is low enough to induce only negligible negative isothermal

remanence. As soon as K is large, as in AuFe [17],

no cycles are detected even in presence of the saturated

remanence [34], while K can be determined in‘ any system from the zero field measurement of xi. The existence of a unidirectional contribution Kd to the anisotropy energy, which seems to be confirmed by

the unique torque experiment [13], has received at present no decisive interpretation. A given number

of spins, bearing no macroscopic magnetization and

not involved in the collective rotation, could induce a

constant field independent upon a direction, as was

first suggested by Kouvel [16]. As recalled in section 2

(10)

up to now NMR data only allow to ensure that 50 %

at least of the spins are involved in the rotation induced

by the r.f. field.

7. Scaling laws of K. - 7.1 CONCENTRATION

DEPENDENCE OF K.

-

In order to clarify the depen-

dence of the anisotropy energy versus Mn concentra- tion in CuMn $pin glass, we have extended our

measurements to 0.6, 1 and 9 at. Mn alloys. Results

are summarized in figure 9, where the anisotropy

energy per atom has been plotted versus the Mn

concentration. Comparison of alloys of different

concentrations in principle requires to extrapolate K(7’) at zero temperature. This was done for the three

highest concentrations using the variation of K(T)

inferred from xl data in the range 1.5-4.2 K. However for the two lowest concentrations, as this extrapola-

tion would not be accurate, we have indicated K as

measured at T = 1.5 K, which provides a lower

estimate of K(T = 0). It is found to increase linearly

with c at a rate of 12.8 ± 1 (G. 9B/at.)/%, at least for

c &#x3E; 1.35 %. For lower c a small disagreement appears

(which is indeed stronger if T corrections are done).

Whether this is a spurious effect linked with residual

, metallurgical defects or impurities (see section 7.2) is

. at present unclear. The concentration dependence of K, 14.5 ± 0.6 (G./at.)/%, deduced from ESR data [19], for c &#x3E; 2 %, is in good agreement with our results which establishes once more the identity

between the values of K deduced from ESR and X, experiments.

We have also investigated the concentration depen-

dence of K in AgMn spin glass in the range 2.8-14.5 %.

We have deduced HA from the field variation of xl and determined K as Ax(0) H 1. Temperature varia-

tions have been neglected. For the 5 and 10.4 % alloys,

for which Q has been moreover measured indepen- dently [37], we checked again the validity of equa- tion (3). The anisotropy energy per atom (see Fig. 9) is

found to increase linearly with c at a rate of (14 ± 1)

Fig. 9.

-

Anisotropy energy per atom versus the Mn concentration in CuMn and AgMn spin glasses. The straight line indicates the best fit to a linear variation.

(G. pB/at.)/% very similar to the one measured in CuMn

spin glass. Let us point out that this linear relation holds even at high concentrations for which the

validity of usual scaling laws [9] is not ensured [37].

7.2 INFLUENCE OF ADDITIONAL IMPARITIES.

-

Anisotropy energy in spin glasses is enhanced by intro-

duction of metallurgical defects by cold working [38]

and by addition of non magnetic impurities. The study by Prejean et al. of hysteresis cycles on CuMn1% Au., samples (with x between 0.01 and 0.15 at.% [39]) provide up to now the most systematic investigation

of the effect of non magnetic impurities. The rema-

nence properties, the isotropic susceptibility and the spin glass temperature are not modified by the addi-

tion of Au. But the width of the hysteresis cycles (determined after the same cooling process) is shown

to increase at a linear rate with gold concentration from its value in pure CuMn 1 %. However the

study of hysteresis cycles presents a few intrinsic limitations. First they disappear when x &#x3E; 0.15 %.

Moreover, as seen here above, the anisotropy energy

Table II.

-

Transverse susceptibility data for CuMn1o/o Aux alloys cooled under 13 kG at T

=

1.27 K. For x &#x3E;, 0.1 %, one cannot detect the field dependence of xl with a sufficient accuracy and the hysteresis cycles disap-

pear. The only available quantity is then the transverse susceptibility Ox(0) due to the magnetization rotation measur-

ed in zero applied field. a calculated as AX(O) HA (last column), when HA can be directly determined, is found to be

constant and to be insensitive to the addition of Au, while HA, Hr and [A X(O)] - ’ are found to increase linearly with x from their values in pure CuMn. Our experimental conditions are similar to those of reference [39]. The slight diffe-

rence between a values is very likely due to the fact that He in cycle exper.iments has been switched off at a slightly

higher temperature than in xl experiments (J. J. Préjean, private communication).

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