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Magnetic properties and phase transitions of RAlxGa2-x (R = Tb, Ho)

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HAL Id: jpa-00218977

https://hal.archives-ouvertes.fr/jpa-00218977

Submitted on 1 Jan 1979

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Magnetic properties and phase transitions of RAlxGa2-x (R = Tb, Ho)

K. Girgis, P. Fischer

To cite this version:

K. Girgis, P. Fischer. Magnetic properties and phase transitions of RAlxGa2-x (R = Tb, Ho). Journal de Physique Colloques, 1979, 40 (C5), pp.C5-159-C5-161. �10.1051/jphyscol:1979560�. �jpa-00218977�

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JOURNAL DE PHYSIQUE Colloque C5, supplément au n° 5, Tome 40, Mai 1979, page C5-159

Magnetic properties and phase transitions of RA^Ga^ (R = Tb, Ho)

K. Girgis

Institut fur Kristallographie und Petrographie, ETHZ, CH 8092 Zurich, Switzerland

and P. Fischer

Institut fur Reaktortechnik, ETHZ, CH 5303 Wtirenlingen, Switzerland

Résumé. — On a étudié la structure cristalline et des propriétés magnétiques des composés RAlxGa2_x

(R = Tb, Ho : 0 ^ x ^ 2,0) par diffraction des rayons X et des neutrons, microanalyse et mesures de la sus- ceptibilité.

Abstract. — Crystal structure and magnetic properties of RAlxGa2_x (R = Tb, Ho ; 0 ^ x < 2.0) were inves- tigated by means of X-ray and neutron diffraction, microprobe analysis and measurements of magnetic suscep- tibility.

Introduction. — RA12 crystallize with cubic struc- tures of MgCu2 type (Laves phase) and order predo- minantly ferromagnetic [1]. On the other hand the antiferromagnetic RGa2 occur with hexagonal AIB2

type structure. Many other compounds of Al and Ga are isostructural [2]. Magnetic structures of RGa2

were investigated at Grenoble [3]. We determined [4]

the influence of Ga substitution by Al in RGa2 on crystal structures and magnetic properties. One anti- cipates enhanced exchange associated with modified interatomic distances and band structures. Similar investigations concerning RAlGa (R = Tb, Ho) were published recently by Gignoux and Asmat [5]. In contrast to this study our results furnish clear evi- dence for magnetic phase transitions in RAIGa and substantially increased Neel temperature of TbAIGa compared with TbGa2. Coexistence of two helical phases is found in TbAl0-5Ga1-5.

1. Sample preparation, metallographic and X-ray investigations. — The samples were synthesized in an arc furnace in purest argon atmosphere from 99.999 % gallium (Alusuisse), 99.99 % aluminium (Alusuisse), 99.9 % holmium (Johnson, Matthey and Co., Ltd.) and 99.9 % terbium (Johnson, Matthey and Co., Ltd.) and remelted several times. The ingots were enclosed under vacuum in tantalum containers, homogenised at 1 000 °C for 24 h and finally annealed at 600 °C for 72 h. The samples were examined metal- lographically, by microprobe analysis and X-ray diffraction. The specimens prove to be homogeneous and correspond well to the nominal compositions.

Two phases exist in the composition range RAlxGa2_:!C. The A1B2 phase exists over a range of

x = 0.0 to 1.6, the MgCu2 phase from x — 1.25 to 2.0, i.e. both phases coexist in the range x = 1.25

to 1.6. Concerning substitution of Ga by Al the cell constants of the A1B2 phase show a remarkably nonlinear dependence, whereas the change of the MgCu2 cell constants is small and linear (cf. figure 1).

HoAlxGa2-x 2 AIB2 .

~Z MgCu2 i

I a A

•2 I oi 7.90 MgCu2 | MgCu2*AIB2

* 7.80 r | - • » - , _ , — 1 _

y 7.70 I

I cA

J 'i0°

I / -3.90 I / -3.80 1 / -3.70

^ ^ ^ -3.60 _ a A c •*•—:- ' — * —

•< t I "3-50

| 4.50- , o- a | .«

m'4.40- ..

< I ^ v .

•fe 4.30- I \ .

3 4-20- I N

* I , 1 , J

0 0.5 1.0 1.5 2.0 6a concentration

Fig. 1. — Cell constants (A) versus Ga-content in HoAl^Ga^^

series.

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphyscol:1979560

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C5-160 K. GIRGIS AND P. FISCHER

2. Magnetic susceptibility. - Figure 2 shows an example of the susceptibility measurements of TbAIGa, where (similar to HoAIGa) two transitions can be recognised.

, xmole-'

I I

20 -40 $0 80 160 1i0 110 160 1b Temp(K) Fig. 2. - Susceptibility measurements of TbAlGa compound (emu).

3. Neutron diffraction studies. - Powder samples of RAI,Ga,

-.

(cf. table I) were investigated by neutron diffraction at Wiirenlingen. Illustrative, absorption corrected patterns (wavelength 2.35 A) are shown in figure 3. The nuclear intensities confirm the AlB,- structure model with statistical distribution of A1 and Ga on B sites. RAl,Ga,-, (R = Tb, H o : x < 1)

order antiferromagnetically (cf. figure 3 and table I).

At x = 1 NCel temperatures are considerably larger compared to x = 0. The low temperature magnetic structure of HoAlGa (cf. figure 4) corresponds to Shubnikov group P,6/mcc and is similar to CsCoCl, [6]. The incommensurate configurations are spiral structures of triangular type within (001) planes [phase angles f (120°, 240°)], with propagation direction c (K = [113, 113, q]) and q increasing syste- matically with composition x.

Table I. - Neutron results for RAI,Ga, -,. T, = Nkel tempe'rature, T, = temperature of magnetic phase tran- sition, MS = magnetic structure. A denotes triangular moment conjiguration with undetermined orientation within (001) planes. ,u = ordered magnetic moment.

Standard deviations within parentheses refer to the last digit. * more stable above 15 K .

T, [K] 20.0 [3] 19.3 [5]

T,

4 0.178

{::iW:*

MS A A

Fig. 4. - Low temperature magnetic structure of RAlGa (R = Tb, Ho) [moments reversed at z = 1/21, Signs indicate z components.

Fig. 3. - Neutron diffraction patterns of HoAlGa. At 4.2 K magnetic reflections are indexed with respect to the magnetic (a, = 3 a, c, = 2 c ) unit cell. 0, = + q.

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MAGNETIC PROPERTIES AND PHASE TRANSITIONS O F RAI,Ga,-, (R = Tb, Ho) C.5-161

References

[I] WALLACE, W. E., Rare Earth Zntemetallics (Academic Press, [5] GIGNOUX, D. and ASMAT, H., Phys. Status Solidi (a) 45 (1978)

New York) 1973. K 149.

[2] GIRGIS, K., Monatsh. Chem. 101 (1970) 721. [6] MELAMUD, M., PINTO, H., MAKOVSKY, J. and SHAKED, H., [3] ASMAT, H., GIGNOUX, D. and LEMAIRE, R., Physica 86-888 Phys. Status Solidi (b) 63 (1974) 699.

(1977) 185.

[4] FISCHER, P. and GIRGIS, K., Wiirenlingen report AF-SSP 106 (1978) 10 and 102 (1977) 21.

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