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170Yb Mössbauer study of the crystalline electric field and exchange interaction in YbFe2 : addendum

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HAL Id: jpa-00208922

https://hal.archives-ouvertes.fr/jpa-00208922

Submitted on 1 Jan 1980

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170Yb Mössbauer study of the crystalline electric field and exchange interaction in YbFe2 : addendum

F. Hartmann-Boutron, C. Meyer

To cite this version:

F. Hartmann-Boutron, C. Meyer. 170Yb Mössbauer study of the crystalline electric field and exchange interaction in YbFe2 : addendum. Journal de Physique, 1980, 41 (9), pp.1075-1076.

�10.1051/jphys:019800041090107500�. �jpa-00208922�

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1075

170Yb Mössbauer study of the crystalline electric field and exchange interaction in YbFe2 : addendum

F. Hartmann-Boutron and C. Meyer

Laboratoire de Spectrométrie Physique (*), Université Scientifique et Médicale de Grenoble, B.P. 53X, 38041 Grenoble Cedex, France

(Reçu le 26 mars 1980, accepté le 22 mai 1980)

Résumé. 2014 Dans la référence [1] nous avons calculé le potentiel cristallin V2 induit par la magnétostriction dans

la série RFe2, en supposant | 03BB100 | ~ | 03BB111 |, comme cela était admis à l’époque par un certain nombre d’auteurs.

Cette hypothèse s’étant révélée non fondée, nous établissons pour V2 des expressions nouvelles qui sont valables quels que soient 03BB100 et 03BB111.

Abstract.

2014

In reference [1] we derived an expression for the crystalline potential V2 induced by magnetostriction

in the RFe2 series, using the assumption, generally accepted at the time, that | 03BB100 | ~ | 03BB111 |. This assumption

has now been shown to be unfounded. We therefore derive new expressions for V2, which are valid whatever

03BB100 and 03BB111.

J. Physique 41 (1980) 1075-1076 SEPTEMBRE 1980,

Classification

Physics Abstracts

76.80

-

75.30

In reference [1], using a simple model, we tried to

estimate the contribution of magnetostriction to crystalline field effects and magnetocrystalline aniso- tropy in the RFe2 series (except for GdFe2, since Gd3+

is an S state ion). At that time, it was more or less admitted in the literature [2] that in this series

For this reason, while eqs. (12) to (24) of [1] are valid

whatever Âloo and Âlll, we dropped the terms in Âloo

in eqs. (29) to (34).

The assumption that ! 10 0 1 « 1 )"111 I was based

on a comparison between the magnetostriction coeffi-

cients of DyFe2 (Àl00 (0 K) = - 70 x 10- 6) and of TbFe2 (111 (0 K)

=

4 400 x 10-6) [2]. Since then, magnetostriction studies have also been performed

on HoFe2 [3]. ;,100 was determined between 300 K and 0 K while à, 111 (hard axis) could only be measured

between 300 K and 270 K. At 270 K, )" 111 1 is about

2.5 times larger than 1 ;,10, but, because of différent thermal variations, its extrapolated value at 0 K,

776 x 10-6 is almost nearly equal to the value

measured for Hioo! (745 x 10-6). Consequently 1 ;, 10 0 1 - 111 ! and the assumption of reference [2]

is not verified. In addition 1 )"100(0 K) 1 for HoFe2

is ten times larger than that for DyFe2 (while still

remaining six times smaller than 2111 (0 K) for TbFe2).

In view of these results, it seems useful to give

corrected expressions for the crystalline potential V2,

eqs. (30) and (31) of [1], when the term in ,1100 is

retained :

or alternatively :

Eqs. (32), (33) and (34) of [1] are no longer valid.

However comparison of (31’) with eq. (23) for the magnetostrictive anisotropy energy KME :

shows that V2 and KME still have comparable orders

of magnitude. Since both quantities contain /oo

(*) Associé au C.N.R.S.

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:019800041090107500

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1076

and à,f i i , they are negligible (less than 1 cm-1) when

calculated with the small values of à,ioo and ;,.111 1 corresponding to HoFe2. Appreciable contributions to V2 and KME will only be obtained with high  values comparable to the Î..lll’S of TbFe2 or TmFe2. The

conclusions of reference [1] then remain unaltered, except for the fact that now V2 is always non zero (but it still depends on the magnetization direction

and it is still too small for explaining the crystal

field variations in the series).

Some additional remarks must be made. In refe-

rence [1], p. 409, note (5), we said that K2 « K1. In reality this is not true at low temperature. On the other hand, one should not forget that the physical

effects of the anisotropy are not characterized by Kl and K2, but by the maximum angular variations, 1 K1 /3 1 and K2/27 1, of the two contributions to the

anisotropy energy (Eq. (A.9) of [1]), as one rotates

the magnetization. The order of magnitude of these quantities at 0 K in the whole series can be estimated with the help of eqs. (A. 10) and (A. 11) of [ 1], together

with tentative values of A4 r4 > and A6 r6 > (1) : 1 K2 (0 K)/27 is found to be smaller than or compa- rable to K1 (0 K)/3 ( but certainly not much smaller.

Therefore, in connection with note (5) of reference [1],

p. 409, the fact of neglecting terms of order higher

A6 a8/kB

= -

1 K and we used the r4 >4f, r 6 )4f values of

Freeman and Watson (Phys. Rev. 127 (1962) 2058); the numerical

results of this calculation are given in C. Meyer’s Doctoral Thesis (Grenoble, 1980). Note that in reality, as shown in [1], A4, A6

are not constant.

than two in the computation of the additional crystal-

line potential due to magnetostriction, must only be

considered as a (widely used) simplifying assump- tion [4], justified by the lack of information concern-

ing the exact mechanisms involved in this change.

Finally one should also recall the limited validity of

the description of anisotropy effects in terms of an anisotropy energy (Eq. (A. 9) of [1]). Strictly speaking,

it can only be valid if the modulations (of the order 1 Kl (0 K)/6 , K2 (0 K)/54) 1) of the Zeeman energy levels of the Rare Earth ion by crystal field effects when the magnetization rotates, are appreciably

smaller than the Zeeman interval 2(gj - 1) IÀB Hex 1

associated with the RE-Fe exchange field. With /’B H,,,,IkB - 150 K and the above mentioned tentative values of the crystalline field, it is found that (except

for Pr3 +) K1 (0 K)/6 and K2 (0 K)/54 are indeed

smaller than the Zeeman interval, but only by a factor

of the order two to five so that the validity condition

is practically never satisfied. Therefore, for precise

calculations it is necessary to use the exact free energy,

as was done in the investigations of ternary phase diagrams [5] and in our own work [6] ; however in

view of the uncertainty on A4 and A6 the simpler description in terms of an anisotropy energy is still of great interest when only orders of magnitude esti-

mates are needed, as in reference [1]. The same remark applies to the standard treatment of magnetostric-

tion given in [1] and also to the Callen and Callen

law [7], [3] :

for the thermal variation of magnetostriction.

References

[1] MEYER, C., GROS, Y., HARTMANN-BOUTRON, F., CAPPONI, J. J., J. Physique 40 (1979) 403.

[2] CULLEN, J. R., CLARK, A. E., Phys. Rev. B 15 (1977) 4510.

HATHAWAY, K. B., CULLEN, J. R., J. Appl. Phys. 49 (1978) 1975.

[3] ABBUNDI, R., CLARK, A. E., KOON, N. C., J. Appl. Phys. 50 (1979) 1671.

[4] For a recent discussion on this subject see CAMPBELL, I. A., CREUZET, G., SANCHEZ, J., Phys. Rev. Lett. 43 (1979) 234.

[5] ATZMONY, U., DARIEL, M. P., DUBLON, G., Phys. Rev. B 15 (1977) 3565.

[6] MEYER, C., SROUR, B., GROS, Y., HARTMANN-BOUTRON, F., CAPPONI, J. J., J. Physique 38 (1977) 1449.

[7] CALLEN, E., CALLEN, H. B., Phys. Rev. 139A (1965) 455.

CALLEN, H. B., CALLEN, E., J. Phys. Chem. Solids 27 (1966)

1271.

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