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170Yb Mössbauer study of the crystalline electric field and exchange interaction in YbFe2
C. Meyer, Y. Gros, F. Hartmann-Boutron, J.J. Capponi
To cite this version:
C. Meyer, Y. Gros, F. Hartmann-Boutron, J.J. Capponi. 170Yb Mössbauer study of the crystalline electric field and exchange interaction in YbFe2. Journal de Physique, 1979, 40 (4), pp.403-415.
�10.1051/jphys:01979004004040300�. �jpa-00209121�
170Yb Mössbauer study of the crystalline electric field and exchange interaction in YbFe2
C. Meyer. Y. Gros. F. Hartmann-Boutron
Laboratoire de Spectrométrie Physique (*), Université Scientifique et Médicale de Grenoble, B.P. 53X. 38041 Grenoble cedex, France
and J. J. Capponi
Laboratoire de Cristallographie du C.N.R.S., B.P. 166X, 38042 Grenoble cedex, France.
(Reçu le 28 septembre 1978, révisé le 29 novembre 1978, accepté le 4 décembre 1978)
Résumé.
2014Nous avons étudié l’effet Mössbauer de 170Yb dans YbFe2 entre 4,2 et 60 K. Les spectres hyperfins
sont compatibles avec une direction de facile aimantation suivant [100]. Les variations thermiques du champ hyperfin et du couplage quadrupolaire électrique suggèrent que les effets de champ cristallin sur l’ion ytterbium
sont réduits, et les courbes s’interprètent bien en le supposant seulement soumis à un champ d’échange (03BCB, Hex/kB
=111 ± 4K);
la contribution des électrons de conduction au champ hyperfin est Hc
=240 ± 100 kOe et le facteur d’écran de Sternheimer est RQ
=0,22 ± 0,01. En relation avec la petitesse du champ cristallin, nous examinons l’influence de la magnétostriction sur le potentiel cristallin vu par un ion de terre rare dans les composés RFe2.
Abstract.
2014The Mössbauer study of 170Yb in YbFe2 was performed in the temperature range 4.2-60 K. The
hyperfine spectra are in agreement with an easy direction of the magnetization along [100]. The thermal variations of the hyperfine field and of the electric quadrupole coupling suggest that the crystalline field effects on the ytter- bium ion are rather small and we get good least square fits with pure exchange only (03BCB Hex/kB
=111 ± 4 K) ;
the corresponding values of the conduction electron field and of the Sternheimer shielding factor are respectively Hc
=240 ± 100 kOe and RQ
=0.22 ± 0.01. In connection with the smallness of the crystalline field, we discuss the influence of the magnetostriction on the crystalline potential seen by a rare earth ion in the RFe2 compounds.
Classification
Physics A bstracts
76.80
-75.30
1. Introduction.
-In a previous paper [1] we
described the synthesis and magnetic properties of
the Laves phase compound YbFe2. Magnetic measure-
ments and 57Fe Môssbauer spectroscopy show that this material is ferrimagnetic and that at low tempe-
rature it is magnetized along a [100] direction. Above 50 K the magnetization seems to slightly deviate
from this direction. In [1] we evaluated the magnetic
moment of Yb3 + in YbFe2 with the help of the crystal-
line field and exchange parameters determined in [2]
by Yanovsky et al. from the Môssbauer effect of l’°Yb
as an impurity in the similar compounds TmFe2 and
(*) Associé au C.N.R.S.
TmxHo1-xFe2 (x
=0.1 ; 0.2) [3]. However TmFe2, magnetized along [111], and TmO.2Hoo.8Fe2l magne-
tized along [ 110] below 40 K, are expected to exhibit important magnetostriction effects at low tempera-
tures and this may influence the crystalline field.
Also the RE-Fe and RE-RE exchange interactions may exhibit some anisotropy, whose manifestations
are similar to a crystalline field and which depends
on the pair of atoms involved (for example Tm-Yb
in TmFe2 : Yb ; Yb-Yb in YbFe2). For these reasons
we performed the Môssbauer study of l’°Yb in YbFe2 to try to determine directly the crystalline
field and exchange interactions in this compound
from the hyperfine data, with a view of comparing
Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:01979004004040300
with the values of [2] and with magnetic anisotropy
data. The whole paper and its appendix 1 are devoted
to this problem. In appendix II we use the results
obtained in order to slightly correct some estimates
of reference [1] which were based on the data of [2].
Also, in connection with recent experiments on NdFe2, we discuss the possible role of an anisotropic hyperfine structure of the iron atoms in the inter- pretation of the 5’Fe Môssbauer spectra of YbFe2
which were reported in [1].
2. Experiment. - The Môssbauer y of 17°Yb has
an energy of 84.4 keV, and it is necessary to cool both the source and the absorber. The apparatus which we use is similar to that of reference [4], which
is characterized by a horizontal movement transmitted to the absorber under vacuum. The 20 mCi source
of 170Tm in TmAl2 is cooled to approximately 15 K through flexible copper wires connected to the helium bath. The minimum linewidth obtained is 2.5 mm/s
with respect to an absorber of YbAl2 at 4.2 K. The
scintillation detector is a 5 mm thick NaI crystal.
The absorber of YbFe2 (about 800-900 mg covering 3 cm2) is a mixture of powders from thirteen different
preparations under 80 kbars. From X-ray powder
data we expect the presence of impurities in the form
of both Yb metal (which was put in slight excess
for the preparation) and YbO (because of unavoi-
dable oxidation) (’). Finally about 40 % of the pre-
parations also contained a very small amount of Yb6Fe23. As this did not appear in the 57Fe spectra
Fig. 1.
-Môssbauer spectra of 17°Yb in YbFe2 at 4.2 K, 20 K and 50 K. The full curve is a theoretical fit with a central impurity
line and with an l’°Yb spectrum composed of five lines with equal height and width.
(1) Most of the unknown X-ray lines mentioned in reference [1]
correspond to YbO. We are indebted to Dr. J. F. Cannon for
suggesting this identification.
we could forecast that it would be absent from the 17°Yb spectra.
Experiments were performed at 4.2 K, 12 K, 20 K,
34 K, 50 K and 60 K . We give in figure 1 the spectra
at 4.2 K, 20 K and 50 K. They exhibit a well defined five lines magnetic hyperfine pattern corresponding
to YbFe2, together with an additional broad line at
zero velocity. We notice that the lines of YbFe2 are
narrow, which indicates that our preparation under high pressure is reproducible. On the other hand,
as far as the statistics can show, the broad central line seems to be best fitted with two more or less
superimposed single lines, one with a rather normal width and one very broad. Their negative isomer
shifts with respect to YbAl2 are characteristic of Yb2+ and we can probably assign them to Yb and YbO, but our limited accuracy does not allow a
detailed study. Anyway these diamagnetic impurities
do not affect the spectrum of interest, i.e. that of YbFe2.
3. Interpretation of the Môssbauer spectra of YbFe2-
-
3. 1 VALENCE STATE OF THE YTTERBIUM IN YbFe2.
-The lattice parameter of YbFe2 (7.244 A) is very
similar to that of TmFe2 (7.247 A) ; in addition it falls on the straight line which gives the lattice para- meter of the other RFe2 versus the atomic number
of the (trivalent) rare earth R : this indicates that
ytterbium is trivalent in YbFe2, as confirmed by the
existence of a compensation point in the magnetiza-
tion curve [1].
[Roughly speaking, when Yb is trivalent in this kind of intermetallic compounds, the lattice para- meter is very similar to that of the homologous Tm3 + compound ; when Yb is divalent the lattice parameter is about 0.1 1 to 0.14 A larger ; when Yb has an inter- mediate valency it is about 0.06 A larger.]
3.2 HYPERFINE CHARACTERISTICS OF (17OYb)3+.
The 84.4 keV y transition takes place between an
excited nuclear state I = 2, and a ground state
Ig=0.
In the nuclear state 1
=2 a (magnetic + quadru- polar) hyperfine structure is present. For the free Yb3 + ion (4f13,
,2F7/2’ J
=7/2) the hyperfine Hamiltonian is [5] :
with :
In these expressions (1
-RQ) is the Sternheimer
shielding factor of the 4f shell ; J il N Il J >, J Il ex )) J ) are reduced matrix elements to be found in Abragam and Bleaney [5] ; ye is the nuclear gyro-
magnetic ratio in state I = 2 ( ge = 0.334 whence Ye/2 n
=0.254 6 kHz/Oe) ; finally A s A’ + A’ is
the sum of a relativistic contribution A r and of the
core polarization contribution A. ([5], p. 296-300).
If the RE ion is now at a cubic site in a magneti- cally ordered alloy (like Yb3 + in YbFe2), and if
the electric field gradient has axial symmetry around the direction OZ of the hyperfine field, eq. (1) is replaced by the effective Hamiltonian :
with
where H.", vii characterize the contributions of the Rare Earth ion and He is an additional contri- bution due to the polarization of the conduction
electrons.
When the rare earth is fully polarized ( J z > = - J)
It is not very easy to determine a value for HFI’
According to the estimates of table 5.5 of [5] (based
on ionic crystals data) (2) :
-
on the other hand, in the cubic salt CaF2 : Yb,
(AJ)exp
=300 MHz for 17°Yb and 879.57 MHz for 1 71 Yb [6b]. After correcting for the difference between
(AJ)CaF2exp exp and A J J for 171Yb this would yield
whence HFI
=4 160 kOe.
Finally there exists a relativistic calculation which leads to HFI
=4 232 kOe [6c]. In what follows we
will tentatively assume that :
In a metallic matrix one must also take account of the conduction electron field He whose origin
(2) In principle HFI defined as AJ/nYn should slightly depend on
the isotope because of the hyperfine anomaly (j 4 ( % 0.5 % in the
RE : see [5] p. 252).
has been discussed by various authors but is not yet quite clear [7]. It may involve both a self polarization
of the conduction electrons by the rare earth itself and also transferred fields associated with the pola-
rization of the conduction electrons by neighbouring
and distant magnetic atoms (Fe and other RE).
The total contribution HcRE associated with the rare
earths should vary like Jz >, i.e. it should give rise
to an apparent variation of the hyperfine coupling
constant, while the contribution HcFe associated
with the irons should stay constant below 60 K. In the interpretation of the experiments we thus defined
a field HFI by :
and varied HFI and HF’. In terms of these two quanti- ties, the total conduction electron field He is :
Let us now look at the quadrupole interaction.
With the values :
we arrive at the maximum value in the fully polarized
state (JZ
= -J) :
On the other hand, according to table 3 of [7a], RQ
defined as
should be of the order 0.21 in metallic compounds.
3.3 HYPERFINE DATA FOR l7°Yb IN YbFe2.-
The Môssbauer spectra between 4.2 K and 60 K are well fitted with the simple Hamiltonian eq. (2) : the
full line curves in figure 1 represent least square fits with five lines with equal amplitude and widths
Table 1.
-Hyperfine parameters of 17°Yb in YbFe2.
The precision is about + 60 kOe for the hyperfine
field and + 60 MHz for the quadrupole coupling.
(FWHM
=2.5 mm/s at 4.2 K). Table 1 shows the corresponding values of Heff in MOe and e2 vii Q
in MHz. (One should however mention that the Môssbauer spectra are not very sensitive to a small asymmetry of the E.F.G., il 0.5.)
In YbFe2 the ytterbium ion is submitted both to
crystalline field effects and to exchange fields, the
main contribution to the exchange being due to RE-Fe exchange which we will assume to be isotropic for simplicity. Then, if the exchange field is parallel to [100] or [ 111 ], the hyperfine field Heff is also parallel to [100] or [111] and the E.F.G. has axial symmetry around the direction of the hyperfine field. Otherwise the gradient is not axial (in particular along [110] the
E.F.G. cannot be specified by a single number). In YbFe2, the gradient being apparently axial around
H,,ff, this suggests that the ytterbium moments can only lie along [100] or [111], in agreement with the data of reference [1] for 57Fe which indicate that the magnetization is along a direction [100] up to 50 K ; in addition the deviation from this direction above 50 K must still be very small at 60 K since it is not detectable in the Môssbauer spectra of 17°Yb. [100]
and [111] being high order symmetry axes this discus- sion would remain valid even in the presence of
anisotropic exchange.
3.4 INTERPRETATION OF THE THERMAL VARIATION OF THE HYPERFINE PARAMETERS.
-We first attempted
to fit our curves for Heff and e2 VZZ Q versus T by using the crystalline field and exchange parameters determined by Yanovsky et al. [2] for 17°Yb as an impurity in TmFe2 and TmxHo1-xFe2 (x
=0.1, 0.2).
The exchange and crystalline field Hamiltonians are
taken as :
with :
with these values, when Hex is along [100] we find that
at 0 K and at 4.2 K : and
(i.e. we are almost in the fully saturated case
Jz > = - 3.5 and 3 Jz2 - J(J + 1) > = 21). If we
take account of these results in order to compare the experimental values at 4.2 K : Heff
=4.44 MOe
Fig. 2.
-a) Hyperfine field, and b) electric quadrupole coupling,
for 170Yb in YbFe2 (heavy dot-dashed curve joining the experi-
mental points 0) compared with theoretical curves computed for
the three principal directions using the crystalline field and exchange
values of reference [2]. Dashed curves and experimental points A D :
results of reference [2] a : result of reference [9]. Full curves :
recomputed as indicated in text.
and e2 Vii Q
=3 210 MHz, with the maximum theo- retical values at 0 K :
we find that :
These figures seem reasonable. In particular RQ
compares favorably with the estimates of reference [7a].
By comparison the results of [2] were
(deduced from an extrapolated value
in figure 2 of [2], which seems to be in disagreement
with the value 2 400 + 250 MHz mentioned in the
abstract). The value RQ ~ 0.36 seems to be anoma- lously large. Because of these differences, we decided to entirely recompute the set of curves giving Heff and
e2 Vii Q as a function of T, with the same crystalline
and exchange parameters as before, but with
He
=320 kG and RQ
=0.22. The results of this calculation [8] are represented by the full line curves in figure 2 while the results of Yanovsky et al. [2] are represented by the dashed lines. Notice that the two sets are not related simply by a translation and/or an affinity. Indeed the results of our diagonalization
seem to differ very slightly from those of [2] ; for example along [111] the distance between our two
lowest electronic states is 1.57 K instead of 2.8 K in reference [2] and the next electronic state is at 50 K from the ground state instead of 55 K in [2]. In addi- tion, as already mentioned, we have found that in the
[110] direction the E.F.G. is far from axial (at 0 K, Vzz oc + 15.48, Vyy oc - 1.94 ; Vxx oc - 13.54) (3);
therefore the quadrupole splitting cannot be characte-
rized by its sole component Vzz along the exchange field, and the experimental points relative to Tmo.2Hoo.8Fe2 at low temperature should not be compared to the [110] curves of figure 2.
If we now look at our experimental points relative
to YbFe2 (dot-dashed curve) we see that they do not
fall at all on the curve computed for the [100] direction using the values of [2] : this means that these values
are not appropriate to YbFe2 and that the parameters relative to this compound must be determined directly by least square fitting of the hyperfine data. Many
least square fit calculations were made, with different numbers of adjustable parameters. The final results
are characterized by the fact that they all lead to
similar r.m.s. deviations with respect to the experi-
mental data : 47 to 58 kOe for the hyperfine field,
25 to 35 MHz for the quadrupole coupling, which
are less than the experimental uncertainties.
(3) OZ // [110], OX ll [001 ], 0 ye [110].
Fig. 3.
-Least square fits of the hyperfine field Heff (3a) and
electric quadrupole coupling e2 V4fzz Q (3b) with only an exchange
field MB Hex/kB
=109.64 K.
Least square fits were made :
-
with pure exchange only (Fig. 3) : IÀB Hex adjus-
-
with exchange + crystalline field : JUB Hex, A4 r4 >, A6 ( r6 ) adjustable
-
and also (although such a contribution is not
expected in the [100] direction even in the presence of
magnetostriction, see Chap. 4 below) with an addi-
tional second order crystalline field :
In all cases it is found that the crystal field coeffi-
cients are very small
while the exchange is comparable to that in TmFe2 :
Yb :
These conclusions remain unaltered when we vary
H§j between 4 100 and 4 400 kOe.
On the other hand, when HF, varies, the value at 0 K
of the conduction electron field He (eq. (6)), always
remains in the range 200-270 kOe : what this means
is that our accuracy is sufficient to determine Hc but
not to separate HcRE and HcFe. When we take account
of the uncertainty on HFI, we may say that
Finally RQ is always comprised between 0.21 and
0.23.
3.5 COMPARISON WITH OTHER DATA.
-We must now try to interpret these results : existence of a large
fourth-order crystalline field A4 r4 > in TmFe2 : Yb
and of a small field in YbFe2. As a matter of fact the
small crystal field in YbFe2 is in contradiction not
only with TmFe2 : Yb [2], but also with the large magnetic anisotropies observed in several RFe2
and with the assumption of constant A4 and A6
which was generally used in the interpretation of magnetic anisotropy data.
Before going further we must however make a
remark concerning TmFe2 : Yb. In fact the Môssbauer spectrum of 170Yb at 4.2 K has also been obtained by a
second group [9] and from their spectrum it follows that Heff
=4 140 k0e instead of 3 750 k0e in [2]
and that (e2 Vzz Q )[111] ] = 2 500 MHz instead of 1 700 MHz in [2]. The authors of [9] have informed us
that their sample was probably not very good [10].
Nevertheless the fact that two different preparations
can lead to such differences in the hyperfine para- meters suggests that new Môssbauer experiments on TmFe2 : Yb are perhaps necessary before detailed
comparisons can be made with YbFe2.
On the other hand, if we look at the magnetic anisotropy data, we see that the estimates rely on two
methods :
-
study of the magnetization direction as a func-
tion of composition in ternary compounds
-
anisotropy measurements on single crystals.
Concerning the first method, examination of the
figures of references [11a] and [11 b] shows that the boundaries in the ternary diagrams are relatively
insensitive to A4 and to /lB Hex : A4 = kB ---- to 50 4 K
a4o a4o in reference [lla] (4) where only major symmetry
idere d, A4 36 K
1 1b] h directions were considered, i- = B 36 a4 K 0 in [11b] where other directions were also considered; similarly
YB Hexl kB
=100 to 150 K in [11a],
=150 K in [11b].
(4) ao is the radius of the first Bohr orbit uo
=0.529 A. These values are deduced from the experimental data A4 r4 > 4f by using the ,.-+ of Freeman and Watson [13]. In practice
In a more recent paper [12] magnetostrictive contribu-
tions associated with the external stress (see next chapter) were incorporated into the calculations ; com- parison with the experimental data on HoxTbl _xFe2
then leads to (in our notation, and neglecting ui) A4/kB
=18 K/aÓ, J1B H,,.IkB
=172 K.
As for direct anisotropy measurements on single crystals, they have been performed on ErFe2 [14] and TmFe2 [15] as a function of T and on TbFe2 and DyFe2 at room temperature [16]. ErFe2 and TmFe2
are magnetized along [111] ] and have a rather large anisotropy at low T ; for this reason the anisotropy at
0 K is only an extrapolated value. In TmFe2 the extrapolated fourth order anisotropy constant at 0 K is K - 5 x 10+ 8 ergs/cm3 [14], i.e., for one
RE ion, K/Tm3 + - 120 cm -1 (see the definition of K below : eq. (27), (26), (23)). If K were entirely due
to the fourth order crystal field, the corresponding
value of A4 r4 >/kB for Tm3+ in TmFe2 would be
36 K (see eq. (26) below).
All these results, although suggesting that A4 r4 >4f is usually fairly large, are not precise enough to prove the constancy of either A4 or J1B Hex
in the RFe2 series.
In addition the possible influence of magnetostric-
tive effects on the effective crystalline potential seen by the Môssbauer atom has never been investigated.
As we will show in the next chapter the existence of a
large and anisotropic (111 1 » Â, 00) magnetostriction
in the RFe2 compounds [19] has two closely related
effects : first the total anisotropy constant K contains a
contribution KME which is probably not negligible
with respect to the contribution Kl due to the crys- talline field V4 ; second, the RE ion sees a second order crystalline field V2 - KME which depends on the
orientation of the magnetization and vanishes only
when it is parallel to [100]; this term V2 should be
taken into account in the interpretation of the hyper-
fine parameters derived from the RE Môssbauer spectra in materials which are not magnetized along [100].
4. Comparison of the effects of crystalline field and magnétostriction on magnetic anisotropy measure-
ments and on the Môssbauer spectra.
-41 1 SIMPLE
MODEL OF MAGNETOSTRICTION WITH ONLY EXTERNAL STRAIN.
-Let us assume that we have a rare earth atom in cubic surroundings, for example that it
is at the centre of a cube of eight charges q in a cubic crystal whose symmetry axes coincide with those of the cube.
Let us now slightly distort the crystal according to
the law
where xi, yi, zi are the coordinates of one of the eight charges with respect to the centre of the cube.
It is easy to show that this will create at the RE
atom a second order (5) crystalline potential of the
form (to order E) :
where xe, y,, ze are the coordinates of the eth electron 4f.
In the particular case of a cube of edge 2a one has
that
On the other hand it is clear from symmetry that V2
will retain a form of the type (13) whatever the nature
of the cubic neighbourhood.
Inside a state J, v2 can be replaced by
where J a Il J > is a Stevens coefficient.
Let us now derive a magnetoelastic coupling at 0 K
from eq. (15). For this we assume that the RE is also
submitted to a coupling with a large magnetic field (IÀB H » V2) with direction cosines oc,, a2, (13 (in practice H is the Fe-RE exchange field) and that in this
field it is fully polarized in the state ! 1 J z
= -J >
quantized along the field. It is easy to check that :
Let us now define the strains (Kittel’s conven-
tion [17]) :
(5) In this standard approach one neglects tne variations of the fourth and sixth order terms in the crystalline potential, eq. (8).
This amounts to neglecting contributions of order six or more in a to the magnetostrictive anisotropy energy EMË, eq. (22) below. This
approximation seems reasonable because of both the experimental
smallness of the sixth order anisotropy energy and the lack of detailed information on the crystalline potential.
and set :
Eq. (16) then reduces to the standard for magneto- elastic coupling :
When one adds to this the elastic energy Xel’
standard treatment of J6ei + HME leads to [18] :
whence the magnetostriction constants :
(C 11, Cl 2, C44 are the elastic stiffness constants).
Inserting eqs. (20) back into eq. (19) we get the magnetoelastic anisotropy energy
with
This contribution to the magnetic anisotropy adds
to the standard contribution arising from the crystal-
line field created by the undistorted neighbourhood :
.f corresponding to
As recalled in appendix 1 the method used for
extracting JCME from V2 can also be used for establish-
ing relationships between K1, K2 at 0 K and A4 r4 >,
Because K2 « KI in all the very anisotropic RFe2
studied up to now, measurements of the magnetic anisotropy essentially yield the fourth order anisotropy
constant :
As shown by this formula, if KME is not known and/
or is not small, this does not give any direct informa- tion about Kl, i.e. A4 r4 ).
Let us now look at the Môssbauer case. The hyper-
fine parameters depend on the wave functions and
energies of the ion, which are determined by the total crystalline potential to which it is submitted :
where, for a given direction al, a2, a3 of the magneti-
zation the magnetostrictive contribution V2 is given by
eq. (15) in which one replaces E« and eij by their
i #i
expressions eqs. (17), (20). From now on we will
assume that À,100
=0 (this will be discussed in the next paragraph). Then :
and :
We see that v2 is zero only in the [100] direction.
Otherwise it is non zero and its strength is directly
related to the magnetostriction energy. We may try to characterize it by the magnitude of its effects
when the magnetization is along [111]. If we quantize J along [111] we have that :
which gives rise to effects of the order KmE.
Let us now try to evaluate KME. A first method is to use the formula
In reference [14], KME was evaluated for TbFe2 at room
temperature using À111 1
=2.4 x 10-3. If we assume
that C44 in TmFe2 at 0 K is the same and use the experimental value À111 = - 3.5 x 10-3 [15] we
arrive at KME
= -9.2 cm-1/ion. Alternatively, if
we take : C44
=5.38 x 1011 ergs/cm3 as in refe-
rence [12] we get that KME
= -7.2 cm -1. We may
also use the formula
into which we put the experimental À111- while we
compute B2 for a tetrahedron of four charges 3+,
which represent half of the charges of the cube consi- dered above and correspond to the four RE nearest neighbours of a RE in the RFe2. We take their dis-
tance to the central atom to be 3.14 A as in TmFe2.
We then find that KME
=+ 14.1 cm-1/ion. All these
estimates are open to criticism because the formulas
they use do not take account of the internal mode to be discussed in the next paragraph. In addition, as
concerns the third one, B2 being negative, eq. (21)
should lead to a positive À111 hence to a negative KME
while the experimental À11l is negative ; this is pro-
bably due to the fact that our estimate of B2 uses a point charge model and does not take account of the
iron nearest neighbours.
4.2 MORE ELABORATE TREATMENT OF MAGNETO- STRICTION IN THE RFe2. - This is done in refe-
rences [19, 20] where it is argued that the great aniso- tropy of the magnetostriction observed in the RFe2 (À111 ~ 50 À100) can only be understood if one assumes that the external strain e is accompanied by an
internal mode u coupled to e.
In the notations of [20] one has that :
(where VIII is some kind of internal magnetostriction)
and :
The magnetoelastic coupling terms in eq. (2) of [20]
are :
(similar to our eq. (19) with B,
=0). The correspond- ing second order crystalline potential is :
and when we substitute eqs. (35) and (36) into (39)
and use eq. (37) we recover the general eq. (31) obtain-
ed in the preceding paragraph which relates V2 and KME. The only difference is that now KME depends on
the properties of the internal mode (CO, g) and on its coupling ( f ) to the external stress which are presently
not known. We may nevertheless hope that the nume-
rical estimates of the preceding paragraph remain roughly valid in the presence of the internal mode.
We have found that KME ~ - 10 cm -1 /ion, which
may well be in error by at least a factor of two or four.
If we compare these estimates with the extrapolated
value at 4 K : K- - 120 cm -1 /ion for Tm3 + in TmFe2, we see that magnetostriction might well
account for something like one tenth to one third
of the magnetic anisotropy of this compound.
Another interesting remark is that in a mixture
(R(1)Fe2-R(2)Fe2)’ the contributions to the magne- toelastic coupling coefficients b2 and g are expected
to be additive, but not those to KME (since it involves
bi, g2, etc...). This could perhaps be a way to estimate the relative contributions to K of Kl (additive) and KME (non additive).
5. Discussion.
-According to the preceding para-
graph the crystalline potential which determines the
hyperfine parameters of the Rare Earth ion in a Môssbauer experiment is :
V4 + V6 in a RFe2 magnetized along [100] (YbFe2), V2 + V4 + V6 in a RFe2 magnetized in any other direction in particular [111] and [110] (TmFe2).
On the other hand the magnetic anisotropy constant
of order four is, in all RFe2 :
V2 (eq. (31)) and KME are magnetostrictive contribu-
tions and the effects of V2 are of order KME.
These expressions show that the quantities observed
in different RFe2 or by different techniques are not necessarily the same. Comparison would make sense only if KME could be evaluated with precision, which
is not possible at present because of the unknown contribution of the internal mode.
We have estimated very roughly that in TmFe2, 1 KME 1 could perhaps be of the order - 10,
-
40 cm -1 /Tm3 + . Comparison with the total ani- sotropy : Kl(V4) + KME
= -120 cm-1/Tm3+, sug- gests that in this compound the crystalline field V4
at the Tm3+ ion, while not responsible for the totality
of K, is certainly not small. We must therefore admit that V4 for Yb3+ in YbFe2 is effectively smaller than
V4 for Tm3+ in TmFe2. One may think of several
explanations for this : either A4 varies and depends
both on the RFe2 matrix and on the RE ion in it or,
A4 being constant, V4 contains another contribution due to anisotropic exchange, whose effects are similar
to those of a crystalline field ; the most likely candidate
would be Fe-RE exchange which is large ; on the
contrary RE-RE exchange, while probably anisotro-
pic, seems too small, as shown by the ordering tem- peratures of the RNi2 where Ni is non magnetic :
What also comes out from all these considerations is the interest of Môssbauer spectroscopy for obtain-
ing information on the crystalline field at low tempera-
tures where, at least in high anisotropy compounds, magnetic anisotropy measurements are no longer possible. There are however some difficulties : first,
the hyperfine parameters are mainly sensitive to the exchange field and only accessorily so to the crystal-
line field ; therefore precise measurements at a number of temperatures are needed. As an illustration of this fact, old Môssbauer measurements on 161 Dy in
DyFe2 [23] and 169Tm in TmFe2 [24] were fitted with pure exchange only ÛlB Hex/kB
=202 K and 165 K respectively) while at least for Tm3 + in TmFe2 the crystalline field is rather large, as discussed above ; these fits were probably made possible by the small
number of points and the limited accuracy. A second
difficulty is that in the RFe2 magnetized along [111]
one should perform a four parameters fit for the hyperfine data ( V2, V4’ Y6, MB Hex) ; this is a source of uncertainty, but it should nevertheless yield some
information about the magnitude of V2 + V4 + V6.
Notice that when a RE impurity R(1) is substituted into a matrix R(2)Fe2’ V2 at the impurity will not be proportional to KME, contrary to the Y2 at R (2).
6. Conclusion.
-In conclusion we have discussed the role of magnetostrictive effects in magnetic anisotropy and Môssbauer measurements. While these effects should be taken into account in the
interpretation of Môssbauer experiments on the RFe2 magnetized along [111 ], they are apparently too small
to account for the difference between the crystalline potentials observed in YbFe2 on the one hand and in
TmFe2 or ErFe2 on the other hand. This difference
seems therefore to arise either from a non constancy of the true crystalline potential V4 + V6 in the RFe2
series or from anisotropic Fe-RE exchange. Addi-
tional magnetic anisotropy and Môssbauer measure-
ments would be of interest for determining more exactly the magnetostrictive anisotropy KME and the crystalline field V4 + V6, as well as their variations
throughout the series. Note that for isotopes like 170Yb the accuracy of the Môssbauer data could be
considerably improved by resorting to high precision spectroscopy based on several Ci sources [25].
Acknowledgments.
-We wish to thank Mr. M.
Merlin and Dr. M. Lombardi for their help with the computer calculations. Mr. Perroux of the Labora- toire de Cristallographie kindly assisted with the
preparation of the samples.
Note added in proof.
-In ref. [19] the assertion that
1 Â 111 1 » 1 À100 I was based on a comparison between TbFe2 (Â 111 (OK) = 4 400 x 10-6) and DyFe2 (Àloo(OK) = - 70 x 10-6). The magnetostriction ÀlOO of HoFe2 has very recently been measured (R. Abbundi and A. E. Clark, Proceedings of the Magnetism Conference, Cleveland, nov. 1978, to be published in J. Appl. Phys.) and has been found to be much greater than that of
Nevertheless 1 îloo IHoFe2 is still six times smaller
than 1 Â 111 ITbFe 2and the considerations of chap. 4
remain valid.
APPENDIX 1
Correspondence between crystalline field and aniso- tropy.
-Let us assume that the RE ion is submitted
to a crystalline field, represented by the equivalent operator
where Okq (J) is the operator equivalent [26] of
Let us assume that in addition to Hc, the RE ion
is also submitted to a large exchange field with polar angles (0, w)
and that kB T Hc « Jez, i.e. the atom is in the state 1 Jz = - J ) quantified along Hex. By rotating Hc
it is possible to demonstrate that [27, 28] :
with
Ean is the anisotropy energy and eq. (A. 5) gives us
the correspondence between the crystalline potential
and the anisotropy.
Let us now assume that we have cubic symmetry :
and that the exchange field has cosines ai a2 a3.
We find that :
We now want to put this into the usual form for cubic symmetry :
We get that :
We see that V6 contributes non only to K2 but also
to Ki . This is due to the fact that the two polynomials
in al, (X2’ a3 in eq. (A. 9) do not belong to an ortho- gonal basis set [29].
In practice the contribution of V6 to Ki is eleven
times smaller than its contribution to K2. It follows
that as long as K2 KI, Ki is essentially due to V4. This is particularly true in the most anisotropic RFe2 where experimentally K2 is found to be very small with respect to Kt.
APPENDIX II
Small corrections to référence [1] ] and possible role
of an anisotropic hyperfine structure of the irons in 57Fe
Môssbauer spectra of YbFe2.
-1 . SMALL CORREC-
TIONS.
-In référence [1] several quaiitities relative
to YbFe2 were estimated with the help of theoretical values of the Yb 31 moment computed with the data
of reference [2] obtained on TmFe2 : Yb ; in parti-
cular the moment of the iron atoms was estimated
by writing that at the compensation temperature JlFe
=1/2 JlYb. We must now correct these quantities
on the basis of the information obtained in the present
paper with the Môssbauer effect of 17°Yb in YbFe2
itself.
Before doing so, we note that the error bars of
reference [1] for the compensation temperature oc
=31 ± 7 K were probably too high. Here we
will admit that ec
=31 ± 2 K which corresponds
to ± 2 % variations of the 17°Yb hyperfine field
in figure 3.
In these conditions we find that the Yb3+ moment at the compensation temperature is comprised between
the values 3.23 YB (obtained by interpolation of the experimental Yb3 + hyperfine fields at 20 K and 34 K
after deducing He
=240 kG) and 3.35 YB (obtained
by calculating Jz > in a pure exchange field
YB Hex/kB
=109.64 K). This leads to
at low T instead of 1.8 YB in [1].
At 85 K we estimate from figure 3 of the present paper thatyyb 1-99 /lB instead of 2.03 /lB computed
in [1]. We have shown in [1] that the theoretical
dipolar parameter Ad which comes into play in the interpretation of the 57Fe Môssbauer spectra is given by (eqs. (6), (14) of [1]) :
With the new values of the moments we find that :
-
at 4 K, Ad
=5 000 Oe instead of 5 200 in [1 ],
- at 85 K, Ad
=3 650 Oe instead of 3 900 in [1].
Also we had found that at room temperature, 285 K (where crystalline field effects are negligible),
J1Yb
=0.59 J1B. We must correct this value for the
change in the exchange field (uB Hex/kB
=111 K instead of 116 K in [2]). This leads to J1Yb
=0.56 J1B.
If we assume in addition that J1Fe oc HnF’, the expected
saturation moment per formula unit at 285 K is :
instead of 2.6 YB in [1 ].
Despite these small corrections the conclusions of reference [1] remain unchanged. We must however
make some remarks relative to the detailed inter-
pretation of the 57Fe Môssbauer spectra in [1].
2. POSSIBLE ROLE OF AN ANISOTROPIC HYPERFINE INTERACTION IN THE 57Fe MÔSSBAUER SPECTRA OF
YbFe2.
-In reference [1] ] the evaluation of tipping effects in the interpretation of the Môssbauer spectra
at 5.2 K was made with the help of the computed
value of the dipolar parameter (,/2-A, = 7.3 kOe).
New fits using a least square program lead to a very
slight improvement of the agreement if one uses the empirical parameter : /2- A = 11.9 kOe, whence
A
=8.43 kOe. The corresponding value for e2 2 qQ
is
-0.52 mm/s instead of the tentative value
-