Download 1 Relationship between the magnetic hyperfine field and the

Survey
yes no Was this document useful for you?
   Thank you for your participation!

* Your assessment is very important for improving the workof artificial intelligence, which forms the content of this project

Document related concepts

Electromagnetism wikipedia , lookup

Mathematical descriptions of the electromagnetic field wikipedia , lookup

Lorentz force wikipedia , lookup

Superconducting magnet wikipedia , lookup

Friction-plate electromagnetic couplings wikipedia , lookup

Magnetic monopole wikipedia , lookup

Magnetic stripe card wikipedia , lookup

Magnetometer wikipedia , lookup

Electromagnetic field wikipedia , lookup

Magnetic nanoparticles wikipedia , lookup

Earth's magnetic field wikipedia , lookup

Electron paramagnetic resonance wikipedia , lookup

Giant magnetoresistance wikipedia , lookup

Magnet wikipedia , lookup

Ferrofluid wikipedia , lookup

Magnetotactic bacteria wikipedia , lookup

Electromagnet wikipedia , lookup

Neutron magnetic moment wikipedia , lookup

Force between magnets wikipedia , lookup

Magnetohydrodynamics wikipedia , lookup

Magnetoreception wikipedia , lookup

Magnetism wikipedia , lookup

Magnetotellurics wikipedia , lookup

History of geomagnetism wikipedia , lookup

Multiferroics wikipedia , lookup

Ferromagnetism wikipedia , lookup

Magnetochemistry wikipedia , lookup

Transcript
Relationship between the magnetic hyperfine field and the magnetic moment
S. M. Dubiel*
Faculty of Physics and Applied Computer Science, AGH University of Science and
Technology, al. A. Mickiewicza 30, PL-30-440 Kraków, Poland
Abstract
Based on experimental data it is shown, for some chosen alloys and compounds of iron, that
there is no one unique relationship between the 57Fe-site magnetic hyperfine field, Bhf, and the
magnetic moment per Fe atom, µ. Instead, the Bhf-µ plot consists of several branches, each of
them being characteristic of a given alloy or compound. Consequently, the effective
proportionality constant (hyperfine coupling constant) depends on the alloy system or
compound, and for a given alloy system or compound it depends on the composition or even
on the lattice site. Consequently, the scaling of Bhf into the underlying µ cannot be done a
priopri.
PACS: 75.50.Bb, 76.80.+y,
•
[email protected]
1
1. Introduction
Magnetic alloy systems and compounds of iron are often investigated with the use of
Mössbauer spectroscopy and the magnetic hyperfine field, Bhf being the main spectral
parameter. A question arises whether or not an information on the underlying magnetic
moment, µ. can be derived from Bhf.. A rather quite frequent practice, applied to
recalculate Bhf into µ., has been to simply divide the measured value of Bhf by ∼15 T/µB, a
figure obtained by dividing the value of Bhf measured for a metallic Fe (33.9 T at 4 K), by
the value of the magnetic moment per Fe atom in iron (2.2 µB). This procedure was
applied for various alloy systems and compounds having not only different compositions
but also different crystallographic structures [1-7], despite theoretical calculations carried
out as early as in 1961 clearly demonstrated that even for the pure metallic iron the two
quantities are not proportional to each other [8]. It is also known from measurements that
the temperature dependence of Bhf do not, in general, follow that of the magnetization, the
difference being temperature dependant [9-11]. This means that the proportionality
constant between the two quantities is also temperature dependent. As will be shown
below on several examples of Fe-containing alloys and compounds, the effective
hyperfine coupling constant, A, i.e. the figure obtained by dividing the measured 57Fe-site
hyperfine field by the magnetic moment per Fe atom determined either from
magnetization or neutron measurements depends on the alloy system, and for a given
alloy it depends on its composition and degree of order. For intermetallic compounds, the
constant depends also on a crystallographic site. An extreme example seems to be a
RuxFeySi system for which the effective coupling constant changes between 189.3 T/µB
for RuFeSi0.5 and 27.7 T/µB for RuFeSi [1]. In other words, there is no one definite value
of this constant, hence the relationship between Bhf and µ is not universal which means
that the rescaling of Bhf into µ cannot be done a priori.
2. Theoretical background
Magnetic hyperfine field as measured, for example by Mössbauer spectroscopy, Bhf, can
be expressed as a vectorial summ of three components:
r
r
r
r
Bhf = Bd + Bo + Bc
(1)
where Bd is a dipole term, Bo is an orbital term and Bc is the Fermi contact term. For iron
alloy systems and compounds, the orbital term is small because the expectation value of
the orbital momentum, <L>, is quenched by the crystalline field [12], and the dipolar term
is of the order of 2 T [13] i.e. the two terms are much smaller than Bhf (equal to 33 T for
metallic Fe at room temperature). In these circumstances with a good approximation Bhf =
Bc.
Bc has its origin in a different density of s-like electrons with spin-up () and spin-down
() within the volume of nucleus, ρ(0). Thus neglecting the first two terms in equ. (1), Bhf
can be expressed as follows:
[
Bhf = a ' ∑ ρ i↑i (0) − ρ i↓ (0)
]
(2)
where a’ is a proportionality constant. The Bc term is often regarded as consisting of two
contributions:
2
Bc = Bcp + Bcep
(3)
with Bcp representing the field due to a polarization of core (1s, 2s, 3s) electrons and Bcep
representing the one due to the polarization of band (conduction or valence) electrons (4s,
3d, 4p). The reason for such separation follows from theoretical calculations by Watson
and Freeman according to which only the first term is proportional to the 3d shell
magnetic moment, µd [8]. Having this in mind, Bhf can be expressed as follows:
[
Bc = aµ d + b ρ ↑ (0) − ρ ↓ (0)
]
(4)
In equ. (4) ρ(0) stands for the total band (conduction or valence) electron contact density.
Bc - µd linearity was also confirmed theoretically by other authors [14-17]. However, the
value of the proportionality constant, a, depends on theoretical approach. In this respect
the most detailed calculations were carried out by Lindgren and Sjøstrøm who calculated
Bcp (1s, 2s, 3s) and Bcep (4s, 3d, 4p) terms for five different exchange correlation potentials
both for a band iron and a free Fe atom (3d74s1), using relativistic and non-relativistic
approximation [6]. They found that a was between –17.1 T/µB and –12.1 T/µB for the
relativistic band calculations, and between –12.1 T/µB and –9.3 T/µB for non-relativistic
free atom calculations, depending on the exchange potential. The corresponding constant
for the total field i.e. Bc was between –20.25 T/µB and –15.0 T/µB. The proportionality
constant b has yet different value; e. g. according to a recent paper, in which the fullpotential linearized augmented plane wave method based on the density function theory
was used, it is equal to 9 T/µB [17], while according to others, b = 26.1 T/µB [15].
Calculations performed with the spin-polarized discrete variational method for clusters of
15 atoms in Fe-Cr alloys showed that both the value and the sign of the proportionality
constant strongly depend on the atomic configurations, and it ranges between 12.0 T/µB
and –12.5 T/µB depending on the number of Fe and Cr atoms in the first two coordination
shells [18]. Neglecting these differences among various approaches applied in the
theoretical calculation it is clear that the proportionality between the measured total
hyperfine field, Bhf, and the magnetic moment, µ, often used in an interpretation of
Mössbauer data should be used with caution since the band (conduction or valence) term
is not necessarily proportional to the magnetic moment. The deviation from the
proportionality should be greater for systems where the Bcep term is relatively large i. e. in
itinerant magnetic systems. Conversely, for magnetic systems with a well localized
magnetic moment, the relationship should be rather linear. In fact, the latter seems to be
the case for R-Fe compounds [19]. In particular, for various Y-Fe ones for which the value
of the proportionality constant between the Fe-site hyperfine field and the Fe-site
magnetic moment is ~15 T/µB [20]. On the other hand, the are also exceptions in this
group of compounds, like YFe6Sn6, for example, where the Bhf - µ relationship shows a
pronounced curvature which likely originates from the fact that only the core electron
contribution is proportional to the Fe magnetic moment while the conduction electron
term is not [19].
2. Experimental relationship
2. 1. Hyperfine field versus magnetic moment
A relationship between Bhf and µ as measured on three types of iron alloy and compound
systems viz. (a) disordered binary Fe-M alloys with M = Co, Cr and Si, (b) ordered (DO3)
3
Fe3Si and Fe3Al intermetallic compounds with Fe atoms substitude by Co, Cr, Ni, Mn and Ru
and (c) sigma-phase FeCr non-stoichiometric compound is presented in Fig. 1. The plot was
constructed based on the data published in [21,22,29,30-35] It is clear that the data do not
follow any unique linear relationship. Instead, different branches, similar to the Slater-Pauling
curves known for magnetic moments or Curie temperatures, can be observed. The types (a)
and (b) of alloys have their own branches and within type (a) each of the three investigated
alloys has its own branch. On the other hand, the data for the sigma-Fe-Cr lie well on the
branch characteristic of the disordered Fe-Si alloys. This branch and the one for the
disordered Fe-Cr alloys have a quasi-linear character, though their slope is significantly
different. However, the branch for the disordered Fe-Co alloys has a pronounced curvature.
40
35
30
Si
Cr
Bhf [T]
25
Co
s-FeCr
20
Fe3Si(A,C)
Fe3Si(B)
15
Fe3Al(B)
Fe3Al(A,C)
10
5
0
0
0,5
1
1,5
2
2,5
3
u [Bohr magneton]
Fig. 1 Hyperfine field, Bhf, versus magnetic moment per Fe atom, µ, for (a) disordered Fe-M
alloys (M = Co, Cr, Si), (b) ordered (DO3) Fe3-xXxSi (X = Co) and Fe3Al alloy and (c) sigmaphase Fe-Cr alloys.
To show further that for a given class of alloys the Bhf - µ relation, hence the value of the
effective coupling constant, A, depends on the composition, such relation is illustrated in Fig.
2 only for the sigma-phase in Fe-Cr and Fe-V systems.
4
14
12
Bhf [T]
10
8
Fe-V
Fe-Cr
6
4
2
0
0
0,2
0,4
0,6
0,8
1
u [Bohr magneton]
Fig. 2 Average hyperfine field, Bhf, versus average magnetic moment per Fe site, µ, for the
sigma-phase in Fe-Cr and Fe-V systems [31].
Here the Bhf - µ relation is non-linear for the Fe-Cr system and perfectly linear over a
much wider range of composition for the Fe-V system.
Further discussion of the issue will depict the value of the effective proportionality
constant (hyperfine coupling constant), A, between the measured hyperfine field and the
magnetic moment per Fe site (for disordered alloys and for the sigma-phase both
quantities are average ones) i. e. calculated assuming Bhf = A µ.
2. 2. Disordered binary alloys
Figure 3 illustrates A as a function of x for Fe100-xMx (M=Co, Cr and Si) obtained from
the data published in [21,22,29,30-35]. It is obvious that A is characteristic of a given
alloy and it is also concentration dependent i.e. it more or less linearly decreases with x.
For x ≤ ∼18, AFeCr ≈ AFeSi but AFeCo > AFeCr,FeSi. For x ≥ ∼75, AFeCr shows a steeper decrease
with x and its value at x≈95 is about 7-8 times smaller than that for a pure iron. For very
diluted Fe100-xCrx alloys ( x < 1), Fe atoms posses the magnetic moment of ∼1.4 µB+, yet
the hyperfine field is as small as 3.5 T [33], consequently the effective hyperfine coupling
constant is equal only to 1.5 T/µB i.e. ten times less than for x = 0.
2. 3. Ordered alloys and compounds
Archetypal examples of the DO3 superstructue are Fe3Al and Fe3Si compounds. Here the
effective proportionality constant, A, that was calculated for the former based on the
results presented in [30,31], and for the latter on the results published in [38], is equal to
16.6 T/µB in Fe3Al, and 15.4 T/µB in Fe3Si for sites A and C against 14.7 T/µB in Fe3Al
and 16.1 T/µB in Fe3Si for site B. Yet a greater difference between the sites for the Fe3Si
compound follows from the results given in [9]. Here AA,C = 17.0 T/µB against AB = 13.3
T/µB. This illustrate well the fact that A in a given compound or ordered alloy can be even
5
site dependent. On the other hand, the kind of element with which Fe makes the
compound also seems to be important as far as the value of A is concerned. In particular,
for Fe3Ge the site average value of A = 12.3 T/µB as determined from the data published in
[39,40] which is significantly less than the value found for Fe3Al and Fe3Si. To further
investigate the issue we consider the Fe3Si compound in which Fe atoms have been
substituted by Co atoms.
A versus x for Fe3-xCoxSi compounds obtained from the data published in [29], is
presented in Fig. 4. The most striking feature to be noticed here is a clear dependence of A
on the crystallographic site, namely AB >AA,C. Other interesting feature that can easily be
noticed is a different concentration dependence of AB and AA,C. The former increases with
x, reaches its maximum at x≈0.8 and falls again for greater x. The latter initially decreases
with x, reaches its minimum at x ≈ 0.5 to increase slowly for larger x – values. In any case,
for all x-values, except x = 0, the values of A differ significantly for the two sites and the
maximum difference equals to 11.5 T/µB for x ≈ 0.8 – 1 i.e at this composition AB is twice
as big as AA,C.
15
A (T/uB)
13
11
9
Cr
Co
Si
7
5
3
1
0
10
20
30
40
50
60
70
80
90
100
x
A [T/Bohr magneton]
Fig. 3 Effective hyperfine coupling constant, A, for disordered Fe100-xMx alloys with M =
Co , Cr and Si versus x, as determined based on the data published in the literature.
26
24
22
20
B
A,C
18
16
14
12
10
0
0,4
0,8
1,2
1,6
2
x
6
Fig. 4. Effective hyperfine coupling constant, A, for ordered (DO3) Fe3-xCoxSi alloys
versus x, as deduced from the data presented in [29].
Quite similar behaviour, as illustrated in Fig. 5, exhibits the Fe3Si alloy with Cr and Ni
atoms substituted for Fe. On the other hand, the AA,C – values for M = Mn do not show
any systematic character. This also contrasts with M = Al where, as it follows from [41],
AA,C ≈ AB ≈ 18 T/µB.
A [T/Bohr magneton]
30
B(Co)
A,C(Co)
A,C(Mn)
B(Cr)
A,C(Cr)
B(Ni)
A,C(Ni)
26
22
18
14
10
0
0,4
0,8
1,2
1,6
2
x
Fig. 5. Effective hyperfine coupling constant, A, for ordered (DO3) Fe3-xTxSi alloys
(T=Co, Cr, Ni, Mn) versus x.
In the case of Fe3-xRuxSi the magnetic moment was determined from the magnetization
measurements, so only its average value per Fe atom is known [23]. Consequently, no
distinction between the two sites could have been made. The average value of A over the
two sites versus x is plotted in Fig. 6, from which it is clear that A ≈ 14-15 T/µB up to x ≈
1.4, followed by a steep quasi-linear increase. The difference between the minimum and
the maximum value of A is here one order of magnitude.
7
160
A [T/Bohr magneton]
140
120
100
80
60
40
20
0
0,4
0,6
0,8
1
1,2
1,4
1,6
1,8
2
x
Fig. 6. Effective hyperfine coupling constant, A, for ordered (DO3) Fe3-xRuxSi alloys
versus x.
Alike effect can be seen in Fig. 7 for DO3 ordered Fe100-xAlx alloys with 22.5 ≤ x ≤ 34 as
derived from the data presented elsewhere [24]. One can readily see that also here A is
concentration dependent, and it increases with x from 14 T/µB at x≈23 to 45 T/µB at x≈34.
A [T/Bohr magneton]
50
45
40
35
30
25
20
15
10
22
24
26
28
30
32
34
x [at% ]
Fig. 7 Effective proportionality constant, A, between Bhf and µ for DO3 ordered Fe100-xAlx
versus x.
Similar effect of the composition on the effective hyperfine coupling constant is shown in
B2 ordered alloys. Figure 8 illustrates this behavior for disordered and ordered Fe100-xCox
alloys.
8
16
A (T/uB)
15
14
D
O
13
12
11
10
0
10
20
30
40
50
60
70
80
x
Fig. 8 Effective hyperfine coupling constant, A, versus x for disordered (D) and ordered
(O) Fe100-xCox alloys. The greatest difference in A can be seen around x = 50 i.e. at the
composition where the degree of the B2 order is at maximum.
Much smaller A - values can be found in other ordered alloys or compounds of iron. In
particular, using the appropriate data for Ni3Fe from [42,43] one arrives at A = 9.1 T/µB,
and at 11.1 T/µB or 9.4 T/µB for site 1 and 2, respectively, in Fe2P [44], and finally at 9.5
T/µB for Fe3Sn2 [45].
3. 3. Sigma-phase Fe-Cr and Fe-V alloys
Sigma-phase alloys have a very complex crystallographic structure with 30 atoms
distributed over five different lattice sites. Consequently, only the average values both of
the hyperfine field, Bhf, as well as those of the magnetic moment per Fe atoms, µ, could
have been determined. The average value of the hyperfine coupling constant, A, derived
from this data for the sigma-phase in the Fe-Cr system is plotted in Fig. 9. As can be seen
it is concentration dependent with a maximum of ∼ 14.5 T/µB at x ≈ 47 and a minimum of
∼ 11.5 T/µB at x ≈ 44.5. On the other hand, the value of A derived in a similar way for the
sigma in the Fe-V system is constant within V concentration of 34 – 60, and equal to
13.15 T/µB.
9
16
A (T/uB)
15
14
13
12
11
10
44
45
46
47
48
49
50
x
Fig. 9 Average hyperfine coupling constant, A, versus Cr concentration, x, in the sigmaFe100-xCrx alloys [22].
4. 4. Amorphous alloys
The relationship between Bhf and µ was also investigated in various amorphous alloys of
iron. Here in many instances a linear relationship was found, but the proportionality constant
vary from system to system. In particular, Dunlop and Stroink found A = 14.9 T/µB for a
series of Fe79SnB20-xSix with 0 ≤ x ≤ 12 [46]. This figure slightly contrasts with the value of
13 T/µB found for similar alloys by Kemeny et al [3]. On the other hand A = 14 T/µB was
deduced from the results measured on FexCr100-xB20 alloys with 50 ≤ x ≤ 100 [4]. Panissod et
al. found A = 12. 5 T/µB after compiling the data on a number of amorphous alloys [5]. It
seems that for many amorphous alloys the magnetic hyperfine field is in a good
approximation proportional to the Fe site magnetic moment and the proportionality constant
lies within a relatively narrow range of 12.5 – 15 T/µB.
5. Conclusions
Based on the results presented in this paper, the following conclusions can be drawn:
1. The magnetic hyperfine field is, in general, not lineraly correlated with the underlying
magnetic moment, and the actual correlation depends on the alloy or compound
system.
2. Consequently, there is no one unique value of the scaling constant between the two
quantities.
3. Instead, it is characteristic of a given alloy or compound system, and for a given
system it depends on its composition.
4. For ordered systems the hyperfine coupling constant is characteristic of a
crystallographic site, but for a given site it also shows a compositional dependence.
10
References
[1] V. S. Patil, R. G. Pillay, A. K. Grover, P. N. Tandon and H. G. Devare, Sol. Stat.
Commun., 48, 945 (1983)
[2] A. M. van der Kraan, D. B. de Mooij and K. H. J. Buschow, Phys. Stat. Sol. (a), 88, 231
(1985)
[3] S. Prasad, V. Srinivas, S. N. Shringi, A. K. Nigam, G. Chandra and R. Krishnanm J.
Magn. Magn. Mater., 92, 92 (1990)
[4] T. Kemeny, B. Fogarassy, I. Vincze, I. W. Donald, M. J. Besnus and H. A. Davies, in
Proc. 4th Intern. Conf. On Rapidly Quenched Metals, vol. 2, eds. T. Matsumoto and K. Suzuki
(Japan Inst. Metals, Sendai, 1982) p. 851
[5] D. Pannisod, J. Durand and J. I. Budnick, Nucl. Instr. and Methods, 199, 99 (1982)
[6] A. P. Malozemoff, A. R. Wiliams, K. Terakura, V. I. Moruzzi and K. Fukamichi, J. Magn.
Magn. Mater., 35, 192 (1985)
[7] M. Sostarich, S. Dey, P. Deppe, M. Rosenberg, G. Czjizek, V. Oestreich, H. Schmidt and
F. E. Luborsky, IEEE Trans. MAG-17, 2612 (1981)
[8] R. E. Watson and A. J. Freeman, Phys. Rev., 123, 2027 (1961)
[9] M. B. Stearns, Phys. Rev., 168, 588 (1968)
[10] D. C. Price, J. Phys. F, 4, 639 (1974)
[11] D. M. Edwards, J. Phys. F: Metal Phys., 6, L185 (1976)
[12] N. W. Ashcroft and J. Mermin, in Solid State Physics (Philadelphia, Saunders College,
1976) p. 657
[13] S. Ohnishi, A. J. Freeman and M. Weinert, Phys. Rev. B, 28, 6741 (1983)
[14] H. Akai, M. Maki, S. Blügel, R. Zeller and P. H. Dederichs, J. Magn. Magn. Mater., 45,
291 (1984)
[15] M. E. Elzain, D. E. Ellis and D. Guenzburger, Phys. Rev. B, 34, 1430 (1986)
[16] B. Lingren, J. Sjøstrøm, J. Phys. F: Metal Phys., 18, 1563 (1988)
[17] S. N. Mishra and S. K. Srivastava, J. Phys.: Condens. Matter, 20, 285204 (2008)
[18] M. E. Elzain, J. Phys.: Condens. Matter, 3, 2089 (1991)
[19] Xiao-lei Rao, J. Cullen, V. Skumryev and J. M. D. Coey, J. Appl. Phys., 83, 6983
(1998))
[20] P. C. M. Gubbens, J. H. F. van Apeldoorn, A. M. van der Kraan and K. H. J. Buschow, J.
Phys. F.: Metal Phys, 4, 921 (1974)
[21] H. H. Hamdeh, B. Fultz and D. H. Pearson, Phys. Rev. B, 35, 11233 (1989)
[22] J. Cieślak, M. Reissner, S. M. Dubiel and W. Steiner, Phys. Stat. Sol. (a), 205, 1791
(2008)
[23] S. N. Mishra, D. Rambabu, A. K. Grover, R. G. Pillay, P. N. Tandon, H. G. Devare and
R. Vijayaraghavan, J. Appl. Phys., 757, 3258 (1985)
[24] E. Voronina, E. Yelsukov, A. Korolyov, A. Yelsukova, S. Godovikov and N.
Chistyakova, in Programme and Abstract Book, ICAME, Kanpur (India), 2007, p. T2-P16
[25] D. Satula, K. Szymański, L. Dobrzyński and J. Waliszewski, J. Magn. Magn. Mater.,
119, 309 (1993)
[26] J. Waliszewski, L. Dobrzyński, A. Malinowski, D. Satula, K. Szymański, W. Pradl, Th.
Brückel, O. Schärpf, J. Magn. Magn. Mater., 132, 349 (1994)
[27] R. Nemanich, C. W. Kimball, B. D. Dunlop and A. T. Aldred, Phys. Rev. B, 16, 124
(1977)
[28] V. A. Niculescu, T. J. Burch and J. I. Budnick, J. Magn. Magn. Mater., 39, 223 (1983)
[29] R. Nathans, M. T. Piggot, C. G. Shull, J. Phys. Chem., 6, 38 (1958)
[30] C. E. Johnson, M. S. Ridout, T. E. Cranshaw, Proc. Phys. Soc., 81, 1079 (1963)
[31] A. T. Aldert, B. D. Rainford, J. S. Kouvel and T. J. Hicks, Phys. Rev. B, 14, 228 (1976)
11
[32] B. Babic, F. Kajzar and G. Parette, J. Phys. Chem. Solids, 41, 1303 (1980)
[33] I. R. Herbert, P. E. Clark and G. V. H. Wilson, J. Phys. Chem. Solids, 33, 979 (1972)
[34] H. Kuwano and K. Ono, J. Phys. Soc. Jpn., 42, 72 (1977)
[35] S. M. Dubiel and J. śukrowski, J. Magn. Magn. Mater., 23, 214 (1981)
[36] J. Cieślak, B. F. O. Costa, S. M. Dubiel, M. Reissner and W. Steiner, „Magnetic ordering
above room temperature in the sigma-phase of Fe66V34 “, arXiv: 0811.2908
[37] E. P. Elsukov, G. N. Konygin, V. A. Barinov and E. V. Voronina, J. Phys. : Condens.
Matter., 4, 7597 (1992)
[38] W. A. Hines, A. H. Menotti, J. I. Budnick, T. J. Burch, T. Litrena, V. Niculescu and K.
Raj, Phys. Rev. B, 13, 4060 (1976)
[39] H. Nakagawa, L. Kanematsu, Jap. J. Appl. Phys., 18, 1579 (1979)
[40] L. Häggström and J. Sjøström, A. Narayanasamy and H. R. Varma, Hyperf. Interact., 23,
109 (1985)
[41] L. Dobrzyński, T. Giebułtowicz, M. Kopcewicz, M. Piotrowski and K. Szymański, Phys.
Stat. Sol. (a), 101, 567 (1987)
[42] J. W. Cable and E. D. Wollan, Phys. Rev. B, 7, 2005 (1973)
[43] M. Kanashiro and N. Kunitomi, J. Phys. Soc. Jpn., 48, 93 (1980)
[44] O. Eriksson and A. Svane, J. Phys. : Condens. Matter, 1, 1589 (1989).
[45] G. Le Caër, B. Malaman and B. Roques, J. Phys. F: Metal Phys., 8, 323 (1978)
[46] R. A. Dunlop and G. Stroink, J. Appl. Phys., 55, 1068 (1984)
12