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Submitted on 1 Jan 1982

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Electronic structure of 3d impurities in ferromagnetic iron

P. Léonard, N. Stéfanou

To cite this version:

P. Léonard, N. Stéfanou. Electronic structure of 3d impurities in ferromagnetic iron. Journal de

Physique, 1982, 43 (10), pp.1497-1502. �10.1051/jphys:0198200430100149700�. �jpa-00209531�

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Electronic structure of 3d impurities in ferromagnetic iron

P. Léonard and N. Stéfanou

Laboratoire de Magnétisme et de Structure Electronique des Solides (*), Université Louis Pasteur, 4, rue Blaise Pascal, 67070 Strasbourg Cedex, France

(Reçu le 17 février 1981, révisé le 17 mai, accepté le 10 juin 1982)

Résumé. 2014 Nous présentons les résultats du calcul de la structure électronique des impuretés (Ti, V, Cr, Mn, Co, Ni, Cu) diluées dans le fer ferromagnétique obtenus par la méthode des combinaisons linéaires d’orbitales « muffin- tin » dans l’approximation de la sphère atomique (LMTO-ASA). Les moments locaux et les champs hyperfins

sur l’impureté ainsi que les changements de coefficient de chaleur spécifique électronique sont comparés aux

résultats expérimentaux.

Abstract.

2014

We present the results of the calculation of the electronic structure of impurities (Ti, V, Cr, Mn, Co, Ni, Cu) diluted in ferromagnetic iron obtained by the method of linear combination of « muffin-tin » orbitals in the atomic sphere approximation (LMTO-ASA). The local moments and the hyperfine fields on the impurity

and the electronic specific heat coefficient charges are compared with the experimental data.

Classification Physics Abstracts

71. 20

1. Introduction.

-

The study of the electronic structure of iron alloys with transitional impurities

has been the subject of numerous experimental and

theoretical works. The electronic structure of the

alloys of a weak ferromagnet such as iron is not as

well understood on the whole as the electronic structure of the alloys of strong ferromagnet such as

Ni or Co. The quantitative theoretical study of the

dilute iron alloys requires therefore a precise know- ledge of the structure of the ferromagnetic iron

where the s-d mixing and the splitting of the sub- bands are essential. Moreover, the method used must be able to take into account the scattering

of the Bloch waves of the matrix by the impurity.

It has been shown recently how the LMTO-ASA

method extended to the case of dilute alloys [1, 2]

allows these requirements to be met without requiring

excessive numerical calculations while taking fully

account of the spectrum of the valence electrons of the matrix.

In section 2, we recall briefly how the electronic structure of the impurities is obtained with the LMTO- ASA method and in section 3, the results for the Ti, V, Cr, Mn, Co, Ni, Cu impurities diluted in iron are

presented and discussed.

Section 4 is devoted to the conclusion.

2. Electronic structure of dilute alloys Ee(Ti, V, Cr, Mn, Co, Ni, Cu).

-

2.1 GENERAL DESCRIPTION OF THE MODEL.

-

It has been shown recently how

the LMTO-ASA method can be extended to the

case of dilute alloys [1, 2]. The impurity potential is

localized on the impurity cell and we take into account fully the self-consistent electronic structure of the matrix. In the LMTO method, the electronic density

on the impurity site is given by :

(*) LA au C.N.R.S. no 306.

In this formula, all primed quantities refer to the impurity.

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:0198200430100149700

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1498

-

nL(E) is the partial density of states of the matrix relating to the representation L

=

{ 1, m } of the symmetry point group of the crystal;

-

RL (r, E) is the normalized wave function,

solution of the Schrodinger equation in the impurity cell ;

where the derivative is taken at the « muffin- tin » sphere ;

, where the energy Ef is defined by DI(E*) I - 1. In the

atomic sphere approximation (ASA), the « muffin- tin » sphere is replaced by the Wigner-Seitz sphere.

In this formulation, the main advantage on the

Green’s function method is that the quantities which depend on the energy, such as the wave functions and their logarithmic derivatives at the atomic

sphere, are evaluated by a restricted expansion from

the parameters of the potential determined once

for all [3].

The change of the number of states between the

alloy and the matrix is, for an energy smaller than E,

where

-1 17; (0) andItl,(O) are the numbers of bound

7C l( ) 7T ( )

states of L symmetry for the impurity and matrix potential ;

If Az is the difference between the atomic numbers of the impurity and matrix atoms, the Friedel screening

rule is :

where EF is the Fermi level.

In the formulae for p’(r, E) and AZ(E), the spin

index is dropped.

2.2 THE ELECTRONIC STRUCTURE OF IRON AND THE IMPURITY POTENTIAL.

-

The self-consistent elec- tronic structure of iron, calculated by the LMTO-

ASA method, has been described previously [4, 1].

In order to determine the impurity potential, first

we consider a fictitious non-magnetic crystal with

the body centred cubic structure. Its parameter is that of ferromagnetic iron. It is built of atoms of the

same chemical species as the impurity. Thus, we

calculate the self-consistent « muffin-tin » potential V

of this metal in the canonical version of the LMTO- ASA method which neglects the hybridization of the

different symmetry states. In this way, we take partial

account of the surrounding of the impurity in the alloy. The impurity potentials seen by the electrons of different spins are obtained by the simple addition

of constants :

These constants are adjusted to satisfy the Friedel

screening rule

and the change of the observed saturation magneti-

zation

where c is the atomic concentration of impurities.

With these constants, the effect of the polarization

on the impurity site due to surrounding electrons of different spins is taken into account. Even though

our impurity potentials are localized on the impurity cell, they are determined by a self-consistent condition which takes into account the electronic screening

inside and outside the impurity cell. Our results are

given in the table I for the Ti, V, Cr, Mn, Cu impurities.

For these impurities, we have represented the partial (T25 and F12 symmetries) and total densities of states

on the figures 1, 2 and 3.

3. Analysis of the results and discussion.

-

3.1 Fe(Ti, V, Cr, Mn, Cu).

-

The comparison bet-

ween the total densities (Fig. 1) and the partial (F’ 25

and F12) densities (Figs. 2 and 3) displays the impor-

tance of the d states for the screening of the impurities.

Results obtained may be analysed as follows :

-

The screening is essentially realized in the T

sub-band for the impurities on the left of iron in the periodic table, so that :

and the average magnetization of the alloy can be

written approximatively

We find again the phenomenological law deduced from the measured magnetizations for these impu-

rities. For Cu impurity, the screening is built in the 1 sub-band.

-

The impurity d states appear as peaks in the

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Table I.

-

Screening of the impurities for the alloys Fe(Ti, V, Cr, Mn, Cu). Caption : C : constant potential.

ns, np, nd, Nimp : numbers of electrons with, s, p, d symmetry and total number of electrons in the impurity cell.

Zs(EF), AZp(EF), AZD(EF) : s, p, d components of the impurity charge. dj:tjdc Ic-0 : change of saturation magne- tization per impurity.

local density of states on the impurity site. These

peaks are located either below (e.g. Cu 1) or in (e.g.

Cr 1) or above (e.g. Ti) the band.

For the T12 symmetry, the peaks of the density

of states T are located, on both sides of the Fermi level (EF = 0.702 Ryd.) ; Ti 0. 8 Ryd. ;

V 0.74 Ryd.; Cr and Mn :. rr 0.70 Ryd.;

Cu 0.6 Ryd. The densities of states I present

two peaks : one peak has an energy in the vicinity

of the maximum of the iron density and another peak lies in the vicinity of the bottom of the band

(Ti, V, Cr, Mn) or below (Cu).

For the F’ 25 symmetry and for the T sub-band,

we observe also resonant states in the vicinity of the

Fermi level (Ti, V, Cr, Mn). For the I sub-band,

the common salient feature is a very weak density

of states at the Fermi level for each impurity. Other

resonances are also present. One, in particular,

located at about 0.56 Ryd., is related to a hole of density in the matrix.

-

In each case, as it should be, one observes a

shift of the states towards the lower energies when the potential becomes more and more attractive.

By subtracting the number of T and I electrons

on the impurity, we calculate the local moments

These are essentially due to the polarization of the d

electrons and it is remarkable that they are in very

good agreement with the measured moments even

though the impurity potential is being determined only by the average magnetization and the screening

rule.

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1500

Fig. 1.

-

T25 partial densities of states for iron and its

alloys.

Once the impurity potential is determined, the

contribution to -the contact interaction to the hyper-

fine field on the impurity for the band states is calculat- ed :

Though it is not possible to neglect the polarization

of the deep states of the impurity, it appears that the calculated field has the correct magnitude compared

with the measured field (Table II and Fig. 5).

In the case of Cu where the local moment is zero

and where it is expected that the contribution of the band states is dominant, the calculated and observed fields are very close. Our calculated hyperfine field

in the case of Cu is comparable to the value obtained by Yoshida et al. [15] who determined the electronic structure of non-magnetic impurities diluted in ferro-

magnetic iron by KKR method.

The measurement of the electronic specific heat

Fig. 2.

-

F12 partial densities of states for iron and its

alloys.

of the alloy gives the density of states at the Fermi level. Effectively, the change Any of the coefficient of electronic specific heat y is, for a concentration c of

impurities,

where n(E) is the electronic density of iron. The

presence of very narrow resonant states in the vicinity

of the Fermi energy is responsible for the large observed

variations of y (Table II and Fig. 6). For the impurities

to the left of iron, the variation of the displaced charge

with the energy is very important in the T sub-band :

it results from the competition between the large

contribution of the T2 5 states with the contribution of the F12 states which changes the sign when these

states go across the Fermi level. Due to very large

variations of the generalized phase shifts at the

Fermi level, our quantitative results should be

considered with care. Nevertheless, we think that the

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Fig. 3.

-

Total densities of states for iron and its alloys.

Fig. 4.

-

Local moments on the impurity site in iron

alloys : A theoretical values; 0 experimental values.

large variations of y are really related to the presence of the F, 2 and F2’5 resonant states in the T sub-band

at the vicinity of EF.

Fig. 5.

-

Hyperfine fields on the impurity site in iron

alloys : A theoretical values; 0 experimental values.

Fig. 6.

-

Change of the electronic specific heat coefficient in iron dilute alloys : A theoretical values; 0 experimental

values.

3.2 Fe(Co, Ni).

-

In the case of Co and Ni, it is

not possible to satisfy the conditions of average

magnetization (d/1/dc [_o - I JlB/at.) and screening

with a couple of constants C t and C I coherent with those of the other impurities. Consequently, it is not possible to find a local screening for Co and Ni intermediate between Mn and Cu. It follows that the modification of the potential due to the impurity

must be extended to its near neighbours. This modi-

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1502

Table II.

-

Hyperfine fields and change of the electronic specific heat coefficient in iron alloys.

fication is furthermore suggested by the deviation to the local neutrality obtained for the other impurities (in electrons) ; Ti : 0.3 5 ; V : 1.21; Cr : 1. 54; Mn : 1.57;

Cu : - 0.21 (Table I). The effect of the perturbation

on the near neighbour sites will be the subject of a forthcoming work.

4. Conclusion.

-

We have calculated the electronic structure of alloys Fe(Ti, V, Cr, Mn, Co, Ni, Cu) by the LMTO-ASA method taking account of the

self-consistent electronic structure of the ferromagne-

tic iron and of localized impurity potentials. The impurity potentials are adjusted in order to satisfy

the screening rule and to give the measured average

magnetization. It follows that the calculated values

of the local moments and hyperfine fields on the impurity and the coefficients of the electronic specific

heat are comparable with the measured values.

The electronic structure is dominated by the presence of resonant d states.

The case of Co and Ni cannot be studied in the

approximation of localized potentials and requires

consideration of the extension of the potential outside

the impurity cell.

In conclusion, taking account of the results obtained elsewhere for the alloys Fe(Al, Si, P, Ga) [1], our

model gives, on the whole, a rather good under- standing of the structure of s-p and d impurities

diluted in ferromagnetic iron provided the screening

of the impurity is localized on its site.

References

[1] KOENIG, C., LÉONARD, P., DANIEL, E., J. Physique 42 (1981) 1015.

[2] KOENIG, C., DANIEL, E., J. Physique-Lett. 42 (1981)

L-193.

[3] ANDERSEN, O. K., Phys. Rev. B 12 (1975) 3060.

[4] KOENIG, C., Thèse d’Etat, Strasbourg (1981).

[5] ARROT, A., NOAKES, J., Thermal, Electrical and Magne-

tic Properties of dilute Iron Alloys, edited by

P. A. Beck (Interscience, New York) 1963, p. 81.

[6] CAMPBELL, I. A., Proc. Phys. Soc. London 85 (1966) 71.

[7] COLLINS, M. F., Low, G. G., Proc. Phys. Soc. Lon-

don 86 (1965) 535.

[8] KAJZAR, F., PARETTE, G., J. Appl. Phys. 50 (1979) 1966.

[9] ALDRED, A. T., RAINFORD, B. D., KOUVEL, J. S., HICKS, T. J., Phys. Rev. B 14 (1976) 228.

[10] ALDRED, A. T., Intern. J. Magnetism 2 (1972) 223.

[11] KAJZAR, F., PARETTE, G., Phys. Rev. B 22 (1980)

5471.

[12] CADEVILLE, M. C., Private communication.

[13] SHINOZAKI, S., ARROT, A., Proc. of the IXth Intern.

Conf. L. T. 9, edited by J. G. Daunt, D. O.

Edwards, F. J. Milford, M. Yaqub (N. Y.), 1965, p. 1066.

[14] RAO, G. N., At. Data Nucl. Data Tables 15 (1975) 553.

[15] YOSMIDA, H. K., TERAKURA, K. and KANAMORI, J., J.

Phys. Soc. Japan 50 (1981) 1942.

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