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Hyperfine fields of S-rare earth impurities in noble hosts

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HAL Id: jpa-00218938

https://hal.archives-ouvertes.fr/jpa-00218938

Submitted on 1 Jan 1979

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Hyperfine fields of S-rare earth impurities in noble hosts

A. Troper, O. de Menezes, A. Gomes

To cite this version:

A. Troper, O. de Menezes, A. Gomes. Hyperfine fields of S-rare earth impurities in noble hosts. Journal de Physique Colloques, 1979, 40 (C5), pp.C5-54-C5-55. �10.1051/jphyscol:1979521�. �jpa-00218938�

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JOURNAL DE PHYSIQUE Colloque C5, supple'ment au no 5, Tome 40, Mai 1979, page C5-54

Hyperfine fields of S-rare earth impurities in noble hosts

A. Troper, 0. L. T. de Menezes and A. A. Gomes Centro Brasileiro de Pesquisas Fisicas

Av. Wenceslau Braz, 71, RJ, Brasil

Rbum6. - Le champ hyperfin d'auto-polarisation d'impuretks de Gd3+ et E u Z + dans les matrices nobles est calcult a partir du mod6le simple dCveloppC pour les impuretes de terre rare dans les matrices s-p [I]. Les rksultats numkriques sont obtenus en fonction du paramttre d'hybridization d'Anderson-Moriya (AM). Les rksultats exptrimentaux peuvent &tre dCcrits par notre modtle. Les impuretks divalentes de Eu2+ dans les mttaux nobles sont d6crites par une bande perturbke a la Slater-Koster (SK) et la rtsonance d'un Ctat d presque vide.

Abstract. - The self-polarization hyperfine field of G d 3 + and Eu2+ impurities in noble hosts is calculated using an extension of a simple model previously developed for rare earth impurities diluted in s-p hosts [I]. Numerical results for the hyperfine field for increasing bandwidths (from Cu to Au) and several strengths of the phenome- nological Anderson-Moriya (AM) hybridization parameter are presented. Experimental results can be understood within our picture. EuZ + impurities in noble metals could be described by a Slater-Koster (SK) perturbed conduc- tion band and an almost empty d-resonance hump.

Theoretical studies of the self-polarization hyper- fine field of rare earth impurities in s-p and transition hosts have been made in previous works [l, 21. Con- cerning transition hosts [2] the main effects are the strong one-electron perturbation associated to the charge difference between host and impurity and the local change of the Coulomb interaction at the impurity site [2]. These effects are at the origin of the almost equal values for the hyperfine constants of these impurities placed in 4d or 5d hosts [3].

In the case of s-p hosts, it is suggested that the triva- lent rare earth impurities acts in two ways. (i) They introduce a strong repulsive potential which locally deforms the s-p conduction band ; (ii) The d-state associated to the rare earth resonates over this deform- ed s-p conduction band thus producing a virtual bound state [I]. Contrary to the transition host case, there is a possibility of a change in sign of the hyper- fine field along the s-p series.

Concerning noble metals, the virtual bound state picture has been invoked previously in the literature to explain anomalous Hall effect [4]. It is known experimentally that Er diluted in Ag and Au hosts exhibit almost the same positive value for the hyper- fine constant.

We have applied the model developed in [l] to the noble host case. An essential difference concerning the SK perturbation occurs in this case as compared to s-p metals. In fact, assuming that the trivalent rare earth (e.g. Gd3+) contributes two s-p electrons, for monovalent hosts like noble metals, the Slater- Koster (SK) potential is an attractive one.

Concerning the host, available band calculations [5]

suggest that the unfilled (s-p) part of the conduction

states may be approximately represented by a Moriya- like parabolic density of states. We adopt Campbell's picture [6] of eight identical subbands ; the half-widths A, of these are 2,3 and 4 eV for Cu, Ag and Au respec-

tively (period effect). From the band calculations it is expected that host s-d hybridization increases in going from Cu to Ag and one expects it still increases for Au [5]. The main lines of the model go as follows cf. [I].

The SK attractive potential (V,,), which perturbes the density of states is determined via Friedel's sum rule.

Concerning the d-resonance, the position of the atomic level ( E ~ ) relative to the Fermi energy (E,) is calculated self-consistently using the extended Friedel sum rule [I].

The local exchange interaction with the 4f-level, is treated in the Born approximation and one obtains the self-polarization hyperfine field in terms of the local magnetic responses [I].

The total hyperfine field for each host, as a function of the strengh of the hybridization

I

V,,

1'

(the only free parameter of the model) is shown in figure 1. The ratio J(d) A:;)/J(') A(Z) is taken fixed and equal to 0.5 as discussed in [l] and [ 2 ] . J'") and J(d) are the exchange couplings between the localized 4f spins and the s-p conduction states and d-resonance states respectively. A,!;) and A(Z) are the induced d-core hypefine constant and the contact hyperfine constant respectively.

We note that the d-f exchange coupling J'd) is taken to be positive, in contrast to the case of hosts exhibit- ing strong d-character [2]. We have changed the J(d)/J(c) ratio from 2 to 1 and the effect on the total hyperfine field is only about 15 "/,. From the results ploted in figure 1, one sees that the region of positive

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphyscol:1979521

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HYPERFINE FIELDS O F S-RARE EARTH IMPURITIES IN NOBLE HOSTS C5-55

i.e., an appreciable period effect occurs, contrary to the case of trivalent impurities. So, experimental results could be very interesting to check this model.

HD~/J(~)A(z I ( ~ 5 ( Vc,

l2

for Ag and Au are roughly 0.12 eV and 0.21 eV

-3 0J

Fig. 1. - Self-polarization field of Gd3+ (in units of J'") A(Z) ( Sz )) ,,o.

as a function of I V,,

IZ

for Cu, Ag and Au hosts (see text).

20-

1.0-

self-polarization fields corresponds to increasingly 0,5.

higher

I

Vcd

IZ

matrix elements when one goes from Cu to Au. This is in agreement with the increasing host

respectively.

Now concerning divalent rare earth impurities, such as Eu2+, one would expect for the total self- polarization hyperfine field the behavior depicted in

f C U figure 2. In fact, for divalent Eu in the absence of occupied d-states, only the SK perturbation remains and the field is always positive. We have plotted the total hyperfine field as a function of the half band-

0- width, since ( VCd

I2

plays no relevant role in this case.

The trend showed in figure 2 is understandable since for larger bandwidths the local magnetic responses should decrease. One predicts

-

men'S performed in ErAg N and ''Au IV systems one may ~ i2. ~- ~ ~ l f - ~ ~ l ~ ~ i ~ ~ t i ~ ~ , field of ~ ~ (in units of J") A(Z) 2 +

estimate from figure 1 that the appropriated values of

<

sZ >) as a function of the band width of the host (see text).

value of the s-d hybridization if

I

Vcd

l2

is interpreted as in [7], i.e., the Anderson-Moriya (AM) resonance

References

L

[I] TROPER, A., DE MENEZES, 0. L. T., LEDERER, P. and GOMES, A. A., Phys. Rev. B 18 (1978) 3709.

[2] TROPER, A,, LEDERER, P., GOMES, A. A. and BISCH, P. M., Phys. Rev. B 17 (1978) 3501.

[3] DAVIDOV, D., ORBACH, R., RETTORI, C., TAO, L. J. and RICKS, B., Phys. Lett. 35A (1971) 339.

[4] FERT, A. and FRIEDERICH, A., Phys. Rev. B 13 (1976) 397.

[5] SNOW, E. C., Phys. Rev. 171 (1968) 785.

[6] CAMPBELL, I. A., J. Phys. C 2 (1969) 1338.

[7] RIEDINGER, R., J. Phys. Chem. Sol. 31 (1970) 2087 ; J. Phys. F (Metal Phys.) 1 (1971) 392.

being associated to host hybridization. From experi- 1.0 2 o 3.0 4.0 A C

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