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HAL Id: jpa-00208886

https://hal.archives-ouvertes.fr/jpa-00208886

Submitted on 1 Jan 1979

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Magnetic circular dichroism study on YIG films

S. Visnovsky, J.C. Canit, B. Briat, R. Krishnan

To cite this version:

S. Visnovsky, J.C. Canit, B. Briat, R. Krishnan. Magnetic circular dichroism study on YIG films.

Journal de Physique, 1979, 40 (1), pp.73-77. �10.1051/jphys:0197900400107300�. �jpa-00208886�

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Magnetic circular dichroism study on YIG films

S. Visnovsky (*), J. C. Canit, B. Briat

Laboratoire d’Optique Physique, EPCI,10, rue Vauquelin, 75231 Paris Cedex 05, France

and R. Krishnan

Laboratoire de Magnétisme, C.N.R.S., 92190 Meudon-Bellewe, France

(Reçu le 20 juillet 1978, accepté le 27 septembre 1978)

Résumé.

2014

Nous présentons la dépendance en temperature (300 2014 1,8 K) des spectres de dichroisme circulaire

magnétique (DCM) de films de YIG entre 19 000 et 33 000 cm-1. Nos résultats sont analyses à l’aide d’un modele à deux sous-réseaux dont les contributions sont additives. Nous montrons ainsi que les transitions optiques du

YIG mettent en jeu simultanément des excitations sur les deux sous-réseaux. Par ailleurs, nos spectres de DCM permettent de localiser avec precision des bandes non observées dans le spectre d’absorption.

Abstract.

2014

This paper presents the temperature dependence (300 2014 1.8 K) of the magnetic circular dichroism

(MCD) spectrum of YIG in the 19 000-33 000 cm-1 energy range. MCD data are analysed in terms of a model

of two sublattices with additive contributions. This analysis provides strong support to the current picture that optical transitions involve simultaneous excitations on the two sublattices. Furthermore, our MCD data enable several new excited states to be located accurately.

1. Introduction.

-

Since the magnetooptic Kerr

effect measurements on Y3Fes012 (YIG) by Kahn

et al. [1] much work has been done in the investigation

of the magnetooptical spectrum of this compound

in the near ultra-violet spectral region. However, with only a few exceptions [2, 3], these experiments

were limited to room temperature [4]. The aim of

these investigations was essentially to explain the origin of the magnetooptic effects and the influence

of various substitutions on their enhancement. It

was also expected that the magnetooptical spectra in this spectral region (where the Fe3 + states are strongly perturbed by surrounding ions) would provide a

better insight into the nature of the exchange coupling

which gives rise to the ferrimagnetic ordering below

the Néel temperature, i.e., 553 K.

The purpose of this paper is twofold : (i) present the magnetic circular dichroism (MCD) spectra of

YIG measured at various temperatures and explain

them in the frame of the model of two lattice contri- butions ; (ii) shed some light on the intensity gaining

mechanism of optical transitions in this material.

2. Experimental.

-

YIG thin films were prepared by liquid phase epitaxy on Gd3GaS012 substrates

with a (110) orientation. Their MCD spectra were measured between 19 000 and 33 000 cm-1 at tempe-

ratures ranging from 1.8 to 300 K in a magnetic

field of 0.7 tesla. All our spectra were taken with a

12 A bandwidth. We checked at 1.8 K that our data

were unafi’ected by a reduction of the bandwidth down to 2 Á. Figure 1 shows our MCD data (Da)

at various temperatures between 10 K and 300 K.

Weak lines originating from the substrate (around

32 000 cm -1 ) were removed from these data. A spectrum taken at 34 K has not been included since it differed only negligibly from that at 10 K. Da is simply related to the measured quantity AA via the relationship Aoa

=

AA/log e x 1 (1, sample thickness éxpressed in cm). Here, dA stands for the difi’erential absorbance between left and right circularly polarized lights respectively.

We also measured the 1.6 K spectrum. It shows little difference with respect to that at 10 K and is therefore not reported here. Actually, in view of our past experience of these materials, we believe that the slight changes observed when comparing the

data at 1.6 K and 10 K, are due to the fact that we

used samples which have been prepared separately,

(*) On leave from the Institute of Physics, Charles University,

12116 Prague 2, Czechoslovakia.

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphys:0197900400107300

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74

Fig. 1.

-

MCD spectra at saturation of a YIG film 850 A thick at various temperatures.

e.g., they might contain different amounts of residual lead. This is substantiated by a comparison of the

data in references [2] and [3].

In thé case of high absorbance (A > 1.2), the light

scattered by the monochromator may cause a reduc- tion of Aa. However, even for the peaks around 30 000

and 32 000 cm -1 (Fig. 1), this reduction cannot reach more than a few percent and does not lead to

any displacement of the peaks. Altogether, the rela-

tive amplitudes of these at different temperatures and for a given sample are estimated to be correct within

1 %. 0

The physically important quantity is the MCD per unit length (Ax). It is therefore necessary to deter- mine 1 precisely. This was done by two independent

methods.

First, we compared the sample absorbance A

(taken on a Cary 17 instrument) and its extinction index k measured previously [5]. We recall that k and A are related via the relationship klA = 1/4 nla log e

where a is the wave number expressed in cm -1. The

measurement of A was performed in a spectral region

where 0.7 A 1 in order to avoid complications

due to interference within the film. Moreover, reflec- tion losses have been fully considered. We obtained 1 = (85 ± 6) 10-’ cm.

Second, we compared our sample MCD (Ax) to

the data derived from the measurement of the Kerr rotation (QK)’ the Kerr ellipticity (03C8K), and the refrac- tion and extinction indices (n and k). This was done by using the following expressions :

e’ and G1 are the real and imaginary parts of the

off-diagonal element Gl of the permittivity tensor.

Both ({JK and 03C8K are expressed in radians.

The above equations are valid for any value of n and k. When k is small however (e.g., k 0.3), a great simplification occurs since one then has :

({JK is known to be (155 :t 3) 10- 5 rad. at 23 700 cm-l

and 300 K [5-7]. The corresponding n has been

determined by several authors to be 2.40 [1], 2.52 [5]

and 2.64 [8]. It seems therefore reasonable to adopt

This leads to Da

=

(2.47 ± 0.34) 101 cm-1. Since

we determined AA at 23 700 cm -1 and 300 K as

(88 ± 5) 104, one finds 1

=

(82 ± 18) 10-’ cm, a result remarkably consistent with that already

obtained. The value 1 = 85 x 10-7 cm has been retained for the forthcoming calculation.

Let us now briefly summarize the main features of the observed spectra. On figure 1, the positions of

the peaks change only slightly with temperature, those at 20 700 (b) and 32 000 cm -1 (d) shifting

towards low energies when temperature increases. So does the minimum in the amplitude at 24 600 cm-1 (i).

The peak at 22 400 cm-1 (h) falls faster with increasing temperature than do the others, while the amplitude

of the peak at 27 600 cm-1 (j) remains practically

constant when the temperature is changed.

3. Discussion.

-

Fe3 + ions in YIG as well as in

a number of ferrimagnetic spinels or diamagnetically

substituted garnets, occupy both octahedral (A) and

tetrahedral (B) sites. There are several reasons to

believe that it is the number of iron ions in each site of a given compound which plays the most important

role as far as its magnetooptical properties are concerned, the specific structure of the material

being of less importance. For example, the polar

Kerr rotation data on Y, Eu and Er iron garnets [1]

present very striking analogies. Similarly, the near IR Faraday rotation spectra of YIG and magnetic

oxides with the spinel structure [14] are closely corre-

lated. These facts probably originate in the fact that the oxygen surrounding Fe3 + ions in Y3Fes012 and

e.g., Lio._5Fe2.-504, have approximately the same

dimensions and symmetry, both exhibiting a similar

geometry of the Fe3 +-02 --Fe3 + units and exchange paths.

It is therefore not surprising that a number of

workers [9-15] have provided a tentative interpreta-

tion of their measurements by assuming that each

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where T is the absolute temperature and :

nA and nB stand for the number of Fe3 + ions per cm3 in the octahedral and tetrahedral sites respectively ;

MA(T)/I MA(0) ) and MB(T)/I MB(O) are the ratios

of the octahedral and tetrahedral sublattice moments at the temperature T to the absolute values of the

corresponding moments at zero Kelvin. The values of MA and MB should be taken with the appropriate algebraic sign in accordance with the orientation of the sublattice moment in the applied magnetic

field. Eq. (5) implicitely assumes that the role of the

external field is only to orient the domains. Actually,

this is fully justified since we checked that the MCD

quickly saturates upon increasing B and is then field independent up to about 4 teslas.

Our goal is twofold here : (i) show that eq. (5)

may serve to explain the temperature dependence of

our MCD spectra ; (ii) get some insight into the microscopic origin of the absorption and, thus, MCD of YIG and related substances, by comparing E 1 A(Q) and 81B(U)’

The determination of both ElA and GIB requires a comparison of the properties of two materials contain-

ing different amounts of Fe3 + ions in sites A and B.

We have chosen YIG and lithium ferrite since the ratio of the iron concentration in B and A sites increases by a factor of 2.25 from the former to the latter. Keeping in mind that E1A and 81B are complex quantities, we need a set of four equations to deter-

mine EIA, eïA, EiB and E1B at 300 K through eq. (5).

The necessary experimental information originates

as follows : (i) 81 and E i for LF are taken from refe-

rence [16] ; (ii) e1,’ 1 and e" 1 for YIG are those of refe-

rence [7] for Q > 23 000 cm-1, while at lower energies E1 was determined from our MCD data via the rela-

tionship eï = - n Aa/nu [17] ; (iii) the ratios of the sublattice moments have been deduced from the data of references [18] and [19] for YIG and LF respecti- vely. Our derivations for e’1A, E 1 A, e’lB and EïB are given in figures 2 and 3.

ârx(a, T) has then been computed from eqs. (1)

and (5) and is shown in figure 4. In view of our absorp-

tion spectra, we have assumed in this calculation that k and n were practically temperature independent.

Comparison of experimental and theoretically esti-

mated MCD data usually proceeds via a moment analysis of the spectra [20]. In our situation, the normalized zeroth order moment

Fig. 2.

-

Spectra of the sublattices components £’lA and 8’lB’

Fig. 3.

-

Spectra of the sublattices components e1A’,, and E’lB’

has been retained as a significant parameter. Measured (Fig. 1) and estimated (Fig. 4) Mo values are shown

in table I. The agreement between the two sets of figures appears satisfactory and is taken to indicate that the phenomenological model employed is indeed

reasonable. This is further supported by the fact that,

as observed experimentally, the peak at 22 400 cm -1 (h) (in Fig. 4) increases significantly more than that at

20 700 cm-1 (b) upon cooling.

A closer examination of figures 1 and 4 indicates significant differences among the details of the

l’able I.

-

Relative normalized zeroth order moment

of our experimental and calculated MCD curves versus temperature. Both have been taken equal to 1

at 300 K so as to facilitate comparison.

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76

Fig. 4.

-

Calculated MCD spectra of YIG at various temperatures.

spectra. For example, the MCD for peaks a, c, f, j

and g in figure 1 does not completely follow the

predictions shown in figure 4. This is expected since dipole strengths corresponding to individual lines are, as we verified, practically temperature indepen- dent, whereas 81A and E1B do vary due to the change

in line widths. The effect of such a modification on

the MCD is illustrated in figure 5a in the case of

two bands P and Q separated by, e.g., 60 arbitrary

units in energy. It is assumed that their band width goes from 57 to 45 units upon cooling, while magne- tization increases by a factor 1.16. The resulting MCD presents a spectral dependence similar to that noted

in region a-c of figure 1.

Peaks f and g in figure 1 deserve special attention

since the MCD decreases upon cooling, in contra-

diction with our predictions in figure 4. The expla-

nation rests upon our previous observation [2] of

two magnetic linear dichroism peaks precisely at

26 900 cm-1 and 28 700 cm-1, these being asso-

ciated with hidden absorption components. There

are corresponding positive MCD peaks at these energies but they are also hidden under the negative

contributions due to neighbouring optical transitions.

This effect is illustrated in figure 5b which resembles

figure 5a, except that a third positive peak R (2.5 times

less intense than P and Q but the same width) has

Fig. 5.

-

Scheme illustrating the MCD at 300 K (- - -) and 0 K ( ) resulting from : a) two negative contributions (P and Q) ; b) two negative (P-Q) and one positive (R) components. All units are arbitrary.

been added between the two major negative compo- nents. The resulting temperature dependence of the

MCD closely follows that observed experimentally.

The two sublattice model therefore provides a satis- factory phenomenological account for our experi-

mental data.

Turning now to the microscopic consequences of this study, the important conclusion is that E1A and Sis (Figs. 2 and 3) have an almost similar spectral dependence, i.e., peaks appear at the same energy..

This demonstrates that absorption bands cannot be

correlated to only one or the other of the two ions.

Actually, they do necessarily involve simultaneous excitations on the two sublattices, e.g., exciton- magnon and exciton-magnon-phonon transitions. Our

study therefore strongly supports current views [3, 21, 22], regarding the interpretation of the magneto-

optical properties of YIG and related ferrimagnetic

materials.

Acknowledgments.

-

One of us (S.V.) would like

to thank C.I.E.S., France, for financial assistance to

support his study. We also acknowledge useful

comments on our manuscript, from J. Ferré and R. H. Petit.

References

[1] KAHN, F. J., PERSHAN, P. S., REMEIKA, J. P., Phys. Rev. 186 (1969) 891.

[2] CANIT, J. C., BADOZ, J., BRIAT, B., KRISHNAN, R., Solid State Commun. 15 (1974) 767.

[3] SCOTT, G. B., LACKLISON, D. E., RALPH, H. I., PAGE, J. L., Phys. Rev. B 12 (1975) 2562.

[4] For a review see WETTLING, W., J. Magn. Magn. Mater. 3

(1976) 147.

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[8] WEMPLE, S. H., BLANK, S. L., SEMAN, J. A., BIOLSI, W. A., Phys. Rev. B 9 (1974) 2134.

[9] MATTHEWS, H., SINGH, S., LE CRAW, R. C., Appl. Phys. Lett. 7 (1965) 165.

[10] CROSSLEY, W. A., COOPER, R. W., PAGE, J. L., VAN STA- PELE, R. P., Phys. Rev. 181 (1969) 896.

[11] ABULAFYA, G., LE GALL, H., Solid State Commun. 11 (1972)

629.

[12] VISNOVSKY, S., PROSSER, V., ZVARA, M., POLIVKA, P., Phys.

Status Solidi (a) 26 (1974) 513.

[13] KRISHNAN, R., TRAN KHANH VIEN, CANIT, J. C., VISNOV-

SKY, S., IEEE Trans. Magn. MAG-13 (1977) 1577.

[17] In view of our own 0394A and Kerr effect measurements below 23 000 cm-1 we believe that the results in reference [7]

are in serious quantitative error (~ 50 %) for this region.

[18] LITSTER, J. D., BENEDEK, G. B., J. Appl. Phys. 37 (1966) 1320.

[19] PRINCE, E., J. Physique 25 (1964) 509.

[20] BRIAT, B. in Electronic States of Inorganic Compounds : New Experimental Techniques, edited by P. Day, D. Reidel (Dordrecht, Holland) 1975.

[21] SCOTT, G. B., PAGE, J. L., Phys. Status Solidi (b) 79 (1977)

203.

[22] ANDLAUER, B., SCHNEIDER, J., WETTLING, W., Appl. Phys. 10

(1976) 189.

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