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Submitted on 1 Jan 1978

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MAGNETIC EXCITATIONS IN THE

INTERMEDIATE VALENCE SYSTEM Sm0.75 Y0.25S

H. Mook, T. Penney, F. Holtzberg, M. Shafer

To cite this version:

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JOURNAL DE PHYSIQUE Colloque C6, supplément au n° 8, Tome 39, août 1978, page C6-837

MAGNETIC EXCITATIONS IN THE INTERMEDIATE VALENCE SYSTEM S m0 > 7 5Y0 # 2 5S

H.A. Mook , T. Penney, F . Holtzberg and M.W. Shafer

Solid State Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee S7830-> U.S.A. IBM T.J. Watson Research Center, lorktown Heights, New York 10598, U.S.A.

Résumé.- Nous avons étudié par la diffusion inélastique de neutrons, les excitations magnétiques des composés SmS et Sn0 75Y0 25S. Pour le SmS les résultats s'expliquent facilement à l'aide d'une théo-rie simple du type champ-moyen. Par contre l'alliage se comporte comme un système à valence mixte. Les largeurs d'énergie d'excitation du Sm0 75Y0 25S sont de l'ordre de 15 meV ce qui correspond à une durée de vie moyenne d'environ 3 x 10 1 3s .

Abstract.- Neutron inelastic scattering measurements have been made for the magnetic excitations in SmS and Smo .75Y0,25s- The results for SmS can be understood using a simple mean-field theory, but the Smo.75Y0.25S measurements show a temperature dependence and linewidth that appear to result from intermediate valence effects. The energy widths of the excitations in Sm Y S are on the order

of 15 meV corresponding to a lifetime of about 3 x l 01 3s . 0.750.25

There has been wide interest recently in the samarium monochalcogenides because of their unusual physical properties /l/. In particular, SmS under-goes a pressure induced semiconductor to metal transition at about 6.5 kbar in which there is a large volume decrease but no change in the crystal structure /2/. This phase transition is thought to result from a change in the Sm ion from a Sm++ (7F0) configuration to an intermediate valence configura-tion which is some sort of mixture of the Sm and Sm ++(6Hst) configuration. A similar lattice collap-se can be obtained by alloying YS with SmS. In this case the Sm configuration change can be studied as a function of temperature and high pressure cells are not needed/3,4/. The unusual magnetic properties associated with this lattice collapse and the absen-ce of magnetic ordering at low temperatures lead Maple and Wohlleben to the conclusion that the col-lapsed phase can be described by a fluctuating sta-te in which there are rapid fluctuations between the Sm and Sm configurations /5/. The configurations of SmS and Sm(Y)S have been examined by both X-ray photoemission/6,8/ and Mossbauer/9/ isomer shift measurements at room temperature. These two sets of measurements show that both the Sm and Sm valen-ce states exist in collapsed SmS but while X-ray

This is a draft of apaper being submitted for pu-blication. Contents of this paper should not be quoted nor referred to without permission of the x authors. .

Research sponsored by the Division of Materials Sciences, U.S. Department of Energy under con-tract W-7405-eng-26 with the Union Carbide Cor-poration.

photoemission results show separate sets of spectra for the two configurations, the Mossbauer measure-ments show a single sharp line corresponding to an intermediate valence. The Mossbauer measurements show that any fluctuations between the two valence statesmustbe faster than 10 9s . The time scale for X-ray photoemission studies is much shorter, on the order of 10 1 6s . so that it appears that the fluctu-ation time must be between 10 9 and 10 1 6s . Neutron scattering studies usually involve energy resolu-tions of a few millivolts. A linewidth of this ma-gnitude would correspond by AEAT'Vh to a time of about !0 1 3 s. which appears to be the time scale of interest in the mixed valence problem.

Our measurements were performed on powdered samples of Smo^ysYo 25S in which the Sm is isotopi-cally enriched to 99 % I51*Sm t6 avoid the high cap-ture cross section of naturally occuring Sm. Latti-ce constant measurements, assuming Vegard's law, suggest that the valence state is 40 % Sm at room temperature when the crystals have a gold color and about 70 % Sm at 100 K when the material is black. The transition takes place over a temperature range of about 50 K centered at 200 K.

The 7F0 state does not split in a crystalli-ne field but transitions can be observed between the 7F0 ground state and the first multiplet level 7Fi. This transition has been studied by Shapiro et al. /10/ for SmS which is thought to be in the pure Sm state at all temperatures. Their measure-ments demonstrated the dispersion of the 7F0 - 7Fi transition but did not include intensity

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ments. We have measured the strength of the 7 ~ o

-

a similar intensity plot as that given in Figure 1 and

7 ~ 1 transition as a function of temperature using we see that the intensities do not fit the (MF-RPA)

++

time-of-flight techniques. The results of the mea- temperature dependence of Sm

.

surements aleshown in figure 1.

E (millivolts) f.2

0.8

400 200 300 TEMPERATURE ( K)

Fig. 1 : Neutron scattering measurements of the 7 ~ o + 7 ~ 1 transition for SmS at various temperatures. The bottom graph shows the intensity of the tran- sition plotted vs temperature on a scale such that the (MF-RPA) temperature dependence is set to unity.

As one warms up from T=O the intensities of the

f 6 20 24 28 32 36 40 44 48 E (millivolts ) 0.6 0.4 0 0 100 200 300 TEMPERATURE ( K )

peaks diminish, they narrow, and the center of gra-

Fig. 2 : Neutron scattering measurements for vity shifts upward in energy. The narrowing and ~ m o -75.~0 -25s made in the same way as those for SmS shift is consistent with the change in dispersion show" in-figure 1. The bottom graph shows the tem- perature dependence of the intensity of the transi- which varies from about 6 meV at 15 K to 3 meV at tion on a scale that is the same as that used in room temperature. The width of the peak is well figure 1. The dotted line+shows the expected tem ++.pin

perature dependence if Sm is converted to Sm accounted for by dispersion and spectrometer reso- a manner described by the lattice constant interpo- lution and no intrinsic broadening of the line was lation'

observed. The plot on the bottom of figure 1 shows the intensity of 7 ~ o - 7 ~ 1 transition plotted against temperature using a scale sucli that the expected temperature behaviour of the cross section calcu- 1ated.from a mean-field-random-phase-approximation (MF-RPA) given in reference /lo/ is set to unity. The agreement appears to be satisfactory and we feel that SmS can be understood in a straightfor- ward manner within the (MF-RPA) approximation.

Figure 2 shows an identical set of measure- ments made on Smo.75Yo,25S. One notices immediately that the lines are much broader and that the tem- perature dependence appears to be different than for SmS. The graph at the bottom of figure 2 shows

The variation from (MF-RPA) theory can be explai-

+I

-ned by a change in the Sm valence state from Sm

-I++

to Sm upon warming and the dotted line shows the expected temperature dependence if the amount of ~ m + + in the system is given by the lattice constant

++

'

*+

interpolation between Sm and Sm

.

The agreement in this case appears to be satisfactory.

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tely. Because some broadening may be due to alloy effects the most we can say from the neutron expe- riments is that there is an upper bound of about 15 meV in the linewidth from mixed valence effects. This tells us that the fluctuation time for the mi- xed valence state must be longer than 3 x 10'-l3 s. a value considerably larger than the lower bound given by the photoemission measurements.

One might expect to see strong transitions

+++

from the crystal field excitations of the Sm (=H*) configuration. However, the crystal field splitting should be at most about 10 meV and if the linewidths are as broad as the 7 ~ o - 7 ~ 1 transition the (6~y2) configuration would not be well defined. This is in agreement with the magnetic measurements /5/ which show no indication of a large Curie c o w ponent to the suceptibility.

References

/I/ Review articles on these and other mixed valen- ce compounds have been written by Varma,C.M., Rev. Mod. Phys.

48

(1976) 219 and Von Molnar,S., Penney,T. and Holtzberg,F., J. Physique Colloq. 37 (1976) C4-239

-

/ 2 / Jayaraman,A., Narayanamurti,V., Bucher,E. and Maines,R.G., Phys. Rev.

5

(1970) 1430

/3/ Ta0,L.T. and Holtzberg,F., Phys. Rev. (1975) 3842

/4/ Penney,T. and Holtzberg,F., Phys. Rev. Lett.

24

(1 975) 322

151 Maple,M.B. and Wohlleben,D., Phys. Rev. Lett. 27 (1971) 511

-

161 Freeouf

,

J.L., Eastman,D .E., Grobman,W.D., Holtz- berg,F. and Torrance,J.B., Phys. Rev. Lett.

33

(1974) 161

/ 7 / Campagna,M., Bucher ,E., Wertheim,G.H. and Longi- notti,L.D., Phys. Rev. Lett.

2

(1974) 165

181 Pollak,R.A., Holtzberg,F., Freeouf,J.L. and Eastman,D.E., Phys. Rev.

33

(1974) 820

/9/ Coey,J.M.D., Ghatak,S.K., Avignon,M. and Holtz- berg,F., Phys. Rev.

B14

(1976) 3744

1101

Shapiro,S., Birgeneau,R.J. and Bucher,E., Phys. Rev. Lett.

24

(1975) 470

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