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SUBSTITUTION EFFECTS ON THE MIXED VALENCE BEHAVIOUR OF Eu in EuCu2Si2
Sujata Patil, B. Padalia, R. Nagarajan, L. Gupta, R. Vijayaraghavan
To cite this version:
Sujata Patil, B. Padalia, R. Nagarajan, L. Gupta, R. Vijayaraghavan. SUBSTITUTION EFFECTS
ON THE MIXED VALENCE BEHAVIOUR OF Eu in EuCu2Si2. Journal de Physique Colloques,
1986, 47 (C8), pp.C8-983-C8-986. �10.1051/jphyscol:19868189�. �jpa-00226095�
JOURNAL DE PHYSIQUE
Colloque CS, supplement au n o 12, Tome 47, decembre 1986
SUBSTITUTION EFFECTS ON THE MIXED VALENCE BEHAVIOUR OF Eu in EuCu,Si,
SUJATA PATIL, B.D. PADALIA, R. NAGARAJAN*, L.C. GUPTA* and R. VIJAYARAGHAVAN*
D e p a r t m e n t of P h y s i c s , I n d i a n I n s t i t u t e of T e c h n o l o g y , Bombay 4 0 0 0 7 6 , I n d i a
' ~ a t a I n s t i t u t e of Fundamental R e s e a r c h , Bombay 4 0 0 0 0 5 , I n d i a
A b s t r a c t
-
R e s u l t s o f t h e L 3 XANES and 1 5 ' ~ u Mossbauer measurements onE U C U ~ ( S ~ ~ - ~ S ~ ~ ) ~ , E U ( C U ~ - ~ A U ~ ) 2 S i 2 w i t h Nx(0.2 and E U ( C U ~ . ~ M ~ . ~ ) S ~ ~ where M=Au, Ag, Ru and N i , a r e r e p o r t e d here.
I n t r o d u c t i o n :
The mixed v a l e n t (MV) systems, EuCu S i and EuPd S i have been e x t e n s i v e l y s t u d i e d b y s e v e r a l i n v e s t i g a t o r s 11-83.
' ~ t f l i t ~
o f ~ o < s b % u e r s p e c t r o s c o p y (MS) and L3-X r a y a b s o r p t i o n near edge s t r u c t u r e (L3-XANES) i n s t u d y i n g t h e Eu v a l e n c e s t a t e i n MV systems has been e s t a b l i s h e d [10]. S u b s t i t u t i o n o f Sn and Au i n EuPd S i 2 has been r e p o r t e d t o a f f e c t t h e v a l e n c e s t a t e o f Eu [10,13]. These c o n s i d e r a t i 6 n s have m o t i v a t e d us t o c a r r y o u t s y s t e m a t i c L3-XANES and MS on t h e s u b s t i t u t e d EuCu2Si2 samples. The r e s u l t s o f o u r L3-XANES and MS measurements on EuCu ( S i Sn ) Eu(Cu Au ) Si2where O(xt.2 and E C ( C ~ ~ . ~ M ~ . ~ ) ~ S ~ ~ where M =Au, Ag, 6u a Q a X ~ i X a R r e p o r k 8 h$&.Experimental :
The samples were p r e p a r e d by a r c m e l t i n g t h e c o n s t i t u e n t s i n argon atmosphere.
S i n g l e phase f o r m a t i o n o f t h e samples was checked b y x - r a y d i f f r a c t i o n method.
L3-XANES was r e c o r d e d w i t h a c o n v e n t i o n a l X - r a y a b s o r p t i o n s p e c t r o s c o p i c setup u s i n g l a b o r a t o r y source o f c o n t i n u o u s X - r a d i a t i o n [9,14]. A t r a n s m i s s i o n geometry Mossbauer spectrometer w o r k i n g i n t h e c o n s t a n t a c c e l e r a t i o n mode was used i n t h e p r e s e n t work.
R e s u l t s and D i s c u s s i o n :
L3-XANES o f a d i v a l e n t o r a t r i v a l e n t Eu i o n i s , g e n e r a l l y dominated b y a s t r o n g peak ( c a l l e d R a i e b l a n c h e o r w h i t e l i n e ) c o r r e s p o n d i n g t o an e l e c t r o n t r a n s i t i o n f r o m 2p c o r e l e v e l t o t h e f i r s t unoccupied l e v e l i n t h e c o n d u c t i o n band w i t h h i g h % $ s i t y o f s t a t e s . I n a MV system, t h e a b s o r p t i o n p r o f i l e c o n s i s t s o f two-peaks p e r t a i n i n g t o d i v a l e n t and t r i v a l e n t components, s e p a r a t e d by -7 eV.
I n t h e p r e s e n t work, a two-peak p a t t e r n w i t h 7ev s e p a r a t i o n c h a r a c t e r i s t i c o f Eu based MV systems has been observed i n t h e L3-XANES o f Eu i n EuCu ( S i Sn ) f o r each o f t h e s e c o m p o s i t i o n s ( F i g . 1 ) . - T h e peak p o s i t i o n s f o r t h e ' ~ n lilbsfi?utlg sample& appear a t t h e same energy v a l u e s as have been observed f o r t h e MV Eu (Eu and Eu ) i n EuCu S i [2]. T h i s i m p l i e s t h a t Eu i n EuCu2(Si Sn ) samples r e t a i n s i t s MV c k a r i i c t e r . I t i s apparent f r o m F i g . 1 t h a t t h e r e l ! i f f v e X i K t e n s i t i e s
o f EU'+ and E U ~ + components a r e s e n s i t i v e t o Sn c o n c e n t r a t i o n . The i n t e n s i t y o f t h e d i v a l e n t component i s seen t o i n c r e a s e w i t h i n c r e a s i n g Sn c o n c e n t r a t i o n . T h i s may b e due t o t h e v a r i a t i o n i n t h e average l o c a l v a l e n c e w h i c h c a n n o t be i d e n t l g f e d b y t h e L3-XANES s t u d y alone. I t was, t h e r e f o r e d e s i r a b l e t o r e c o r d t h e Eu Mossbauer s p e c t r a o f the same samples.
Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphyscol:19868189
C8-984 JOURNAL DE PHYSIQUE
F i g . 2 shows t h e l5' Eu Mossbauer s p e c t r a of EuCu ( S i Sn ) a t 300K and 77K The s p e c t r a o f t h e Sn s u b s t i t u t e d samples a r e s i m ? l a r 1 t 6 t # a ? o f t h e MV EuCu S i compound e x c e p t f 4 ~ t h e presence o f a s a t e l l i t e l i n e which appears a t t h e p o s i Z i o 6 expected f o r Eu
.
The isomer s h i f t ( I S ) o f t h e s a t e l l i t e l i n e appears t o be t e m p e r a t u r e independent b u t i t s r e l a t i v e i n t e n s i t y ( w i t h r e s p e c t t o t h e main l i n e ) seems t o be t e m p e r a t u r e dependent. Also, t h e s a t e l l i t e l i n e grows i n i n t e n s i t y w i t h i n c r e a s e i n Sn c o n c e n t r a t i o n .F i g u r e s 3,4,5 and 6 show L3-XANES and 1 5 1 ~ u Mossbauer s p e c t r a o f Eu(Cu M ) S i w i t h M = Au ,Ag ,Ru and N i . S i m i l a r t o EuCu ( S i Sn ) t h e L ~ - X A ~ E ~ P6? Zu ~ C I J 2 ) 2 S i Z e x h i b i t t h e c h a r a c t e r i s t i c two-pgak
'p8tt6r6'
f o r each o f t h e s e sa~p?!~: I t$3
e v i d e n t from F i g . 3 t h a t s u b s t i t u t i o n o f Au has enhanced t h e i n t e n s i t y o f t h e Eu component compared t o t h a t o f EuCu S i.
TheL3-XANES r e c o r d e d f o r E ~ ~ C U Au S i f o r O t x f ~ 2 s u g g e s t t h a t s u b s t i t u t i 6 n 6f Au i s d r i v i n g t h e MV Eu(Eu a~d"Eu"f tdwards Eu
.
T h i r would i m p l y t h a t t h e s i n g l e Mossbauer l i n e w i t h IS=-7.9 mm/sec observed f o r 20% Au s u b s t i t u t e d sample i s a mixed v a l e n t l i n e ( F i g . 5 ) . F u r t h e r c o n c e n t r a t i o n o f Au may s t a b i l i z e t h e Eu i n E U ~ + s t a t e as a r e s u l t of i n c r e a s e i n t h e volume and r e d u c t i o n i n s c r e e n i n g o f Eu c o r e h o l e due t o t h e 3d band o f Cu. F i g . 4 i n d i c a t e s t h a t f o r 20% Ag s u b s t i t u t e d sample, t h e enhancement o f d i v a l e n t component i s l e s s t h a n t h a t f o r 20% Au s u b s t i t u t e d sample eventhough t h e y have s i m i l a r e l e c t r o n i c s t r u c t u r e . T h i s d i f f e r e n c e i n b e h a v i o u r may be due t o volume e f f e c t s a r i s i n g o u t o f d i f f e r e n c e i n t h e i o n i c r a d i i . I t should be n o t e d t h a t t h e I S o f t h e Mossbauer l i n e f o r t h e 20% Ag s u b s t i t u t e d sample does n o t show a s h i f t towards t r i v a l e n t p o s i t i o n as one would e x p e c t , b u t shows a b r o a d e r l i n e a t 300K and t h e development o f a satellite l i n e towards t r i v a l e n t p o s i t i o n a t 77K. T h i s i n t e r e s t i n g aspect w i l l be d i s c u s s e d elsewhere.The L3-XANES (Fig. 4) of Ru substituted sample is similar to that of However, t h e MS measurements show two l i n e s i n t h e MV regime; t h e m a j o r
:Y::2SI~.
n e a r l y a t t h e same p o s i t i o n a k t h a t o f EuCu2SiZ and t h e m i n o r l i n e has IS= -6-9 mm/sec. which i s more towards Eu.
The s u b s t i t u t i o n o f N i f o r Cu i n EuCu S i may n o t change t h e u n i t c e l l volume as N i and Cu have almost t h e same i o n q c p a d i u s b u t may t r y t o f i l l u p i t s incornglete 3d s h e l l demanding e l e c t r o n s f r o m Eu, t h e r e b y t r y i n g t o s t a b i l i z e t h e Eu i n Eu s t a t e . T h i s has indeed been r e f l e c t e d i n t h e L3-XANES and Mossbauer s p e c t r a (Fig.4,5,6).
The m i x e d v a l e n c e b e h a v i o u r o f Eu i n EuCu S i has been i n t e r p r e t e d i n terms of t h e e x c i t a t i o n energy (E ) and a p o s s i b l e d i s ? r i g u t i o n i n E e i t h e r due t o t h e w i d t h o f t h e 4 f l e v e l
8P
due t o t h e d i f f e r e n t l o c a l e n v i r o 8 4 e n t[a].
The p r e s e n t r e s u l t s i n d i c a t e t h a t t h e v a l u e and d i s t r i b u t i o n o f E i s a f f e c t e d b y t h e s u b s t i t u t i o n o f Sn, Au, Ag, Ru and N i . An a t t e m g l i s in b e i nEUCUifi$
m de t o deduce t h e v a l u e o f E and i t s c o r r e l a t i o n t o t h e s u b s t i t u t i o n a l atoms.~ c k n o $ ? e d ~ e m e n t : We express o u r thanks t o P.L. Paulose f o r u s e f u l d i s c u s s i o n s and h e l p i n d a t a a n a l y s i s .
References:
[l] Sampathkumaran, E.V., Gupta, L.C. and Vijayaraghavan, R., Phys. L e t t . 43 (1979) 1189.
121 Hatwar, T.K., Nayak, R.M., P a d a l i a , B.D., G h a t i k a r , M.N., Sampathkumaran, E.V., Gupta, L.C., and Vijayaraghavan, R., S o l i d S t a t e Commun.
2
(1980) 617 [3] Gupta, L.C., Sampathkumaran, E.V., Vijayaraghavan, R., Prabhawalkar, V.,Prabhawalkar, P.D., and P a d a l i a , B.D., Phys. Rev. B
3
(1981) 4283 [ 4 ] Nagarajan, R., Sampathkumaran, E.V., Gupta, L.C., Vijayaraghavan, R.,Darshan, B., and P a d a l i a , B.D., Phys. L e t t . 81A (1981) 397.
[S] R o h l e r , J., and K a i n d l , G., S o l i d S t a t e Commun 36(1981) 1055.
[ 6 ] R o h l e r , J., Wohlleben, D., K a i n d l , G., and B a l s t e r , H., Phys. Rev. L e t t . 49 (1982) 65.
[7] Sampathkumaran, E.V., Gupta, L.C., Vijayaraghavan, R., Gopalakrishnan, K.V., P i l l a y , R.G., and Devare, H.G., J . Phys. C 14 (1981) 2237.
[8] Nowik, I . , H y p e r f i n e I n t e r a c t i o n s 13 (1983) 89.
[g] M a l i k , S.K., and Vijayaraghavan, R., Phys. Rev. B 30 (1984) 4031.
[ l 0 1 Kemly, E., C r o f t , M., Murgai, V., Gupta, L.C., Godart, C., Parks, R.D., and Segre, C.V., 3. Mag. Mag. Mat.
47&48
(1985) 403.[l11
Segre, C.V., C r o f t , M., Hodges, J.A., Murgai, V., Gupta, L.C., and Parks, R.D., Phys. Rev. L e t t . 49 (1982) 1947.[ l 2 1 Gupta
,
L.C., Murgai, V., Yeshurun, Y., and Parks, R.D., i n Valence I n s t a - b i l i t i e s , e d i t o r s P. Wachter and H. Boppart ( N o r t h H o l l a n d ) (1982) 225 and see o t h e r r e f e r e n c e s .[ l 3 1 Mishra, S.N., and Devare, H.G., H y p e r f i n e I n t e r a c t i o n s 15/16 (1983) 633.
[ l 4 1 P a d a l i a , B.D., Darshan, B., Dhar, S.K., Nagarajan, R., M a l i k , S.K., and Vijayaraghavan, R., Phys. L e t t . 103A (1984) 79.
ENERGY IeV) --r
F i g . 1. L XANES o f Sn s u b s t i - t u t e d ~ u ~ u ~ s i 2.
F i g . 2. Mossbauer s p e c t r a o f Sn s u b s t i t u t e d EuCu2Si2.
VELOCITY l M M / S E C )
CS-986 JOURNAL DE PHYSIQUE
ENERGY leV1
-
F i g . 3. L -XANES o f Au s u b s t i - t u t e d ~ u ~ u $ i
*.
I 1 I ,
*
.I , I I I-13 -8 -4 0 4 8 12 VELOCITY ( MM /SEC)
ENERGY I e V ) --r
F i g . 4. L3-XANES o f
Eu(Cu ) S i where
M = AI;~!~;'R~ azd N i .
[-12 I -8 1 -4 I . . =\. '5 i 2 !0 I 4 I 8 I 12
I I
VELOCITY (MM/SEC) F i g . 5. Mossbauer s p e c t r a o f F i g . 6. Mossbauer s p e c t r a o f
Eu(Cu M ) S i where M = Au, Eu(Cu M ) S i where M = Au,
Ag,