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HAL Id: jpa-00218563

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Submitted on 1 Jan 1979

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MÖSSBAUER SPECTRUM OF 119Sn DISSOLVED IN Al

S. Umeyama, M. Taniwaki, Y. Ishida, M. Kato

To cite this version:

S. Umeyama, M. Taniwaki, Y. Ishida, M. Kato. MÖSSBAUER SPECTRUM OF 119Sn DISSOLVED IN Al. Journal de Physique Colloques, 1979, 40 (C2), pp.C2-539-C2-541. �10.1051/jphyscol:19792186�.

�jpa-00218563�

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JOURNAL DE PHYSIQUE

Colloque C2, suppl6ment au no 3, Tome 40, mars 1979, page (2-539

MOSSBAUER SPECTRUM OF I 1 9 S n DISSOLVED IN A 1

S. Umeyama, M. Taniwaki, Y . I s h i d a and M. Kato

I n s t i t u t e of I n d u s t r i a l Science, University o f Tokyo,

7

Roppongi, Minato, Tokyo,

Japan.

R6sumd.- Des a l l i a g e s A1-Sn s o n t t r a i t d s thermiquement e t l e s v a r i a t i o n s c o r r e s p o n d a n t e s d e s spec- t r e s Miissbauer s o n t a n a l y s d e s . On e n d d d u i t que l a r a i e a t t r i b u a b l e ii " ' ~ n e n s o l u t i o n s o l i d e d a n s A1 s e t r o u v e 1 2,32 mm/s e t que l a t e m p e r a t u r e de Debye e f f e c t i v e e s t 173 K. Le s p e c t r e d e " ' ~ n d a n s d e s c l u s t e r s d'atome d e Sn e t d e l a c u n e s e s t dgalement o b t e n u 1 p a r t i r d ' a l l i a g e s t r e m p s s . A b s t r a c t . - AI-Sn a l l o y s a r e h e a t - t r e a t e d and changes o f M&sbauer s p e c t r u m a r e a n a l y z e d . I t i s de- duced t h a t t h e l i n e p o s i t i o n o f l l ' s n i n s o l i d s o l u t i o n i n A1 i s 2.32 1mn1s and t h e e f f e c t i v e Debye t e m p e r a t u r e i s 173 K. The s p e c t r u m of " ' ~ n i n t h e c l u s t e r s c o n s i s t i n g o f v a c a n c i e s and Sn atoms is a l s o deduced from t h e a n a l y s i s of t h e quenched a l l o y .

l . I n t r o d u c t i o n . - Mgssbauer s p e c t r o s c o p y i s t h e use- f u l t e c h n i q u e f o r t h e s t u d y of p o i n t d e f e c t i n me- t a l s . It p r o v i d e s i n f o r m a t i o n s o f l o c a l e l e c t r o n i c s t r u c t u r e and l a t t i c e dynamical p r o p e r t i e s a r o u n d t h e p o i n t d e f e c t . The c o n c e n t r a t i o n of p o i n t d e f e c t i n m e t a l s i s n o r m a l l y s m a l l t o b e d e t e c t e d . Most i n v e s t i g a t i o n s u s e ~ a s s b a u e r atoms a s i m p u r i t y i n m e t a l s . The i n t e r a c t i o n between i m p u r i t y atoms and p o i n t d e f e c t s i n c r e a s e s t h e c o n c e n t r a t i o n o f l a t t e r around t h e G s s b a u e r atoms. Many s t u d i e s have b e e n r e p o r t e d on t h e i n t e r a c t i o n between 5 7 ~ e / 5 7 ~ o and p o i n t d e f e c t i n A l . 11-51. While few r e p o r t have a p p e a r e d on " ' ~ n . SBrensen and C o t t e r i l l s t u d i e d t h e s p e c t r u m o f t h e " ' ~ n i n AI-Sn a l l o y s 161, b u t t h e i r r e s u l t s a r e n o t v e r y c o n c l u s i v e . T i n impuri- t y i n A1 i s more i n t e r e s t i n g t h a n Fe o r CO; a l a r g e b i n d i n g e n e r g y h a s been r e p o r t e d between Sn and vacancy i n Al. 171. It h a s been c l a i m e d t h a t t h e e f f e c t o f Sn i m p u r i t i e s on t h e a g i n g p r o c e s s o f A1 a l l o y s was c a u s e d by t h i s l a r g e b i n d i n g e n e r g y 181.

2. Experimenta1s.- Specimens were p r e p a r e d from 99.999ZAl and 80% e n r i c h e d l l 9 s n . A l l o y s c o n t a i n i n g

1 x 1 0 - ~

-

5x10-' Sn were used f o r t h e s t u d y of con- c e n t r a t i o n dependence o f t h e spectrum. S h e e t spe- cimens Im t h i c k n e s s were a i r - c o o l e d o r quenched fkom 873 K. An a n n e a l i n g e x p e r i m e n t was made up t o 453 K u s i n g t h e quenched a l l o y c o n t a i n i n g 2 . 5 x 1 0 - ~ Sn. A l l measurements o f t h e s e specimens were per- formed a t 1 i q . N ~ te m p e r a t u r e . F o r t h e s t u d y o f l a t t i c e dynamical p r o p e r t i e s , t e m p e r a t u r e dependen- c e o f t h e s p e c t r u m was measured from liq.Nz tempera- t u r e up t o room t e m p e r a t u r e on t h e a i r - c o o l e d s p e c i - men and up t o 200 K on t h e quenched specimen. Spe- cimen t e m p e r a t u r e was c o n t r o l l e d u s i n g a s m a l l h e a t e r i n t h e c r y o s t a t .

G s s b a u e r s p e c t r u m was measured b y o r d i n a r y c o n s t a n t a c c e l e r a t i o n t y p e s p e c t r o m e t e r u s i n g t h e CaSnO, s o u r c e a t room t e m p e r a t u r e . O b t a i n e d s p e c t r a were i n i t i a l l y a n a l y z e d by s i n g l e L o r e n t z i a n l i n e .

I n c a s e t h a t f i t t i n g was n o t s a t i s f a c t o r y , superpo- s i t i o n o f l i n e s was assumed.

3 . R e s u l t s and d i s c u s s i o n . - F i g u r e 1 shows t h e ty- p i c a l s p e c t r a , s o l i d l i n e s a r e t h e b e s t f i t t e d Lo- r e n t z i a n l i n e s .

F i g . I : The bf6ssbauer s p e c t r a o f

"

' ~ n i n t h e AI-2. S X I O - ~ S ~ a l l o y a i r - c o o l e d ( A ) and quenched(B) from 8 7 3 K.

F i g u r e 2 shows t h e c o n c e n t r a t i o n dependence o f t h e s p e c t r a . L i n e p o s i t i o n and w i d t h i n f i g u r e 2 were deduced from t h e a n a l y s i s u s i n g a s i n g l e l i n e .

F o r t h e a i r - c o o l e d specimen, which Sn concen- t r a t i o n was lower t h a n 1 x 1 0 - ~ , s p e c t r u m was w e l l r e p r e s e n t e d by s i n g l e ~ o r e n t z i a n l i n e ( F i g . l ( A ) ) . L i n e p o s i t i o n was c o n s t a n t , 2.32 m/s, i n d e p e n d e n t on t h e c o n c e n t r a t i o n . L i n e w i d t h was a l s o c o n s t a n t and narrow, c o r r e s p o n d i n g t o t h e s i n g l e s t a t e o f Sn

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphyscol:19792186

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JOURNAL DE PHYSIQUE

Fig. 2 : Sn concentration dependence of line posi- tion and width; 0 = air-cooled specimen, = quen- ched specimen.

These results showed that Sn atoms of these speci- mens were dissolved in the A1 matrix and not influ- enced by lattice defects or other impurities. It was concluded that solid solution was obtained by the air-cooling of an alloy containing less than 1x10-'~n.

Figure 3 shows the temperature dependence of the line intensity and position of the air-cooled specimen containing 2.5x10-~~n. Line intensity was analyzed by simple Debye model.

L 0 . 0 * I

100 2 0 0 300

Temperature ( K )

Fig. 3 : Temperature dependence of line position and intensity. Specimen was air-cooled A1-2.5~10-~ Sn alloy. Line intensity was normalized by that of liq.Np temperature.

temperature approximation of the second-order Doppler shift showed that OD was about 300 K. The discrepan- cy seems to be caused by the deviation from simple Debye model and/or temperature dependence of the isomer shift. The temperature dependent isomer shift of B-Sn / 9 / suggests that the latter is more impor- tant.

Quenched specimens showed the same concentra- tion dependence as reported by Sdrensen and Cotte- rill 161. The spectrum was not fitted to a single Lorentzian line (Fig. I ( B ) ) . It was suggested that multiple state of Sn were formed by the effects of quenched-in vacancies. Figure

4

shows the analysis using two Lorentzian lines.

VELOCITY (m/s)

Fig. 4 : Analysis of spectrum using two Lorentzian lines. Specimen was quenched ~ 1 - 2 . 5 x 1 0 - ~ ~ n alloy.

The position of main component in the spectrum was near that of solid solution, but slight shift toward lower velocity side was observed. The position of sub-component was about 2.8 m / s . The annealing experiment showed that the sub-component was stable up to 453

K

and that the cluster of vacancies and Sn atoms. This suggestion was supported by the concen- tration dependence of the line position. In the low impurity concentration alloy, the fraction of impu- rity associated with the cluster increases and as the result, the fraction of sub-component may in- crease. The effective Debye temperature of the sub- component was estimated as 105

K

from the tempera- ture dependence of the line intensity. The low Debye temperature also suggested that Sn atoms associated with defects.

The effective Debye temperature OD was 173

K 2

10

K.

In contrast, analysis of line position using the

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References

/ I /

Vogl,

G . ,

Mansel, W. and Vogl. W.,

3 .

Phys.F e t a 1

Phys.5

(1974) 2321.

/ 2 /

Mansel, W. and Vogl, G.,

3 .

Phys. F Metal Phys. 1

(1977) 253.

/ 3 /

Mansel, W., Mayer, H., and Vogl,

G . ,

Radiat. Eff.

35 (1978) 69.

/ 4 /

Ichinose, H., Sassa, K., Ishida, Y., and Kato,

M.

Philos.

Mag.

36

(1977) 1367.

1.51

Sassa, K., Goto, H., Ishida, Y. and Kato,

M.,

Scr.

Met. 11

(1977) 1029.

/6/

Sirensen, K.O. and Cotterill, R.M.J., Acta

Met.;, (1974) 1331.

/ 7 /

Kimura, H. and Hasiguti, R.R.,

3 .

Phys. Soc. Japan

I8 (1963) 73.

-

/8/

Kimura,

H.

and Hasiguti, R.R., Acta Met. 9

(1961)

1076.

/9/

Rothberg,

G.M.,

Guimard, S. and Benczer-Koller, N.

Phys. Rev. fl

(1970) 136.

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