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IMPURITY-DEFECT STRUCTURES OF Sn, Sb AND Te IMPLANTED α-TIN SINGLE CRYSTALS
J. Petersen, S. Damgaard, G. Weyer, Jacques Chevallier, H. Nielsen
To cite this version:
J. Petersen, S. Damgaard, G. Weyer, Jacques Chevallier, H. Nielsen. IMPURITY-DEFECT STRUC-
TURES OF Sn, Sb AND Te IMPLANTED α-TIN SINGLE CRYSTALS. Journal de Physique Collo-
ques, 1980, 41 (C1), pp.C1-443-C1-444. �10.1051/jphyscol:19801172�. �jpa-00219660�
JOURNAL DE PHYSIQUE
ColIoqw Ct , supplt5ment au n
O1 , Tome
41,janvier
1980,page C1-443
IMPURITY-DEFECT
STRUCTURE$ OFSn,
Sb AND TeIMPlJW@
~ T T I N SINGLE CRYSTALSJ . W . P e t e r s e n , S. Damgaard, G. Weyer, J. C h e v a l l i e r and H.L. N i e l s e n I n s t i t u t e of Physics, U n i v e r s i t y of Aarhus, DK 8aDO Amhus C, Denmark.
1. I n t r o d u c t i o n
Massbauer emission spectroscopy on t h e 24-keV y t r a n s i t i o n of ' " ~ n h a s been a p p l i e d p r e v i o u s l y t o s t u d y i m p u r i t y d e f e c t s i n group-IV semiconduct- o r s from i o n i m p l a n t a t i o n of l g m ~ e [ 11
.
Here we r e - p o r t on experiments with a - t i n s i n g l e c r y s t a l s i n -1 1 9 m 119
v o l v i n g i m p l a n t a t i o n s of $n
,
Sb,
and m ~ e ,2. Experimental procedure
The a - t i n s i n g l e c r y s t a l s were grown from a tin-mercury a l l o y . The lgml'e a c t i V J t y was o b t a i n e d from an i r r a d i a t i o n of n a t u r a l t i n w i t h 24 MeV
-
1 1 9
p a r t i c l e s . The ; %e (T = 4.7 d ) was s e p a r a t e d 1 l9m
chemically from t h e t i n t a r g e t . Te deoays t o 119 Sb (T = 38 h) which i n t u r n p o p u l a t e s t h e Mass-
bauer l e v e l of " $ ~ n . The ' " ~ b a c t i v i t y was milked l i s m
from t h e Te. I m p l a n t a t i o n s were performed a t room temperature with an i s o t o p e s e p a r a t o r a t a p e-
1 3
nergy of 80 keV. Doses of 510 a t o m s / ~ n ~ were i m -
ll9m 119
p l a n t e d f o r Te and Sb and 5
-
10 '4atoms/cm2 ll9mf o r Sn. Massbauer emission s p e c t r a were meas- u r e d a t s o u r c e t e m p e r a t u r e s between 77 and 3 0 0 K with a resonance c o u n t e r of t h e p a r a l l e l p l a t e a v i a l a n c h e t y p e [ 21.
3 . Experimental r e s u l t s and d i s c u s s i o n l l 9 m 11s S p e c t r a from i m p l a n t a t i o n s of Sn, Sb, and l l g m ~ e i n a - t i n s i n g l e c r y s t a l s a r e d i s p l a y e d
119m
i n F i g u r e 1. The Sn spectrum h a s been decompos- e d i n t o two b i o s i o n l i n e s ( t a k i n g t h e known w a ~ d r u p o l e s p l i t t i n g of t h e SnO, a b s o r b e r m a t e r i a l i n t o account f o r each l i n e ) a s i n d i c a t e d i n t h e f i g u r e .
VELOCITY f m m l s e c l
F i g u r e 1 : Massbauer s p e c t r a measured a t s o u r c e t e m p e r a t u r e s of 77 K f o r i m p l a n t a t i o n g of
'
l g m s n (a), 1 1 9S b ( b )
,'
lgm'l'e ( a ) i n a - t i n s i n g l e c r y s t a l s . Line 1 a + 61 =0.0 rqm/s i s a t t r i b u t e d t o a minorl l 9 m
f r a c t i o n of Sn implanted i n t o t h e s u r f a c e oxide l a y e r of t h e sample. Line 2,6, = 2.16(5) mm/s,sbems
l l 9 m
from Sn atoms on s u b s t i t u t i o n a l l a t t i c e sites.
Compared t o an a b s o r p t i o n spectrum measured f o r t h e unimplanted s i n g l e c r y s t a l sample, t h i s l i n e i s s l i g h t l y broadened by
-
0.1 mm/s and s h i f t e d to a h i g h e r isomer s h i f t v a l u e b y - 0 . 1 m m / s . This i s dye30
Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphyscol:19801172
cl-444 JOURNAL DE PHYSIQUE
to the influence of unannealed radiation damage from the implantation. The Debye temperature of line 2 is determined to G2 = 162 (5) K from temper- ature-dependent measurements. This is in agreement with a value of 0 = 162(5) K for the undamaged mat- erial [3]. It should be mentioned that the shoulder on line 2 may indicate the presence of a weak third line at 6
=
3.4 mm/s in the spectrum.The spectrum from the '19sb implantation has been analysed in terms of three lines, a surface ox- ide line 6 1 = 0.0 mm/s, a substitutional line at 6, = 2.1 m/s, and an additional line 3 at 6 3 =
= 2.6 (1) m/s. This line is broadened by
-
0.3 mm/scompared to line 2 and has a lower Dehye temperature,
o3
=. 135 (15) K.
Analogous to conclusions drawn for a very similar line in silicon [4], this line is at- tributed to Sn atoms on (nearly) substitutional si- tes with one or two vacancies in the nearest neigh- bour shell. The change in the Mossbauer parameters compared to an undisturbed substitutional site can be explained by the presence of dangling bonds atthe Sn atoms.
~ o s t likely the same iine ( 6= 2.67 (3)
,
AE = Q 0.4 (2) mm/s, 0 = 130 (20) K ) has been observed by119m
vogl and Vogl [5] for Sd produced by neutron irradiation of a-tin at low temperatures. This de- fect line annealed at -120K in accordance with the fact that the defect is not formed in room temper-
119m
ature implantations of Sn. However, the vacancy defect is more stable when associated with Sb, thus the same Sn-vacancy structure may exist after the decay of Sb for times longer than the lifetime
( .c= 27 ns) of the Mossbauer level.
119111
The spectrum for implanted Te is decompos- ed into four lines.,Three with parameters very close to those for lines 1 - 3 and an additional line at 6, = 3.9(1) m/s. For polycrystalline a-Sn, which has a thicker surface oxide layer, this line was
observed with much larger intensity [I]. This is in agreement with a tentative assignment of this line to an oxygen-containing defect structure.
4. Conclusions
Different l19Sn defect structures have been ob- tained from implantations of g m ~ e , Sb, and 119
1 1 9m
Sn in a-tin single crystals. Implantations of 119m
Sn result in no specific defect line, however, the spectra are influenced by radiation damage and, due to the high implanted dose, the material may be amorphized. A vacancy associated impurity defect is formed in implantations of "9 Sb and
-
with evenlarger intensity
-
of l g m ~ e . Additionally, in 119mTe implantations a line is observed which is assigned to an oxygen containing defect.
This work has been supported by the Danish Nat- ural Science Research Council.
References
[I] Weyer, G., Nylandsted Larsen, A., Deutch, B.I., Antoncik, E., and Nielsen, H.L., 1nst.Phys.
Conf .Ser.l (1977) 491
[2] Weyer, G., Mdssb.Eff.Method.(eds.Gruvermann, I.J. and Seidel, C.W.)
10
(1976) 301 [3] Petersen, J.W., thesis, Aarhus 1979[4] Weyer, G., Nylandsted Larsen, A., Holm, N.E.,, and Nielsen, H.L., to be published
[5] Vogl, W. and Vogl, G., J.Physique Col1oq.z (1974) C 6
-
321and Uogl, W., thesis, Miinchen 1974