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Submitted on 1 Jan 1984
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FIM AND ATOM-PROBE STUDIES OF Ni-GaAs INTERFACE
M. Wada, H. Kita, O. Nishikawa
To cite this version:
M. Wada, H. Kita, O. Nishikawa. FIM AND ATOM-PROBE STUDIES OF Ni-GaAs INTERFACE.
Journal de Physique Colloques, 1984, 45 (C9), pp.C9-471-C9-476. �10.1051/jphyscol:1984978�. �jpa-
00224467�
FIM AND ATOM-PROBE STUDIES OF Ni-GaAs INTERFACE
M. vada, H. Kita and 0. Nishikawa
Department of Materiazs Science and Engineering, The Graduate SchooZ a t Nagatsuta, Tokyo I n s t i t u t e of TechnoZogy, 4259 Nagatsuta, Midori-ku, Yokohama 227, Japan
Résumé - Une fine couche de Ni a été déposée sur un substrat dtAsGa et la formation d'un interface Ni/GaAs a été examinée en microscopie ionique de champ et par sonde à atomes.
Abstract - A thin layer of Ni was deposited on a GaAs substrate and the formation of Ni/GaAs interface layer was examined by the field ion microscope and the atom-probe.
Metal-semiconductor interface is a subject of considerable 5nterest and the structure and properties of the interfaces havebeenextensive- ly studied /1/. Ogawa /2/ has shown that Ni is highly reactive with GaAs and' forms compounds with Ga and As. In his study. chemical com- positions of the alloy layer formed by heating below 500°C were ex- amined by thé AES and the) structure of the layer was identified by the electron diiffraction (RHEED and TED) patterns. It has been demon-
formed on th& substrate was examined by field ion image and the compos~itiondl variation of the formed layer was analyzed by the AP.
1 1
Square rods 'of GaAs of a size 0.4 x 0.4 x 0.7 mm3 were sharpened in a solution of H2S04(l) and H202(1) and used for FIM and AP studies. The field ion image was observed with - 5 x 10-3 Pa of H2 gas at a tip temperature of -20 K. Ni was deposited on the field-evaporated GaAs tip surface while keeping the specimen temperature near 20 K. The backgro nd pressure during the Ni deposition was normally - 1 0 - ~ ~ a .
h
After 't e deposition, the specimen was heated at 500°C or at 600°C.
The dpec$men was again cooled down to near 20 K and the FIM image qf the heatkd specimen was observed. The compositional variation of /e Ni/GaAs interface was examined by the time-of-flight AP /6/. The tip temherature was about 200K which was considered to be an optimum tempeirature for the AP1analysis of the present GaAs specimens.
Fig. l(a) is an image of the [O011 -0riented GaAs substrate. Fig. l(b) is 4 e limage of as-deposited Ni layer on the substrate. Bright spots are]dnomly distributed and no ring pattern is neen. apd this is very dif $rent fr m the hydrogen image of a Ni crystal. When thisapparent- ly don-oryst2lline layer was field evaporated. a substrate image quite similaq ~to tAat in Fig. l(a) appeared and there was no indication of a presence O-f an interface layer between the Ni layer and the substrate.
Fig. l(c) is the image obtained after the Ni-deposited tip was heated for 3 s at 600°C. By this heating, a new phase seems to have appeared in the central region of Fig. l(c). The boundaries between this phase
Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphyscol:1984978
C9-472 JOURNAL DE PHYSIQUE
F i g . 1 - (a);FIM image of t h e [001]- o r i e n t e d GaAs s u b s t r a t e a t 3.6 kV. The
(111) and ( ï I 1 > p l a n e s a r e e q u v a l e n t . The o t h e r s e t of (111) and (111) p l a n e s a r e n o t recognized, i n d i c a t i n g d i f f e r e n t evap- o r a t i o n behavior of t h e (111) and (711) t y p e s of p l a n e s . ( b ) ; A f t e r N i d e p o s i t i o n a t t i p temperature n e a r 20 K . No i n d i c a - t i o n o f c r y s t a l l i n e s t r u c t u r e i s seen.
Imaged a t 4.5 kV. (c);The Ni-deposited t i p was heated f o r 3 s a t 600°C. Ring p a t t e r n s due t o low-index p l a n e s a r e seen on t h e s i r e s corresponding t o t h e (OOl),
( I l l ) , (011) and (101) s u b s t r a t e p l a n e s . Imaged a t 4 . 5 kV.
and t h e s u b s t r a t e a r e c l e a r . The r e g i o n 1s s t a b l e under a h i g h f i e l d and t h e image becomes b l u r r e d a t a h i g h e r v o l t a g e , i n d i c a t i n g a pro- t r u s i o n of t h i s r e g i o n from t h e o r i g i n a l GaAs s u r f a c e . F i g . l ( c ) c l e a r l y shows t h e p r e s e n c e o f r i n g p a t t e r n s o r i g i n a t i n g from low-index p l a n e s . M i l l e r i n d i c e s i n t h e f i g u r e i s t h o s e f o r t h e GaAs s u b s t r a t e . I t i s n o t i c e d t h a t t h e low-index p l a n e s o f t h i s r e g i o n c o i n c i d e w i t h t h o s e o f t h e s u b s t r a t e ; l a r g e r i n g s due t o low-index p l a n e s o f t h e new phase a r e s e e n on t h e (001) s u b s t r a t e p l a n e and a l s o t h e r i n g s a r e n o t i c e d on p o s i t i o n s c o r r e s p o n d i n g t o t h e (011) and (101) s u b s t r a t e p l a n e s , a l t h o u g h t h e s e s u b s t r a t e p l a n e s t h e m s e l v e s do n o t show t h e r i n g p a t t e r n s a s shown i n F i g . l ( a ) . An a t o m i c p l a n e i s a l s o recog- n i z e d on t h e (111) s u b s t r a t e p l a n e . F i g . 1 seems t o i n d i c a t e t h a t t h e Ni-contained r e g i o n formed by h e a t i n g a t 6 0 0 ° C i s c o h e r e n t w i t h t h e s u b s t r a t e . The c o i n c i d e n c e of t h e s i t e s o f low-index p l a n e s o f t h i s r e g i o n w i t h t h e ( O O l ) , (101) and (111) GaAs s u b s t r a t e i n F i g . l ( c ) s u g g e s t s t h a t t h e s t r u c t u r e of t h e r e g i o n i s a l s o c u b i c , p o s s i b l y w i t h t h e same l a t t i c e c o n s t a n t a s t h a t of t h e s u b s t r a t e .
A t lower t e m p e r a t u r e s , i t was d i f f i c u l t t o o b s e r v e s t a b l e and l a r g e
( c ) ; N i - d e p o s i t e d t i p was h e a t e d f o r 600 s a t 500°C. Imaged a t 7 . 1 kV.
Ni-contained r e g i o n s . F i g . 2 i s t h e r e s u l t o b t a i n e d a f t e r 500°C h e a t - i n g . F i g . 2 ( a ) i s t h e [ O l l l - o r i e n t e d s u b s t r a t e image and 2 ( b ) i s t h e imageof t h e N i - d e p o s i t e d t i p h e a t e d f o r 30 s a t 500°C. Small i s l a n d s
o f a b o u t 2 t o 10 nm i n d i a m e t e r a r e o b s e r v e d . S i n c e t h e y a r e n o t s t a b l e a s t h o s e l a r g e r o n e s , c o m p o s i t i o n a l a n a l y s i s o f t h e s e s m a l l i s l a n d s by t h e AP was n o t p o s s i b l e . When t h e amount of N i d e p o s i t i o n was s u f f i c i e n t l y l a r g e and t h e h e a t i n g p e r i o d was i n c r e a s e d , l a r g e
i s l a n d s s u c h a s t h a t shown i n F i g . 2 ( c ) was sometimes o b s e r v e d . The r i n g p a t t e r n on t h e image i s n o t c l e a r .
Compositions of t h e Ni-contained r e g i o n s formed by h e a t i n g a t 500°C
and 600°C a r e a n a l y z e d by t h e AP. F i g . 3 i s t h e r e s u l t f o r a specimen
h e a t e d a t 500°C f o r 60 S . The a b s c i s s a i s a c u m u l a t i v e number of t h e
d e t e c t e d A s and Ga atoms and t h e o r d i n a t e i s a c u m u l a t i v e number of
t h e d e t e c t e d N i atoms. When one N i atom i s d e t e c t e d , t h e l i n e i s
drawn upwards by a u n i t l e n g t h and f o r a d e t e c t i o n o f an A s o r a Ga
atom, t h e l i n e i s t o t h e r i g h t . I n t h e f i g u r e , d e t e c t i o n of atoms
s t a r t s £romL t h e o r i g i n and p r o c e e d s t o a , b , ..., and t o g beyond
which t h e GaAs s u b s t r a t e a p p e a r s . From t h e o r i g i n t o t h e d e p t h a t f ,
C9-474 JOURNAL DE PHYSIQUE
F i g . 3 - Atom-probe a n a l y s i s o f Ni/GaAs i n t e r f a c e h e a t e d f o r 60 s a t 500°C. From t h e o r i g i n t o f , o n l y two A s atoms a r e d e t e c t e d , one i n b t o c and t h e o t h e r i n d t o e . Beyond f , Ga and A s a r e mixed .
Ni on GaAs Heated at 500°C for 60s.
20k,, O 0 20 40 60
l80 (1
Number of A s t G a atoms
t h e d e t e c t e d atoms a r e m o s t l y N i and some Ga atoms, and t h e r e a r e o n l y two A s atoms d e t e c t e d , one between b and c and one between d and e . From f t o g , Ga and A s a r e mixed i n N i b a s e . The f i g u r e i n d i c a t e s t h a t by t h i s h e a t i n g Ga atoms have d i f f u s e d o u t £rom t h e s u b s t r a t e i n t o t h e N i l a y e r . There i s a n i n d i c a t i o n o f a Ga r i c h r e g i o n i n t h e outmost s u r f a c e l a y e r , £rom t h e o r i g i n t o a , i n which no A s i s d e t e c t - e d . One i n t e r e s t i n g o b s e r v a t i o n i s t h a t i n t h e N i r i c h l a y e r between p o s i t i o n s a and f , Ga atoms a r e n o t randomly d i s t r i b u t e d i n t h e N i m a t r i x . I n t h e f i g u r e , r e g i o n s b t o c and d t o e which c o n t a i n Ga a r e surrounded by N i l a y e r s . The Ga-Ni phase diagram shows a p r e s e n c e o f NijGa (Cu3Au t y p e ) s u p e r l a t t i c e i n t h e N i b a s e / 7 / . Although t h e number o f d e t e c t e d atoms i n t h e s e r e g i o n s a r e s m a l l and a c c u r a t e com- p o s i t i o n a l d e t e r m i n a t i o n i s n o t p o s s i b l e , it i s l i k e l y t h a t t h e s e r e g i o n s c o r r e s p o n d t o t h e Ni3Ga s u p e r l a t t i c e phase. The Ga composi- t i o n i n t h e s e r e g i o n s i s r e a s o n a b l y c l o s e t o t h a t o f Ni3Ga.
Compositional p r o f i l e o f N i - d e p o s i t e d GaAs h e a t e d a t 600°C f o r 60 s i s
shown i n F i g . 4 . I t shows t h a t t h e r e a r e two d i s t i n c t r e g i o n s , 1 and
I I , o f d i f f e r e n t c o m p o s i t i o n s i n t h e Ni-contained phase. Region I I I
i s t h e GaAs s u b s t r a t e . Region 1 c o n s i s t s mostly o f N i and A s , and
o n l y two Ga atoms o u t o f 8 0 t o t a l atoms a r e d e t e c t e d i n t h i s r e g i o n .
Nurnbers o f d e t e c t e d N i and A s atoms a r e 55 and 23, r e s p e c t i v e l y . A
known b u l k compound o f N i and A s w i t h c o m p o s i t i o n s s i m i l a r t o t h i s i s
Ni5As2 /7/. Compositions i n r e g i o n II i s a p p a r e n t l y d i f f e r e n t £rom
t h a t i n r e g i o n 1. Although t h e t o t a l nurnber o f d e t e c t e d atoms i n II
i s 40 and r a t h e r s m a l l , t h e a v e r a g e s l o p e i n t h i s r e g i o n seems t o
l n d i c a t e a p r e s e n c e o f N ~ ( A S , G ~ ) ~ l a y e r . The r a t i o o f t h e nurnber of
A s atoms t o t h a t o f Ga i s a b o u t 2 . The i n t e r f a c e between r e g i o n II
and t h e s u b s t r a t e i s a b r u p t and t h e r e i s no s i g n o f a t r a n s i t i o n a l
r e g i o n . The t h i c k n e s s of r e g i o n I I l a y e r i s r o u g h l y e s t i m a t e d t o b e
2 p r 3 a t o m i c l a y e r s , B e c a u s e t h e number o f atoms d e t e c t e d £rom one
60- 600°C. I n r e g i o n 1, d e t e c t e d
+ - atoms a r e m o s t l y N i and A s ,
and o n l y 2 Ga atoms a r e i n Ni on GaAs t h i s r e g i o n . I n r e g i o n I I , Heated at GO& - t h e r a t i o o f nurnber o f A s for 60 s atoms t o t h a t of Ga atoms i s
Q