films by backscattering techniques - nasa · of thin films by backscattering techniques by james w....
TRANSCRIPT
![Page 1: FILMS BY BACKSCATTERING TECHNIQUES - NASA · OF THIN FILMS BY BACKSCATTERING TECHNIQUES by James W. Mayer and Marc-A. Nicolet California Institute of Technology Pasadena, California](https://reader031.vdocuments.us/reader031/viewer/2022021903/5b9e63d109d3f26e288b5abf/html5/thumbnails/1.jpg)
Project Title: EXPLORATORY STUDY ON MICROANALYSIS OF THIN
FILMS BY BACKSCATTERING TECHNIQUES
NSF Grant: AER 73-03265
Duration: 24 Months, August 1974 - August 1976 Amount: $1308400000
Principal Investigators: James W. Mayer
Marc-A. Nicolet
Paper presented on July 24, 1975 at the National Solar Photo-
voltaic Program Review Meeting, L o s Angeles, California,
July 22 - 258 19750
513
https://ntrs.nasa.gov/search.jsp?R=19760005409 2018-09-16T14:15:29+00:00Z
![Page 2: FILMS BY BACKSCATTERING TECHNIQUES - NASA · OF THIN FILMS BY BACKSCATTERING TECHNIQUES by James W. Mayer and Marc-A. Nicolet California Institute of Technology Pasadena, California](https://reader031.vdocuments.us/reader031/viewer/2022021903/5b9e63d109d3f26e288b5abf/html5/thumbnails/2.jpg)
OVERALL OBJECTIVES
1, To use backscattering spectrometry in the 1-2 MeV range
for the determination of the composition and the detection
of interdiffusion in thin film structures of interest to
photovoltaic conversion.
2, To investigate the solid-phase epitaxial growth (SPEG) of
Si layers at low temperaturesobtained by interdiffusion
processes,
3, To investigate backscattering spectrometry in the sub-MeV
range and to assess its possibilities and problems.
Caltech 2
PLANNED ACTIVITY FOR LAST SIX MONTHS
1. Investigate electrical properties of the SPEG layer.
2. Investigate the possibility of SPEG with metal films other
than Pd as transport medium.
3 . Investigate BS below 1 .-lev
514
![Page 3: FILMS BY BACKSCATTERING TECHNIQUES - NASA · OF THIN FILMS BY BACKSCATTERING TECHNIQUES by James W. Mayer and Marc-A. Nicolet California Institute of Technology Pasadena, California](https://reader031.vdocuments.us/reader031/viewer/2022021903/5b9e63d109d3f26e288b5abf/html5/thumbnails/3.jpg)
EXPLORHT3RY STUDY ON MICROANALYSIS OF THIN FILMS BY BACKSCATTERING TECHNIQUES
by James W. Mayer and Marc-A. Nicolet Cal i forn ia I n s t i t u t e of Technology
Pasadena, Ca l i fo rn ia 91125
ABSTRACT I. SPEG
To be p o t e n t i a l l y usefu l , SPEG layers must have con- t r o l l a b l e electrical characteristics, p a r t i c u l a r l y with regards to conduct ivi ty type and r e s i s t i v i t y value. E f f o r t s w e r e there- f o r e undertaken t o e s t a b l i s h t h a t such a con t ro l is possible .
W e added one processing s t e p t o the standard sample f ab r i ca t ion procedure by vacuum-depositing a t h i n l aye r (nominally 5s) of S i layer , as shown i n diagram l a b e l l e d Caltech 4 ( C 4 ) . Anneal steps remained unchanged. lyzed i n four d i f f e r e n t ways: (a) Auger Electron Spectroscopy (see CS),perfonned a f t e r t h e uppermost PdxSi confirmed that Sb w a s p resent within the SPEG l aye r of S i . The I ( V ) c h a r a c t e r i s t i c s of the SPEG layer aga ins t t h e S i sub- strate ( < l o o > , 1-10 Qcm p-type) was r e c t i f y i n g , and t h e l aye r i t s e l f afforded uood electrical conduct ivi ty and easy ohmic contact ing w i t t W wires v i a the PdxSi layer (see C 6 ) . (c) A
scanning niczm-sht 2 i c t u r e of a cleaved sampled taken i n t h e e1ectron-bea.v- 5 r.9u;sd cur ren t mode es tab l i shed t h e presence of a deple t ion r e a i m more than 1 p below t h e sur face (see C7 and C3). (d) H a l l e f f e c t da t a ind ica ted t h a t t h e SPEG l aye r w a s n-type, had an average f r e e c a r r i e r concentrat ion of about
2 10" and an average e l ec t ron mobil i ty En of a b u t 40 cm /Vs (see C 9 ) . These r e s u l t s apply t o a t y p i c a l sample obtained w i t h i n i t i a l l a y e r s of about 10002 Pd, 5 2 Sb and 1 p of amorphous S i annealed i n vacuum, f i r s t a t 280° f o r 30 min and then under slowly increasing temperatures (2 0 . 2 "C/min) up t o 525 OC. The evidence t h a t the l aye r is n type and w e l l doped is con- vincing.
Sb before t h e depos i t ion of t he amorphous
The r e s u l t i n g SPEG l a y e r w a s ana-
l aye r w a s removed, Y
(b)
Y e
W e plan t o determine t h e p rope r t i e s of t h e doped SPEG
515
![Page 4: FILMS BY BACKSCATTERING TECHNIQUES - NASA · OF THIN FILMS BY BACKSCATTERING TECHNIQUES by James W. Mayer and Marc-A. Nicolet California Institute of Technology Pasadena, California](https://reader031.vdocuments.us/reader031/viewer/2022021903/5b9e63d109d3f26e288b5abf/html5/thumbnails/4.jpg)
l a y e r s more a c c u r a t e l y , and t o t r y o t h e r methods of i n t r o - ducing t h e dopant species of v a r i o u s kinds. are inadequate p rocess c o n t r o l and marginal s e n s i t i v i t y of a n a l y t i c a l tools.
C 1 0 ) : (a) I n i t i a l f a s t (-10 g/s a t 5oOOC) t r a n s i e n t regime. growth starts w i t h i s l a n d s which u l t i m a t e l y j o i n t o form a l a y e r ( C 1 1 ) . The f i n a l Ll ickness is equa l t o tha t of t h e
i n i t i a l PdZSi l a y e r ((212). (b) Steady s ta te regime. The growth is much slower (- 1 g/s) , l i n e a r , and independent of the t h i c k n e s s of the t r a n s p o r t medium ( C 1 3 ) . The rate is thus
n o t d i f fus ion - l imi t ed .
The main problems
SPEG w i t h PdZSi as t r a n s p o r t l a y e r has two s t a g e s (see The
SPEG wi th N i silicide i n l i e u of Pd si l icide as t r a n s p o r t medium has been demonstrated by b a c k s c a t t e r i n g spec- t romet ry (C14) . A s a whole, N i SPEG is q u i t e similar t o t h a t cf Pd SPEG (C15). The t r a n s i e n t is less d i s t i n c t , because slower, and i n the s t e a d y state regime, the boundar ies of the t r a n s p o r t medium lose t h e i r d e f i n i t i o n as t h e growth proceeds, which i n d i c a t e s poore r q u a l i t y of the grown l a y e r . Reac t ions r e q u i r e tempera tures which are t y p i c a l l y 90°C above t h e corres- ponding temperatures of Pd SPEG.
11. BACKSCATTERING SPECTROMETRY (BS) To develope BS a t e n e r g i e s helow 1 MeV, depth calib-
r a t i o n must be provided f i r s t by a b s o l u t e measurements of s top- ping cross s e c t i o n s . Typical p a s t errors of f 10% are unde- s i r a b l y l a rge . W e have compared v a r i o u s methods of data e v a l u a t i o n and t h e i r errors w i t h computer programs tested a g a i n s t real 4 H e s p e c t r a . A l l methods can a t t a i n a few %, b u t v a l u e s derived from f i l m s of known MSS per u n i t area are g e n e r a l l y most reliable. Main sources of errors are caused by detector n o i s e and background s i g n a l s . Absolute measurements are planned next . a c t i v i t y and renewal proposa l are g iven i n C16 t o C19.
Summaries o f main r e s u l t s , major problems, planned
516
![Page 5: FILMS BY BACKSCATTERING TECHNIQUES - NASA · OF THIN FILMS BY BACKSCATTERING TECHNIQUES by James W. Mayer and Marc-A. Nicolet California Institute of Technology Pasadena, California](https://reader031.vdocuments.us/reader031/viewer/2022021903/5b9e63d109d3f26e288b5abf/html5/thumbnails/5.jpg)
0
0
0
0
d 2 l 0
0 0 0
nJ
2
.J
X
I- W
a a
a.
- -
5 17
![Page 6: FILMS BY BACKSCATTERING TECHNIQUES - NASA · OF THIN FILMS BY BACKSCATTERING TECHNIQUES by James W. Mayer and Marc-A. Nicolet California Institute of Technology Pasadena, California](https://reader031.vdocuments.us/reader031/viewer/2022021903/5b9e63d109d3f26e288b5abf/html5/thumbnails/6.jpg)
o-00 Si(1620 eV) A+A Pd(330eV)
(Grown Layer ) P: 31
FULLY GROWN AND ETCHED
t / Pd Sb
'0 10 20 30 40 50 60 70 80 90 I00 SPUTTERING TIME (min.)
518
![Page 7: FILMS BY BACKSCATTERING TECHNIQUES - NASA · OF THIN FILMS BY BACKSCATTERING TECHNIQUES by James W. Mayer and Marc-A. Nicolet California Institute of Technology Pasadena, California](https://reader031.vdocuments.us/reader031/viewer/2022021903/5b9e63d109d3f26e288b5abf/html5/thumbnails/7.jpg)
![Page 8: FILMS BY BACKSCATTERING TECHNIQUES - NASA · OF THIN FILMS BY BACKSCATTERING TECHNIQUES by James W. Mayer and Marc-A. Nicolet California Institute of Technology Pasadena, California](https://reader031.vdocuments.us/reader031/viewer/2022021903/5b9e63d109d3f26e288b5abf/html5/thumbnails/8.jpg)
![Page 9: FILMS BY BACKSCATTERING TECHNIQUES - NASA · OF THIN FILMS BY BACKSCATTERING TECHNIQUES by James W. Mayer and Marc-A. Nicolet California Institute of Technology Pasadena, California](https://reader031.vdocuments.us/reader031/viewer/2022021903/5b9e63d109d3f26e288b5abf/html5/thumbnails/9.jpg)
EBIC 52 1
![Page 10: FILMS BY BACKSCATTERING TECHNIQUES - NASA · OF THIN FILMS BY BACKSCATTERING TECHNIQUES by James W. Mayer and Marc-A. Nicolet California Institute of Technology Pasadena, California](https://reader031.vdocuments.us/reader031/viewer/2022021903/5b9e63d109d3f26e288b5abf/html5/thumbnails/10.jpg)
HALL EFFECT
Data obtained at room temperature with van der Pauw patterns. Values are averages over tt..lt whole thickness (- 1 m) of the SPEG layer-
Comparison with SPEG Layer bulk single crystal
Conductivity type n n
Mobility pn - 40-50 140 cm2/ws
-3 Carrier Concentration 1 d 9 cm
Resistivity - - 0 2 304 Qcm
Caltech 9
522
![Page 11: FILMS BY BACKSCATTERING TECHNIQUES - NASA · OF THIN FILMS BY BACKSCATTERING TECHNIQUES by James W. Mayer and Marc-A. Nicolet California Institute of Technology Pasadena, California](https://reader031.vdocuments.us/reader031/viewer/2022021903/5b9e63d109d3f26e288b5abf/html5/thumbnails/11.jpg)
0.4 0.6 0.8 1.0 1.2 1.4 1.6 1.8 ENERGY (MeV)
n 5 0.6
0 0.5- w I- a .0.4 0 e V) 0.3- z Q
+
Y
a 0.2-
v> 0.1
o f
- (100) Substrate 475O c
-
' 7 -#-
. I
i I I I I I I I I 1 I I I I
523
![Page 12: FILMS BY BACKSCATTERING TECHNIQUES - NASA · OF THIN FILMS BY BACKSCATTERING TECHNIQUES by James W. Mayer and Marc-A. Nicolet California Institute of Technology Pasadena, California](https://reader031.vdocuments.us/reader031/viewer/2022021903/5b9e63d109d3f26e288b5abf/html5/thumbnails/12.jpg)
![Page 13: FILMS BY BACKSCATTERING TECHNIQUES - NASA · OF THIN FILMS BY BACKSCATTERING TECHNIQUES by James W. Mayer and Marc-A. Nicolet California Institute of Technology Pasadena, California](https://reader031.vdocuments.us/reader031/viewer/2022021903/5b9e63d109d3f26e288b5abf/html5/thumbnails/13.jpg)
\ \
I
- II Q,
1 I - 0
0 rr)
0 €
<n N
U
a,
LL 0.
<n v)
W 7
IrL -0
G
,
0
(u
J~
) HIM
08
9 lN
31
SN
Wl
1V
IlINI A0
SS
3N
WH
l
525
![Page 14: FILMS BY BACKSCATTERING TECHNIQUES - NASA · OF THIN FILMS BY BACKSCATTERING TECHNIQUES by James W. Mayer and Marc-A. Nicolet California Institute of Technology Pasadena, California](https://reader031.vdocuments.us/reader031/viewer/2022021903/5b9e63d109d3f26e288b5abf/html5/thumbnails/14.jpg)
526
![Page 15: FILMS BY BACKSCATTERING TECHNIQUES - NASA · OF THIN FILMS BY BACKSCATTERING TECHNIQUES by James W. Mayer and Marc-A. Nicolet California Institute of Technology Pasadena, California](https://reader031.vdocuments.us/reader031/viewer/2022021903/5b9e63d109d3f26e288b5abf/html5/thumbnails/15.jpg)
4 + 2.0 MeV He
I I
59OOC 5 m l n
I I
I I
I I
NI
I
1 I I I 1 0
0.2 0.4 0.6 0.8 1.0 I .2 I .4 I .6
ENERGY (MeV) 3
527
![Page 16: FILMS BY BACKSCATTERING TECHNIQUES - NASA · OF THIN FILMS BY BACKSCATTERING TECHNIQUES by James W. Mayer and Marc-A. Nicolet California Institute of Technology Pasadena, California](https://reader031.vdocuments.us/reader031/viewer/2022021903/5b9e63d109d3f26e288b5abf/html5/thumbnails/16.jpg)
COMPARISON OF SPEG WITH Pd AND N i
SAMPLE
Substrate
Metal Film
S i ( a ) Film
Pd N i
< l o o > < l o o > -1000 -1000
-01 -1
FORMATION OF TRANSPORT MEDIUM
Typica l Temperature 28 0 3 50 OC
Typica l Time 30 30 min
Composition by BS Pd - 2 s1 1
- - N i - - 1 S i 1 7--
b: :-rays Pd2Si N i s i
TRANSPORT OF Si
Typica l Temperature -500 -590 OC
T r a n s i e n t Rate 410 - 2 a / s
Form i s land no i S k n f )
Steady S t a t e i ta te -1 -1 Iz/s
AFparent A c t i v a t i o n Energy - 4 - 4 ev
S t r u c t u r e ep i t ax ia l e p i t a x i a l (poor)
Ca l t ech 1 5
52 8
![Page 17: FILMS BY BACKSCATTERING TECHNIQUES - NASA · OF THIN FILMS BY BACKSCATTERING TECHNIQUES by James W. Mayer and Marc-A. Nicolet California Institute of Technology Pasadena, California](https://reader031.vdocuments.us/reader031/viewer/2022021903/5b9e63d109d3f26e288b5abf/html5/thumbnails/17.jpg)
SUMMARY OF KEY RESULTS
1. Doping of SPEG layers is possib1e;proof obtained with Sb and established via:
- I(V) characteristics - Hall effect measurements - EBIC u-probe pictures - AES
2. SPEG with PdZSi has two stages: Initial transient regime
- 10 A o / s rate - island growth - thickness = that of PdaSi layer
- 1 A o / s rate, independent of PdxSi - continuous film growth
Steady State regime layer thickness
Y
3 . SPEG with Nisi also works; generally similar to SPEG with PdZSi:
- Corresponding process temperatures are typically - 9 0 ° C higher for N i
Pd2Si - Layer quality presently inferior to obtained with
4 . Identified best methods for stopping power measurements below 1 MeV from backscattering spectra.
529
![Page 18: FILMS BY BACKSCATTERING TECHNIQUES - NASA · OF THIN FILMS BY BACKSCATTERING TECHNIQUES by James W. Mayer and Marc-A. Nicolet California Institute of Technology Pasadena, California](https://reader031.vdocuments.us/reader031/viewer/2022021903/5b9e63d109d3f26e288b5abf/html5/thumbnails/18.jpg)
MAJOR PROBLEMS
S PEG
Control of fabrication processes
- cleanliness of interfaces - purity of deposited layers - amount of doping - annealing ambient
Characterization ot final product
- limitations of analytical tools
Limitations in system
- detector noise - preamplifier noise
Limitations in target
- purity
density - thickness - mass/cm 2
5 3 0
![Page 19: FILMS BY BACKSCATTERING TECHNIQUES - NASA · OF THIN FILMS BY BACKSCATTERING TECHNIQUES by James W. Mayer and Marc-A. Nicolet California Institute of Technology Pasadena, California](https://reader031.vdocuments.us/reader031/viewer/2022021903/5b9e63d109d3f26e288b5abf/html5/thumbnails/19.jpg)
PLANNED ACTIVITY FOR NEXT SIX MONTHS
1. Characterization Gf doped SPEG layers.
2. Doping of SPEG layers by other dopants or other incorporation
methods.
3. Compare SPEG with regrowth of amorphous Si layers on single
crystal Si substrates.
4. Obtain stopping cross sections in 0.3 - 1.0 MeV range.
Caltech 18
53 1
![Page 20: FILMS BY BACKSCATTERING TECHNIQUES - NASA · OF THIN FILMS BY BACKSCATTERING TECHNIQUES by James W. Mayer and Marc-A. Nicolet California Institute of Technology Pasadena, California](https://reader031.vdocuments.us/reader031/viewer/2022021903/5b9e63d109d3f26e288b5abf/html5/thumbnails/20.jpg)
PLANNED RENEWAL REQUEST
Ma j or Goa 1 s
Inves t iga te SPEG
Assess p r a c t i c a l p o t e n t i a l of SPEG to solar cel l , and to semiconductor d e v i c e s genera l ly
Liberate SPEG from s i n g l e c r y s t a l subs tra te
Develop sub-MeV backscattering spectrometry
Estimated Dates and Costs
August, 1976 to August, 1978 ( 2 4 Months) $150,000.00
Caltech 19
532