thin films prepared by rapid thermal oxidation (RTO) and in situ steam generation (ISSG) were characterized by infrared spectroscopy (IR) with gradient etching preparation and grazing incidence x-ray reflectometry. The IR spectra of the RTO films show a lower wave number shift as the film thickness decreases. On the other hand, the IR spectra of the ISSG film produced by the addition of 5% hydrogen did not show such large peak shifts. This means that the 5% hydrogen ISSG film has a very low concentration of lower wave number components that exhibit Si–O stretching mode. These are responsible for defect structures including dangling bonds and/or oxygen deficient defects near the interface.
REFERENCES
1.
2.
J. C.
Chen
, G. H.
Shen
, and L. J.
Chen
, Appl. Surf. Sci.
142
, 120
(1999
).3.
4.
T. Y.
Luo
, M.
Laughery
, G. A.
Brown
, H. N.
Al-Shareef
, V. H. C.
Watt
, A.
Karamcheti
, M. D.
Jackson
, and H. R.
Huff
, IEEE Electron Device Lett.
21
, 430
(2000
).5.
J. S.
Lee
, S. C.
Sun
, S. M.
Jang
, and M. C.
Yu
, J. Vac. Sci. Technol. A
18
, 2986
(2000
).6.
7.
Y. Muraji, K. Yoshikawa, M. Nakamura, and Y. Nakagawa, Jpn. J. Appl. Phys. (to be published).
8.
B.
Garrido
, J.
Samitier
, S.
Bota
, J. A.
Moreno
, J.
Montserrat
, and J. R.
Morante
, J. Appl. Phys.
81
, 126
(1997
).9.
M. C.
Busch
, A.
Slaoui
, P.
Siffert
, E.
Dooryhee
, and M.
Toulemonde
, J. Appl. Phys.
71
, 2596
(1992
).10.
N.
Nagai
, Y.
Yamaguchi
, R.
Saito
, S.
Hayashi
, and M.
Kudo
, Appl. Spectrosc.
55
, 1207
(2001
).11.
J. Y.
Zhang
, X. M.
Bao
, N. S.
Li
, and H. Z.
Song
, J. Appl. Phys.
83
, 3609
(1998
).12.
R.
Tohmon
, H.
Mizuno
, Y.
Ohki
, K.
Sasagane
, K.
Nagasawa
, and Y.
Hama
, Phys. Rev.
39
, 1337
(1989
).13.
14.
M.
Kohketsu
, K.
Awazu
, H.
Kawazoe
, and M.
Yamane
, Jpn. J. Appl. Phys., Part 1
28
, 615
(1989
).15.
16.
17.
18.
K. T.
Queeney
, M. K.
Weldon
, J. P.
Chang
, Y. J.
Chabal
, A. B.
Gurevich
, J.
Sapjeta
, and R. L.
Opila
, J. Appl. Phys.
87
, 1322
(2000
).19.
B.
Harbecke
, B.
Heinz
, and P.
Grosse
, Appl. Phys. A: Solids Surf.
38
, 263
(1984
).20.
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