Dangling bond (DB) defects in unhydrogenated microcrystalline silicon prepared by rf sputtering have been studied. Raman spectra and x-ray diffraction indicate that the fraction has been formed at the Ar sputtering pressure higher than 26.6 Pa while only amorphous silicon has been produced at the lower pressure. The electron paramagnetic resonance (EPR) spectrum in the film is broad and unsymmetrical with the average g value of compared with that of a-Si The X- and Q-band EPR measurements suggest that the line shape is mainly governed by the inhomogeneous broadening due to the g anisotropy, indicating relatively large distribution of the structure of the DB defects.
REFERENCES
1.
2.
3.
T.
Okada
, T.
Iwaki
, K.
Yamamoto
, H.
Kasahara
, and K.
Abe
, Solid State Commun.
49
, 809
(1984
).4.
Y.
Uchida
, T.
Ichimura
, M.
Ueno
, and H.
Haruki
, Jpn. J. Appl. Phys., Part 2
21
, L586
(1982
).5.
H.
Okada
, Y.
Uchida
, and M.
Matsumura
, Jpn. J. Appl. Phys., Part 2
25
, L718
(1986
).6.
7.
P. C. Taylor, Semiconductors and Semimetals (Academic, New York, 1984), Vol. 21, Part C, p. 129.
8.
W. L.
Warren
, F. C.
Rong
, E. H.
Poindexter
, J.
Kanicki
, and G. J.
Gerardi
, Appl. Phys. Lett.
58
, 2417
(1991
).9.
F.
Finger
, C.
Malten
, P.
Hapke
, R.
Carius
, R.
Flueckiger
, and H.
Wagner
, Philos. Mag. Lett.
70
, 247
(1994
).10.
T. Ehara and T. Nagasawa, Mater. Lett. (in press).
11.
M. H.
Brodsky
, M.
Cardona
, and J. J.
Cuomo
, Phys. Rev. B
16
, 3556
(1977
).12.
Y.
Mishima
, T.
Hamasaki
, H.
Kurta
, M.
Hirose
, and Y.
Osaka
, Jpn. J. Appl. Phys.
20
, L121
(1981
).13.
T. Ehara, T. Ikoma, and S. Tero-Kubota, J. Non-Cryst. Solids (in press).
14.
15.
V. Y.
Bratus
, S. S.
Ishchenko
, S. M.
Okulov
, and I. P.
Vorona
, Phys. Rev. B
50
, 15449
(1994
).16.
F. C.
Rong
, J. F.
Harvey
, E. H.
Poindexter
, and G. J.
Gerardi
, Appl. Phys. Lett.
63
, 920
(1993
).17.
18.
M. E.
Zvanut
, W. E.
Carlos
, J. A.
Freitas
, Jr., K. D.
Jamison
, and R. P.
Hellmer
, Appl. Phys. Lett.
65
, 2287
(1994
).
This content is only available via PDF.
© 2000 American Institute of Physics.
2000
American Institute of Physics
You do not currently have access to this content.