Effects of microwave power on the structural and emission properties of hydrogenated amorphous silicon carbide deposited by electron cyclotron resonance chemical vapor deposition
Sf. Cui, J",rusli,"yoon et al., Effects of microwave power on the structural and emission properties of hydrogenated amorphous silicon carbide deposited by electron cyclotron resonance chemical vapor deposition, J APPL PHYS, 89(5), 2001, pp. 2699-2705
Hydrogenated amorphous silicon carbide (a-Si1-xCx:H) films have been deposi
ted using an electron cyclotron resonance chemical vapor deposition system.
The effects of varying the microwave power from 100 to 1000 W on the depos
ition rate, optical band gap, film composition, and disorder were studied u
sing various techniques such as Rutherford backscattering spectrometry, spe
ctrophotometry, Fourier-transform infrared absorption, and Raman scattering
. Samples deposited at 100 W are found to have a carbon fraction (x) of 0.4
9 which is close to that of stoichiometric SiC, whereas samples deposited a
t higher microwave powers are carbon rich with x which are nearly independe
nt of the microwave power. The optical gaps of the films deposited at highe
r microwave powers were noted to be related to the strength of the C-H-n bo
nd in the films. The photoluminescence (PL) peak emission energy and bandwi
dth of these films were investigated at different excitation energies (E-ex
) and correlated to their optical band gaps and Urbach tail widths. Using a
n E-ex of 3.41 eV, the PL peak energy was found to range from 2.44 to 2.79
eV, with the lowest value corresponded to an intermediate microwave power o
f 600 W. At increasing optical gap, the PL peak energy was found to be blue
shifted, accompanied by a narrowing of the bandwidth. Similar blueshift was
also observed at increasing E-ex, but in this case accompanied by a broade
ning of the bandwidth. These results can be explained using a PL model for
amorphous semiconductors based on tail-to-tail states radiative recombinati
on. A linear relation between the full width at half maximum of the PL spec
tra and the Urbach energy was also observed, suggesting the broadening of t
he band tail states as the main factor that contributes to the shape of the
PL spectra observed. (C) 2001 American Institute of Physics.