The correlation between composition, microstructure, and optical prope
rties of a-Si1-xCx:H thin films with different stoichiometries was est
ablished. The alloys were deposited by radio frequency glow discharge
under ''starving'' plasma conditions from mixtures of SiH4 and CH4. Th
e samples were characterized by small angle x-ray scattering, ultravio
let-visible and infrared spectrometry, and Auger electron spectroscopy
. The results showed the presence of microvoids with sizes between sim
ilar or equal to 3 Angstrom and similar or equal to 8 Angstrom. The re
lative microvoid volume fraction displayed a maximum for x around 55 a
t. % and decreased for higher values of x. High carbon content alloys
(x similar or equal to 70 at. %) not only have a lower relative microv
oid volume fraction, but show optical gaps as high as 3.7 eV, high res
istivity, and very low refractive index, indicating the presence of a
diamond-like C-C structure. These remarkable results are attributed to
the deposition under ''starving'' plasma conditions.