Using infrared absorption (ir) spectroscopy, H evolution, and x-ray diffrac
tion (XRD), the structure of high-H-dilution, plasma-enhanced chemical vapo
r deposition a-Si:H films "on the edge of crystallinity" is examined. From
the ir Si-H wag mode peak frequency and the XRD results, we postulate the e
xistence of very small Si crystallites contained within the as-grown amorph
ous matrix with the majority of the bonded H located on these crystallite s
urfaces. Upon annealing, a low-temperature H-evolution peak appears, and fi
lm crystallization is observed at temperatures as low as 500 degrees C, whi
ch is far below that observed for a-Si:H films grown without H dilution. Wh
ile the crystallite sizes and volume fraction are too small to be detected
by XRD in the as-grown films, these crystallites catalyze the crystallizati
on of the remainder of the amorphous matrix upon annealing, enabling the ev
olution of H at low temperatures. The large spatial inhomogeneity in the H
bonding thus produced throughout the-film is suggested to be one of the rea
sons for the reduced Staebler-Wronski effect observed in solar cells utiliz
ing these films.