The structure of a-Si:H, deposited at rates in excess of 100 Angstrom /s by
the hot wire chemical vapor deposition technique, has been examined by x-r
ay diffraction (XRD), Raman spectroscopy, H evolution, and small-angle x-ra
y scattering (SAXS). The films examined in this study were chosen to have r
oughly the same bonded H content C-H as probed by infrared spectroscopy. As
the film deposition rate R-d is increased from 5 to > 140 Angstrom /s, we
find that the short range order (from Raman), the medium range order (from
XRD), and the peak position of the H evolution peak are invariant with resp
ect to deposition rate, and exhibit structure consistent with a state-of-th
e-art, compact a-Si:H material deposited at low deposition rates. The only
exception to this behavior is the SAXS signal, which increases by a factor
of similar to 100 over that for our best, low H content films deposited at
similar to5 Angstrom /s. We discuss the invariance of the short and medium
range order in terms of growth models available in the literature, and rela
te changes in the film electronic structure (Urbach edge, as-grown defect d
ensity) to the increase in the SAXS signals. We also note the invariance of
the saturated defect density versus R-d, measured after light soaking, and
discuss possible reasons why the increase in the microvoid density apparen
tly does not play a role in the Staebler-Wronski effect for this type of ma
terial. (C) 2001 American Institute of Physics.