K. Pinardi et al., A METHOD TO INTERPRET MICRO-RAMAN EXPERIMENTS MADE TO MEASURE NONUNIFORM STRESSES - APPLICATION TO LOCAL OXIDATION OF SILICON STRUCTURES, Journal of applied physics, 84(5), 1998, pp. 2507-2512
A method is described to calculate the Raman spectrum from a nonunifor
mly strained sample taking into account the effects that arise due to
finite depth of penetration and diameter of the laser beam. Both the p
arallel and the focused beams are considered. The case of stress in. S
i substrate decaying monotonically with depth z (rapidly near the inte
rface and slowly at larger depths) is considered in detail. The predic
ted Raman shifts are found to be sensitive to both the distribution of
stress and to the absorption coefficient alpha for the laser light wa
velength used. It is found that light scattered from distances much la
rger than 1/alpha still contribute significantly to the observed Raman
spectrum. The observed shift in the peak of the spectrum does not cor
respond to the stress close to the interface. If the stress decays mor
e rapidly than the light intensity, the Raman line that originates fro
m the unstrained lower part of the substrate dominates. For transparen
t material (alpha=0) and unfocused beam the Raman spectrum consists of
only the unstrained Si line; the contribution to Raman line from the
strained interface region is completely masked. For measurements of st
resses near the interface short wavelength light with an absorption de
pth of 5-10 nm is recommended. The calculated and observed Raman shift
s in a local oxidation of silicon (a processing technique for isolatio
n) with polysilicon buffer between the nitride stripe and the Si subst
rate are compared. The agreement between the calculated and the observ
ed Raman shifts is very good. The salient points of our approach which
enabled us to obtain this agreement are: We took into account the eff
ects of laser beam width, penetration depth, and focusing; we included
the stresses in the polysilicon layer and near the polysilicon/silico
n interface, and we included contributions from large depths. (C) 1998
American Institute of Physics. [S0021-8979(98)02415-3].