Optical absorption and light emission of oxygen incorporated small sil
icon (Si14H24) clusters as a function of oxygen content were theoretic
ally simulated by using a self-consistent semiempirical molecular orbi
tal method (MNDO-PM3). Two different models of oxygen incorporation we
re considered. Changes in the appropriate energies were traced when ox
ygen atoms were introduced either to the cluster surface (OH-group pas
sivation) or inside the cluster. An increase of the number of oxy gen
atoms both at the surface and inside the cluster results in a decrease
of the absorption energy with respect to the values typical for the c
luster passivated only by hydrogen, while the emission energy appears
to be influenced mainly by the incorporated oxygen content. There is a
Stokes shift reaching the significant value of about 0.7 eV. It reduc
es with the increase of the oxygen content down to a value of 0.2 eV i
n the case of OH-group terminated clusters while it is almost constant
for the oxygen incorporated ones.