The crystalline formation of CuInSe2 thin films has been investigated
using micro-Raman spectroscopy and AES composition analysis. It is con
firmed that the Raman peaks are stongly dependent on the surface morph
ology and the Cu:In:Se ratio. In the films annealed at 315 degrees C,
crystalline grains larger than 2 mu m show Raman peaks at 174 cm(-1) a
nd 258 cm(-1). The In content is very low and the Cu:Se ratio is about
1:1 in these grains. The low In concentration is thought to be due to
the formation of In2O3 on the surface. On the other hand, random stru
ctures of 1-2 mu m grains found in films annealed at temperatures belo
w 305 degrees C show peaks at 174 cm(-1) and 186 cm(-1) instead of 258
cm(-1) and have a Cu: In: Se ratio of 1 : 1 : 3-4. Thus the 186 cm(-1
) peak is thought to be related to a Cu, In-deficient phase when compa
red to stoichiometric CuInSe,. The optimum annealing condition was fou
nd by analyzing the Raman spectra and composition of different crystal
line CuInSe, grains. Films annealed under this condition exhibited a c
lear Raman peak at 174 cm(-1) and consisted of clusters of crystals le
ss than 1 mu m in size.