L. Simon et al., A C 1S CORE-LEVEL X-RAY PHOTOELECTRON DIFFRACTION CHARACTERIZATION OFSUBSTITUTIONAL CARBON IN EPITAXIAL SI1-YCY ALLOYS GROWN ON SI(111) AND SI(001), Journal of applied physics, 81(6), 1997, pp. 2635-2642
Epitaxial strained growth of Si1-yCy alloys with rather high C concent
rations (y similar to 1.5%) has been performed on Si(111) and Si(001)
using molecular beam epitaxy (MBE) Si evaporation and thermal interact
ion of the growth surface with a low C2H4 pressure at 500 degrees C. C
arbon contents, determined by secondary ion mass spectrometry, infrare
d (ir) spectrometry, in situ C 1s and Si 2p x-ray photoelectron spectr
oscopy measurements and x-ray diffraction (XRD), are being compared. M
onocrystalline quality of the epilayers is checked by low energy elect
ron diffraction and x-ray photoelectron diffraction (XPD). As indirect
ly ascertained by the ir local vibration mode (LVM) and a shifted part
ially strain induced epilayer diffraction line in the theta-2 theta XR
D analysis, carbon is accommodated in substitutional sites (C-sub) who
se local atomic order,is investigated for the first time by XPD, C 1s
polar angle distributions being measured in different azimuthal direct
ions. As the data reveal, for a C emitter, next nearest neighbor bond
orientations identical to those for Si atoms in a Si matrix, XPD readi
ly provides direct evidence in favor of C-sub positions. UP to now our
limited angular resolution does not allow observation of possible bon
d orientation changes due to local strain-induced lattice distortions
around C atoms. Nevertheless, by increasing growth temperature (600-65
0 degrees C) and promoting formation of more C-rich phases (SinC or Si
C), the effects of substitution of second or higher nearest Si neighbo
rs by C atoms can be clearly evidenced. By the way, a significant C 1s
binding energy difference between C-sub and C in C-rich phases is obs
erved and may be used as a signature of the C dilution in the grown ep
ilayer: a characteristic value of 283.8 eV is obtained for the C-sub S
ite giving rise to the LVM. (C) 1997 American Institute of Physics.