TY - JOUR
T1 - Comparison between ultraviolet-photoelectron spectroscopy and reflection high-energy electron diffraction intensity oscillations during Si epitaxial growth on Si(100)
AU - Enta, Y.
AU - Irimachi, H.
AU - Suemitsu, M.
AU - Miyamoto, N.
PY - 1997
Y1 - 1997
N2 - In ultraviolet-photoelectron spectroscopy on a Si(100) surface during solid-source or gas-source molecular-beam epitaxy (MBE), intensity oscillations of photoelectrons from the valence-band surface states are observed. Recent studies by authors [Enta et al., Surf. Sci. 313, L797 (1994)] have revealed that the photoelectron intensity oscillations (PIOs) most probably originate from an alternation between the 2×1 and the 1×2 surface reconstructions during growth. This model consequently suggests that the period of the oscillations corresponds to the growth time of 2 ML. To confirm this relation, reflection high-energy electron diffraction (RHEED) intensity oscillation was measured during gas-source MBE, using Si2H6 under identical growth conditions with those used for PIO observations. The oscillation period at the half-order diffraction spots of RHEED agreed well with that of PIO at various Si2H6 pressures, providing a direct support for the above interpretation for the origin of PIO.
AB - In ultraviolet-photoelectron spectroscopy on a Si(100) surface during solid-source or gas-source molecular-beam epitaxy (MBE), intensity oscillations of photoelectrons from the valence-band surface states are observed. Recent studies by authors [Enta et al., Surf. Sci. 313, L797 (1994)] have revealed that the photoelectron intensity oscillations (PIOs) most probably originate from an alternation between the 2×1 and the 1×2 surface reconstructions during growth. This model consequently suggests that the period of the oscillations corresponds to the growth time of 2 ML. To confirm this relation, reflection high-energy electron diffraction (RHEED) intensity oscillation was measured during gas-source MBE, using Si2H6 under identical growth conditions with those used for PIO observations. The oscillation period at the half-order diffraction spots of RHEED agreed well with that of PIO at various Si2H6 pressures, providing a direct support for the above interpretation for the origin of PIO.
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U2 - 10.1116/1.580731
DO - 10.1116/1.580731
M3 - Review article
AN - SCOPUS:5844219919
VL - 15
SP - 911
EP - 914
JO - Journal of Vacuum Science and Technology A
JF - Journal of Vacuum Science and Technology A
SN - 0734-2101
IS - 3
ER -